Object Information:

 

 M51 (NGC 5194)  "Whirlpool Galaxy"
 Mag. -   8.4
 Constellation - Canes Venatici
 Location -  R.A. 13:29.9,  Dec. 47.12
 Size - 124,000 light years across (estimated),
 Distance -  37 million light years (estimated),

 

Messier 51, also known as NGC 5194, is a star party favorite and has an interesting history.  First observed by Charles Messier in October 1773, the spiral structure was not noted until 1845 by Lord Rosse.  At the time of the discovery of the spiral structure, it was thought that Messier 51 was an example of a new solar system in formation within our Milky Way Galaxy.  It was not until 1923 with the construction of larger, more powerful telescopes that  Messier 51 was recognized as a distinct galaxy with its own stars and nebulae.  Also shown in the above image is Messier 51's companion galaxy, NGC 5195.  Although some have theorized that the two galaxies are connected.  It is now generally recognized that they are two separate and distinct galaxies.  However, it is believed that the prominent spiral structure of Messier 51 is due to its gravitational interaction with NGC 5195.

 

Messier 51 can be spotted with binoculars under a dark country sky.  However, hints as to its spiral structure can only be detected under dark skies with telescopes of 8" and larger.

  Imaged at: 

 

Desert Center, Riverside County, California.

  Equipment:  

 

Optics - Takahashi MT-200 8" classical Newtonian at f/6.0
Mount - Astro-Physics 1200 GTO,
Camera - Santa Barbara Instrument Group (SBIG) ST-10XME CCD,

  Exposure Information:

 

A combination of 14 separate 6 minute images for a total exposure time of 84 minutes for the monochrome image.

 

The color image is a combination of a 2002 LRGB image with the MT-160 and an ST-7E NABG and a cropped portion of the monochrome image above.  The old and new images were aligned with RegiStar.

  Camera Control Software:

 

MaxIm DL Ver. 4.06

  Image Processing Software:

 

Mira 7, Photoshop 8