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Stellar HostProfile

GJ 3293

M2.5 • 20.19 pc

Records

5

literature rows

Planets

4

system count

References

6

distinct source labels

TIC: TIC 178872239

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: Astudillo-Defru et al. 2015 • System source: TICv8

Temperature

3466 K

3466 to 3545

4 values • 3 distinct

Mass

0.42 Msun

0.42 to 0.45

3 values • 2 distinct

Radius

0.40 Rsun

0.40 to 0.45

3 values • 2 distinct

Luminosity

-1.66 log(Lsun)

-1.66 to -1.58

3 values • 3 distinct

Distance

20.19 pc

single adopted value

5 values • 1 distinct

Spectral Type

M2.5

Consistent across records

M2.5 (3)

Planets

4

Stable across source rows

4

Scale Comparison

Radius against the Sun

Current adopted radius: 0.40 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

GJ 3293

0.40 R☉

System Layout

Known planets

4 planets linked to this host

GJ 3293 b

Radial Velocity

◌

Discovery

2015

Period

30.60 days

Radius

—

Mass

23.54 M⊕

Eq. Temp

—

GJ 3293 c

Radial Velocity

◌

Discovery

2015

Period

122.6 days

Radius

—

Mass

21.09 M⊕

Eq. Temp

—

GJ 3293 d

Radial Velocity

◌

Discovery

2017

Period

48.13 days

Radius

—

Mass

7.60 M⊕

Eq. Temp

—

GJ 3293 e

Radial Velocity

◌

Discovery

2017

Period

13.25 days

Radius

—

Mass

3.28 M⊕

Eq. Temp

—

GJ 3293 and Its Four Known Planets

GJ 3293 is a small, cool red dwarf of spectral type M2.5, located 65.9 light-years from Earth. Its reported mass is 0.42 solar masses, its radius is 0.404 solar radii, and its temperature is 3470 K - all smaller or cooler than the corresponding values for the Sun. Four planets have been found in orbit around this star.

GJ 3293 e has a minimum mass of 3.28 Earth masses and an orbital period of 13.3 days. GJ 3293 b has a minimum mass of 23.5 Earth masses and a period of 30.6 days. GJ 3293 d has a minimum mass of 7.6 Earth masses and a period of 48.1 days. GJ 3293 c has a minimum mass of 21.1 Earth masses and a period of 123 days.

All four planets have minimum masses larger than Earth's. Among them, GJ 3293 e has the smallest minimum mass, while GJ 3293 b has the largest, with GJ 3293 d and GJ 3293 c falling in between as the second-smallest and second-largest, respectively. GJ 3293 e also has the shortest reported year, and GJ 3293 c the longest, with GJ 3293 b and GJ 3293 d occupying the second-shortest and second-longest positions.

The planets were detected using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. GJ 3293 b and GJ 3293 c were announced in 2015, and GJ 3293 d and GJ 3293 e in 2017.

Provenance

Underlying measurements and references

Evidence Summary

Rows

5

Stellar refs

5

System refs

1

Distancestable

5 values • 1 distinct

Parallaxstable

5 values • 1 distinct

Temperaturedisputed

4 values • 3 distinct

Massdisputed

3 values • 2 distinct

Radiusdisputed

3 values • 2 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitystable

1 values • 1 distinct

Metallicitystable

2 values • 1 distinct

Spectral Typestable

3 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
34660.420.40—-1.66M2.520.19Astudillo-Defru et al. 2015TICv8
34690.450.45—-1.58—20.19TICv8TICv8
3545—————20.19Gaia DR2TICv8
—————M2.520.19Hawley et al. 1996TICv8
34660.420.40—-1.66M2.520.19Astudillo-Defru et al. 2017TICv8