Astronomy News


NASA to Attempt Historic Solar Sail Deployment

06.26.2008 


"Hold your hands out to the sun. What do you feel? Heat, of course. But there's pressure as well - though you've never noticed it, because it's so tiny. Over the area of your hands, it only comes to about a millionth of an ounce. But out in space, even a pressure as small as that can be important - for it's acting all the time, hour after hour, day after day. Unlike rocket fuel, it's free and unlimited. If we want to, we can use it; we can build sails to catch the radiation blowing from the sun."


These words were spoken not by a NASA scientist but by a fictional character - John Merton - in Arthur C. Clarke's short story The Wind from the Sun. If all goes well, Merton's prophetic words are about to become fact.

NASA researchers, thinking "out of the box" (or maybe "out of the rocket") have long dreamed of the possibility of sailing among the planets with sails propelled by sunlight instead of by wind. Except in works of fiction, though, no one has yet successfully deployed such a sail anywhere beyond Earth.

Right: An artist's concept of a sailing ship and a solar sail.


"There's a first time for everything," says Edward "Sandy" Montgomery of NASA's Marshall Space Flight Center.

Montgomery's team and a team from Ames Research Center (led by Elwood Agasid) hope to make history this summer by deploying a solar sail called NanoSail-D. It will travel to space onboard a SpaceX Falcon 1 rocket, scheduled for launch from Omelek Island in the Pacific Ocean during a window extending from July 29th to August 6th (a back-up window extends from August 29th to September 5th).


"NanoSail-D will be the first fully deployed solar sail in space, and the first spacecraft to use solar pressure as a primary means of attitude control or orbital maneuvering," says Montgomery, who is NanoSail-D's payload manager.


"We are always on the lookout for opportunities. Ames owns a slot on the Falcon 1 launch and asked us if we wanted to go along. We said, 'Yes!' We'll use the Poly Picosatellite Orbital Deployer, or P-POD, developed by the University of California Polytechnic Institute to deploy our sail."

A few years ago, the Planetary Society attempted a mission like NanoSail-D called Cosmos I, but the launch vehicle failed and destroyed the undeployed spacecraft. Montgomery and team believe that NanoSail-D, however, will unfurl four gossamer wings from its pod in the blackness of space like a butterfly from a cocoon.


"The structure is made of aluminum and space-age plastic," says Montgomery. "The whole spacecraft weighs less than ten pounds. We carry it around in a special suitcase -- airplane carry-on luggage size." Fully opened, the kite-shaped sail spreads out to about 100 square feet of light-catching surface.



Above: The Huntsville-based NanoSail-D team stands with the fully deployed sail at ManTech SRS technologies on April 16, 2008, after the successful deployment test.


"A success would be huge for the future of space exploration," Montgomery believes.


Why so important? Solar sails could extend our reach as far as our dreams. Because there's no friction in space, once a solar sail starts moving, it can go on forever. Indeed, long after a rocket would run out of gas and begin to coast, a solar sailship could still be accelerating, achieving speeds much faster and covering distances far greater than any rocket. No rocket in existence could carry enough fuel to reach the outer solar system in as short a time. And like a marine sail, a solar sail could also bring you home. You could use the solar sail to tack your vessel, making it travel "against the wind," back to Earth.


"It's not so much about how far a sail will go compared to a rocket; the key is how fast," says Montgomery. "The Voyagers have escaped the solar system, and they were sent by rockets, but it's taken more than three decades to do it. A sail launched today would probably catch up with them in a single decade. Sails are slower to get started though. So, for example, between the Earth and the moon, rockets might be preferred for missions with a short timeline. It's a trip of days for rockets, but months for a solar sail. The rule of thumb, therefore, would be to use rockets for short hops and solar sails for the long hauls."


Right: University of Alabama research technician Doug Huie holds the future in his hands. Folded-up, NanoSail-D occupies a space no bigger than a bread box.


All of this may sound like speculation, but NanoSail-D could show that solar sails are truly feasible. And there's an added bonus to this technology demo:

"Currently, micro-satellites in orbit above a few hundred kilometers can stay in orbit for decades after completing their mission," explains Montgomery. "This creates an orbital debris collision risk for other spacecraft. NanoSail-D will demonstrate the feasibility of using a drag sail to decrease the time satellites clutter up Earth's orbit. Although our sail looks like a kite, it will act like a parachute (or like a drag sail) in the very thin upper atmosphere around Earth. It will slow the spacecraft and make it lose altitude, re-enter the Earth's atmosphere and burn off in a relatively short period of time. A drag sail is a lighter alternative to carrying a propulsion system to de-orbit a satellite."


And finally, the question everyone wants answered: What does D stand for?

"We chose the 'D' in the name, not because it came after models A, B, and C, but because it can stand for demonstrate, deploy, drag, and/or de-orbit," says Montgomery.

Soon, 'D' may stand for something new: "DID IT!"


Author: Dauna Coulter | Editor: Dr. Tony Phillips | Credit: Science@NASA




Nothing to Fear from Atom Smasher

By DOUGLAS BIRCH, Associated Press WriterSat Jun 28,  2008


The most powerful atom-smasher ever built could make some bizarre discoveries, such as invisible matter or extra dimensions in space, after it is switched on in August.


But some critics fear the Large Hadron Collider could exceed physicists' wildest conjectures: Will it spawn a black hole that could swallow Earth? Or spit out particles that could turn the planet into a hot dead clump?


Ridiculous, say scientists at the European Organization for Nuclear Research, known by its French initials CERN — some of whom have been working for a generation on the $5.8 billion collider, or LHC.


"Obviously, the world will not end when the LHC switches on," said project leader Lyn Evans.


David Francis, a physicist on the collider's huge ATLAS particle detector, smiled when asked whether he worried about black holes and hypothetical killer particles known as strangelets.


"If I thought that this was going to happen, I would be well away from here," he said.


The collider basically consists of a ring of supercooled magnets 17 miles in circumference attached to huge barrel-shaped detectors. The ring, which straddles the French and Swiss border, is buried 330 feet underground.


The machine, which has been called the largest scientific experiment in history, isn't expected to begin test runs until August, and ramping up to full power could take months. But once it is working, it is expected to produce some startling findings.


Scientists plan to hunt for signs of the invisible "dark matter" and "dark energy" that make up more than 96 percent of the universe, and hope to glimpse the elusive Higgs boson, a so-far undiscovered particle thought to give matter its mass.


The collider could find evidence of extra dimensions, a boon for superstring theory, which holds that quarks, the particles that make up atoms, are infinitesimal vibrating strings.


The theory could resolve many of physics' unanswered questions, but requires about 10 dimensions — far more than the three spatial dimensions our senses experience.


The safety of the collider, which will generate energies seven times higher than its most powerful rival, at Fermilab near Chicago, has been debated for years. The physicist Martin Rees has estimated the chance of an accelerator producing a global catastrophe at one in 50 million — long odds, to be sure, but about the same as winning some lotteries.


By contrast, a CERN team this month issued a report concluding that there is "no conceivable danger" of a cataclysmic event. The report essentially confirmed the findings of a 2003 CERN safety report, and a panel of five prominent scientists not affiliated with CERN, including one Nobel laureate, endorsed its conclusions.


Critics of the LHC filed a lawsuit in a Hawaiian court in March seeking to block its startup, alleging that there was "a significant risk that ... operation of the Collider may have unintended consequences which could ultimately result in the destruction of our planet."


One of the plaintiffs, Walter L. Wagner, a physicist and lawyer, said Wednesday CERN's safety report, released June 20, "has several major flaws," and his views on the risks of using the particle accelerator had not changed.


On Tuesday, U.S. Justice Department lawyers representing the Department of Energy and the National Science Foundation filed a motion to dismiss the case.


The two agencies have contributed $531 million to building the collider, and the NSF has agreed to pay $87 million of its annual operating costs. Hundreds of American scientists will participate in the research.


The lawyers called the plaintiffs' allegations "extraordinarily speculative," and said "there is no basis for any conceivable threat" from black holes or other objects the LHC might produce. A hearing on the motion is expected in late July or August.


In rebutting doomsday scenarios, CERN scientists point out that cosmic rays have been bombarding the earth, and triggering collisions similar to those planned for the collider, since the solar system formed 4.5 billion years ago.


And so far, Earth has survived.


"The LHC is only going to reproduce what nature does every second, what it has been doing for billions of years," said John Ellis, a British theoretical physicist at CERN.


Critics like Wagner have said the collisions caused by accelerators could be more hazardous than those of cosmic rays.


Both may produce micro black holes, subatomic versions of cosmic black holes — collapsed stars whose gravity fields are so powerful that they can suck in planets and other stars.


But micro black holes produced by cosmic ray collisions would likely be traveling so fast they would pass harmlessly through the earth.


Micro black holes produced by a collider, the skeptics theorize, would move more slowly and might be trapped inside the earth's gravitational field — and eventually threaten the planet.


Ellis said doomsayers assume that the collider will create micro black holes in the first place, which he called unlikely. And even if they appeared, he said, they would instantly evaporate, as predicted by the British physicist Stephen Hawking.


As for strangelets, CERN scientists point out that they have never been proven to exist. They said that even if these particles formed inside the Collider they would quickly break down.


When the LHC is finally at full power, two beams of protons will race around the huge ring 11,000 times a second in opposite directions. They will travel in two tubes about the width of fire hoses, speeding through a vacuum that is colder and emptier than outer space.


Their trajectory will be curved by supercooled magnets — to guide the beams around the rings and prevent the packets of protons from cutting through the surrounding magnets like a blowtorch.


The paths of these beams will cross, and a few of the protons in them will collide, at a series of cylindrical detectors along the ring. The two largest detectors are essentially huge digital cameras, each weighing thousands of tons, capable of taking millions of snapshots a second.


Each year the detectors will generate 15 petabytes of data, the equivalent of a stack of CDs 12 miles tall. The data will require a high speed global network of computers for analysis.


Wagner and others filed a lawsuit to halt operation of the Relativistic Heavy Ion Collider, or RHIC, at the Brookhaven National Laboratory in New York state in 1999. The courts dismissed the suit.


