Temperature
4296 K
4296 to 4391
K5 III • 1322.5 pc
Records
4
literature rows
Planets
1
system count
References
5
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: Gettel et al. 2012 • System source: TICv8
Temperature
4296 K
4296 to 4391
Mass
0.80 Msun
0.80 to 1.17
Radius
17.30 Rsun
17.30 to 43.41
Luminosity
1.96 log(Lsun)
1.96 to 2.73
Distance
1322.5 pc
single adopted value
Spectral Type
K5 III
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Current adopted radius: 17.30 R☉ • circles scaled linearly by radius
Sun
1.0 R☉ baseline
BD+20 274
17.30 R☉
System Layout
1 planets linked to this host
Radial Velocity
Discovery
2012
Period
578.2 days
Radius
—
Mass
1334.9 M⊕
Eq. Temp
—
BD+20 274 is a star located 4310 light-years away, and it hosts one known planet. The star is a K5 III type with a mass of 0.8 solar masses and a radius of 17.3 solar radii, making its reported radius estimate larger than the Sun's. Its temperature is 4300 K, which is cooler than the Sun's.
The planet BD+20 274 b was discovered in 2012 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. BD+20 274 b has a minimum mass of 1330 Earth masses, a lower bound on its true mass. This minimum mass is larger than Earth's and is roughly 4.2 times Jupiter's mass. The planet completes one orbit in 578 days.
Provenance
Evidence Summary
Rows
4
Stellar refs
4
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4391 | 1.17 | — | — | — | — | 1322.5 | Mortier et al. 2013 | TICv8 |
| 4296 | — | 43.41 | — | — | — | 1322.5 | TICv8 | TICv8 |
| 4322.6 | — | 41.32 | — | 2.73 | — | 1322.5 | Gaia DR2 | TICv8 |
| 4296 | 0.80 | 17.30 | — | 1.96 | K5 III | 1322.5 | Gettel et al. 2012 | TICv8 |