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Kepler-90e - Exoplanet
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Kepler-90e

description Kepler-90e Overview

Kepler-90e is a confirmed transiting exoplanet orbiting the G-type star Kepler-90. The NASA Exoplanet Archive lists a radius of about 2.66 Earth radii and an orbital period of 91.94 days. Its radius is larger than Earth's but smaller than Neptune's, so the measurement alone does not determine whether its interior is rocky, gaseous, or a mixture. The planet belongs to the eight-planet Kepler-90 system identified in data from NASA's Kepler mission.

help Kepler-90e FAQ

How large is Kepler-90e compared with Earth and Neptune?

Kepler-90e has a radius of about 2.66 Earth radii. That makes it larger than Earth but smaller than Neptune, although radius alone does not reveal its composition.

How long is a year on Kepler-90e?

Kepler-90e completes one orbit around its star in about 91.94 days. Its host star, Kepler-90, is a G-type star similar in broad classification to the Sun.

How was Kepler-90e discovered?

Kepler-90e is a confirmed transiting exoplanet. Its transit was detected when the planet passed in front of Kepler-90 and caused a small, measurable dip in the star's brightness.

Where can I find data about Kepler-90e?

The NASA Exoplanet Archive lists Kepler-90e as a confirmed planet. Its catalog data include an estimated radius of about 2.66 Earth radii and an orbital period near 91.94 days.

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