do not follow here
Stellar Catalog
more icon
Nearby stars catalogue
more icon
WISE J071322.55-291751.9
more icon

Star WISE J071322.55-291751.9

Sub-brown dwarf WISE J071322.55-291751.9 is located 30 light years away from the Sun. It is a single star of spectral class Y0 , that has typically about 1.5 % of solar mass. For now, there are no known exoplanets in this star system.
Sun distance
30 light years

WISE J071322.55-291751.9

Spectral class: Y0

Location

Ascension iconRight ascension: 7h 13m 22.56s
Declination iconDeclination: -29° 17' 51.961'' (southern hemisphere)
Parallax iconParallax: 108.7
Distance iconSun distance: 30.005 ly | 9.2 pc

Basic characteristic

icon weight
Mass: 2 % M Sun | 21 M Jupiter (estimate)
radius icon
Size: 10 % R Sun | 0.9 R Jupiter (estimate)

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).

WISE J071322.55-291751.9 system structure

WISE J071322.55-291751.9
More about WISE J071322.55-291751.9
       WISE J071322.55-291751.9 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope. 
External sources
simbad icon
Simbad database (WISE J071322.55-291751.9)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
Class of stars Sub-brown dwarf
Brown dwarfs are not really stars, because there is no thermonuclear fusion in their core. These objects are smaller and cooler than stars, but too massive to be considered planets. Brown dwarfs of spectral class Y are the coolest and only a few of them have been discovered so far.
Closest stars

2MASS 0729-3954
0.04 M☉ 6.8 ly

Gliese 3459
- 6.9 ly

Gliese 283
0.62 M☉ 7 ly

AP Columbae
0.25 M☉ 8 ly

SCR J0740-4257
- 8.2 ly
3D map of stellar neighborhood
List of all nearby stars
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.