Temperature
3466 K
3466 to 3545
M2.5 • 20.19 pc
Records
5
literature rows
Planets
4
system count
References
6
distinct source labels
Approximate color
from effective temperature
Canonical Summary
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
Mass
0.42 Msun
0.42 to 0.45
Radius
0.40 Rsun
0.40 to 0.45
Luminosity
-1.66 log(Lsun)
-1.66 to -1.58
Distance
20.19 pc
single adopted value
Spectral Type
M2.5
Consistent across records
Planets
4
Stable across source rows
Scale Comparison
Current adopted radius: 0.40 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
GJ 3293
0.40 R☉
System Layout
4 planets linked to this host
Radial Velocity
Discovery
2015
Period
30.60 days
Radius
—
Mass
23.54 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2015
Period
122.6 days
Radius
—
Mass
21.09 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2017
Period
48.13 days
Radius
—
Mass
7.60 M⊕
Eq. Temp
—
Radial Velocity
Discovery
2017
Period
13.25 days
Radius
—
Mass
3.28 M⊕
Eq. Temp
—
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
Evidence Summary
Rows
5
Stellar refs
5
System refs
1
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 3466 | 0.42 | 0.40 | — | -1.66 | M2.5 | 20.19 | Astudillo-Defru et al. 2015 | TICv8 |
| 3469 | 0.45 | 0.45 | — | -1.58 | — | 20.19 | TICv8 | TICv8 |
| 3545 | — | — | — | — | — | 20.19 | Gaia DR2 | TICv8 |
| — | — | — | — | — | M2.5 | 20.19 | Hawley et al. 1996 | TICv8 |
| 3466 | 0.42 | 0.40 | — | -1.66 | M2.5 | 20.19 | Astudillo-Defru et al. 2017 | TICv8 |