Temperature
4422 K
4290 to 4465
←Back to Stellar Hosts
Stellar HostProfile
Kepler-1460
Unclassified star • 553.2 pc
Records
10
literature rows
Planets
1
system count
References
11
distinct source labels
TIC: TIC 352011765
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
0.70 Msun
0.62 to 0.70
Radius
0.67 Rsun
0.62 to 0.77
Age
3.98 Gyr
single adopted value
Distance
553.2 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.67 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1460
0.67 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1460 b
Transit
◌
Discovery
2016
Period
29.96 days
Radius
1.96 R⊕
Mass
—
Eq. Temp
—
Kepler-1460 b: A Super-Earth in a Distant System
Kepler-1460 is a star located 1800 light-years away, and it hosts one planet. The star is estimated to be 3.98 billion years old, with a mass of 0.7 solar masses and a radius of 0.67 solar radii. Its temperature is 4420 K. The star's reported mass and radius estimates are smaller than the Sun's, and its reported temperature is cooler than the Sun's.
The planet Kepler-1460 b is a Super-Earth 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. It orbits once every 30 days and has a radius of 1.96 Earth radii, which is larger than Earth's. In size classification, a Super-Earth reaches up to 2.5 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
10
Stellar refs
10
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 4465 | — | 0.63 | — | — | — | 553.2 | Berger et al. 2018 | TICv8 |
| 4422 | 0.70 | 0.67 | 3.98 | — | — | 553.2 | Morton et al. 2016 | TICv8 |
| 4463 | 0.62 | 0.64 | — | — | — | 553.2 | Q1-Q12 KOI Table | TICv8 |
| 4353 | 0.68 | 0.67 | — | -0.84 | — | 553.2 | TICv8 | TICv8 |
| 4441 | — | 0.62 | — | -0.88 | — | 553.2 | Gaia DR2 | TICv8 |
| 4290 | — | 0.77 | — | — | — | 553.2 | Latham et al. 2005 | TICv8 |
| 4463 | 0.62 | 0.64 | — | — | — | 553.2 | Q1-Q17 DR25 KOI Table | TICv8 |
| 4463 | 0.62 | 0.64 | — | — | — | 553.2 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 553.2 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 4463 | 0.62 | 0.64 | — | — | — | 553.2 | Q1-Q16 KOI Table | TICv8 |