Temperature
5750 K
5742 to 6195
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Stellar HostProfile
Kepler-412
G3 V • 1086.2 pc
Records
17
literature rows
Planets
1
system count
References
18
distinct source labels
TIC: TIC 158170594
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: Deleuil et al. 2014 • System source: TICv8
Mass
1.17 Msun
1.05 to 1.18
Radius
1.29 Rsun
1.03 to 1.38
Age
5.10 Gyr
2 to 5.37
Distance
1086.2 pc
single adopted value
Spectral Type
G3 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.29 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-412
1.29 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-412 b
Transit
◌
Discovery
2014
Period
1.72 days
Radius
15.03 R⊕
Mass
299.1 M⊕
Eq. Temp
1850 K
Kepler-412 and Its Jupiter-Like Planet
Kepler-412 is a G3 V star, a Sun-like main-sequence dwarf, located 3540 light-years away. Its measured mass is 1.17 solar masses and its radius is 1.29 solar radii, both larger than the Sun's corresponding values. The star's temperature is 5750 K, and its age is 5.1 billion years. One planet is known to orbit this host.
That planet is Kepler-412 b, classified as Jupiter-like because its radius exceeds four times Earth's. It was discovered in 2014 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. Kepler-412 b has a radius of 15 Earth radii and a mass of 299 Earth masses. Its orbital period is 1.72 days. Its mean density is 0.485 g/cm³, which is 0.0881 times Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
17
Stellar refs
17
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 6195 | 1.18 | 1.12 | — | — | — | 1086.2 | Q1-Q16 KOI Table | TICv8 |
| 5912 | — | 1.05 | — | — | — | 1086.2 | Q1-Q6 KOI Table | TICv8 |
| 5912 | — | 1.04 | — | — | — | 1086.2 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 1086.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5858 | 1.08 | 1.21 | 5.37 | — | — | 1086.2 | Morton et al. 2016 | TICv8 |
| 5912 | — | 1.05 | — | — | — | 1086.2 | Batalha et al. 2013 | TICv8 |
| 6195 | 1.18 | 1.12 | — | — | — | 1086.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5832.8 | 1.05 | 1.33 | — | 0.27 | — | 1086.2 | TICv8 | TICv8 |
| 5750 | — | 1.34 | — | — | — | 1086.2 | Berger et al. 2018 | TICv8 |
| 5832.8 | — | 1.33 | — | — | — | 1086.2 | ExoFOP | TICv8 |
| 6119 | 1.06 | 1.03 | 2 | — | — | 1086.2 | Q1-Q8 KOI Table | TICv8 |
| 5742 | 1.07 | 1.22 | — | — | — | 1086.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5750 | 1.17 | 1.29 | — | — | — | 1086.2 | Esteves et al. 2015 | TICv8 |
| 5750 | 1.17 | 1.29 | 5.10 | — | G3 V | 1086.2 | Deleuil et al. 2014 | TICv8 |
| 5750 | 1.17 | 1.29 | 5.10 | — | — | 1086.2 | Bonomo et al. 2017 | TICv8 |
| 5757.8 | — | 1.38 | — | 0.27 | — | 1086.2 | Gaia DR2 | TICv8 |
| 6195 | 1.18 | 1.12 | — | — | — | 1086.2 | Q1-Q12 KOI Table | TICv8 |