Temperature
5816 K
5427 to 6091
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Stellar HostProfile
Kepler-1077
Unclassified star • 1101.4 pc
Records
13
literature rows
Planets
1
system count
References
14
distinct source labels
TIC: TIC 159574927
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
1.02 Msun
1.02 to 1.06
Radius
1.02 Rsun
0.92 to 1.13
Age
4.17 Gyr
0.60 to 4.17
Distance
1101.4 pc
single adopted value
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.02 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1077
1.02 R☉
System Layout
Known planets
1 planets linked to this host
Kepler-1077 b
Transit
◌
Discovery
2016
Period
34.35 days
Radius
2.77 R⊕
Mass
—
Eq. Temp
—
Kepler-1077 and Its Neptune-Like Planet
Kepler-1077 is a star located 3590 light-years away. It has one planet. The host star is 4.17 billion years old, with a mass of 1.02 solar masses and a radius of 1.02 solar radii. Its temperature is 5820 K.
The planet is Kepler-1077 b, a Neptune-like world discovered in 2016 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. Kepler-1077 b orbits once every 34.4 days. Its radius is 2.77 Earth radii, and its reported radius estimate is larger than Earth's. A Neptune-like planet reaches 4 times Earth's radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
13
Stellar refs
13
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agedisputed
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5837 | 1.02 | 0.92 | — | — | — | 1101.4 | Batalha et al. 2013 | TICv8 |
| 6091 | 1.04 | 0.97 | — | — | — | 1101.4 | Q1-Q12 KOI Table | TICv8 |
| 6091 | 1.04 | 0.97 | — | — | — | 1101.4 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6074 | 1.06 | 0.97 | 0.60 | — | — | 1101.4 | Q1-Q8 KOI Table | TICv8 |
| 6091 | 1.04 | 0.97 | — | — | — | 1101.4 | Q1-Q16 KOI Table | TICv8 |
| 5427 | — | 1.13 | — | -2.86e-3 | — | 1101.4 | Gaia DR2 | TICv8 |
| 5837 | — | 0.92 | — | — | — | 1101.4 | Q1-Q6 KOI Table | TICv8 |
| 5699.4 | 1.02 | 1.03 | — | 6.38e-3 | — | 1101.4 | TICv8 | TICv8 |
| 6091 | 1.04 | 0.97 | — | — | — | 1101.4 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5837 | — | 0.96 | — | — | — | 1101.4 | Latham et al. 2005 | TICv8 |
| — | — | — | — | — | — | 1101.4 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5816 | 1.02 | 1.02 | 4.17 | — | — | 1101.4 | Morton et al. 2016 | TICv8 |
| 6084 | — | 0.98 | — | — | — | 1101.4 | Berger et al. 2018 | TICv8 |