Astronomy:Alpha Herculis

From HandWiki
Short description: Multiple star system in the constellation Hercules
α Herculis
Hercules constellation map.svg
Red circle.svg
Location of α Herculis (circled)
Observation data
{{#ifeq:J2000|J2000.0 (ICRS)|Epoch J2000.0      Equinox J2000.0 (ICRS)| Epoch J2000      [[Astronomy:Equinox (celestial coordinates)|Equinox J2000}}
Constellation Hercules
A
Right ascension  17h 14m 38.853s[1]
Declination +14° 23′ 25.34″[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
Evolutionary stage AGB[3]
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: −7.32[5] mas/yr
Dec.: 36.07[5] mas/yr
Parallax (π)9.07 ± 1.32[5] mas
Distanceapprox. 360 ly
(approx. 110 pc)
Absolute magnitude (MV)−2.3[6] + 1.8 + 2.8[7]
Details
A
Mass2.5+1.6
−1.1[8] M☉
Radius284 ± 60, 264–303[3] R☉
Luminosity7,244–9,333[3] L☉
Surface gravity (log g)−0.41±0.19[9] cgs
Temperature3,155–3,365[3] K
Ba
Mass~2.5[3] M☉
Luminosity126[3] L☉
Temperature4,900[3] K
Bb
Mass~2[3] M☉
Luminosity26[3] L☉
Temperature7,350[3] K
Age0.41–1.25[3] Gyr
Other designations
Ras Algethi, Rasalgethi, α Her, 64 Her, BD+14°3207, HIP 84345, CCDM J17146+1424, AAVSO 1710+14, WDS J17146+1423[10]
A: HD 156014, HR 6406, SAO 102680
B: HD 156015, HR 6407, SAO 102681
Database references
SIMBADα Her
A
B

Alpha Herculis (α Herculis, abbreviated Alpha Her, α Her), also designated 64 Herculis, is a multiple star system in the constellation of Hercules. Appearing as a single point of light to the naked eye, it is resolvable into a number of components through a telescope. It has a combined apparent magnitude of 3.08, although the brightest component is variable in brightness. Based on parallax measurements obtained during the Hipparcos mission, it is approximately 360 light-years (110 parsecs) distant from the Sun.

System

A view of Alpha Herculis in a small telescope. The components A and B are resolved with angular separation of 4.64'' (in 2020).

Alpha Herculis is a triple star system. The primary (brightest) of the three stars, designated α1 Herculis or α Herculis A, is a pulsating variable star on the asymptotic giant branch (AGB), and is the second nearest AGB star after Mira. The primary star forms a visual binary pair with a second star, which is itself a spectroscopic binary.[3]

Alpha Herculis also forms the A and B components of a wider system designated WDS J17146+1423, with two additional faint visual companions designated WDS J17146+1423C and D.[11] The two fainter stars are far more distant than the triple system.[12]

Nomenclature

α Herculis (Latinised to Alpha Herculis) is the system's Bayer designation; α1 and α2 Herculis, those of its two visible components. 64 Herculis is the system's Flamsteed designation. WDS J17146+1423 is the wider system's designation in the Washington Double Star Catalog. The designations of Alpha Herculis' main components as Alpha Herculis A and B and the wider system's four components as WDS J17146+1423A, B, C and D, together with the spectroscopic pair - Alpha Herculis Ba and Bb - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[13]

Alpha Herculis bore the traditional name Rasalgethi or Ras Algethi (Arabic: رأس الجاثي ra‘is al-jāthī 'Head of the Kneeler').[14] 'Head' comes from the fact that in antiquity Hercules was depicted upside down on maps of the constellation. In 2016, the IAU organized a Working Group on Star Names (WGSN)[15] to catalog and standardize proper names for stars. The WGSN approved the name Rasalgethi for the component Alpha Herculis A (α1) on 30 June 2016 and it is now so included in the List of IAU-approved Star Names.[15]

The term ra's al-jaθiyy or Ras al Djathi appeared in the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, which was translated into Latin as Caput Ingeniculi.[16]

In Chinese astronomy, Alpha Herculis is called 帝座, Pinyin: Dìzuò, meaning 'Emperor's Seat'. The star is seen as marking itself, and stands alone in the center of the Emperor's Seat asterism, Heavenly Market enclosure (see: Chinese constellations).[17] 帝座 (Dìzuò) was westernized into Ti Tso by R.H. Allen, with the same meaning [18]

Properties

A light curve for Alpha Herculis A, plotted from data published by Wasatonic (1997)[19]

Alpha Herculis A and B are more than 500 AU apart, with an estimated orbital period of approximately 3600 years.[citation needed] A presents as a relatively massive red bright giant, but radial velocity measurements suggest a companion with a period of the order of a decade.[11] B's two components are a primary yellow giant star and a secondary, yellow-white dwarf star in a 51.578 day orbit.[20]

Alpha Herculis A is an asymptotic giant branch (AGB) star, a luminous red giant that has both hydrogen and helium shells around a degenerate carbon-oxygen core. It is the second nearest AGB star to the Sun.[3] The angular diameter of the star has been measured with an interferometer as 34 ± 0.8 mas, or 0.034 arcseconds.[21] At its estimated distance of 110 parsecs this corresponds to a radius of about 280 million kilometers (or 170 million miles), which is roughly 400 R☉ or 1.87 AU.[lower-alpha 1] If Alpha Herculis were at the center of the 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]

