Gamma Andromedae: Difference between revisions
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==Location== |
==Location== |
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The shjkjhjkhjkh |
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The star's location is shown in the following chart of the Andromeda constellation: |
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[[Image:Andromeda constellation map.png|thumb|none|250px|Andromeda Constellation]] |
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{{-}} |
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==Visual companion== |
==Visual companion== |
Revision as of 02:18, 9 December 2009
Gamma Andromedae (Gamma And / γ And / γ Andromedae) is the third brightest star in the constellation of Andromeda. It is also known by the traditional name Almach (also spelt as Almaach, Almaack, Almak, Almaak, or Alamak), from the Arabic العناق الأرض al-‘anāq al-’arđ̧[1] "the caracal" (desert lynx).[2] It was known as 天大將軍一 (the First Star of the Great General of the Heaven) in Chinese.[1]
In 1778, Johann Tobias Mayer discovered that γ Andromedae was a double star. When examined in a small telescope, it appears to be a bright, golden yellow star (γ1 Andromedae) next to a dimmer, greenish-blue star (γ2 Andromedae), separated by approximately 10 arcseconds. It is considered by stargazers to be a beautiful double star with a striking contrast of color.[3][4][5] It was later discovered that γ2 Andromedae is itself a triple star system. What appears as a single star to the naked eye is thus a quadruple star system, approximately 350 light-years from the Earth.[3][6]
In the Babylonian star catalogues, γ And together with Triangulum formed the constellation known as MULAPIN (𒀯𒀳) "The Plough".[7]
Astrologically this star was considered "honourable and eminent." [8]
γ1 Andromedae
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Andromeda |
Right ascension | 02h 03m 53.9531s[4] |
Declination | +42° 19′ 47.009″[4] |
Apparent magnitude (V) | 2.26[4] |
Characteristics | |
Spectral type | K3IIb[9] |
U−B color index | +1.58[9] |
B−V color index | +1.37[9] |
R−I color index | +0.68[9] |
Astrometry | |
Radial velocity (Rv) | −11.7 ± 0.9[4] km/s |
Proper motion (μ) | RA: 43.08[4] mas/yr Dec.: −50.85[4] mas/yr |
Parallax (π) | 9.19 ± 0.73 mas[4] |
Distance | 350 ± 30 ly (109 ± 9 pc) |
Absolute magnitude (MV) | −2.9[10] |
Details | |
Radius | 80[11] R☉ |
Luminosity | 2,000[11] L☉ |
Temperature | 4,500[11] K |
Rotational velocity (v sin i) | < 17[9] km/s |
Other designations | |
Almach, Almaach, Almak, Almaak, Alamak, γ1 And, Gamma1 Andromedae, Gamma1 And, γ Andromedae A, γ And A, Gamma Andromedae A, Gamma And A, 57 Andromedae A, 57 And A, STF 205A, ADS 1630 A, BD+41 395, CCDM J02039+4220A, FK5 73, GC 2477, HD 12533, HIP 9640, HR 603, IDS 01578+4151 A, PPM 44721, SAO 37734, WDS 02039+4220A.[4][9][12] | |
Database references | |
SIMBAD | data |
γ1 Andromedae is a bright giant star with a spectral classification of K3IIb. It has an apparent visual magnitude of approximately 2.26.[9]
γ2 Andromedae
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Andromeda |
Right ascension | 02h 03m 54.720s (B)[13] |
Declination | +42° 19′ 51.41″ (B)[13] |
Apparent magnitude (V) | 4.84 (BC) (combined) 5.5 (B) |
Characteristics | |
Spectral type | B9.5V/B9.5V (B) |
U−B color index | −0.12[14] |
B−V color index | +0.03[14] |
Astrometry | |
Radial velocity (Rv) | −14 ± 5 (B)[5] km/s |
Proper motion (μ) | RA: 37 (B)[5] mas/yr Dec.: −57 (B)[5] mas/yr |
Parallax (π) | 9.19 ± 0.73 mas[13] |
Distance | 350 ± 30 ly (109 ± 9 pc) |
Absolute magnitude (MV) | −0.3 (BC)[10] |
Orbit[17] | |
Period (P) | 63.67 ± 1.0 yr |
Semi-major axis (a) | 0.302 ± 0.001″ |
Eccentricity (e) | 0.927 ± 0.03 |
Inclination (i) | 109.8 ± 5.0° |
Longitude of the node (Ω) | 109.6 ± 5.0° |
Periastron epoch (T) | B2015.5 ± 1.5 |
Argument of periastron (ω) (secondary) | 183.4 ± 15.0° |
Position (relative to γ1 And) | |
Epoch of observation | 2004 |
Angular distance | 9.6″ [12] |
Position angle | 63° [12] |
