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[M]Wahl hurt himself while trying to field a bunt[/M] in the sixth inning of Game 2, he said. | Brandon Nimmo thought a disabled-list stay was off the table regarding his left index finger. He was struck by a pitch while grounding out Thursday. There was pain. But no break. So he thought no DL. Wrong.
Nimmo went on the 10-day disabled list Monday, retroactive to Friday. The outfielder will take the DL stay in a heartbeat.
“We really dodged a bullet and that’s what I’ve been told by two doctors,” Nimmo said. “Not sure how, but it’s not broken and that’s great, so that would have been season-ending pretty much. | n |
[M]Wahl hurt himself[/M] while trying to field a bunt in the sixth inning of Game 2, he said. | Brandon Nimmo thought a disabled-list stay was off the table regarding his left index finger. He was struck by a pitch while grounding out Thursday. There was pain. But no break. So he thought no DL. Wrong.
Nimmo went on the 10-day disabled list Monday, retroactive to Friday. The outfielder will take the DL stay in a heartbeat.
“We really dodged a bullet and that’s what I’ve been told by two doctors,” Nimmo said. “Not sure how, but it’s not broken and that’s great, so that would have been season-ending pretty much. | n |
The Mets sent a [M]player[/M] to the disabled list Friday, [M]but not the one everyone expected.[/M] | Brandon Nimmo thought a disabled-list stay was off the table regarding his left index finger. He was struck by a pitch while grounding out Thursday. There was pain. But no break. So he thought no DL. Wrong.
Nimmo went on the 10-day disabled list Monday, retroactive to Friday. The outfielder will take the DL stay in a heartbeat.
“We really dodged a bullet and that’s what I’ve been told by two doctors,” Nimmo said. “Not sure how, but it’s not broken and that’s great, so that would have been season-ending pretty much. | n |
[M]The Mets sent a player to the disabled list Friday[/M], but not the one everyone expected. | Brandon Nimmo thought a disabled-list stay was off the table regarding his left index finger. He was struck by a pitch while grounding out Thursday. There was pain. But no break. So he thought no DL. Wrong.
Nimmo went on the 10-day disabled list Monday, retroactive to Friday. The outfielder will take the DL stay in a heartbeat.
“We really dodged a bullet and that’s what I’ve been told by two doctors,” Nimmo said. “Not sure how, but it’s not broken and that’s great, so that would have been season-ending pretty much. | e |
“It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of [M]Nimmo[/M], who [M]did not start Friday.[/M] | Brandon Nimmo thought a disabled-list stay was off the table regarding his left index finger. He was struck by a pitch while grounding out Thursday. There was pain. But no break. So he thought no DL. Wrong.
Nimmo went on the 10-day disabled list Monday, retroactive to Friday. The outfielder will take the DL stay in a heartbeat.
“We really dodged a bullet and that’s what I’ve been told by two doctors,” Nimmo said. “Not sure how, but it’s not broken and that’s great, so that would have been season-ending pretty much. | n |
“It’s just a blow to the index finger and [M]he’s going to play as tolerated,” Mickey Callaway said of Nimmo[/M], who did not start Friday. | Brandon Nimmo thought a disabled-list stay was off the table regarding his left index finger. He was struck by a pitch while grounding out Thursday. There was pain. But no break. So he thought no DL. Wrong.
Nimmo went on the 10-day disabled list Monday, retroactive to Friday. The outfielder will take the DL stay in a heartbeat.
“We really dodged a bullet and that’s what I’ve been told by two doctors,” Nimmo said. “Not sure how, but it’s not broken and that’s great, so that would have been season-ending pretty much. | n |
[M]“It’s just a blow to the index finger[/M] and he’s going to play as tolerated,” [M]Mickey Callaway said of Nimmo[/M], who did not start Friday. | Brandon Nimmo thought a disabled-list stay was off the table regarding his left index finger. He was struck by a pitch while grounding out Thursday. There was pain. But no break. So he thought no DL. Wrong.
