Phi Andromedae

φ Andromedae

Location of φ Andromedae (upper left).
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 01h 09m 30.13s[1]
Declination +47° 14′ 30.5″[1]
Apparent magnitude (V) 4.252
Characteristics
Spectral type B7V
U−B color index -0.34
B−V color index -0.07
R−I color index -0.05
Variable type Emission-line Star
Astrometry
Radial velocity (Rv) -0.1 km/s
Proper motion (μ) RA: 4.05 ± 0.52[1] mas/yr
Dec.: -12.43 ± 0.38[1] mas/yr
Parallax (π) 4.55 ± 0.60[1] mas
Distance approx. 720 ly
(approx. 220 pc)
Absolute magnitude (MV) 4.197
Details
Mass 18 M
Radius 7 R
Luminosity 20.000 L
Temperature 10.000–30.000 K
Rotational velocity (v sin i) 71 Km/s km/s
Orbit
Companion φ Andromedae B
Period (P) 371.6 yr
Semimajor axis (a) 0.447"
Eccentricity (e) 0.21
Inclination (i) 131°
Longitude of the node (Ω) 148.2°
Periastron epoch (T) 1889.9
Other designations
42 Andromedae, HR 335, HD 6811, BD+46°275, HIP 5434, SAO 36972, GC 1394, ADS 940, CCDM 01095+4715.
Database references
SIMBAD data
Database references
SIMBAD data

Phi Andromedae (φ Andromedae, φ And) is a binary star system near the border of the constellation of Andromeda, approximately 720 light years from the Earth.[1] With χ And it forms the Chinese asterism 軍南門 (Keun Nan Mun, Mandarin jūnnánmén), "the South Gate of the Camp".[2][3]

Double star

The primary component, φ And A, is a blue-white B-type subgiant with an apparent magnitude of 4.6m. The companion star, φ And B, is a blue-white B-type main sequence dwarf with an apparent magnitude of 5.6m. The two stars are separated by 0.64 arcseconds and have an orbital period of 371.6 years. The combined brightness of the system is 4.26m.

References

  1. ^ a b c d e f van Leeuwen, F. (2007). "HIP 5434". Hipparcos, the New Reduction. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=I/311/hip2&recno=5423. Retrieved 2009-12-06. 
  2. ^ Allen, R. H. (1899). Star-names and Their Meanings. New York: G. E. Stechart.  p.39.
  3. ^ In Chinese literature, φ Andromedae is stand alone in the asterism and χ Andromeda is member of Tien Ta Tseang (Heaven's Great General) asterism, see (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 9 日 and (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 10 日

External links