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Star HR 5183

Yellow star HR 5183 is located 103 light years away from the Sun. It is a single star of spectral class G0V C, that has 107 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
103 light years

HR 5183

Yellow star, High proper motion star
Spectral class: G0V C

Location +

Ascension iconRight ascension: 13h 46m 57.123s
Declination iconDeclination: 6° 21' 1.346'' (equatorial region)
Parallax iconParallax: 31.757
Distance iconSun distance: 102.704 ly | 31.5 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: 107 % M Sun
| 1121 M Jupiter
+
Star mass
Mass of the star HR 5183 is 1.07 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
radius icon
Size: 120 % R Sun
| 11.8 R Jupiter
(estimate)
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Star size
Radius of the star HR 5183 is not known. Its estimated value based on other similar stars is about 120 % 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: 6000 K
 (estimate)
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Star temperature
Surface temperature of HR 5183 is estimated to be 5966 K, which is 104 % 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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HR 5183 system structure

HR 5183
HR 5183 b 18 AU 1026.8 M⊕ 27400 days

More about HR 5183

Star HR 5183 is a main sequence star that fuses hydrogen atoms into helium.
       HR 5183 can be found in northern celestial hemisphere. 
Other designations of this star
HD 120066, LHS 2798, AG+06 1648, BD+07 2690, GC 18625, HIC 67246, HIP 67246, IRAS 13444+0635, LFT 1036, LTT 14020, 2MASS J13465711+0621013, SAO 120108, ROT 1995, TD1 17051, TIC 379117362, TYC 314-1369-1, WEB 11833, WISEA J134656.76+062059.8
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External sources
simbad icon
Simbad database (HD 120066)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)

Frequently Asked Questions

How far is the HR 5183 system from the Sun?

The HR 5183 system is 103 light years or 31.5 parsecs from the Sun.

What galaxy is the HR 5183 star in?

The HR 5183 is in the Milky Way galaxy just like the Sun.

How many stars are in the HR 5183 system?

The HR 5183 is a single star, there are no other known stars in the system.

What type of star is the HR 5183?

The star HR 5183 is a Yellow star star.

What temperature is the HR 5183?

The primary in the HR 5183 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Yellow star
Sun-like stars belong mainly to spectral type G and are commonly called yellow dwarfs. They have surface temperatures of roughly 5,300–6,000 K (about 5,000–5,700 °C), giving them a slightly yellow-white appearance. With masses typically between about 0.8 and 1.1 times that of the Sun, they sit between hotter, more massive white stars and cooler orange and red stars on the main sequence. The Sun itself is a standard G2V star and serves as the benchmark for understanding the structure and behavior of this stellar class.

These stars generate energy by fusing hydrogen into helium in their cores through the proton–proton chain. Their total lifetimes on the main sequence are around 10 billion years, during which their brightness slowly increases. After exhausting hydrogen in their cores, Sun-like stars expand into red giants, shed their outer layers to form planetary nebulae, and eventually leave behind dense white dwarfs. Many known exoplanet systems orbit Sun-like stars, making them key targets in the search for potentially habitable worlds.
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