Site hosted by Build your free website today!









Part of the Nebula (also known as NGC 3372) around the star Eta Carinae.

This giant diffuse nebula is one of the largest H II regions (ionized hydrogen gas) in our galaxy.  Eta Carinae itself is a very peculiar star, having varied widely in brightness in the past.  At one time in 1843, it was the brightest star in the sky after Sirius.  It is thought to be among the most massive and luminous stars in our Milky Way, at more than 100 solar masses.


Image info

Telescope:  Orion 80ED apochromatic refractor at f/7.5

Focus:  Prime focus

Filter:  Astronomik Hydrogen Alpha 13nm FWHM, Astronomik RGB.

Mount:  Vixen GPD with Skysensor2000

Camera:  Artemis 285 CCD camera

Guiding:  700mm refractor guidescope, SAC7 camera, autoguided with Guidedog software

Exposure:  Total 105 mins (15 x 420s) L, 30, 25, 40 mins R,G,B.

Date:  4th Feb, 3rd March 2006

Processing:  Offset and flat fielding, registering and stacking done in IRIS.  No dark frames.  Curve stretching,  Levels, Smart Sharpen in Photoshop CS2.  Luminance layering with the RGB.




Copyright 2003 to 2014, by TG Tan.  All rights reserved.  Copyright exists in all original material available on this website.  This material is for your personal individual, nonprofit use only.  Redistribution and/or public reproduction of this material is strictly prohibited without prior express written permission from the author.