page:  = WASP @-@ 44 = 
   
   WASP @-@ 44 is a G @-@ type star in constellation Cetus that has the Jupiter @-@ size planet WASP @-@ 44b in orbit . The star is slightly less massive and slightly smaller than the Sun ; it is also slightly cooler , but is more metal @-@ rich . The star was observed by SuperWASP , an organization in search of planets , starting in 2009 ; manual follow @-@ up observations used WASP @-@ 44 's spectrum and measurements of its radial velocity led to the discovery of the transiting planet WASP @-@ 44b . The planet and its star were presented along with WASP @-@ 45b and WASP @-@ 46b on May 17 , 2011 by a team of scientists testing the idea that Hot Jupiters tend to have circular orbits , an assumption that is made when the orbital eccentricity of such planets are not well @-@ constrained . 
   
   = = Observational history = = 
   
   WASP @-@ 44 was observed between July and November 2009 by the WASP @-@ South , a station of the SuperWASP planet @-@ searching program based at the South African Astronomical Observatory . Observations of the star revealed a periodic decrease in its brightness . WASP @-@ South , along with the SuperWASP @-@ North station at the Roque de los Muchachos Observatory on the Canary Islands , collected 15 @,@ 755 photometric observations , allowing scientists to produce a more accurate light curve . Another set of observations yielded a 6 @,@ 000 point photometric data set , but the light curve was prepared late and was not considered in the discovery paper . 
   In 2010 , a European science team investigated the star using the CORALIE spectrograph and collected seventeen spectra of WASP @-@ 44 . From the spectra , radial velocity measurements were extrapolated . Analysis of collected CORALIE data ruled out the possibility that the detected radial velocity was caused by the blended spectrum of a spectroscopic binary star , supporting the possibility that the body orbiting WASP @-@ 44 was indeed a planet , designated WASP @-@ 44b . 
   The Leonhard Euler Telescope at La Silla Observatory in Chile was used to follow up on the discovery circling WASP @-@ 44 , searching for a point at which the planet transited , or crossed in front of , its host star . One transit was detected . 
   WASP @-@ 44 , its recently discovered planet , the planets orbiting WASP @-@ 45 and WASP @-@ 46 , and a discussion exploring the validity of the common assumption amongst scientists that closely orbiting Hot Jupiter planets have highly circular orbits unless proven otherwise , were reported in a single discovery paper that was published on May 17 , 2011 by the Royal Astronomical Society . The paper was submitted to the Monthly Notices of the Royal Astronomical Society on May 16 , 2011 . 
   
   = = Characteristics = = 
   
   WASP @-@ 44 is a G @-@ type star ( the same class of star as the Sun ) that is located in the Cetus constellation . WASP @-@ 44 has a mass that is 0 @.@ 951 times that of the Sun . In terms of size , WASP @-@ 44 has a radius that is 0 @.@ 927 times that of the Sun . WASP @-@ 44 has an effective temperature of 5410 K , cooler than the Sun . However , the star is metal @-@ rich with relation to the Sun . Its measured metallicity is [ Fe / H ] = 0 @.@ 06 , or 1 @.@ 148 times that the amount of iron found in the Sun . WASP @-@ 44 's chromosphere ( outermost layer ) is not active . The star also does not rotate at a high velocity . 
   The star has an apparent magnitude of 12 @.@ 9 . It cannot be seen from Earth with the naked eye . 
   
   = = Planetary system = = 
   
   There is one known planet in the orbit of WASP @-@ 44 : WASP @-@ 44b . The planet is a Hot Jupiter with a mass of 0 @.@ 889 Jupiters . Its radius is 1 @.@ 14 times that of Jupiter . WASP @-@ 44b orbits its host star every 2 @.@ 4238039 days at a distance 0 @.@ 03473 AU , approximately 3 @.@ 47 % the mean distance between the Earth and Sun . With an orbital inclination of 86.02º , WASP @-@ 44b has an orbit that exists almost edge @-@ on to its host star with respect to Earth . WASPA @-@ 44b 's orbital eccentricity is fit to 0 @.@ 036 , indicating a mostly circular orbit . 
   
   