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The Moon Is Wet!

A Shortcut for Detecting Alien Worlds

Evidence of water found on moon

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The ocean is a potentially vast source of electric power, yet as engineers test new technologies for capturing it, the devices are plagued by battering storms, limited efficiency, and the need to be tethered to the seafloor.

Shown is the view from the far downstream end into the test section of the U.S. Air Force Academy water tunnel. Three blades of the cycloidal turbine are visible at the far end. Engineer Stefan Siegel and his colleagues test the turbine using the tunnel, with both steady and oscillating flow conditions simulating a shallow-water wave-flow field. (Credit: SSgt Danny Washburn, U.S. Air Force Academy, Department of Aeronautics)

Shown is the view from the far downstream end into the test section of the U.S. Air Force Academy water tunnel. Three blades of the cycloidal turbine are visible at the far end. Engineer Stefan Siegel and his colleagues test the turbine using the tunnel, with both steady and oscillating flow conditions simulating a shallow-water wave-flow field. (Credit: SSgt Danny Washburn, U.S. Air Force Academy, Department of Aeronautics)

Now, a team of aerospace engineers is applying the principles that keep airplanes aloft to create a new wave-energy system that is durable, extremely efficient, and can be placed anywhere in the ocean, regardless of depth.

While still in early design stages, computer and scale-model tests of the system suggest higher efficiencies than wind turbines. The system is designed to effectively cancel incoming waves, capturing their energy while flattening them out, providing an added application as a storm-wave breaker.

The researchers, from the U.S. Air Force Academy, will present their design at the 62nd annual meeting of the American Physical Society’s Division of Fluid Dynamics on Nov. 24, 2009, in Minneapolis, Minn.

“Our group was working on very basic research on feedback flow control for years,” says lead researcher Stefan Siegel, referring to efforts to use sensors and adjustable parts to control how fluids flow around airfoils like wings. “For an airplane, when you control that flow, you better control flight–for example, enabling you to land a plane on a shorter runway.”

A colleague had read an article on wave energy in a magazine and mentioned it to Siegel and the other team members, and they realized they could operate a wave energy device using the same feedback control concepts they had been developing.

Supported by a grant from the National Science Foundation, the researchers developed a system that uses lift instead of drag to cause the propeller blades to move.

“Every airplane flies with lift, not with drag,” says Siegel. “Compare an old style windmill with a modern one. The new style uses lift and is what made wind energy viable–and it doesn’t get shredded in a storm like an old windmill. Fluid dynamics fixed the issue for windmills, and can do the same for wave energy.”

Windmills have active controls that turn the blades to compensate for storm winds, eliminating lift when it is a risk, and preventing damage.

The Air Force Academy researchers used the same approach with a hydrofoil (equivalent to an airfoil, but for water) and built it into a cycloidal propeller, a design that emerged in the 1930s and currently propels tugboats, ferries and other highly maneuverable ships.

The researchers changed the propeller orientation from horizontal to vertical, allowing direct interaction with the cyclic, up and down motion of wave energy. The researchers also developed individual control systems for each propeller blade, allowing sophisticated manipulations that maximize (or minimize, in the case of storms) interaction with wave energy.

Ultimately, the goal is to keep the flow direction and blade direction constant, cancelling the incoming wave and using standard gear-driven or direct-drive generators to convert the wave energy into electric energy. A propeller that is exactly out of phase with a wave will cancel that wave and maximize energy output.

The cancellation will also allow the float-mounted devices to function without the need of mooring, important for deep-sea locations that hold tremendous wave energy potential and are currently out of reach for many existing wave energy designs.

While the final device may be as large as 40 meters across, laboratory models are currently less than a meter in diameter. A larger version of the system will be tested next year at NSF’s Network for Earthquake Engineering Simulation (NEES) tsunami wave basin at Oregon State University, an important experiment for proving the efficacy of the design.

The conference takes place from Nov. 22-24, 2009, at the Minneapolis Convention Center. The conference is the year’s largest devoted to fluid dynamics, bringing together researchers from across the world and across a wide range of disciplines.

The talk, “Deep Ocean Wave Cancellation Using a Cycloidal Turbine” is by Stefan Siegel, Tiger Jeans, and Thomas McLaughlin of the U.S. Air Force Academy.

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The ocean is a potentially vast source of electric power, yet as engineers test new technologies for capturing it, the devices are plagued by battering storms, limited efficiency, and the need to be tethered to the seafloor.

Shown is the view from the far downstream end into the test section of the U.S. Air Force Academy water tunnel. Three blades of the cycloidal turbine are visible at the far end. Engineer Stefan Siegel and his colleagues test the turbine using the tunnel, with both steady and oscillating flow conditions simulating a shallow-water wave-flow field. (Credit: SSgt Danny Washburn, U.S. Air Force Academy, Department of Aeronautics)

Shown is the view from the far downstream end into the test section of the U.S. Air Force Academy water tunnel. Three blades of the cycloidal turbine are visible at the far end. Engineer Stefan Siegel and his colleagues test the turbine using the tunnel, with both steady and oscillating flow conditions simulating a shallow-water wave-flow field. (Credit: SSgt Danny Washburn, U.S. Air Force Academy, Department of Aeronautics)

Now, a team of aerospace engineers is applying the principles that keep airplanes aloft to create a new wave-energy system that is durable, extremely efficient, and can be placed anywhere in the ocean, regardless of depth.

