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Stellar Catalog
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Nearby stars catalogue
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TOI-2337
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Star TOI-2337

Red giant TOI-2337 is located 1762 light years away from the Sun. It is a single star, that has 133 % of solar mass. There is at least one exoplanet in this system.
Sun distance
1762 light years

TOI-2337

Location

Ascension iconRight ascension: 19h 22m 29s
Declination iconDeclination: 60° 51' 14'' (northern hemisphere)
Parallax iconParallax: 1.851
Distance iconSun distance: 1762.017 ly | 540.2 pc

Basic characteristic

icon weight
Mass: 132.5 % M Sun | 1388 M Jupiter
radius icon
Size: 322 % R Sun | 32 R Jupiter
temperature iconTemperature: 4780 K | 0.83 T Sun
time iconAge: 4.9 billions years | 1.07 Sun

Photometry

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-2337 system structure

TOI-2337
TOI-2337 b 2.99 AU 317.9 M 10.1 R 3 days
More about TOI-2337
Star TOI-2337 is is approximately 3 times bigger than the Sun and temperature on its surface is around 4780 K (4507 °C), which is about 83 % of Sun's temperature.
       TOI-2337 can be found in northern 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 230001847, TYC 4217-01423-1, 2MASS J19222878+6051140, GAIA DR2 2239684947894267392
External sources
tess icon
TESS database (TOI 2337.01)
Archive from the TESS mission
Class of stars Red giant
part of star image
part of star image
The red giant is one of the final stages in the evolution of main sequence stars. These stars have already fused most of their hydrogen into helium, and their outer layers are gradually expanding. A white dwarf will form from the dense core of the original star, and the discarded upper layers will become a planetary nebula.  

In 5 billion years the Sun will also enter the red giant phase. Its size will then inflate to the orbit of Earth or Mars.
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