Temperature
5284 K
5130 to 5289
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Stellar HostProfile
Kepler-1757
Unclassified star โข 807.3 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 273378480
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: Q1-Q12 KOI Table โข System source: TICv8
Mass
0.82 Msun
0.82 to 0.87
Radius
0.74 Rsun
0.49 to 0.82
Distance
807.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.74 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1757
0.74 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1757 b
Transit
โ
Discovery
2021
Period
19.66 days
Radius
2.95 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1757 b: A Neptune-Like World Around a Small Cool Star
Kepler-1757 is a star located 2,630 light-years away, and it hosts one known planet. The star's reported mass estimate is 0.817 solar masses, smaller than the Sun's, and its radius estimate is 0.741 solar radii, also smaller than the Sun's. Its reported temperature is 5,280 K, cooler than the Sun's.
The planet Kepler-1757 b was discovered in 2021 by the transit method, which occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness, with repeated dips helping establish orbital periods. Kepler-1757 b is Neptune-like, a size class for planets reaching 4 times Earth's radius, and its radius estimate is 2.95 Earth radii, larger than Earth's. It completes an orbit every 19.7 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5284 | 0.82 | 0.74 | โ | โ | โ | 807.3 | Q1-Q12 KOI Table | TICv8 |
| 5146 | 0.87 | 0.82 | โ | -0.37 | โ | 807.3 | TICv8 | TICv8 |
| 5130 | โ | 0.69 | โ | โ | โ | 807.3 | Batalha et al. 2013 | TICv8 |
| 5130 | โ | 0.69 | โ | โ | โ | 807.3 | Q1-Q6 KOI Table | TICv8 |
| 5284 | 0.82 | 0.74 | โ | โ | โ | 807.3 | Q1-Q16 KOI Table | TICv8 |
| 5130 | โ | 0.49 | โ | โ | โ | 807.3 | Latham et al. 2005 | TICv8 |
| 5288 | 0.83 | 0.74 | โ | โ | โ | 807.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | 807.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5289 | 0.84 | 0.74 | 0.70 | โ | โ | 807.3 | Q1-Q8 KOI Table | TICv8 |
| 5284 | 0.82 | 0.74 | โ | โ | โ | 807.3 | Q1-Q17 DR24 KOI Table | TICv8 |