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KOI 7368
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Star KOI 7368

Orange star KOI 7368 is located 862 light years away from the Sun. It is a single star, that has 88 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
862 light years
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KOI 7368

Orange star

Location +

Ascension iconRight ascension: 19h 35m 47.400s
Declination iconDeclination: 48° 3' 55.000'' (northern hemisphere)
Parallax iconParallax: 3.785
Distance iconSun distance: 861.638 ly | 264.2 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: 88.3 % M Sun
| 925 M Jupiter
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Star mass
Mass of the star KOI 7368 is 0.883 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: 83 % R Sun
| 8.2 R Jupiter
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Star size
Radius of the star KOI 7368 is 0.827 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: 5225 K | 0.9 T Sun
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Star temperature
Surface temperature of KOI 7368 is 5225 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 iconAbsolute magnitude (V): -7.1
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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KOI 7368 system structure

 KOI 7368
KOI 7368 b 0.07 AU 2.2 R⊕ 6.8 days

More about KOI 7368

Star KOI 7368 is approximately 80 % of the size of Sun and temperature on its surface is around 5225 K (4952 °C), which is about 90 % of Sun's temperature.
       KOI 7368 can be found in northern celestial hemisphere.
Other designations of this star
KIC 10736489, 2MASS J19354742+4803549, TIC 27010191
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Frequently Asked Questions

How far is the KOI 7368 system from the Sun?

The KOI 7368 system is 862 light years or 264.2 parsecs from the Sun.

What galaxy is the KOI 7368 star in?

The KOI 7368 is in the Milky Way galaxy just like the Sun.

How many stars are in the KOI 7368 system?

The KOI 7368 is a single star, there are no other known stars in the system.

What type of star is the KOI 7368?

The star KOI 7368 is a Orange star star.

What temperature is star KOI 7368?

The star KOI 7368 has an effective temperature of 5225 K. Find out more about the temperature of stars in Stellar guide

stellar brief logoStellar Brief

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24. 10. 2026
stellar brief logo
A planet’s helium atmosphere streams ahead of its orbit, while infrared observations reveal the hidden rhythms of its star. New work also shows how neutron-star tilt can reshape X-ray light, traces the past of massive blue supergiants, and maps cloudy and clear zones on the hot Jupiter WASP-43 b.
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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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