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CWISEP J225628.97+400227.3
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Star CWISEP J225628.97+400227.3

Sub-brown dwarf CWISEP J225628.97+400227.3 is located 35 light years away from the Sun. It is a single star, that has typically about 1.5 % of solar mass. For now, there are no known exoplanets in this star system.
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Nearby stars catalogue
Sun distance
35 light years

CWISEP J225628.97+400227.3

Location +

Ascension iconRight ascension: 22h 56m 28.154s
Declination iconDeclination: 40° 2' 29.981'' (northern hemisphere)
Parallax iconParallax: 92.592
Distance iconSun distance: 35.225 ly | 10.8 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: 2 % M Sun
| 21 M Jupiter
 (estimate)
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Star mass
The estimated mass of the star CWISEP J225628.97+400227.3 is about 2 % of the Sun's mass, or approximately 21 Jupiter 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: 10 % R Sun
| 0.6 R Jupiter
(estimate)
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Star size
Radius of the star CWISEP J225628.97+400227.3 is not known. Its estimated value based on other similar stars is about 10 % 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: 341 K | 0.06 T Sun
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Star temperature
Surface temperature of CWISEP J225628.97+400227.3 is 341 K, which is 6 % 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 iconAbsolute magnitude (V): -0.2
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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CWISEP J225628.97+400227.3 system structure

CWISEP J225628.97+400227.3

More about CWISEP J225628.97+400227.3

Nearby brown dwarf CWISEP J225628.97+400227.3 is is is much smaller than the Sun and temperature on its surface is around 341 K (68 °C), which is about 6 % of Sun's temperature.
       CWISEP J225628.97+400227.3 can be found in northern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope. 
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Frequently Asked Questions

How far is the CWISEP J225628.97+400227.3 system from the Sun?

The CWISEP J225628.97+400227.3 system is 35 light years or 10.8 parsecs from the Sun.

What galaxy is the CWISEP J225628.97+400227.3 star in?

The CWISEP J225628.97+400227.3 is in the Milky Way galaxy just like the Sun.

How many stars are in the CWISEP J225628.97+400227.3 system?

The CWISEP J225628.97+400227.3 is a single star, there are no other known stars in the system.

What type of star is the CWISEP J225628.97+400227.3?

The star CWISEP J225628.97+400227.3 is a Sub-brown dwarf star.

What temperature is star CWISEP J225628.97+400227.3?

The star CWISEP J225628.97+400227.3 has an effective temperature of 341 K. Find out more about the temperature of stars in Stellar guide
Class of stars Sub-brown dwarf
Brown dwarfs are not really stars, because there is no thermonuclear fusion in their core. These objects are smaller and cooler than stars, but too massive to be considered planets. Brown dwarfs of spectral class Y are the coolest and only a few of them have been discovered so far.
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