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Thursday, April 10, 2008

Scientists Find A Fingerprint Of Evolution Across The Human Genome


DNA double helix. Researchers have found signs that evolution rejects some types of mutations even in these regions of the genome. (Credit: NIH/National Human Genome Research Institute)

The Human Genome Project revealed that only a small fraction of the 3 billion “letter” DNA code actually instructs cells to manufacture proteins, the workhorses of most life processes. This has raised the question of what the remaining part of the human genome does. How much of the rest performs other biological functions, and how much is merely residue of prior genetic events?

Scientists from Cold Spring Harbor Laboratory (CSHL) and the University of Chicago now report that one of the steps in turning genetic information into proteins leaves genetic fingerprints, even on regions of the DNA that are not involved in coding for the final protein. They estimate that such fingerprints affect at least a third of the genome, suggesting that while most DNA does not code for proteins, much of it is nonetheless biologically important – important enough, that is, to persist during evolution.

Conservation of genetic information

To gauge how critical a particular stretch of DNA is, biologists often look at the detailed sequence of “letters” it consists of, and compare it with a corresponding stretch in related creatures like mice. If the stretch serves no purpose, the thinking goes, the two sequences will differ because of numerous mutations since the two species last shared an ancestor. In contrast, it’s believed that the sequences of important genes will be similar, or “conserved,” in different species, because animals with mutations in these genes did not survive. Biologists therefore regard conserved sequences as a sign of biological importance.

To test for conservation, researchers need to find matching stretches in the two species. This is relatively easy for stretches that “code” for proteins, where scientists long ago learned the meaning of the sequence. For “noncoding” regions, however, the comparison is often ambiguous. Even within a gene, stretches of DNA that code for pieces of the target protein are usually interspersed with much larger noncoding stretches, called introns, that are removed from the RNA working copy of the DNA before the protein is made.

Signs of splicing

Previous researchers assumed that mutations in the middle of introns do not affect the final protein, so they simply accumulate. In the new work, however, the researchers found signs that evolution rejects some types of mutations even in these regions of the genome. Although the selection is weak, “introns are not neutral,” in their effect on survival, says CSHL professor Michael Zhang, a bioinformatics expert who headed the research team.

To look for selection, CSHL researcher Chaolin Zhang, a doctoral candidate at Stony Brook University, looked in the human genome for a subtle statistical imbalance in how often various “letters” appear. The researchers attribute this imbalance to special short stretches of DNA that mark regions to be removed. Unless these signal sequences are sprinkled throughout an intron, the data suggest, it may not be properly spliced out, with potentially fatal consequences. Other sequences must likewise be preserved in the regions to be retained.

The scientists found a preference for some “letters” across intron regions, and the opposite preference in coding regions. Together, these regions make up at least a third of the genome, which is thus under selective pressure during evolution. The result supports other recent studies that suggest that, although most DNA does not code for proteins, much of it is nonetheless biologically important.

In addition to demonstrating how splicing affects genetic evolution, the statistical analysis identified possible signaling sequences, some that were already known and others that are new. According to co-author Adrian Krainer, a CSHL professor and splicing expert, “the exciting thing will be to experimentally test whether these predicted elements are really true.”

Original here


Wednesday, April 9, 2008

Rare Quasar Discovered That Produces More X-rays Than Thought Possible


Artist's impression of a rare type of quasar, called a broad absorption line (BAL) quasar. Quasars are vast cosmic engines that pump energy into their surroundings. It is thought an enormous black hole drives each quasar. (Credit: ESA, Image by C. Carreau)

XMM-Newton has been surprised by a rare type of galaxy, from which it has detected a higher number of X-rays than thought possible. The observation gives new insight into the powerful processes shaping galaxies during their formation and evolution.

Scientists working with XMM-Newton were looking into the furthest reaches of the universe, at celestial objects called quasars. These are vast cosmic engines that pump energy into their surroundings. It is thought an enormous black hole drives each quasar.

As matter falls into the black hole, it collects in a swirling reservoir called the accretion disc, which heats up. Computer simulations suggest that powerful radiation and magnetic fields present in the region eject some of gas from the gravitational clutches of the black hole, throwing it back into space.

This outflow has a profound effect on its surrounding galaxy. It can create turbulence in the gas throughout the galaxy, hampering star formation. Thus, understanding quasars is an important step to understanding the early history of galaxies.

However, the structure surrounding a quasar is difficult to see because they are so distant. The light and X-rays from them takes thousands of millions of years to reach us.

About 10-20% of quasars are of a special type called BAL quasars. The BAL stands for ‘broad absorption line’ and seems to indicate that a thick cocoon of gas surrounds the quasar.

Most researchers believe that gas flows away from a BAL quasar along the equatorial direction of the accretion disc. These quasars show little X-ray emission, indicating that there is enough gas to absorb most of the X-rays given out from the region near the black hole.

But some BAL quasars appear to be spewing material out along their polar axes, at right angles to the accretion discs.

JunXian Wang, Center for Astrophysics, University of Science and Technology of China, Hefei, and his colleagues including Tinggui Wang and Hongyan Zhou, used XMM-Newton to target four such polar BAL quasars, identified by them previously. They were investigating whether the X-rays were being absorbed strongly.