While still in early design stages, computer and scale-model tests of the system suggest higher efficiencies than wind turbines. The system is designed to effectively cancel incoming waves, capturing their energy while flattening them out, providing an added application as a storm-wave breaker.

The researchers, from the U.S. Air Force Academy, will present their design at the 62nd annual meeting of the American Physical Society’s Division of Fluid Dynamics on Nov. 24, 2009, in Minneapolis, Minn.

“Our group was working on very basic research on feedback flow control for years,” says lead researcher Stefan Siegel, referring to efforts to use sensors and adjustable parts to control how fluids flow around airfoils like wings. “For an airplane, when you control that flow, you better control flight–for example, enabling you to land a plane on a shorter runway.”

A colleague had read an article on wave energy in a magazine and mentioned it to Siegel and the other team members, and they realized they could operate a wave energy device using the same feedback control concepts they had been developing.

Supported by a grant from the National Science Foundation, the researchers developed a system that uses lift instead of drag to cause the propeller blades to move.

“Every airplane flies with lift, not with drag,” says Siegel. “Compare an old style windmill with a modern one. The new style uses lift and is what made wind energy viable–and it doesn’t get shredded in a storm like an old windmill. Fluid dynamics fixed the issue for windmills, and can do the same for wave energy.”

Windmills have active controls that turn the blades to compensate for storm winds, eliminating lift when it is a risk, and preventing damage.

The Air Force Academy researchers used the same approach with a hydrofoil (equivalent to an airfoil, but for water) and built it into a cycloidal propeller, a design that emerged in the 1930s and currently propels tugboats, ferries and other highly maneuverable ships.

The researchers changed the propeller orientation from horizontal to vertical, allowing direct interaction with the cyclic, up and down motion of wave energy. The researchers also developed individual control systems for each propeller blade, allowing sophisticated manipulations that maximize (or minimize, in the case of storms) interaction with wave energy.

Ultimately, the goal is to keep the flow direction and blade direction constant, cancelling the incoming wave and using standard gear-driven or direct-drive generators to convert the wave energy into electric energy. A propeller that is exactly out of phase with a wave will cancel that wave and maximize energy output.

The cancellation will also allow the float-mounted devices to function without the need of mooring, important for deep-sea locations that hold tremendous wave energy potential and are currently out of reach for many existing wave energy designs.

While the final device may be as large as 40 meters across, laboratory models are currently less than a meter in diameter. A larger version of the system will be tested next year at NSF’s Network for Earthquake Engineering Simulation (NEES) tsunami wave basin at Oregon State University, an important experiment for proving the efficacy of the design.

The conference takes place from Nov. 22-24, 2009, at the Minneapolis Convention Center. The conference is the year’s largest devoted to fluid dynamics, bringing together researchers from across the world and across a wide range of disciplines.

The talk, “Deep Ocean Wave Cancellation Using a Cycloidal Turbine” is by Stefan Siegel, Tiger Jeans, and Thomas McLaughlin of the U.S. Air Force Academy.

Start uga_filter:

Astrophysicists at the University of Warwick and Kiel University have discovered two earth sized bodies with oxygen rich atmospheres — however there is a bit of a disappointing snag for anyone looking for a potential home for alien life, or even a future home for ourselves, as they are not planets but are actually two unusual white dwarf stars.

Sloan Digital Sky Survey spectroscopy of this inconspicuous blue object -- SDSS1102+2054 -- reveals it to be an extremely rare stellar remnant: a white dwarf with an oxygen-rich atmosphere (Credit: The Sloan Digital Sky Survey)

Sloan Digital Sky Survey spectroscopy of this inconspicuous blue object -- SDSS1102+2054 -- reveals it to be an extremely rare stellar remnant: a white dwarf with an oxygen-rich atmosphere (Credit: The Sloan Digital Sky Survey)

The two white dwarf stars SDSS 0922+2928 and SDSS 1102+2054 are 400 and 220 light years from Earth. They are both the remnants of massive stars that are at the end of their stellar evolution having consumed all the material they had available for nuclear fusion.

Theoretical models suggest that massive stars (around 7 — 10 times the mass of our own Sun) will consume all of their hydrogen, helium and carbon, and end their lives either as white dwarfs with very oxygen-rich cores, or undergo a supernova and collapse into neutron stars. Finding such oxygen-rich white dwarfs would be an important confirmation of the models.

Unfortunately, almost all white dwarfs have hydrogen and/or helium envelopes that, while low in mass, are sufficiently thick to shield the core from direct view. However should such a core lose its remaining hydrogen envelope, astrophysicists could then detect an extremely oxygen-rich spectrum from the surface of the white dwarf.

