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Star HD 85503

Red giant HD 85503 is located 125 light years away from the Sun. It is a single star of spectral class K2III, that has 130 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
125 light years

HD 85503

Spectral class: K2III

Location +

Ascension iconRight ascension: 9h 52m 45.568s
Declination iconDeclination: 26° 0' 24.142'' (northern hemisphere)
Parallax iconParallax: 26.097
Distance iconSun distance: 124.978 ly | 38.3 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: 130 % M Sun
| 1362 M Jupiter
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Star mass
Mass of the star HD 85503 is 1.30 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: 1620 % R Sun
| 161 R Jupiter
(estimate)
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Star size
Radius of the star HD 85503 is not known. Its estimated value based on other similar stars is about 1620 % 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 iconTemperature: 4500 K
 (estimate)
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Star temperature
Surface temperature of HD 85503 is estimated to be 4470 K, which is 78 % 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
luminosity icon
Luminosity: 1.52 L Sun
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Star luminosity
Luminosity is the total amount of energy a star gives off every second. Think of it as the star’s true brightness — not just how bright it looks from Earth. This is important because some stars may appear dim simply because they are far away, not because they’re actually faint... icon More about Star luminosity in StellarGuide

Photometry

Magnitude iconAbsolute magnitude (V): -2.9
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 85503 system structure

HD 85503

More about HD 85503

       HD 85503 can be found in northern celestial hemisphere, and it is possible to see it with naked eye. The star is easily observable from Northern America, Europe and Asia. 
Other designations of this star
Gaia DR3 643819484617141504
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External sources
icon study
Chemical abundances of 20 barium stars from the OHP spectra
Scientific study, Accepted: 16. 10. 2024
gaia icon
Gaia database (Gaia DR3 643819484617141504)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 85503 system from the Sun?

The HD 85503 system is 125 light years or 38.3 parsecs from the Sun.

What galaxy is the HD 85503 star in?

The HD 85503 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 85503 system?

The HD 85503 is a single star, there are no other known stars in the system.

What type of star is the HD 85503?

The star HD 85503 is a Red giant star.

What temperature is the HD 85503?

The primary in the HD 85503 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Red giant
White dwarfs are the hot, extremely dense stellar remnants left behind by stars that originally had masses between about 0.5 and 8 times the mass of the Sun during their main sequence lifetimes. After exhausting their nuclear fuel, these stars shed their outer layers and leave behind a compact core. Although white dwarfs contain between roughly 0.2 and 1.44 solar masses, this mass is packed into a volume comparable to that of an Earth-sized planet, making them some of the densest objects in the Universe.
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Estimated values
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