Temperature
4939 K
4807 to 5011
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Stellar HostProfile
Kepler-1423
Unclassified star
Records
9
literature rows
Planets
1
system count
References
10
distinct source labels
TIC: TIC 121599740
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 โข System source: TICv8
Mass
0.79 Msun
0.79 to 0.93
Radius
0.75 Rsun
0.75 to 2.05
Age
4.68 Gyr
4.68 to 14
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.75 Rโ (circles scaled linearly by radius)
Sun
1.0 Rโ baseline
Kepler-1423
0.75 Rโ
System Layout
Known planets
1 planets linked to this host
Kepler-1423 b
Transit
โ
Discovery
2016
Period
23.96 days
Radius
1.06 Rโ
Mass
โ
Eq. Temp
โ
Kepler-1423 and Its Earth-like Planet
Kepler-1423 is a star with one known planet in its system. The host star is estimated to be 4.68 billion years old, with a mass of 0.79 solar masses and a radius of 0.75 solar radii. Its reported temperature is 4940 K.
The star's reported mass estimate is smaller than the Sun's, and its reported radius estimate is also smaller than the Sun's. Its reported temperature is cooler than the Sun's.
The sole cataloged planet, Kepler-1423 b, is classified as Earth-like. It was discovered in 2016 by the transit method, in which a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Repeated dips help establish orbital periods.
Kepler-1423 b has an orbital period of 24 days and a radius of 1.06 Earth radii. Its size classification compares radius with Earth's: an Earth-like planet stays within 1.5 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
9
Stellar refs
9
System refs
1
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4807 | โ | 1.33 | โ | โ | โ | โ | Latham et al. 2005 | TICv8 |
| 4934 | 0.92 | 2.05 | 14 | โ | โ | โ | Q1-Q8 KOI Table | TICv8 |
| 5011 | 0.93 | 1.78 | โ | โ | โ | โ | Q1-Q17 DR25 KOI Table | TICv8 |
| 5011 | 0.93 | 1.78 | โ | โ | โ | โ | Q1-Q16 KOI Table | TICv8 |
| 4869.3 | โ | โ | โ | โ | โ | โ | Gaia DR2 | TICv8 |
| 5011 | 0.93 | 1.78 | โ | โ | โ | โ | Q1-Q17 DR24 KOI Table | TICv8 |
| โ | โ | โ | โ | โ | โ | โ | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5011 | 0.93 | 1.78 | โ | โ | โ | โ | Q1-Q12 KOI Table | TICv8 |
| 4939 | 0.79 | 0.75 | 4.68 | โ | โ | โ | Morton et al. 2016 | TICv8 |