Searching within an astronomical data set of the Sloan Digital Sky Survey (SDSS), the University of Warwick and Kiel University astrophysicists did indeed discover two white dwarfs with large atmospheric oxygen abundances.

Lead author on the paper, astrophysicist Dr. Boris Gänsicke from the University of Warwick, said: “These surface abundances of oxygen imply that these are white dwarfs displaying their bare oxygen-neon cores, and that they may have descended from the most massive progenitors stars in that class.”

Most stellar models producing white dwarfs with such oxygen and neon cores also predict that a sufficiently thick carbon-rich layer should surround the core and avoid upward diffusion of large amounts of oxygen. However, calculations also show that the thickness of this layer decreases the closer the progenitor star is to upper mass limit for stars ending their lives as white dwarfs. Hence one possibility for the formation of SDSS 0922+2928 and SDSS 1102+2054 is that they descended from the most massive stars avoiding core-collapse, in which case they would be expected to be very massive themselves. However current data is insufficient to provide any unambiguous measure of the masses of these two unusual white dwarves.

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Astrophysicists at the University of Warwick and Kiel University have discovered two earth sized bodies with oxygen rich atmospheres — however there is a bit of a disappointing snag for anyone looking for a potential home for alien life, or even a future home for ourselves, as they are not planets but are actually two unusual white dwarf stars.

Sloan Digital Sky Survey spectroscopy of this inconspicuous blue object -- SDSS1102+2054 -- reveals it to be an extremely rare stellar remnant: a white dwarf with an oxygen-rich atmosphere (Credit: The Sloan Digital Sky Survey)

Sloan Digital Sky Survey spectroscopy of this inconspicuous blue object -- SDSS1102+2054 -- reveals it to be an extremely rare stellar remnant: a white dwarf with an oxygen-rich atmosphere (Credit: The Sloan Digital Sky Survey)

The two white dwarf stars SDSS 0922+2928 and SDSS 1102+2054 are 400 and 220 light years from Earth. They are both the remnants of massive stars that are at the end of their stellar evolution having consumed all the material they had available for nuclear fusion.

Theoretical models suggest that massive stars (around 7 — 10 times the mass of our own Sun) will consume all of their hydrogen, helium and carbon, and end their lives either as white dwarfs with very oxygen-rich cores, or undergo a supernova and collapse into neutron stars. Finding such oxygen-rich white dwarfs would be an important confirmation of the models.

Unfortunately, almost all white dwarfs have hydrogen and/or helium envelopes that, while low in mass, are sufficiently thick to shield the core from direct view. However should such a core lose its remaining hydrogen envelope, astrophysicists could then detect an extremely oxygen-rich spectrum from the surface of the white dwarf.

Searching within an astronomical data set of the Sloan Digital Sky Survey (SDSS), the University of Warwick and Kiel University astrophysicists did indeed discover two white dwarfs with large atmospheric oxygen abundances.

Lead author on the paper, astrophysicist Dr. Boris Gänsicke from the University of Warwick, said: “These surface abundances of oxygen imply that these are white dwarfs displaying their bare oxygen-neon cores, and that they may have descended from the most massive progenitors stars in that class.”

Most stellar models producing white dwarfs with such oxygen and neon cores also predict that a sufficiently thick carbon-rich layer should surround the core and avoid upward diffusion of large amounts of oxygen. However, calculations also show that the thickness of this layer decreases the closer the progenitor star is to upper mass limit for stars ending their lives as white dwarfs. Hence one possibility for the formation of SDSS 0922+2928 and SDSS 1102+2054 is that they descended from the most massive stars avoiding core-collapse, in which case they would be expected to be very massive themselves. However current data is insufficient to provide any unambiguous measure of the masses of these two unusual white dwarves.

Start uga_filter:

Slamming a spent rocket booster into the frigid, inky shadow of a lunar crater last month sent up a plume of dust laced with water, NASA scientists reported in a press conference today. Observers on Earth were denied a view of the fireworks in October, but “we found water, a significant amount of water,” said LCROSS (Lunar Crater Observation and Sensing Satellite) mission principal investigator Anthony Colaprete of NASA’s Ames Research Center in Mountain View, California.

After several decades of controversy, scientists now know that over billions of years, water from who knows where–impacting comets or perhaps the solar wind–can collect in some of the coldest places in the solar system. Whether the predicted amount of water is enough to sustain future astronauts–as either sustenance or rocket fuel–remains to be seen, however.

The LCROSS mission worked to perfection, with the exception of the show that unfolded on Earth. Before the impact, NASA scientists had predicted that ground-based observers, even amateurs, would see the plume in the gap between two mountains. As it turned out, Colaprete said, the impact’s plume of debris “was as bright as thought, but it was behind a hill” because the debris did not rise as high as impact modeling had suggested.

