Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  IC 4263  ·  IC 4278  ·  M 51  ·  NGC 5169  ·  NGC 5173  ·  NGC 5194  ·  NGC 5195  ·  NGC 5198  ·  Whirlpool galaxy
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M51 (Whirlpool Galaxy) and NGC5195; Canes Venatici, Thomas V. Davis
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M51 (Whirlpool Galaxy) and NGC5195; Canes Venatici

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M51 (Whirlpool Galaxy) and NGC5195; Canes Venatici, Thomas V. Davis
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M51 (Whirlpool Galaxy) and NGC5195; Canes Venatici

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Description

M51 Whirlpool Galaxy and NGC5195; Canes Venatici

Astro Systeme Austria 12" f/3.5 astrograph

KAI-11000M; SBIG STL

Total Exposure: 7.5 hours (LRGB  120:90:120:120 minutes;  unbinned)

March-April 2008;  Inkom, ID

Comments: M51 was the first spiral structure ever observed by Lord Rosse in 1850 at a time when the true nature of galaxies was unknown. Its undeniable beauty explains its recognition as a true showpiece of the night sky. Probably less appreciated is that M51 represents a dramatic demonstration of an interacting pair of galaxies. As truly immense structures, galaxies are relatively large compared to the average distance between them. Most galaxies are separated by a distance of only 20 times their diameter compared to stars which are separated by 10 million times their diameter. As a result most galaxies are likely to encounter other galaxies at least a few times over their immense lifetimes. The encounters run the gamut from "major" mergers involving the collision of two comparable mass galaxies to more "minor" mergers involving the consumption of a small companion or satellite galaxy by the more dominant galaxy (Gendler).

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M51 (Whirlpool Galaxy) and NGC5195; Canes Venatici, Thomas V. Davis