Temperature
6014 K
5289.4 to 6014
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Stellar HostProfile
Kepler-757
Unclassified star • 1068.7 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 360022783
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
1.08 Msun
0.88 to 1.08
Radius
1.13 Rsun
0.67 to 1.29
Age
3.31 Gyr
0.50 to 3.31
Distance
1068.7 pc
single adopted value
Planets
1
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-757
1.13 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-757 b
Transit
◌
Discovery
2016
Period
1.02 days
Radius
1.36 R⊕
Mass
—
Eq. Temp
—
Kepler-757 b: A Close-Orbiting Earth-Like World
Kepler-757 is a star located 3490 light-years away, with an age of 3.31 billion years. Its mass is 1.08 solar masses, its radius is 1.13 solar radii, and its temperature is 6010 K. One planet orbits this host.
That planet is Kepler-757 b, an Earth-like world detected by the transit method in 2016. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-757 b completes an orbit in 1.02 days, and its radius is 1.36 Earth radii. Its reported radius estimate is larger than Earth's.
The star's properties describe it specifically: at 6010 K it is hotter than the Sun, and at 1.08 solar masses it is slightly more massive, with a radius of 1.13 solar radii.
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 |
|---|---|---|---|---|---|---|---|---|
| 5364 | — | 0.74 | — | — | — | 1068.7 | Q1-Q6 KOI Table | TICv8 |
| 5559 | 0.88 | 0.81 | — | — | — | 1068.7 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5366 | 0.88 | 1.02 | — | — | — | 1068.7 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5559 | 0.88 | 0.81 | — | — | — | 1068.7 | Q1-Q16 KOI Table | TICv8 |
| — | — | — | — | — | — | 1068.7 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5364 | — | 0.74 | — | — | — | 1068.7 | Batalha et al. 2013 | TICv8 |
| 5289.4 | — | 1.29 | — | 0.07 | — | 1068.7 | Gaia DR2 | TICv8 |
| 5559 | 0.88 | 0.81 | — | — | — | 1068.7 | Q1-Q12 KOI Table | TICv8 |
| 5365 | — | 1.27 | — | — | — | 1068.7 | Berger et al. 2018 | TICv8 |
| 5667 | 1.01 | 1.25 | — | 0.16 | — | 1068.7 | TICv8 | TICv8 |
| 5549 | 0.91 | 0.81 | 0.50 | — | — | 1068.7 | Q1-Q8 KOI Table | TICv8 |
| 6014 | 1.08 | 1.13 | 3.31 | — | — | 1068.7 | Morton et al. 2016 | TICv8 |
| 5364 | — | 0.67 | — | — | — | 1068.7 | Latham et al. 2005 | TICv8 |