HD 202772 Ab is a hot Jupiter orbiting the brighter component of the visual binary star HD 202772, located in the constellation Capricornus at a distance of about 480 light-years from Earth. The discovery was announced on 5 October 2018. HD 202772 Ab orbits its host star once every 3.3 days. It is an inflated hot Jupiter, and a rare example of hot Jupiters around evolved stars. It is also one of the most strongly irradiated planets known, with an equilibrium temperature of . References
Bron en licentie
Gebaseerd op: Wikipedia — HD 202772 Ab · auteursgeschiedenis.
Tekst: CC BY-SA 4.0.
Over de bewerking
Wikisyntaxis en sjablonen zijn verwijderd; langere teksten zijn ingekort.