Other image sizes:  

1000 x 784 pixels

1600 x 1254 pixels

2400 x 1881 pixels

2400 x 1850 pixels (h-alpha only)

 

Rosette in Hubble Colors

 

    MAPPED COLOR - SII/Ha/OIII LIGHT

"WHEN ROSES AREN'T RED"
NGC 2244 - THE ROSETTE NEBULA in "HUBBLE" COLORS
Red = SII, Green = Ha, Blue = OIII
2 frame MOSAIC 

About this Image:  

No, this isn't a Hubble shot.  But this image was acquired and processed just like the gorgeous Hubble telescope images that we've come to love.  To accomplish this, the image was taken through specialized, narrowband emission line filters.  This information was then "mapped" to the traditional red, green, and blue channels of an RGB image.  The greenish portions of the image represent Hydrogen-alpha ionized gases., the bluish color represents doubly ionized Oxygen gases, and the reddish areas represent singly ionized Sulfur gases.  While the stars glow heavily in the sulfur wavelength, there is only a light concentration of it in the nebula, mostly throughout the brighter portions.

Such images, while obviously beautiful, have a real scientific purpose. Because the colors are mapped specifically to certain gases, it's easy to understand the concentrations of ionizations and how (where) they interact with each other.

Named NASA's Astronomy Picture of the Day for March 24, 2006...coined, "When Roses Aren't Red."  See it <here> on APOD.

To see this same data in CFHT-mapped colors, click
<here>
For NGC 2244 in regular RGB, click
<here>

Location:  Ballauer Observatory near Azle, Texas and Date: November, 2005 to January 2006
Seeing:
Varied
Transparency: Varied
Scope/Mount: 12.5" RCOS RC and Paramount ME
Camera: SBIG STL-6303e astro CCD camera
Filters: Custom Scientific 4.5nm Ha, OIII, and SII spectral line filters.
Exposure Info: Mapped color mosaic - SII/Ha/OIII - 90:210:60 minutes for left side and 90:150:90 minutes for right side (20 and 30 minute subexposures unbinned)
Processing Information:  Calibration, Registration, and DDP in CCDStack.  Color mapping, cropping, color balance, levels/curves, sharpening, and noise removal (Astronomy Tools/Pro Digital Software) in Photoshop CS.  

Exposure Notes:    The SII data is mapped to the red channel, Ha to green, and OIII to blue.  Seeing was exceptional for the left side of the mosaic, but poor for the right.  Interesting to note that despite similar conditions, the left side is much cleaner than the right side despite having less exposure time in Ha.


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