Alpha Herculis

Coordinates: Sky map 17h 14m 38.858s, +14° 23′ 25.20″
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Alpha Herculis

Historical view of the Hercules constellation showing Rasalgethi as the α star and "Head of the Kneeler"
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
A
Right ascension 17h 14m 38.853s[1]
Declination +14° 23′ 25.0″[1]
Apparent magnitude (V) 3.350[1] (2.7 - 4.0[2])
B
Right ascension 17h 14m 39.181s[1]
Declination +14° 23′ 23.98″[1]
Apparent magnitude (V) 5.322[1]
Characteristics
A
Spectral type M5 Ib-II[3]
U−B color index +1.01[4]
B−V color index +1.45[4]
Variable type SRc[2]
B
Spectral type G8III + A9IV-V[3]
Astrometry
Proper motion (μ) RA: -6.71[5][6][7] mas/yr
Dec.: 32.78[5][6][7] mas/yr
Parallax (π)9.07 ± 1.32 mas[5][6]
Distanceapprox. 360 ly
(approx. 110 pc)
Absolute magnitude (MV)−2.3[8] + 1.8 + 2.8[9]
Details[3]
A
Mass2.5 M
Radius264 - 303 R
Luminosity7,244 - 9,333 L
Surface gravity (log g)−0.41 ± 0.19[10] cgs
Temperature3,155 - 3,365 K
Ba
Mass~2.5 M
Luminosity126 L
Temperature4,900 K
Bb
Mass~2 M
Luminosity26 L
Temperature7,350 K
Age0.41 - 1.25 Gyr
Other designations
Ras Algethi, Rasalgethi, α Her, 64 Her, BD+14°3207, HIP 84345, CCDM J17146+1424, AAVSO 1710+14
A: HD 156014, HR 6406, SAO 102680
B: HD 156015, HR 6407, SAO 102681
Database references
SIMBADdata

Alpha Herculis (α Her, α Herculis) is a multiple star system in the constellation Hercules. It has the traditional name Rasalgethi or Ras Algethi (Arabic: رأس الجاثي ra's al-jaθiyy Head of the Kneeler), and the Flamsteed designation 64 Herculis.[11] The traditional name "Head" comes from the fact that in antiquity Hercules was depicted upside down on the constellation maps.

The term ra's al-jaθiyy or Ras al Djathi was appeared in the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, which was translated into Latin as Caput Ingeniculi.[12]

In Chinese astronomy, Rasalgethi is called 帝座, Pinyin: Dìzuò, meaning Emperor's Seat, this star is marking itself and stands alone in the center of Emperor's Seat asterism, Heavenly Market enclosure (see : Chinese constellations).[13] 帝座 (Dìzuò) was westernized into Ti Tso by R.H. Allen, with the same meaning [14]

Properties

The primary star, α1 Her, is an asymptotic giant branch (AGB) star, a luminous red giant that has both hydrogen and helium shells around a degenerate carbon-oxygen core. Its angular diameter has been measured with an interferometer as 34 ± 0.8 mas, or 0.034 arcseconds.[15] At an estimated distance of 110 parsecs from Hipparcos,[5][6][16] this corresponds to a radius of about 280 million kilometers (or 170 million miles), which is roughly 400 R or 1.87 AU.[note 1] If Rasalgethi were at the center of our Solar System its radius would extend past the orbit of Mars at 1.5 AU but not quite as far as the asteroid belt. The red giant is estimated to have started its life with about 2.175-3.250 M.[3] Like most type M stars near the end of their lives, Rasalgethi is experiencing a high degree of stellar mass loss creating a sparse, gaseous envelope that extends at least 90 astronomical units.[17]

Star system

When viewed through a telescope, this system is resolved into two components designated α1 and α2. These two components are more than 500 astronomical units apart, with an estimated orbital period of approximately 3600 years. α1 is a relatively massive red bright giant. α2 is actually a double star system with a primary yellow giant star and a secondary, yellow-white dwarf star in a 51.578 day orbit. (These components are sometimes designated α Herculis A, Ba and Bb, respectively.)[18]

See also

Notes

  1. ^ To determine the Rasalgheti's radius in terms of solar units, the calculations begin with the formula for angular diameter as follows:
    where δ equals Rasalgethi's angular diameter in arcseconds, dR the star's diameter in AU, and DR the Distance from Earth in parsecs. If we know the angular diameter and the Distance, then we can solve for dR as follows:
    .
    To obtain Rasalgheti's radius:
    .
    Converting into Solar units, 1 AU = 149,597,871 km and the mean radius of the Sun = 696,000 km, hence the calculation:
    (rounded).

