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GJ 667 C

M1.5 V โ€ข 7.24 pc

Records

8

literature rows

Planets

5

system count

References

9

distinct source labels

TIC: TIC 154385809

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: Anglada-Escude et al. 2013 โ€ข System source: TICv8

Temperature

3350 K

3350 to 3775.4

4 values โ€ข 4 distinct

Mass

0.33 Msun

single adopted value

2 values โ€ข 1 distinct

Age

2 Gyr

single adopted value

1 values โ€ข 1 distinct

Luminosity

-1.86 log(Lsun)

-1.86 to -1.85

2 values โ€ข 2 distinct

Distance

7.24 pc

single adopted value

8 values โ€ข 1 distinct

Spectral Type

M1.5 V

Multiple classifications reported

M1.5 (1), M1.5 V (1)

Planets

5

Stable across source rows

5

System Layout

Known planets

5 planets linked to this host

GJ 667 C b

Radial Velocity

โ—Œ

Discovery

2012

Period

7.20 days

Radius

โ€”

Mass

โ€”

Eq. Temp

โ€”

GJ 667 C c

Radial Velocity

โ—Œ

Discovery

2013

Period

28.14 days

Radius

โ€”

Mass

3.80 MโŠ•

Eq. Temp

โ€”

GJ 667 C e

Radial Velocity

โ—Œ

Discovery

2013

Period

62.24 days

Radius

โ€”

Mass

2.70 MโŠ•

Eq. Temp

โ€”

GJ 667 C f

Radial Velocity

โ—Œ

Discovery

2013

Period

39.03 days

Radius

โ€”

Mass

2.70 MโŠ•

Eq. Temp

โ€”

GJ 667 C g

Radial Velocity

โ—Œ

Discovery

2013

Period

256.2 days

Radius

โ€”

Mass

4.60 MโŠ•

Eq. Temp

โ€”

The Planets of GJ 667 C

GJ 667 C is an M1.5 V star 23.6 light-years away with five planets orbiting it. Its spectral type describes a small, cool red dwarf, and its reported temperature of 3350 K is cooler than the Sun's. The star's reported mass is 0.33 solar masses, smaller than the Sun's, and its age carries a reported lower limit of 2 billion years.

Radial velocity observations revealed the planets, which range in minimum mass from 2.7 to 4.6 Earth masses. A minimum mass is a lower bound on a planet's true mass, so each of these values marks how light the world could be rather than a precise figure. Two of the planets, GJ 667 C e and GJ 667 C f, share the same minimum mass of 2.7 Earth masses, while GJ 667 C c reaches 3.8 Earth masses and GJ 667 C g is the heaviest of the group at 4.6 Earth masses. All four are more massive than Earth. GJ 667 C b, discovered in 2012, is the remaining planet and has no reported mass, only an orbital period.

The planets complete their orbits in periods ranging from 7.2 to 256 days. GJ 667 C b has the shortest year among the listed planets at 7.2 days, followed by GJ 667 C c at 28.1 days. GJ 667 C f orbits in 39 days and GJ 667 C e in 62.2 days, with GJ 667 C e holding the second-longest year. GJ 667 C g completes the group with the longest year at 256 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

8

Stellar refs

8

System refs

1

Distancestable

8 values โ€ข 1 distinct

Parallaxstable

8 values โ€ข 1 distinct

Temperaturedisputed

4 values โ€ข 4 distinct

Massstable

2 values โ€ข 1 distinct

Agestable

1 values โ€ข 1 distinct

Luminositydisputed

2 values โ€ข 2 distinct

Surface Gravitystable

1 values โ€ข 1 distinct

Metallicitystable

1 values โ€ข 1 distinct

Spectral Typedisputed

2 values โ€ข 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
โ€”โ€”โ€”โ€”โ€”โ€”7.24Nidever et al. 2002TICv8
โ€”โ€”โ€”โ€”โ€”โ€”7.24Wright et al. 2004TICv8
3775.4โ€”โ€”โ€”โ€”โ€”7.24Gaia DR2TICv8
33500.33โ€”2-1.86M1.5 V7.24Anglada-Escude et al. 2013TICv8
โ€”โ€”โ€”โ€”โ€”M1.57.24Hawley et al. 1996TICv8
โ€”โ€”โ€”โ€”โ€”โ€”7.24Anglada-Escudé et al. 2012TICv8
36000.33โ€”โ€”-1.85โ€”7.24Delfosse et al. 2013TICv8
3650โ€”โ€”โ€”โ€”โ€”7.24TICv8TICv8