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TOI 1648
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Star TOI 1648

Orange star TOI 1648 is located 228 light years away from the Sun. It is a single star of spectral class K2V, that has 82 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
228 light years
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TOI 1648

Orange star
Spectral class: K2V

Location +

Ascension iconRight ascension: 3h 1m 36.290s
Declination iconDeclination: 69° 13' 47.727'' (northern hemisphere)
Parallax iconParallax: 14.335
Distance iconSun distance: 227.527 ly | 69.8 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 % M Sun
| 859 M Jupiter
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Star mass
Mass of the star TOI 1648 is 0.82 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: 83 % R Sun
| 8.3 R Jupiter
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Star size
Radius of the star TOI 1648 is 0.83 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: 4836.0 K | 0.84 T Sun
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Star temperature
Surface temperature of TOI 1648 is 4836.0 K, which is 84 % 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): 10.4
Magnitude iconAbsolute magnitude (V): 6.2
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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TOI 1648 system structure

 TOI 1648
TOI 1648 b 0.07 AU 7.4 M⊕ 2.5 R⊕ 7.3 days

More about TOI 1648

Star TOI 1648 is approximately 80 % of the size of Sun and temperature on its surface is around 4836.0 K (4563 °C), which is about 84 % of Sun's temperature.
       TOI 1648 can be found in northern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is easily observable from Northern America, Europe and Asia.
Other designations of this star
TOI-1648, Gaia DR3 540977282990133888
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External sources
icon study
gaia icon
Gaia database (Gaia DR3 540977282990133888)
Archive from the Gaia mission

Frequently Asked Questions

How far is the TOI 1648 system from the Sun?

The TOI 1648 system is 228 light years or 69.8 parsecs from the Sun.

What galaxy is the TOI 1648 star in?

The TOI 1648 is in the Milky Way galaxy just like the Sun.

How many stars are in the TOI 1648 system?

The TOI 1648 is a single star, there are no other known stars in the system.

What type of star is the TOI 1648?

The star TOI 1648 is a Orange star star.

What temperature is star TOI 1648?

The star TOI 1648 has an effective temperature of 4836.0 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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