Exoplanet HIP 63242 b

Exoplanet HIP 63242 b orbits star HIP 63242 that lies 510 light years away from the Sun. It weighs about 2918.377 Earth masses and orbits its star closer than Earth orbits Sun.
Sun distance
510 light years
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iconHIP 63242 b

Exoplanet, gas giant
Star: HIP 63242
icon distanceDistance from the star: 0.565 AU
icon time Orbit around star: 124.6 days +
Orbital period
Orbital period of exoplanet HIP 63242 b around its star is 124.6 days.

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... icon More about Orbital period in StellarGuide
icon timeEccentricity: 0.23

Basic characteristic

icon weight
Mass: 2918.377 M Earth
| 9.1831 M Jupiter
+
Exoplanet mass
Exoplanet HIP 63242 b has 2918.377 Earth masses (or 9.1831 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... icon More about Exoplanet mass in StellarGuide
Other designations of this exoplanet
HIP 63242 b, HD 112410 b, GSC 09001-00513 b, PPM 359773 b, CD-64 676 b, HIC 63242 b, SAO 252106 b, CPC 21 2790 b
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HIP 63242 system structure

Exoplanet HIP 63242 b orbits star HIP 63242, which has bigger mass than Sun. It is the only known exoplanet orbiting this star
HIP 63242
HIP 63242 b 0.57 AU 2918.4 M⊕ 124.6 days

Comparison

When comparing to the Solar system planets, HIP 63242 b has 9.18 times the mass of Jupiter and it orbits its star a little closer than Venus.
Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune
icon mass Mass 53061.43580.832918.3826530.79.1830.66199.89169.67
icon distance Distance1.450.780.570.370.110.060.030.02

Habitability

Habitable zone of the star: 6.7 - 9.6 AU
check icon
The planet is too hot to sustain liquid water.

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