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Stellar HostProfile

GJ 581

M3.0 V • 6.30 pc

Records

12

literature rows

Planets

3

system count

References

13

distinct source labels

TIC: TIC 36853511HIP: HIP 74995

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: von Stauffenberg et al. 2024 • System source: TICv8

Temperature

3500 K

3375 to 3660.3

5 values • 5 distinct

Mass

0.29 Msun

0.29 to 0.33

6 values • 5 distinct

Radius

0.30 Rsun

0.29 to 0.34

6 values • 5 distinct

Luminosity

-1.91 log(Lsun)

-2 to -1.89

5 values • 5 distinct

Distance

6.30 pc

single adopted value

12 values • 1 distinct

Spectral Type

M3.0 V

Multiple classifications reported

M3 V (2), M2.5 V (1), M3 (1), M3.0 V (1), M3.0V (1)

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 0.30 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

GJ 581

0.30 R☉

System Layout

Known planets

3 planets linked to this host

GJ 581 b

Radial Velocity

◌

Discovery

2005

Period

5.37 days

Radius

—

Mass

20.50 M⊕

Eq. Temp

—

GJ 581 c

Radial Velocity

◌

Discovery

2007

Period

12.92 days

Radius

—

Mass

6.81 M⊕

Eq. Temp

—

GJ 581 e

Radial Velocity

◌

Discovery

2009

Period

3.15 days

Radius

—

Mass

2.48 M⊕

Eq. Temp

—

GJ 581: A Nearby Red Dwarf and Its Three Known Worlds

GJ 581 is an M3.0 V star, a small, cool red dwarf, located 20.5 light-years from Earth. Its spectral type places it in the coolest and reddest temperature class. The star has a reported mass of 0.295 solar masses and a reported radius of 0.302 solar radii. Both estimates are reported as smaller than the Sun's corresponding values, and its temperature of 3500 K is reported as cooler than the Sun's. Three planets orbit this star.

All three planets were found using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. GJ 581 e was discovered first among the group, in 2009, and has a minimum mass of 2.48 Earth masses and an orbital period of 3.15 days. GJ 581 b was discovered in 2005, with a mass of 20.5 Earth masses and an orbital period of 5.37 days. GJ 581 c, discovered in 2007, has a mass of 6.81 Earth masses and an orbital period of 12.9 days. The reported mass estimates for all three are larger than Earth's.

Among the listed planets, GJ 581 e has the shortest year by reported estimates, while GJ 581 c has the longest. GJ 581 b has the second-shortest year. In terms of mass, GJ 581 e has the smallest reported mass among the listed planets, GJ 581 c has the second-smallest, and GJ 581 b has the largest reported mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

12

Stellar refs

12

System refs

1

Distancestable

12 values • 1 distinct

Parallaxstable

12 values • 1 distinct

Temperaturedisputed

5 values • 5 distinct

Massdisputed

6 values • 5 distinct

Radiusdisputed

6 values • 5 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

5 values • 5 distinct

Surface Gravitydisputed

3 values • 3 distinct

Metallicitydisputed

3 values • 3 distinct

Spectral Typedisputed

6 values • 5 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—0.310.294.30-1.89M3 V6.30Vogt et al. 2010TICv8
33750.330.34—-2M3.0V6.30Turnbull 2015TICv8
33960.310.33—-1.89—6.30TICv8TICv8
——————6.30Mayor et al. 2009TICv8
—0.310.292-1.89M3 V6.30Bonfils et al. 2005TICv8
—————M36.30Hawley et al. 1996TICv8
3490.40.320.32———6.30Rosenthal et al. 2021TICv8
—————M2.5 V6.30Henry et al. 1994TICv8
——————6.30Wright et al. 2004TICv8
3660.3—————6.30Gaia DR2TICv8
35000.290.30—-1.91M3.0 V6.30von Stauffenberg et al. 2024TICv8
——————6.30Nidever et al. 2002TICv8