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Click the image for a wider view. (1722 x
1148 - 735 KB)
Instrument |
12.5" RCOS @
~f/9 (2880 mm fl) 1.28 arcsec / pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/ internal filter wheel, AstroDon Gen I Filters |
Acquisition Data |
9/4/2010 to 9/8/2010 Chino Valley, AZ... with CCDAutoPilot3
& CCDSoft. AOL guided |
Exposure |
RGB 225 min (15 x 5 min each, bin 2x2) |
Software |
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CCDSoft, CCDStack and
PixInsight
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eXcalibrator v5.0 for
(g:r)
color balancing, using 80 stars from the APASS database.
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CCDBand-Aid to repair
KAI-11000M vertical bars.
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CCDStack to calibrate,
register, normalize, data reject, combine the sub exposures and RGB
color.
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PixInsight for gradient removal
and non-linear stretching with HistogramTransformation.
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Comment |
North is to the top.
Albireo is a beautiful gold and blue double star in the
constellation Cygnus. It is still unknown if Albireo is a
gravitationally bound binary system or simply a chance alignment
optical double. At a distance of 380 light-years, and with a
separation of 35 arcsec, the possible orbital period is at least
75,000 years. Given this long orbital period, it will probably take
several hundred more years to determine the nature of this double.
In 1976, gold colored Albireo-A was discovered to be a binary star,
with a separation of only 0.4 arcseconds. Albireo-B is a fast
rotating blue-green star with a surface temperature of about 13,200
K.
Although much about this double is unknown, we know that is a truly
magnificent sight, when viewed with a telescope. Even the smallest
of backyard telescopes will reveal Albireo's beauty.
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