Temperature
3799 K
3671 to 3799
M1.0 V • 16.97 pc
Records
4
literature rows
Planets
1
system count
References
5
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Gorrini et al. 2023 • System source: TICv8
Temperature
3799 K
3671 to 3799
Mass
0.53 Msun
0.46 to 0.54
Radius
0.52 Rsun
0.52 to 0.55
Luminosity
-1.29 log(Lsun)
-1.30 to -1.29
Distance
16.97 pc
single adopted value
Spectral Type
M1.0 V
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.52 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
GJ 724
0.52 R☉
System Layout
1 planets linked to this host
Radial Velocity
Discovery
2023
Period
5.10 days
Radius
—
Mass
10.75 M⊕
Eq. Temp
611 K
GJ 724 is a star 55.3 light-years from Earth with a spectral type of M1.0 V, making it a small, cool red dwarf. The star has a reported mass estimate of 0.527 solar masses and a radius estimate of 0.522 solar radii, both smaller than the Sun's. Its reported temperature is 3800 K, cooler than the Sun's. One planet is known to orbit this host.
That planet, GJ 724 b, was discovered in 2023 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. GJ 724 b has a minimum mass of 10.8 Earth masses, larger than Earth's, and an orbital period of 5.1 days. A minimum mass is a lower bound on a planet's true mass, distinct from an ordinary mass estimate.
Provenance
Evidence Summary
Rows
4
Stellar refs
4
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 3671 | 0.46 | 0.55 | — | -1.30 | M | 16.97 | Turnbull 2015 | TICv8 |
| 3799 | 0.53 | 0.52 | — | -1.29 | M1.0 V | 16.97 | Gorrini et al. 2023 | TICv8 |
| — | — | — | — | — | M1 | 16.97 | Hawley et al. 1996 | TICv8 |
| — | 0.54 | 0.54 | — | — | — | 16.97 | TICv8 | TICv8 |