Temperature
4945 K
4750.2 to 5012.8
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Stellar HostProfile
Kepler-675
Unclassified star • 665.7 pc
Records
19
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 27006665
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
0.79 Msun
0.76 to 0.85
Radius
0.75 Rsun
0.67 to 0.82
Age
4.68 Gyr
1.80 to 4.68
Distance
665.7 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.75 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-675
0.75 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-675 b
Transit
◌
Discovery
2016
Period
2.34 days
Radius
2.44 R⊕
Mass
—
Eq. Temp
—
Kepler-675 and Its Super-Earth
Kepler-675 is a star 2170 light-years away with one known planet in orbit. The host star is 4.68 billion years old, with a mass of 0.79 solar masses, a radius of 0.75 solar radii, and a temperature of 4950 K. Its reported mass, radius, and temperature are each smaller or cooler than the Sun's.
The planet, Kepler-675 b, was discovered in 2016 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. Its orbital period is 2.34 days. With a radius of 2.44 Earth radii, it is a Super-Earth, and its reported radius estimate is larger than Earth's.
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 |
|---|---|---|---|---|---|---|---|---|
| 4833 | — | 0.70 | — | — | — | 665.7 | Latham et al. 2005 | TICv8 |
| 5005 | 0.85 | 0.77 | — | — | — | 665.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | — | — | — | — | — | 665.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5007 | — | 0.76 | — | — | — | 665.7 | Berger et al. 2018 | TICv8 |
| — | — | — | — | — | — | 665.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4989 | 0.78 | 0.73 | — | — | — | 665.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4989 | 0.78 | 0.73 | — | — | — | 665.7 | Q1-Q16 KOI Table | TICv8 |
| 4833 | — | 0.67 | — | — | — | 665.7 | Q1-Q6 KOI Table | TICv8 |
| 5005 | 0.85 | 0.77 | — | — | — | 665.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5012.8 | — | 0.70 | — | -0.56 | — | 665.7 | Gaia DR2 | TICv8 |
| 4989 | 0.78 | 0.73 | — | — | — | 665.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 4989 | 0.78 | 0.73 | — | — | — | 665.7 | Q1-Q12 KOI Table | TICv8 |
| 4989 | 0.78 | 0.73 | — | — | — | 665.7 | Q1-Q16 KOI Table | TICv8 |
| 4945 | 0.79 | 0.75 | 4.68 | — | — | 665.7 | Morton et al. 2016 | TICv8 |
| 4750.2 | 0.76 | 0.82 | — | -0.51 | — | 665.7 | TICv8 | TICv8 |
| 4963 | 0.76 | 0.67 | 1.80 | — | — | 665.7 | Q1-Q8 KOI Table | TICv8 |
| 4963 | 0.76 | 0.67 | 1.80 | — | — | 665.7 | Q1-Q8 KOI Table | TICv8 |
| 4989 | 0.78 | 0.73 | — | — | — | 665.7 | Q1-Q12 KOI Table | TICv8 |
| 4833 | — | 0.67 | — | — | — | 665.7 | Batalha et al. 2013 | TICv8 |