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HD 37792
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Star HD 37792

Yellow-White star HD 37792 is located 244 light years away from the Sun. It is a single star, that has 107 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
244 light years
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HD 37792

Yellow-White star

Location +

Ascension iconRight ascension: 5h 40m 17.284s
Declination iconDeclination: -19° 13' 40.853'' (equatorial region)
Parallax iconParallax: 13.356
Distance iconSun distance: 244.203 ly | 74.9 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: 107 % M Sun
| 1121 M Jupiter
+
Star mass
Mass of the star HD 37792 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
| 12.3 R Jupiter
(estimate)
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Star size
Radius of the star HD 37792 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 icon
Temperature: 6500 K | 1.12 T Sun
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Star temperature
Surface temperature of HD 37792 is 6500 K, which is 112 % 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): 7.7
Magnitude iconAbsolute magnitude (V): 3.3
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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HD 37792 system structure

 HD 37792

More about HD 37792

Star HD 37792 is is approximately 24 % bigger than the Sun and temperature on its surface is around 6500 K (6227 °C), which is about 112 % of Sun's temperature.
       HD 37792 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is also observable from Northern America, Europe and Asia.
Other designations of this star
Gaia DR3 2967141533259094400
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External sources
icon study
gaia icon
Gaia database (Gaia DR3 2967141533259094400)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 37792 system from the Sun?

The HD 37792 system is 244 light years or 74.9 parsecs from the Sun.

What galaxy is the HD 37792 star in?

The HD 37792 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 37792 system?

The HD 37792 is a single star, there are no other known stars in the system.

What type of star is the HD 37792?

The star HD 37792 is a Yellow-White star star.

What temperature is star HD 37792?

The star HD 37792 has an effective temperature of 6500 K. Find out more about the temperature of stars in Stellar guide
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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.
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