The leafy campus of CERN, a short drive from the shores of Lake Geneva, hardly seems like ground zero for doomsday. And locals don't seem overly concerned. Thousands attended an open house here this spring.


"There is a huge army of scientists who know what they are talking about and are sleeping quite soundly as far as concerns the LHC," said project leader Evans.


Copyright © 2008 The Associated Press. All rights reserved. The information contained in the AP News report may not be published, broadcast, rewritten or redistributed without the prior written authority of The Associated Press.

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Old Solar Cycle Returns

03.28.2008


March 28, 2008: Solar Cycle 23, how can we miss you if you won't go away?

Barely three months after forecasters announced the beginning of new Solar Cycle 24, old Solar Cycle 23 has returned. Actually, it never left. Read on.


"This week, three big sunspots appeared and they are all old cycle spots," says NASA solar physicist David Hathaway. "We know this because of their magnetic polarity."


Earlier today, the Solar and Heliospheric Observatory (SOHO) made this magnetic map of the sun:




It shows the north and south magnetic poles of the three sunspots. All are oriented according to the patterns of Solar Cycle 23. Cycle 24 spots would be reversed.


What's going on? Hathaway explains: "We have two solar cycles in progress at the same time. Solar Cycle 24 has begun (the first new-cycle spot appeared in January 2008), but Solar Cycle 23 has not ended."


Strange as it sounds, this is perfectly normal. Around the time of solar minimum--i.e., now--old-cycle spots and new-cycle spots frequently intermingle. Eventually Cycle 23 will fade to zero, giving way in full to Solar Cycle 24, but not yet.


Meanwhile, on March 25th, sunspot 989, the smallest of the three sunspots, unleashed an M2-class solar flare. Flares are measured on a "Richter scale" ranging from A-class (puny) to X-class (powerful). M-class flares are of medium intensity. This one hurled a coronal mass ejection or "CME" into space (movie), but the billion-ton cloud missed Earth.


While the CME was still plowing through the sun's atmosphere, amateur radio astronomer Thomas Ashcraft heard "a heaving sound" coming from the loudspeaker of his 21 MHz shortwave receiver in New Mexico: listen. It was a Type II solar radio burst generated by shock waves at the leading edge of the CME. A thousand miles away in Virginia, David Thomas recorded the same emissions on a chart recorder he connected to his 20 MHz ham rig: look. "What a pleasant surprise," says Thomas.




Above: Sunspot counts vs. year: 2008 is a low point in the solar cycle. Smoothed curves are predictions of future activity. [More]

We could get more of this kind of activity in the next 7 to 10 days. It will take about that long for the sunspots to cross the face of the sun. The sun's rotation is turning the spots toward Earth, which means the next CME, if there is one, might not miss. CME strikes do no physical harm to Earth but they can cause Northern Lights, satellite glitches and, in extreme cases, power outages.

The real significance of these spots is what they say about the solar cycle, says Hathaway. "Solar Cycle 24 has begun, but we won't be through solar minimum until the number of Cycle 24 spots rises above the declining number of Cycle 23 spots." Based on this latest spate of "old" activity, he thinks the next Solar Max probably won't arrive until 2012.


Stay tuned to Science@NASA for solar cycle updates.

Author: Dr. Tony Phillips | Credit: Science@NASA


US to try to shoot down spy satellite

(Editor's follow up: We got it!)

By LOLITA C. BALDOR, Associated Press Writer 2-14-08 


Taking a page from Hollywood science fiction, the Pentagon said Thursday it will try to shoot down a dying, bus-size U.S. spy satellite loaded with toxic fuel on a collision course with the Earth.


The military hopes to smash the satellite as soon as next week — just before it enters Earth's atmosphere — with a single missile fired from a Navy cruiser in the northern Pacific Ocean.


The dramatic maneuver may well trigger international concerns, and U.S. officials have begun notifying other countries of the plan — stressing that it does not signal the start of a new American anti-satellite weapons program.


Military and administration officials said the satellite is carrying fuel called hydrazine that could injure or even kill people who are near it when it hits the ground. That reason alone, they said, persuaded President Bush to order the shoot-down.

"That is the only thing that breaks it out, that is worthy of taking extraordinary measures," said Gen. James Cartwright, vice chairman of the Joint Chiefs of Staff, during a Pentagon briefing.


He predicted a fairly high chance — as much as 80 percent — of hitting the satellite, which will be about 150 miles up when the shot is fired. The window of opportunity for taking the satellite down, Cartwright said, opens in three or four days and lasts for about seven or eight days.


"We'll take one shot and assess," he said. "This is the first time we've used a tactical missile to engage a spacecraft."

Deputy National Security Adviser James Jeffrey discounted comparisons to an anti-satellite test conducted by the Chinese last year that triggered criticism from the U.S. and other countries.


"This is all about trying to reduce the danger to human beings," Jeffrey said. "Specifically, there was enough of a risk for the president to be quite concerned about human life."


There might also be unstated military aims, some outside the administration suggested.


Similar spacecraft re-enter the atmosphere regularly and break up into pieces, said Ivan Oelrich, vice president for strategic security programs at the Federation of American Scientists. He said, "One could be forgiven for asking if this is just an excuse to test an anti-satellite weapon."


A key issue when China shot down its defunct weather satellite was that it created an enormous amount of space debris.

"All of the debris from this encounter, as carefully designed as it is, will be down at most within weeks, and most of it will be down within the first couple of orbits afterward," said Jeffrey. "There's an enormous difference to spacefaring nations in ... those two things."


He and others dismissed suggestions that this was simply an attempt by the U.S. to flex its muscles, and that officials were overstating the toxic fuel threat.


Left alone, the satellite would be expected to hit Earth during the first week of March. About half of the 5,000-pound spacecraft would be expected to survive its blazing descent through the atmosphere and would scatter debris over several hundred miles.

If the missile shot is successful, officials said, much of the debris would burn up as it fell. They said they could not estimate how much would make it through the atmosphere. They said the largest piece that would survive re-entry would be the spherical fuel tank, which is about 40 inches wide — assuming it is not hit directly by the missile.


The goal, however, is to hit the fuel tank in order to minimize the amount of fuel that returns to Earth, Cartwright said.

A Navy missile known as Standard Missile 3 would be fired at the spy satellite in an attempt to intercept it just before it re-enters Earth's atmosphere. It would be "next to impossible" to hit the satellite after that because of atmospheric disturbances, he said.

Known by its military designation US 193, the satellite was launched in December 2006. It lost power and its central computer failed almost immediately afterward, leaving it uncontrollable. It carried a sophisticated and secret imaging sensor.


Software associated with the Standard Missile 3 has been modified to enhance the chances of the missile's sensors recognizing that the satellite is its target. The missile's designed mission is to shoot down ballistic missiles, not satellites. Other officials said the missile's maximum range, while a classified figure, is not great enough to hit a satellite operating in normal orbits.

"It's a one-time deal," Cartwright said when asked whether the modified Standard Missile 3 should be considered a new U.S. anti-satellite technology.


He said that if an initial shoot-down attempt fails, the military would have about two days to reassess and decide whether to take a second shot.


NASA Administrator Michael Griffin told reporters that analysis shows the hydrazine tank would survive a fall to Earth under normal circumstances, much as one did when the Space Shuttle Columbia crashed.


"The hydrazine which is in it is frozen solid, as it is now. Not all of it will melt," he said. If the tank hits the ground it will have been breached because the fuel lines will have broken off and hydrazine will vent out, he said.


Jeffrey said members of Congress were briefed on the plan earlier Thursday and that diplomatic notifications to other countries were being made by the end of the day.


"It should be understood by all, at home and abroad, that this is an exceptional circumstance and should not be perceived as the standard U.S. policy for dealing with errant satellites," said House Armed Services Chairman Ike Skelton.

___

Associated Press Writers Pauline Jelinek, Robert Burns and Ted Bridis contributed to this report.

___

On the Net:

Defense Department: http://www.defenselink.mil

 

Copyright © 2008 The Associated Press. All rights reserved.


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NASA to Launch Beatles Tune Into Space

February 1, 2008


The Beatles are about to become radio stars in a whole new way. NASA on Monday will broadcast the Beatles' song "Across the Universe" across the galaxy to Polaris, the North Star.


This first-ever beaming of a radio song by the space agency directly into deep space is nostalgia-driven. It celebrates the 40th anniversary of the song, the 45th anniversary of NASA's Deep Space Network, which communicates with its distant probes, and the 50th anniversary of NASA.


"Send my love to the aliens," Paul McCartney told NASA through a Beatles historian. "All the best, Paul."


The song, written by McCartney and John Lennon, may have a ticket to ride and will be flying at the speed of light. But it will take 431 years along a long and winding road to reach its final destination. That's because Polaris is 2.5 quadrillion miles away.


NASA loaded an MP3 of the song, just under four minutes in its original version, and will transmit it digitally at 7 p.m. EST Monday from its giant antenna in Madrid, Spain. But if you wanted to hear it on Polaris, you would need an antenna and a receiver to convert it back to music, the same way people receive satellite television.


The idea came from Martin Lewis, a Los Angeles-based Beatles historian, who then got permission from McCartney, Yoko Ono and the two companies that own the rights to Beatles' music. One of those companies, Apple, was happy to approve the idea because is "always looking for new markets," Lewis said.


Perhaps coincidentally, the song's launching comes a day before the release of the DVD of the Julie Taymor movie named after the Beatles hit.


Copyright © 2008 The Associated Press. All rights reserved. The information contained in the AP News report may not be published, broadcast, rewritten or redistributed without the prior written authority of The Associated Press. 

A Big Step Toward a Big Telescope

Just about every amateur astronomer has wondered what it'd be like to have an even-bigger telescope — we call it "aperture envy" — and professional astronomers are no different.
 

Each of the 492 mirror segments that comprise the Thirty Meter Telescope's f/1 primary mirror will be constantly adjusted for optimum alignment. An 11½-by-8-foot pickoff mirror protrudes through the central opening and directs light sideways to one of several planned instruments.

