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LP 596-30
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Star LP 596-30

Red dwarf LP 596-30 is located 98 light years away from the Sun. It is a single star, 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
98 light years
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LP 596-30

Red dwarf, High proper motion star

Location +

Ascension iconRight ascension: 4h 59m 28.689s
Declination iconDeclination: 2° 20' 0.634'' (equatorial region)
Parallax iconParallax: 33.372
Distance iconSun distance: 97.734 ly | 30.0 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: 10 % M Sun
| 136.2 M Jupiter
 (estimate)
+
Star mass
The mass of the star LP 596-30 is unknown. Based on its other characteristics, it is estimated to be about 10 % 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: 20 % R Sun
| 1.6 R Jupiter
(estimate)
+
Star size
Radius of the star LP 596-30 is not known. Its estimated value based on other similar stars is about 20 % 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: 3100 K
 (estimate)
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Star temperature
Surface temperature of LP 596-30 is estimated to be 3053 K, which is 54 % 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

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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LP 596-30 system structure

 LP 596-30

More about LP 596-30

       LP 596-30 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
Gaia DR3 3232115103881666944
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External sources
simbad icon
Simbad database (LP 596-30)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 3232115103881666944)
Archive from the Gaia mission

Frequently Asked Questions

How far is the LP 596-30 system from the Sun?

The LP 596-30 system is 98 light years or 30.0 parsecs from the Sun.

What galaxy is the LP 596-30 star in?

The LP 596-30 is in the Milky Way galaxy just like the Sun.

How many stars are in the LP 596-30 system?

The LP 596-30 is a single star, there are no other known stars in the system.

What type of star is the LP 596-30?

The star LP 596-30 is a Red dwarf star.

What temperature is the LP 596-30?

The primary in the LP 596-30 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

 HD 33636
 - 6.4 ly

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 - 6.5 ly

HD 290054
 - 7.9 ly

HD 31208
 - 8.9 ly

RX J0506.2+0439
 - 8.9 ly
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