Temperature
6655 K
6596.1 to 6655
F5 V • 43.41 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: Franson et al. 2023 • System source: TICv8
Temperature
6655 K
6596.1 to 6655
Mass
1.40 Msun
1.30 to 1.40
Age
0.65 Gyr
0.65 to 0.75
Distance
43.41 pc
single adopted value
Spectral Type
F5 V
Consistent across records
Planets
1
Stable across source rows
System Layout
1 planets linked to this host
Imaging
Discovery
2022
Period
22000 days
Radius
—
Mass
7627.9 M⊕
Eq. Temp
1300 K
HIP 21152 is a star 142 light-years from us with a spectral type of F5 V, placing it among the hotter, more massive F-class dwarfs. It is part of a system with two cataloged stars, though its stellar measurements describe the host alone: an age of 0.65 billion years, a mass of 1.4 solar masses, and a temperature of 6660 K. That mass is larger than the Sun's, and the star is likewise hotter than the Sun. One planet orbits this host.
That planet, HIP 21152 b, was discovered by imaging in 2022. Its mass is 7630 Earth masses, roughly 24 times Jupiter's mass and larger than Earth's. It completes an orbit in 22000 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 |
|---|---|---|---|---|---|---|---|---|
| 6655 | 1.40 | — | 0.65 | — | F5 V | 43.41 | Franson et al. 2023 | TICv8 |
| 6596.1 | 1.38 | 1.59 | — | 0.64 | — | 43.41 | TICv8 | TICv8 |
| — | 1.30 | — | 0.75 | — | F5 V | 43.41 | Kuzuhara et al. 2022 | TICv8 |