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TOI-5699
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Star TOI-5699

Subgiant TOI-5699 is located 995 light years away from the Sun. It is a single star of spectral class G0IV, that has 113 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
995 light years
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TOI-5699

Subgiant
Spectral class: G0IV

Location +

Ascension iconRight ascension: 16h 44m 54.309s
Declination iconDeclination: 31° 12' 39.301'' (northern hemisphere)
Parallax iconParallax: 3.280
Distance iconSun distance: 994.526 ly | 304.9 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: 113 % M Sun
| 1184 M Jupiter
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Star mass
Mass of the star TOI-5699 is 1.13 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: 164 % R Sun
| 16.3 R Jupiter
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Star size
Radius of the star TOI-5699 is 1.64 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: 5905 K | 1.02 T Sun
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Star temperature
Surface temperature of TOI-5699 is 5905 K, which is 102 % 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: 6.6 billions years | 1.43 Sun
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Star age
Star TOI-5699 is 6.6 billion years old, which is about 1.43 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): 10.9
Magnitude iconAbsolute magnitude (V): 3.4
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-5699 system structure

 TOI-5699
TOI-5699 b 0.16 AU 79.5 M⊕ 11.2 R⊕ 22 days

More about TOI-5699

Star TOI-5699 is is approximately 64 % bigger than the Sun and temperature on its surface is around 5905 K (5632 °C), which is about 102 % of Sun's temperature.
       TOI-5699 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
TIC 224328450, TYC 2582-02794-1
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Frequently Asked Questions

How far is the TOI-5699 system from the Sun?

The TOI-5699 system is 995 light years or 304.9 parsecs from the Sun.

What galaxy is the TOI-5699 star in?

The TOI-5699 is in the Milky Way galaxy just like the Sun.

How many stars are in the TOI-5699 system?

The TOI-5699 is a single star, there are no other known stars in the system.

What type of star is the TOI-5699?

The star TOI-5699 is a Subgiant star.

What temperature is star TOI-5699?

The star TOI-5699 has an effective temperature of 5905 K. Find out more about the temperature of stars in Stellar guide
Class of stars Subgiant
A subgiant is a term used to describe a luminous star that is typically running out of hydrogen for nuclear fusion and is thus departing from the main sequence. These stars are classified as Yerkes luminosity class IV.
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