Temperature
5614 K
5600 to 5680
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Stellar HostProfile
HD 10697
Unclassified star • 33.12 pc
Records
18
literature rows
Planets
1
system count
References
18
distinct source labels
TIC: TIC 456905162HD: HD 10697HIP: HIP 8159
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: Jofré et al. 2015 • System source: TICv8
Mass
1.11 Msun
0.99 to 1.22
Radius
1.75 Rsun
1.73 to 1.86
Age
6.98 Gyr
6.98 to 7.84
Luminosity
0.42 log(Lsun)
0.42 to 0.48
Distance
33.12 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.75 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 10697
1.75 R☉
System Layout
Known planets
1 planets linked to this host
HD 10697 b
Radial Velocity
◌
Discovery
1999
Period
1075.4 days
Radius
—
Mass
1825.3 M⊕
Eq. Temp
—
HD 10697 and Its Planet
HD 10697 is a G3 V star 108 light-years away, a Sun-like dwarf with a reported mass of 1.11 solar masses and a radius of 1.75 solar radii. Its temperature is 5610 K, and its age is 6.98 billion years.
One planet orbits this host. HD 10697 b was discovered in 1999 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion. The planet has a reported mass of 1830 Earth masses, roughly 5.74 times Jupiter's mass, and an orbital period of 1080 days. Its reported mass is larger than Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
18
Stellar refs
17
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 |
|---|---|---|---|---|---|---|---|---|
| 5641 | 1.22 | — | — | — | — | 33.12 | Santos et al. 2004 | TICv8 |
| — | — | — | — | — | — | 33.12 | Nordstrom et al. 2004 | TICv8 |
| 5600 | 1.13 | 1.79 | — | — | — | 33.12 | Luhn et al. 2019 | TICv8 |
| — | — | — | — | — | — | 33.12 | Nidever et al. 2002 | TICv8 |
| — | 0.99 | — | — | — | — | 33.12 | Feng et al. 2022 | TICv8 |
| 5614 | 1.11 | 1.75 | 6.98 | 0.42 | — | 33.12 | Jofré et al. 2015 | TICv8 |
| — | — | — | — | — | — | 33.12 | Duncan et al. 1991 | TICv8 |
| 5680 | 1.11 | — | — | — | G5 IV | 33.12 | Wittenmyer et al. 2009 | TICv8 |
| — | — | — | — | — | — | 33.12 | Duncan et al. 1991 | TICv8 |
| 5645.1 | 1.16 | 1.86 | — | — | — | 33.12 | Rosenthal et al. 2021 | TICv8 |
| — | — | — | — | — | — | 33.12 | Valenti & Fischer 2005 | TICv8 |
| 5641 | 1.13 | — | — | — | G3 V | 33.12 | Xiao et al. 2023 | TICv8 |
| 5654 | — | 1.81 | — | 0.48 | — | 33.12 | Gaia DR2 | TICv8 |
| 5665 | 1.22 | — | — | — | — | 33.12 | Santos et al. 2003 | TICv8 |
| — | 1.11 | 1.73 | 7.84 | — | — | 33.12 | Takeda et al. 2007 | TICv8 |
| 5600 | 0.99 | 1.84 | — | 0.48 | — | 33.12 | TICv8 | TICv8 |
| — | — | — | — | — | — | 33.12 | Wright et al. 2004 | TICv8 |
| — | — | — | — | — | G5 | 33.12 | Cannon & Pickering 1918 | TICv8 |