GJ 676 A is 52.3 light-years from the Sun. The NASA Exoplanet Archive lists 4 planets around this M0 star; the first was found in 2010 by radial velocity (La Silla Observatory).
Fly there in 3DGJ 676 A d goes round its star every 3.60 days, 24 times as often as Mercury goes round the Sun.
GJ 676 A is one of 2 stars in its system: the other is drawn where the Washington Double Star Catalog measures it on the sky.
| Spectral type | M0 |
| Surface temperature | 3,734 K |
| Mass | 0.626 solar masses |
| Radius | 0.69 solar radii |
| Luminosity | 0.09068 times the Sun |
| Apparent magnitude | 9.58 |
| Distance from the Sun | 52.3 light-years (16.0 parsecs) |
| Position (J2000) | RA 262.5449°, Dec -51.6378° |
| Constellation | Ara |
GJ 676 B is a M3V star of magnitude 13.37, judged a true companion. In 2016 it was 47.6″ from GJ 676 A, at position angle 101° (Washington Double Star Catalog, 17302-5138 LDS 599): 763 AU on the sky at this distance. The true distance can only be larger.
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| GJ 676 A d | 3.60 days | 0.0390 AU | 1.78 R⊕ estimated | 3.8139 M⊕ minimum | Radial Velocity, 2012 |
| GJ 676 A e | 35.5 days | 0.181 AU | 2.47 R⊕ estimated | 6.6744 M⊕ minimum | Radial Velocity, 2012 |
| GJ 676 A b | 2.9 years | 1.735 AU | 12.8 R⊕ estimated | 1840.9 M⊕ | Radial Velocity, 2010 |
| GJ 676 A c | 38.1 years | 9.726 AU | 12.3 R⊕ estimated | 4288.1 M⊕ | Radial Velocity, 2016 |
Values are the NASA Exoplanet Archive’s composite parameters. A radius marked estimated comes from a mass–radius relation; a mass marked minimum is M sin i. Planet sizes and colours in the 3D view are renderings: none of these worlds has been photographed as more than a point of light.