Dates & Location |
April 20 - 28th 2009 from the SMAP
site at Weed, New Mexico. Elevation 7269 ft. Lat 32.8°N Long 195.5W |
Catalogue identification |
NGC 5194 - Large galaxy = M51 |
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Equipment Used | Officina Stellare
RC400 at 3304 mm focal length. |
Where it is in space |
In
the nonstellation of Canes Venatici,
North is to the right, East is up. |
|
Acquisition | Remote
session using RADMIN PC control from Ravenshead, UK.
LRGB exposures:- 120:70:70:60mins total, 10 min sub-exposures, |
What it is | The Whirlpool galaxy's spiral arms and dust clouds are the birth sites of massive and luminous stars. This galaxy is having a close encounter with a nearby companion galaxy, NGC 5195. The companion's gravitational influence is triggering star formation in the Whirlpool, as seen by the numerous clusters of bright, young stars which are ionising the clouds that they formed from (HII regions). The galaxy's massive core, the bright ball of light in the centre of the image, is about 80 light-years across (a light-year is 9.6 million million km or six million million miles) and has a brightness of about 100 million Suns. Astronomers estimate that it is about 400 million years old and has a mass 40 million times greater than our Sun. This concentration of stars is about 5,000 times higher than in our solar neighbourhood. |
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Processing Methods |
Images acquisition and telescope control with MaxIm DL V4.53 | |||
Data reduction and Luminence De-convolution with CCDStack. | ||||
Master RGB image and Master Lum Image finished with Photoshop CS2. |