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Albireo

Beta (β) Cygni
Contrast Optical Double Star

Right Ascension 19h 30m 43s Best Seen 6/15 - 11/15
Declination 27° 57' 35" Magnitude (combined) 3.05
Apparent Separation 34.4" Constellation Cygnus
4,620 au

Actual
Compared
to Sun
Distance 385 / 376 ly --
Actual Brightness -- 497 / 94
Apparant Magnitude 3.08 / 5.12
Absolute Magnitude -2.2 / -0.2
Size -- ~20 / ~3 Solar Radius
Mass -- ~4 / ~6 Solar Mass
Surface Gravity -- --
Surface Composition (by mass) 74% hydrogen
24% helium
2% everything else
same
Spectral Type K3 II / B8 Ve G2 V
Density (gram/cubic cm) -- --

What To Look For Through The Telescope


  1. Recommended eyepiece: 24mm or 40 mm.

  2. When people look through the telescope they should see two stars next to each other. The brighter star should appear yellow and the dimmer star blue.

Albireo Information:

  1. The 5th brightest star in Cygnus, Albireo is one of the best known contrast optical double stars.

  2. The yellow star is actually a multiple star system: the star and an unseen companion orbit each other.

  3. In Arabic, “Minqar al-Dajajah,” meaning “the hen’s beak” - otherwise known as the “beak star”.

  4. Light we’re seeing left in 1586 AD:

    • 1580 - Sir Francis Drake completes his circumnavigation of the globe…his is the 2nd journey to do that and the first under the same commander.
    • 1582 – the Gregorian calendar is implemented
    • 1582 – Shakespeare marries Anne Hathaway
    • 1580s – Chocolate is introduced commercially to Europe
    • 1587 – Mary Queen of Scots is beheaded
    • 1587 – English settlers arrive at Roanoake Island in North Carolina and re-establish the deserted colony
  5. If they are orbiting each other (we don’t know for certain), their orbital period is at least 75,000 years

  6. Beta1 Cyg or Albireo A (the golden amber star):

    Color Orange, K3 II, bright giant
    Luminosity 889 Suns; 1460 Suns total
    Diameter 66 Suns
    Absolute Magnitude -2.55 visual; -3.16 total

    a. In 1976, it was discovered that this is a binary system in itself, separated by 40 AU, and orbiting each other every 100-200 years. Our telescope can’t distinguish between them.

    • The brighter star is a helium-fusing giant, class K3 (orange)

      Temperature 7440⁰ F
      Luminosity 950 Suns
      Diameter 50 Suns
      Mass 5 Suns
    • The other is a hydrogen-fusing main sequence, class B9 (blue)

      Temperature 19,340⁰ F
      Luminosity 100 Suns
      Mass 3.2 Suns
  7. Beta2 Cyg or Albireo B (the blue-white star):

    Color B8 Ve, main sequence
    Temperature 20,100⁰ F
    Luminosity 117 Suns visual; 229 Suns total
    Diameter 3.88 Suns
    Absolute Magnitude -0.35 visual; -1.15 total

    a. Very fast spinning star (150 miles per second), rotation period of about 14 hours, this causes a gas disk around it

    b. From Albireo B, Albireo A would appear as brilliant orange and blue points about ½ degree apart. The orange star would shine with light equal to about 35 full moons, and the blue/white companion about ½ half that.

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References
Item Updated Notes
Coordinates 2002-07-24 SIMBAD, The Flamsteed Collection
Combined Magnitude 2002-07-24 with Scott’s The Flamsteed Collection
Apparent Separation 2002-07-24 http://www.astronomical.org/constellations/cyg.html
Distance --
Actual Brightness --
Magnitude 2002-07-24 with Scott’s Starlist 2000
Mass --
Surface Gravity --
Surface Composition 2003-01-06 OK for all stars
Spectral Type 2002-07-24 SIMBAD
Density --
Other Information
Size, Mass 2005-05-04 1. previous: “About 60 of our solar systems could be laid edge to edge between these two stars.” – BUT much more, so took out.
2. Add info about binary found at http://www.daviddarling.info/encyclopedia/A/Albireo.html
Other data found using app.mag, dist. and spectral class on a graph of the HR diagram