Temperature
5200 K
4993 to 5332
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Stellar HostProfile
Kepler-75
K0 V • 835.4 pc
Records
18
literature rows
Planets
1
system count
References
19
distinct source labels
TIC: TIC 122785299
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: Bonomo et al. 2015 • System source: TICv8
Mass
0.91 Msun
0.77 to 0.92
Radius
0.89 Rsun
0.77 to 0.98
Age
6.20 Gyr
6 to 12.90
Distance
835.4 pc
single adopted value
Spectral Type
K0 V
Multiple classifications reported
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.89 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-75
0.89 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-75 b
Transit
◌
Discovery
2013
Period
8.88 days
Radius
11.77 R⊕
Mass
3209.9 M⊕
Eq. Temp
767 K
Kepler-75 and Its Jupiter-Like Planet
Kepler-75 is a K0 V star located 2720 light-years away, with a mass of 0.91 solar masses, a radius of 0.89 solar radii, and a temperature of 5200 K. Its reported mass and radius estimates are smaller than the Sun's, and its temperature is cooler. The star is 6.2 billion years old, and one planet orbits it.
That planet, Kepler-75 b, is a Jupiter-like world discovered by transit in 2013. It has a mass of 3210 Earth masses and a radius of 11.8 Earth radii, both larger than Earth's, and orbits every 8.88 days. Its mean density is 10.8 g/cm³, 1.97 times Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
18
Stellar refs
18
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typedisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5200 | 0.91 | 0.89 | 6.20 | — | — | 835.4 | Bonomo et al. 2017 | TICv8 |
| 5332 | 0.82 | 0.84 | — | — | — | 835.4 | Q1-Q12 KOI Table | TICv8 |
| 5206 | 0.83 | 0.83 | 9.12 | — | — | 835.4 | Morton et al. 2016 | TICv8 |
| 5152 | 0.77 | 0.77 | 12.90 | — | — | 835.4 | Q1-Q8 KOI Table | TICv8 |
| 5332 | 0.82 | 0.84 | — | — | — | 835.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5101 | — | 0.84 | — | — | — | 835.4 | Q1-Q6 KOI Table | TICv8 |
| 5101 | — | 0.84 | — | — | — | 835.4 | Batalha et al. 2013 | TICv8 |
| 5306 | — | 0.96 | — | — | — | 835.4 | Berger et al. 2018 | TICv8 |
| 5101 | — | 0.93 | — | — | — | 835.4 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 835.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5160 | — | 0.98 | — | — | — | 835.4 | ExoFOP | TICv8 |
| 5332 | 0.82 | 0.84 | — | — | — | 835.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5200 | 0.91 | 0.89 | 6.20 | — | K0 V | 835.4 | Bonomo et al. 2015 | TICv8 |
| 4993 | — | 0.96 | — | -0.29 | — | 835.4 | Gaia DR2 | TICv8 |
| 5306 | 0.92 | 0.95 | 7.76 | — | — | 835.4 | Fulton & Petigura 2018 | TICv8 |
| 5160 | 0.87 | 0.98 | — | -0.21 | — | 835.4 | TICv8 | TICv8 |
| 5332 | 0.82 | 0.84 | — | — | — | 835.4 | Q1-Q16 KOI Table | TICv8 |
| 5330 | 0.88 | 0.88 | 6 | — | G8 V | 835.4 | Hebrard et al. 2013 | TICv8 |