Gliese 667 C

Gliese 667 C

Star

Gliese 667 C - a red dwarf 23.6 light-years away in Scorpius, the smallest member of a triple star system (it orbits a close pair of orange dwarfs about 230 AU away). It hosts two confirmed planets, including a super-Earth in its temperate zone; several further claimed planets remain disputed and are not shown.

Open in 3D viewSee Gliese 667 C in the live, interactive 3D map

Key facts

Mass
6.56 × 10²⁹ kg
0.33 M☉
Radius
292,194 km
42% of the Sun's radius
Surface temperature
3,350 K (3,077 °C)
Luminosity
5.24 × 10²⁴ W
Spectral type
M1.5V (red dwarf)

Science

Physical

Mass
6.56 × 10²⁹ kg · 0.33 M☉
Radius
292,194 km · 42% of the Sun's radius
Density
6,281 kg/m³ · 6.3× water
Computed from mass and radius
Spectral type
M1.5V (red dwarf)

Motion through space

Proper motion
1.15 arcseconds per year · its drift across our sky
SIMBAD — 2020yCat.1350....0G, 2018A&A...616A...7S
Radial velocity
+6.4 km/s · moving away from the Sun
SIMBAD — 2020yCat.1350....0G, 2018A&A...616A...7S
Speed across our line of sight
39.5 km/s
Computed from proper motion and parallax
Speed through space, relative to the Sun
40.1 km/s
Computed from proper motion, parallax and radial velocity

Composition

By mass
A metal-poor red dwarf about 33% of the Sun's mass; the faint third star of the GJ 667 triple.

Temperature

Surface
3,350 K (3,077 °C)

Radiation & temperature

Luminosity
5.24 × 10²⁴ W · 0.0137 L☉
Surface temperature
3,350 K (3,077 °C)
Peak wavelength
865 nm · near-infrared (mostly invisible to the eye)
Computed (Wien's law) from the surface temperature

Discovery & history

Method
Telescope
Name
'Gliese 667 C' is the third (faintest) component of the GJ 667 triple star system in Scorpius.

The bright pair GJ 667 AB has been known for centuries; the faint red companion C was found to host planets by ESO's HARPS from 2011. Claims of up to seven planets (2013) were pared back - only two survive robust scrutiny.

Images

Images from open archives · credit shown per image