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Stellar HostProfile

GJ 849

M3.5 • 8.80 pc

Records

13

literature rows

Planets

2

system count

References

14

distinct source labels

HIP: HIP 109388TIC: TIC 248027247

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: Pinamonti et al. 2023 • System source: TICv8

Temperature

3467 K

3241 to 3856.5

6 values • 6 distinct

Mass

0.45 Msun

0.42 to 0.65

8 values • 6 distinct

Radius

0.45 Rsun

0.45 to 0.55

5 values • 5 distinct

Luminosity

-1.59 log(Lsun)

-1.59 to -1.52

4 values • 4 distinct

Distance

8.80 pc

single adopted value

13 values • 1 distinct

Spectral Type

M3.5

Multiple classifications reported

M3.5 (3), M3 V (2), M3 (1), M3.5 V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.45 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

GJ 849

0.45 R☉

System Layout

Known planets

2 planets linked to this host

GJ 849 b

Radial Velocity

◌

Discovery

2006

Period

1925.3 days

Radius

—

Mass

283.8 M⊕

Eq. Temp

—

GJ 849 c

Radial Velocity

◌

Discovery

2014

Period

5990 days

Radius

—

Mass

314.7 M⊕

Eq. Temp

—

The Nearby Red Dwarf GJ 849 and Its Two Known Planets

GJ 849 is an M3.5 star, a cool red dwarf, located 28.7 light-years away. Its spectral class places it among the smallest and coolest stellar types. The star's reported mass is 0.45 solar masses and its radius is 0.45 solar radii, both smaller than the Sun's. Its temperature of 3470 K is cooler than the Sun's.

Two planets are known to orbit this host. The first, GJ 849 b, was found by the radial velocity method in 2006. That technique detects the wobble a planet's gravity induces in its star's motion, with repeated wobbles revealing the planet and its orbital period. GJ 849 b has a minimum mass of 284 Earth masses, meaning its true mass is at least that value, and an orbital period of 1930 days - the shortest reported year among the listed planets.

GJ 849 c was discovered by the same method in 2014. Its minimum mass is 315 Earth masses - the largest among the listed planets - and its orbital period is 5990 days, the longest reported year among them. Both planets' minimum masses are larger than Earth's.

The star's reported mass estimate and radius estimate are each smaller than the Sun's, and its reported temperature is cooler than the Sun's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

13

Stellar refs

13

System refs

1

Distancestable

13 values • 1 distinct

Parallaxstable

13 values • 1 distinct

Temperaturedisputed

6 values • 6 distinct

Massdisputed

8 values • 6 distinct

Radiusdisputed

5 values • 5 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

4 values • 3 distinct

Metallicitydisputed

5 values • 5 distinct

Spectral Typedisputed

7 values • 4 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—0.49—3—M3.5 V8.80Butler et al. 2006TICv8
34070.460.46—-1.58—8.80TICv8TICv8
34670.450.45—-1.59M3.58.80Pinamonti et al. 2023TICv8
32410.650.53———8.80Stassun et al. 2017TICv8
—0.49——-1.55M3 V8.80Bonfils et al. 2013TICv8
——————8.80Wright et al. 2004TICv8
3856.5—————8.80Gaia DR2TICv8
3562.70.500.47———8.80Rosenthal et al. 2021TICv8
—0.49———M3.58.80Montet et al. 2014TICv8
—————M3 V8.80Walker 1983TICv8
——————8.80Nidever et al. 2002TICv8
33430.420.55—-1.52M38.80Turnbull 2015TICv8
—————M3.58.80Hawley et al. 1996TICv8