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Showing posts with label New Discovery. Show all posts
Showing posts with label New Discovery. Show all posts

Thursday, September 26, 2013

The Most Crowded Galaxy Discovered : 200 million Stars, only 54 million Light Years Away


Using the combined imaging capabilities of ground-based observatories with the high-flying Hubble Space Telescope and its cousin, the Chandra X-Ray Observatory, the ultra-compact dwarf galaxy known as M60-UCD1 turns out to be 15,000 times denser than what is found in our own galaxy, the Milky Way.



“Traveling from one star to another would be a lot easier in M60-UCD1 than it is in our galaxy, but it would still take hundreds of years using present technology,” said lead author of the new study, astronomer Michigan State University’s Jay Strader, in a press release.

What’s even more remarkable about M60-USD1 is that the galaxy’s most crowded part–its core, where half its 200 million solar masses resides–spans a radius of only 80 light years. That means the stars in this little galaxy are about 25 times closer to each other than those we find around the Sun’s galactic neighborhood.

Chandra observations have revealed that the galaxy’s tiny core harbors a strong x-ray source, which belongs to a giant black hole that weighs 10 million times the mass of our sun. That makes it about twice the size of the black hole in our own galaxy.
Astronomers theorize that a close encounter with a neighboring galaxy billions of years ago may have ripped away stars from M60-USD1 and may have led to the supermassive black hole pulling in the surviving stars close together.

“We think nearly all of the stars have been pulled away from the exterior of what once was a much bigger galaxy,” said co-author Duncan Forbes of Swinburne University in Australia in the press release.

“This leaves behind just the very dense nucleus of the former galaxy, and an overly massive black hole.”


Updated at: Thursday, September 26, 2013

Thursday, August 15, 2013

Carbyne: A new form of Carbon Stronger than Diamond or Graphene : Science Desk


The new material is called carbyne. It is a chain of carbon atoms that are linked either by alternate triple and single bonds or by consecutive double bonds.

The sixth element, carbon, has given us an amazing abundance of extraordinary materials. Once there was simply carbon, graphite and diamond. But in recent years chemists have added buckyballs, nanotubes and any number of exotic shapes created out of graphene, the molecular equivalent of chickenwire.

So it’s hard to believe that carbon has any more surprises up its sleeve. And yet today, Mingjie Liu and pals at Rice University in Houston calculate the properties of another form of carbon that is stronger, stiffer and more exotic than anything chemists have seen before.

The new material is called carbyne. It is a chain of carbon atoms that are linked either by alternate triple and single bonds or by consecutive double bonds.

Carbyne is something of a mystery. Astronomers believe they have detected its signature in interstellar space but chemists have been bickering for decades over whether they had ever created this stuff on Earth. A couple of years ago, however, they synthesised carbyne chains up to 44 atoms long in solution.

The thinking until now has been that carbyne must be extremely unstable. In fact some chemists have calculates that two strands of carbyne coming into contact would react explosively.

Nevertheless, nanotechnologists have been fascinated with potential of this material because it ought to be both strong and stiff and therefore useful. But exactly how strong and how stiff, no one has been quite sure.

This is where Liu and co step in. These guys have calculated from first principles the bulk properties of carbyne and the results make for interesting reading.

For a start, they say that carbyne is about twice as stiff as the stiffest known materials today. Carbon nanotubes and grapheme, for example, have a stiffness of 4.5 x 10^8 N.m/kg but carbyne tops them with a stiffness of around 10^9 N.m/kg.

Just as impressive is the new material’s strength. Liu and co calculate that it takes around 10 nanoNewtons to break a single strand of carbyne. “This force translates into a specific strength of 6.0–7.5×10^7 N∙m/kg, again significantly outperforming every known material including graphene (4.7–5.5×10^7 N∙m/ kg), carbon nanotubes (4.3–5.0×10^7 N∙m/ kg), and diamond (2.5–6.5×10”7 N∙m/kg4),” they say.

Carbyne has other interesting properties too. Its flexibility is somewhere between that of a typical polymer and double-stranded DNA. And when twisted, it can either rotate freely or become torsionally stiff depending on the chemical group attached to its end....




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Updated at: Thursday, August 15, 2013

Wednesday, August 14, 2013

Universe Is Not Expanding At All!, claims Scientist : Science Desk


Washington, July 18 (ANI): A cosmologist has proposed a radical theory, which claims that the Universe may not be expanding .

Washington, July 18 (ANI): A cosmologist has proposed a radical theory, which claims that the Universe may not be expanding .

Christof Wetterich, a theoretical physicist at the University of Heidelberg in Germany, devised a cosmology in which the universe doesn't expand but the mass of everything increases, the Huffington Post reported.

He said that such an interpretation could help physicists understand issues like the so-called singularity present at the Big Bang.

Though the paper is yet to be peer-reviewed, some experts have not dismissed it as wrong, and some even found the idea worth pursuing.

Hongsheng Zhao, a cosmologist at the University of St Andrews, UK, said that he believes it's fascinating to explore the alternative representation and Wetterich's treatment looks rigorous enough to be entertained.

Wetterich pointed out that the characteristic light emitted by atoms is also governed by the masses of the atoms' elementary particles, and in particular of their electrons.

