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Star TOI 2411

Orange star TOI 2411 is located 194 light years away from the Sun. It is a single star of spectral class K5V, that has 65 % of solar mass. There are multiple known exoplanets in this system.
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Sun distance
194 light years

TOI 2411

Spectral class: K5V

Location +

Ascension iconRight ascension: 1h 23m 42.000s
Declination iconDeclination: -8° 42' 5.000'' (equatorial region)
Parallax iconParallax: 16.770
Distance iconSun distance: 194.488 ly | 59.6 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: 65 % M Sun
| 681 M Jupiter
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Star mass
Mass of the star TOI 2411 is 0.65 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: 68 % R Sun
| 6.8 R Jupiter
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Star size
Radius of the star TOI 2411 is 0.68 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: 4099 K | 0.71 T Sun
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Star temperature
Surface temperature of TOI 2411 is 4099 K, which is 71 % 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): 11.3
Magnitude iconAbsolute magnitude (V): 7.4
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 2411 system structure

TOI 2411
TOI 2411 c n/a 2.9 R⊕ 18.8 days
TOI 2411 b 0.01 AU 3.9 M⊕ 1.7 R⊕ 0.8 days

More about TOI 2411

Star TOI 2411 is a main sequence star that fuses hydrogen atoms into helium. It is approximately 70 % of the size of Sun and temperature on its surface is around 4099 K (3826 °C), which is about 71 % of Sun's temperature.
       TOI 2411 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope. 
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External sources

Frequently Asked Questions

How far is the TOI 2411 system from the Sun?

The TOI 2411 system is 194 light years or 59.6 parsecs from the Sun.

What galaxy is the TOI 2411 star in?

The TOI 2411 is in the Milky Way galaxy just like the Sun.

How many stars are in the TOI 2411 system?

The TOI 2411 is a single star, there are no other known stars in the system.

What type of star is the TOI 2411?

The star TOI 2411 is a Orange star star.

What temperature is star TOI 2411?

The star TOI 2411 has an effective temperature of 4099 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 star’s hidden vibrations, a planet’s escaping helium, and worlds wrapped in shifting clouds reveal how much can be learned from changing light. Recent observations trace WASP 121’s surface motions in infrared for the first time, map the uneven clouds of WASP-43 b, and catch helium streaming ahead of TOI-3884 b. Light patterns also place the massive star HD 74371 on a return journey toward bluer colors after its red supergiant phase, while search interest spans Proxima Centauri b, Alpha Centauri, and many other stellar neighbors.
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