Exoplanet HD 69830 c

Exoplanet HD 69830 c orbits star HD 69830 that lies 41 light years away from the Sun. It weighs about 11.8 Earth masses and orbits its star closer than Earth orbits Sun.
Sun distance
41 light years
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iconHD 69830 c

Exoplanet, sub-neptune
Star: HD 69830
icon distanceDistance from the star: 0.186 AU

Basic characteristic

icon weight
Mass: 11.8 M Earth
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Exoplanet mass
Exoplanet HD 69830 c has 11.8 Earth masses, or 0.81 times the mass of Uranus.

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
icon radiusSize: 3.363 R Earth | 0.3 R Jupiter
icon densityDensity: 1711 kg/m3 | 31.04 % Earth
Other designations of this exoplanet
285 G. Puppis c, BD−12°2449 c, Gliese 302 c, GJ 302 c, HIP 40693 c, HR 3259 c, LHS 245 c, SAO 154093 c, 2MASS J08182389-1237541 c, Gaia DR2 5726982995343100928 c
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HD 69830 system structure

Exoplanet HD 69830 c orbits star HD 69830, which has lower mass than Sun. It is one of 3 known exoplanets orbiting this star.
HD 69830
HD 69830 b 0 AU 10.2 M⊕ 3.4 R⊕ -
HD 69830 c 0.19 AU 11.8 M⊕ 3.4 R⊕ -
HD 69830 d 0.63 AU 18.1 M⊕ 4.5 R⊕ -
HD 69830 belt 1 AU (HZ) -

Comparison

When comparing to the Solar system planets, HD 69830 c has 81 % of mass of Uranus and it orbits its star closer than Mercury orbits the Sun.
Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune
icon mass Mass 214.5514.4811.8107.270.040.120.810.69
icon size Size8.783.543.366.350.30.370.840.89
icon density Density0.320.330.310.421.382.461.360.99
icon distance Distance0.480.260.190.120.040.020.010.01

Habitability

Habitable zone of the star: 0.82 - 1.2 AU
check icon
The planet is too hot to sustain liquid water.
question icon
The planet is bigger than Earth and smaller than Neptune. Its average density 1711 kg/m3 points to a hot gas planet.

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