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Stellar HostProfile

GJ 357

M2.5 V • 9.44 pc

Records

11

literature rows

Planets

3

system count

References

12

distinct source labels

TIC: TIC 413248763HIP: HIP 47103

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. 2019 • System source: TICv8

Temperature

3505 K

3490 to 3805.5

6 values • 4 distinct

Mass

0.34 Msun

0.34 to 0.35

5 values • 4 distinct

Radius

0.34 Rsun

0.34 to 0.36

6 values • 4 distinct

Luminosity

-1.80 log(Lsun)

-1.80 to -1.70

3 values • 3 distinct

Distance

9.44 pc

single adopted value

11 values • 1 distinct

Spectral Type

M2.5 V

Multiple classifications reported

M2.5 V (4), K (1), M2.5 (1)

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 0.34 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

GJ 357

0.34 R☉

System Layout

Known planets

3 planets linked to this host

GJ 357 b

Transit

◌

Discovery

2019

Period

3.93 days

Radius

1.20 R⊕

Mass

—

Eq. Temp

518 K

GJ 357 c

Radial Velocity

◌

Discovery

2019

Period

9.12 days

Radius

—

Mass

3.40 M⊕

Eq. Temp

401.2 K

GJ 357 d

Radial Velocity

◌

Discovery

2019

Period

55.66 days

Radius

—

Mass

6.10 M⊕

Eq. Temp

219.6 K

The Planets of GJ 357

GJ 357 is an M2.5 V star, a small, cool red dwarf, located 30.8 light-years away. Its mass is 0.342 solar masses, its radius is 0.337 solar radii, and its temperature is 3510 K, all smaller or cooler than the Sun's corresponding values. Three planets are known to orbit this star: GJ 357 b, GJ 357 c, and GJ 357 d.

GJ 357 b was discovered in 2019 by the transit method, which detects the small dip in a star's brightness when a planet crosses in front of it. This planet's radius is 1.2 Earth radii, making it larger than Earth and placing it within the Earth-like size class, and its orbital period is 3.93 days, the shortest year among the listed planets.

GJ 357 c and GJ 357 d were both discovered in 2019 by the radial velocity method, which measures the wobble a planet's gravity induces in its star. GJ 357 c has a minimum mass of 3.4 Earth masses and an orbital period of 9.12 days, the second-shortest year among the listed planets. GJ 357 d has a minimum mass of 6.1 Earth masses and an orbital period of 55.7 days, the longest year among the listed planets. Both minimum masses are larger than Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

11

Stellar refs

11

System refs

1

Distancestable

11 values • 1 distinct

Parallaxstable

11 values • 1 distinct

Temperaturedisputed

6 values • 4 distinct

Massdisputed

5 values • 4 distinct

Radiusdisputed

6 values • 4 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

5 values • 4 distinct

Metallicitystable

3 values • 1 distinct

Spectral Typedisputed

6 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
——————9.44Wright et al. 2004TICv8
—————M2.59.44Hawley et al. 1996TICv8
—————M2.5 V9.44Gray et al. 2006TICv8
—0.350.36——M2.5 V9.44Weisserman et al. 2026TICv8
35050.340.34——M2.5 V9.44Oddo et al. 2023TICv8
35050.340.34—-1.80M2.5 V9.44Luque et al. 2019TICv8
34900.350.36—-1.76—9.44TICv8TICv8
——————9.44Nidever et al. 2002TICv8
3505—0.36———9.44ExoFOPTICv8
3805.5—————9.44Gaia DR2TICv8
35010.340.34—-1.70K9.44Turnbull 2015TICv8