Nimmo went on the 10-day disabled list Monday, retroactive to Friday. The outfielder will take the DL stay in a heartbeat.
“We really dodged a bullet and that’s what I’ve been told by two doctors,” Nimmo said. “Not sure how, but it’s not broken and that’s great, so that would have been season-ending pretty much. | n |
[M]Brandon Nimmo thought a disabled-list stay[/M] was off the table [M]regarding his left index finger[/M]. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | n |
[M]Brandon Nimmo thought a disabled-list stay was off the table[/M] regarding his left index finger. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | n |
[M]There was pain[/M]. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | n |
“We really dodged a bullet and [M]that’s what I’ve been told by two doctors,” Nimmo said[/M]. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | e |
[M]“We[/M] really [M]dodged a bullet[/M] and that’s what I’ve been told by two doctors,” Nimmo said. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | n |
[M]The outfielder will take the DL stay in a heartbeat[/M]. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | n |
[M]The outfielder will take the DL stay[/M] in a heartbeat. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | n |
“Not sure how, but [M]it’s not broken[/M] and that’s great, so that would have been season-ending pretty much. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | e |
[M]He[/M] was struck by a pitch while [M]grounding out Thursday.[/M] | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | n |
[M]He was struck by a pitch[/M] while grounding out Thursday. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | e |
[M]Nimmo went on the 10-day disabled list[/M] Monday, [M]retroactive to Friday.[/M] | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | n |
[M]Nimmo went on the 10-day disabled list Monday[/M], retroactive to Friday. | The Mets sent a player to the disabled list Friday, but not the one everyone expected.
Brandon Nimmo, who took a pitch to the left index finger in Game 1 of Thursday’s doubleheader, has no structural damage and is day-to-day. Nimmo, whose X-ray and MRI were clean, was examined by two hand specialists, both of whom gave him a clean bill of health. “It’s just a blow to the index finger and he’s going to play as tolerated,” Mickey Callaway said of Nimmo, who did not start Friday.
"I’ve kind of played around with [gripping a bat] just a little bit just to see where it’s at [and] it’s not great," said Nimmo, who classified his injury as a bone bruise. "I don’t really feel good even tying my shoes right now. That’s not great. But they said this thing can really surprise you in how quickly it gets better."
Righthanded reliever Bobby Wahl was put on the 10-day DL with a Grade 1 right hamstring strain, Callaway said.
Wahl hurt himself while trying to field a bunt in the sixth inning of Game 2, he said. “I felt something kind of grab at me,” Wahl said. | c |
Black holes may be capable of emitting one type of radiation, [M]Hawking radiation, conjectured[/M] by Stephen Hawking [M]in the 1970s[/M]. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
Black holes may be capable of emitting one type of radiation, [M]Hawking radiation, conjectured by Stephen Hawking[/M] in the 1970s. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]Black holes may be capable of emitting[/M] one type of radiation, [M]Hawking radiation[/M], conjectured by Stephen Hawking in the 1970s. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | e |
[M]Black holes may be capable of emitting one type of radiation[/M], Hawking radiation, conjectured by Stephen Hawking in the 1970s. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | e |
(In 2021, [M]reflections of light were observed in the farthest part of the black hole[/M].) | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
([M]In 2021, reflections of light were observed in the farthest part of the black hole[/M].) | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle[/M], not even light, [M]can escape from it.[/M] | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | e |
[M]A black hole is a finite region of space[/M] within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
This curvature is studied by [M]general relativity[/M], which predicted the [M]existence of black holes[/M] and [M]was its first indication.[/M] | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
This curvature is studied by [M]general relativity[/M], which [M]predicted the existence of black holes[/M] and was its first indication. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | e |
[M]This curvature is studied by general relativity[/M], which predicted the existence of black holes and was its first indication. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | e |
The gravity of a black hole, or "space-time curvature," causes [M]a singularity surrounded by a closed surface, called the event horizon[/M]. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
The gravity of a black hole, or [M]"space-time curvature," causes a singularity surrounded by a closed surface[/M], called the event horizon. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]The gravity of a black hole[/M], or "space-time curvature," [M]causes a singularity surrounded by a closed surface[/M], called the event horizon. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]The gravity of a black hole, or "space-time curvature,"[/M] causes a singularity surrounded by a closed surface, called the event horizon. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]This is predicted by the Einstein field equations[/M]. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]The event horizon[/M] separates the black hole region from the rest of the universe, and [M]no[/M] particle [M]can exit from it[/M], including [M]photons[/M]. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]The event horizon[/M] separates the black hole region from the rest of the universe, and [M]no particle can exit from it[/M], including photons. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]The event horizon separates the black hole region from the rest of the universe[/M], and no particle can exit from it, including photons. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | e |
