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February 11th, 2009, 18:01 GMT · By

Groundbreaking Image Reveals the 'Cosmic Dawn'

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Scientists have used a computer simulation to predict what the very early Universe looked like 500 million years after the Big Bang
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Just today, researchers at the Durham University in the UK released the first computer model of how the Universe must have looked only 500 million years after the Big Bang, right at the time when the first stars and black holes began to take shape. The “Cosmic Dawn” is the name used to describe the formation of the first and earliest galaxies, which brought light in an otherwise pitch-black and cold space. Experts from the University's Institute for Computational Cosmology (ICC) have been behind the new simulation, and they hope that their design will help astrophysicists improve their level of knowledge and expertise on the elusive dark matter.

The calculations made by the ICC team also hint at the fact that the first galaxies were formed from the remnants of supermassive blue stars, which died explosively once they consumed their fuel. From the “ashes” of these enormous celestial bodies, galaxies started taking shape, as gas and dust were channeled to their central core on filaments of dark energy, according to some theories. At the same time, black holes formed from the same original stars, and they began to impose a circular motion to the objects that were gathered around them.

The new study, published in the journal Monthly Notices of the Royal Astronomical Society, and founded by the Science and Technology Facilities Council (STFC) and the European Commission, relies on a complex and very sophisticated computer model that accounts for everything, from the way structures would grow in dark matter to how regular matter such as gas behaves, which has allowed the machines to predict the development of galaxies.

“We are effectively looking back in time and, by doing so, we hope to learn how galaxies like our own were made and to understand more about dark matter. The presence of dark matter is the key to building galaxies – without dark matter we wouldn’t be here today,” Alvaro Orsi, an ICC research postgraduate and the lead author of the new paper, explains.

“Our research predicts which galaxies are growing through the formation of stars at different times in the history of the Universe, and how these relate to the dark matter. We give the computer what we think is the recipe for galaxy formation, and we see what is produced, which is then tested against observations of real galaxies,” ICC Royal Society Research Fellow Dr Carlton Baugh, who is also the co-author of the newly-published study, adds.

“Computational cosmology plays an important part in our understanding of the Universe. Not only do these simulations allow us to look back in time to the early Universe, but they complement the work and observations of our astronomers,” Chief Executive of the Science and Technology Facilities Council professor Keith Mason concludes.


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Comment #1 by: Rich Murray on 23 Feb 2009, 00:39 UTC reply to this comment

short introduction re viewing lovely subtle earliest structures in HUDF: AstroDeep, Rich Murray 2009.02.23

I've found since 2005 myriad ubiquitous bright blue sources, always on a darker fractal 3D web, along with a variety of sizes of irregular early galaxies, in the Hubble Ultra Deep Field, simply by increasing the gamma from 1.00 to 2.00 and saturating the colors, while minimizing the green band to simplify the complex overlays of complex fractal structures.

Dozens of these images, covering the entire HUDF in eight ~20 MB segments, are available for viewing at many scales [ To change the size of images on Windows PCs, use Control - and + ] on www.Flickr.com at the "rmforall" photostream. Try #86 for the central 20% of the HUDF.

ubiquitous bright blue 1-12 pixel sources on darker 3D fractal web in five 2007.09.06 IR and visible light HUDF images, Nor Pirzkal, Sangeeta Malhotra, James E Rhoads, Chun Xu, -- might be clusters of earliest hypernovae in recent cosmological simulations: Rich Murray 2008.08.17 2009.01.20
rmforall.blogspot.com/2008_08_01_archive.htm
Sunday, August 17, 2008
groups.yahoo.com/group/AstroDeep/25
groups.yahoo.com/group/rmforall/85

www.flickr.com/photos/rmforall/1349101458/in/photostream/

The 5 closeups are about 2.2x2.2 arc-seconds wide and high, about 70x70 pixels.
The HUDF is 315x315 arc-seconds, with N at top and E at left.
Each side has 10,500x10,500 pixels at 0.03 arc-second per pixel.

Click on All Sizes and select Original to view the highest resolution image of 3022x2496 pixels, which can be also be conveniently seen directly at their Zoomable image:

www.spacetelescope.org/images/html/zoomable/heic0714a.html

Notable in the deep background of the five closeups are ubiquitous bright blue sources, presumably extremely hot ultraviolet before redshifting, 1 to a dozen or so pixels, as single or short lines of spots, and a few irregular tiny blobs, probably, as predicted in many recent simulations, the earliest massive, short-lived hypernovae, GRBs with jets at various angles to our line of sight, expanding bubbles, earliest molecular and dust clouds with light echoes and bursts of star formation, and first small dwarf galaxies, always associated with a subtle darker 3D random fractal mesh of filaments of H and He atomic gases.

As a scientific layman, I am grateful for specific cogent, civil feedback, based on the details readily visible in images in the public domain.

www.spacetelescope.org/images/html/heic0714a.html

Hubble and Spitzer Uncover Smallest Galaxy Building Blocks

Rich Murray, MA Room For All rmforall@comcast.net 505-501-2298
1943 Otowi Road, Santa Fe, New Mexico 87505
groups.yahoo.com/group/rmforall/messages
groups.yahoo.com/group/AstroDeep/messages
www.sfcomplex.org Santa Fe Complex

You are welcome to visit me and share your comments as I share these images at home on a 4X8 foot screen -- no fee.

Anyone may view and download for free 91 images, presenting the HUDF in eight 20 MB pieces at rmforall at www.FlickR.com -- #86 is about 20% of the HUDF in their red and blue colors, as leaving out the green greatly simplifies interpreting the overlapping layers of transparent fractal webs of gas with a wide range of sizes of rather distant sources, beyond z = 5.

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