References

  1. ^ a b c d e f Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27. Bibcode:2000A&A...355L..27H.
  2. ^ a b Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S.
  3. ^ a b c d Moravveji, Ehsan; Guinan, Edward F.; Khosroshahi, Habib; Wasatonic, Rick (2013). "The Age and Mass of the α Herculis Triple-star System from a MESA Grid of Rotating Stars with 1.3 <= M/M ⊙ <= 8.0". The Astronomical Journal. 146 (6): 148. arXiv:1308.1632. Bibcode:2013AJ....146..148M. doi:10.1088/0004-6256/146/6/148.
  4. ^ a b Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
  5. ^ a b c d Perryman, M. A. C.; Lindegren, L.; Kovalevsky, J.; et al. (July 1997), "The Hipparcos Catalogue", Astronomy and Astrophysics, 323: L49–L52, Bibcode:1997A&A...323L..49P
  6. ^ a b c d van Leeuwen, F (November 2007). "Hipparcos, the New Reduction". Astronomy and Astrophysics. 474 (2). Centre de Données astronomiques de Strasbourg: 653. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
  7. ^ a b "SIMBAD query result:NAME RASALGETHI -- Semi-regular pulsating Star". Centre de Données astronomiques de Strasbourg. Retrieved 2010-09-26.
  8. ^ Huang, W.; Wallerstein, G.; Stone, M. (2012). "A catalogue of Paschen-line profiles in standard stars". Astronomy & Astrophysics. 547: A62. arXiv:1210.7893. Bibcode:2012A&A...547A..62H. doi:10.1051/0004-6361/201219804.
  9. ^ Reimers, D. (1977). "On the absolute scale of mass-loss in red giants. I - Circumstellar absorption lines in the spectrum of the visual companion of Alpha-1 HER". Astronomy and Astrophysics. 61: 217. Bibcode:1977A&A....61..217R.
  10. ^ Schröder, K.-P.; Cuntz, M. (April 2007), "A critical test of empirical mass loss formulas applied to individual giants and supergiants", Astronomy and Astrophysics, 465 (2): 593–601, arXiv:astro-ph/0702172, Bibcode:2007A&A...465..593S, doi:10.1051/0004-6361:20066633
  11. ^ Kurt Vonnegut. "Constellations: Hercules 'the Strongman'". The BBC (British Broadcasting Corporation). Retrieved 2010-11-14.
  12. ^ Knobel, E. B. (June 1895). "Al Achsasi Al Mouakket, on a catalogue of stars in the Calendarium of Mohammad Al Achsasi Al Mouakket". Monthly Notices of the Royal Astronomical Society. 55 (8): 429. Bibcode:1895MNRAS..55..429K. doi:10.1093/mnras/55.8.429.
  13. ^ Template:Zh icon AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 25 日
  14. ^ Richard Hinckley Allen: Star Names — Their Lore and Meaning: Hercules
  15. ^ Benson, J. A.; Dyck, H. M.; Mason, W. L.; Howell, R. R.; Ridgway, S. T.; et al. (December 1991). "The infrared angular diameter of Alpha Herculis measured with a Michelson interferometer". Astronomical Journal. 102: 2091–2097. Bibcode:1991AJ....102.2091B. doi:10.1086/116033.
  16. ^ Perryman, Michael (2010), The Making of History's Greatest Star Map, Astronomers’ Universe, Heidelberg: Springer-Verlag, doi:10.1007/978-3-642-11602-5, ISBN 978-3-642-11601-8
  17. ^ Deutsch, Armin J. (March 1956). "The Circumstellar Envelope of Alpha Herculis". Astrophysical Journal. 123: 210–227. Bibcode:1956ApJ...123..210D. doi:10.1086/146152.
  18. ^ Tokovinin, A. A. (1997). "MSC - a catalogue of physical multiple stars". Astronomy & Astrophysics Supplement Series. 124: 75. Bibcode:1997A&AS..124...75T. doi:10.1051/aas:1997181.

External links