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TOI-2202
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Star TOI-2202

Orange star TOI-2202 is located 769 light years away from the Sun. It is a single star of spectral class K8V, that has 82 % of solar mass. There are multiple known exoplanets in this system.
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Sun distance
769 light years
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TOI-2202

Orange star
Spectral class: K8V

Location +

Ascension iconRight ascension: 3h 24m 54.900s
Declination iconDeclination: -73° 57' 27.000'' (southern hemisphere)
Parallax iconParallax: 4.210
Distance iconSun distance: 769.236 ly | 235.8 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: 82.3 % M Sun
| 862 M Jupiter
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Star mass
Mass of the star TOI-2202 is 0.823 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: 79 % R Sun
| 7.9 R Jupiter
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Star size
Radius of the star TOI-2202 is 0.794 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: 5064 K | 0.88 T Sun
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Star temperature
Surface temperature of TOI-2202 is 5064 K, which is 88 % 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: 7.48 billions years | 1.63 Sun
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Star age
Star TOI-2202 is 7.48 billion years old, which is about 1.63 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): 13
Magnitude iconAbsolute magnitude (V): 6.1
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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TOI-2202 system structure

 TOI-2202
TOI-2202 b 0.1 AU 310.9 M⊕ 11.2 R⊕ 11.9 days
TOI-2202 c 0.16 AU 117.3 M⊕ 24.7 days

More about TOI-2202

Star TOI-2202 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 80 % of the size of Sun and temperature on its surface is around 5064 K (4791 °C), which is about 88 % of Sun's temperature.
       TOI-2202 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.
Other designations of this star
TIC 358107516
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Frequently Asked Questions

How far is the TOI-2202 system from the Sun?

The TOI-2202 system is 769 light years or 235.8 parsecs from the Sun.

What galaxy is the TOI-2202 star in?

The TOI-2202 is in the Milky Way galaxy just like the Sun.

How many stars are in the TOI-2202 system?

The TOI-2202 is a single star, there are no other known stars in the system.

What type of star is the TOI-2202?

The star TOI-2202 is a Orange star star.

What temperature is star TOI-2202?

The star TOI-2202 has an effective temperature of 5064 K. Find out more about the temperature of stars in Stellar guide

stellar brief logoStellar Brief

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24. 10. 2026
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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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