Temperature
3768 K
3109 to 3768
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Stellar HostProfile
Kepler-1624
M V โข 259.0 pc
Records
11
literature rows
Planets
1
system count
References
12
distinct source labels
TIC: TIC 137683938
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: Im et al. 2025 โข System source: TICv8
Mass
0.54 Msun
0.17 to 0.56
Radius
0.55 Rsun
0.19 to 4.96
Distance
259.0 pc
single adopted value
Spectral Type
M V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.55 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1624
0.55 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1624 b
Transit
โ
Discovery
2016
Period
3.29 days
Radius
6.59 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1624 and Its Jupiter-like Planet
Kepler-1624 is a small, cool red dwarf star of spectral type M V. It lies 845 light-years away and hosts one known planet. The star's reported mass estimate is 0.541 solar masses, its reported radius estimate is 0.552 solar radii, and its reported temperature is 3770 K, all smaller or cooler than the corresponding solar values.
The sole planet, Kepler-1624 b, is classified as Jupiter-like, a size class for planets whose radius exceeds 4 times Earth's. Its reported radius estimate is 6.59 Earth radii, larger than Earth's. It was discovered by the transit method in 2016, when it passed in front of its star from our viewpoint, dimming the observed brightness. Its orbital period is 3.29 days, the time it takes to complete one orbit.
Provenance
Underlying measurements and references
Evidence Summary
Rows
11
Stellar refs
11
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| โ | โ | โ | โ | โ | โ | 259.0 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 3109 | โ | 4.96 | โ | โ | โ | 259.0 | Latham et al. 2005 | TICv8 |
| 3636 | 0.50 | 0.47 | 4.47 | โ | โ | 259.0 | Morton et al. 2016 | TICv8 |
| 3579 | 0.56 | 0.57 | โ | -1.32 | โ | 259.0 | TICv8 | TICv8 |
| 3440.8 | โ | 0.73 | โ | -1.17 | โ | 259.0 | Gaia DR2 | TICv8 |
| 3560 | โ | 0.57 | โ | โ | โ | 259.0 | Berger et al. 2018 | TICv8 |
| 3212 | 0.17 | 0.19 | โ | โ | โ | 259.0 | Q1-Q16 KOI Table | TICv8 |
| 3579 | โ | 0.57 | โ | โ | โ | 259.0 | ExoFOP | TICv8 |
| 3386 | 0.43 | 0.43 | โ | โ | โ | 259.0 | Q1-Q17 DR25 KOI Table | TICv8 |
| 3212 | 0.17 | 0.19 | โ | โ | โ | 259.0 | Q1-Q17 DR24 KOI Table | TICv8 |
| 3768 | 0.54 | 0.55 | โ | โ | M V | 259.0 | Im et al. 2025 | TICv8 |