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Stellar Catalog
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TOI-1201
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Star TOI-1201

Binary star TOI-1201 is located 124 light years away from the Sun. It consists of 2 red dwarf stars. There is at least one exoplanet in this system.
Sun distance
124 light years

TOI-1201 A

Red dwarf (spectral class M2.0)

Location

Ascension iconRight ascension: 2h 48m 59.282s
Declination iconDeclination: -14° 32' 14.943'' (equatorial region)
Parallax iconParallax: 26.365
Distance iconSun distance: 123.707 ly | 37.9 pc

Basic characteristic

icon weight
Mass: 51.2 % M Sun | 536 M Jupiter
radius icon
Size: 48 % R Sun | 4.8 R Jupiter
temperature iconTemperature: 3476 K | 0.6 T Sun
time iconAge: 0.7 billions years | 0.15 Sun

1 exoplanet

TOI-1201 A b 0.03 AU 6.3 M 2.4 R 2.5 days

Photometry

Magnitude iconApparent magnitude (V): 12.3
Magnitude iconAbsolute magnitude (V): 9.4
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-1201 B

Red dwarf (spectral class M2.5V)

Basic characteristic

icon weight
Mass: 40 % M Sun | 429.5 M Jupiter (estimate)
radius icon
Size: 40 % R Sun | 4.2 R Jupiter (estimate)
(No known exoplanets yet)
More about TOI-1201
      TOI-1201 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
UCAC3 151-6986, DENIS J024859.2-143215, 2MASS J02485926-1432152, TIC 29960110, TIC-29960110, PMJ02489−1432W
News from this star system
Article image:

Rare warm mini-neptune discovered 123 light years away

Around one of the stars in a binary system TOI-1201 was discovered new exoplanet. It orbits its star ten times closer than Mercury orbits the Sun. It's about 2.5 times bigger than Earth and more than 6 times heavier. From its calculated density scientists expect it to be a member of sub-neptune class of exoplanets.

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