The Whirlpool Galaxy

 
Messier Object 51, The Whirlpool Galaxy
 
 

 

Image Information
Date Imaged

05/28/2009

Location Imaged From

Barking Pumpkin Observatory


Mt Wilson, CA

Equipment Telescope: 18"RC
Mount: Unknown
Camera: SBIG STL-6303
Focal Ratio: f/8.1
Exposure Information

LRGB - 100:40:40:40

Eric Edegaard approach our group asking for help in processing the data he obtained from the 18" RC at Mt Wilson. This is my attempt . I wasn't able to bring out the blues as well as I've seen in other images, but this is a learning process.

The Whirlpool Galaxy (also known as Messier 51a, M51a, or NGC 5194) is an interacting grand-design spiral galaxy located at a distance of approximately 23 million light-years in the constellation Canes Venatici. It is one of the most famous spiral galaxies in the sky. The galaxy and its companion (NGC 5195) are easily observed by amateur astronomers, and the two galaxies may even be seen with binoculars. The Whirlpool Galaxy is also a popular target for professional astronomers, who study it to further understand galaxy structure (particularly structure associated with the spiral arms) and galaxy interactions.

The Whirlpool Galaxy was discovered by Charles Messier on October 13, 1773. Its companion galaxy, NGC 5195, was discovered in 1781 by Pierre Méchain. It was however not until 1845 that the Whirlpool became the first galaxy to be recognized as a spiral. This was achieved by Lord Rosse employing a 72-inch reflecting telescope which he constructed at Birr Castle, Ireland. In 2005 a supernova (SN 2005cs) was observed in the Whirlpool Galaxy, peaking at apparent magnitude 14. Sometimes M51 is used to refer to the pair of galaxies, in which case the individual galaxies may be referred to as M51A (NGC 5194) and M51B (NGC 5195).