Tag: Science

  • Big Mystery: Jupiter Loses a Stripe

    Lost: A giant belt of brown clouds big enough to swallow Earth twenty times over. If found, please return to Jupiter. In a development that has transformed the appearance of the solar system’s largest planet, one of Jupiter’s two main cloud belts has completely disappeared.

    “This is a big event,” says planetary scientist Glenn Orton of NASA’s Jet Propulsion Lab. “We’re monitoring the situation closely and do not yet fully understand what’s going on.”

    These side by side images of Jupiter taken by Australian astrophotographer Anthony Wesley show the SEB in August 2009, but not in May 2010. Credit: Anthony Wesley

    Known as the South Equatorial Belt (SEB), the brown cloudy band is twice as wide as Earth and more than twenty times as long. The loss of such an enormous “stripe” can be seen with ease halfway across the solar system.

    “In any size telescope, or even in large binoculars, Jupiter’s signature appearance has always included two broad equatorial belts,” says amateur astronomer Anthony Wesley of Australia. “I remember as a child seeing them through my small backyard refractor and it was unmistakable. Anyone who turns their telescope on Jupiter at the moment, however, will see a planet with only one belt–a very strange sight.”

    Wesley is a veteran observer of Jupiter, famous for his discovery of a comet hitting the planet in 2009. Like many other astronomers, he noticed the belt fading late last year, “but I certainly didn’t expect to see it completely disappear,” he says. “Jupiter continues to surprise.”

    Orton thinks the belt is not actually gone, but may be just hiding underneath some higher clouds.

    “It’s possible,” he hypothesizes, “that some ‘ammonia cirrus’ has formed on top of the SEB, hiding the SEB from view.” On Earth, white wispy cirrus clouds are made of ice crystals. On Jupiter, the same sort of clouds can form, but the crystals are made of ammonia (NH3) instead of water (H20).

    What would trigger such a broad outbreak of “ammonia cirrus”? Orton suspects that changes in global wind patterns have brought ammonia-rich material into the clear, cold zone above the SEB, setting the stage for formation of the high-altitude, icy clouds.

    “I’d love to send a probe in there to find out what’s really going on.”

    Without the SEB present, Jupiter’s Great Red Spot is surrounded by almost uninterrupted white. Anthony Wesley took this picture on May 18, 2010. Credit: Anthony Wesley

    Indeed, Jupiter’s atmosphere is a mysterious place which would benefit from exploration. No one knows, for instance, why the Great Red Spot is red—or what has sustained the raging storm for so many years. Neither does theory explain why the twin equatorial belts are brown, nor why one should vanish while the other remains. “We have a long list of questions,” says Orton.

    This isn’t the first time the SEB has faded out.

    “The SEB fades at irregular intervals, most recently in 1973-75, 1989-90, 1993, 2007, 2010,” says John Rogers, director of the British Astronomical Association’s Jupiter Section. “The 2007 fading was terminated rather early, but in the other years the SEB was almost absent, as at present.”

    The return of the SEB can be dramatic.

    “We can look forward to a spectacular outburst of storms and vortices when the ‘SEB Revival’ begins,” says Rogers. “It always begins at a single point, and a disturbance spreads out rapidly around the planet from there, often becoming spectacular even for amateurs eyeballing the planet through medium-sized telescopes. However we can’t predict when or where it will start. On historical precedent it could be any time in the next 2 years. We hope it will be in the next few months so that everyone can get a good view.

    “I’ll be watching every chance I get,” says Wesley. “The revival will likely be sudden and dramatic, with planet-circling groups of storms appearing over the space of just a week or so.”

    Indeed, says Orton, “anyone could be the first to spot the return of the SEB.”

    via spacefellowship.com

  • Dr Craig Venter Announces First Synthetic Living Cell. Never did god look smaller and pettier.

    Can we say that we’re just a step away from disproving the existence of god? 

    The least we can say is that god and religion are getting smaller and pettier by the minute.

    [youtube=http://www.youtube.com/watch?v=eoqBSNmYJYI&hl=en_US&fs=1&rel=0&color1=0x006699&color2=0x54abd6&border=1]

    Dr Craig Venter, of the J Craig Venter Institute, explained how they created what he described as “the first species…. to have its parents be a computer”.

     

     

    Figure 1

    Man-made DNA has booted up a cell for the first time.

    In a feat that is the culmination of two and a half years of tests and adjustments, researchers at the J. Craig Venter Institute inserted artificial genetic material — chemically printed, synthesized and assembled — into cells that were then able to grow naturally.

    “We all had a very good feeling that it was going to work this time,” said Venter Institute synthetic biologist Daniel Gibson, co-author of the study published May 20 in Science. “But we were cautiously optimistic because we had so many letdowns following the previous experiments.”

