Temperature
4799 K
single adopted value
K5 V • 39.74 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: Frensch et al. 2023 • System source: TICv8
Temperature
4799 K
single adopted value
Mass
0.69 Msun
0.69 to 0.80
Radius
0.66 Rsun
0.66 to 0.68
Age
6.90 Gyr
4.30 to 6.90
Luminosity
-0.68 log(Lsun)
-0.68 to -0.66
Distance
39.74 pc
single adopted value
Spectral Type
K5 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 0.66 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HIP 54597
0.66 R☉
System Layout
1 planets linked to this host
Radial Velocity
Discovery
2023
Period
3274 days
Radius
—
Mass
762.8 M⊕
Eq. Temp
—
HIP 54597 is a K5 V star 130 light-years away. Its spectral type marks it as a main-sequence dwarf. The star is 6.9 billion years old, with a mass of 0.69 solar masses and a radius of 0.66 solar radii. Its temperature is 4800 K, and its reported mass, radius, and temperature are all smaller or cooler than the Sun's.
One planet orbits this host. HIP 54597 b was discovered in 2023 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. The planet's mass is 763 Earth masses, roughly 2.4 times Jupiter's mass, and larger than Earth's. Its orbital period is 3270 days.
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 |
|---|---|---|---|---|---|---|---|---|
| 4799 | 0.78 | 0.68 | — | -0.66 | — | 39.74 | TICv8 | TICv8 |
| 4799 | 0.69 | 0.66 | 6.90 | -0.68 | K5 V | 39.74 | Frensch et al. 2023 | TICv8 |
| 4799 | — | 0.68 | — | — | — | 39.74 | ExoFOP | TICv8 |
| — | 0.80 | — | 4.30 | — | K5 V | 39.74 | Philipot et al. 2023 | TICv8 |