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Stellar HostProfile

HD 260655

M0 V • 10.01 pc

Records

12

literature rows

Planets

2

system count

References

11

distinct source labels

HIP: HIP 31635TIC: TIC 307809773HD: HD 260655

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: Luque et al. 2022 • System source: TICv8

Temperature

3803 K

3803 to 3843

5 values • 3 distinct

Mass

0.44 Msun

0.43 to 0.46

4 values • 4 distinct

Radius

0.44 Rsun

0.43 to 0.47

6 values • 5 distinct

Age

5 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-1.44 log(Lsun)

-1.44 to -1.39

3 values • 3 distinct

Distance

10.01 pc

single adopted value

12 values • 1 distinct

Spectral Type

M0 V

Multiple classifications reported

M0 V (2), K2 (1), K7 (1), M1: (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.44 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 260655

0.44 R☉

System Layout

Known planets

2 planets linked to this host

◌

Discovery

2022

Period

2.77 days

Radius

1.24 R⊕

Mass

2.14 M⊕

Eq. Temp

709 K

◌

Discovery

2022

Period

5.71 days

Radius

1.53 R⊕

Mass

3.09 M⊕

Eq. Temp

557 K

HD 260655 and Its Two Planets

HD 260655 is an M0 V star, a small, cool red dwarf, located 32.6 light-years away. Its reported mass and radius are each 0.439 solar masses and 0.439 solar radii, both smaller than the Sun's, and its temperature of 3800 K is cooler than the Sun's. The star is 5 billion years old, and two planets are known to orbit it.

Both planets were discovered by transit in 2022. HD 260655 b is classified as Earth-like, with a radius of 1.24 Earth radii and a mass of 2.14 Earth masses, both larger than Earth's. It completes an orbit in 2.77 days. Its mean density is 6.18 g/cm³, 1.12 times Earth's. Among the listed planets, HD 260655 b has the shortest year, the smallest radius, and the smallest reported mass.

HD 260655 c is classified as a Super-Earth. Its radius is 1.53 Earth radii and its mass is 3.09 Earth masses, each larger than Earth's. It orbits in 5.71 days, and its mean density is 4.73 g/cm³, 0.858 times Earth's. Among the listed planets, HD 260655 c has the longest year, the largest radius, and the largest reported mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

12

Stellar refs

10

System refs

1

Distancestable

12 values • 1 distinct

Parallaxstable

12 values • 1 distinct

Temperaturedisputed

5 values • 3 distinct

Massdisputed

4 values • 4 distinct

Radiusdisputed

6 values • 5 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

5 values • 3 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typedisputed

5 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
——————10.01Wright et al. 2004TICv8
38430.430.43—-1.40M1:10.01Turnbull 2015TICv8
38030.440.445-1.44M0 V10.01Luque et al. 2022TICv8
—0.460.47——M0 V10.01Weisserman et al. 2026TICv8
3807—0.47———10.01ExoFOPTICv8
—————K710.01Hawley et al. 1996TICv8
——————10.01Duncan et al. 1991TICv8
——————10.01Nidever et al. 2002TICv8
38070.460.47—-1.39—10.01TICv8TICv8
——————10.01Duncan et al. 1991TICv8
3807—0.47———10.01ExoFOPTICv8
—————K210.01Cannon & Pickering 1918TICv8