The heavily instrumented LCROSS spacecraft, however, had a fine view of the rocket booster’s impact and aftermath as it sped to its own impact 4 minutes later. LCROSS instruments delivered a “good, strong detection” of water, Colaprete said. At infrared and ultraviolet wavelengths, they gave clear indications of water vapor, water ice, and hydroxyl ions produced when sunlight splits water molecules.

All told, LCROSS detected about 100 kilograms of water, Colaprete said. It came from a 20-meter-wide crater maybe 3 meters deep, but he declined to guess how abundant water ice had been beneath the impact site. Team members must still calculate what portion of subsurface ice actually rose into view and could have been measured, Colaprete noted. “It would probably be safe to say it’s wetter than the Atacama Desert,” the driest place on Earth, he said. Some remote sensing had suggested about 1% water ice by volume in the upper 3 meters, which was regarded as a substantial amount. Impact modeler and LCROSS team member David Goldstein of the University of Texas, Austin, says 1% “is not inconsistent with what’s been observed. I haven’t convinced myself yet whether it’s 0.1% or 10%. I think we’ll work that out.”

Whatever the amount, the principle of cold-trapping water in permanently shadowed craters–as had been demonstrated for Mercury using radar–is now firmly established for the moon. The LCROSS results give only an inkling of where the water might have come from. Colaprete reported that spectra hint at the presence of volatile compounds besides water, such as carbon dioxide, methane, sulfur dioxide, and methanol, just the sort of compounds found in comets and ice-rich asteroids. So the moon may have retained a tiny bit of the objects that have pummeled it for eons.

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Slamming a spent rocket booster into the frigid, inky shadow of a lunar crater last month sent up a plume of dust laced with water, NASA scientists reported in a press conference today. Observers on Earth were denied a view of the fireworks in October, but “we found water, a significant amount of water,” said LCROSS (Lunar Crater Observation and Sensing Satellite) mission principal investigator Anthony Colaprete of NASA’s Ames Research Center in Mountain View, California.

After several decades of controversy, scientists now know that over billions of years, water from who knows where–impacting comets or perhaps the solar wind–can collect in some of the coldest places in the solar system. Whether the predicted amount of water is enough to sustain future astronauts–as either sustenance or rocket fuel–remains to be seen, however.

The LCROSS mission worked to perfection, with the exception of the show that unfolded on Earth. Before the impact, NASA scientists had predicted that ground-based observers, even amateurs, would see the plume in the gap between two mountains. As it turned out, Colaprete said, the impact’s plume of debris “was as bright as thought, but it was behind a hill” because the debris did not rise as high as impact modeling had suggested.

The heavily instrumented LCROSS spacecraft, however, had a fine view of the rocket booster’s impact and aftermath as it sped to its own impact 4 minutes later. LCROSS instruments delivered a “good, strong detection” of water, Colaprete said. At infrared and ultraviolet wavelengths, they gave clear indications of water vapor, water ice, and hydroxyl ions produced when sunlight splits water molecules.

All told, LCROSS detected about 100 kilograms of water, Colaprete said. It came from a 20-meter-wide crater maybe 3 meters deep, but he declined to guess how abundant water ice had been beneath the impact site. Team members must still calculate what portion of subsurface ice actually rose into view and could have been measured, Colaprete noted. “It would probably be safe to say it’s wetter than the Atacama Desert,” the driest place on Earth, he said. Some remote sensing had suggested about 1% water ice by volume in the upper 3 meters, which was regarded as a substantial amount. Impact modeler and LCROSS team member David Goldstein of the University of Texas, Austin, says 1% “is not inconsistent with what’s been observed. I haven’t convinced myself yet whether it’s 0.1% or 10%. I think we’ll work that out.”

Whatever the amount, the principle of cold-trapping water in permanently shadowed craters–as had been demonstrated for Mercury using radar–is now firmly established for the moon. The LCROSS results give only an inkling of where the water might have come from. Colaprete reported that spectra hint at the presence of volatile compounds besides water, such as carbon dioxide, methane, sulfur dioxide, and methanol, just the sort of compounds found in comets and ice-rich asteroids. So the moon may have retained a tiny bit of the objects that have pummeled it for eons.

Start uga_filter:

Finding new alien worlds may become a lot easier. Astronomers have discovered that stars containing low amounts of the element lithium tend to host solar systems, a result that could dramatically reduce the time it will take to detect another Earth-like planet.

Chemical clue. Stars that form solar systems tend to deplete their lithium content. Credit: ESO/L. Calcada

Thus far, attempting to determine whether other stars play host to planets has required great patience and painstaking measurements. Astronomers scan the skies for two stellar phenomena. One is the barely perceptible but regular dimming of a star’s brightness that occurs when an orbiting planet passes between the star and Earth. The other is the regular but minuscule variation in a star’s radial velocity–its speed through the galaxy relative to Earth’s speed–which indicates that the star is being tugged by an orbiting planet’s gravity. Astronomers casually refer to the two phenomena as blink and wobble. Efforts to detect planets via these methods can take months–and they often come up empty.

