Temperature
5496 K
5087 to 5496
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Stellar HostProfile
Kepler-570
Unclassified star • 568.1 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 407001624
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
0.93 Msun
0.84 to 0.93
Radius
0.90 Rsun
0.81 to 0.92
Age
5.01 Gyr
5.01 to 8.50
Distance
568.1 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.90 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-570
0.90 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-570 b
Transit
◌
Discovery
2016
Period
4.30 days
Radius
2.45 R⊕
Mass
—
Eq. Temp
—
Kepler-570 and Its Lone Known Planet
Kepler-570 is a star located 1,850 light-years away. It is 5.01 billion years old, holds 0.93 solar masses, spans 0.9 solar radii, and has a temperature of 5500 K. Its reported mass estimate is smaller than the Sun's, and its reported temperature is cooler than the Sun's. One known planet orbits this star.
That planet is Kepler-570 b, a Super-Earth 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. It completes an orbit every 4.3 days and has a radius of 2.45 Earth radii, a reported radius estimate larger than Earth's. A Super-Earth reaches 2.5 times Earth's radius, so the planet sits within that size class by radius alone.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
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 |
|---|---|---|---|---|---|---|---|---|
| 5447 | 0.84 | 0.85 | 8.50 | — | — | 568.1 | Q1-Q8 KOI Table | TICv8 |
| 5480 | 0.88 | 0.86 | — | — | — | 568.1 | Q1-Q12 KOI Table | TICv8 |
| 5324 | — | 0.85 | — | — | — | 568.1 | Q1-Q6 KOI Table | TICv8 |
| 5480 | 0.88 | 0.86 | — | — | — | 568.1 | Q1-Q16 KOI Table | TICv8 |
| 5324 | — | 0.92 | — | — | — | 568.1 | Latham et al. 2005 | TICv8 |
| 5480 | 0.88 | 0.86 | — | — | — | 568.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5496 | 0.93 | 0.90 | 5.01 | — | — | 568.1 | Morton et al. 2016 | TICv8 |
| 5481 | — | 0.81 | — | — | — | 568.1 | Berger et al. 2018 | TICv8 |
| 5363.9 | 0.93 | 0.82 | — | -0.30 | — | 568.1 | TICv8 | TICv8 |
| 5480 | 0.88 | 0.86 | — | — | — | 568.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5087 | — | 0.91 | — | -0.30 | — | 568.1 | Gaia DR2 | TICv8 |
| 5324 | — | 0.85 | — | — | — | 568.1 | Batalha et al. 2013 | TICv8 |
| — | — | — | — | — | — | 568.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |