Temperature
6095 K
5974 to 6161
←Back to Stellar Hosts
Stellar HostProfile
HD 75289
G0V • 29.12 pc
Records
19
literature rows
Planets
1
system count
References
20
distinct source labels
TIC: TIC 181741837HD: HD 75289HIP: HIP 43177
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
1.19 Msun
1.12 to 1.29
Radius
1.28 Rsun
1.23 to 1.31
Age
3.28 Gyr
3.28 to 15
Luminosity
0.33 log(Lsun)
0.28 to 0.33
Distance
29.12 pc
single adopted value
Spectral Type
G0V
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.28 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 75289
1.28 R☉
System Layout
Known planets
1 planets linked to this host
HD 75289 b
Radial Velocity
◌
Discovery
1999
Period
3.51 days
Radius
—
Mass
155.7 M⊕
Eq. Temp
—
HD 75289 and Its Solitary Known Planet
HD 75289 is a G0V star 95 light-years away, a Sun-like dwarf with one known planet in its cataloged system. The radial velocity method, which measures the wobble a planet's gravity induces in its star's motion, revealed HD 75289 b in 1999.
HD 75289 b has a minimum mass of 156 Earth masses, meaning its true mass is at least that great, and orbits in 3.51 days. Its minimum mass is larger than Earth's.
The host star is 3.28 billion years old, with a mass of 1.19 solar masses, a radius of 1.28 solar radii, and a temperature of 6100 K. Its mass and radius estimates are larger than the Sun's, and it is hotter than the Sun.
Provenance
Underlying measurements and references
Evidence Summary
Rows
19
Stellar refs
19
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 |
|---|---|---|---|---|---|---|---|---|
| — | 1.19 | 1.28 | 3.28 | — | — | 29.12 | Takeda et al. 2007 | TICv8 |
| — | — | — | — | — | — | 29.12 | Valenti & Fischer 2005 | TICv8 |
| 6139 | — | — | — | — | — | 29.12 | Suárez-Andrés et al. 2016 | TICv8 |
| 6095 | 1.19 | 1.28 | 3.28 | 0.33 | G0V | 29.12 | Turnbull 2015 | TICv8 |
| — | 1.15 | — | — | — | — | 29.12 | Butler et al. 2001 | TICv8 |
| — | — | — | — | — | G0 | 29.12 | Cannon & Pickering 1918 | TICv8 |
| 6095 | 1.21 | — | — | — | — | 29.12 | Butler et al. 2006 | TICv8 |
| 6000 | 1.15 | — | 5.60 | — | G0 | 29.12 | Udry et al. 2000 | TICv8 |
| — | — | — | — | — | G0 V | 29.12 | Michigan Catalog, Vol. 2 | TICv8 |
| 6161 | 1.24 | — | — | 0.28 | — | 29.12 | Sousa et al. 2008 | TICv8 |
| 5974 | 1.20 | 1.31 | 3.50 | 0.29 | — | 29.12 | Ghezzi et al. 2010 | TICv8 |
| 6143 | 1.23 | — | — | — | — | 29.12 | Santos et al. 2004 | TICv8 |
| 6044.3 | 1.12 | 1.30 | — | 0.31 | — | 29.12 | TICv8 | TICv8 |
| — | — | — | 15 | — | — | 29.12 | Sanz-Forcada et al. 2010 | TICv8 |
| 6107 | — | 1.28 | — | 0.31 | — | 29.12 | Gaia DR2 | TICv8 |
| 6117 | 1.29 | 1.23 | — | — | — | 29.12 | Stassun et al. 2017 | TICv8 |
| — | — | — | — | — | — | 29.12 | Henry et al. 1996 | TICv8 |
| — | — | — | — | — | — | 29.12 | Nordstrom et al. 2004 | TICv8 |
| — | — | — | — | — | F9 V Fe+0.3 | 29.12 | Gray et al. 2006 | TICv8 |