Top Qs
Timeline
Chat
Perspective
WASP-58
High proper motion star in the constellation Lyra From Wikipedia, the free encyclopedia
Remove ads
WASP-58 is a binary star system in the constellation Lyra. It comprises a G-type main-sequence star and a red dwarf at a separation of 384 astronomical units. WASP-58 is slightly depleted in heavy elements, having 80% of the solar abundance of iron. The system is much older than the Sun at 12.80+0.20
−2.10 billion years. Based on parallax measurements, it lies at a distance of 960 light-years (290 parsecs).
Lithium was detected in the stellar spectrum of WASP-58A, making the star anomalous for its advanced age.[3]
A multiplicity survey in 2015 detected a red dwarf stellar companion[9] at a projected separation of 1.281±0.002″ to WASP-58A, and it was confirmed to be gravitationally bound in 2016.[4]
Remove ads
Planetary system
In 2012 a transiting hot Jupiter planet, WASP-58b, was detected on a tight, circular orbit around the primary star WASP-58A.[3] The planetary equilibrium temperature is 1270±80 K.[3]
Remove ads
References
Wikiwand - on
Seamless Wikipedia browsing. On steroids.
Remove ads