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Best Cetus

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Best 1 Mira
Mira

Mira, designated Omicron Ceti, is a red giant star located approximately 420 light-years away in the constellation Cetus. It serves as the prototype for a class of long-period variable stars, known as Mira variables, which undergo dramatic changes in brightness due to physical pulsations. The star's...

2 LHS 1140
LHS 1140

LHS 1140 is an M-type red dwarf star located approximately 40 light-years from Earth in the constellation Cetus. The star hosts at least two confirmed exoplanets, including LHS 1140 b, a rocky super-Earth orbiting within the star's habitable zone that was discovered in 2017 by the MEarth survey. LHS...

3 UV Ceti
UV Ceti

UV Ceti is a red dwarf star located approximately 8.7 light-years from Earth in the constellation Cetus, making it one of the closest known star systems to the Sun. It serves as the prototype for the UV Ceti class of variable flare stars, which are characterized by dramatic, sudden increases in lumi...

4 L 726-8
L 726-8

L 726-8, formally designated Luyten 726-8, is a binary star system situated approximately 8.7 light-years from Earth in the constellation Cetus. The system consists of two red dwarf stars, BL Ceti and UV Ceti, which orbit each other in a highly eccentric path. UV Ceti serves as the prototype for a c...

Star Binary Cetus M Type Flare Star Uv Ceti Prototype
5 Luyten 726-8A

Luyten 726-8A, also cataloged as BL Ceti, is a red dwarf star located roughly 8.7 light-years away in the constellation Cetus. It is the brighter primary component of the L 726-8 binary system, which was jointly cataloged by Dutch-American astronomer Willem Luyten. Both components are flare stars, m...

6 GJ 3293
GJ 3293

GJ 3293 is an M-type red dwarf star situated approximately 57 light-years away in the constellation Cetus. It is known to host multiple confirmed exoplanets, including at least two super-Earths that were detected using radial velocity measurements. The planetary system's discovery has contributed to...

7 Skull Nebula (NGC 246)

A planetary nebula in Cetus discovered by William Herschel in 1785, notable for its large apparent size of about 4 arcminutes and a central white dwarf binary system.

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