do not follow here
Stellar Catalog
more icon
Nearby stars catalogue
more icon
TOI 4559
more icon

Star TOI 4559

Red dwarf TOI 4559 is located 103 light years away from the Sun. It is a single star, that has 39 % of solar mass. There is at least one exoplanet in this system.
Sun distance
103 light years

TOI 4559

Red dwarf

Location

Ascension iconRight ascension: 14h 4m 3.251s
Declination iconDeclination: -30° 0' 50.974'' (southern hemisphere)
Parallax iconParallax: 31.639
Distance iconSun distance: 103.088 ly | 31.6 pc

Basic characteristic

icon weight
Mass: 39.2 % M Sun | 411 M Jupiter
radius icon
Size: 37 % R Sun | 3.7 R Jupiter
temperature iconTemperature: 3558 K | 0.62 T Sun
time iconAge: 7 billions years | 1.52 Sun
luminosity iconLuminosity: 0.0203 L Sun

1 exoplanet

TOI 4559 b 0.04 AU 2.7 M 1.4 R 4 days

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).
More about TOI 4559
Star TOI 4559 is approximately 40 % of the size of Sun and temperature on its surface is around 3558 K (3285 °C), which is about 62 % of Sun's temperature.
      TOI 4559 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 271169413, LP 912-46, Gaia DR3 6173120554255287808
External sources
simbad icon
Simbad database (LP 912-46)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 6173120554255287808)
Archive from the Gaia mission
tess icon
TESS database (TOI 4559.01)
Archive from the TESS 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.
Get your next news from nearby stars
This is a new project, and partly still in development. There will be soon more information and functions. We would love your support on social media.
Visit profile