jueves, 2 de agosto de 2012


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Stanley Miller and the Quest to Understand Life’s Beginning




Thursday 26th July saw the launch of SciLogs.com, a new English language science blog network. SciLogs.com, the brand-new home for Nature Network bloggers, forms part of the SciLogs international collection of blogs which already exist inGermanSpanish and Dutch. To celebrate this addition to the NPG science blogging family, some of the NPG blogs are publishing posts focusing on “Beginnings.”Participating in this cross-network blogging festival is nature.com’s Soapbox Science blogScitable’s Student Voices blog and bloggers from SciLogs.com, SciLogs.deScitable and Scientific American’s Blog Network. Join us as we explore the diverse interpretations of beginnings – from scientific examples such as stem cells to first time experiences such as publishing your first paper. You can also follow and contribute to the conversations on social media by using the #BeginScights hashtag. – Bora
In the spirit of “beginnings,” I’m serving up this lightly edited excerpt from The End of Science (1996) on life’s origin, which–tellingly–has not been rendered obsolete by any subsequent research.– John Horgan
One of the 20th century’s most diligent and respected origin-of-life researchers is Stanley Miller. He was a 23-year-old graduate student in 1953 when he sought to recreate the origin of life in a laboratory. He filled a sealed glass apparatus with a few liters of methane, ammonia and hydrogen (representing the atmosphere) and some water (the oceans). A spark-discharge device zapped the gases with simulated lightning, while a heating coil kept the waters bubbling. Within a few days, the water and gases were stained with a reddish goo. On analyzing the substance, Miller found to his delight that it was rich in amino acids. These organic compounds are the building blocks of proteins, the basic stuff of life.
Miller’s results seemed to provide stunning evidence that life could arise out what the British chemist J.B.S. Haldane had called the “primordial soup.” Pundits speculated that scientists, like Mary Shelley’s Dr. Frankenstein, would shortly conjure up living organisms in their laboratories and thereby demonstrate in detail how genesis unfolded. It hasn’t worked out that way. In fact, almost 40 years after his original experiment, Miller told me that solving the riddle of the origin of life had turned out to be more difficult than he or anyone else had envisioned. He recalled one prediction, made shortly after his experiment, that within 25 years scientists would “surely” know how life began. “Well, 25 years have come and gone,” Miller said drily.
After his 1953 experiment, Miller had dedicated himself to the search for the secret of life. He developed a reputation as both a rigorous experimentalist and a bit of a curmudgeon, someone who is quick to criticize what he feels is shoddy work. When I met Miller in 1990 in his office at the University of California at San Diego, where he is a professor of biochemistry, he fretted that his field still has a reputation as a fringe discipline, not worthy of serious pursuit.
“Some work is better than others,” he said. “The stuff that is awful does tend to drag it down. I tend to get very upset about that. People do good work, and then you see this garbage attract attention.” In fact, Miller seemed unimpressed with any of the current proposals on the origin of life, referring to them as “nonsense” or “paper chemistry.” He was so contemptuous of some hypotheses that, when I asked his opinion of them, he merely shook his head, sighed deeply and snickered–as if overcome by the folly of humanity. Stuart Kauffman’s theory of “autocatalysis” fell into this category. “Running equations through a computer does not constitute an experiment,” Miller sniffed.
Miller acknowledged that scientists may never know precisely where and when life emerged. “We’re trying to discuss an historical event, which is very different from the usual kind of science, and so criteria and methods are very different,” he remarked. But when I suggested that Miller sounded pessimistic about the prospects for discovering life’s secret, he looked appalled. Pessimistic? Certainly not! He was optimistic!
One day, he vowed, scientists would discover the self-replicating molecule that triggered the great saga of evolution. Just as the discovery of the microwave radiation pervading space legitimized cosmology, so would the discovery of the first genetic material legitimize Miller’s field. “It would take off like a rocket,” Miller muttered through clenched teeth. Will such a discovery be immediately self-apparent? Miller nodded. “It will be in the nature of something that will make you say, ‘Jesus, there it is. How could you have overlooked this for so long?’ And everybody will be totally convinced.”
When Miller performed his landmark experiment in 1953, most scientists still shared Darwin’s belief that proteins were the likeliest candidates for self-reproducing molecules, since proteins were thought to be capable of reproducing and organizing themselves into cells. After the discovery that DNA is the basis for genetic transmission, many researchers began to favor nucleic acids over proteins as the ur-molecules. But there was a major hitch in this scenario. DNA can make neither proteins nor copies of itself without the help of catalytic proteins called enzymes. This fact turned the origin of life into a classic chicken-or-egg problem: Which came first, proteins or DNA?
