M101 - The Pinwheel Galaxy


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Designations:
M101, NGC 5457, Pinwheel Galaxy
Object Type:
Spiral Galaxy
Constellation:
Ursa Major
14 hr 3.2 min
+54° 21 min
7.9
Size:
28.8 X 26.9 arcminutes
Distance:
17.5 million light years
Discoverer:
Pierre Mechain, 1781

Visual Description:

M101's numerous, far flung arms and distinct asymmetry make it readily identifiable in photographs. Visually, its pale 9th- magnitude glow is diffuse and difficult to make out, yet it has much to offer if you are patient. It is easy to locate, because you can star-hop to it from the famous visual double star Alcor and Mizar in the handle of the Big Dipper. Southeast of this pair is a path of four 5th- magnitude stars (81, 83, 84 and 86 Ursae Majoris) that leads in the direction of M101, which lies 1½° east-northeast of 86 Ursae at the end of the trail. The galaxy is visible in binoculars, so try them first before taking to the telescope. Telescopically, at 23 X the galaxy's core is compact but slightly elliptical. Knots in phantom spirals emerge from the galactic mists, but moderate power is much more effective in coaxing them out. Low power is best saved for determining the full extent of the far-flung arms. High power on the other hand, is your best bet for examining the inner region which shows a sharp nucleus inside a pentagon-shaped core. Only two arms are very definite; beyond that everything fades out of view. You may have to alternate between moderate and low power to preserve your sanity as you try to keep track of their directions.


Telescope:
Focal Length:
1200 mm
Mount:
Camera
Guider:
Exposures:
15 12-minute exposures for luminance and 4 15-minute exposures for each color (R,G,B). Total exposure time is 6-hours.
Location:
Heart of America Star Party south of Kansas City, MO
Software:
CCDSoft for image acquisition, processed with CCDStack and Photoshop CS2



The Visual description of M101 was written by Steven James O'Meara in the book "The Messier Objects" by Stephen James O'Meara. Page 265.
 ISBN number 0-521-55332-6.






Copyright(c) 2009 Doug Sanqunetti All rights reserved.

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