Kepler-87c explained

Kepler-87c
Discoverer:Ofir et al.
Discovered:8 October 2013
Discovery Method:Transit (Kepler Mission)
Apsis:astron
Semimajor:0.664AU
Eccentricity:0.039
Period:191 d
Inclination:89.588
Star:Kepler-87 (KOI-1574)
Mean Radius:6.14±0.29
Mass:6.4±0.8
Density:0.152g/cm3
Single Temperature:403K [1]

Kepler-87c is a planet orbiting Kepler-87, a star slightly more massive than the Sun and nearing the end of its main-sequence period. [1]

Characteristics

Despite being larger than Neptune, Kepler-87c is only about 6.4 times more massive than Earth. This means that its density is only 0.152 g/cm3. This is the first planet with a comparable mass to have such a low density. Its equilibrium temperature is 130 °C.

External links

Notes and References

  1. Web site: The Extrasolar Planet Encyclopaedia — Kepler-87c . . 10 September 2023.