Temperature
5943 K
5412.2 to 5943
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Stellar HostProfile
Kepler-610
Unclassified star • 845.8 pc
Records
19
literature rows
Planets
2
system count
References
14
distinct source labels
TIC: TIC 275491028
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: Morton et al. 2016 • System source: TICv8
Mass
1.10 Msun
0.94 to 1.10
Radius
1.13 Rsun
0.60 to 1.13
Age
3.55 Gyr
0.40 to 3.55
Distance
845.8 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.13 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-610
1.13 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-610 b
Transit
◌
Discovery
2016
Period
7.00 days
Radius
4.19 R⊕
Mass
—
Eq. Temp
—
Kepler-610 c
Transit
◌
Discovery
2016
Period
151.9 days
Radius
3.30 R⊕
Mass
—
Eq. Temp
—
Kepler-610: A Distant Star With Two Known Worlds
Kepler-610 is a star located 2760 light-years away, and it hosts two planets: Kepler-610 b and Kepler-610 c. The star is 3.55 billion years old, with a mass of 1.1 solar masses and a radius of 1.13 solar radii. Its temperature is 5940 K, hotter than the Sun, and both its mass and radius estimates are larger than the Sun's.
Kepler-610 b is a Jupiter-like planet discovered by transit in 2016, with a radius of 4.19 Earth radii. That radius is larger than Earth's and is the largest among the listed planets. It completes an orbit in 7 days, the shortest year among the listed planets. Kepler-610 c is a Neptune-like planet, also discovered by transit in 2016, with a radius of 3.3 Earth radii, larger than Earth's but the smallest among the listed planets. Its orbital period is 152 days, the longest year among the listed planets.
Provenance
Underlying measurements and references
Evidence Summary
Rows
19
Stellar refs
13
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5713 | 1.01 | 0.89 | — | — | — | 845.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5412.2 | — | 0.96 | — | -0.15 | — | 845.8 | Gaia DR2 | TICv8 |
| — | — | — | — | — | — | 845.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5581 | 0.99 | 0.94 | — | -0.11 | — | 845.8 | TICv8 | TICv8 |
| 5713 | 1.01 | 0.89 | — | — | — | 845.8 | Q1-Q16 KOI Table | TICv8 |
| 5514 | — | 0.86 | — | — | — | 845.8 | Q1-Q6 KOI Table | TICv8 |
| 5659 | 0.94 | 0.83 | 0.40 | — | — | 845.8 | Q1-Q8 KOI Table | TICv8 |
| 5713 | 1.01 | 0.89 | — | — | — | 845.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5713 | 1.01 | 0.89 | — | — | — | 845.8 | Q1-Q12 KOI Table | TICv8 |
| 5514 | — | 0.60 | — | — | — | 845.8 | Latham et al. 2005 | TICv8 |
| 5716 | — | 0.87 | — | — | — | 845.8 | Berger et al. 2018 | TICv8 |
| 5713 | 1.01 | 0.89 | — | — | — | 845.8 | Q1-Q16 KOI Table | TICv8 |
| 5943 | 1.10 | 1.13 | 3.55 | — | — | 845.8 | Morton et al. 2016 | TICv8 |
| 5713 | 1.01 | 0.89 | — | — | — | 845.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5713 | 1.01 | 0.89 | — | — | — | 845.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 845.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5514 | — | 0.86 | — | — | — | 845.8 | Batalha et al. 2013 | TICv8 |
| 5659 | 0.94 | 0.83 | 0.40 | — | — | 845.8 | Q1-Q8 KOI Table | TICv8 |
| 5713 | 1.01 | 0.89 | — | — | — | 845.8 | Q1-Q12 KOI Table | TICv8 |