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Exoplanet HD 202432 b
Exoplanet HD 202432 b orbits star HD 202432 that lies 527 light years away from the Sun.
It weighs about 604.023 Earth masses and orbits its star further than Earth orbits Sun.
Sun distance
527 light years
527 light years
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HD 202432 b
Exoplanet, gas giant
Star: HD 202432
Distance from the star: 1.2 AU
Orbit around star: 418.8 days
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Orbital period
Orbital period of exoplanet HD 202432 b around its star is 418.8 days (or 1.1 years).
The orbital period of an exoplanet is the time it takes to complete one full orbit around its star, usually measured in days. Most of the exoplanets discovered so far have orbital periods of less than one year...
More about Orbital period in StellarGuide
Eccentricity: 0.21Basic characteristic
Mass: 604.023 M Earth
| 1.9006 M Jupiter
Exoplanet mass
Exoplanet HD 202432 b has 604.023 Earth masses (or 1.9006 Jupiter masses).
The mass of an exoplanet is one of the most important characteristics for understanding what kind of world it is — whether it’s small and rocky like Earth or large and gaseous like Jupiter. Mass provides key information about the planet’s composition, gravity, and formation history...
More about Exoplanet mass in StellarGuide
Year of discovery: 2018 (radial velocity)
Other designations of this exoplanet
HIP 104632 b
HIP 104632 b
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HD 202432 system structure
Exoplanet HD 202432 b orbits star HD 202432, which has bigger mass than Sun. It is the only known exoplanet orbiting this star
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HD 202432 | ||||||||
| HD 202432 b | 1.2 AU | 604 M⊕ | 418.8 days | ||||||
Comparison
When comparing to the Solar system planets, HD 202432 b has 1.9 times the mass of Jupiter and it orbits its star between distances of Earth and Mars from the Sun.
| Mercury | Venus | Earth | Mars | Jupiter | Saturn | Uranus | Neptune | ||
|---|---|---|---|---|---|---|---|---|---|
|
Mass | 10982.24 | 741.13 | 604.02 | 5491.12 | 1.9 | 6.34 | 41.37 | 35.12 |
|
Distance | 3.08 | 1.66 | 1.2 | 0.79 | 0.23 | 0.13 | 0.06 | 0.04 |
Habitability
Habitable zone of the star: 7.8 - 11.2 AU
The planet is too hot to sustain liquid water.