In the 1960s the molecular biologist Gunther Stent proposed that this conundrum could be solved by a self-replicating molecule that could act as its own catalyst. In the early 1980′s, researchers identified just such a molecule: ribonucleic acid, or RNA, a single-strand molecule that serves as DNA’s helpmate in manufacturing proteins. Experiments revealed that certain types of RNA could act as their own enzymes, snipping themselves in two and splicing themselves back together again. If RNA could act as an enzyme then it might also be able to replicate itself without help from proteins. RNA could serve as both gene and catalyst, egg and chicken.
But the so-called “RNA-world” hypothesis suffers from several problems. RNA and its components are difficult to synthesize under the best of circumstances, in a laboratory, let alone under plausible prebiotic conditions. Once RNA is synthesized, it can make new copies of itself only with a great deal of chemical coaxing from the scientist. The origin of life “has to happen under easy conditions, not ones that are very special,” Miller said. He is convinced that some simpler–and possibly quite dissimilar–molecule must have paved the way for RNA.
Lynn Margulis, for one, doubts whether investigations of the origin of life will yield the kind of simple, self-validating answer that Miller dreams of. “I think that may be true of the cause of cancer but not of the origin of life,” Margulis said when I spoke to her in 1994. Life, she pointed out, emerged under complex environmental conditions. “You have day and night, winter and summer, changes in temperature, changes in dryness. These things are historical accumulations. Chemical systems are effectively historical accumulations. So I don’t think there is ever going to be a packaged recipe for life: add water and mix and get life. It’s not a single step process. It’s a cumulative process that involves a lot of changes.”
The smallest bacterium, she noted, “is so much more like people than Stanley Miller’s mixtures of chemicals, because it already has these system properties. So to go from a bacterium to people is less of a step than to go from a mixture of amino acids to that bacterium.”
Francis Crick once wrote that “the origin of life appears to be almost a miracle, so many are the conditions which would have to be satisfied to get it going.” (Crick, it should be noted, is an agnostic leaning toward atheism.) Crick proposed that aliens visiting the earth in a spacecraft billions of years ago may have deliberately seeded it with microbes.
Perhaps Stanley Miller’s hope will one day be fulfilled: scientists will find some clever chemical or combination of chemicals that can reproduce, mutate and evolve under plausible prebiotic conditions. The discovery is sure to launch a new era of applied chemistry. (The vast majority of researchers focus on this goal, rather than the elucidation of life’s origin.) But given our lack of knowledge about the conditions under which life began, any theory of life’s origin based on such a finding will always be subject to doubts. Miller has faith that biologists will know the answer to the riddle of life’s origin when they see it. But his belief rests on the premise that the answer will be plausible, if only retrospectively. Who said the origin of life on earth was plausible? Life might have emerged from a freakish convergence of improbable and even unimaginable events.
Moreover, the discovery of a plausible ur-molecule, when or if it happens, is unlikely to tell us what we really want to know: Was life on earth inevitable or a freak occurrence? Has it happened elsewhere or only in this lonely, lonely spot? These questions can only be resolved if we discover life beyond the earth. Society seems increasingly reluctant to underwrite such investigations. In 1993, Congress shut down NASA’s SETI (Search for Extraterrestrial Intelligence) program, which scanned the heavens for radio signals generated by other civilizations. The dream of missions to Mars–manned or otherwise–is growing fainter.
Even so, scientists may find evidence of life beyond the earth tomorrow. Such a discovery would transform all of science and philosophy and human thought. Stephen Jay Gould and Richard Dawkins might be able to settle their argument over whether natural selection is a cosmic or merely terrestrial phenomenon (although each would doubtless find ample evidence for his point of view). Stuart Kauffman might be able to determine whether the “laws” he discerns in his computer simulations prevail in the real world. If the extraterrestrials are intelligent enough to have developed their own science, physicist Edward Witten may learn whether superstring theory really is the inevitable culmination of any search for the fundamental rules governing reality. Science fiction will become fact. The New York Times will resemble one of those supermarket tabloids that prints “photographs” of Presidents hobnobbing with aliens. One can always hope.
Postscript: Of the scientists mentioned above, only Stuart Kauffman, Richard Dawkins and Ed Witten are still alive. Stanley Miller, Lynn Margulis, Gunther Stent, Stephen Jay Gould and Francis Crick have died, and their scientific survivors seem as far as ever from understanding life’s beginning(s?).
Photo of Stanley Miller from Wikimedia Commons.
About the Author: Every week, John Horgan takes a puckish, provocative look at breaking science. A former staff writer at Scientific American, he is the author of four books, including The End of Science (Addison Wesley, 1996) and The End of War (McSweeney's Books, January 2012). Follow on Twitter@Horganism.
The views expressed are those of the author and are not necessarily those of Scientific American.

