Temperature
6072 K
5990.7 to 6072
F9 • 55.52 pc
Records
3
literature rows
Planets
1
system count
References
4
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: Sreenivas et al. 2022 • System source: TICv8
Temperature
6072 K
5990.7 to 6072
Mass
1.28 Msun
1.10 to 1.28
Radius
2.22 Rsun
2.22 to 2.28
Age
3.68 Gyr
single adopted value
Luminosity
0.79 log(Lsun)
0.78 to 0.79
Distance
55.52 pc
single adopted value
Spectral Type
F9
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 2.22 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 103891
2.22 R☉
System Layout
1 planets linked to this host
Radial Velocity
Discovery
2022
Period
1919 days
Radius
—
Mass
457.7 M⊕
Eq. Temp
—
HD 103891 is a star 181 light-years away with a spectral type of F9. It hosts one planet. The star is 3.68 billion years old and has 1.28 solar masses, 2.22 solar radii, and a temperature of 6070 K. Its mass and radius estimates are larger than the Sun's, and its temperature is hotter than the Sun's.
The planet HD 103891 b was discovered in 2022 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. The planet has a minimum mass of 458 Earth masses, a lower bound on its true mass that is larger than Earth's and roughly 1.44 times Jupiter's mass. Its orbital period is 1920 days.
Provenance
Evidence Summary
Rows
3
Stellar refs
3
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6072 | 1.28 | 2.22 | 3.68 | 0.79 | F9 | 55.52 | Sreenivas et al. 2022 | TICv8 |
| 5990.7 | 1.10 | 2.28 | — | 0.78 | — | 55.52 | TICv8 | TICv8 |
| 6072 | 1.28 | — | — | — | F8 V | 55.52 | Xiao et al. 2023 | TICv8 |