Stellar HostProfile

HD 56957

Unclassified star • 61.49 pc

Records

literature rows

Planets

system count

References

distinct source labels

HD: HD 56957TIC: TIC 22972926

Approximate color

from effective temperature

Stellar source: TICv8 • System source: TICv8

Temperature

5743 K

single adopted value

1 values • 1 distinct

Mass

1.03 Msun

single adopted value

2 values • 1 distinct

Radius

1.78 Rsun

single adopted value

1 values • 1 distinct

Luminosity

0.49 log(Lsun)

single adopted value

1 values • 1 distinct

Distance

61.49 pc

single adopted value

2 values • 1 distinct

Planets

Stable across source rows

Sun

1.0 R☉ baseline

HD 56957

1.78 R☉

Discovery

2022

Period

5859.1 days

Radius

—

Mass

1880.9 M⊕

Eq. Temp

—

HD 56957 and Its Giant Planet

HD 56957 is a star 201 light-years from Earth with one known planet. The star has a mass of 1.03 solar masses, a radius of 1.78 solar radii, and a temperature of 5740 K. Its radius is larger than the Sun's.

The orbiting planet, HD 56957 b, was discovered in 2022 by 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. HD 56957 b has a mass of 1880 Earth masses and an orbital period of 5860 days. Its mass is larger than Earth's and roughly 5.92 times Jupiter's mass.

Evidence Summary

Rows

Stellar refs

System refs

Distancestable

2 values • 1 distinct

Parallaxstable

2 values • 1 distinct

Temperaturestable

1 values • 1 distinct

Massstable

2 values • 1 distinct

Radiusstable

1 values • 1 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitystable

1 values • 1 distinct

ST TEFF	ST MASS	ST RAD	ST AGE	ST LUM	ST SPECTYPE	SY DIST	Stellar Ref	System Ref
5743	1.03	1.78	—	0.49	—	61.49	TICv8	TICv8
—	1.03	—	—	—	—	61.49	Feng et al. 2022	TICv8

HD 56957

Adopted host values from one source row

Radius against the Sun

Known planets

HD 56957 b

HD 56957 and Its Giant Planet

Underlying measurements and references