XMM-Newton observed the quasars at specific times during 2006 and 2007. Two of them emitted more X-rays than the researchers anticipated, indicating that there is no veil of absorbing gas surrounding these particular quasars. “Our results can help refine the computer simulations of how these quasars work,” says Wang.

It may mean that BAL quasars are more complicated than originally thought. “Perhaps there can be both equatorial outflows and polar outflows simultaneously from these objects,” says Wang. Maybe, the outflows are even produced by similar means.

Computer simulations suggest that the polar outflows, like the gas ejected from the accretion disc, are also material falling in, turned away by fierce radiation before it comes near the black hole.

Wang and colleagues are now following this work up. They hope to monitor more BAL quasars over a longer period of time. “We need more data so that we can look into the details of the X-ray emission,” says Wang.

It seems that the more astronomers look into the distant universe, the more complex it becomes.

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Do We Have the 'Right Stuff' to Put an Astronaut on Mars?

Mars_2_3_2 "All civilizations become either spacefaring or extinct."

Carl Sagan

It only took eight years for JFK’s dream to land a man on the moon to be fulfilled, but plans to to land a man on Mars is going to take just that little bit longer -24 years to be exact, but at least we know how we’re going to go about getting our astronauts there.


NASA is serious about launching the most difficult mission ever attempted by the human race - putting an astronaut on Mars. The voyage will cover hundreds of millions of miles and take two and half years roundtrip. It sounds like science fiction. To make it scientific fact, the United States needs to first flex its deep space muscles again on familiar terrain - the moon. It's called the Constellation program.

"The accuracy with which you need to target a landing site on the surface is like throwing a basketball from New York to Los Angeles and having it go through without touching the rim," explains Steve Squyres, the principal investigator for the Mars rovers Spirit and Opportunity..

If the astronauts actually that shot, and if they land on Mars, they will face a deadly environment - radiation from solar flares, dangerous dust and temperatures that average 60 degrees below zero. And they’ll have to do it for up to 18 months, before the Earth and Mars align properly again for a faster return home. No astronauts have ever spent that amount of time on an alien world. Neil Armstrong was on the moon for less than a day.

"And I think it’s more responsible for us to go to the moon, check out these systems, make sure the life-support systems, the space suits, the little things we need for these long voyages, work properly," explains Dr. Rick Gilbrech is NASA’s exploration chief.

During Apollo, the furthest the astronauts could ever venture out on their lunar rovers was six miles. NASA hopes the new rovers will let the astronauts explore 60 miles from their spacecraft. Technological advancements will help in another way. Think about this: There is more computing power in your average cell phone today than there was on any of the Apollo spacecraft that took the astronauts to the moon.

Another example of how the new missions might be different is the robonaut, which looks like a cousin of C-3PO. It’s an early model of a robot that might assist the astronauts with mundane and sometimes dangerous tasks on the moon.

NASA isn’t using the moon just to train for Mars. Next year, it will launch orbiters around the moon and then essentially blast the lunar surface. In the midst of the debris field, NASA hopes to find evidence of hydrogen, which could one day help fuel trips home for the astronauts. But will there be any missions for the astronauts at all?

The biggest obstacle NASA faces is money. One critic has called the Constellation program "Apollo on food stamps." During the 1960s, 4 percent of the entire national budget was spent on space. Today one-sixth of 1 percent goes to NASA.

Thanks to some new details released by NASA for their new Constellation manned Mars mission, we now have an insight in to what the missions will look like.

A 400,000kg (880,000lb) spacecraft would be constructed, in space. Due to the necessity of a craft that can act autonomously of NASA control, make the distance, and provide for its crew for a 900 day mission, the size of the ‘marscraft’ is obviously going to exceed that of the current space shuttles.

It would take three to four Ares V rockets to launch the elements of the spacecraft in to a low Earth orbit.

A ‘minimal crew’ would make the journey to Mars, taking approximately six to seven months to traverse the distance. A total of 550 days would be spent on the surface of Mars, before returning. Sent every 26 months to the red planet, the crews would need to take up to 50,000kg of cargo with them. They’d need an ‘aerodynamic and powered descent’ and autonomy or at least asynchronous from NASA control.

However, sending the crew is not the only part of this mission. Where are they going to live? How will all their equipment make the journey? That’s why their mission will be preceded by two separate missions.

With a theoretical launch date for the manned mission to Mars arriving in February of 2031, a cargo lander and surface habitat would be launched December 2028 and January 2029, respectively using two Ares V launches. Subsequently, the launder will arrive October 2029, and the habitat a month later; the crew will arrive August 2031.

The second set of pre-launches will occur in late 2030/early 2031, and anticipated to reach Mars at the same time as the first crew. Thus, in the first quarter of 2033, the second mission’s crew will launch to arrive on Mars by December, with the first crew having left January that same year, after a 17-month stay.

Will we see human settlements on Mars? Or is it all just a dream? Will the American public even support traveling to places humans can barely imagine?

Posted by Josh Hill with Casey Kazan.

Original here