Temperature
6412 K
6154 to 6503.6
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Stellar HostProfile
Kepler-348
Unclassified star • 570.8 pc
Records
20
literature rows
Planets
2
system count
References
16
distinct source labels
TIC: TIC 169180792
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
1.27 Msun
1.15 to 1.33
Radius
1.39 Rsun
1.00 to 1.40
Age
2.29 Gyr
0.29 to 2.29
Distance
570.8 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.39 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-348
1.39 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-348 b
Transit
◌
Discovery
2014
Period
7.06 days
Radius
1.52 R⊕
Mass
—
Eq. Temp
—
Kepler-348 c
Transit
◌
Discovery
2014
Period
17.27 days
Radius
1.33 R⊕
Mass
—
Eq. Temp
—
Kepler-348: A Star with Two Small Worlds
Kepler-348 is a star located 1860 light-years away. It is 2.29 billion years old and has a mass of 1.27 solar masses, a radius of 1.39 solar radii, and a temperature of 6410 K. The star's reported mass estimate is larger than the Sun's, its reported radius estimate is larger than the Sun's, and its reported temperature is hotter than the Sun's. Two planets are known to orbit this star.
Kepler-348 b is a Super-Earth discovered by transit in 2014. It has an orbital period of 7.06 days and a radius of 1.52 Earth radii, larger than Earth's. Kepler-348 c is an Earth-like planet, also discovered by transit in 2014. It has an orbital period of 17.3 days and a radius of 1.33 Earth radii, likewise larger than Earth's. Among the listed planets, Kepler-348 b has the shortest year and the largest radius, while Kepler-348 c has the longest year and the smallest radius. A transit occurs when a planet passes in front of its star from our viewpoint, causing a small dip in observed brightness.
Provenance
Underlying measurements and references
Evidence Summary
Rows
20
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 |
|---|---|---|---|---|---|---|---|---|
| — | — | — | — | — | — | 570.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6154 | 1.15 | 1.06 | — | — | — | 570.8 | Batalha et al. 2013 | TICv8 |
| — | — | — | — | — | — | 570.8 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 6395 | 1.20 | 1.19 | — | — | — | 570.8 | Q1-Q12 KOI Table | TICv8 |
| 6503.6 | 1.33 | 1.30 | — | 0.43 | — | 570.8 | TICv8 | TICv8 |
| 6335 | — | 1.25 | — | 0.36 | — | 570.8 | Gaia DR2 | TICv8 |
| 6395 | 1.20 | 1.19 | — | — | — | 570.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6388 | 1.26 | 1.40 | — | — | — | 570.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6154 | — | 1.00 | — | — | — | 570.8 | Latham et al. 2005 | TICv8 |
| 6388 | 1.26 | 1.40 | — | — | — | 570.8 | Q1-Q17 DR25 KOI Table | TICv8 |
| 6395 | 1.20 | 1.19 | — | — | — | 570.8 | Q1-Q16 KOI Table | TICv8 |
| 6421 | 1.19 | 1.30 | 2.29 | — | — | 570.8 | Fulton & Petigura 2018 | TICv8 |
| 6412 | 1.27 | 1.39 | 2.29 | — | — | 570.8 | Morton et al. 2016 | TICv8 |
| 6395 | 1.20 | 1.19 | — | — | — | 570.8 | Q1-Q12 KOI Table | TICv8 |
| 6395 | 1.20 | 1.19 | — | — | — | 570.8 | Q1-Q17 DR24 KOI Table | TICv8 |
| 6421 | — | 1.32 | — | — | — | 570.8 | Berger et al. 2018 | TICv8 |
| 6154 | — | 1.06 | — | — | — | 570.8 | Q1-Q6 KOI Table | TICv8 |
| 6395 | 1.20 | 1.19 | — | — | — | 570.8 | Q1-Q16 KOI Table | TICv8 |
| 6177 | — | 1.36 | — | — | — | 570.8 | Rowe et al. 2014 | TICv8 |
| 6361 | 1.16 | 1.08 | 0.29 | — | — | 570.8 | Q1-Q8 KOI Table | TICv8 |