M92

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Globular Cluster in Hercules


About this Object

Globular cluster M92 is one of the original discoveries of Johann Elert Bode, who found it on December 27, 1777. Charles Messier independently rediscovered it and cataloged it on March 18, 1781, the same day as he cataloged another 8 objects, all of them Virgo Cluster galaxies (M84-M91). It was William Herschel who first resolved it into stars in 1783. According to newer sources, M92 is about 26,000 light years distant, only little more than its brighter apparent neighbor M13. From its HRD (or CMD), it may be a bit younger than M13 as its turnoff point is shifted to the brighter and bluer end. A semi-recent estimate of M92's age has given a value of about 16 billion years (anyway more than 14 billion years).

More informations are available at the seds.org website


Technical Data

Optics

130 mm f/12.6 Astro-Physics EDF Refractor

Mount

Astro-Physics AP 900GTO

Camera SBIG ST-10XE.
Filters SBIG CFW8A.With Astrodon LRGB Ha filters
Focuser Robofocus focuser and Focusmax software
Dates 30 May 2006.
Location Lentin Observatory
Exposure L=60mn bin1 RGB=36:36:36 minutes.bin2. Scale 0.85^s/pixel
Acquisition All data's were acquired unattended with ACP Observatory Control Software V4 DC3 Dreams and MaxIm DL 4, including sky flats,
Processing MaxIm DL 4, Photoshop CS, Registar, Neat Image.


All content are copyright Antoine Vergara