Kepler-90g
Discovery Transit | |
---|---|
Designations | |
KOI-351 g, KOI-351.02 | |
Orbital characteristics | |
0.71±0.08 AU[1] | |
Eccentricity | 0.049+0.011 −0.007[2] |
210.48+0.05 −0.05 d[2] | |
Inclination | 89.92°+0.03° −0.01°[2] |
90°+20° −20°[2] | |
Star | Kepler-90 |
Physical characteristics | |
Mean radius | 8.1±0.8 R🜨[1] |
Mass | 15.0+0.9 −0.8 M🜨[2] |
Mean density | 0.15±0.05 g/cm3[2] |
Temperature | 349 K (76 °C) |
Kepler-90g (also known by its
Kepler-90g's orbital period changes by 25.7 hours between two consecutive transits, caused by gravitational perturbations from other planets in the system. Additionally, changes in the depth and duration of transit events led to an exomoon being hypothesized to orbit this planet.[1] However, this candidate moon was later found to be a false positive.[4]
A 2020 analysis of transit-timing variations of Kepler-90g and
Host star
The planet orbits a G-type star named Kepler-90, its host star. The star is 1.2 times as massive as the Sun and is 1.2 times as large as the Sun. It is estimated to be 2 billion years old, with a surface temperature of 6080 K. In comparison, the Sun is about 4.6 billion years old[5] and has a surface temperature of 5778 K.[6]
See also
References
- ^ S2CID 118875825.
- ^ S2CID 226975548.
- .
- S2CID 119118726.
- ^ Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 19 February 2011.
- ^ Fraser Cain (15 September 2008). "Temperature of the Sun". Universe Today. Retrieved 19 February 2011.