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May 2012 - We passed one million page views - thanks and Join already :-) September 2010 I am pleased to report that my essay titled A NEW METRIC WITH APPLICATIONS TO PHYSICS AND SOLVING CERTAIN HIGHER ORDERED DIFFERENTIAL EQUATIONS' has been published by Physics Essays published by the American Institute of Physics and appeared in their June 2010 quarterly. 40 years ago I took an honors degree in applied mathematics from the University of Waterloo. My interest was Relativity and my last year there saw me complete a 900 level course under Hanno Rund on his work in relativity,as well as differential geometry(pure math) and of course analysis. I continued researching new ideas and knowledge since that time and I have prepared a book for publication titled 'Paradigms Shift'. I maintain my blog as a day book and research tool to retain data and record impressions and interpretations on material read. Do take this moment to join my blog and receive Four items of interest daily Monday through Saturday. Since my topics are usually unique or at least obscure, the ads running through adsense are often interesting and worth dipping into while also supporting this blog in a small way.

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Friday, July 2, 2010





Neat image here to add to the steadily increasing collection of pictures of the sky.

Beautiful New Image of a Rare Blue Nebula


This wispy blue cloud of gas and dust is a star-forming region surrounding the star R Coronae Australis, which is about 420 light-years away. The new portrait was taken with the Wide Field Imager at the La Silla Observatory in Chile. The image, a combination of 12 separate snapshots in three different colors, depicts a young family of stars still embedded in and interacting with the cloud of dust and gas from which they formed.
The image spans about 4 light-years, and focuses on a nascent star-forming region located in the small, tiara-shaped constellation Coronae Australis, the Southern Crown. The infant stars there give off hot, intense radiation, and the surrounding gas and dust either reflects or absorbs this radiation and re-emits it at a different wavelength.
While most nebulae glow with a characteristic red tint, the R Coronae Australis region takes an unusual blue hue. The stars are about the mass of the sun, and don’t emit enough ultraviolet light to strip the surrounding hydrogen gas of its electrons, which would produce the familiar red glow. The blue fog is mostly due to starlight reflecting off small dust particles.
In some regions, like the dark band that crosses the image from the bottom left, the starlight is completely absorbed by dust. Any stars hiding in this region would only be visible with an infrared telescope that can detect their heat.
High-resolution versions of the image are here.


Read More http://www.wired.com/wiredscience/2010/06/blue-nebula/#ixzz0sWL9G073





And another image



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