Kepler-90

Kepler-90

Star

Kepler-90 — a yellow-white star a little larger and hotter than the Sun (~1.2 solar masses and radii), ~2,770 light-years away in Draco. Ordinary in itself, it is remarkable for what orbits it: a full family of eight planets, the Solar System's equal.

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

Key facts

Mass
2.39 × 10³⁰ kg
1.2 M☉
Radius
834,840 km
1.2× wider than the Sun
Surface temperature
6,080 K (5,807 °C)
Spectral type
G-type dwarf (a little hotter and larger than the Sun)

Science

Physical

Mass
2.39 × 10³⁰ kg · 1.2 M☉
Radius
834,840 km · 1.2× wider than the Sun
Density
979 kg/m³ · 0.98× water
Computed from mass and radius
Spectral type
G-type dwarf (a little hotter and larger than the Sun)

Motion through space

Proper motion
0.00543 arcseconds per year · its drift across our sky
SIMBAD — 2020yCat.1350....0G, 2022yCat.1355....0G
Radial velocity
-15.5 km/s · approaching the Sun
SIMBAD — 2020yCat.1350....0G, 2022yCat.1355....0G
Speed across our line of sight
22 km/s
Computed from proper motion and parallax
Speed through space, relative to the Sun
27 km/s
Computed from proper motion, parallax and radial velocity

Composition

By mass
A yellow-white main-sequence star of about 1.2 solar masses and radii, hydrogen/helium like the Sun. Notable not for itself but for its full family of eight transiting planets — the only star known to tie the Sun's count.

Temperature

Surface
6,080 K (5,807 °C)

Radiation & temperature

Luminosity
6.79 × 10²⁶ W · 1.77 L☉
Surface temperature
6,080 K (5,807 °C)
Peak wavelength
477 nm · blue light
Computed (Wien's law) from the surface temperature

Discovery & history

Method
Telescope
Name
A Kepler-mission catalogue designation; no proper name.

Monitored by NASA's Kepler telescope, its light showed the tell-tale dips of many transiting planets; seven were confirmed by 2013 and an eighth by machine learning in 2017.

Images

Images from open archives · credit shown per image