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HD 80883
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Star HD 80883

Orange star HD 80883 is located 113 light years away from the Sun. It is a single star of spectral class K0V, that has 88 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
113 light years
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HD 80883

Orange star, High proper motion star
Spectral class: K0V

Location +

Ascension iconRight ascension: 9h 19m 43.966s
Declination iconDeclination: -59° 28' 41.135'' (southern hemisphere)
Parallax iconParallax: 28.929
Distance iconSun distance: 112.743 ly | 34.6 pc
Star position
The position of a star tells us where it appears in the sky, similar to how we use coordinates like latitude and longitude on Earth. In astronomy, the three main coordinates are right ascension, declination and distance. .. icon More about Star position in StellarGuide

Basic characteristic

icon weight
Mass: 88 % M Sun
| 922 M Jupiter
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Star mass
Mass of the star HD 80883 is 0.88 solar masses.

The mass of a star is the total amount of matter it contains. It is one of the most important properties of a star, as it determines almost everything about how the star lives, changes, and dies. In astronomy, star mass is usually measured in solar masses (M☉) — where 1 solar mass is equal to the mass of our Sun... icon More about Star mass in StellarGuide
radius icon
Size: 81 % R Sun
| 8.1 R Jupiter
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Star size
Radius of the star HD 80883 is 0.8148 solar radii.

The size of a star refers to its radius — the distance from its center to its surface. Star size is usually measured in solar radii (R☉), where 1 solar radius equals approximately 696,000 kilometers. Depending on their type and life stage, stars can be much smaller or larger than the Sun... icon More about Star size in StellarGuide
temperature icon
Temperature: 5177 K | 0.9 T Sun
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Star temperature
Surface temperature of HD 80883 is 5177 K, which is 90 % of the temperature on the surface of the Sun.

The temperature of a star refers to the temperature at its surface, also called the photosphere. It is measured in kelvins (K), the standard unit for temperature in astronomy. A star’s temperature tells us a lot about its physical properties and where it stands in its evolutionary stage... icon More about Star temperature in StellarGuide

Photometry

Magnitude iconApparent magnitude (V): 8.6
Magnitude iconAbsolute magnitude (V): 5.9
Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).
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
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HD 80883 system structure

 HD 80883
HD 80883 b 6.46 AU 1748.5 M⊕ 6383.8 days

More about HD 80883

Star HD 80883 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 80 % of the size of Sun and temperature on its surface is around 5177 K (4904 °C), which is about 90 % of Sun's temperature.
       HD 80883 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope.
Other designations of this star
Gaia DR3 5300239064919282816
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External sources
simbad icon
Simbad database (HD 80883)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 5300239064919282816)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 80883 system from the Sun?

The HD 80883 system is 113 light years or 34.6 parsecs from the Sun.

What galaxy is the HD 80883 star in?

The HD 80883 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 80883 system?

The HD 80883 is a single star, there are no other known stars in the system.

What type of star is the HD 80883?

The star HD 80883 is a Orange star star.

What temperature is star HD 80883?

The star HD 80883 has an effective temperature of 5177 K. Find out more about the temperature of stars in Stellar guide

stellar brief logoStellar Brief

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23. 10. 2026
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A planet’s escaping helium, a star’s hidden infrared rhythms, and a possible distant world in the WISPIT 2 system reveal how much we can learn by watching light across the spectrum. New observations also trace the changing radio and X-ray activity of young V1298 Tauri, while detailed models map cloudy and clear regions across the hot Jupiter WASP-43 b.
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