Source: SCIENTIFIC AMERICAN

Running Lights: Did Expelled Stars Reionize the Ancient Universe?

Hot stars booted out of their galactic homes may be responsible for creating the conditions that led to today's universe
Permanent Address: http://www.scientificamerican.com/article.cfm?id=running-lights-did-expelled-stars-reionize-the-ancient-universe

Chandra Deep Field SouthBEYOND HUBBLE Not even the Hubble Space Telescope can crack the mystery of the universe's re-ionizationImage: flickr/NASA's Marshall Space Flight Center

In the beginning there was light—the brilliant light of the big bang shining through a sea of protons, neutrons and electrons. But as the universe expanded and cooled, the electrons joined the protons, making neutral hydrogen atoms, and as the universe cooled further, the light went dark. Eventually, however, something tore the electrons from the protons, thereby re-ionizing the universe. Space has remained ionized—a plasma of positive ions and electrons—ever since. Now an upcoming paper proposes the surprising cause: runaway stars flung from their galactic birthplaces.
"Re-ionization was one of the major cataclysmic events in the history of the universe," says Charlie Conroy, an astronomer at the University of California, Santa Cruz. Yet because re-ionization occurred so long ago, even the greatest telescopes struggle to probe this distant epoch. Observations of the farthest quasars as well as the big bang's afterglow indicate that re-ionization took place sometime between a redshift of 6 and 12, a measure of astronomical distance that corresponds to the time when the universe was only 380 million to 960 million years old. But exactly what caused this great transformation is a mystery.
The culprit must have been something hot, because only hot objects emit extreme ultraviolet light, whose wavelength is less than 912 angstroms, or 91.2 nanometers (a nanometer is a billionth of a meter), and whose photons are so energetic they rip electrons from protons. Quasars once seemed a logical bet, because they are hot and bright and existed long ago. But astronomers have failed to find enough quasars at great distances to do the job.
So the focus has turned instead to hot stars. Trouble is, these stars presumably lived in galaxies filled with neutral hydrogen gas—which absorbs extreme ultraviolet light.
"Of all the ionizing photons that hot stars are producing in today's galaxies, only about a percent of the photons actually leave the galaxy," Conroy says. "Those ionizing photons are being wasted in the galaxy."
Now, in work to appear in the August 20 issue of The Astrophysical Journal, Conroy and Kaitlin Kratter of the Harvard-Smithsonian Center for Astrophysics propose a resolution to this dilemma. They say that hot stellar runaways—stars shot out of their nurseries—may have reionized the early universe.
Stars born with the most mass—more than 16 times that of the sun—are so hot that astronomers classify them as spectral type O. These O-type stars glow blue and emit most of their radiation at ultraviolet wavelengths, then explode just a few million years after birth. In our own galaxy, the Milky Way, about 30 percent of them are runaway stars. One famous example, visible to the naked eye, is the star Mu Columbae, which is fleeing its birthplace in the constellation Orion and now resides in another constellation altogether.
A runaway star can make its escape when one star orbiting another explodes, freeing its partner at high speed. Runaways also emerge from star clusters, where gravitational encounters among stars fling some of the members away.
