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HD 92786
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Star HD 92786

Orange star HD 92786 is located 87 light years away from the Sun. It is a single star of spectral class G9V, that has typically about 70 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
87 light years
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HD 92786

Orange star, High proper motion star
Spectral class: G9V

Location +

Ascension iconRight ascension: 10h 43m 33.302s
Declination iconDeclination: 48° 12' 53.698'' (northern hemisphere)
Parallax iconParallax: 37.280
Distance iconSun distance: 87.488 ly | 26.8 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: 70 % M Sun
| 743.8 M Jupiter
 (estimate)
+
Star mass
The mass of the star HD 92786 is unknown. Based on its other characteristics, it is estimated to be about 70 % 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: 70 % R Sun
| 7.2 R Jupiter
(estimate)
+
Star size
Radius of the star HD 92786 is not known. Its estimated value based on other similar stars is about 70 % 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: 4400 K
 (estimate)
+
Star temperature
Surface temperature of HD 92786 is estimated to be 4434 K, which is 76 % 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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HD 92786 system structure

 HD 92786

More about HD 92786

       HD 92786 can be found in northern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is easily observable from Northern America, Europe and Asia.
Other designations of this star
TYC 3445-421-1, HIP 52470, Gaia DR3 832417236660307072
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External sources
simbad icon
Simbad database (HD 92786)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 832417236660307072)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 92786 system from the Sun?

The HD 92786 system is 87 light years or 26.8 parsecs from the Sun.

What galaxy is the HD 92786 star in?

The HD 92786 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 92786 system?

The HD 92786 is a single star, there are no other known stars in the system.

What type of star is the HD 92786?

The star HD 92786 is a Orange star star.

What temperature is the HD 92786?

The primary in the HD 92786 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
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stellar brief logoStellar Brief

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30. 10. 2026
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The early architecture of planetary systems may be set at birth: a study of Sun-like stars found similar rates of star-planet misalignment across different stages of development. Other findings trace how water and carbon dioxide ice fade around young stars, why white-dwarf debris resists breaking into tiny pieces, and why a reported planet around Gliese 48 remains unconfirmed.
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