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HD 136834
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Star HD 136834

Subgiant HD 136834 is located 85 light years away from the Sun. It is a single star of spectral class K3IV-V, that has typically about 300 % of solar mass. For now, there are no known exoplanets in this star system.
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Sun distance
85 light years
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HD 136834

Subgiant, High proper motion star
Spectral class: K3IV-V

Location +

Ascension iconRight ascension: 15h 22m 42.165s
Declination iconDeclination: 1° 25' 1.227'' (equatorial region)
Parallax iconParallax: 38.501
Distance iconSun distance: 84.714 ly | 26.0 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: 80 % M Sun
| 859 M Jupiter
 (estimate)
+
Star mass
The mass of the star HD 136834 is unknown. Based on its other characteristics, it is estimated to be about 80 % 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: 90 % R Sun
| 8.8 R Jupiter
(estimate)
+
Star size
Radius of the star HD 136834 is not known. Its estimated value based on other similar stars is about 90 % 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: 4800 K
 (estimate)
+
Star temperature
Surface temperature of HD 136834 is estimated to be 4842 K, which is 83 % 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 136834 system structure

 HD 136834

More about HD 136834

       HD 136834 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
LHS 3067, GJ 1192, Gliese 1192, 2MASS J15224254+0125069, WISEA J152242.30+012503.3, TYC 337-615-1, Gaia DR3 4420712604009198080
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External sources
simbad icon
Simbad database (HD 136834)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 4420712604009198080)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 136834 system from the Sun?

The HD 136834 system is 85 light years or 26.0 parsecs from the Sun.

What galaxy is the HD 136834 star in?

The HD 136834 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 136834 system?

The HD 136834 is a single star, there are no other known stars in the system.

What type of star is the HD 136834?

The star HD 136834 is a Subgiant star.

What temperature is the HD 136834?

The primary in the HD 136834 system has an effective temperature of K ( °C). Find out more about the temperature of stars in Stellar guide
Class of stars Subgiant
A subgiant is a term used to describe a luminous star that is typically running out of hydrogen for nuclear fusion and is thus departing from the main sequence. These stars are classified as Yerkes luminosity class IV.
Closest stars

 5 Serpentis
 1.2 M☉ 3.1 ly

PM J15169-0037
 - 3.9 ly

2MASS J15210327+0131426
 - 5.8 ly

PM J15214+0414
 - 5.8 ly

BD+03 3032
 - 8 ly
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