Our galaxy is so huge, with a disk more than 100,000 light-years across, that runaway O-type stars don't escape it during their short lives. In the early universe, however, galaxies were much smaller. During the epoch of re-ionization, they may have been just a few hundred light-years across. "If a star is traveling at a high velocity, it can actually leave the parent galaxy," Kratter says. Then the star's extreme ultraviolet light shines into the space beyond the galaxy. As a result, Conroy says, "These stars could be a very important player in the re-ionization of the universe."
"It seems like a viable hypothesis that these runaway stars can contribute significantly to the ionizing radiation," says Brian Siana of the University of California, Riverside. "But the question is: Are they the dominant factor?" Siana says supernova explosions may have punched holes in the gas of the first galaxies, producing a Swiss cheese–like structure that allowed extreme ultraviolet radiation from hot stars to seep out of the galaxies, obviating the need for runaways.
Conroy and Kratter suggest a way to test their idea. Astronomers can't see individual stars at the great distances corresponding to the epoch of re-ionization. But if hot stars escaped the first galaxies, the galaxies themselves should look larger at wavelengths where they emitted ultraviolet light than at longer wavelengths, because the hot, ultraviolet-bright runaway stars had fled their homes. Seeing such distant galaxies is too tough a task even for the Hubble Space Telescope, but Conroy and Kratter say that 30-meter ground-based telescopes planned for the future should find them, shedding new light on the universe's ancient metamorphosis.
Source: SCIENTIFIC AMERICAN


miércoles, 1 de agosto de 2012



Spontaneous B-L breaking as the origin of the hot early universe

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Title:
Spontaneous B-L breaking as the origin of the hot early universe
Authors:
Buchmüller, W.Domcke, V.Schmitz, K.
Affiliation:
AA(Deutsches Elektronen-Synchrotron DESY, 22607 Hamburg, Germany), AB(Deutsches Elektronen-Synchrotron DESY, 22607 Hamburg, Germany), AC(Deutsches Elektronen-Synchrotron DESY, 22607 Hamburg, Germany)
Publication:
Nuclear Physics B, Volume 862, Issue 3, p. 587-632.
Publication Date:
09/2012
Origin:
ELSEVIER
Abstract Copyright:
Elsevier B.V.
DOI:
10.1016/j.nuclphysb.2012.05.001
Bibliographic Code:
2012NuPhB.862..587B

Abstract

The decay of a false vacuum of unbroken B-L symmetry is an intriguing and testable mechanism to generate the initial conditions of the hot early universe. If B-L is broken at the grand unification scale, the false vacuum phase yields hybrid inflation, ending in tachyonic preheating. The dynamics of the B-L breaking Higgs field and thermal processes produce an abundance of heavy neutrinos whose decays generate entropy, baryon asymmetry and gravitino dark matter. We study the phase transition for the full supersymmetric Abelian Higgs model. For the subsequent reheating process we give a detailed time-resolved description of all particle abundances. The competition of cosmic expansion and entropy production leads to an intermediate period of constant 'reheating' temperature, during which baryon asymmetry and dark matter are produced. Consistency of hybrid inflation, leptogenesis and gravitino dark matter implies relations between neutrino parameters and superparticle masses. In particular, for a gluino mass of 1 TeV, we find a lower bound on the gravitino mass of 10 GeV.
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