Enter lithium. Some young stars form inside a small rotating disk of dust and gas, whereas others coalesce inside a much larger rotating disk, called a protoplanetary disk. Astronomers think that in the former case, the star rotates much faster because it isn’t subject to the gravitational drag imposed by the larger disk. This faster rotation, the thinking goes, pushes the star’s lighter elements, such as lithium, closer to the surface, where they can persist for billions of years. The presence of a protoplanetary disk, on the other hand, could hinder the star’s rotation, thereby causing lithium and other lighter elements to sink deep inside the star’s nuclear furnace, where they are consumed. If these scenarios are correct, stars with low levels of lithium should be more likely to host planets.

That’s what astronomers have found. In today’s issue of Nature, a team led by Garik Israelian of the Instituto de Astrofisica de Canarias in Spain’s Canary Islands surveyed 46 stars in our galactic neighborhood that host planets, along with 116 stars where so far no planets have been detected. Analysis of the light from the 46 stars showed low lithium content, the team reports, whereas the 116 stars all had higher levels of lithium–with over half sporting about 10 times more than the planet-hosting stars.

Physicist Dejan Vinkovi?, of the University of Split in Croatia calls the paper exciting, but he says it’s still unclear exactly why stars that host planets have low lithium levels. It’s possible, he says, that something other than the protoplanetary disk is contributing to the chemical’s loss.

By Phil Berardelli

Start uga_in_feed Ending uga_in_feed: Start uga_track_user Start uga_get_option: ignore_users uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: ignore_users (1) Start uga_get_option: max_user_level uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: max_user_level (8) Tracking user with level 0 Ending uga_track_user: 1 Calling preg_replace_callback: ]*?)href\s*=\s*['"](.*?)['"]([^>]*)>(.*?) Start uga_preg_callback: Array Get tracker for full url Start uga_track_full_url: www.nature.com/nature/journal/v462/n7270/abs/nature08483.html Start uga_is_url_internal: www.nature.com/nature/journal/v462/n7270/abs/nature08483.html Start uga_get_option: internal_domains uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: internal_domains (www.humacon.org,humacon.org) Checking hostname www.humacon.org Checking hostname humacon.org Ending uga_is_url_internal: Get tracker for external URL Start uga_track_external_url: www.nature.com/nature/journal/v462/n7270/abs/nature08483.html Start uga_get_option: track_ext_links uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: track_ext_links (1) Tracking external links enabled Start uga_get_option: prefix_ext_links uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: prefix_ext_links (/outgoing/) Ending uga_track_external_url: www.nature.com/nature/journal/v462/n7270/abs/nature08483.html Ending uga_track_full_url: /outgoing/www.nature.com/nature/journal/v462/n7270/abs/nature08483.html Adding onclick attribute for /outgoing/www.nature.com/nature/journal/v462/n7270/abs/nature08483.html Ending uga_preg_callback: surveyed Ending uga_filter:

Finding new alien worlds may become a lot easier. Astronomers have discovered that stars containing low amounts of the element lithium tend to host solar systems, a result that could dramatically reduce the time it will take to detect another Earth-like planet.

Chemical clue. Stars that form solar systems tend to deplete their lithium content. Credit: ESO/L. Calcada

Thus far, attempting to determine whether other stars play host to planets has required great patience and painstaking measurements. Astronomers scan the skies for two stellar phenomena. One is the barely perceptible but regular dimming of a star’s brightness that occurs when an orbiting planet passes between the star and Earth. The other is the regular but minuscule variation in a star’s radial velocity–its speed through the galaxy relative to Earth’s speed–which indicates that the star is being tugged by an orbiting planet’s gravity. Astronomers casually refer to the two phenomena as blink and wobble. Efforts to detect planets via these methods can take months–and they often come up empty.

Enter lithium. Some young stars form inside a small rotating disk of dust and gas, whereas others coalesce inside a much larger rotating disk, called a protoplanetary disk. Astronomers think that in the former case, the star rotates much faster because it isn’t subject to the gravitational drag imposed by the larger disk. This faster rotation, the thinking goes, pushes the star’s lighter elements, such as lithium, closer to the surface, where they can persist for billions of years. The presence of a protoplanetary disk, on the other hand, could hinder the star’s rotation, thereby causing lithium and other lighter elements to sink deep inside the star’s nuclear furnace, where they are consumed. If these scenarios are correct, stars with low levels of lithium should be more likely to host planets.

That’s what astronomers have found. In today’s issue of Nature, a team led by Garik Israelian of the Instituto de Astrofisica de Canarias in Spain’s Canary Islands surveyed 46 stars in our galactic neighborhood that host planets, along with 116 stars where so far no planets have been detected. Analysis of the light from the 46 stars showed low lithium content, the team reports, whereas the 116 stars all had higher levels of lithium–with over half sporting about 10 times more than the planet-hosting stars.

