| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Andromeda |
| Right ascension | 02h 11m 02.56581s [2] |
| Declination | 48° 56′ 45.0634″ [2] |
| Apparent magnitude (V) | 9.0–11.5 [3] |
| Characteristics | |
| Spectral type | M4e [3] |
| B−V color index | 1.607 [4] |
| Variable type | Semi-regular [3] |
| Astrometry | |
| Radial velocity (Rv) | −10.0±2.0 [5] km/s |
| Proper motion (μ) | RA: 10.456(48) [2] mas/yr Dec.: −0.958(56) [2] mas/yr |
| Parallax (π) | 1.0950±0.0483 mas [2] |
| Distance | 3,000 ± 100 ly (910 ± 40 pc) |
| Other designations | |
| BD+48 616, HIP 10192 [5] | |
| Database references | |
| SIMBAD | data |
RV Andromedae is a variable star in the constellation of Andromeda. It is classified as a semiregular variable pulsating giant star, and varies from an apparent visual magnitude of 11.5 at minimum brightness to a magnitude of 9.0 at maximum brightness, with a period of approximately 168.9 days. [3]
In 1904, English amateur astronomer Arthur Stanley Williams examined photographic plates taken during the previous two years and determined that RV Andromedae was a variable star whose period he estimated to be 182 days. [6] In 1907, Annie Jump Cannon listed it with its variable star designation in her Second Catalogue of Variable Stars. [7]
This is one of the Mira variables where mode switching of pulsations have been observed; amplitude and periods have been seen decreasing and subsequently increasing back to values near the previous ones. [8]