
The Whirlpool galaxy (M51) in Canes Venatici.
Thris was the first galaxy where spiral structure was seen
by the Earl of Rosse in 1845. M51 consists of two interacting
galaxies NGC 5194 and 5195 (the smaller one). It is visible
in small telescopes, but the interesting structure is only
visible with larger apertures. It's distance is about 15 million
light years.

This is an uncropped version of the image above.
Leo Triplett (M65, M66 & NGC 3628)

M65, M66 and NGC 3628 are a striking sight in a larger telescope.
In my 10" I can see the differences in structure between
the two Messier galaxies and the dust-lane in the much fainter
NGC 3628. M65 and M66 are located in the constellation Leo
about 20-25 millon light years away.

This evening I had to take unguided exposures
because my QHY5 autoguider decided it will not work with our
Notebook.
Additionally It seems I am still not getting
perfect focus, even though I used a Bahtinov mask.
| Telescope: |
Astro-Professional 80mm f/7 Doublet
with TS Flattener |
| Camera |
Nikon D7000 |
| Exposure: |
M51: 37x 30" @ ISO 3200
Leo Triplett: 38x30" @ ISO 3200 |
| Date: |
6th May 2011 |
|