Alpha Herculis A has been specified as a standard star for the spectral class M5 Ib-II.[3] Like most type M stars near the end of their lives, Alpha Herculis is experiencing a high degree of stellar mass loss creating a sparse, gaseous envelope that extends at least 930 AU.[20] It is a semiregular variable with complex changes in brightness with periods ranging from a few weeks to many years. The most noticeable variations occur at timescales of 80–140 days and at 1,000 - 3,000 days. The strongest detectable period is 128 days.[22] The full range in brightness is from magnitude 2.7 to 4.0,[2] but it usually varies over a much smaller range of around 0.6 magnitudes.[22]

Notes

  1. ↑ To determine Rasalgethi's radius in terms of solar units, the calculations begin with the formula for angular diameter as follows:
    [math]\displaystyle{ \begin{smallmatrix} {\delta} = \frac{d_R}{D_R}\end{smallmatrix} }[/math]
    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 one knows the angular diameter and the Distance, then one can solve for dR as follows:
    [math]\displaystyle{ \begin{smallmatrix}d_R = \delta \cdot D_R = {0.034} \cdot 110.0 = 3.740 AU \end{smallmatrix} }[/math].
    To obtain Rasalgheti's radius:
    [math]\displaystyle{ \begin{smallmatrix}R_R = {\left ( {\frac {d_R}{2}} \right )} = {\left ( {\frac {3.740}{2}} \right )} = 1.870 AU \end{smallmatrix} }[/math].
    Converting into Solar units, 1 AU = 149,597,871 km and the mean radius of the Sun = 696,000 km, hence the calculation:
    [math]\displaystyle{ \begin{smallmatrix}d_B = {\left ( 1.87 AU \right )} {\left ( {\frac {149,597,871 km}{696,000 km}} \right )} = 280,000,000 km = 402 R_{\odot} \end{smallmatrix} }[/math] (rounded).

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27. doi:10.1888/0333750888/2862. ISBN 0333750888. Bibcode: 2000A&A...355L..27H. 
  2. ↑ 2.0 2.1 2.2 Samus, N. N. 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. ↑ 3.00 3.01 3.02 3.03 3.04 3.05 3.06 3.07 3.08 3.09 3.10 3.11 3.12 3.13 3.14 3.15 3.16 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. doi:10.1088/0004-6256/146/6/148. Bibcode: 2013AJ....146..148M. 
  4. ↑ 4.0 4.1 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. ↑ 5.0 5.1 5.2 van Leeuwen, F (November 2007). "Hipparcos, the New Reduction". Astronomy and Astrophysics 474 (2): 653–664. doi:10.1051/0004-6361:20078357. Bibcode: 2007A&A...474..653V. 
  6. ↑ Huang, W.; Wallerstein, G.; Stone, M. (2012). "A catalogue of Paschen-line profiles in standard stars". Astronomy & Astrophysics 547: A62. doi:10.1051/0004-6361/201219804. Bibcode: 2012A&A...547A..62H. 
  7. ↑ 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. 
  8. ↑ Moravveji, E.; Guinan, E. F.; Sobouti, Y. (2011). "On the Mass and Evolutionary Status of the Bright Red AGB Supergiant α1 Herculis". Why Galaxies Care About Agb Stars Ii: Shining Examples and Common Inhabitants 445: 163. Bibcode: 2011ASPC..445..163M. 
  9. ↑ 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, doi:10.1051/0004-6361:20066633, Bibcode: 2007A&A...465..593S 
  10. ↑ "alf Her". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=alf+Her. 
  11. ↑ 11.0 11.1 "Washington Double Star Catalog". United States Naval Observatory. http://ad.usno.navy.mil/wds/. 
  12. ↑ Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. 
  13. ↑ Hessman, F. V.; Dhillon, V. S.; Winget, D. E.; Schreiber, M. R.; Horne, K.; Marsh, T. R.; Guenther, E.; Schwope, A.; Heber, U. (2010). "On the naming convention used for multiple star systems and extrasolar planets". arXiv:1012.0707 [astro-ph.SR].
  14. ↑ Kurt Vonnegut. "Constellations: Hercules 'the Strongman'". The BBC (British Broadcasting Corporation). https://www.bbc.co.uk/dna/h2g2/A29778916. 
  15. ↑ 15.0 15.1 "IAU Working Group on Star Names (WGSN)". https://www.iau.org/science/scientific_bodies/working_groups/280/. 
  16. ↑ 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. doi:10.1093/mnras/55.8.429. Bibcode: 1895MNRAS..55..429K. 
  17. ↑ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 25 日
  18. ↑ Richard Hinckley Allen: Star Names — Their Lore and Meaning: Hercules
  19. ↑ Wasatonic, Richard P. (January 1997). "Photoelectric Photometry of TX Psc, Alpha Her A, Omicron Cet, and RT Cyg". The Journal of the American Association of Variable Star Observers 26 (1): 1–13. Bibcode: 1997JAVSO..26....1W. https://app.aavso.org/jaavso/article/1637/. Retrieved 18 December 2022. 
  20. ↑ 20.0 20.1 Deutsch, Armin J. (March 1956). "The Circumstellar Envelope of Alpha Herculis". Astrophysical Journal 123: 210–227. doi:10.1086/146152. Bibcode: 1956ApJ...123..210D. 
  21. ↑ 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. doi:10.1086/116033. Bibcode: 1991AJ....102.2091B. 
  22. ↑ 22.0 22.1 Percy, John R; Wilson, Joseph B; Henry, Gregory W (2001). "Long‐TermVRIPhotometry of Small‐Amplitude Red Variables. I. Light Curves and Periods". Publications of the Astronomical Society of the Pacific 113 (786): 983. doi:10.1086/322153. Bibcode: 2001PASP..113..983P. 

External links

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



Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:Alpha_Herculis&oldid=3426600"