TMT ProjectSo the pros were understandably thrilled last week to learn that a telescope with an aperture of 30 meters (nearly 100 feet) is moving from wishful thinking to not-too-distant reality. That's because the Gordon and Betty Moore Foundation has pledged $200 million over the next nine years to aid construction of a giant eye called the Thirty Meter Telescope.
 
Building on experience gained with previous segmented-mirror designs, the TMT will employ 492 hexagonal mirrors, each about 1.44 meters (57 inches) across its corners, arrayed together into a 30-meter-wide f/1 primary mirror. Six artificial guide stars, created by lasers illuminating spots in the upper atmosphere, will allow the telescope to continuously cancel out the image-degrading effects of atmospheric turbulence.
 
It's hard to imagine a telescope this big. This 140-ton giant will gather eight times more light than any other telescope — heck, even its secondary mirror is 10 feet across!
 

When completed in 2016, the mammoth Thirty Meter Telescope will have eight times the light-gathering area of any otherWhen completed in 2016, the mammoth Thirty Meter Telescope will have eight times the light-gathering area of any other optical telescope. optical telescope.

TMT ProjectA site for the TMT hasn't been chosen; five locations in Chile, Hawaii, and Mexico are being studied, though Cerro Armazones in northern Chile is the one being used for planning purposes. Construction should begin in 2009, with "first light" expected in 2016.
 
If you're an aspiring astrophysicist wondering where to go to college, note that TMT is a collaboration involving Caltech, the University of California, AURA (a consortium of universities), and ACURA (AURA's Canadian counterpart). Caltech and the UC system, which previously joined forces to build the Keck telescopes, have each committed $50 million toward the TMT, and their astronomers will get the lion's share of observing time.
 
The TMT project already has an informative website, and if you're a real gearhead eager to see the technical details, I recommend perusing the recently completed 229-page "TMT Construction Proposal".
 
And, just in case you're wondering, the TMT won't have an eyepiece.
 
 
 

Posted by Kelly Beatty, December 12, 2007



NASA pressed to avert catastrophic Deep Impact

by Jitendra Joshi Thu Nov 8, 2007 


NASA penny-pinching risks exposing humankind to a planetary catastrophe if a big enough asteroid evades detection and slams into Earth, US lawmakers warned Thursday.


But the US space agency said the chances of a new "Near-Earth Object" (NEO) like the one that wiped out the dinosaurs were too remote to divert scarce resources.


Scott Pace, head of program analysis and evaluation at NASA, said the agency could not do more to detect NEOs "given the constrained resources and the strategic objectives NASA already has been tasked with."

Pace and other NASA officials were grilled at a congressional hearing on the existing NEO program, which seized the public imagination in the late 1990s through the movies "Armageddon" and "Deep Impact."


Lawmakers decried the threatened closure of a giant radio telescope in Puerto Rico run with NASA's assistance that is the world's foremost facility for tracking space objects.


"We're talking about minimal expense compared to the cost of having to absorb this type of damage," Republican Congressman Dana Rohrabacher said. "After all, it may be the entire planet that is destroyed!"

Puerto Rico delegate Luis Fortuno fretted over the economic impact on his impoverished US territory, but also warned of the broader consequences for the entire planet.


"We must take action now to enhance our awareness to prevent a catastrophe," he told the hearing.

The National Science Foundation has earmarked the Arecibo Observatory, which featured in science-fiction movie "Contact" and the James Bond installment "Goldeneye," for closure after 2011 if new private-sector money is not found.

NASA officials said they would get by with new monitoring systems, including a network of four telescopes being built in Hawaii by the US Air Force.


Critics say NASA has imposed big cuts on many research programs in a bid to meet President George W. Bush's goal of returning astronauts to the Moon by 2020 and use it as a stepping stone for manned missions to Mars and beyond.

The hearing of the House of Representatives space and aeronautics subcommittee highlighted one small asteroid named Apophis, about 250 meters (273 yards) wide, which some scientists say could swing by Earth on Friday, April 13, 2029.

NASA says there is a one in 45,000 chance that Apophis could pass through a "gravitational keyhole" and return to hit the planet in 2036.


"It's a very unlikely situation and one we can drive to zero, probably," said Donald Yeomans, who manages the NEO program at NASA's Jet Propulsion Laboratory.

NASA now only tracks NEOs larger than one kilometer (0.62 miles) in diameter, which come near Earth only once every few hundred thousand years.

Objects of that size can cause global disaster through their immediate surface impact and by triggering rapid climate change.


"Extinction-class" objects measuring at least 10 kilometers, such as the object that crashed into Mexico's Yucatan peninsula about 65 million years ago, would be rarer still.

Yeomans said also that while the European and Japanese space agencies are stepping up their own NEO programs, more than 98 percent of the work is now done by NASA.


Copyright © 2007 Agence France Presse. All rights reserved. The information contained in the AFP News report may not be published, broadcast, rewritten or redistributed without the prior written authority of Agence France Presse.

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Scientists Ask Congress To Fund $50 Billion Science Thing


WASHINGTON, DC—Top physicists from several major American universities appeared before a Congressional committee Monday to request $50 billion for a science thing that would further U.S. advancement science-wise and broaden human knowing.


The scientists spoke for approximately three hours about the complicated science machine, which is expensive, and large, telling members of the House Committee on Science and Technology that the tubular, gamma-ray-using mechanism is vital in some big way. Yet the high price tag of the thing, which would be built on a 40-square-mile plot of land where the science would ultimately occur, remained a pressing question.


"While expense is something to consider, I think it's very important that we have this kind of scientific apparatus, because, in the end, I have always said that science is more important than it is unimportant," Committee chairman Rep. Bart Gordon (D-TN) said. "And it's essential we stay ahead of China, Japan, and Germany in science. We are ahead in space, with the NASA rockets going to other planets, so we should be ahead in science too."


According to the scientists, the electromagnetic science-maker will make atoms move and spin around very quickly, though spectators at the hearing said afterward they could not account for how one could get some atoms to move around faster than other ones if everything is made of atoms anyway. In addition, the scientists said that the device would be several miles in circumference, which puzzled onlookers who had long assumed that atoms were tiny. Despite these apparent inconsistencies, the scientists, in Rep. Gordon's words, appeared "very smart-sounding" and confident that their big spinner would solve some kind of problem they described.


The highlight of the scientists' testimony was a series of several colorful diagrams of how the big machine would work. One consisted of colored dots resembling Skittles banging into one another. Noting the motion lines behind the circle-ball things, committee members surmised that they were slamming together in a "fast, forceful manner." Yet some expressed doubts as to whether they justified the $50 billion price tag.


"These scientists could trim $10 million if they would just cut out some of the purple and blue spheres," said Rep. Roscoe Bartlett (R-MD), explaining that he understood the need for an abundance of reds and greens. "With all of those molecules and atoms going in every direction, the whole thing looks a bit unorganized, especially for science."

Another diagram presented to lawmakers contained several important squiggly lines, numbers, and letters. Despite not being numbers, the letters were reportedly meant to represent mathematics too. The scientists seemed to believe that correct math was what would help make the science thing go.


The scientists concluded their presentation by informing the committee that, if constructed correctly, the super science-flyer would be able to answer questions about many, many things, mainly stuff about the universe that sounded like it would be very good to know about.


"Now, I'm no science major, but if I'm being told by a group of people that the protons, neutrons, and electrons need unifying, then I think we owe it to the American people to go in and unify them," Rep. Mark Udall (D-CO) said. "After all, isn't a message of unity what we want to send to our children?"


Still, some committee members were not as convinced, saying that the building of a micro-macro isotope-making science generator should not be a top priority.


"Fifty billion dollars to buy atoms is too much," Rep. Tom Feeney (R-FL) said. "Frankly, I don't understand why they don't just gather up all the leftover atoms in their test tubes and Bunsen burners. I think the scientists should have to use those up before getting new ones."


The scientists remained hopeful that their federal funding will be approved.


"The congressmen appeared receptive to what we were saying, and I think that we made a very convincing case as to why we need a [science gadget] of this magnitude on American soil," said Caltech physicist David Kaminski, who added various other scientific information. "[Some complicated physics-related act] would be possible in our lifetime only through the creation of a [science thing]."

Mystery Illness Strikes After Meteorite Hits Peruvian Village

Mon Sep 17, 11:23 PM ET

 

Villagers in southern Peru were struck by a mysterious illness after a meteorite made a fiery crash to Earth in their area, regional authorities said Monday.


Around midday Saturday, villagers were startled by an explosion and a fireball that many were convinced was an airplane crashing near their remote village, located in the high Andes department of Puno in the Desaguadero region, near the border with Bolivia.


Residents complained of headaches and vomiting brought on by a "strange odor," local health department official Jorge Lopez told Peruvian radio RPP.


Seven policemen who went to check on the reports also became ill and had to be given oxygen before being hospitalized, Lopez said.


Rescue teams and experts were dispatched to the scene, where the meteorite left a 100-foot-wide (30-meter-wide) and 20-foot-deep (six-meter-deep) crater, said local official Marco Limache.

"Boiling water started coming out of the crater and particles of rock and cinders were found nearby. Residents are very concerned," he said.


Copyright © 2007 Agence France Presse. All rights reserved. The information contained in the AFP News report may not be published, broadcast, rewritten or redistributed without the prior written authority of Agence France Presse. Copyright © 2007 Yahoo! Inc. All rights reserved.



Mysterious Solar Ripples Detected

Dave Mosher, Staff Writer

SPACE.com

 

Mysterious waves that help transport the sun's energy out into space have been detected by scientists for the first time.

Researchers hope their discovery of the energetic ripples, known as Alfven waves, will shed light on other solar phenomena such as the sun's magnetic fields and its super-hot corona, or outermost atmosphere. A new video shows the ripples in action.


"Alfven waves can provide us with a window into processes that are fundamental to the workings of the sun and its impacts on Earth," said Steve Tomczyk, a space scientist with the National Center for Atmospheric Research (NCAR).

Like a wave traveling along a string, Alfven waves run along the sun's magnetic field lines and reach deep into space. While astrophysicists have identified the waves far away from the sun, they've never been detected close to our star-the ripples were too small and too fast to spot.


