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Stellar Catalog
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Nearby stars catalogue
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HD 19467
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Star HD 19467

Binary star HD 19467 is located 104 light years away from the Sun. It consists of a yellow star and a brown dwarf. For now, there are no known exoplanets in this star system.
Sun distance
104 light years

HD 19467 A

Yellow star, High proper motion star
Spectral class: G3V

Location

Ascension iconRight ascension: 3h 7m 18.568s
Declination iconDeclination: -13° 45' 46.588'' (equatorial region)
Parallax iconParallax: 31.219
Distance iconSun distance: 104.473 ly | 32 pc

Basic characteristic

icon weight
Mass: 96 % M Sun | 1006 M Jupiter
radius icon
Size: 120 % R Sun | 11.9 R Jupiter
temperature iconTemperature: 5747 K | 0.99 T Sun
time iconAge: 9.4 billions years | 2.04 Sun
luminosity iconLuminosity: 1.42 L Sun

Photometry

Magnitude iconApparent magnitude (V): 7
Magnitude iconAbsolute magnitude (V): 4.5
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).

HD 19467 B

Brown dwarf, , High proper motion star
Spectral class: T5+

Basic characteristic

icon weight
Mass: 6.7 % M Sun | 70 M Jupiter
radius icon
Size: 6.4 % R Sun | 0.6 R Jupiter
temperature iconTemperature: 1000 K | 0.17 T Sun

HD 19467 system structure

HD 19467 A
HD 19467 B
More about HD 19467
       HD 19467 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. 
External sources
icon study
First Observations of the Brown Dwarf HD 19467 B with JWST
Scientific study, Accepted: 26. 01. 2023
News from this star system
Article image:

Astronomers used JWST and TESS telescopes to study nearby brown dwarf HD 19467 B

Brown dwarfs are objects between planets and stars. Astronomers divide them into 3 categories according to their temperature - L, T, Y. Their relatively low temperatures and brightness allow them to stay hidden for most part. Only the most powerful infrared telescopes are able to see them and that is where James Webb Space Telescope comes in.

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