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Gliese 450
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Star Gliese 450

Red dwarf Gliese 450 is located 29 light years away from the Sun. It is a single star of spectral class M1.5 V, that has 49 % of solar mass. For now, there are no known exoplanets in this star system.
Sun distance
29 light years

Gliese 450

Red dwarf, Low-mass star
Spectral class: M1.5 V

Location

Ascension iconRight ascension: 11h 51m 6.981s
Declination iconDeclination: 35° 16' 23.303'' (northern hemisphere)
Parallax iconParallax: 114.085
Distance iconSun distance: 28.589 ly | 8.8 pc

Basic characteristic

icon weight
Mass: 49 % M Sun | 513 M Jupiter
radius icon
Size: 50 % R Sun | 5.3 R Jupiter (estimate)
temperature iconTemperature: 3645 K | 0.63 T Sun
luminosity iconLuminosity: 0.03 L Sun

Photometry

Magnitude iconApparent magnitude (V): 9.8
Magnitude iconAbsolute magnitude (V): 10.1
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).

Gliese 450 system structure

Gliese 450
More about Gliese 450
Nearby star Gliese 450 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 50 % of the size of Sun and temperature on its surface is around 3645 K (3372 °C), which is about 63 % of Sun's temperature.
       Gliese 450 can be found in northern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is easily observable from Northern America, Europe and Asia. 
Other designations of this star
HIP 57802, G 148-13, MCC 135, NLTT 28756, HIC 57802, HIP 57802, NGP 36 11, 2MASS J11510737+3516188, BD+36 2119, MCC 135, Gaia EDR3 4031586157514097024
External sources
simbad icon
Simbad database (MCC 135)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 4031586157514097024)
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.
Closest stars

Argelanders Star
0.66 M☉ 1.8 ly

61 Ursae Majoris
0.85 M☉ 2.9 ly

Xi Ursae Majoris Aa
0.97 M☉ 3.9 ly

Beta Canum Venaticorum
1 M☉ 5.1 ly

Gliese 436
0.41 M☉ 5.7 ly
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