Temperature
6210 K
6210 to 6596
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Stellar HostProfile
HD 86264
Unclassified star • 67.81 pc
Records
12
literature rows
Planets
1
system count
References
13
distinct source labels
HD: HD 86264HIP: HIP 48780TIC: TIC 348964243
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
1.42 Msun
1.26 to 1.42
Radius
1.88 Rsun
1.67 to 1.88
Age
2.24 Gyr
single adopted value
Luminosity
0.66 log(Lsun)
0.61 to 0.66
Distance
67.81 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.88 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HD 86264
1.88 R☉
System Layout
Known planets
1 planets linked to this host
HD 86264 b
Radial Velocity
◌
Discovery
2009
Period
1488.8 days
Radius
—
Mass
3117.3 M⊕
Eq. Temp
—
HD 86264 and Its One Known Planet
HD 86264 is a star 221 light-years away with a spectral type of F8, placing it among the hotter stars rather than the Sun's G-type class. It is 2.24 billion years old, holds 1.42 solar masses, spans 1.88 solar radii, and has a temperature of 6210 K. Its mass, radius, and temperature are larger or hotter than the Sun's.
One planet is known around this star. HD 86264 b was found in 2009 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. That period is 1490 days, and the planet's mass is 3120 Earth masses, larger than Earth's and roughly 9.81 times Jupiter's mass.
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 |
|---|---|---|---|---|---|---|---|---|
| 6210 | 1.42 | 1.88 | 2.24 | 0.66 | — | 67.81 | Fischer et al. 2009 | TICv8 |
| — | — | — | — | — | — | 67.81 | Wright et al. 2004 | TICv8 |
| — | 1.26 | — | — | — | — | 67.81 | Feng et al. 2022 | TICv8 |
| — | — | — | — | — | F8 | 67.81 | Cannon & Pickering 1918 | TICv8 |
| — | — | — | — | — | — | 67.81 | Valenti & Fischer 2005 | TICv8 |
| 6596 | 1.42 | — | — | — | — | 67.81 | Santos et al. 2013 | TICv8 |
| 6210 | 1.42 | — | — | — | F7 V | 67.81 | Xiao et al. 2023 | TICv8 |
| 6324.8 | — | 1.69 | — | 0.61 | — | 67.81 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 67.81 | Nordstrom et al. 2004 | TICv8 |
| 6300 | — | — | — | — | — | 67.81 | Tsantaki et al. 2014 | TICv8 |
| — | — | — | — | — | F7 V | 67.81 | Michigan Catalog, Vol. 4 | TICv8 |
| 6352.2 | 1.26 | 1.67 | — | 0.61 | — | 67.81 | TICv8 | TICv8 |