Temperature
4884 K
4833 to 4884
K1 III • 94.03 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: Jenkins et al. 2025 • System source: TICv8
Temperature
4884 K
4833 to 4884
Mass
1.30 Msun
1.30 to 1.61
Radius
3.94 Rsun
3.94 to 3.98
Age
4.55 Gyr
single adopted value
Luminosity
0.89 log(Lsun)
0.89 to 0.89
Distance
94.03 pc
single adopted value
Spectral Type
K1 III
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 3.94 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HIP 90988
3.94 R☉
System Layout
1 planets linked to this host
Radial Velocity
Discovery
2021
Period
455.7 days
Radius
—
Mass
668.1 M⊕
Eq. Temp
—
HIP 90988 is a K1 III star located 307 light-years away. The star has a measured age of 4.55 billion years, a mass of 1.3 solar masses, and a radius of 3.94 solar radii, with a temperature of 4880 K. Its reported mass and radius estimates are larger than the Sun's, while its reported temperature is cooler.
One planet is known to orbit this host. HIP 90988 b was discovered in 2021 by 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 668 Earth masses and an orbital period of 456 days. Its minimum mass is larger than Earth's and roughly 2.1 times Jupiter's mass.
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 |
|---|---|---|---|---|---|---|---|---|
| 4884 | 1.30 | 3.94 | 4.55 | 0.89 | K1 III | 94.03 | Jenkins et al. 2025 | TICv8 |
| 4883 | 1.30 | 3.94 | 4.55 | 0.89 | K1 III | 94.03 | Jones et al. 2021 | TICv8 |
| 4833 | — | 3.98 | — | — | — | 94.03 | TICv8 | TICv8 |
| — | 1.61 | — | — | — | — | 94.03 | Feng et al. 2022 | TICv8 |