    On a Friday in March, scientists inserted over 1 million base pairs of synthetic DNA into Mycoplasma capricolum cells before leaving for the weekend. When they returned on Monday, their cells had bloomed into colonies.

     

    “When we look at life forms, we see fixed entities,” said J. Craig Venter, president of the Institute, in a recent podcast. “But this shows in fact how dynamic they are. They change from second to second. And that life is basically the result of an information process. Our genetic code is our software.”

    Coaxing the software to power a cell proved harder than expected.

    Figure 5 [Converted]

    After the Venter Institute announced in early 2008 that it had assembled a synthetic Mycoplasma genitalium genome, the assumption was that it would be running cells in no time. But this particular cell type, despite its minimal size, was not an ideal research partner. One problem was speed.

    “We had to deal with the fact that M. genitalium had an extremely slow growth rate,” Gibson said. “For every experiment that was done, it took more than a month to get results.”

    Moreover, transplanting the code into recipient cells was failing. So researchers cut their losses and called in a substitute, opting for the larger, speedier and less finicky Mycoplasma mycoides. The choice was a good one.

    “Over the last five years the field has seen a 100-fold increase in the length of genetic material wholly constructed from raw chemicals,” said synthetic biologist Drew Endy of Stanford University. “This is over six doublings in the max length of a genome that can be constructed.”

    Plunging costs of synthesis allowed a leap past the 1 million base-pair mark, from code to assembly. “Imagine doubling the diameter of a silicon wafer that can be manufactured that much, going from 1 cm to 1 meter [fabrications] in just five years,” Endy said. “That would have been an incredible achievement.”

    “They rebuilt a natural sequence and they put in some poetry,” said University of California at San Francisco synthetic biologist Chris Voigt. “They recreated some quotes in the genome sequence as watermarks.”

    It’s an impressive trick, no doubt, but replicating a natural genome with a little panache is also the limit of our present design capabilities.

    Researchers, for instance, figure yeast can handle the assembly of 2 million base pairs, but they’re not sure about more. And an energy-producing cyanobacteria that sequesters carbon, Gibson says, is still several years off.

    The ultimate goal, of course, is a brand-new genome from the ground up. Now, Voigt said, “what do you do with all that design capacity?”

    Images: 1) Schematic demonstrating the assembly of a synthetic M. mycoides genome in yeast./Science/AAAS. 2) Images of the phenotype of the JCVI-syn1.0 and WT strains./Science/AAAS.

    Posted via web from Monicks: Unleashed

  • Astronomy Picture of the Day | Hubble Observes the Large Magellanic Cloud

    The massive, young stellar grouping, called R136, is only a few million years old and resides in the 30 Doradus Nebula, a turbulent star-birth region in the Large Magellanic Cloud (LMC), a satellite galaxy of our Milky Way. Many of the stars are among the most massive known. Several of them are over 100 times more massive than our Sun. These hefty stars are destined to become supernovae in a few million years.

    Hubble Observes the Large Magellanic Cloud’s Star-Forming Region, 30 Doradus. Credit: NASA, ESA, and F. Paresce (INAF-IASF, Bologna, Italy)

    via spacefellowship.com

    The image, taken by Hubble’s Wide Field Camera 3, spans about 100 light-years. The nebula is close enough to Earth that Hubble can resolve individual stars, giving astronomers important information about the stars’ birth and evolution.

    The brilliant stars are carving deep cavities in the surrounding material by unleashing a torrent of ultraviolet light, and hurricane-force stellar winds (streams of charged particles), which are etching away the enveloping hydrogen gas cloud in which the stars were born. The image reveals a fantasy landscape of pillars, ridges, and valleys, as well as a dark region in the center that roughly looks like the outline of a holiday tree. Besides sculpting the gaseous terrain, the brilliant stars can also help create a successive generation of offspring. When the winds hit dense walls of gas, they create shocks, which may be generating a new wave of star birth.

    The movement of the LMC around the Milky Way may have triggered the massive cluster’s formation in several ways. The gravitational tug of the Milky Way and the companion Small Magellanic Cloud may have compressed gas in the LMC. Also, the pressure resulting from the LMC plowing through the Milky Way’s halo may have compressed gas in the satellite. The cluster is a rare, nearby example of the many super star clusters that formed in the distant, early universe, when star birth and galaxy interactions were more frequent. Previous Hubble observations have shown astronomers that super star clusters in faraway galaxies are ubiquitous. The LMC is located 170,000 light-years away and is a member of the Local Group of Galaxies, which also includes the Milky Way.

    The Hubble image was taken at infrared wavelengths (1.1 microns and 1.6 microns). Hubble sees through the dusty nebula, revealing many stars that cannot be seen in visible light. The large bright star just above the center of the image is in the 30 Doradus nebula. The Hubble observations of 30 Doradus were made October 20-27, 2009.

    Posted via web from Monicks: Unleashed