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Star HR 858

Yellow-White star HR 858 is located 104 light years away from the Sun. It is a single star of spectral class F6V C, that has 115 % of solar mass. There are multiple known exoplanets in this system.
Sun distance
104 light years

HR 858

Yellow-White star (spectral class F6V C)

Location

Ascension iconRight ascension: 2h 51m 56.255s
Declination iconDeclination: -30° 48' 52.259'' (southern hemisphere)
Parallax iconParallax: 31.257
Distance iconSun distance: 104.348 ly | 32 pc

Basic characteristic

icon weight
Mass: 114.5 % M Sun | 1199 M Jupiter
radius icon
Size: 131 % R Sun | 13 R Jupiter
temperature iconTemperature: 6201 K | 1.07 T Sun

3 exoplanets

HR 858 b 0.05 AU 2.1 R 3.6 days
HR 858 c 0.07 AU 1.9 R 6 days
HR 858 d 0.1 AU 2.2 R 11.2 days

Photometry

Magnitude iconApparent magnitude (V): 6.4
Magnitude iconAbsolute magnitude (V): 3.9
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).
More about HR 858
Star HR 858 is a main sequence star that fuses hydrogen atoms into helium. It is is approximately 31 % bigger than the Sun and temperature on its surface is around 6201 K (5928 °C), which is about 107 % of Sun's temperature.
      HR 858 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
HD 17926, CD-31 1148, GC 3443, HIC 13363, HIP 13363, 2MASS J02515623-3048524, TIC 178155732, TOI-396, TYC 7012-833-1
External sources
simbad icon
Simbad database (HD 17926)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
tess icon
TESS database (TOI 396.01)
Archive from the TESS mission
News from this star system
Article image:

Stars flying by each other might pose a great opportunity in search for advanced civilisations

New list of pairs of gravitationaly unbound stars in our neighborhood might present a new set of interesting targets for those who look for advanced civilisations. When two stars come close to each other, the advanced enough civilisation might take an advantage and migrate from one system to the other. In new study a list is presented of best candidate stars.

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