Exoplanet Kepler 1520 b

Exoplanet Kepler 1520 b orbits star Kepler 1520 that lies 2074 light years away from the Sun. It weighs about 0.02 Earth masses and orbits its star much closer than Earth orbits Sun.
Sun distance
2074 light years
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iconKepler 1520 b

Exoplanet, ultra-short period
icon distanceDistance from the star: 0.013 AU
icon time Orbit around star: 0.653553 days +
Orbital period
Orbital period of exoplanet Kepler 1520 b around its star is 0.653553 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

Basic characteristic

icon weight
Mass: 0.02 M Earth
+
Exoplanet mass
Exoplanet Kepler 1520 b has 0.02 Earth masses, or 0.36 times the mass of Mercury.

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 discoveryYear of discovery: 2016 (transit)
Other designations of this exoplanet
2MASS J19235189+5130170 b, KIC 12557548 b, KOI-3794 b, WISE J192351.88+513017.0 b
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Kepler 1520 system structure

Exoplanet Kepler 1520 b orbits star Kepler 1520, which has lower mass than Sun. It is the only known exoplanet orbiting this star
Kepler 1520
Kepler 1520 b 0.01 AU 0 M⊕ 0.7 days

Comparison

When comparing to the Solar system planets, Kepler 1520 b has 36 % of mass of Mercury and it orbits its star closer than Mercury orbits the Sun.
Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune
icon mass Mass 0.360.020.020.180000
icon distance Distance0.030.020.010.010000

Habitability

Habitable zone of the star: 0.49 - 0.7 AU
check icon
The planet is too hot to sustain liquid water.
check icon
The planet has mass comparable to Earth.

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