Gliese 180
(Red dwarf)- CSI-17-04516
- HIC 22762
- HIP 22762
- LFT 377
- L 736-30
- LP 776-27
- LPM 198
- LTT 2116
- 2MASS J04534995-1746235
- NLTT 14144
- PLX 1097
- PLX 1097.00
- TYC 5903-680-1
- [RHG95] 838
- GJ 180
- Gaia EDR3 2979590513145784192
Gliese 180 is a main sequence star that undergoes hydrogen fusion into helium. It is classified as a red dwarf, a common type of star in our solar vicinity. Its size is approximately 40% that of the Sun, and the surface temperature reaches around 3572 K.
LOCATION
Discover the celestial coordinates and distances that help us locate and understand this star's position in space.
When looking at celestial coordinates, you'll see three main position types: Right Ascension (RA) measures east-west position like longitude, Declination (Dec) measures north-south position like latitude, and Parallax helps determine a star's distance from Earth. Together, these coordinates help us pinpoint exactly where objects are in our night sky!
BASIC CHARACTERISTICS
Explore the fundamental properties that define this star's physical nature and evolution.
A star's basic characteristics - its mass, size, temperature, age, and luminosity - are all interconnected. These properties determine the star's life cycle and how it appears to us from Earth. Understanding these relationships helps astronomers classify stars and predict their future evolution.
PHOTOMETRY
Understand how bright this star appears from Earth and its true luminosity in space.
Apparent magnitude is how bright a star looks from Earth, while absolute magnitude is its true brightness from a standard distance of 10 parsecs. The lower the number, the brighter the star - and negative numbers mean extremely bright objects!
Closest stars
Discover the stellar neighbors closest to this star in our cosmic neighborhood.
58 Eridani
2MASS J0439-2353
LP 775-31
Gliese 173
2MASS J0523-1403
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