Temperature
5432.3 K
5356 to 5693
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Stellar HostProfile
Kepler-1693
Unclassified star • 760.1 pc
Records
20
literature rows
Planets
2
system count
References
10
distinct source labels
TIC: TIC 406948151
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: TICv8 • System source: TICv8
Mass
0.95 Msun
0.94 to 0.95
Radius
0.88 Rsun
0.84 to 1.10
Luminosity
-0.22 log(Lsun)
-0.23 to -0.22
Distance
760.1 pc
single adopted value
Planets
2
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.88 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
Kepler-1693
0.88 R☉
System Layout
Known planets
2 planets linked to this host
Kepler-1693 b
Transit
◌
Discovery
2020
Period
12.10 days
Radius
1.29 R⊕
Mass
—
Eq. Temp
—
Kepler-1693 c
Transit
◌
Discovery
2021
Period
5.36 days
Radius
0.98 R⊕
Mass
—
Eq. Temp
—
Planets of Kepler-1693
Kepler-1693 is a star 2480 light-years away with two known planets. The host star has a reported mass of 0.95 solar masses and a radius of 0.878 solar radii. Its reported temperature is 5430 K. Both planets were found 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. Repeated dips help establish orbital periods.
Kepler-1693 b is classified as Earth-like and was discovered in 2020. Its orbital period is 12.1 days, and its radius is 1.29 Earth radii, larger than Earth's. Kepler-1693 c is classified as Sub-Earth and was discovered in 2021. Its orbital period is 5.36 days, and its radius is 0.977 Earth radii, smaller than Earth's. Among the listed planets, Kepler-1693 c has the shortest year by reported estimates, while Kepler-1693 b has the longest year by reported estimates. Kepler-1693 c also has the smallest radius by reported estimates, and Kepler-1693 b has the largest radius by reported estimates.
Provenance
Underlying measurements and references
Evidence Summary
Rows
20
Stellar refs
9
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 |
|---|---|---|---|---|---|---|---|---|
| 5553 | 0.94 | 1.10 | — | — | — | 760.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5693 | 0.95 | 0.86 | — | — | — | 760.1 | Q1-Q12 KOI Table | TICv8 |
| 5693 | 0.95 | 0.86 | — | — | — | 760.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5693 | 0.95 | 0.86 | — | — | — | 760.1 | Q1-Q16 KOI Table | TICv8 |
| 5553 | 0.94 | 1.10 | — | — | — | 760.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| 5677 | 0.94 | 0.84 | 0.80 | — | — | 760.1 | Q1-Q8 KOI Table | TICv8 |
| 5356 | — | 0.89 | — | -0.23 | — | 760.1 | Gaia DR2 | TICv8 |
| 5677 | 0.94 | 0.84 | 0.80 | — | — | 760.1 | Q1-Q8 KOI Table | TICv8 |
| — | — | — | — | — | — | 760.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5693 | 0.95 | 0.86 | — | — | — | 760.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| 5432.3 | 0.95 | 0.88 | — | -0.22 | — | 760.1 | TICv8 | TICv8 |
| 5693 | 0.95 | 0.86 | — | — | — | 760.1 | Q1-Q16 KOI Table | TICv8 |
| 5553 | 0.94 | 1.10 | — | — | — | 760.1 | Q1-Q17 DR25 KOI Table | TICv8 |
| — | — | — | — | — | — | 760.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5693 | 0.95 | 0.86 | — | — | — | 760.1 | Q1-Q16 KOI Table | TICv8 |
| 5503 | — | 0.86 | — | — | — | 760.1 | Latham et al. 2005 | TICv8 |
| 5693 | 0.95 | 0.86 | — | — | — | 760.1 | Q1-Q17 DR24 KOI Table | TICv8 |
| — | — | — | — | — | — | 760.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |
| 5693 | 0.95 | 0.86 | — | — | — | 760.1 | Q1-Q12 KOI Table | TICv8 |
| — | — | — | — | — | — | 760.1 | Q1-Q17 DR25 Supplemental KOI Table | TICv8 |