Ross 128
Star
Ross 128 — a quiet red dwarf (M4V) 11 light-years away in Virgo, and the host of the second-closest known temperate exoplanet after Proxima b. Unusually inactive for its type — it flares rarely — which makes its planet an interesting target. About 17% of the Sun's mass.
Open in 3D viewSee Ross 128 in the live, interactive 3D map
Key facts
Mass
3.34 × 10²⁹ kg
0.168 M☉
Radius
137,053 km
20% of the Sun's radius
Surface temperature
3,192 K (2,919 °C)
Luminosity
1.39 × 10²⁴ W
Spectral type
M4V (red dwarf; variable FI Virginis)
Science
Physical
- Mass
- 3.34 × 10²⁹ kg · 0.168 M☉
- Radius
- 137,053 km · 20% of the Sun's radius
- Density
- 30,987 kg/m³ · 31× water
- Computed from mass and radius
- Spectral type
- M4V (red dwarf; variable FI Virginis)
Motion through space
- Proper motion
- 1.37 arcseconds per year · its drift across our sky
- SIMBAD — 2020yCat.1350....0G, 2018MNRAS.475.1960F
- Radial velocity
- -30.7 km/s · approaching the Sun
- SIMBAD — 2020yCat.1350....0G, 2018MNRAS.475.1960F
- Speed across our line of sight
- 21.8 km/s
- Computed from proper motion and parallax
- Speed through space, relative to the Sun
- 37.6 km/s
- Computed from proper motion, parallax and radial velocity
Rotation
- Note
- Rotates slowly (~120 days) and is comparatively inactive for a red dwarf.
Composition
- By mass
- A red dwarf about 17% of the Sun's mass, radiating ~0.4% of its light. Unusually quiet magnetically — it flares only rarely — which is part of why its temperate planet is of such interest.
Temperature
- Surface
- 3,192 K (2,919 °C)
Radiation & temperature
- Luminosity
- 1.39 × 10²⁴ W · 0.00362 L☉
- Surface temperature
- 3,192 K (2,919 °C)
- Peak wavelength
- 908 nm · near-infrared (mostly invisible to the eye)
- Computed (Wien's law) from the surface temperature
Discovery & history
- Discovered
- 1926
- By
- Frank Elmore Ross
- Method
- Telescope
- Name
- Named for the American astronomer Frank Elmore Ross and its catalogue number; its variable-star name is FI Virginis.
Catalogued by Frank Elmore Ross in 1926 (entry 128). In 2017 ESO's HARPS spectrograph revealed a temperate planet, Ross 128 b, orbiting this comparatively calm star.
Images
Images from open archives · credit shown per image