To observe the elusive waves, Tomczyk and his colleagues pointed the coronal multichannel polarimeter (CoMP) instrument, located at the National Solar Observatory's Sacramento Peak Observatory in New Mexico, at the sun's hot, hazy corona. Thanks to CoMP's imaging speed of one picture every 15 seconds, the scientists captured the waves traveling at about 9 million mph (14.5 million kilometers per hour).


"The waves are visible all the time and they occur all over the corona, which was initially surprising to us," said Scott McIntosh, a space scientist at the Southwest Research Institute in Boulder, Colo.

The waves might help explain how energy is transferred to the sun's corona, which is millions of degrees hotter than the solar surface.


Tomczyk and his colleagues' findings will be detailed in the Aug. 30 online edition of the journal Science.

SEE THE VIDEO: Solar Ripples GALLERY: The Sun's Summer Storms IMAGE: One Big Sun Spot Original Story: Mysterious Solar Ripples Detected


Copyright © 2007 SPACE.com


Astronomers puzzled by cosmic black hole

By SETH BORENSTEIN, AP Science Writer


Astronomers have stumbled upon a tremendous hole in the universe. That's got them scratching their heads about what's just not there. The cosmic blank spot has no stray stars, no galaxies, no sucking black holes, not even mysterious dark matter. It is 1 billion light years across of nothing. That's an expanse of nearly 6 billion trillion miles of emptiness, a University of Minnesota team announced Thursday.


Astronomers have known for many years that there are patches in the universe where nobody's home. In fact, one such place is practically a neighbor, a mere 2 million light years away. But what the Minnesota team discovered, using two different types of astronomical observations, is a void that's far bigger than scientists ever imagined.


"This is 1,000 times the volume of what we sort of expected to see in terms of a typical void," said Minnesota astronomy professor Lawrence Rudnick, author of the paper that will be published in Astrophysical Journal. "It's not clear that we have the right word yet ... This is too much of a surprise."


Rudnick was examining a sky survey from the National Radio Astronomy Observatory, which essentially takes radio pictures of a broad expanse of the universe. But one area of the universe had radio pictures indicating there was up to 45 percent less matter in that region, Rudnick said.


The rest of the matter in the radio pictures can be explained as stars and other cosmic structures between here and the void, which is about 5 to 10 billion light years away.


Rudnick then checked observations of cosmic microwave background radiation and found a cold spot. The only explanation, Rudnick said, is it's empty of matter.


It could also be a statistical freak of nature, but that's probably less likely than a giant void, said James Condon, an astronomer at the National Radio Astronomy Observatory. He wasn't part of Rudnick's team but is following up on the research.


"It looks like something to be taken seriously," said Brent Tully, a University of Hawaii astronomer who wasn't part of this research but studies the void closer to Earth.


Tully said astronomers may eventually find a few cosmic structures in the void, but it would still be nearly empty.


Holes in the universe probably occur when the gravity from areas with bigger mass pull matter from less dense areas, Tully said. After 13 billion years "they are losing out in the battle to where there are larger concentrations of matter," he said.

Retired NASA astronomer Steve Maran said of the discovery: "This is incredibly important for something where there is nothing to it."





Greatest Mysteries: Where is the Rest of the Universe?

Dave Mosher

Staff Writer

SPACE.com 

 

Scientists trying to create a detailed inventory of all the matter and energy in the cosmos run into a curious problem--the vast majority of it is missing.


"I call it the dark side of the universe," said Michael Turner, a cosmologist at the University of Chicago, referring to the great mysteries of dark matter and dark energy.


In fact, only 4 percent of the matter and energy in the universe has been found. The other 96 percent remains elusive, but scientists are looking in the farthest reaches of space and deepest depths of Earth to solve the two dark riddles.


Missing matter

 

Einstein's famous equation "E=mc^2" describes energy and matter (or mass) as one and the same--maps of the cosmos refer to the energy-matter combination as energy density, for short. The problem with detecting dark matter, thought to make up 22 percent of the universe's mass/energy pie, is that light doesn't interact with it.

But it does exhibit the tug of gravity.


Initial evidence for the mysterious matter was discovered 75 years ago when astrophysicists noticed an anomaly in a jumble of galaxies: The galactic cluster had hundreds of times more gravitational pull than it should have, far outweighing its visible mass of stars.


"We can predict the motions of the sun and planets very accurately, but when we measure distant things we see anomalies," said Scott Dodelson, an astrophysicist at Fermi National Accelerator Laboratory in Illinois. "Dark matter is currently the best possible solution, even though we've never seen any of it."


Another hallmark of dark matter is gravitational lensing, similar to the effect of light passing through a piece of polished glass. Massive objects like the sun can bend light, but colossal clouds of dark matter create "bubbles" in the cosmos that magnify, distort and duplicate the light of galaxies or stars behind them.


Gravitational lensing recently exposed evidence of the unseen mass in the Bullet cluster as well as in a ring around a cluster of colliding galaxies called ZwCl0024+1652.


Particle hunt

 

In spite of the ghostly evidence, pieces of dark matter have yet to be pinned down by researchers. "Until we actually discover particles, we're not home yet," Dodelson said.


Particle physicists have detected neutrinos, which are extremely lightweight particles that pour out of the sun and hardly interact into ordinary matter, but Turner said they make up an extremely small fraction of dark matter in the universe.

"We arrested one of the members of the gang, but not the leader of the gang," Turner said of neutrinos. He thinks the leader is actually a WIMP: a weakly interactive, massive particle. Unfortunately, WIMPS are just a theory so far.


The thinking goes that WIMPs are very heavy, yet like neutrinos they rarely bump into matter to produce a detectable signal. But the idea that WIMPS--such as theoretical axion or neutralino particles--can bump into visible matter at all gives scientists hope.


"This is a story that may soon be at its end," Turner said, noting that the Cryogenic Dark Matter Search in the Soudan mine of Minnesota and other experiments below the ground should be sensitive enough to detect a WIMP.


The anti-gravity

 

Perhaps the biggest mystery of all is dark matter's big cousin, dark energy.


The invisible force is thought to be a large-scale "anti-gravity," pushing apart galactic clusters and causing the unexplainable, accelerating expansion of the universe. Turner thinks dark energy is the biggest mystery of them all--and quite literally, since physicists predict that it makes up 74 percent of energy density in the universe.

"So far, the greatest achievement with dark energy is giving it a name," Turner said of the elusive force. "We are really at the very beginning of this puzzle."


Turner described dark energy as "really weird stuff," best thought of as an elastic, repulsive gravity that can't be broken down into particles. "We know what it does, but we don't know what it is," Turner said.

While astrophysicists look deep into space to gather more details about dark energy's effects, Turner noted that theoretical physicists are focusing on explaining how the force actually works. And at this point, he joked, any physicist's explanation for dark energy is probably good enough to consider.


"We're at this very early stage, at the crime scene of dark energy's existence, if you will," Turner said. "It's a highly creative period, and now is the time for ideas."


Copyright © 2007 SPACE.com


Click for Full Sized Pop-up






NASA's Hubble Space Telescope photographed three magnificent sections of the Veil Nebula

-- the shattered remains of a supernova that exploded thousands of years ago. This series of images provides beautifully detailed views of the delicate, wispy structure resulting from this cosmic explosion. The Veil Nebula is one of the most spectacular supernova remnants in the sky. The entire shell spans about 3 degrees on the sky, corresponding to about 6 full moons.







Click for Larger Scale Image


Technical facts about this news release:


About the Object

Object Name:

Veil Nebula

Object Description:

Supernova Remnant

Position (J2000):

R.A. 20h 50m

Dec. +30° 30'

Constellation:

Cygnus

Distance:

Approximately 1,500 light-years (460 pc) away.

About the Data

Data Description:

The Hubble image was created from HST data from proposals 5774 and 5779: J. Hester (Arizona State Universitry) and J. Westphal (Caltech).

Instrument:

WFPC2

Exposure Date(s):

November 1994, August 1997

Filters:

F502N ([O III]), F656N (Halpha), and F673N ([S II])

About the Image

Image Credit:

NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration

Release Date:

August 2, 2007

Color:

This image is a composite of many separate exposures made by the WFPC2 instrument on the Hubble Space Telescope. Three filters were used to sample narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are:


F502N ([O III])

blue

F656N (Halpha)

green

F673N ([S II])

red

Copyright Notice

Material credited to STScI on this article was created, authored, and/or prepared for NASA under Contract NAS5-26555. Unless otherwise specifically stated, no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA's contract.


 

Report: NASA let astronauts fly drunk


NASA let astronauts fly drunk on at least two occasions, an independent panel said in a report released Friday.


The report gave no names and did not say when the drinking occurred, how many astronauts were involved, or whether they were flying on the space shuttle, the Russian Soyuz spaceship, or aboard NASA's training airplanes.


NASA officials let them fly even after flight surgeons and fellow astronauts raised concerns that flight safety might be jeopardized, according to the report, done by a panel created by NASA after the arrest of astronaut Lisa Nowak in February on charges she tried to kidnap her rival in a love triangle.


In a statement Friday, NASA said the panel has not given the space agency details of the allegations. "As a result, NASA must independently determine the facts of the reported incidents," the space agency said.


The panel said that astronauts and flight surgeons told the committee about heavy drinking by crew members just before flights. Also, the panel said alcohol is freely used in the crew quarters, where astronauts are quarantined at the Kennedy Space Center in the three days before launch.


Only four paragraphs of the 12-page report dealt with alcohol use by astronauts.


"Two specific instances were described where astronauts had been so intoxicated prior to flight that flight surgeons and-or fellow astronauts raised concerns to local on-scene leadership regarding flight safety," the panel. "However, the individuals were still permitted to fly."


The panel said that NASA is not set up in such a way to deal with such problems.


"The medical certification of astronauts for flight duty is not structured to detect such episodes, nor is any medical surveillance program by itself likely to detect them or change the pattern of alcohol use," the panel wrote.

The panel recommended that NASA hold individuals and supervisors accountable for responsible use of alcohol, and that policies be instituted involving drinking before flight.


