Temperature
5058 K
4744.9 to 5058
Unclassified star • 62.77 pc
Records
15
literature rows
Planets
2
system count
References
16
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: Jofré et al. 2015 • System source: TICv8
Temperature
5058 K
4744.9 to 5058
Mass
1.37 Msun
1.03 to 1.91
Radius
2.81 Rsun
2.62 to 3.58
Age
3.46 Gyr
3.24 to 4.40
Luminosity
0.60 log(Lsun)
0.60 to 0.77
Distance
62.77 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Current adopted radius: 2.81 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 177830
2.81 R☉
System Layout
2 planets linked to this host
Radial Velocity
Discovery
1999
Period
410.1 days
Radius
—
Mass
537.1 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2010
Period
110.9 days
Radius
—
Mass
47.67 M⊕
Eq. Temp
—
HD 177830 is a K0 star located 205 light-years away. Its reported mass is 1.37 solar masses and its reported radius is 2.81 solar radii, both larger than the Sun's corresponding values. The star's reported temperature of 5060 K is cooler than the Sun's, and its age is given as 3.46 billion years. Two planets have been found around this star.
HD 177830 b was discovered in 1999 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. The planet's minimum mass is 537 Earth masses and its orbital period is 410 days; among the listed planets, it has the longest year. That minimum mass is larger than Earth's and is roughly 1.69 times Jupiter's mass.
HD 177830 c was discovered in 2010, also by radial velocity. Its minimum mass is 47.7 Earth masses and its orbital period is 111 days; among the listed planets, it has the shortest year and the smallest minimum mass. Its minimum mass is likewise larger than Earth's, while the minimum mass of HD 177830 b remains the largest among the listed planets.
A minimum mass is a lower bound on a planet's true mass, so these figures represent how light each world could be rather than its exact mass.
Provenance
Evidence Summary
Rows
15
Stellar refs
15
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4949 | 1.47 | 2.62 | 4.40 | 0.69 | — | 62.77 | Meschiari et al. 2011 | TICv8 |
| — | — | — | — | — | — | 62.77 | Valenti & Fischer 2005 | TICv8 |
| 4840 | 1.03 | — | — | — | — | 62.77 | Santos et al. 2003 | TICv8 |
| 4901 | 1.70 | 3.26 | — | — | — | 62.77 | Stassun et al. 2017 | TICv8 |
| — | — | — | — | — | — | 62.77 | Duncan et al. 1991 | TICv8 |
| — | — | — | — | — | K0 | 62.77 | Cannon & Pickering 1918 | TICv8 |
| 4923.8 | — | 3.31 | — | — | — | 62.77 | TICv8 | TICv8 |
| 4847.5 | — | 3.45 | — | 0.77 | — | 62.77 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 62.77 | Nidever et al. 2002 | TICv8 |
| 4804 | — | — | — | — | — | 62.77 | Santos et al. 2004 | TICv8 |
| — | — | — | — | — | — | 62.77 | Wright et al. 2004 | TICv8 |
| 5058 | 1.37 | 2.81 | 3.46 | 0.60 | — | 62.77 | Jofré et al. 2015 | TICv8 |
| 4752 | 1.17 | — | — | — | — | 62.77 | Mortier et al. 2013 | TICv8 |
| — | 1.91 | 2.62 | 3.24 | — | — | 62.77 | Takeda et al. 2007 | TICv8 |
| 4744.9 | 1.32 | 3.58 | — | — | — | 62.77 | Rosenthal et al. 2021 | TICv8 |