Temperature
6018 K
5539.5 to 6064
←Back to Stellar Hosts
Stellar HostProfile
Kepler-175
Unclassified star • 1312.3 pc
Records
22
literature rows
Planets
2
system count
References
16
distinct source labels
TIC: TIC 159099116
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
1.12 Msun
0.97 to 1.12
Radius
1.17 Rsun
0.93 to 1.34
Age
3.39 Gyr
0.40 to 9.12
Distance
1312.3 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.17 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-175
1.17 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-175 b
Transit
◌
Discovery
2014
Period
11.90 days
Radius
2.56 R⊕
Mass
—
Eq. Temp
—
Kepler-175 c
Transit
◌
Discovery
2014
Period
34.04 days
Radius
3.10 R⊕
Mass
—
Eq. Temp
—
Kepler-175 and Its Two Neptune-Like Planets
Kepler-175 is a star located 4280 light-years away, and two planets orbit it. The host star is 3.39 billion years old, with a mass of 1.12 solar masses and a radius of 1.17 solar radii. Its temperature is 6020 K, and its reported mass, radius, and temperature are all larger or hotter than the Sun's.
Both planets were discovered by the transit method in 2014. Kepler-175 b is Neptune-like, with a radius of 2.56 Earth radii and an orbital period of 11.9 days. Kepler-175 c is also Neptune-like, with a radius of 3.1 Earth radii and an orbital period of 34 days. Both planets are larger than Earth in radius. Among the listed planets, Kepler-175 b has the shortest year and the smallest radius, while Kepler-175 c has the longest year and the largest radius.
Provenance
Underlying measurements and references
Evidence Summary
Rows
22
Stellar refs
15
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 |
|---|---|---|---|---|---|---|---|---|
| 5735 | 0.97 | 1.18 | 9.12 | — | — | 1312.3 | Fulton & Petigura 2018 | TICv8 |
| — | — | — | — | — | — | 1312.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6064 | — | 1.01 | — | — | — | 1312.3 | Rowe et al. 2014 | TICv8 |
| 6029 | 1.04 | 0.95 | 0.40 | — | — | 1312.3 | Q1-Q8 KOI Table | TICv8 |
| 5721 | 1.02 | 1.27 | — | 0.19 | — | 1312.3 | TICv8 | TICv8 |
| — | — | — | — | — | — | 1312.3 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5539.5 | — | 1.34 | — | 0.18 | — | 1312.3 | Gaia DR2 | TICv8 |
| 6063 | 1.08 | 1.00 | — | — | — | 1312.3 | Q1-Q12 KOI Table | TICv8 |
| 6063 | 1.08 | 1.00 | — | — | — | 1312.3 | Q1-Q16 KOI Table | TICv8 |
| 5735 | — | 1.21 | — | — | — | 1312.3 | Berger et al. 2018 | TICv8 |
| 6063 | 1.08 | 1.00 | — | — | — | 1312.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6018 | 1.12 | 1.17 | 3.39 | — | — | 1312.3 | Morton et al. 2016 | TICv8 |
| 6063 | 1.08 | 1.00 | — | — | — | 1312.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6063 | 1.08 | 1.00 | — | — | — | 1312.3 | Q1-Q16 KOI Table | TICv8 |
| 5807 | — | 0.93 | — | — | — | 1312.3 | Q1-Q6 KOI Table | TICv8 |
| 6063 | 1.08 | 1.00 | — | — | — | 1312.3 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6063 | 1.08 | 1.00 | — | — | — | 1312.3 | Q1-Q12 KOI Table | TICv8 |
| 5807 | 1.04 | 0.93 | — | — | — | 1312.3 | Batalha et al. 2013 | TICv8 |
| 5807 | — | 0.93 | — | — | — | 1312.3 | Q1-Q6 KOI Table | TICv8 |
| 5807 | — | 0.94 | — | — | — | 1312.3 | Latham et al. 2005 | TICv8 |
| 6063 | 1.08 | 1.00 | — | — | — | 1312.3 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6029 | 1.04 | 0.95 | 0.40 | — | — | 1312.3 | Q1-Q8 KOI Table | TICv8 |