In another finding, the panel reported that flight surgeons' medical opinions were not valued by higher-ups. Several senior flight surgeons told the panel that officials only wanted to hear that all medical systems "were `go' for on-time mission completion."


The flight surgeons told the panel that higher-ups in NASA were notified of "major crew medical or behavioral problems," but that the flight surgeons' medical advice was ignored.


"This disregard was described as 'demoralizing' to the point where they said they are less likely to report concerns of performance decrement," the panel wrote. "Crew members raised concerns regarding substandard astronaut task performance which were similarly disregarded."


Fourteen astronauts, all but one with spaceflight experience, were interviewed by the panel, as well as five family members. All volunteered to take part in the review. In addition, eight flight surgeons were interviewed.


Copyright © 2007 The Associated Press. All rights reserved. The information contained in the AP News report may not be published, broadcast, rewritten or redistributed without the prior written authority of The Associated Press


NASA Chief Under Fire For Personal Shuttle Use


CAPE CANAVERAL, FL—NASA Administrator Michael Griffin has yet to respond to recent allegations that he used NASA space shuttles on as many as one dozen unauthorized outings to such destinations as New York City, the French Riviera, and his vacation home near Ketchum, ID.


A report issued Monday by NASA's Oversight Commission indicates a cumulative 1.8 million miles unaccounted for on the Atlantic, Discovery, and Endeavor shuttles. In addition, shuttle pilot James Kelly reported numerous occasions on which he found the pilot seat "adjusted for someone else."


The report also revealed that radio presets on the shuttles had been changed to receive various talk-radio stations from across the country, and that the cargo bays contained foreign items such as an old pair of sneakers, "aviator"-style sunshades, two empty Big Gulp Los Angeles Dodgers collector cups, and CDs that shuttle astronauts say are not theirs.

Griffin's apparent joyrides came to light last week, when sharp-eyed patrons at Georgia's Augusta National Golf Club spotted Discovery in the club's parking lot. Within hours, NASA employees began coming forward with their own observations.


"Every now and then on a Friday, Mr. Griffin would stop by Launch Complex 39B and say, 'Well, I'm off early today, taking the wife shopping on Fifth Avenue,' and I wouldn't think twice about it," said assistant fuel-cell technician Lawrence Clemmons. "But about half an hour later, the ground would shake, I'd hear this earsplitting roar from the pad, and then the shuttle would fly off."


"Sometimes I'd think, 'Hey, it looked like he had his overnight bag with him,'" continued Clemmons. "Then, on Monday, we'd get an e-mail from Mr. Griffin saying he was running behind, but he was just leaving Edwards Air Force Base and he'd be in soon."


Trajectory-optimization engineer Russ Holcum said he'd long suspected that Griffin "had an in" with the staff in Engineering and Fabrication. Said Holcum: "I figured he knew someone who cut him an extra set of keys or two."

Holcum added: "More than once, I heard him ask the Mission Control guys if they'd mind 'counting him down' on his way out before a long weekend."


In a press conference held Tuesday, NASA spokesperson Arjun Congrove apologized to taxpayers for the billions of dollars expended on the unauthorized missions.


"The shuttle costs an estimated $2 billion per launch, not counting delays and repairs, and for Mr. Griffin to use it to take his wife on luxury shopping trips to Europe is not appropriate," Congrove said. "We apologize to affected personnel at NASA, and to the good people of New York City whose homes were vaporized by Mr. Griffin's several unauthorized launches near LaGuardia Airport."


Griffin may face penalties ranging from dismissal to having his salary garnished for the next 376 years in order to pay for fuel.

Columbia Astronomer Offers New Theory Into 400-year-old Lunar Mystery



Image of TLP taken in 1953, courtesy of Columbia's Department of Astronomy. The TLP is the small, bright spot in the center of the image.

- Photo by Leon Stuart


Columbia astronomy professor Arlin Crotts thinks he has solved a 400-year-old mystery: the origin of strange optical flashes often reported as appearing on the moon’s surface.


Transient Lunar Phenomena (TLPs), in which the lunar surface reportedly changes in brightness, blurriness or color, have been photographed and observed by thousands of astronomers over the centuries. Yet explanations of why they occur and even their reality as true lunar phenomena have been hotly debated. The TLPs typically cover a space of a few kilometers and last for several minutes.

Crotts has uncovered a strong statistical relationship between TLPs and so-called outgassing events on the lunar surface. Outgassing occurs when gases trapped beneath a moon or planet are released and, if only briefly, become part of the object’s atmosphere. A key component of this gas is radon.

”People over the years have attributed TLPs to all sorts of effects: turbulence in Earth's atmosphere, visual physiological effects, atmospheric smearing of light like a prism, and even psychological effects like hysteria or planted suggestion“ says Crotts, ”but TLPs correlate strongly with radon gas leaking from the moon. No earth-bound effect can fake that.“

To arrive at his theory, Crotts correlated TLPs with known gas outbursts from the lunar surface as seen by several spacecraft, particularly NASA’s Apollo 15 mission in 1971 and the robotic Lunar Prospector in 1998. What he discovered was a remarkable similarity in the pattern of outgassing event locations recorded by spacecraft across the face of the moon and reported TLP sites.


The pattern was further strengthened after Crotts performed a statistical test to rid the sample list of false reports and one time events that might not represent true outgassing sources. ”The result,“ says Crotts ”shows that some lunar event sites that were the focus of great observer excitement over recent decades disappeared from the more highly refined list of TLP sites.“  Crotts used two catalogs of such sightings amassed and edited three decades ago by now retired astronomers Barbara Middlehurst and Winifred Cameron.


Crotts says this research might lead to optical imaging of the lunar surface that could monitor how, when and where gas escapes from the moon.  While the exact composition of this gas is largely unknown, he explains, hints from previous measurements indicate that it might contain substances beneficial for future moon explorations, especially water.


Until now, Crotts says two factors have worked against researchers solving the mystery of TLPs.  Historically, outgassing has often been discussed by scientists, but many have considered the moon volcanically dead despite moonquakes and episodes of gas, such as argon, observed coming from the lunar surface. Another deterrent to researchers is the daunting volume of visual data associated with TLPs – a fact that plays to Crotts’ particular research interest and skills.


Along with collaborators Professors Paul Hickson from the University of British Columbia, and Thomas Pfrommer and Cameron Hummels of Columbia, Crotts recently built the robotic camera at Cerro Tololo Inter-American Observatory in northern Chile. It will automatically scan the moon for TLPs every few seconds and produce an unbiased map of the distribution, free of potentially flawed sightings due to human error, poor equipment, or improperly recorded observations that have dominated TLP studies until now. The scientists are planning even more monitors and hope they will establish with much greater accuracy the exact locations of gas leaks on the moon.

Crotts says improved TLP maps are already pointing to intriguing features on the lunar surface, and he is currently preparing a separate article on that subject.

 – Written by David Poratta


Jupiter is Changing Stripes


Massive Jupiter is undergoing dramatic atmospheric changes that have never been seen before with the keen "eye" of NASA's Hubble Space Telescope.

Jupiter's turbulent clouds are always changing as they encounter atmospheric disturbances while sweeping around the planet at hundreds of miles per hour. But these Hubble images reveal a rapid transformation in the shape and color of Jupiter's clouds near the equator, marking an entire face of the globe.


The planet is wrapped in bands of yellows, browns, and whites. These bands are produced by the atmosphere flowing in different directions at various latitudes. Lighter-hued areas where the atmosphere rises are called zones. Darker regions where the atmosphere falls are called belts. When these opposing flows interact, storms and turbulence appear.


Between March 25 and June 5, Hubble's Wide Field and Planetary Camera 2 captured entire bands of clouds changing color. Zones have darkened into belts and belts have lightened and transformed into zones. Cloud features have rapidly altered in shape and size.


The image at left shows a thin band of white clouds above Jupiter's equator. The white color indicates clouds at higher altitudes in Jupiter's atmosphere. In the image at right, the band's white hue has turned brown, showing clouds deep within the planet's atmosphere. The whole band appears to have merged with the one below it.


In the same cloud band above the equator, the small swirls in the left-hand image have morphed into larger wave-like features in the right-hand photo. Dominating the band is a dark streak that resembles a snake. This serpent-shaped structure is actually a small tear in the cloud deck, which gives astronomers a view deep within the atmosphere.


Below the equatorial region, the brownish upside-down shark fin in the left-hand image disappears in the photo at right. Appearing instead are brownish tongue-shaped clouds with a stream of white swirls below them.


These global upheavals have been seen before, but not with Hubble's sharp resolution. Astronomers using ground-based telescopes first spied drastic atmospheric transformation in the 1980s. Another major disturbance was seen in the early 1990s, after Hubble was launched into space. The telescope, however, did not have the resolution to view the upheaval in fine detail. These higher-quality Hubble images may help astronomers understand how such global upheavals develop on Jupiter.



Crater Could Solve 1908 Tunguska Meteor Mystery


Dave Mosher

Staff Writer

SPACE.comTue Jun 26, 2007


In late June of 1908, a fireball exploded above the remote Russian forests of Tunguska, Siberia, flattening more than 800 square miles of trees. Researchers think a meteor was responsible for the devastation, but neither its fragments nor any impact craters have been discovered.


Astronomers have been left to guess whether the object was an asteroid or a comet, and figuring out what it was would allow better modeling of potential future calamities.


Italian researchers now think they've found a smoking gun: The 164-foot-deep Lake Cheko, located just 5 miles northwest of the epicenter of destruction.


"When we looked at the bottom of the lake, we measured seismic waves reflecting off of something," said Giuseppe Longo, a physicist at the University of Bologna in Italy and co-author of the study. "Nobody has found this before. We can only explain that and the shape of the lake as a low-velocity impact crater."


Should the team turn up conclusive evidence of an asteroid or comet on a later expedition, when they obtain a deeper core sample beneath the lake, remaining mysteries surrounding the Tunguska event may be solved.


The findings are detailed in this month's online version of the journal Terra Nova.


Submerged evidence

During a 1999 expedition, Longo's team didn't plan to investigate Lake Cheko as an impact crater, but rather to look for meteoroid dust in its submerged sediments. While sonar-scanning the lake's topography, they were struck by its cone-like features.