Physicist Dejan Vinkovi?, of the University of Split in Croatia calls the paper exciting, but he says it’s still unclear exactly why stars that host planets have low lithium levels. It’s possible, he says, that something other than the protoplanetary disk is contributing to the chemical’s loss.

By Phil Berardelli

Start uga_filter:

Scientists announced tonight that they have discovered “buckets” of water on the Moon following the analysis of data from a spacecraft that was deliberately crashed into a lunar crater last month.


The researchers said the evidence for the existence of significant bodies of water ice hidden in polar craters on the Moon is “definitive” and that the total quantities could be big enough to support a permanently-manned lunar base.

It is the first time that the US National Aeronautics and Space Administration (Nasa) has been so categorical about the discovery of water on the Moon. Previous studies had only suggested that the presence of water might be possible and then only in trace amounts.

However, a painstakingly detailed analysis of the data from the LCROSS spacecraft, which was deliberately crashed into the Cabeus crater near the Lunar South Pole, has revealed a definitive chemical signature of water vapour in the plume of dust and debris that was released on impact.

In just one crater, the team estimates that there was at least 100 kilograms of water, enough to fill a dozen, two-gallon buckets. If similar amounts of water exist in other polar craters permanently shaded from sunlight there could be enough water available on the Moon to be used as drinking water for a lunar base – or used as a source of rocket fuel.

Anthony Colaprete, the principal scientist of LCROSS (the Lunar Crater Observation and Sensing Satellite), said that the “eureka moment” came when the team saw a spectroscopic line indicating the presence of the OH water molecule, which could only exist if water was present in the crater.

“What we found was indeed water…We vetted it, vetted it, vetted it, vetted it and vetted it some more as a team…I’m pretty impressed by the amount of water we see in this small, 20-metre crater,” Dr Colaprete said at a press briefing from Nasa’s Ames Research Centre in California.

“It’s safe to say it’s not a frozen lake with a perfectly frozen surface. It was probably mixed in with the surface. It would be an interesting place to walk around,” Dr Colaprete said.

Mike Wargo from Nasa said: “We’ve discovered significant quantities of water in a permanently-shaded crater on the Moon. We’re not just talking of water on the Moon, but lots of water.”

When LCROSS was crashed into the Moon, it was expected to eject a visible plume of debris six-miles high that was supposed to have been visible from Earth. However, Nasa scientists said at the time that the absence of a visible plume did not mean that the mission was a failure.

Nasa’s Gregory Delory said that the discovery is one of the most exciting to be made in connection with lunar exploration. “If we find water in large enough amounts it could be used as a resource for human exploration,” Dr Delory said.

“Now we know there’s water there thanks to LCROSS we can go to the next set of questions. It’s a new picture of the Moon. It’s going to be a very exciting time,” he said.

One of the unresolved questions is how the water could have got to the Moon. One theory is that it arrived on a comet and never evaporated in the shaded polar craters where temperatures are minus 220C.

Another possibility is that the water arrived on a solar wind, which is a stream of ionised hydrogen gas. A third theory is that is was dropped by a molecular cloud, or dropped by ice-laden cosmic dust. It might even be terrestrial water kicked up from Earth in a gigantic asteroid impact.

Nasa estimates that there are 12,500 square kilometres of permanently-shadowed terrain on the Moon and if the top 1 metre of this area were to hold just 1 per cent by mass of water, this would still produce thousands of litres of water.

It is not the first time that spacecraft have crashed into the Moon. In 1998, Nasa’s Lunar Prospector mission was deliberately crashed into a crater, which confirmed the presence of hydrogen, which may or may not have come from ancient stores of frozen water deposited in lunar craters over billions of years by passing comets.

By Steve Connor

Start uga_in_feed Ending uga_in_feed: Start uga_track_user Start uga_get_option: ignore_users uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: ignore_users (1) Start uga_get_option: max_user_level uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: max_user_level (8) Tracking user with level 0 Ending uga_track_user: 1 Calling preg_replace_callback: ]*?)href\s*=\s*['"](.*?)['"]([^>]*)>(.*?) Ending uga_filter:

Scientists announced tonight that they have discovered “buckets” of water on the Moon following the analysis of data from a spacecraft that was deliberately crashed into a lunar crater last month.


The researchers said the evidence for the existence of significant bodies of water ice hidden in polar craters on the Moon is “definitive” and that the total quantities could be big enough to support a permanently-manned lunar base.

It is the first time that the US National Aeronautics and Space Administration (Nasa) has been so categorical about the discovery of water on the Moon. Previous studies had only suggested that the presence of water might be possible and then only in trace amounts.

However, a painstakingly detailed analysis of the data from the LCROSS spacecraft, which was deliberately crashed into the Cabeus crater near the Lunar South Pole, has revealed a definitive chemical signature of water vapour in the plume of dust and debris that was released on impact.

In just one crater, the team estimates that there was at least 100 kilograms of water, enough to fill a dozen, two-gallon buckets. If similar amounts of water exist in other polar craters permanently shaded from sunlight there could be enough water available on the Moon to be used as drinking water for a lunar base – or used as a source of rocket fuel.

