←Back to Stellar Hosts
Stellar HostProfile

GJ 486

M3.5 V • 8.07 pc

Records

10

literature rows

Planets

1

system count

References

11

distinct source labels

HIP: HIP 62452TIC: TIC 390651552

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: Caballero et al. 2022 • System source: TICv8

Temperature

3291 K

3267 to 3588.5

7 values • 6 distinct

Mass

0.33 Msun

0.31 to 0.34

5 values • 5 distinct

Radius

0.34 Rsun

0.32 to 0.37

6 values • 5 distinct

Age

4 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-1.92 log(Lsun)

-2 to -1.92

5 values • 5 distinct

Distance

8.07 pc

single adopted value

10 values • 1 distinct

Spectral Type

M3.5 V

Multiple classifications reported

M3.5 V (2), M3.5 (1), M4 (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

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

Sun

1.0 R☉ baseline

GJ 486

0.34 R☉

System Layout

Known planets

1 planets linked to this host

GJ 486 b

Radial Velocity

◌

Discovery

2021

Period

1.47 days

Radius

1.29 R⊕

Mass

2.77 M⊕

Eq. Temp

696.3 K

GJ 486 and Its Earth-Like Planet

GJ 486 is an M3.5 V star, a small, cool red dwarf, located 26.3 light-years from Earth. It has one known planet. Its spectral type places it in the M class, the coolest and reddest of the main-sequence temperature classes. The star's mass is 0.333 solar masses, its radius is 0.339 solar radii, and its temperature is 3290 K. Its age is 4 billion years. Each of these stellar measurements applies to the host star itself, and the reported mass, radius, and temperature estimates all fall below the corresponding values for the Sun.

The single planet, GJ 486 b, was discovered in 2021 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. GJ 486 b orbits its host in 1.47 days, and its mean density is 7.13 g/cm³, 1.29 times Earth's. The planet's radius is 1.29 Earth radii, larger than Earth's, which keeps it within the Earth-like size class of 1.5 times Earth's radius. Its mass is 2.77 Earth masses, also larger than Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

10

Stellar refs

10

System refs

1

Distancestable

10 values • 1 distinct

Parallaxstable

10 values • 1 distinct

Temperaturedisputed

7 values • 6 distinct

Massdisputed

5 values • 5 distinct

Radiusdisputed

6 values • 5 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

5 values • 5 distinct

Surface Gravitydisputed

4 values • 4 distinct

Metallicitydisputed

3 values • 2 distinct

Spectral Typedisputed

4 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
32970.310.33—-1.93—8.07TICv8TICv8
—————M3.58.07Hawley et al. 1996TICv8
——————8.07Nidever et al. 2002TICv8
——————8.07Wright et al. 2004TICv8
3297—0.33———8.07ExoFOPTICv8
32910.330.344-1.92M3.5 V8.07Caballero et al. 2022TICv8
32670.340.37—-2M48.07Turnbull 2015TICv8
3588.5—————8.07Gaia DR2TICv8
33400.320.33—-1.92M3.5 V8.07Trifonov et al. 2021TICv8
33170.310.32—-1.94—8.07Weiner Mansfield et al. 2024TICv8