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Todd Suomela

Technology Review: Blogs: arXiv blog: Why ET's genetic code could be just like ours - 0 views

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    "The combined actions of thermodynamics and subsequent natural selection suggest that the genetic code we observe on the Earth today may have significant features in common with life throughout the cosmos."
Sandra Flores

Why Video Marketing - 0 views

IF YOU ARE NOT Using the video marketing Channel SO YOU YOU ARE MISSING the most cost effective chanNel right nOw .want to see real NUMBERS ? TAKE A LOOK AT THIS PROFESSIONAL VIDEO MARKETING INFO-G...

started by Sandra Flores on 05 Jan 15 no follow-up yet
Sandra Flores

Why Video Marketing - 0 views

IF YOU ARE NOT Using the video marketing Channel SO YOU YOU ARE MISSING the most cost effective chanNel right nOw .want to see real NUMBERS ? TAKE A LOOK AT THIS PROFESSIONAL VIDEO MARKETING INFO-G...

started by Sandra Flores on 09 Jan 15 no follow-up yet
Janos Haits

Cosmos Portal - 2 views

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    Cosmos Portal  is a gateway on the Web to astronomy and space science. We invite astronomy professionals to publish articles, blogs, news items, image galleries, videos, class notes, lectures, powerpoint presentations, links to other high quality websites or other educational material. 
Todd Suomela

Lifeboat News: The Blog » The 'Sustainability Solution' to the Fermi Paradox - 0 views

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    The Sustainability Solution states: the absence of ETI observation can be explained by the possibility that exponential or other faster-growth is not a sustainable development pattern for intelligent civilizations.
Todd Suomela

Reclaiming the Nighttime Sky - Environment and Energy - 0 views

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    On the International Dark Sky Association starting to lobby Washington D.C.
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    Will 2009 be the year the federal government finally takes light pollution seriously?
Todd Suomela

the physics arXiv blog » Blog Archive » The puzzle of planet formation - 0 views

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    "At the heart of the problem is the fascinating question: why are all the planets different? The ones in our solar system ought to have formed out of the same stuff at more or less the same time and yet no two are alike. And now the extrasolar planets seem to be demonstrating a similar variety."
Sandra Flores

Choosing the right channel of Marketing. - 0 views

There are so many ways of advertising and reaching out to the right people/ the las word is inbound marketing.The Digital marketing comes in all shapes and sizes, but often the runt of the litter i...

started by Sandra Flores on 05 Jan 15 no follow-up yet
anees_100

Everyday Science | Learn Facts about Daily Life| Blogs and Articles - 0 views

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    Everyday Science explores science concepts from everyday and beyond. Read these interesting articles and learn daily new facts about science and technology.
Janos Haits

collectSPACE - space history, space memorabilia, space artifacts, and space collectibles - 0 views

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    The Source for Space History and Artifacts
Janos Haits

SpaceCollective - 1 views

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    "Space Collective.org is a cross-media information and entertainment channel for post-ideological, non-partisan, forward thinking terrestrials. © 2006-2014 SpaceCollective. "
Todd Suomela

FQXi Community: Articles, Forums, Blogs, News - Judgment Day at the End of Time (the Es... - 0 views

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    list of winning essays for the Foundational Questions in Physics and Cosmology Institute
Todd Suomela

Astronomers Crowdsource the Definition of a Galaxy - Technology Review - 2 views

  • So what to do? Today, Duncan Forbes at Swinburne University in Australia and Pavel Kroup at the University of Bonn in Germany put forward a novel solution. They outline the various characteristics that astronomers think about when classifying galaxies. These include factors such as the presence of stars, so gas clouds can't be defined as galaxies; being gravitationally bound, so materials that has been stripped away by another galaxy wouldn't count; whether the system is stable or not; whether it hosts a good variety of different types of star, which excludes globular clusters which contain only similar stars; and whether it is held together by dark matter, which many galaxies seem to be. There are other factors too, of course. (Although they do not include the presence of a black hole at the centre of a galaxy as a defining characteristic , which is odd given the growing interest in the link between galactic evolutoin and black holes.) Forbes and Kroup go on to suggest that the best way to achieve consensus is to crowdsource the problem. In other works, they want to use the wisdom of the crowd to determine what factors are important what aren't.
Todd Suomela

Guest Post: Evalyn Gates on Cosmic Magnification (or - Invasion of the Giant Blue Space... - 0 views

  • This is not just a pretty picture, however – the image packs a lot of scientific information. The authors extract the mass distribution in the cluster (which has implications for cosmological models), measure the mass-to-light ratio of the bright galaxy in the center of the cluster, and use the magnifying power of the lens to search for even more distant galaxies. The basic idea is to construct a model of the lens, starting with the cluster galaxies and a dark matter halo; then refine the model to reproduce the multiple images that are seen. Using this refined model it’s possible to predict the location of additional images of a given source, and to identify regions of high magnification that can then be examined for multiple images of other sources. Any additional images that are found can be used to further refine the model and so on.
  • This galaxy has been lensed by the warp in spacetime created by the cluster. Light from the galaxy, which lies almost directly behind the center of the cluster but much farther away from us, travels along several curved paths through the cluster lens, producing multiple magnified images of the galaxy. The inset box shows a computer generated model of the unlensed source galaxy, enlarged by a factor of four so that the details, including the spiral arm structure, are visible. Without the lensing power of the cluster, we would see this galaxy as a single small blue smudge. In general, lensing will both magnify and distort (shear) images of a background source. This lens is fairly unique in that we see large but relatively intact images of the spiral galaxy, which implies that the mass distribution in the central region of the cluster must be nearly uniform.
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