Temperature
3939 K
3888 to 4072
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Stellar HostProfile
Kepler-1735
Unclassified star • 245.3 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 123206821
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 • System source: TICv8
Mass
0.54 Msun
0.54 to 0.55
Radius
0.52 Rsun
0.51 to 0.67
Distance
245.3 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.52 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1735
0.52 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1735 b
Transit
◌
Discovery
2021
Period
7.72 days
Radius
1.19 R⊕
Mass
—
Eq. Temp
—
Kepler-1735 b: A Close-In Earth-Sized World
Kepler-1735 is a star located 800 light-years away, and it hosts one known planet. The star has a reported mass of 0.54 solar masses and a reported radius of 0.52 solar radii, both smaller than the Sun's corresponding values. Its reported temperature is 3940 K, which is cooler than the Sun's temperature.
The planet Kepler-1735 b was discovered in 2021 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. Repeated dips help establish orbital periods. Kepler-1735 b orbits its star every 7.72 days.
Kepler-1735 b is classified as Earth-like, a size class that stays within 1.5 times Earth's radius. Its reported radius is 1.19 Earth radii, larger than Earth's radius. This radius estimate is an approximate value rather than an exact measurement.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositystable
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 245.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4072 | 0.55 | 0.53 | 14 | — | — | 245.3 | Q1-Q8 KOI Table | TICv8 |
| 3978 | — | 0.55 | — | — | — | 245.3 | Batalha et al. 2013 | TICv8 |
| 3978 | — | 0.55 | — | — | — | 245.3 | Q1-Q6 KOI Table | TICv8 |
| 3978 | — | 0.67 | — | — | — | 245.3 | Latham et al. 2005 | TICv8 |
| — | — | — | 8.17 | — | — | 245.3 | Gaidos et al. 2024 | TICv8 |
| 3888 | 0.55 | 0.56 | — | -1.19 | — | 245.3 | TICv8 | TICv8 |
| 3939 | 0.54 | 0.52 | — | — | — | 245.3 | Q1-Q16 KOI Table | TICv8 |
| 3975 | 0.54 | 0.51 | — | — | — | 245.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 3939 | 0.54 | 0.52 | — | — | — | 245.3 | Q1-Q12 KOI Table | TICv8 |
| 3939 | 0.54 | 0.52 | — | — | — | 245.3 | Q1-Q17 DR24 KOI Table | TICv8 |