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Stellar Catalog
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TOI 2384
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Star TOI 2384

Red dwarf TOI 2384 is located 613 light years away from the Sun. It is a single star, that has 64 % of solar mass. There is at least one exoplanet in this system.
Sun distance
613 light years

TOI 2384

Location

Ascension iconRight ascension: 2h 24m 37.482s
Declination iconDeclination: -65° 0' 0.731'' (southern hemisphere)
Parallax iconParallax: 5.322
Distance iconSun distance: 612.858 ly | 187.9 pc

Basic characteristic

icon weight
Mass: 63.5 % M Sun | 665 M Jupiter
radius icon
Size: 61 % R Sun | 6.1 R Jupiter
temperature iconTemperature: 3943 K | 0.68 T Sun
time iconAge: 9.4 billions years | 2.04 Sun

Photometry

Magnitude iconApparent magnitude (V): 15.4
Magnitude iconAbsolute magnitude (V): 9
5
10
15
20
25
30
35
K
2.1
H
1.6
J
1.2
Grp
0.8
I
0.8
G
0.6
V
0.5
Gbp
0.5
B
0.4
U
0.3
Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).

TOI 2384 system structure

TOI 2384
TOI 2384 b 0.03 AU 625 M 11.5 R 2.1 days
More about TOI 2384
Star TOI 2384 is approximately 60 % of the size of Sun and temperature on its surface is around 3943 K (3670 °C), which is about 68 % of Sun's temperature.
       TOI 2384 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope. 
Other designations of this star
TIC 382602147, 2MASS J02243746-6459599, Gaia DR3 4699702272124241152
External sources
gaia icon
Gaia database (Gaia DR3 4699702272124241152)
Archive from the Gaia mission
Class of stars Red dwarf
Red dwarfs are small reddish stars, that are by far the most common type of star in solar neighborhood. Their mass is usually between 10 and 50 % of solar mass.
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