He said that if an atom grows in mass, the photons, which it emits becomes more energetic.

Wetterich confessed that as higher energies correspond to higher frequencies, the emission and absorption frequencies move towards spectrum's blue part.

Conversely, if the particles become lighter, the frequencies get redshifted.

Because the speed of light is finite, when distant galaxies are looked at, we look backwards in time - seeing them as they would have been when they emitted the light that is being observed.

If all masses were once lower, and have been constantly increasing, the colours of old galaxies will look redshifted in comparison to current frequencies, and the amount of redshift is going to be proportionate to their distances from Earth.

Thus, the redshift will make galaxies seem to be receding even if they were not....




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Updated at: Wednesday, August 14, 2013

Tuesday, July 23, 2013

Science : Slow Down in Global Warming, not by much!


London: Global warming has not stopped, but is just on pause, according to scientists, who have revealed that the Earth's rate of warming has slowed down.

Huge amounts of heat - equivalent to the power of 150 billion electric kettles - are being continuously absorbed by the deep ocean, which could explain why global warming has "paused" over the past 10 to 15 years, the Independent reported.


Global average temperatures are higher now than they have ever been since modern records began.

However, after a period of rapid temperature increases during the 1980s and 1990s there has been a significant slow-down since the turn of the century, leading some sceptics to claim that global warming has stopped.

A scientific assessment of the planet's heat balance has found that the most likely explanation for the recent hiatus in global warming is the continual absorption of thermal energy by the huge "heat sink" of the deep ocean many hundreds of metres below the sea surface, according to scientists from the Met Office.

Senior climate scientists said that they had always expected periods when the rate of increase in temperatures would level off for a few years and emphasised that the last decade was still warmer than any previous decade, with 12 of the 14 hottest years on record occurring since 2000.

Professor Rowan Sutton, a climate scientist at Reading University, said the temperatures have levelled off in the past, the latest example being in the 1940s and 1950s when sulphate pollutants from the post-war boom in industrial production may have acted as a shield against incoming solar radiation.

The problem for the Met Office is to explain why the rate of increase in global temperatures has declined in recent years while concentrations of carbon dioxide in the atmosphere have continued to accelerate.

Sceptics claim that this shows there is not a strong link between the two, whereas climate scientists insist that rising carbon dioxide concentrations are largely responsible for the rise in global temperatures.

Professor Stephen Belcher, head of the Met Office Hadley Centre, said that a pause in the rate of increase in global temperatures lasting this long is unusual but not exceptional, with similar pauses of about 10 years expected on average twice every century...




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Updated at: Tuesday, July 23, 2013

Science : Dolphins Calls Each Other By Name!!


Scientists have found further evidence that dolphins call each other by "name".

Research has revealed that the marine mammals use a unique whistle to identify each other.

A team from the University of St Andrews in Scotland found that when the animals hear their own call played back to them, they respond.

The study is published in the Proceedings of the National Academy of Sciences.

Dr Vincent Janik, from the university's Sea Mammal Research Unit, said: "(Dolphins) live in this three-dimensional environment, offshore without any kind of landmarks and they need to stay together as a group.

"These animals live in an environment where they need a very efficient system to stay in touch."

Signature whistles

It had been-long suspected that dolphins use distinctive whistles in much the same way that humans use names.

Previous research found that these calls were used frequently, and dolphins in the same groups were able to learn and copy the unusual sounds.

But this is the first time that the animals response to being addressed by their "name" has been studied.

To investigate, researchers recorded a group of wild bottlenose dolphins, capturing each animal's signature sound...



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Updated at: Tuesday, July 23, 2013

Friday, July 19, 2013

Science : Curiosity suspects a massive collision killed Mars


Dual tests by instruments on the Curiosity rover, combined with data from the first Viking probes and Mars meteorites that have fallen to Earth, suggests that the Red Planet lost its atmosphere within the first billion years of its history, according to two papers in the latest issue of Science.

Curiosity's tunable laser spectrometer and quadrupole mass spectrometer, which make up part of Curiosity's Sample Analysis at Mars (SAM) laboratory, took separate readings of the Martian atmosphere to sort out the elements and measure the pattern of carbon, oxygen, and hydrogen isotopes, the papers report.

"As atmosphere was lost, the signature of the process was embedded in the isotopic ratio," said Paul Mahaffy of NASA Goddard Space Flight Center and the principal investigator for SAM and lead author of one of the two papers about Curiosity.

The results were compared with the very crude readings taken from the 1976 Viking probes and with analysis of the isotope variation found in meteorites that have been blasted off Mars by eruptions or impacts. The new data fits current climate models, and NASA says it's confident about the results.

"Getting the same result with two very different techniques increased our confidence that there's no unknown systematic error underlying the measurements," said Chris Webster of the lead investigator behind the tunable laser spectrometer. "The accuracy in these new measurements improves the basis for understanding the atmosphere's history."

Taken together, the data suggests that the atmosphere was lost from the top down, rather than by the interaction of the atmosphere with the Martian surface. This loss appears to have occurred before Mars made it to 10 figures-worth of birthdays, and has left it fairly barren place ever since...



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Updated at: Friday, July 19, 2013