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Star TOI 3493

Subgiant TOI 3493 is located 317 light years away from the Sun. It is a single star of spectral class G0IV-V, that has 102 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
317 light years

TOI 3493

Spectral class: G0IV-V

Location +

Ascension iconRight ascension: 13h 43m 11.771s
Declination iconDeclination: -22° 35' 7.635'' (southern hemisphere)
Parallax iconParallax: 10.295
Distance iconSun distance: 316.825 ly | 97.1 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: 102.3 % M Sun
| 1072 M Jupiter
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Star mass
Mass of the star TOI 3493 is 1.023 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: 123 % R Sun
| 12.2 R Jupiter
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Star size
Radius of the star TOI 3493 is 1.228 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: 5844 K | 1.01 T Sun
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Star temperature
Surface temperature of TOI 3493 is 5844 K, which is 101 % 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: 7.3 billions years | 1.59 Sun
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Star age
Star TOI 3493 is 7.3 billion years old, which is about 1.59 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 iconAbsolute magnitude (V): -4.9
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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TOI 3493 system structure

TOI 3493
TOI 3493 b n/a 9 M⊕ 3.2 R⊕ 8.2 days

More about TOI 3493

Star TOI 3493 is a main sequence star that fuses hydrogen atoms into helium. It is is approximately 23 % bigger than the Sun and temperature on its surface is around 5844 K (5571 °C), which is about 101 % of Sun's temperature.
       TOI 3493 can be found in southern celestial hemisphere, you cannot see it with naked eye, but you can observe this star with basic telescope. The star is also observable from Northern America, Europe and Asia. 
Other designations of this star
TIC 203377303, HD 119355, Gaia DR3 6192360843805622528
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External sources

Frequently Asked Questions

How far is the TOI 3493 system from the Sun?

The TOI 3493 system is 317 light years or 97.1 parsecs from the Sun.

What galaxy is the TOI 3493 star in?

The TOI 3493 is in the Milky Way galaxy just like the Sun.

How many stars are in the TOI 3493 system?

The TOI 3493 is a single star, there are no other known stars in the system.

What type of star is the TOI 3493?

The star TOI 3493 is a Subgiant star.

What temperature is star TOI 3493?

The star TOI 3493 has an effective temperature of 5844 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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