[M]In the 1970s[/M], Stephen Hawking, Ellis, and [M]Penrose proved several important theorems about the occurrence and geometry of black holes[/M]. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]In the 1970s[/M], Stephen Hawking, [M]Ellis[/M], and Penrose [M]proved several important theorems about the occurrence and geometry of black holes[/M]. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]In the 1970s, Stephen Hawking[/M], Ellis, and Penrose [M]proved several important theorems about the occurrence and geometry of black holes[/M]. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
The [M]radiation emitted by[/M] black holes like [M]Cygnus X-1 does not come from the black hole itself[/M] but from its disk. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
The [M]radiation emitted by black holes[/M] like Cygnus X-1 does not come from the black hole itself but from its disk. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk[/M]. | A black hole is a region of spacetime where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which you cannot escape is called the event horizon. Although the event horizon has a huge effect on the fate and circumstances of an object passing through it, it has no detectable local characteristics. In many ways, a black hole acts like an ideal black body because it doesn't reflect light. Furthermore, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a blackbody with a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for stellar-mass black holes, making it virtually impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were there are widely considered a mathematical curiosity; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | n |
[M]General relativity theory predicts that a sufficiently compact mass can deform spacetime[/M] to form a black hole. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]General relativity theory predicts that a sufficiently compact mass can deform spacetime to form a black hole[/M]. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century[/M] by John Michell and Pierre-Simon Laplace. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]Objects whose gravitational fields are too strong for light to escape were first considered[/M] in the 18th century [M]by[/M] John Michell and [M]Pierre-Simon Laplace[/M]. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]Objects whose gravitational fields are too strong for light to escape were first considered[/M] in the 18th century [M]by John Michell[/M] and Pierre-Simon Laplace. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
In many ways, [M]a black hole[/M] acts like an ideal black body because it [M]doesn't reflect light.[/M] | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | c |
In many ways, [M]a black hole acts like an ideal black body[/M] because it doesn't reflect light. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
Furthermore, [M]quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation[/M], with the same spectrum as a blackbody [M]with a temperature inversely proportional to its mass.[/M] | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
Furthermore, [M]quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation[/M], [M]with the same spectrum as a blackbody[/M] with a temperature inversely proportional to its mass. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
Furthermore, [M]quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation[/M], with the same spectrum as a blackbody with a temperature inversely proportional to its mass. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
The first modern solution of general relativity that would characterize a black hole was found by [M]Karl Schwarzschild[/M] in 1916, although his [M]interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958[/M]. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
The first modern solution of general relativity that would characterize a black hole was found by [M]Karl Schwarzschild[/M] in 1916, although his [M]interpretation as a region of space from which nothing can escape[/M] was first published by David Finkelstein in 1958. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]The first modern solution of general relativity that would characterize a black hole was found[/M] by Karl Schwarzschild [M]in 1916[/M], although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild[/M] in 1916, although his interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]Black holes[/M] were there are widely considered a mathematical curiosity; it was [M]in the 1960s that theoretical work showed that they were a general prediction of general relativity.[/M] | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]Black holes[/M] were there are widely considered a mathematical curiosity; it was in the 1960s that [M]theoretical work showed that they were a general prediction of general relativity.[/M] | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | e |
[M]Black holes[/M] were there [M]are widely considered a mathematical curiosity[/M]; it was in the 1960s that theoretical work showed that they were a general prediction of general relativity. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]A black hole is a region of spacetime where the gravitational field is so intense that[/M] nothing—[M]no[/M] particles or [M]electromagnetic radiation like light—can escape it.[/M] | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | e |
[M]A black hole is a region of spacetime where the gravitational field is so intense that[/M] nothing—[M]no particles[/M] or electromagnetic radiation like light—[M]can escape it.[/M] | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | e |
