Near Gamma-Leonis
Two images taken about 30 minutes apart
Starlight Express SXV on 4" Tak FSQ-106
1st image:
22:27--22:34 EST, Feb 14, 2010.
R=G=B=20 seconds in 1 second increments
2nd image:
22:59--23:01 EST, Feb 14, 2010.
R=G=B= 5 seconds in 1 second increments
Gamma Leonis is a binary star. It's two components are separated by 4
arcseconds. I took some short 0.1 second exposures, but even in these images
Gamma Leonis saturated the CCD chip. However, applying a Richard-Lucy
deconvolution followed by a logarthmic stretch, it is possible to see
elongation in the binary. Click the image to see the full frame with
Vesta.