The topic of HD 92036 is one that has generated great interest over time. With diverse edges and approaches, HD 92036 has captured the attention of experts and fans alike. In this article, we will explore different aspects related to HD 92036, from its origin to its implications in today's society. Through a detailed and exhaustive analysis, we will seek to better understand HD 92036 and its relevance in the current context. From its origins to its impact today, HD 92036 has been the subject of debate and reflection, and through this article, we will seek to shed light on its key points.
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Hydra |
Right ascension | 10h 37m 13.72508s[1] |
Declination | −27° 24′ 45.4713″[1] |
Apparent magnitude (V) | 4.87[2] |
Characteristics | |
Evolutionary stage | AGB[3] |
Spectral type | M1III:Ba0.5[4] |
B−V color index | +1.626±0.009[2] |
Astrometry | |
Radial velocity (Rv) | +16.9±2.8[2] km/s |
Proper motion (μ) | RA: −114.142[1] mas/yr Dec.: +19.712[1] mas/yr |
Parallax (π) | 6.5530±0.2634 mas[1] |
Distance | 500 ± 20 ly (153 ± 6 pc) |
Absolute magnitude (MV) | −1.00[2] |
Details | |
Radius | 57.46+5.43 −4.05[1] R☉ |
Luminosity | 740.8±33.7[1] L☉ |
Temperature | 3,972+148 −175[1] K |
Other designations | |
CD−26°8033, FK5 2848, HD 92036, HIP 51979, HR 4162, SAO 179041[5] | |
Database references | |
SIMBAD | data |
HD 92036 is a single[6] star in the equatorial constellation of Hydra. Its apparent magnitude is 4.87.[2] This is an aging red giant star on the asymptotic giant branch[3] with a stellar classification of M1III:Ba0.5.[4]