Eyepiece Simulations |
Diffuse Nebula M-42 (NGC-1976)
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ABOUT THE IMAGES:PICTURE NO. 1 (left): Drawing of M-42 by Jaakko Saloranta, done with the aid of an 8" f/4.5 Dobsonian scope. He has outlined the farthest extent of the nebulosity he could see. Waldee has inverted the picture for a negative view. PICTURE NO. 2 (middle left): M-42 looks very much like this in author Waldee's similar 8" f/5.2 Newtonian scope, using low power with a wide-field ocular and a 6mm exit pupil, at a naked eye stellar limit of about 5th magnitude, with some light pollution. An effort was made to include the four brightest members of the Trapezium. PICTURE NO. 3 (middle right): If a hydrogen/oxygen-line general narrowband nebular filter (UHC type) is added, fainter nebulosity and higher contrast are obtained in the central "bowl" of the nebula, at the expense of some dimming of the stars. If an O-III filter is used, the large, faint outer halo of nebulosity may sometimes be glimpsed. PICTURE NO. 4 (far right): Made with Ron Wood's home-built 8" f/5.2 photographic scope, this image is in spectacular color from his prime focus exposure of 30 minutes, using a Newtonian off-axis guider and LPR filter, with forming-gas-hypered Kodak Ektapress 1600 film. |
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Last Edited: Thursday 8 March 2007 at 5:02 pm. Copyright © 1996-2007 Regina L. Roper & Stephen R. Waldee - All Rights Reserved. All Trademarks or Copyrights are © or Property of Their Respective Copyright Holders.Copyright statement: permission is not granted for reprinting these articles anywhere else. Aside from brief quotes of a few sentences allowed under "fair use" permissions that may be allowed by copyright law, we do not sanction the use of these articles on other websites or in newsletters, or on CD-ROM drive astronomy compilations. You may link to this page or to the individual articles.