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V* CL Oct
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Star V* CL Oct

White dwarf V* CL Oct is located 96 light years away from the Sun. It is a single star of spectral class DAP, that has typically about 60 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
96 light years
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V* CL Oct

White dwarf
Spectral class: DAP

Location +

Ascension iconRight ascension: 3h 17m 14.837s
Declination iconDeclination: -85° 32' 25.750'' (southern hemisphere)
Parallax iconParallax: 34.035
Distance iconSun distance: 95.829 ly | 29.4 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: 70 % M Sun
| 691.4 M Jupiter
 (estimate)
+
Star mass
The mass of the star V* CL Oct is unknown. Based on its other characteristics, it is estimated to be about 70 % of the Sun's mass.

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: 0 % R Sun
| 0.1 R Jupiter
(estimate)
+
Star size
Radius of the star V* CL Oct is not known. Its estimated value based on other similar stars is about 0 % 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: 11100 K
 (estimate)
+
Star temperature
Surface temperature of V* CL Oct is estimated to be 11117 K, which is 192 % 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): 13.7
Magnitude iconAbsolute magnitude (V): 11.3
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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V* CL Oct system structure

 V* CL Oct

More about V* CL Oct

       V* CL Oct 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
2MASS J03171580-8532254, WD 0316-849, Gaia DR3 4613612951211823104
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External sources
simbad icon
Simbad database (V* CL Oct)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 4613612951211823104)
Archive from the Gaia mission

Frequently Asked Questions

How far is the V* CL Oct system from the Sun?

The V* CL Oct system is 96 light years or 29.4 parsecs from the Sun.

What galaxy is the V* CL Oct star in?

The V* CL Oct is in the Milky Way galaxy just like the Sun.

How many stars are in the V* CL Oct system?

The V* CL Oct is a single star, there are no other known stars in the system.

What type of star is the V* CL Oct?

The star V* CL Oct is a White dwarf star.

What temperature is the V* CL Oct?

The primary in the V* CL Oct system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Possible companions

 LB 9802
 - 0 ly
Closest stars

 Gaia DR3 4616346096599046912
 - 4.7 ly

UCAC4 027-000023
 - 7.1 ly

L 12-6
 - 8.5 ly

HD 10800 Aa
 1.1 M☉ 9.6 ly

SCR J0725-8530
 - 11.3 ly
3D map of stellar neighborhood
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stellar brief logoStellar Brief

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24. 10. 2026
stellar brief logo
A planet’s helium atmosphere streams ahead of its orbit, while infrared observations reveal the hidden rhythms of its star. New work also shows how neutron-star tilt can reshape X-ray light, traces the past of massive blue supergiants, and maps cloudy and clear zones on the hot Jupiter WASP-43 b.
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exoplanet iconAbout Stellar Catalog

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Working with real data
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.
Fresh and validated
icon Stellar Catalog is continuously updated with new information from research papers. Stellar and planetary data are validated by automatic processes as well as humans.

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