"Expeditions in the 1960s concluded the lake was not an impact crater, but their technologies were limited," Longo said. With the advent of better sonar and computer technologies, he explained, the lake took shape.


Going a step further, Longo's team dove to the bottom and took 6-foot core samples, revealing fresh mud-like sediment on top of "chaotic deposits" beneath. Still, Longo explained the samples are inconclusive of a meteorite impact.


"To really find out if this is an impact crater," Long said, "we need a core sample 10 meters (33 feet) into the bottom" in order to investigate a spot where the team detected a "reflecting" anomaly with their seismic instruments. They think this could be where the ground was compacted by an impact or where part of the meteorite itself lays: The object, if found, could be more than 30 feet in diameter and weigh almost 1,700 tons-the weight of about 42 fully-loaded semi-trailers.


Caution for now

From a UFO crash to a wandering black hole, wild (and wildly unsupported) explanations for the Tunguska event have been proposed. Alan Harris, a planetary scientist at the Space Science Institute in Boulder, Colorado, said the proposal by Longo's team isn't one of them.

"I was impressed by their work and I don't think it's something you can wave off," said Harris, who was not involved in the research.


Longo and his team "are among the recognized authorities on Tunguska" in the world, Harris told SPACE.com. "It would be thrilling to dig up chunks of the meteor body, if they can manage to. It would lay the question to rest whether or not Tunguska was a comet or asteroid."


Some researchers, however, are less confident in the team's conclusions.


"We know from the entry physics that the largest and most energetic objects penetrate deepest," said David Morrison, an astronomer with NASA's Ames Research Center. That only a fragment of the main explosion reached the ground and made a relatively small crater, without creating a larger main crater, seems contradictory to Morrison.


Harris agreed that physics could work against Longo's explanation, but did note that similar events-with impact craters-have been documented all over the world.


"In 1947, the Russian Sikhote-Alin meteorite created 100 small craters. Some were 20 meters (66 feet) across," Harris said. A site in Poland also exists, he explained, where a large meteor exploded and created a series of small lakes. "If the fragment was traveling slowly enough, there's actually a good chance (Longo's team) will unearth some meteorite material," Harris said.


Longo's team plans to return to Lake Cheko next summer, close to the 100th anniversary of the Tunguska Event. "This is important work because we can make better conclusions about how cosmic bodies impact the Earth, and what they're made of," Longo said. "And it could help us find ways to protect our planet from future impacts of this kind."


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Earth's Future Glimpsed on Titan


Charles Q. Choi

SPACE.comTue Jun 12-07 


The enigmatic Saturnian moon Titan is still yielding surprising new details years after scientists first pierced its thick haze veil. The vision now emerging of Saturn's largest moon, with its giant dunes and oceanless surface, is perhaps a glimpse of Earth's desert future.


"Titan may be very different from Earth today, but maybe not Earth tomorrow," Jonathan Lunine, Cassini-Huygens interdisciplinary scientist at the University of Arizona, told SPACE.com.


The surface of Titan was a total mystery before the Huygens probe infiltrated past its dense hazy atmosphere in 2005. After a seven-year voyage aboard the Cassini spacecraft, Huygens spent roughly two-and-a-half hours parachuting down and then sent transmissions from Titan's surface for another 70 minutes before Cassini moved out of range. The mission was a joint project of NASA, the European Space Agency and the Italian Space Agency.


"Even though we have only four hours of data, it is so rich that after two years of work we have yet to retrieve all the information it contains," says François Raulin, Huygens interdisciplinary scientist at the Laboratory of Environmental Physics and Chemistry in Paris.


Lunine explained that "a number of instruments aboard Huygens simply require quite a lot of calibration and cross-checking to get a sensible result."


Episodic rain

Stereoscopic images from Huygens now reveal extremely rugged terrain in the bright highlands north of the probe's landing site. This includes channels divided by ridges that can rise some 500 to 650 feet high, with slopes of 30 degrees. Their shapes suggest they are drainage channels, cut by liquid methane falling as rain, findings detailed in a special issue of Planetary and Space Science magazine.


"Rains on deserts on Earth can take be spaced by months to years, but on Titan we're talking about hundreds, maybe thousands, of years between episodes of major rainfall that comes down perhaps violently," Lunine said. "Because Titan is so much farther from the sun than Earth is, it takes longer for solar energy to evaporate methane and build it up in the atmosphere enough to generate storms."


The fact that methane apparently moves from the atmosphere to the surface and back again on Titan just as water does on Earth makes Titan "in some ways the best analog for an Earth-like planet we have," Lunine said, as compared to Mars, which has too tenuous an atmosphere, or Venus, which has just the opposite. "Essentially all the processes we see in Titan are in some sense connected with methane, just as processes on Earth are in some sense involved with water."


Desert world

Before Huygens penetrated Titan's haze, scientists suspected oceans of liquid methane and ethane covered its surface, evaporation from which could explain the smog-like compounds in its atmosphere.


Instead, they found giant dunes likely composed of sugar-sized hydrocarbon grains girdling its equator, each stretching up to 60 miles long across dark plains that bear markings suggesting occasional flash flooding.


Any surface lakes and seas might be confined to Titan's polar regions.

"There's a sense here of a desert world. Not in terms of being hot-Titan is very cold-but in terms of being very dry," Lunine said. "Titan lacks oceans, but someday Earth will, too, as the sun increases in brightness, boiling the oceans away and leaving Earth a desert planet."


Hidden liquid

Mysteries remain as to where the liquid that carved Titan's valleys, channels and gullies is hiding. Enigmatic radio waves Huygens detected could help reveal this liquid is hiding in the deep interior of Titan, perhaps released by geysers or vulcanism.


The probe's Permittivity, Waves and Altimetry (PWA) sensor detected an extremely low frequency (ELF) radio wave during Huygens' descent. If this signal is natural and not accidentally generated by the instrument, studying how ELF waves resonate on Titan could shed light on any oceans that may exist below Titan's surface and how deep they are. Researchers have already ruled out electrical interference from the instrument itself.


As to what may have generated this ELF wave in the first place, no one is quite sure yet.

"It might be generated by an interaction with Saturn's magnetosphere or related to Titan's intrinsic fields," suggested Fernando Simões, a member of the PWA team. "Titan is proving to be an intriguing environment."



Nasa Unveils Hubble's Successor 



The James Webb Space Telescope (JWST) is intended to replace the ageing Hubble telescope. Image of New Mirror


It will be larger than its predecessor, sit farther from Earth and have a giant mirror to enable it to see more.


Officials said the JWST - named after a former Nasa administrator - was on course for launch in June 2013.


The full-scale model is being displayed outside the Smithsonian National Air and Space Museum in the US capital, Washington DC.


It was recently shown off in Seattle at the American Astronomical Society meeting.



The $4.5bn (£2.3bn) telescope will take up a position some 1.5 million km (930,000 miles) from Earth.


It will measure 24m (80ft) long by 12m (40ft) high and incorporate a hexagonal mirror 6.5m (21.3ft) in diameter, almost three times the size of Hubble's.


Hubble, launched in 1990, has sent back pictures of our solar system, distant stars, and remote fledgling galaxies formed not long after the Big Bang.


But scientists say the JWST will enable them to look deeper into space and even further back at the origins of the Universe.


"Clearly we need a much bigger telescope to go back much further in time to see the very birth of the Universe," said Edward Weiler, director of Nasa's Goddard Space Flight Centre.


Martin Mohan of Northrop Grumman, the contractor building the telescope, said that the team was making excellent progress.


"There's engineering to do, but invention is done, more than six years ahead of launch," he said.


When ready, the JWST will be launched by a European Ariane 5 rocket. It is expected to have a 10-year lifespan.


Until then, the 17-year-old Hubble telescope will continue to do its work. Nasa plans to send astronauts on the space shuttle to service it in 2008.





California-Sized Area of Ice Melts in Antarctica

LiveScience Staff


LiveScience.comTue May 15, 2007


Warm temperatures melted an area of western Antarctica that adds up to the size of California in January 2005, scientists report.


Satellite data collected by the scientists between July 1999 and July 2005 showed clear signs that melting had occurred in multiple distinct regions, including far inland and at high latitudes and elevations, where melt had been considered unlikely.


”Antarctica has shown little to no warming in the recent past with the exception of the Antarctic Peninsula,“ said Konrad Steffen of the University of Colorado, Boulder. ”But now large regions are showing the first signs of the impacts of warming as interpreted by this satellite analysis.“


Changes in the ice mass of Antarctica, Earth's largest freshwater reservoir, are important to understanding global sea level rise. Large amounts of Antarctic freshwater flowing into the ocean also could affect ocean salinity, currents and global climate.


NASA’s QuikScat satellite detected snowmelt by radar pulses that bounce off of ice that formed when snowmelt refroze (just as ice cream turns to ice when it is refrozen after being left out on the counter too long.)


Maximum high temperatures of 41 degrees Fahrenheit that persisted for about a week in Antarctica caused a melt intense enough to create an extensive ice layer.


Evidence of melting was found up to 560 miles inland from the open ocean, farther than 85 degrees south (about 310 miles from the South Pole) and higher than 6,600 feet above sea level.


Water from the melted snow can penetrate cracks and the ice, lubricating the continent’s ice sheets, sending them toward the ocean faster and raising sea levels, the scientists said.


”Increases in snowmelt, such as this in 2005, definitely could have an impact on larger scale melting of Antarctica’s ice sheets if they were severe or sustained over time,“ Steffen said.


No further melting has been detected through March 2007.



NASA Finds Vast Regions of West Antarctica Melted in Recent Past


05.15.07



A team of NASA and university scientists has found clear evidence that extensive areas of snow melted in west Antarctica in January 2005 in response to warm temperatures. This was the first widespread Antarctic melting ever detected with NASA's QuikScat satellite and the most significant melt observed using satellites during the past three decades. Combined, the affected regions encompassed an area as big as California.


