deep-sky
galaxy (spiral)
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Discovered in 1773, M51 (& NGC5195) is one of the most well known galaxies in the sky and is a good example of a face-on spiral galaxy.
Its distance is approximately 23 million light years.
Just as M81 and M82, M51 and NGC 5195 (right part) are also gravitationally interacting galaxies.
Sometimes M51 is used to refer to both galaxies, in which case the individual galaxies are referred to as M51A (NGC5194) and M51B (NGC5195).
In 2005 as well as 2011 a supernova was observed in the Whirlpool Galaxy. These events helped to derive a more correct distance of 23 Mly as it was previously estimated to be around 37 Mly
Other / older versions :
Image information:
Object info
Name: M51 – The Whirlpool Galaxy
Type: Galaxy (spiral)
Constellation: Canes Venatici
Distance: 23 Mly
Date & location
Date: March 22, 2012
Location: Landgraaf, The Netherlands
Equipment & optics
Total integration: 2h40m
Camera: SBIG ST-8300M
Optics: Orion Optics SPX 10″ Newton
Mount: Losmandy G-11 Gemini
Image comments
Distance from Paracorr to CCD is not correct.