←Back to Stellar Hosts
Stellar HostProfile

HD 3651

K0V • 11.13 pc

Records

36

literature rows

Planets

1

system count

References

21

distinct source labels

HIP: HIP 3093HD: HD 3651TIC: TIC 434210589

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: Turnbull 2015 • System source: TICv8

Temperature

5221 K

5173 to 5280

10 values • 8 distinct

Mass

0.88 Msun

0.76 to 0.90

8 values • 6 distinct

Radius

0.88 Rsun

0.85 to 0.88

6 values • 5 distinct

Age

8.20 Gyr

3 to 11.80

4 values • 4 distinct

Luminosity

-0.27 log(Lsun)

-0.30 to -0.27

4 values • 4 distinct

Distance

11.13 pc

single adopted value

36 values • 1 distinct

Spectral Type

K0V

Multiple classifications reported

K0 V (2), K0 (1), K0V (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 0.88 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 3651

0.88 R☉

System Layout

Known planets

1 planets linked to this host

HD 3651 b

Radial Velocity

◌

Discovery

2003

Period

62.25 days

Radius

—

Mass

72.47 M⊕

Eq. Temp

—

HD 3651 b: A Close-Orbiting Planet Around a Cool Dwarf

HD 3651 is a K0V star 36.3 light-years away. K-type stars are cooler and redder than the Sun, and this one has a reported mass of 0.88 solar masses and a radius of 0.88 solar radii, smaller than the Sun on both counts. Its temperature is 5220 K, cooler than the Sun's, and its age is 8.2 billion years. One planet orbits this host.

HD 3651 b was found in 2003 using the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. The planet's minimum mass is 72.5 Earth masses, a lower bound on its true mass that is larger than Earth's. It completes one orbit every 62.3 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

36

Stellar refs

20

System refs

1

Distancestable

36 values • 1 distinct

Parallaxstable

36 values • 1 distinct

Temperaturedisputed

10 values • 8 distinct

Massdisputed

8 values • 6 distinct

Radiusdisputed

6 values • 5 distinct

Agedisputed

4 values • 4 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

8 values • 7 distinct

Metallicitydisputed

7 values • 6 distinct

Spectral Typedisputed

4 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
52210.80————11.13Wittenmyer et al. 2019TICv8
——————11.13Valenti & Fischer 2005TICv8
——————11.13Duncan et al. 1991TICv8
52520.900.853-0.30—11.13Ghezzi et al. 2010TICv8
———4.46——11.13Sanz-Forcada et al. 2010TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Duncan et al. 1991TICv8
—0.880.8811.80——11.13Takeda et al. 2007TICv8
5274.90.900.87—-0.27—11.13TICv8TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Pizzolato et al. 2003TICv8
5205.90.890.87———11.13Rosenthal et al. 2021TICv8
——————11.13Nordstrom et al. 2004TICv8
5203—————11.13Harada et al. 2025TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Duncan et al. 1991TICv8
—————K0 V11.13Gray et al. 2003TICv8
52210.88———K0 V11.13Wittenmyer et al. 2009TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Nidever et al. 2002TICv8
51730.76————11.13Santos et al. 2004TICv8
—————K011.13Cannon & Pickering 1918TICv8
——————11.13Duncan et al. 1991TICv8
5249—————11.13Maldonado et al. 2015TICv8
52210.880.888.20-0.27K0V11.13Turnbull 2015TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Duncan et al. 1991TICv8
5280—0.88—-0.27—11.13Gaia DR2TICv8
——————11.13Duncan et al. 1991TICv8
——————11.13Wright et al. 2004TICv8
——————11.13Duncan et al. 1991TICv8