Temperature
3803 K
3803 to 3843
M0 V • 10.01 pc
Records
12
literature rows
Planets
2
system count
References
11
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: Luque et al. 2022 • System source: TICv8
Temperature
3803 K
3803 to 3843
Mass
0.44 Msun
0.43 to 0.46
Radius
0.44 Rsun
0.43 to 0.47
Age
5 Gyr
single adopted value
Luminosity
-1.44 log(Lsun)
-1.44 to -1.39
Distance
10.01 pc
single adopted value
Spectral Type
M0 V
Multiple classifications reported
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 0.44 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 260655
0.44 R☉
System Layout
2 planets linked to this host
Transit
Discovery
2022
Period
2.77 days
Radius
1.24 R⊕
Mass
2.14 M⊕
Eq. Temp
709 K
Transit
Discovery
2022
Period
5.71 days
Radius
1.53 R⊕
Mass
3.09 M⊕
Eq. Temp
557 K
HD 260655 is an M0 V star, a small, cool red dwarf, located 32.6 light-years away. Its reported mass and radius are each 0.439 solar masses and 0.439 solar radii, both smaller than the Sun's, and its temperature of 3800 K is cooler than the Sun's. The star is 5 billion years old, and two planets are known to orbit it.
Both planets were discovered by transit in 2022. HD 260655 b is classified as Earth-like, with a radius of 1.24 Earth radii and a mass of 2.14 Earth masses, both larger than Earth's. It completes an orbit in 2.77 days. Its mean density is 6.18 g/cm³, 1.12 times Earth's. Among the listed planets, HD 260655 b has the shortest year, the smallest radius, and the smallest reported mass.
HD 260655 c is classified as a Super-Earth. Its radius is 1.53 Earth radii and its mass is 3.09 Earth masses, each larger than Earth's. It orbits in 5.71 days, and its mean density is 4.73 g/cm³, 0.858 times Earth's. Among the listed planets, HD 260655 c has the longest year, the largest radius, and the largest reported mass.
Provenance
Evidence Summary
Rows
12
Stellar refs
10
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 10.01 | Wright et al. 2004 | TICv8 |
| 3843 | 0.43 | 0.43 | — | -1.40 | M1: | 10.01 | Turnbull 2015 | TICv8 |
| 3803 | 0.44 | 0.44 | 5 | -1.44 | M0 V | 10.01 | Luque et al. 2022 | TICv8 |
| — | 0.46 | 0.47 | — | — | M0 V | 10.01 | Weisserman et al. 2026 | TICv8 |
| 3807 | — | 0.47 | — | — | — | 10.01 | ExoFOP | TICv8 |
| — | — | — | — | — | K7 | 10.01 | Hawley et al. 1996 | TICv8 |
| — | — | — | — | — | — | 10.01 | Duncan et al. 1991 | TICv8 |
| — | — | — | — | — | — | 10.01 | Nidever et al. 2002 | TICv8 |
| 3807 | 0.46 | 0.47 | — | -1.39 | — | 10.01 | TICv8 | TICv8 |
| — | — | — | — | — | — | 10.01 | Duncan et al. 1991 | TICv8 |
| 3807 | — | 0.47 | — | — | — | 10.01 | ExoFOP | TICv8 |
| — | — | — | — | — | K2 | 10.01 | Cannon & Pickering 1918 | TICv8 |