Other designations | |
Database references | |
SIMBAD | data |
γ2 Andromedae, with an overall apparent visual magnitude of 4.84,[14] is 9.6 arcseconds away from γ1 Andromedae at a position angle of 63 degrees.[12] In October 1842, Wilhelm Struve found that γ2 Andromedae was itself a double star whose components were separated by less than an arcsecond.[1] The components are an object of apparent visual magnitude 5.5, γ Andromedae B, and a type-A main sequence star with apparent visual magnitude 6.3, γ Andromedae C.[14] They have an orbital period of about 64 years.[17] Spectrograms taken from 1957 to 1959 revealed that γ Andromedae B was itself a spectroscopic binary, composed of two type-B main sequence stars orbiting each other with a period of 2.67 days.[15]
Location
The shjkjhjkhjkh
Visual companion
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Andromeda |
Right ascension | 02h 03m 51.74s[19] |
Declination | +42° 19′ 35.4″[19] |
Apparent magnitude (V) | 15.0[19] |
Position (relative to γ1 And) | |
Epoch of observation | 1898 |
Angular distance | 27.9″ [20] |
Position angle | 245° [20] |
Database references | |
SIMBAD | data |
Other designations | |
CCDM J02039+4220D, a star with apparent visual magnitude 15.0, has been observed 28 arcseconds away from γ1 Andromedae.[20]
See also
References
- ^ a b c p. 36–37, Star-names and Their Meanings, Richard Hinckley Allen, New York: G. E. Stechert, 1899.
- ^ p. 23, Star tales, Ian Ridpath, James Clarke & Co., 1989, ISBN 0718826957.
- ^ a b pp. 113–114, vol. 1, Burnham's Celestial Handbook: An Observer's Guide to the Universe Beyond the Solar System, Robert Burnham, New York: Courier Dover Publications, 1978, ISBN 048623567X.
- ^ a b c d e f g h i NAME ALMACH -- Star in double system, database entry, SIMBAD. Accessed on line August 19, 2008.
- ^ a b c d e HD 12534 -- Spectroscopic binary, database entry, SIMBAD. Accessed on line August 19, 2008.
- ^ 01578+4151, database entry, MSC - a catalogue of physical multiple stars, A. A. Tokovinin, CDS database ID J/A+AS/124/75.
- ^ Origins of the ancient constellations: I. The Mesopotamian traditions, J. H. Rogers, Journal of the British Astronomical Association 108, #1 (February 1998), pp. 9–28, Bibcode:1998JBAA..108....9R.
- ^ p.27, Star Lore of All Ages, William Tyler Olcott, G.P. Putnam's Sons, New York and London, The Knickerbocker Press, 1911
- ^ a b c d e f g HR 603, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line August 19, 2008.
- ^ a b From apparent magnitude and parallax.
- ^ a b c Almach, Jim Kaler, Stars. Accessed on line August 19, 2008.
- ^ a b c d e Entry 02039+4220, discoverer code STF 205, components A-BC, The Washington Double Star Catalog, United States Naval Observatory. Accessed on line August 27, 2008.
- ^ a b c Component 2, HIP 9640, database entry, Hipparcos catalogue, CDS ID I/239.
- ^ a b c d e HR 604, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line August 19, 2008.
- ^ a b A Preliminary Study of the Spectroscopic Binary Gamma Andromedae B, L. A. Maestre and J. A. Wright, Astrophysical Journal 131 (January 1960), pp. 119–121, Bibcode:1960ApJ...131..119M.
- ^ Entry 02039+4220, discoverer code STT 38BC, The Washington Double Star Catalog, United States Naval Observatory. Accessed on line August 19, 2008.
- ^ a b Entry 02039+4220, Sixth Catalog of Orbits of Visual Binary Stars, William I. Hartkopf & Brian D. Mason, United States Naval Observatory. Accessed on line August 21, 2007.
- ^ BD+41 395C -- Star in double system, database entry, SIMBAD. Accessed on line August 21, 2008.
- ^ a b c CCDM J02039+4220D -- Star in double system, database entry, SIMBAD. Accessed on line August 19, 2008.
- ^ a b c d Entry 02039+4220, discoverer code BAR 22, components AD, The Washington Double Star Catalog, United States Naval Observatory. Accessed on line August 19, 2008.
External links
- Alamak at Alcyone Software's Star Data Pages
- Almaak (Gamma Andromedae) at The Internet Encyclopedia of Science
- Image ALMACH
- Gamma Andromedae on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images