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WASP 189
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Star WASP 189

Subgiant WASP 189 is located 323 light years away from the Sun. It is a single star of spectral class A6IV-V, that has 203 % of solar mass. There is at least one exoplanet in this system.
Sun distance
323 light years

WASP 189

Spectral class: A6IV-V

Location

Ascension iconRight ascension: 15h 2m 44.821s
Declination iconDeclination: -3° 1' 53.367'' (equatorial region)
Parallax iconParallax: 10.1
Distance iconSun distance: 322.936 ly | 99 pc

Basic characteristic

icon weight
Mass: 203 % M Sun | 2127 M Jupiter
radius icon
Size: 236 % R Sun | 23.5 R Jupiter

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).

WASP 189 system structure

WASP 189
WASP 189 b 0.05 AU 632.6 M 17.9 R 2.7 days
More about WASP 189
       WASP 189 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is also observable from Northern America, Europe and Asia. 
Other designations of this star
Gaia DR3 6339097679918871168
External sources
gaia icon
Gaia database (Gaia DR3 6339097679918871168)
Archive from the Gaia mission
Class of stars Subgiant
A subgiant is a term used to describe a luminous star that is typically running out of hydrogen for nuclear fusion and is thus departing from the main sequence. These stars are classified as Yerkes luminosity class IV.
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