Temperature
6180 K
6124 to 6436
9 values • 7 distinct
F8 V • 136.2 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
Approximate color
from effective temperature
Canonical Summary
Numeric fields use the median of non-null measurements. Disagreement stays visible through ranges, counts, and provenance.
Temperature
6180 K
6124 to 6436
9 values • 7 distinct
Mass
1.23 Msun
1.14 to 1.76
8 values • 6 distinct
Radius
1.35 Rsun
0.73 to 1.54
8 values • 6 distinct
Age
2.80 Gyr
1 to 3.29
3 values • 3 distinct
Luminosity
0.47 log(Lsun)
0.45 to 0.48
2 values • 2 distinct
Distance
136.2 pc
single adopted value
11 values • 1 distinct
Spectral Type
F8 V
Consistent across records
F8 V (1)
Planets
1
Stable across source rows
1
System Layout
1 planets linked to this host
Transit
Discovery
2010
Period
6.87 days
Radius
12.22 R⊕
Mass
841.6 M⊕
Eq. Temp
—
Provenance
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
11 values • 1 distinct
11 values • 1 distinct
9 values • 7 distinct
8 values • 6 distinct
8 values • 6 distinct
3 values • 3 distinct
2 values • 2 distinct
5 values • 3 distinct
8 values • 3 distinct
1 values • 1 distinct
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6436 | 1.28 | 1.35 | 2.80 | — | — | 136.2 | Borsato et al. 2021 | TICv8 |
| 6200 | — | — | 1 | — | F8 V | 136.2 | Salz et al. 2015 | TICv8 |
| 6180 | 1.76 | 1.52 | — | — | — | 136.2 | Stassun et al. 2017 | TICv8 |
| — | 1.23 | 1.35 | — | — | — | 136.2 | Brown et al. 2012 | TICv8 |
| 6436 | 1.14 | 0.73 | — | — | — | 136.2 | Mortier et al. 2013 | TICv8 |
| 6124 | 1.16 | 1.54 | — | 0.48 | — | 136.2 | TICv8 | TICv8 |
| — | 1.23 | — | — | — | — | 136.2 | Knutson et al. 2014 | TICv8 |
| 6170 | — | 1.47 | — | 0.45 | — | 136.2 | Gaia DR2 | TICv8 |
| 6150 | 1.20 | 1.33 | — | — | — | 136.2 | Barros et al. 2010 | TICv8 |
| 6247 | — | — | — | — | — | 136.2 | Tsantaki et al. 2014 | TICv8 |
| 6180 | 1.23 | 1.35 | 3.29 | — | — | 136.2 | Bonomo et al. 2017 | TICv8 |