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V484 Tauri
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Star V484 Tauri

Red dwarf V484 Tauri is located 52 light years away from the Sun. It is a single flare star of spectral class M3.5, 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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V484 Tauri

Red dwarf, flare star
Spectral class: M3.5

Location +

Ascension iconRight ascension: 4h 30m 23.966s
Declination iconDeclination: 17° 29' 59.056'' (equatorial region)
Parallax iconParallax: 63.000
Distance iconSun distance: 51.771 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: 30 % M Sun
| 272.4 M Jupiter
 (estimate)
+
Star mass
The mass of the star V484 Tauri is unknown. Based on its other characteristics, it is estimated to be about 30 % 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: 30 % R Sun
| 2.9 R Jupiter
(estimate)
+
Star size
Radius of the star V484 Tauri is not known. Its estimated value based on other similar stars is about 30 % 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: 3300 K
 (estimate)
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Star temperature
Surface temperature of V484 Tauri is estimated to be 3300 K, which is 57 % 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): 14.5
Magnitude iconAbsolute magnitude (V): 13.5
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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V484 Tauri system structure

 V484 Tauri

More about V484 Tauri

       V484 Tauri can be found in northern 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* V484 Tau, GJ 3294, Gliese 3294
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External sources
simbad icon
Simbad database (V* V484 Tau)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)

Frequently Asked Questions

How far is the V484 Tauri system from the Sun?

The V484 Tauri system is 52 light years or 15.9 parsecs from the Sun.

What galaxy is the V484 Tauri star in?

The V484 Tauri is in the Milky Way galaxy just like the Sun.

How many stars are in the V484 Tauri system?

The V484 Tauri is a single star, there are no other known stars in the system.

What type of star is the V484 Tauri?

The star V484 Tauri is a Red dwarf star.

What temperature is the V484 Tauri?

The primary in the V484 Tauri 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

 LP 415-217
 - 4 ly

EGGR 169
 - 4.9 ly

39 Tauri
 1.1 M☉ 7.5 ly

PM J04429+2128
 - 7.7 ly

G 8-41
 - 7.9 ly
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