Kepler-90 h

Planet· orbits the Sun

Kepler-90 h — the outermost planet, a Jupiter-size giant (11.3 R⊕) on a 332-day orbit near where Earth sits in our own system. Its measured mass (~203 M⊕) gives a real density somewhat below Jupiter's. The system's giant, it anchors the 'other solar system'. Never imaged.

Open in 3D viewSee Kepler-90 h in the live, interactive 3D map

Key facts

Mass
1.21 × 10²⁷ kg
0.639 M♃ (203 M⊕)
Radius
71,992 km
11.3× wider than Earth
Surface gravity
15.6 m/s²
1.59× Earth's
Year
332 Earth days
0.91 Earth years
Distance from Kepler-90
0.971 AU

Science

Physical

Mass
1.21 × 10²⁷ kg · 0.639 M♃ (203 M⊕)
Radius
71,992 km · 11.3× wider than Earth
Density
776 kg/m³ · 0.78× water
Surface gravity
15.6 m/s² · 1.59× Earth's
Escape velocity
47.4 km/s · 4.24× Earth's

Orbital

Semi-major axis
0.971 AU
Eccentricity
0.0276
Inclination
0.00 °
Orbital period
331.6 days
Perihelion
0.944 AU
Aphelion
0.997 AU
Mean orbital velocity
31.8 km/s

Composition

Bulk composition
A Jupiter-size giant (11.3 R⊕) with a measured mass (~203 M⊕) from transit timing, giving a real density somewhat below Jupiter's. The system's anchor, near where Earth sits in ours. Mass: Shaw et al. 2025; radius: Cabrera et al. 2014.
Cloud appearance
Appearance based on NASA/JPL-Caltech's artist's concept. No spacecraft has imaged this world, so its real appearance is unknown — The banded clouds shown are a representation of its class, shown only in Vision mode; Realism shows a plain spectral colour.

Radiation & temperature

Insolation
1.88 S⊕ · 1.88× the sunlight Earth receives
Equilibrium temperature
294 K (21 °C)

Discovery & history

Method
Transit detection
Name
Designated 'h' under the IAU convention that letters a star's planets 'b', 'c', 'd'... in the order found (the star is the unwritten 'a'); no IAU proper name has been assigned.

The outermost of Kepler-90's eight planets, confirmed in 2013. Its mass is measured from transit-timing variations (Shaw et al. 2025); the radius is the Kepler discovery value (Cabrera et al. 2014, adopted by Shaw).

Images

No telescope has imaged this world — it is known only from the tiny dip it makes crossing its star. Only its host system has been pictured (see the system view); its true surface appearance is unknown.