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TIC 402710280
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Star TIC 402710280

TIC 402710280 is an orange dwarf star located approximately 218 light-years from the Sun. It serves as the host for a newly identified sub-Neptune planet candidate.
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Nearby stars catalogue
Sun distance
218 light years

TIC 402710280

Location +

Ascension iconRight ascension: 16h 34m 5.810s
Declination iconDeclination: -63° 32' 58.629'' (southern hemisphere)
Parallax iconParallax: 14.964
Distance iconSun distance: 217.966 ly | 66.8 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: 88 % M Sun
| 922 M Jupiter
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Star mass
Mass of the star TIC 402710280 is 0.88 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: 82 % R Sun
| 8.1 R Jupiter
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Star size
Radius of the star TIC 402710280 is 0.817 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: 5182 K | 0.9 T Sun
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Star temperature
Surface temperature of TIC 402710280 is 5182 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
luminosity icon
Luminosity: 0.43 L Sun
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Star luminosity
Luminosity is the total amount of energy a star gives off every second. Think of it as the star’s true brightness — not just how bright it looks from Earth. This is important because some stars may appear dim simply because they are far away, not because they’re actually faint... icon More about Star luminosity in StellarGuide

Photometry

Magnitude iconApparent magnitude (V): 10
Magnitude iconAbsolute magnitude (V): 5.9
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 402710280 system structure

TIC 402710280
TIC 402710280 b
unconfirmed
0.21 AU 3.8 R⊕ 36.3 days

More about TIC 402710280

Star TIC 402710280 is approximately 80 % of the size of Sun and temperature on its surface is around 5182 K (4909 °C), which is about 90 % of Sun's temperature.
       TIC 402710280 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. 
Other designations of this star
TIC 402710280; Gaia DR3 5828441289812582400, Gaia DR3 5828441289812582400
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External sources

Frequently Asked Questions

How far is the TIC 402710280 system from the Sun?

The TIC 402710280 system is 218 light years or 66.8 parsecs from the Sun.

What galaxy is the TIC 402710280 star in?

The TIC 402710280 is in the Milky Way galaxy just like the Sun.

How many stars are in the TIC 402710280 system?

The TIC 402710280 is a single star, there are no other known stars in the system.

What type of star is the TIC 402710280?

The star TIC 402710280 is a Orange star star.

What temperature is star TIC 402710280?

The star TIC 402710280 has an effective temperature of 5182 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 blue supergiant’s changing light reveals that it is moving back toward hotter temperatures after a red-supergiant phase. New findings also trace infrared ripples on WASP 121, map the uneven clouds of WASP-43 b, and reveal helium escaping ahead of TOI-3884 b. Meanwhile, observations of the young star V1298 Tauri show how magnetic activity can make a star brighten and fade across radio and X-ray light.
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