Anthony Colaprete, the principal scientist of LCROSS (the Lunar Crater Observation and Sensing Satellite), said that the “eureka moment” came when the team saw a spectroscopic line indicating the presence of the OH water molecule, which could only exist if water was present in the crater.

“What we found was indeed water…We vetted it, vetted it, vetted it, vetted it and vetted it some more as a team…I’m pretty impressed by the amount of water we see in this small, 20-metre crater,” Dr Colaprete said at a press briefing from Nasa’s Ames Research Centre in California.

“It’s safe to say it’s not a frozen lake with a perfectly frozen surface. It was probably mixed in with the surface. It would be an interesting place to walk around,” Dr Colaprete said.

Mike Wargo from Nasa said: “We’ve discovered significant quantities of water in a permanently-shaded crater on the Moon. We’re not just talking of water on the Moon, but lots of water.”

When LCROSS was crashed into the Moon, it was expected to eject a visible plume of debris six-miles high that was supposed to have been visible from Earth. However, Nasa scientists said at the time that the absence of a visible plume did not mean that the mission was a failure.

Nasa’s Gregory Delory said that the discovery is one of the most exciting to be made in connection with lunar exploration. “If we find water in large enough amounts it could be used as a resource for human exploration,” Dr Delory said.

“Now we know there’s water there thanks to LCROSS we can go to the next set of questions. It’s a new picture of the Moon. It’s going to be a very exciting time,” he said.

One of the unresolved questions is how the water could have got to the Moon. One theory is that it arrived on a comet and never evaporated in the shaded polar craters where temperatures are minus 220C.

Another possibility is that the water arrived on a solar wind, which is a stream of ionised hydrogen gas. A third theory is that is was dropped by a molecular cloud, or dropped by ice-laden cosmic dust. It might even be terrestrial water kicked up from Earth in a gigantic asteroid impact.

Nasa estimates that there are 12,500 square kilometres of permanently-shadowed terrain on the Moon and if the top 1 metre of this area were to hold just 1 per cent by mass of water, this would still produce thousands of litres of water.

It is not the first time that spacecraft have crashed into the Moon. In 1998, Nasa’s Lunar Prospector mission was deliberately crashed into a crater, which confirmed the presence of hydrogen, which may or may not have come from ancient stores of frozen water deposited in lunar craters over billions of years by passing comets.

By Steve Connor

Start uga_filter:

An international team of astronomers have found an unexpected link between mysterious ‘dark matter’ and the visible stars and gas in galaxies that could revolutionise our current understanding of gravity.


One of the astronomers, Dr Hongsheng Zhao of the SUPA Centre of Gravity, University of St. Andrews, suggests that an unknown force is acting on dark matter. The findings are published this week in the scientific journal Nature.

Only 4% of the universe is made of known material. Stars and gas in galaxies move so fast that astronomers have speculated that the gravity from a hypothetical invisible halo of dark matter is needed to keep galaxies together. However, a solid understanding of dark matter as well as direct evidence of its existence has remained elusive.

Now the team believes that the interactions between dark and ordinary matter could be more important and more complex than previously thought, and even speculate that dark matter might not exist and that the anomalous motions of stars in galaxies are due to a modification of gravity on extragalactic scales.

Dr. Benoit Famaey (Universities of Bonn and Strasbourg) explains: “The dark matter seems to ‘know’ how the visible matter is distributed. They seem to conspire with each other such that the gravity of the visible matter at the characteristic radius of the dark halo is always the same. This is extremely surprising since one would rather expect the balance between visible and dark matter to strongly depend on the individual history of each galaxy.”

Dr. Zhao at the SUPA Centre of Gravity notes, “The pattern that the data reveal is extremely odd. It’s like finding a zoo of animals of all ages and sizes miraculously having identical, say, weight in their backbones or something. It is possible that a non-gravitational fifth force is ruling the dark matter with an invisible hand, leaving the same fingerprints on all galaxies, irrespective of their ages, shapes and sizes.”

Such a force might solve an even bigger mystery, known as ‘dark energy’, which is ruling the accelerated expansion of the Universe. A more radical solution is a revision of the laws of gravity first developed by Isaac Newton in 1687 and refined by Albert Einstein’s theory of General Relativity in 1916. Einstein never fully decided whether his equation should add an omnipresent constant source, now called dark energy.

Dr Famaey added, “If we account for our observations with a modified law of gravity, it makes perfect sense to replace the effective action of hypothetical dark matter with a force closely related to the distribution of visible matter.”

The implications of the new research could change some of the most widely held scientific theories about the history and expansion of the universe.

Lead researcher Dr. Gianfranco Gentile at the University of Ghent concludes, “Understanding this puzzling conspiracy is probably the key to unlock the formation of galaxies and their structures.”

