Temperature
6249 K
6025 to 6431
F7V • 26.19 pc
Records
20
literature rows
Planets
3
system count
References
21
distinct source labels
Approximate color
from effective temperature
Canonical Summary
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
Temperature
6249 K
6025 to 6431
Mass
1.23 Msun
1.15 to 1.29
Radius
1.40 Rsun
1.35 to 1.47
Age
3.12 Gyr
2.50 to 3.12
Luminosity
0.48 log(Lsun)
0.42 to 0.48
Distance
26.19 pc
single adopted value
Spectral Type
F7V
Multiple classifications reported
Planets
3
Stable across source rows
Scale Comparison
Current adopted radius: 1.40 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 142
1.40 R☉
System Layout
3 planets linked to this host
Radial Velocity
Discovery
2022
Period
108.5 days
Radius
—
Mass
82.64 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2001
Period
351.4 days
Radius
—
Mass
397.0 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2012
Period
1.02e4 days
Radius
—
Mass
3464.6 M⊕
Eq. Temp
—
HD 142 is an F7V star located 85.4 light-years from Earth. It is 3.12 billion years old and has a reported mass of 1.23 solar masses, larger than the Sun's. Its reported radius of 1.4 solar radii is also larger than the Sun's, and its temperature of 6250 K is hotter than the Sun's. Three planets are known to orbit this host.
HD 142 A d was discovered by radial velocity in 2022. Its minimum mass is 82.6 Earth masses, a lower bound on its true mass, and its orbital period is 108 days.
HD 142 b was also found by radial velocity, in 2001. It has a minimum mass of 397 Earth masses, larger than Earth's and roughly 1.25 times Jupiter's mass. Its orbital period is 351 days.
HD 142 c, discovered by radial velocity in 2012, has a reported mass of 3460 Earth masses, larger than Earth's and roughly 10.9 times Jupiter's mass. Its orbital period is 10200 days, the longest among the listed planets, while HD 142 A d has the shortest at 108 days and HD 142 b the second-shortest at 351 days.
Provenance
Evidence Summary
Rows
20
Stellar refs
20
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 26.19 | Nordstrom et al. 2004 | TICv8 |
| 6249 | 1.24 | — | — | — | — | 26.19 | Butler et al. 2006 | TICv8 |
| 6338 | 1.25 | 1.35 | 2.50 | 0.42 | — | 26.19 | Ghezzi et al. 2010 | TICv8 |
| 6403 | 1.29 | — | — | 0.43 | — | 26.19 | Sousa et al. 2008 | TICv8 |
| 6290 | 1.26 | — | — | — | — | 26.19 | Santos et al. 2003 | TICv8 |
| 6271 | — | — | — | — | — | 26.19 | Tsantaki et al. 2014 | TICv8 |
| 6252.0 | 1.21 | 1.46 | — | 0.47 | — | 26.19 | TICv8 | TICv8 |
| 6302 | 1.28 | — | — | — | — | 26.19 | Santos et al. 2004 | TICv8 |
| 6273 | — | — | — | — | — | 26.19 | Maldonado et al. 2015 | TICv8 |
| 6245 | 1.23 | 1.47 | — | — | — | 26.19 | Wittenmyer et al. 2012 | TICv8 |
| — | — | — | — | — | G0 | 26.19 | Cannon & Pickering 1918 | TICv8 |
| 6431 | — | — | — | — | — | 26.19 | Suárez-Andrés et al. 2016 | TICv8 |
| 6025 | 1.15 | — | — | — | G1 IV | 26.19 | Tinney et al. 2002 | TICv8 |
| 6379.2 | — | 1.41 | — | 0.47 | — | 26.19 | Gaia DR2 | TICv8 |
| — | — | — | — | — | F7 V | 26.19 | Michigan Catalog, Vol. 2 | TICv8 |
| — | 1.21 | — | — | — | — | 26.19 | Feng et al. 2022 | TICv8 |
| — | — | — | — | — | F7 V | 26.19 | Gray et al. 2006 | TICv8 |
| 6249 | 1.23 | 1.40 | 3.12 | 0.48 | F7V | 26.19 | Turnbull 2015 | TICv8 |
| — | — | — | — | — | — | 26.19 | Valenti & Fischer 2005 | TICv8 |
| — | 1.23 | 1.40 | 3.12 | — | — | 26.19 | Takeda et al. 2007 | TICv8 |