Star Kepler 52

Red dwarf Kepler 52 is located 1043 light years away from the Sun. It is a single star, that has 54 % of solar mass. There are multiple known exoplanets in this system.

Kepler 52

Red dwarf

Location

Right ascension: 19h 6m 57.133s

Declination: 49° 58' 32.658'' (northern hemisphere)

Parallax: 3.128

Sun distance: 1042.587 ly | 319.7 pc

Basic characteristic

Mass: 54 % M Sun

Size: 56 % R Sun

Temperature: 4263.0 K | 0.74 T Sun

Photometry

Apparent magnitude (V): 15.5

Absolute magnitude (V): 8

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

Absolute stellar magnitude in different parts of the electromagnetic spectrum from infrared (K band) to ultraviolet (U band).

System structure

Kepler 52		AU
	Kepler 52 b	n/a	8.7 M⊕	2.1 R⊕	7.9 days
	Kepler 52 c	n/a	10.4 M⊕	1.8 R⊕	16.4 days
	Kepler 52 d	0.18 AU		2 R⊕	36.4 days

More about Kepler 52

Star Kepler 52 is approximately 60 % of the size of Sun and temperature on its surface is around 4263.0 K (3990 °C), which is about 74 % of Sun's temperature.

       Kepler 52 can be found in northern celestial hemisphere, however it is too dim to be seen with the naked eye or even a small telescope.

Other designations of this star
Gaia DR3 2133589776693414016, 2MASS J19065712+4958327, KIC 11754553, KOI-775, WISE J190657.12+495832.6

Class of stars Red dwarf

Red dwarfs are small reddish stars, that are by far the most common type of star in solar neighborhood. Their mass is usually between 10 and 50 % of solar mass.

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