Double Clusters NGC869 and NGC884



Object Data
Description The famous double cluster in Perseus was known in ancient times, and was first cataloged by the Greek astronomer Hipparcos. Both clusters are situated in the Perseus OB-1 association and are both quite young (5.6 and 3.2 million years). Their hottest main sequence stars are of spectral type B0.
Constellation Perseus, the Rescuer of Andromeda
Right Ascension 2h 20m 59s
Declination +57° 9' 6"
Magnitude 4.3 & 4.4
Angular size 58 arcminutes (both clusters together)
Distance 2.25 kiloparsecs (7,300 light years)
Radial Velocity -40 kilometers per second (approaching)
Image Data
Photographer Fred Lehman
Main Scope Meade 14" LX200GPS
Imaging Scope Celestron 5" SCT @ f/3.3 (415mm)
Guide Camera Not needed
Imaging Camera Starlight Xpress MX7C
Resolution 780 x 580 @ 1.44 arcseconds per pixel
Exposure Thirty exposures of 10 seconds each. Aligned, stacked, and processed with AstroArt.
Date January 16, 2004
Location Area 51 in Big Cypress National Preserve in central South Florida.


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