Star HD 114082

Yellow-White star HD 114082 is located 310 light years away from the Sun. It is a single star of spectral class F3V C, that has 147 % of solar mass. There is at least one exoplanet in this system.

HD 114082 is a member of Lower Centaurus Crux association.

HD 114082

Yellow-White star (spectral class F3V C)

Location

Right ascension: 13h 9m 16.11s

Declination: -60° 18' 30.375'' (southern hemisphere)

Parallax: 10.52

Sun distance: 310.032 ly | 95.1 pc

Basic characteristic

Mass: 1.47 M Sun

Size: 1.49 R Sun

Temperature: 6651 K | 1.15 T Sun

Age: 0.015 billions years | 0 Sun

1 exoplanet

HD 114082 b

0.51 AU

2543.3 M⊕

11.2 R⊕

109.8 days

Photometry

Apparent magnitude (V): 8.2

Absolute magnitude (V): 3.3

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 HD 114082

      Star HD 114082 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope.  HD 114082 is  about 49 % bigger than the Sun and temperature on its surface is around 6651 K (6378 °C), which is about 115 % of Suns temperature.

Other designations of this star
Gaia DR3 6055854551117476480, HIP 64184, 2MASS J13091620-6018300, TIC 441546821, TYC 8990-1653-1, SAO 252171

External sources

Radial Velocity Survey for Planets around Young stars (RVSPY) A transiting warm super-Jovian planet around HD 114082, a young star with a debris disk

Scientific study,

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