Temperature
6096 K
5050 to 6096
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Stellar HostProfile
Kepler-1267
Unclassified star • 1379.4 pc
Records
16
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 268604100
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
1.15 Msun
0.92 to 1.15
Radius
1.20 Rsun
0.84 to 1.20
Age
3.24 Gyr
single adopted value
Distance
1379.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.20 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1267
1.20 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1267 b
Transit
◌
Discovery
2016
Period
13.03 days
Radius
3.01 R⊕
Mass
—
Eq. Temp
—
Kepler-1267 and Its Neptune-Like Planet
Kepler-1267 is a star 4500 light-years away with one known planet. The host star is estimated to be 3.24 billion years old, with a mass of 1.15 solar masses and a radius of 1.2 solar radii. Its temperature is 6100 K, hotter than the Sun, and both its reported mass and radius estimates are larger than the Sun's.
The planet Kepler-1267 b was discovered by transit in 2016. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness. Kepler-1267 b completes an orbit every 13 days. Its radius of 3.01 Earth radii is larger than Earth's and places it among the Neptune-like planets, whose radii reach up to four times Earth's.
Provenance
Underlying measurements and references
Evidence Summary
Rows
16
Stellar refs
13
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 |
|---|---|---|---|---|---|---|---|---|
| 5565 | 0.97 | 0.87 | — | — | — | 1379.4 | Q1-Q16 KOI Table | TICv8 |
| 5363 | — | 0.85 | — | — | — | 1379.4 | Q1-Q6 KOI Table | TICv8 |
| 5514 | 0.93 | 1.07 | — | — | — | 1379.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | — | — | — | — | — | 1379.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5050 | — | 1.16 | — | -0.10 | — | 1379.4 | Gaia DR2 | TICv8 |
| 5559 | 0.98 | 1.08 | — | 2.50e-3 | — | 1379.4 | TICv8 | TICv8 |
| 5512 | — | 1.08 | — | — | — | 1379.4 | Berger et al. 2018 | TICv8 |
| 5565 | 0.97 | 0.87 | — | — | — | 1379.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5514 | 0.93 | 1.07 | — | — | — | 1379.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5363 | 0.92 | 0.85 | — | — | — | 1379.4 | Batalha et al. 2013 | TICv8 |
| 5565 | 0.97 | 0.87 | — | — | — | 1379.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6096 | 1.15 | 1.20 | 3.24 | — | — | 1379.4 | Morton et al. 2016 | TICv8 |
| 5363 | — | 0.84 | — | — | — | 1379.4 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 1379.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5565 | 0.97 | 0.87 | — | — | — | 1379.4 | Q1-Q12 KOI Table | TICv8 |
| 5363 | 0.99 | 0.84 | — | — | — | 1379.4 | Q1-Q8 KOI Table | TICv8 |