|
|
|
NGC 6397 - a globular cluster in the constellation
Ara |
|
This image
is the first test of Deep Sky Lucky Imaging at the CDK12 with exposure times of
1 s per single image. The used QHY 163M camera was kindly provided by Martin
Miller for a test. A total of 900 1-second single images were taken in each
color channel. The worst were sorted out and about 700 images per color channel
were processed. The luminance channel was artificially generated from the RGB
images to further minimize background noise. The finished image is therefore
not a pure LRGB, but a (RGB)RGB image. Compared to images with 120 s exposure
time, the seeing in the summed image improved from 2.5'' to 2.1''
(FHWM).
The Moon, illuminated to about 80 %, was
only 40 degrees away from NGC 6397 at the time of imaging. Due to the
brightened background the weaker stars in the outer area could not be detected
in this test.
A second test image with ultra-short exposure
times, the globular cluster NGC 6441,
is shown here in
comparison to a long exposed image.. |
|
|
Object description:
NGC 6397 is the second closest globular cluster to our
solar system after Messier 4. It is only 7,800 light years away and contains
about 400,000 stars. It was first observed by Nicolas Lacaille in 1751. With a
brightness of 5m7 it is visible to the naked eye under a dark sky.
Due
to the proximity to the solar system and the lack of intergalactic extinction,
the distance of NGC 6397 could be determined very accurately. The average age
of the stars was derived to 13.4 billion years, they are only slightly younger
than the universe.
« Click here or the thumbnail image for a comparison with the
size of the Moon |
|
|
|
|