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Stellar HostProfile

Kepler-1907

Unclassified star • 292.1 pc

Records

16

literature rows

Planets

2

system count

References

11

distinct source labels

TIC: TIC 123130285

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: Fulton & Petigura 2018 • System source: TICv8

Temperature

4866 K

4866 to 5159

14 values • 6 distinct

Mass

0.67 Msun

0.67 to 0.83

12 values • 4 distinct

Radius

0.67 Rsun

0.65 to 1.03

13 values • 5 distinct

Age

8.91 Gyr

8.91 to 14

3 values • 2 distinct

Distance

292.1 pc

single adopted value

16 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.67 R☉ • circles scaled linearly by radius

Sun

1.0 R☉ baseline

Kepler-1907

0.67 R☉

System Layout

Known planets

2 planets linked to this host

Discovery

2021

Period

5.65 days

Radius

0.87 R⊕

Mass

Eq. Temp

Discovery

2021

Period

14.86 days

Radius

1.16 R⊕

Mass

Eq. Temp

Kepler-1907: A Cool Dwarf with Two Small Worlds

Kepler-1907 is a star located 953 light-years away, and it hosts two known planets. The star is estimated to be 8.91 billion years old, with a mass of 0.673 solar masses and a radius of 0.665 solar radii. Its temperature is 4870 K, making it cooler than the Sun, and both its mass and radius are smaller than the Sun's.

Both planets were discovered in 2021 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-1907 b is classified as a Sub-Earth, meaning its radius is smaller than Earth's. It has an orbital period of 5.65 days and a radius of 0.87 Earth radii, which is smaller than Earth's. Among the listed planets, Kepler-1907 b has the shortest year and the smallest radius.

Kepler-1907 c is classified as Earth-like, a size class that stays within 1.5 times Earth's radius. It has an orbital period of 14.9 days and a radius of 1.16 Earth radii, larger than Earth's. Among the listed planets, Kepler-1907 c has the longest year and the largest radius.

Provenance

Underlying measurements and references

Evidence Summary

Rows

16

Stellar refs

10

System refs

1

Distancestable

16 values • 1 distinct

Parallaxstable

16 values • 1 distinct

Temperaturedisputed

14 values • 6 distinct

Massdisputed

12 values • 4 distinct

Radiusdisputed

13 values • 5 distinct

Agedisputed

3 values • 2 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitydisputed

13 values • 5 distinct

Metallicitydisputed

11 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
51590.750.80292.1Q1-Q17 DR25 KOI TableTICv8
51420.760.7814292.1Q1-Q8 KOI TableTICv8
49821.03292.1Latham et al. 2005TICv8
4895292.1KIC - SCPKEYTICv8
51590.750.80292.1Q1-Q17 DR24 KOI TableTICv8
51590.750.80292.1Q1-Q16 KOI TableTICv8
50070.830.65-0.62292.1TICv8TICv8
51590.750.80292.1Q1-Q17 DR24 KOI TableTICv8
292.1Q1-Q17 DR25 Supplemental KOI TableTICv8
292.1Q1-Q17 DR25 Supplemental KOI TableTICv8
48660.670.678.91292.1Fulton & Petigura 2018TICv8
51590.750.80292.1Q1-Q17 DR25 KOI TableTICv8
51590.750.80292.1Q1-Q16 KOI TableTICv8
51420.760.7814292.1Q1-Q8 KOI TableTICv8
51590.750.80292.1Q1-Q12 KOI TableTICv8
51590.750.80292.1Q1-Q12 KOI TableTICv8