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Star AR Scorpii

Binary star AR Scorpii is located 382 light years away from the Sun. It consists of a white dwarf and a red dwarf. For now, there are no known exoplanets in this star system.
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Sun distance
382 light years

AR Scorpii A

Location +

Ascension iconRight ascension: 16h 21m 47.302s
Declination iconDeclination: -22° 53' 11.210'' (southern hemisphere)
Parallax iconParallax: 8.544
Distance iconSun distance: 381.751 ly | 117.0 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: 100 % M Sun
| 1048 M Jupiter
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Star mass
Mass of the star AR Scorpii A is 1 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
temperature icon
Temperature: 4283 K | 0.74 T Sun
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Star temperature
Surface temperature of AR Scorpii A is 4283 K, which is 74 % 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 iconAbsolute magnitude (V): -5.3
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

AR Scorpii B

Basic characteristic

icon weight
Mass: 31 % M Sun
| 325 M Jupiter
+
Star mass
Mass of the star AR Scorpii B is 1 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

Photometry

Magnitude iconAbsolute magnitude (V): -5.3
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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AR Scorpii system structure

AR Scorpii A
AR Scorpii B

More about AR Scorpii

       AR Scorpii can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope. 
Other designations of this star
Gaia DR3 6050296829033196032
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External sources
icon study
VLBI astrometry on the white dwarf pulsar AR Scorpii
Scientific study, Accepted: 31. 01. 2023

Frequently Asked Questions

How far is the AR Scorpii system from the Sun?

The AR Scorpii system is 382 light years or 117.0 parsecs from the Sun.

What galaxy is the AR Scorpii star in?

The AR Scorpii is in the Milky Way galaxy just like the Sun.

How many stars are in the AR Scorpii system?

The AR Scorpii system contains 2 stars.

What type of star is the AR Scorpii?

The primary in the AR Scorpii system is a White dwarf star.

What temperature is star AR Scorpii?

The primary in the AR Scorpii system has a temperature of 4283 K. Find out more about the temperature of stars in Stellar guide
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exoplanet iconAbout Stellar Catalog

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icon Data in Stellar Catalog come from trusted scientific sources. Primary source is Gaia space telescope mapping the stars in Milky Way. Other sources include research papers, Simbad catalog and Exoplanet.eu database.
Estimated values
icon Objects listed in the Stellar Catalog often have values that are estimates. These estimates are determined using their known characteristics, such as spectral type, brightness across different wavelengths, distance from a star, and other factors.
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