Alpha Cephei

Alderamin, α Cep

Location of α Cephei (bottom right).
Observation data
Epoch J2000      Equinox J2000
Constellation Cepheus
Right ascension 21h 18m 34.7715s[1]
Declination 62° 35′ 08.061″[1]
Apparent magnitude (V) 2.5141 [2]
Characteristics
Spectral type A7IV-V [2]
U−B color index +0.12[3]
B−V color index +0.21 [3]
Variable type Delta Scuti
Astrometry
Radial velocity (Rv) -10[1] km/s
Proper motion (μ) RA: +150.55[2] mas/yr
Dec.: 49.09[2] mas/yr
Parallax (π) 66.50 ± 0.11[2] mas
Distance 49.05 ± 0.08 ly
(15.04 ± 0.02 pc)
Absolute magnitude (MV) 1.63 [2]
Details
Mass 1.9 [4] M
Radius 2.5[4] R
Luminosity 18[4] L
Temperature 7,600 [4] K
Metallicity ? Fe/H
Rotational velocity (v sin i) 246[5] km/s
Age ? years
Other designations
Alderamin, 5 Cep, 2MASS J21183475+6235081, AG+62° 1226, Gl 826, HR 8162, BD +61°2111, HD 203280, GCTP 5139.00, SAO 19302, FK5 803, HIP 105199 CCDM J21186+6236A.
Database references
SIMBAD data

Coordinates: 21h 18m 34.8s, +62° 35′ 08″

Alpha Cephei (α Cep, α Cephei) is a second magnitude star in the constellation of Cepheus that is relatively close to Earth at only 49 light years. It has the traditional name Alderamin, an Arabic name meaning "the right arm".

Contents

Visibility

With a declination in excess of 62 degrees north, Alderamin is mostly visible to observers in the northern hemisphere, though the star is still visible as far south as ± 27° South latitude, albeit just above the horizon. The star is circumpolar throughout all of Europe, northern Asia, Canada and American cities as far south as San Diego on the west coast but not quite as far as Miami on the east coast. All other locations around the globe having a latitude greater than ± 27° North will notice that the star is always visible in the night sky. Since Alderamin has an apparent magnitude of about 2.5, the star is easily observable to the naked eye, even in light polluted cities.

Properties

Alderamin is a white Class A star, evolving off of the main sequence into a subgiant, probably on its way to becoming a red giant as its hydrogen supply runs low. In 2007, the star's apparent magnitude was recalibrated at 2.5141 along with an updated parallax of 66.50 ± 0.11 mas yielding a distance of 15 parsecs or approximately 49 light years from Earth.[2]

Given a surface temperature of 7,600 Kelvin, theoretical calculations would yield a total luminosity for the star of about 18.7L.Alderamin has a radius of 2.5R boasting a mass that is almost twice that of the Sun at 1.9M. Like other stars in its class, it is slightly variable with a range in brightness of 0.06 magnitude, and is listed as a Delta Scuti variable.

Alderamin has a very high rotation speed of at least 246 km/s, completing one complete revolution in less than 12 hours, with such a rapid turnover appearing to inhibit the differentiation of chemical elements usually seen in such stars.[5] By comparison, the Sun takes almost a month to turn on its axis. α Cep is also known to emit an amount of X radiation similar to the Sun, which along with other indicators suggests the existence of considerable magnetic activity—something unexpected (though not at all unusual) for a fast rotator.

Pole star

Alderamin is located near the precessional path traced across the celestial sphere by the Earth's north pole. That means that it periodically comes within 3° of being a pole star, much as Polaris is at present. This will next occur about the year 7500 AD.

Preceded by Pole Star Succeeded by
Iota Cephei circa 6,800 BC Deneb

Ethnological influences

Etymology

The name Alderamin is a contraction of the Arabic phrase الذراع اليمين að-ðirā‘ al-yamīn "the right arm," with the first definite article transliterated literally as al, as is often the case with Arabic star names.

This star, along with β Cep (Alfirk) and η Cep (Alkidr) were Al Kawākib al Firḳ (الكوكب الفرق), meaning "the Stars of The Flock" by Ulug Beg.[6][7]

In Chinese, 天鈎 (Tiān Gōu), meaning Celestial Hook, refers to an asterism consisting of α Cephei, 4 Cephei, HD 194298, η Cephei, θ Cephei, ξ Cephei, 26 Cephei, ι Cephei and ο Cephei.[8] Consequently, α Cephei itself is known as 天鈎五 (Tiān Gōu wu, English: the Fifth Star of the Celestial Hook.).[9]

Namesakes

USS Alderamin (AK-116) was a United States Navy Crater class cargo ship named after the star.

See also

References

  1. ^ a b c "SIMBAD query result: NAME ALDERAMIN -- Variable Star". Centre de Données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Alderamin&submit=SIMBAD+search. Retrieved 2010-12-20. 
  2. ^ a b c d e f g van Leeuwen, F (November 2007). "Hipparcos, the New Reduction". Astronomy and Astrophysics (Centre de Données astronomiques de Strasbourg) 474 (2): 653–664. Bibcode 2007A&A...474..653V. doi:10.1051/0004-6361:20078357. http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HIP%20105199. Retrieved 2010-12-19. 
  3. ^ a b Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV data.. Bibcode 1986EgUBV........0M. 
  4. ^ a b c d Professor James B. (Jim) Kaler. "ALDERAMIN (Alpha Cephei)". University of Illinois. http://stars.astro.illinois.edu/sow/alderamin.html. Retrieved 2010-12-20. 
  5. ^ a b "Bright Star Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR. Centre de Données astronomiques de Strasbourg. http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HR%208162. Retrieved 2010-12-20. 
  6. ^ Allen, R. H. (1963). Star Names: Their Lore and Meaning (Reprint ed.). New York: Dover Publications Inc. p. 157. ISBN 0486210790. http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Cepheus*.html. Retrieved 2010-12-12. 
  7. ^ Davis Jr., G. A., "The Pronunciations, Derivations, and Meanings of a Selected List of Star Names,"Popular Astronomy, Vol. LII, No. 3, Oct. 1944, p. 16.
  8. ^ (Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
  9. ^ (Chinese) 香港太空館 - 研究資源 - 亮星中英對照表, Hong Kong Space Museum. Accessed on line November 23, 2010.

External links