[M]A black hole is a region of spacetime where the gravitational field is so intense that nothing[/M]—no particles or electromagnetic radiation like light—[M]can escape it.[/M] | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | e |
[M]A black hole is a region of spacetime[/M] where the gravitational field is so intense that nothing—no particles or electromagnetic radiation like light—can escape it. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | e |
[M]This temperature[/M] is on the order of billionths of a kelvin for stellar-mass black holes, making it [M]virtually impossible to observe[/M]. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]This temperature is on the order of billionths of a kelvin for stellar-mass black holes[/M], making it virtually impossible to observe. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]This temperature is on the order of billionths of a kelvin[/M] for stellar-mass black holes, making it virtually impossible to observe. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]The boundary of the region from which you cannot escape is called the event horizon[/M]. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | e |
Although [M]the event horizon[/M] has a huge effect on the fate and circumstances of an object passing through it, it [M]has no detectable local characteristics[/M]. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
Although [M]the event horizon has a huge effect on the[/M] fate and [M]circumstances of an object passing through it[/M], it has no detectable local characteristics. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | e |
Although [M]the event horizon has a huge effect on the fate[/M] and circumstances [M]of an object passing through it[/M], it has no detectable local characteristics. | A black hole is a finite region of space within which there is a concentration of mass high enough to generate a gravitational field such that no material particle, not even light, can escape from it. (In 2021, reflections of light were observed in the farthest part of the black hole.) Black holes may be capable of emitting one type of radiation, Hawking radiation, conjectured by Stephen Hawking in the 1970s. The radiation emitted by black holes like Cygnus X-1 does not come from the black hole itself but from its disk. accretion.
The gravity of a black hole, or "space-time curvature," causes a singularity surrounded by a closed surface, called the event horizon. This is predicted by the Einstein field equations. The event horizon separates the black hole region from the rest of the universe, and no particle can exit from it, including photons. This curvature is studied by general relativity, which predicted the existence of black holes and was its first indication. In the 1970s, Stephen Hawking, Ellis, and Penrose proved several important theorems about the occurrence and geometry of black holes. | n |
[M]This time[/M], [M]the stats shared concern just 2018[/M] rather than your entire history with PS4. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
This time, [M]the stats shared concern just 2018[/M] rather than your entire history with PS4. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
This time, [M]the stats shared[/M] concern just 2018 rather than your entire history with PS4. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
[M]Hopefully Sony can expand the reach to all PSN accounts rather than just North America[/M]. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | n |
[M]Hopefully Sony can expand the reach to all PSN accounts[/M] rather than just North America. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | n |
[M]These include[/M] your total trophy count, the titles you played the most, how much time you spent playing games, even [M]which time of day was your most common period for gaming[/M]. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | n |
[M]These include[/M] your total trophy count, the titles you played the most, [M]how much time you spent playing games[/M], even which time of day was your most common period for gaming. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
[M]These include[/M] your total trophy count, the [M]titles you played the most[/M], how much time you spent playing games, even which time of day was your most common period for gaming. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
[M]These include your total trophy count[/M], the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
Those in North America unfortunately missed out on this, but now, [M]another website enables US users to get their very own batch of stats.[/M] | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
[M]Those in North America unfortunately missed out on this[/M], but now, another website enables US users to get their very own batch of stats. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
Last year, Sony opened a webpage where [M]European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan.[/M] | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
[M]Last year, Sony opened a webpage where European PS4 owners could create a video[/M], describing various interesting statistics about their gaming habits over the console's lifespan. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | e |
[M]There are also reports of people receiving[/M] an email with this information, as well as [M]a code for three dynamic themes for your PS4.[/M] | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | n |
[M]There are also reports of people receiving an email with this information[/M], as well as a code for three dynamic themes for your PS4. | PS4 gaming stats for 2018 have been revealed for gamers in the US and Europe. Last year Sony launched the My PS4 Life feature, which created a bespoke video for PS4 users showing their major stats and milestones. From the amount of trophies they earned to the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers. However, the My PS4 Life feature only launched at the end of last year in Europe - with those in North America missing out.
