Temperature
4907 K
4756 to 4907
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Stellar HostProfile
HD 63454
Unclassified star • 37.69 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
HIP: HIP 37284TIC: TIC 278380701HD: HD 63454
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: Ghezzi et al. 2010 • System source: TICv8
Mass
0.80 Msun
0.42 to 0.84
Radius
0.64 Rsun
0.64 to 1.05
Age
1 Gyr
single adopted value
Luminosity
-0.67 log(Lsun)
-0.67 to -0.53
Distance
37.69 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.64 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 63454
0.64 R☉
System Layout
Known planets
1 planets linked to this host
HD 63454 b
Radial Velocity
◌
Discovery
2005
Period
2.82 days
Radius
—
Mass
79.46 M⊕
Eq. Temp
—
HD 63454 and Its Close-Orbiting Planet
HD 63454 is a K3 V (k) star 123 light-years away, and one planet is known to orbit it. The K-type dwarf is cooler than the Sun, with a temperature of 4910 K, and it is smaller than the Sun in both mass and radius, at 0.8 solar masses and 0.64 solar radii. Its age is given as a reported upper limit of 1 billion years.
The lone planet, HD 63454 b, was found in 2005 using the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. It has a minimum mass of 79.5 Earth masses, larger than Earth's, and an orbital period of 2.82 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
12
Stellar refs
12
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typedisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4812 | 0.42 | 0.77 | — | — | — | 37.69 | Stassun et al. 2017 | TICv8 |
| 4840 | 0.66 | — | — | -0.60 | — | 37.69 | Sousa et al. 2008 | TICv8 |
| 4756 | — | — | — | — | — | 37.69 | Suárez-Andrés et al. 2016 | TICv8 |
| 4784.4 | — | 0.79 | — | -0.53 | — | 37.69 | Gaia DR2 | TICv8 |
| 4840 | 0.84 | 1.05 | — | — | — | 37.69 | Kane et al. 2011 | TICv8 |
| 4818.1 | 0.78 | 0.78 | — | -0.54 | — | 37.69 | TICv8 | TICv8 |
| — | — | — | — | — | K0 | 37.69 | Cannon & Pickering 1918 | TICv8 |
| — | — | — | — | — | K4 V | 37.69 | Michigan Catalog, Vol. 1 | TICv8 |
| — | — | — | — | — | K3 V (k) | 37.69 | Gray et al. 2006 | TICv8 |
| 4841 | 0.80 | — | 1 | -0.59 | K4 V | 37.69 | Moutou et al. 2005 | TICv8 |
| 4907 | 0.80 | 0.64 | 1 | -0.67 | — | 37.69 | Ghezzi et al. 2010 | TICv8 |
| 4833 | — | — | — | — | — | 37.69 | Tsantaki et al. 2014 | TICv8 |