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TIC 365102760
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Star TIC 365102760

Red giant TIC 365102760 is located 1840 light years away from the Sun. It is a single star, that has 121 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
1840 light years

TIC 365102760

Location +

Ascension iconRight ascension: 20h 23m 21.562s
Declination iconDeclination: 54° 23' 39.552'' (northern hemisphere)
Parallax iconParallax: 1.773
Distance iconSun distance: 1,839.677 ly | 564.0 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: 121 % M Sun
| 1268 M Jupiter
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Star mass
Mass of the star TIC 365102760 is 1.21 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: 323 % R Sun
| 32.1 R Jupiter
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Star size
Radius of the star TIC 365102760 is 3.23 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: 4694.0 K | 0.81 T Sun
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Star temperature
Surface temperature of TIC 365102760 is 4694.0 K, which is 81 % 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
time icon
Age: 7.2 billions years | 1.57 Sun
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Star age
Star TIC 365102760 is 7.2 billion years old, which is about 1.57 of the Sun's age.

The age of a star tells us how long it has been shining since it formed. Knowing a star’s age helps astronomers understand its life stage, how it has changed over time, and what will happen to it in the future... icon More about Star age in StellarGuide

Photometry

Magnitude iconApparent magnitude (V): 12
Magnitude iconAbsolute magnitude (V): 3.2
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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TIC 365102760 system structure

TIC 365102760
TIC 365102760 b 0.06 AU 19.2 M⊕ 6.2 R⊕ 4.2 days

More about TIC 365102760

Star TIC 365102760 is is approximately 3 times bigger than the Sun and temperature on its surface is around 4694.0 K (4421 °C), which is about 81 % of Sun's temperature.
       TIC 365102760 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
2MASS J20232153+5423395, Gaia DR3 2185044477033336064
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External sources

Frequently Asked Questions

How far is the TIC 365102760 system from the Sun?

The TIC 365102760 system is 1840 light years or 564.0 parsecs from the Sun.

What galaxy is the TIC 365102760 star in?

The TIC 365102760 is in the Milky Way galaxy just like the Sun.

How many stars are in the TIC 365102760 system?

The TIC 365102760 is a single star, there are no other known stars in the system.

What type of star is the TIC 365102760?

The star TIC 365102760 is a Red giant star.

What temperature is star TIC 365102760?

The star TIC 365102760 has an effective temperature of 4694.0 K. Find out more about the temperature of stars in Stellar guide
Class of stars Red giant
White dwarfs are the hot, extremely dense stellar remnants left behind by stars that originally had masses between about 0.5 and 8 times the mass of the Sun during their main sequence lifetimes. After exhausting their nuclear fuel, these stars shed their outer layers and leave behind a compact core. Although white dwarfs contain between roughly 0.2 and 1.44 solar masses, this mass is packed into a volume comparable to that of an Earth-sized planet, making them some of the densest objects in the Universe.
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