But now, thankfully for PlayStation 4 fans in that region, another website has launched for US gamers. The brand new Wrap Up website launched this week for PS4 gamers in the US. Much like My PS4 Life, Wrap Up gives PS4 fans a pretty comprehensive rundown of major stats and milestones. It shows PS4 gamers how many titles they’ve played, trophies earned and which games they spent the most time with it.
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. If you’re a gamer in the US wanting to check our your PlayStation stats, click here to head to the Wrap Up website. | n |
[M]It shows PS4 gamers[/M] how many titles they’ve played, trophies earned and [M]which games they spent the most time with it.[/M] | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | e |
[M]It shows PS4 gamers how many[/M] titles they’ve played, [M]trophies earned[/M] and which games they spent the most time with it. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | e |
[M]It shows PS4 gamers how many titles they’ve played[/M], trophies earned and which games they spent the most time with it. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | n |
However, [M]the My PS4 Life feature[/M] only launched at the end of last year in Europe - [M]with those in North America missing out.[/M] | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | e |
However, [M]the My PS4 Life feature only launched at the end of last year in Europe[/M] - with those in North America missing out. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | n |
From the amount of trophies they earned to [M]the total number of hours they played on the PS4, My PS4 Life was a nice, personalised touch for gamers[/M]. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | n |
[M]From the amount of trophies they earned[/M] to the total number of hours they played on [M]the PS4, My PS4 Life was a nice, personalised touch for gamers[/M]. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | n |
But now, thankfully for [M]PlayStation 4 fans[/M] in that region, [M]another website has launched for US gamers[/M]. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | e |
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
[M]It[/M] even [M]shows which genre a PS4 owner has played the most during 2018[/M]. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | n |
PS4 gaming stats 2018 - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
[M]It[/M] even [M]shows which genre a PS4 owner has played the most[/M] during 2018. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | n |
[M]PS4 gaming stats 2018[/M] - How to get your PS4 gaming stats from Wrap Up or My PS4 Life
It even shows which genre a PS4 owner has played the most during 2018. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | n |
Last year Sony launched [M]the My PS4 Life feature[/M], which created a bespoke video [M]for PS4 users showing their[/M] major stats and [M]milestones[/M]. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | n |
Last year Sony launched [M]the My PS4 Life feature[/M], which created a bespoke video for [M]PS4 users showing their major stats[/M] and milestones. | Last year, Sony opened a webpage where European PS4 owners could create a video, describing various interesting statistics about their gaming habits over the console's lifespan. Those in North America unfortunately missed out on this, but now, another website enables US users to get their very own batch of stats.
This time, the stats shared concern just 2018 rather than your entire history with PS4. Click here to go to the website where, once you've signed into your PSN account, you'll be treated to various neat statistics from last year. These include your total trophy count, the titles you played the most, how much time you spent playing games, even which time of day was your most common period for gaming. It's a nifty page if you interested in that sort of thing. Hopefully Sony can expand the reach to all PSN accounts rather than just North America. Better yet -- let's get this sort of information on the console itself.
There are also reports of people receiving an email with this information, as well as a code for three dynamic themes for your PS4. So, if you have a US account, check your inbox or visit the website to check out your 2018 stats. | n |
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