dancing with the stars started this season on september 24, 2018.
when did dancing with the stars start this season?
september 24 , 2018
dancing with the stars is an american dance competition television series that premiered on june 1, 2005, on abc. it is the us version of the uk series "strictly come dancing". the show is hosted by tom bergeron, alongside erin andrews, who became co-host in season eighteen. lisa canning was co-host in the first season, samantha harris co-hosted seasons two through nine and brooke burke-charvet in seasons ten through seventeen. the twenty-seventh season premiered on september 24, 2018, and its spin-off "" premiered on october 7, 2018. "dancing with the stars" did not premiere for a spring season in 2019, but is set to return in the fall of 2019.
dancing with the stars (american tv series)
asymptotic-giant-branch (agb) and post-agb stars are highly evolved lower-mass red giants with luminosities that can be comparable to more massive red supergiants, but because of their low mass, being in a different stage of development (helium shell burning), and their lives ending in a different way (planetary nebula and white dwarf rather than supernova), astrophysicists prefer to keep them separate. the dividing line becomes blurred at around (or as high as in some models) where stars start to undergo limited fusion of elements heavier than helium. specialists studying these stars often refer to them as super agb stars, since they have many properties in common with agb such as thermal pulsing. others describe them as low-mass supergiants since they start to burn elements heavier than helium and can explode as supernovae. many post-agb stars receive spectral types with supergiant luminosity classes. for example, rv tauri has an ia (bright supergiant) luminosity class despite being less massive than the sun. some agb stars also receive a supergiant luminosity class, most notably w virginis variables such as w virginis itself, stars that are executing a blue loop triggered by thermal pulsing. a very small number of mira variables and other late agb stars have supergiant luminosity classes, for example α herculis.
supergiant star