Son Nghiem of NASA's Jet Propulsion Laboratory, Pasadena, Calif., and Konrad Steffen, director of the Cooperative Institute for Research in Environmental Sciences at the University of Colorado, Boulder, led the team. Using data from QuikScat, they measured snowfall accumulation and melt in Antarctica and Greenland from July 1999 through July 2005.


Image of AntArticaThe observed melting occurred in multiple distinct regions, including far inland, at high latitudes and at high elevations, where melt had been considered unlikely. Evidence of melting was found up to 900 kilometers (560 miles) inland from the open ocean, farther than 85 degrees south (about 500 kilometers, or 310 miles, from the South Pole) and higher than 2,000 meters (6,600 feet) above sea level. Maximum air temperatures at the time of the melting were unusually high, reaching more than five degrees Celsius (41 degrees Fahrenheit) in one of the affected areas. They remained above melting for approximately a week.


"Antarctica has shown little to no warming in the recent past with the exception of the Antarctic Peninsula, but now large regions are showing the first signs of the impacts of warming as interpreted by this satellite analysis," said Steffen. "Increases in snowmelt, such as this in 2005, definitely could have an impact on larger-scale melting of Antarctica's ice sheets if they were severe or sustained over time."


The satellite's scatterometer instrument sends radar pulses to the ice sheet surface, measuring the echoed pulses that bounce back. When snow melts and then refreezes, it changes to ice, just as ice cream crystallizes when it is left out too long and is then refrozen. QuikScat can differentiate this icy fingerprint in the snow cover and can map on a continental scale the extent of strong snowmelt and the subsequently formed ice layer. Available ground station measurements validate the satellite results.


The 2005 melt was intense enough to create an extensive ice layer when water refroze after the melt. However, the melt was not prolonged enough for the melt water to flow into the sea.


"Water from melted snow can penetrate into ice sheets through cracks and narrow, tubular glacial shafts called moulins," Steffen said. "If sufficient melt water is available, it may reach the bottom of the ice sheet. This water can lubricate the underside of the ice sheet at the bedrock, causing the ice mass to move toward the ocean faster, increasing sea level."


Changes in the ice mass of Antarctica, Earth's largest freshwater reservoir, are important to understanding global sea level rise. Large amounts of Antarctic freshwater flowing into the ocean also could affect ocean salinity, currents and global climate.


Nghiem said while no further melting had been detected through March 2007, more monitoring is needed. "Satellite scatterometry is like an X-ray that sees through snow and finds ice layers beneath as early as possible," he said. "It is vital we continue monitoring this region to determine if a long-term trend may be developing."


QuikScat data are helping scientists better understand how Antarctica's and Greenland's ice sheets gain or lose mass. "We need to know what's coming in and going out of the ice sheets," Nghiem said. "QuikScat data, combined with data from NASA's IceSat and Gravity Recovery and Climate Experiment satellites, along with aircraft and ground measurements, all contribute to more accurate estimates of how the polar ice sheets are changing."


The study, "Snow Accumulation and Snowmelt Monitoring in Greenland and Antarctica," appears in the recently published book "Dynamic Planet."


Additional media contacts for this story include Jim Scott of the University of Colorado, Boulder, at 303-492-3114, or Adriana Raudzens Bailey of the Cooperative Institute for Research in Environmental Sciences, Boulder, at 303-492-6289.


For more information about QuikScat, visit: http://winds.jpl.nasa.gov/index.cfm .


JPL is managed for NASA by the California Institute of Technology in Pasadena.



 


 

Note: I consider this story serious enough to include it here.  M13

 

Honeybee Die-Off Threatens Food Supply


By SETH BORENSTEIN, AP Science Writer

May 2, 2007

 

Unless someone or something stops it soon, the mysterious killer that is wiping out many of the nation's honeybees could have a devastating effect on America's dinner plate, perhaps even reducing us to a glorified bread-and-water diet.


Honeybees don't just make honey; they pollinate more than 90 of the tastiest flowering crops we have. Among them: apples, nuts, avocados, soybeans, asparagus, broccoli, celery, squash and cucumbers. And lots of the really sweet and tart stuff, too, including citrus fruit, peaches, kiwi, cherries, blueberries, cranberries, strawberries, cantaloupe and other melons.


In fact, about one-third of the human diet comes from insect-pollinated plants, and the honeybee is responsible for 80 percent of that pollination, according to the U.S. Department of Agriculture.


Even cattle, which feed on alfalfa, depend on bees. So if the collapse worsens, we could end up being "stuck with grains and water," said Kevin Hackett, the national program leader for USDA's bee and pollination program.


"This is the biggest general threat to our food supply," Hackett said.

While not all scientists foresee a food crisis, noting that large-scale bee die-offs have happened before, this one seems particularly baffling and alarming.


U.S. beekeepers in the past few months have lost one-quarter of their colonies — or about five times the normal winter losses — because of what scientists have dubbed Colony Collapse Disorder. The problem started in November and seems to have spread to 27 states, with similar collapses reported in Brazil, Canada and parts of Europe.


Scientists are struggling to figure out what is killing the honeybees, and early results of a key study this week point to some kind of disease or parasite.


Even before this disorder struck, America's honeybees were in trouble. Their numbers were steadily shrinking, because their genes do not equip them to fight poisons and disease very well, and because their gregarious nature exposes them to ailments that afflict thousands of their close cousins.


"Quite frankly, the question is whether the bees can weather this perfect storm," Hackett said. "Do they have the resilience to bounce back? We'll know probably by the end of the summer."


Experts from Brazil and Europe have joined in the detective work at USDA's bee lab in suburban Washington. In recent weeks, Hackett briefed Vice President Cheney's office on the problem. Congress has held hearings on the matter.


"This crisis threatens to wipe out production of crops dependent on bees for pollination," Agriculture Secretary Mike Johanns said in a statement.


A congressional study said honeybees add about $15 billion a year in value to our food supply.


Of the 17,000 species of bees that scientists know about, "honeybees are, for many reasons, the pollinator of choice for most North American crops," a National Academy of Sciences study said last year. They pollinate many types of plants, repeatedly visit the same plant, and recruit other honeybees to visit, too.


Pulitzer Prize-winning insect biologist E.O. Wilson of Harvard said the honeybee is nature's "workhorse — and we took it for granted."


"We've hung our own future on a thread," Wilson, author of the book "The Creation: An Appeal to Save Life on Earth," told The Associated Press on Monday.


Beginning this past fall, beekeepers would open up their hives and find no workers, just newborn bees and the queen. Unlike past bee die-offs, where dead bees would be found near the hive, this time they just disappeared. The die-off takes just one to three weeks.


National Academy of Sciences study on pollinators:

http://maarec.cas.psu.edu/ColonyCollapseDisorder.html


National Academy of Sciences study on pollinators: http://www.nap.edu/catalog.php?record_id11761


Copyright © 2007 The Associated Press. All rights reserved. The information contained in the AP News report may not be published, broadcast, rewritten or redistributed without the prior written authority of The Associated Press.




Potentially habitable planet found

By SETH BORENSTEIN, AP Science Writer


For the first time astronomers have discovered a planet outside our solar system that is potentially habitable, with Earth-like temperatures, a find researchers described Tuesday as a big step in the search for "life in the universe."


The planet is just the right size, might have water in liquid form, and in galactic terms is relatively nearby at 120 trillion miles away. But the star it closely orbits, known as a "red dwarf," is much smaller, dimmer and cooler than our sun.


There's still a lot that is unknown about the new planet, which could be deemed inhospitable to life once more is known about it. And it's worth noting that scientists' requirements for habitability count Mars in that category: a size relatively similar to Earth's with temperatures that would permit liquid water. However, this is the first outside our solar system that meets those standards.


"It's a significant step on the way to finding possible life in the universe," said University of Geneva astronomer Michel Mayor, one of 11 European scientists on the team that found the planet. "It's a nice discovery. We still have a lot of questions."


The results of the discovery have not been published but have been submitted to the journal Astronomy and Astrophysics.


Alan Boss, who works at the Carnegie Institution of Washington where a U.S. team of astronomers competed in the hunt for an Earth-like planet, called it "a major milestone in this business."

The planet was discovered by the European Southern Observatory's telescope in La Silla, Chile, which has a special instrument that splits light to find wobbles in different wave lengths. Those wobbles can reveal the existence of other worlds.


What they revealed is a planet circling the red dwarf star, Gliese 581. Red dwarfs are low-energy, tiny stars that give off dim red light and last longer than stars like our sun. Until a few years ago, astronomers didn't consider these stars as possible hosts of planets that might sustain life.

The discovery of the new planet, named 581 c, is sure to fuel studies of planets circling similar dim stars. About 80 percent of the stars near Earth are red dwarfs.


The new planet is about five times heavier than Earth. Its discoverers aren't certain if it is rocky like Earth or if its a frozen ice ball with liquid water on the surface. If it is rocky like Earth, which is what the prevailing theory proposes, it has a diameter about 1 1/2 times bigger than our planet. If it is an iceball, as Mayor suggests, it would be even bigger.


Based on theory, 581 c should have an atmosphere, but what's in that atmosphere is still a mystery and if it's too thick that could make the planet's surface temperature too hot, Mayor said.


However, the research team believes the average temperature to be somewhere between 32 and 104 degrees and that set off celebrations among astronomers.


Until now, all 220 planets astronomers have found outside our solar system have had the "Goldilocks problem." They've been too hot, too cold or just plain too big and gaseous, like uninhabitable Jupiter.

The new planet seems just right — or at least that's what scientists think.


"This could be very important," said NASA astrobiology expert Chris McKay, who was not part of the discovery team. "It doesn't mean there is life, but it means it's an Earth-like planet in terms of potential habitability."


Eventually astronomers will rack up discoveries of dozens, maybe even hundreds of planets considered habitable, the astronomers said. But this one — simply called "c" by its discoverers when they talk among themselves — will go down in cosmic history as No. 1.


Besides having the right temperature, the new planet is probably full of liquid water, hypothesizes Stephane Udry, the discovery team's lead author and another Geneva astronomer. But that is based on theory about how planets form, not on any evidence, he said.


