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Stellar HostProfile

K2-260

F6 V • 663.8 pc

Records

5

literature rows

Planets

1

system count

References

6

distinct source labels

TIC: TIC 293612446

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: Johnson et al. 2018 • System source: TICv8

Temperature

6367 K

5859 to 6860

5 values • 4 distinct

Mass

1.39 Msun

1.32 to 1.64

3 values • 3 distinct

Radius

1.69 Rsun

1.69 to 1.81

5 values • 5 distinct

Age

1.90 Gyr

0.65 to 1.90

2 values • 2 distinct

Distance

663.8 pc

single adopted value

5 values • 1 distinct

Spectral Type

F6 V

Consistent across records

F6 V (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.69 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

K2-260

1.69 R☉

System Layout

Known planets

1 planets linked to this host

K2-260 b

Transit

◌

Discovery

2018

Period

2.63 days

Radius

18.42 R⊕

Mass

546.7 M⊕

Eq. Temp

2090 K

K2-260 b: A Giant World Around an F-Type Star

K2-260 is a single known planet system located 2170 light-years away. Its host star is an F6 V main-sequence dwarf with a mass of 1.39 solar masses, a radius of 1.69 solar radii, and a temperature of 6370 K. The star is 1.9 billion years old. Its reported mass and radius estimates are larger than the Sun's, and its temperature is hotter.

The system's only known planet is K2-260 b, a Jupiter-like world discovered in 2018 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. K2-260 b orbits its star every 2.63 days. Its radius is 18.4 Earth radii, well beyond the roughly 4-Earth-radius threshold that defines the Jupiter-like class. With a mass of 547 Earth masses, the planet is roughly 1.72 times Jupiter's mass, and both its mass and radius estimates are larger than Earth's. Its mean density is 0.482 g/cm³, which is 0.0875 times Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

5

Stellar refs

5

System refs

1

Distancestable

5 values • 1 distinct

Parallaxstable

5 values • 1 distinct

Temperaturedisputed

5 values • 4 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

5 values • 5 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

4 values • 3 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
63671.391.691.90—F6 V663.8Johnson et al. 2018TICv8
64751.321.77—0.70—663.8TICv8TICv8
6475—1.77———663.8ExoFOPTICv8
5859—1.81—0.54—663.8Gaia DR2TICv8
68601.641.750.650.79—663.8Thygesen et al. 2023TICv8