Temperature
5627 K
5586.7 to 5627
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Stellar HostProfile
HD 140901
G6IV • 15.25 pc
Records
12
literature rows
Planets
2
system count
References
13
distinct source labels
HD: HD 140901HIP: HIP 77358TIC: TIC 179348425
Approximate color
from effective temperature
Canonical Summary
Adopted host values from one source row
Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.
Stellar source: Turnbull 2015 • System source: TICv8
Mass
0.99 Msun
0.95 to 1.06
Radius
0.95 Rsun
0.95 to 0.96
Age
4.16 Gyr
3.20 to 4.16
Luminosity
-0.06 log(Lsun)
-0.10 to -0.06
Distance
15.25 pc
single adopted value
Spectral Type
G6IV
Multiple classifications reported
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.95 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 140901
0.95 R☉
System Layout
Known planets
2 planets linked to this host
HD 140901 b
Radial Velocity
◌
Discovery
2022
Period
9.02 days
Radius
—
Mass
15.57 M⊕
Eq. Temp
—
HD 140901 c
Radial Velocity
◌
Discovery
2022
Period
14386 days
Radius
—
Mass
572.1 M⊕
Eq. Temp
—
HD 140901 and Its Two Known Planets
HD 140901 is a G6IV star located 49.7 light-years from Earth. It is estimated to be 4.16 billion years old, with a mass of 0.99 solar masses and a radius of 0.95 solar radii. Its temperature is 5630 K, cooler than the Sun's. Two planets are known to orbit this host.
HD 140901 b was discovered in 2022 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. Its minimum mass is 15.6 Earth masses, larger than Earth's, and its orbital period is 9.02 days, the shortest among the listed planets.
HD 140901 c was also discovered in 2022 by radial velocity. Its mass is 572 Earth masses, roughly 1.8 times Jupiter's mass and larger than Earth's. Its orbital period is 14400 days, the longest among the listed planets.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
12
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typedisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 15.25 | Nordstrom et al. 2004 | TICv8 |
| — | — | — | — | — | G7 IV-V | 15.25 | Gray et al. 2006 | TICv8 |
| — | — | — | — | — | G6 IV | 15.25 | Michigan Catalog, Vol. 3 | TICv8 |
| 5610 | 0.95 | — | — | -0.10 | — | 15.25 | Sousa et al. 2008 | TICv8 |
| — | — | — | — | — | G0 | 15.25 | Cannon & Pickering 1918 | TICv8 |
| — | — | — | — | — | — | 15.25 | Henry et al. 1996 | TICv8 |
| 5586.7 | 0.99 | 0.96 | — | -0.09 | — | 15.25 | TICv8 | TICv8 |
| 5627 | 0.99 | 0.95 | 4.16 | -0.06 | G6IV | 15.25 | Turnbull 2015 | TICv8 |
| — | 0.98 | 0.95 | 4.16 | — | — | 15.25 | Takeda et al. 2007 | TICv8 |
| — | 1.06 | — | 3.20 | — | G7 IV | 15.25 | Philipot et al. 2023 | TICv8 |
| — | — | — | — | — | — | 15.25 | Valenti & Fischer 2005 | TICv8 |
| — | 0.99 | — | — | — | — | 15.25 | Feng et al. 2022 | TICv8 |