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KIC 1718360
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Star KIC 1718360

Subgiant KIC 1718360 is located 1027 light years away from the Sun. It is a single star of spectral class G1.5IV-V, that has typically about 300 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
1027 light years
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KIC 1718360

Subgiant
Spectral class: G1.5IV-V

Location +

Ascension iconRight ascension: 19h 23m 4.499s
Declination iconDeclination: 37° 13' 48.973'' (northern hemisphere)
Parallax iconParallax: 3.175
Distance iconSun distance: 1,027.299 ly | 315.0 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: 110 % M Sun
| 1162.8 M Jupiter
 (estimate)
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Star mass
The mass of the star KIC 1718360 is unknown. Based on its other characteristics, it is estimated to be about 110 % 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: 91 % R Sun
| 9.1 R Jupiter
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Star size
Radius of the star KIC 1718360 is 0.91 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: 5800 K
 (estimate)
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Star temperature
Surface temperature of KIC 1718360 is estimated to be 5757 K, which is 100 % 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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KIC 1718360 system structure

 KIC 1718360
KIC 1718360 b 0.04 AU 1 R⊕ 2.9 days

More about KIC 1718360

       KIC 1718360 can be found in northern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.
Other designations of this star
Gaia DR3 2051029235274657280
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External sources
icon study
gaia icon
Gaia database (Gaia DR3 2051029235274657280)
Archive from the Gaia mission

Frequently Asked Questions

How far is the KIC 1718360 system from the Sun?

The KIC 1718360 system is 1027 light years or 315.0 parsecs from the Sun.

What galaxy is the KIC 1718360 star in?

The KIC 1718360 is in the Milky Way galaxy just like the Sun.

How many stars are in the KIC 1718360 system?

The KIC 1718360 is a single star, there are no other known stars in the system.

What type of star is the KIC 1718360?

The star KIC 1718360 is a Subgiant star.

What temperature is the KIC 1718360?

The primary in the KIC 1718360 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.
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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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