Alpha 1 Capricorni

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Double star
α 1 Capricorni
α 1 cap in the constellation "Capricorn"
AladinLite
Observation
dates equinoxJ2000.0 , epoch : J2000.0
Constellation Capricorn
Right ascension 20 h 17 m 38.87 s
declination -12 ° 30 ′ 29.6 ″
Apparent brightness 4.41 mag
Typing
B − V color index 1.07 
U − B color index 0.80 
R − I index 0.55 
Spectral class G3 Ib
Astrometry
Radial velocity −25.79 ± 0.15 km / s
parallax (5.73 ± 0.33)  mas
distance (570 ± 33)  ly
(175 ± 10)  pc
Bolometric absolute brightness M bol −2.79 mag
Proper movement 
Rec. Share: (22.98 ± 0.32)  mas / a
Dec. portion: (1.28 ± 0.28)  mas / a
Physical Properties
Dimensions 5.3  M
radius 130  R
Luminosity

1050  L

Effective temperature 5300  K
Metallicity [Fe / H] +0.22
Other names
and catalog entries
Bayer name α 1 capricorni
Flamsteed name 5 capricorni
Bonn survey BD −12 ° 5683
Bright Star Catalog HR 7747 [1]
Henry Draper Catalog HD 192876 [2]
Hipparcos catalog HIP 100027 [3]
SAO catalog SAO 163422 [4]
Tycho catalog TYC 5748-2598-1 [5]Template: Infobox star / maintenance / specification of the TYC catalog
2MASS catalog 2MASS 20173888-1230295 [6]
Other names WDS 20176-1230
CCDM 20176-1231

Alpha 1 Capricorni1 Cap) is a telescopic and spectroscopic multiple star in the constellation Capricorn . It has a total brightness of 4.4 mag and its distance is about 570 light years .

Alpha 1 Capricorni is a system made up of at least five components. The main star A is a yellow supergiant with a little over 5 times the mass, 130 times the radius and 1000 times the luminosity of the sun . Its surface temperature is around 5300 K, a little below that of the sun.

In 1827, John Herschel found a companion C, 120 times weaker, with an apparent magnitude of 9.6 mag, next to the bright star A for around 30 arc seconds. This star is also called BD −12 ° 5682. Later, in 1874 , Sherburne Wesley Burnham was able to describe a third component B. This star has a brightness of only 14.1 mag and was about 15 arc seconds away from the main star A at the time of its discovery, today the distance is a little over 50 ".

In 1905 Carl Wilhelm Wirtz was finally able to recognize another companion D with a brightness of 14.2 mag and a distance of 30 ″ to component C, and on the other hand he was able to identify the main star A itself as a narrow spectroscopic double star. Its two components Aa and Ab have apparent magnitudes of 4.4 and 8.6 mag.

Alpha 1 was together with the star Alpha 2 Capricorni also with the proper name " Algiedi " or "Algedi" (from Arabic الجدي, DMG al-ǧady  'the billy goat'). To distinguish it from this, it was also called "Prima Giedi". According to the “IAU Catalog of Star Names” of the Working Group on Star Names (WGSN) of the IAU for the standardization of star names, the name in the form “Algedi” was only assigned to the lighter Alpha 2 Capricorni in 2016 .

Scientific research

In 2005, the influence of the star's rotation speed on the occurrence of various elements in its atmosphere was investigated for Alpha 1 Capricorni and other medium-weight stars with a mass between 5 and 20 M from observations at the European Southern Observatory in Chile . Values ​​for the effective temperature, the force of gravity on the surface, microturbulence speed, brightness and mass, as well as the frequency of various elements were determined.

Individual evidence

  1. a b c d e VizieR: Hipparcos, the New Reduction (van Leeuwen, 2007) - The Astrometric Catalog
  2. a b VizieR: Stellar Photometry in Johnson's 11-color system (Ducati, 2002)
  3. ^ VizieR: Southern B and Be stars (Levenhagen +, 2006)
  4. VizieR: General Catalog of Stellar Radial Velocities (Wilson, 1953)
  5. a b c d e f g R. Smiljanic, B. Barbuy, JR De Medeiros, A. Maeder: CNO in evolved intermediate mass stars. In: Astronomy & Astrophysics. Vol. 449, 2006, doi: 10.1051 / 0004-6361: 20054377 , pp. 655-671 ( bibcode : 2006A & A ... 449..655S ).
  6. ^ VizieR: Catalog of Stellar Diameters (CADARS) (Pasinetti-Fracassini + 2001)
  7. VizieR: The Washington Visual Double Star Catalog (Mason + 2001-2014)
  8. Bulletin of the IAU Working Group on Star Names, No. 2. IAU Division C Education, Outreach and Heritage, 2016 ( PDF; 158 KB ).