Temperature
5843 K
5752 to 5891
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Stellar HostProfile
HD 23127
Unclassified star โข 93.86 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
HD: HD 23127HIP: HIP 17054TIC: TIC 311924816
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: Barbato et al. 2018 โข System source: TICv8
Mass
1.21 Msun
1.05 to 1.42
Radius
1.49 Rsun
1.46 to 1.69
Age
4.51 Gyr
4.51 to 7.68
Distance
93.86 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.49 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
HD 23127
1.49 Rโ
System Layout
Known planets
1 planets linked to this host
HD 23127 b
Radial Velocity
โ
Discovery
2006
Period
1211.2 days
Radius
โ
Mass
485.3 Mโ
Eq. Temp
โ
HD 23127 and Its Planet
HD 23127 is a star 306 light-years away with a spectral type of G5, making it a Sun-like dwarf. It is 4.51 billion years old, has 1.21 solar masses, a radius of 1.49 solar radii, and a temperature of 5840 K. Its reported mass and radius estimates are larger than the Sun's, and its reported temperature is hotter than the Sun's. One planet orbits this host.
That planet, HD 23127 b, was discovered in 2006 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. Its minimum mass is 485 Earth masses, roughly 1.53 times Jupiter's mass, and it completes an orbit every 1210 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
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 |
|---|---|---|---|---|---|---|---|---|
| 5824.2 | 1.05 | 1.64 | โ | 0.45 | โ | 93.86 | TICv8 | TICv8 |
| โ | 1.13 | โ | 7.10 | โ | G2 V | 93.86 | O'Toole et al. 2007 | TICv8 |
| โ | 1.13 | 1.46 | 7.68 | โ | โ | 93.86 | Takeda et al. 2007 | TICv8 |
| 5843 | 1.21 | 1.49 | 4.51 | โ | โ | 93.86 | Barbato et al. 2018 | TICv8 |
| โ | 1.25 | 1.57 | 6 | 0.39 | โ | 93.86 | Ghezzi et al. 2010 | TICv8 |
| 5752 | โ | 1.69 | โ | 0.45 | โ | 93.86 | Gaia DR2 | TICv8 |
| 5891 | 1.24 | โ | โ | โ | โ | 93.86 | Santos et al. 2013 | TICv8 |
| 5773 | 1.42 | 1.64 | โ | โ | โ | 93.86 | Stassun et al. 2017 | TICv8 |
| โ | โ | โ | โ | โ | โ | 93.86 | Valenti & Fischer 2005 | TICv8 |
| โ | โ | โ | โ | โ | G2 V | 93.86 | Michigan Catalog, Vol. 1 | TICv8 |
| โ | โ | โ | โ | โ | G5 | 93.86 | Cannon & Pickering 1918 | TICv8 |