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Stellar HostProfile

GJ 676 A

Unclassified star • 16.03 pc

Records

9

literature rows

Planets

4

system count

References

10

distinct source labels

HIP: HIP 85647TIC: TIC 369021303

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: Stassun et al. 2017 • System source: TICv8

Temperature

3734 K

3734 to 4006.0

4 values • 3 distinct

Mass

0.73 Msun

0.56 to 0.73

5 values • 5 distinct

Radius

0.69 Rsun

0.63 to 0.73

4 values • 4 distinct

Distance

16.03 pc

single adopted value

9 values • 1 distinct

Planets

4

Stable across source rows

4

Scale Comparison

Radius against the Sun

Current adopted radius: 0.69 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

GJ 676 A

0.69 R☉

System Layout

Known planets

4 planets linked to this host

GJ 676 A b

Radial Velocity

◌

Discovery

2010

Period

1051.4 days

Radius

—

Mass

1840.9 M⊕

Eq. Temp

—

GJ 676 A c

Radial Velocity

◌

Discovery

2016

Period

1.39e4 days

Radius

—

Mass

4288.1 M⊕

Eq. Temp

—

GJ 676 A d

Radial Velocity

◌

Discovery

2012

Period

3.60 days

Radius

—

Mass

3.81 M⊕

Eq. Temp

—

GJ 676 A e

Radial Velocity

◌

Discovery

2012

Period

35.47 days

Radius

—

Mass

6.67 M⊕

Eq. Temp

—

GJ 676 A and Its Four Planets

GJ 676 A is an M0 V star, a small, cool red dwarf, located 52.3 light-years away. Its reported mass estimate is 0.73 solar masses, its radius is 0.69 solar radii, and its temperature is 3730 K. Each of these values is smaller or cooler than the corresponding value for the Sun. Four planets have been reported orbiting this star.

GJ 676 A b was discovered in 2010 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. Its mass is 1840 Earth masses, roughly 5.79 times Jupiter's mass, and its orbital period is 1050 days. GJ 676 A c, also found by radial velocity, was discovered in 2016. Its mass is 4290 Earth masses, roughly 13.5 times Jupiter's mass, and its orbital period is 13900 days, the longest among these four planets.

The two remaining planets were both discovered in 2012 by radial velocity. GJ 676 A d has a minimum mass of 3.81 Earth masses and an orbital period of 3.6 days, the shortest among the listed planets. GJ 676 A e has a minimum mass of 6.67 Earth masses and an orbital period of 35.5 days. For both of these planets, the reported minimum mass is larger than Earth's, and the value represents a lower bound on the planet's true mass rather than an ordinary mass estimate.

Provenance

Underlying measurements and references

Evidence Summary

Rows

9

Stellar refs

9

System refs

1

Distancestable

9 values • 1 distinct

Parallaxstable

9 values • 1 distinct

Temperaturedisputed

4 values • 3 distinct

Massdisputed

5 values • 5 distinct

Radiusdisputed

4 values • 4 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

2 values • 2 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typedisputed

4 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
37340.730.69———16.03Stassun et al. 2017TICv8
4006.0—0.63—-1.04—16.03Gaia DR2TICv8
—————M0 V16.03Forveille et al. 2011TICv8
38510.630.65—-1.08—16.03TICv8TICv8
—0.71———M0 V16.03Anglada-Escude & Tuomi 2012TICv8
—————M0.016.03Hawley et al. 1996TICv8
—0.63————16.03Feng et al. 2022TICv8
38510.560.73—-0.96M016.03Turnbull 2015TICv8
——————16.03Sahlmann et al. 2016TICv8