do not follow here
Stellar Catalog
more icon
Nearby stars catalogue
more icon
EGGR 148
more icon

Star EGGR 148

White dwarf EGGR 148 is located 36 light years away from the Sun. It is a single star of spectral class DQ6, that has typically about 60 % of solar mass. For now, there are no known exoplanets in this star system.
Sun distance
36 light years

EGGR 148

Spectral class: DQ6

Location

Ascension iconRight ascension: 21h 42m 40.756s
Declination iconDeclination: 20° 59' 47.73'' (northern hemisphere)
Parallax iconParallax: 90.545
Distance iconSun distance: 36.021 ly | 11 pc

Basic characteristic

icon weight
Mass: 60 % M Sun | 586.6 M Jupiter (estimate)
temperature iconTemperature: 8220 K | 1.42 T 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).

EGGR 148 system structure

EGGR 148
More about EGGR 148
Temperature on its surface is around 8220 K (7947 °C), which is about 142 % of Sun's temperature.
       EGGR 148 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
GJ 836.5, Gliese 836.5, G 145-63, G 126-27, LFT 1655, LHS 3703, L 1363-3, LP 458-64, LTT 16348, NLTT 51906, 2MASS J21424099+2059582, SDSS J214240.92+205954.9, TIC 354568302, WD 2140+207, WISEA J214240.83+205951.2, Gaia EDR3 1792830060723673472
External sources
simbad icon
Simbad database (EGGR 148)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 1792830060723673472)
Archive from the Gaia mission
Closest stars

Ross 271
0.5 M☉ 5.2 ly

Iota Pegasi
1.3 M☉ 5.4 ly

Gaia EDR3 1800808220172866048
- 6.9 ly

V374 Pegasi
0 M☉ 8 ly

BD+27 4120
- 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.