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Star K2-33

Red dwarf K2-33 is located 453 light years away from the Sun. It is a single star of spectral class M3.3, that has 56 % of solar mass. There is at least one exoplanet in this system.
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Sun distance
453 light years

K2-33

Spectral class: M3.3

Location +

Ascension iconRight ascension: 16h 10m 14.729s
Declination iconDeclination: -19° 19' 9.791'' (equatorial region)
Parallax iconParallax: 7.193
Distance iconSun distance: 453.442 ly | 139.0 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: 56 % M Sun
| 587 M Jupiter
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Star mass
Mass of the star K2-33 is 0.56 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: 105 % R Sun
| 10.4 R Jupiter
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Star size
Radius of the star K2-33 is 1.05 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: 3540 K | 0.61 T Sun
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Star temperature
Surface temperature of K2-33 is 3540 K, which is 61 % 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: 0.009 billions years | 0 Sun
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Star age
Star K2-33 is 0.009 billion years old, which is about 0 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

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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K2-33 system structure

K2-33
K2-33 b 0.04 AU 1144.5 M⊕ 5 R⊕ 5.4 days

More about K2-33

Star K2-33 is is approximately 5 % bigger than the Sun and temperature on its surface is around 3540 K (3267 °C), which is about 61 % of Sun's temperature.
       K2-33 can be found in southern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope. 
Other designations of this star
EPIC 205117205, 2MASS J16101473-1919095, WISE J161014.73-191909.6, Gaia DR3 6245758900889486720
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Frequently Asked Questions

How far is the K2-33 system from the Sun?

The K2-33 system is 453 light years or 139.0 parsecs from the Sun.

What galaxy is the K2-33 star in?

The K2-33 is in the Milky Way galaxy just like the Sun.

How many stars are in the K2-33 system?

The K2-33 is a single star, there are no other known stars in the system.

What type of star is the K2-33?

The star K2-33 is a Red dwarf star.

What temperature is star K2-33?

The star K2-33 has an effective temperature of 3540 K. Find out more about the temperature of stars in Stellar guide
Class of stars Red dwarf
Red dwarfs are small, cool stars with surface temperatures of about 2,000–3,800 K, much cooler than the Sun. They usually have 8–50% of the Sun’s mass and shine very faintly, sometimes at just a tiny fraction of the Sun’s brightness. Classified mainly as spectral type M, they are the most common stars in the Milky Way, making up roughly 70–75% of its stellar population.

They fuse hydrogen slowly through the proton–proton chain and are fully convective, which allows them to use their fuel very efficiently. As a result, red dwarfs can live for tens of billions to trillions of years—far longer than the Sun. Many exoplanets orbit red dwarfs, including some in close habitable zones, though strong stellar activity can affect planetary environments.
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