The European Southern Observatory: http://www.eso.org


Copyright © 2007 The Associated Press. All rights reserved. The information contained in the AP News report may not be published, broadcast, rewritten or redistributed without the prior written authority of The Associated Press.



Study: Global Warming Could Hinder Hurricanes

By Andrea Thompson

LiveScience Staff Writer

posted: 17 April 2007

06:01 pm ET

 

Global warming might not fuel more intense hurricanes in the Atlantic after all. Despite increasing ocean temperatures that feed the monstrous storms, climate change may also be ramping up the winds that choke off a hurricane’s development, a new study claims.


”The environmental changes here do not suggest a strong increase in tropical Atlantic hurricane activity during the 21st century,“ said study team member Brian Soden of the University of Miami.


Hurricanes form as storms shoot off the coast of Africa and pull energy from the warm, moist air over the oceans. As the hurricane intensifies, it begins to rotate. But when winds vary in speed and direction at different heights in the atmosphere, a phenomenon known as wind shear, they prevent the organization of the storm’s circulation, stopping its development or intensification.


Other studies have found that global warming will increase ocean temperatures over the coming century, fueling more intense hurricanes, but this study is the first to suggest that wind shear may also increase and counteract the effects of ocean warming.


”Wind shear is one of the dominant controls to hurricane activity, and the models project substantial increases in the Atlantic,“ said study leader Gabriel Vecchi of the National Oceanic and Atmospheric Administration. ”Based on historical relationships, the impact on hurricane activity of the projected shear change could be as large—and in the opposite sense—as that of the warming oceans.“


Kevin Trenberth, a climate scientist with the National Center for Atmospheric Research who was not affiliated with the study, pointed out that the model predictions in the new study were  averaged. For a given four-year period, for instance, three years could yield suppressed hurricane development, while the fourth could turn out like 2005 (the season that generated Hurricane Katrina), he said.


The models used in the study, detailed in the April 18 issue of the journal Geophysical Research Letters, did show that global warming could lead to a more favorable environment for hurricanes to develop in other regions, including the western tropical Pacific.


”This study does not, in any way, undermine the widespread consensus in the scientific community about the reality of global warming,“ Soden said. ”In fact, the wind shear changes are driven by global warming.“




Next time you look at Orion, consider this...












Porter Garden Telescope Changes Hands

April 9, 2007

by Roger W. Sinnott


It’s not every day that a Porter Garden Telescope goes on the auction block — try once a decade or so. But this did happen March 24th at the Science & Technology Auction held by Skinner, Inc., in Boston, Massachusetts. A bidder from the Internet quickly snapped it up for $18,000, to the dismay of several hopefuls in the audience almost before they could react.


Russell W. Porter, founder of the amateur-telescope-making movement in America, designed and patented this fully operational 6-inch f/4 telescope in the 1920s. Magazines like House Beautiful and Country Life carried ads for them. Their ornate bronze castings were meant to stay outdoors as garden statuary, the owner simply detaching the primary mirror and eyepiece-diagonal assembly to take in out of the weather.

Perhaps fewer than 60 garden telescopes were ever made. Porter biographer Berton C. Willard knows of only 14 that have certainly survived, one being serial number 49 at the Smithsonian Institution in Washington, DC. (But if you’ve ”gotta have one,“ take note: A fully functioning reproduction of the garden telescope should be available this summer.)


Another Porter item in the sale was a rugged, pier-mounted 6-inch reflector that looked a little the worse for wear. No surprise here: It is believed to have been hauled by mule up various mountains to perform site tests for the Hale 200-inch reflector in the 1930s. Fitted with its original primary mirror inscribed "R.W.P., Fred" (referring to Porter’s friend and collaborator, Fred B. Ferson of Biloxi, Mississippi), it fetched $1,000.

The bidding reached $1,300 on a 4-inch refractor by the early-20th-century American maker W. & D. Mogey, but that wasn't high enough to meet the reserve placed on it by its owner. Right afterward, however, an original printed catalog from the Mogey firm sold for $150.


Among other items, an octant by the London firm of Spencer, Browning & Rust went for $2,500. Also on display was a rare school’s tellurion and hand-cranked orrery showing a miniature Earth, Moon, seven planets, and their satellites as known in the 1850s. This auction highlight brought $37,500. (Note: All amounts mentioned in this article are ”hammer prices“ and do not include buyer’s premium.)


The Liquid Lens: Telescope Technology Takes a Leap

By Barry Shanko

Special to SPACE.com

posted: 08:00 am ET

24 September 2000

 

So many astronomers, so little time -- telescope time that is.

Todays behemoths cost hundreds of millions of dollars. Since individual ownership is impossible they must be shared. Until now.


Later this year, at a cost of slightly more than a million dollars, a team of astronomers has exclusive use of a telescope larger than the Mount Palomar giant. What makes it inexpensive is not the ski-chalet-like wood frame observatory or the aluminum tubes that suspends the instruments over the main mirror, but the mirror itself.


By a happy accident of physics, a spinning liquid forces its surface into the perfect shape for a telescope mirror. Capitalizing on this, scientists at the University of British Columbia (UBC) have built a 236-inch (6-meter) Liquid Mirror Telescope, or LMT, set to capture its "first light" later this summer.

A telescope mirror's job is to hold a thin reflecting layer in the right shape. Over the years astronomers have used polished metal, solid glass and large mirrors created from many smaller ones.

The LMT uses a dish of liquid mercury. If it works, "classical telescopes with solid mirrors will go the way of the great refractors that were replaced with reflecting telescopes," said physicist Ermanno Borra.


Turn, turn, turn


Imagine a lazy Susan holding a bowl full of water. When spinning, the water's surface becomes the perfect shape for a telescope mirror. If the liquid is mercury, an excellent telescope mirror is formed, the core of a Liquid Mirror Telescope [LMT].


Cosmologist Paul Hickson is using this physics to make the world's 13th largest telescope. It collects starlight with a plate of mercury 6 meters across spinning at about 5 rotations per minute.


This University of British Columbia telescope costs about $1 million. A conventional telescope with a regular solid glass mirror of the same size would require an outlay of about $100 million. A large part of the savings comes from not making, polishing, testing and mounting a standard mirror.


The low cost means Hickson and his fellow cosmologists are able to afford a large telescope for their exclusive use to do the science they would like to do -- but can't.


"I didn't start out to be a telescope builder. I only wanted to build a telescope, collect good data and get scientific results," Hickson said.


What's old is new again


It sounds simple: Spin a plate of mercury, place a camera above it at the focal plane and -- voila -- a telescope is born. Yet making it work wasn't easy.


The concept of LMTs can be mapped back to the 18th century. Experiments that utilized the concept were conducted in the 1800s and the early 1900s, but the results were disappointing.


The concept was sound, but the technology available was too crude to make it work. Vibrations from the ground around the telescope made image-smearing waves in the mercury. To achieve sharp images, the focal plane must not move. This requires the rotation of the vessel holding the mercury to vary less than one part in 100,000 during the exposure.


Following these experiments, LMTs were a curiosity in the history of physics until the early 1980s. "It was nearly a forgotten concept that had a bad reputation because past attempts were unsuccessful," said Borra.

After rethinking the idea, he thought that this mirror married to modern technology would give birth to a large, cheap telescope.


In Borra's Laval University lab he began to first experiment with a 19.7-inch (50-centimeter) mirror, quickly progressing to one at 39.5 inches (1-meter). After about a decade, he fabricated a mirror that produced images equal to those made by conventional glass mirrors.


He and his students figured out how to use air bearings to support the vessel holding the mirror. To get sharp images, they also cast a layer of epoxy resin atop the mercury and used a crystal-controlled motor to keep the rotational speed constant.


Turning a mirror into a telescope


A telescope needs more than a mirror. "[I] had been following Borra's work and I realized this could be a way to build a large, low-cost telescope for cosmological surveys" said Hickson.

To discover the large-scale structure of the universe Hickson needs to map the position and distance of millions of galaxies. Only a large telescope will allow him to see the faint galaxies to make this effort worthwhile.


Hickson's hobby is building and flying aircraft, which provided him the base of knowledge to use and shape composite materials like Kevlar and carbon fiber. He invented a lightweight, yet strong cell to hold the mercury.


In the event of a mercury-spilling cell breakage, Hickson dug a waist-deep, epoxy-lined concrete pit to contain the spill. To this floor was bolted one end of an aluminum tube hexapod.


At the other end, directly above the mirror, is attached a platform holding the CCD cameras and other instruments. This represents another cost-saving measure, since the massive piece of metal, called a telescope mount, is eliminated. Hickson noted: "We just throw the mount away."


A costly dome, which shelters many large observing telescopes, isn't required since LMTs only point straight up. At the UBC research forest, 60 miles (97 kilometers) east of Vancouver, British Columbia, Hickson built a ski-chalet-type, 4-story wooden building which uses a roll-off roof.


With the exception of the air bearing and other specialty items, the LMT was built by Hickson and his graduate students, or by tradesmen using locally purchased materials. The result was a professional-sized observatory with a cheap price tag.


Into the unknown


Hickson's first LMT, built in 1993, was 106-inches (2.7-meters). It was intended to be a "proof-of-concept" instrument, but from the beginning the results were "about the same as a conventional glass-mirrored telescope" he said. This proved LMTs' astronomical worth.


It was dismantled two years ago to make way for its larger sibling. "We're taking it one step at a time. We know how to build 3-meter (118-inch) telescopes and we're now developing the technology to make larger ones," he said. The 6-meter starts operation later this year.


Hickson built a near twin of his first LMT for NASA in 1996. It scans low Earth orbit for space junk too small for ground-based radars to see. So far it is finding five times as much stuff as the radars see.

Own your own Palomar


Just as many of us feel like we're not paid enough, many astronomers believe they never get enough time on a large telescope. With new observatories costing $100 million or more, there is no way an individual or a team of like-minded astronomers could hope to own one for their own use.


This leads to rationing. Even astronomers with the most exciting ideas must be satisfied to work with a state-of-the-art instrument like the Keck Observatory in Hawaii for no more than three or four nights a year.

This shortage is holding back cosmological research. Borra notes that in order to do mean