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HD 214759
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Star HD 214759

Subgiant HD 214759 is located 87 light years away from the Sun. It is a single star of spectral class K0IV-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
87 light years
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HD 214759

Subgiant, High proper motion star
Spectral class: K0IV-V

Location +

Ascension iconRight ascension: 22h 40m 55.612s
Declination iconDeclination: -31° 59' 23.880'' (southern hemisphere)
Parallax iconParallax: 37.490
Distance iconSun distance: 86.998 ly | 26.7 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: 140 % M Sun
| 1414.2 M Jupiter
 (estimate)
+
Star mass
The mass of the star HD 214759 is unknown. Based on its other characteristics, it is estimated to be about 140 % 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: 320 % R Sun
| 32.2 R Jupiter
(estimate)
+
Star size
Radius of the star HD 214759 is not known. Its estimated value based on other similar stars is about 320 % 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: 5200 K
 (estimate)
+
Star temperature
Surface temperature of HD 214759 is estimated to be 5151 K, which is 90 % 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): 7.4
Magnitude iconAbsolute magnitude (V): 5.3
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 214759 system structure

 HD 214759

More about HD 214759

       HD 214759 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 6606890608810806528
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External sources
simbad icon
Simbad database (HD 214759)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
gaia icon
Gaia database (Gaia DR3 6606890608810806528)
Archive from the Gaia mission

Frequently Asked Questions

How far is the HD 214759 system from the Sun?

The HD 214759 system is 87 light years or 26.7 parsecs from the Sun.

What galaxy is the HD 214759 star in?

The HD 214759 is in the Milky Way galaxy just like the Sun.

How many stars are in the HD 214759 system?

The HD 214759 is a single star, there are no other known stars in the system.

What type of star is the HD 214759?

The star HD 214759 is a Subgiant star.

What temperature is the HD 214759?

The primary in the HD 214759 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

 LP 984-80
 - 2 ly

HD 215641
 - 3.4 ly

2MASS J22305403-3358331
 - 5.6 ly

CD-31 19078
 - 7.1 ly

LP 985-32
 - 8.7 ly
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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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