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	Click the image for a 70% 
	size, 4.95 
	arcsec/pixel display (1800 x 1200) 
	
		
			| 
			 Instrument  | 
			
			 
			Takahashi FSQ-106ED @ 
			f/5.0 (530 mm F.L.)  Captured at 3.5 arcsec/pixel.  Shown 
			resampled to 11.9 arcsec/pixel.  | 
		 
		
			| 
			 Mount  | 
			
			 Paramount ME  | 
		 
		
			| 
			 Camera  | 
			
			 SBIG STL-11000 w/ 
			internal filter wheel, AstroDon Filters  | 
		 
		
			| 
			 Acquisition Data  | 
			
			 
			1/11/2009 
			to 1/28/2009 Chino Valley... with CCDAutoPilot3  | 
		 
		
			| 
			 
			
			Exposure  | 
			
			 
			SII:Ha:OIII    
			45 min. (15 x 1 min. each filter, bin 1x1)  
			SII:Ha:OIII  225 
			min. (15 x 5 min.  each filter, bin 1x1)  
			SII:Ha:OIII  675 
			min. (15 x 15 min. each filter, bin 1x1) 
			 
			SII,Ha & OIII are mapped 
			to RGB respectivly.  An RGB overlay was added for the star 
			colors. 
			
			Click
			here for the natural colored image. 
			Click here for the B & W  Ha filtered 
			image.  | 
		 
		
			| 
			 
			
			Software  | 
			
			 CCDSoft, 
			CCDStack, Photoshop CS w/ the Fits Liberator plugin and Noel Carboni's actions. 
			CCDStack to calibrate, register, 
			normalize, data reject & combine sub exposures. 
			PhotoShop for 
			non-linear stretching and color combine.  | 
		 
		
			| 
			 
			Comment  | 
			
			 
			North is to the top. 
			This image was created 
			using the Hubble color palette. The colors  
			follow the spirit of the palette and the hydrogen (green), sulfur 
			(red) and oxygen (blue) areas can easy be identified. 
			 
			The Orion Nebula (also 
			known as Messier 42, M42, or NGC 1976) is a diffuse nebula situated 
			south of Orion's Belt. It is one of the brightest nebulae, and is 
			visible to the naked eye. M42 is located at a distance of 1,270±76 
			light years and is the closest region of massive star formation to 
			Earth. The M42 nebula is estimated to be 24 light years across. 
			Source:
			
			Wikipedia 
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