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DG Phoenix
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Star DG Phoenix

Red dwarf DG Phoenix is located 52 light years away from the Sun. It is a single star of spectral class M8.5e, that has typically about 25 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
52 light years
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DG Phoenix

Red dwarf, Low-mass star
Spectral class: M8.5e

Location +

Ascension iconRight ascension: 1h 9m 1.894s
Declination iconDeclination: -51° 0' 48.161'' (southern hemisphere)
Parallax iconParallax: 62.789
Distance iconSun distance: 51.945 ly | 15.9 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: 8 % M Sun
| 83.8 M Jupiter
 (estimate)
+
Star mass
The estimated mass of the star DG Phoenix is about 8 % of the Sun's mass, or approximately 83.8 Jupiter 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: 10 % R Sun
| 1.1 R Jupiter
(estimate)
+
Star size
Radius of the star DG Phoenix is not known. Its estimated value based on other similar stars is about 10 % 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: 2400 K
 (estimate)
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Star temperature
Surface temperature of DG Phoenix is estimated to be 2400 K, which is 42 % 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): 18.8
Magnitude iconAbsolute magnitude (V): 17.8
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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DG Phoenix system structure

 DG Phoenix

More about DG Phoenix

       DG Phoenix 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
V* DG Phe, Gaia EDR3 4928644747924606848
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External sources
simbad icon
Simbad database (V* DG Phe)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia EDR3 4928644747924606848)
Archive from the Gaia mission

Frequently Asked Questions

How far is the DG Phoenix system from the Sun?

The DG Phoenix system is 52 light years or 15.9 parsecs from the Sun.

What galaxy is the DG Phoenix star in?

The DG Phoenix is in the Milky Way galaxy just like the Sun.

How many stars are in the DG Phoenix system?

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

What type of star is the DG Phoenix?

The star DG Phoenix is a Red dwarf star.

What temperature is the DG Phoenix?

The primary in the DG Phoenix system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Red dwarf
Red dwarfs are small, cool stars with surface temperatures of about 2,000–3,800 K, much cooler than the Sun. They usually have 8–50% of the Sun’s mass and shine very faintly, sometimes at just a tiny fraction of the Sun’s brightness. Classified mainly as spectral type M, they are the most common stars in the Milky Way, making up roughly 70–75% of its stellar population.

They fuse hydrogen slowly through the proton–proton chain and are fully convective, which allows them to use their fuel very efficiently. As a result, red dwarfs can live for tens of billions to trillions of years—far longer than the Sun. Many exoplanets orbit red dwarfs, including some in close habitable zones, though strong stellar activity can affect planetary environments.
Closest stars

 Gliese 3082
 0.47 M☉ 3.7 ly

HD 4391
 1.2 M☉ 5.4 ly

UCAC3 85-1637
 - 5.4 ly

Nu Phoenicis
 1.2 M☉ 5.4 ly

Gaia DR2 4975284381905517824
 - 5.7 ly
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