R Andromedae

R Andromedae (R And) is a Mira-type variable star in the constellation Andromeda. Its spectral class is type S because it shows absorption bands of zirconium monoxide (ZrO) in its spectrum. It was among the stars found by Paul Merrill to show absorption lines of the unstable element technetium, establishing that nucleosynthesis must be occurring in stars. The SH molecule was found for the first time outside earth in the atmosphere of this star. The star is losing mass due to stellar winds at a rate of 1.09×10−6 M/yr.

R Andromedae
Location of R Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 00h 24m 01.946s
Declination +38° 34 37.37
Apparent magnitude (V) 5.8 - 15.2
Characteristics
Spectral type S3,5e-S8,8e(M7e)
B−V color index 1.97
Variable type Mira
Astrometry
Radial velocity (Rv)−6.40  km/s
Proper motion (μ) RA: −16.021±0.148 mas/yr
Dec.: −32.794±0.141 mas/yr
Parallax (π)2.6444 ± 0.1600 mas
Distance1,230 ± 70 ly
(380 ± 20 pc)
Absolute magnitude (MV)−5.19
Details
Radius476±120 - 493±129 R
Luminosity6,300 L
Surface gravity (log g)−1.02 cgs
Temperature2,500 K
Metallicity [Fe/H]−1.01 dex
Other designations
HR 90, BD +37°58, HD 1967, SAO 53860, HIP 1901.
Database references
SIMBADdata
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