Temperature
5950 K
5906 to 5977.8
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Stellar HostProfile
HD 89307
Unclassified star • 32.01 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 61125572HD: HD 89307HIP: HIP 50473
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: Fischer et al. 2009 • System source: TICv8
Mass
1.03 Msun
1 to 1.27
Radius
1.05 Rsun
1.01 to 1.11
Age
6.76 Gyr
2.31 to 7
Luminosity
0.09 log(Lsun)
0.09 to 0.13
Distance
32.01 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.05 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 89307
1.05 R☉
System Layout
Known planets
1 planets linked to this host
HD 89307 b
Radial Velocity
◌
Discovery
2009
Period
2166 days
Radius
—
Mass
670.6 M⊕
Eq. Temp
—
HD 89307 and Its Solitary Known Planet
HD 89307 is a G-type main-sequence star located 104 light-years from Earth. Its spectral type is G0 V, classifying it as a Sun-like dwarf, and it hosts one known planet. The star has an age of 6.76 billion years, a mass of 1.03 solar masses, and a radius of 1.05 solar radii, making it slightly larger than the Sun. Its temperature of 5950 K is hotter than the Sun's.
The sole known planet, HD 89307 b, was discovered in 2009 using the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. The planet has a minimum mass of 671 Earth masses - a lower bound on its true mass - which is roughly 2.11 times Jupiter's mass. It completes one orbit every 2170 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
Stellar refs
13
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 |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | G0 | 32.01 | Cannon & Pickering 1918 | TICv8 |
| — | — | — | — | — | — | 32.01 | Valenti & Fischer 2005 | TICv8 |
| — | — | — | — | — | — | 32.01 | Nidever et al. 2002 | TICv8 |
| 5906 | 1.05 | 1.01 | 2.31 | 0.11 | — | 32.01 | Liu et al. 2014 | TICv8 |
| 5956.1 | 1.09 | 1.09 | — | 0.13 | — | 32.01 | TICv8 | TICv8 |
| — | 1.03 | — | — | — | — | 32.01 | Boisse et al. 2012 | TICv8 |
| — | — | — | — | — | — | 32.01 | Wright et al. 2004 | TICv8 |
| 5950 | 1.03 | 1.05 | 6.76 | 0.09 | — | 32.01 | Fischer et al. 2009 | TICv8 |
| 5955 | 1.27 | 1.10 | — | — | — | 32.01 | Stassun et al. 2017 | TICv8 |
| 5950 | 1.03 | — | — | — | G0 V | 32.01 | Xiao et al. 2023 | TICv8 |
| 5977.8 | — | 1.08 | — | 0.13 | — | 32.01 | Gaia DR2 | TICv8 |
| 5914 | 1 | 1.11 | 7 | 0.13 | — | 32.01 | Ghezzi et al. 2010 | TICv8 |
| — | — | — | — | — | — | 32.01 | Nordstrom et al. 2004 | TICv8 |