Start uga_in_feed Ending uga_in_feed: Start uga_track_user Start uga_get_option: ignore_users uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: ignore_users (1) Start uga_get_option: max_user_level uga_options: array ( 'internal_domains' => 'www.humacon.org,humacon.org', 'account_id' => 'UA-10399907-2', 'enable_tracker' => true, 'track_adm_pages' => false, 'ignore_users' => true, 'max_user_level' => '8', 'footer_hooked' => true, 'filter_content' => true, 'filter_comments' => true, 'filter_comment_authors' => true, 'track_ext_links' => true, 'prefix_ext_links' => '/outgoing/', 'track_files' => true, 'prefix_file_links' => '/downloads/', 'track_extensions' => 'gif,jpg,jpeg,bmp,png,pdf,mp3,wav,phps,zip,gz,tar,rar,jar,exe,pps,ppt,xls,doc', 'track_mail_links' => true, 'prefix_mail_links' => '/mailto/', 'debug' => true, 'check_updates' => true, 'version_sent' => '1.6.0', 'advanced_config' => true, ) Ending uga_get_option: max_user_level (8) Tracking user with level 0 Ending uga_track_user: 1 Calling preg_replace_callback: ]*?)href\s*=\s*['"](.*?)['"]([^>]*)>(.*?) Ending uga_filter:

An international team of astronomers have found an unexpected link between mysterious ‘dark matter’ and the visible stars and gas in galaxies that could revolutionise our current understanding of gravity.


One of the astronomers, Dr Hongsheng Zhao of the SUPA Centre of Gravity, University of St. Andrews, suggests that an unknown force is acting on dark matter. The findings are published this week in the scientific journal Nature.

Only 4% of the universe is made of known material. Stars and gas in galaxies move so fast that astronomers have speculated that the gravity from a hypothetical invisible halo of dark matter is needed to keep galaxies together. However, a solid understanding of dark matter as well as direct evidence of its existence has remained elusive.

Now the team believes that the interactions between dark and ordinary matter could be more important and more complex than previously thought, and even speculate that dark matter might not exist and that the anomalous motions of stars in galaxies are due to a modification of gravity on extragalactic scales.

Dr. Benoit Famaey (Universities of Bonn and Strasbourg) explains: “The dark matter seems to ‘know’ how the visible matter is distributed. They seem to conspire with each other such that the gravity of the visible matter at the characteristic radius of the dark halo is always the same. This is extremely surprising since one would rather expect the balance between visible and dark matter to strongly depend on the individual history of each galaxy.”

Dr. Zhao at the SUPA Centre of Gravity notes, “The pattern that the data reveal is extremely odd. It’s like finding a zoo of animals of all ages and sizes miraculously having identical, say, weight in their backbones or something. It is possible that a non-gravitational fifth force is ruling the dark matter with an invisible hand, leaving the same fingerprints on all galaxies, irrespective of their ages, shapes and sizes.”

Such a force might solve an even bigger mystery, known as ‘dark energy’, which is ruling the accelerated expansion of the Universe. A more radical solution is a revision of the laws of gravity first developed by Isaac Newton in 1687 and refined by Albert Einstein’s theory of General Relativity in 1916. Einstein never fully decided whether his equation should add an omnipresent constant source, now called dark energy.

Dr Famaey added, “If we account for our observations with a modified law of gravity, it makes perfect sense to replace the effective action of hypothetical dark matter with a force closely related to the distribution of visible matter.”

The implications of the new research could change some of the most widely held scientific theories about the history and expansion of the universe.

Lead researcher Dr. Gianfranco Gentile at the University of Ghent concludes, “Understanding this puzzling conspiracy is probably the key to unlock the formation of galaxies and their structures.”

Start uga_filter:

The first all-sky maps developed by NASA’s Interstellar Boundary Explorer (IBEX) spacecraft, the initial mission to examine the global interactions occurring at the edge of the solar system, suggest that the galactic magnetic fields had a far greater impact on Earth’s history than previously conceived, and the future of our planet and others may depend, in part, on how the galactic magnetic fields change with time.


“The IBEX results are truly remarkable, with emissions not resembling any of the current theories or models of this never-before-seen region,” says Dr. David J. McComas, IBEX principal investigator and assistant vice president of the Space Science and Engineering Division at Southwest Research Institute. “We expected to see small, gradual spatial variations at the interstellar boundary, some 10 billion miles away. However, IBEX is showing us a very narrow ribbon that is two to three times brighter than anything else in the sky.”

A “solar wind” of charged particles continuously travels at supersonic speeds away from the Sun in all directions. This solar wind inflates a giant bubble in interstellar space called the heliosphere — the region of space dominated by the Sun’s influence in which the Earth and other planets reside. As the solar wind travels outward, it sweeps up newly formed “pickup ions,” which arise from the ionization of neutral particles drifting in from interstellar space. IBEX measures energetic neutral atoms (ENAs) traveling at speeds of roughly half a million to two and a half million miles per hour. These ENAs are produced from the solar wind and pick-up ions in the boundary region between the heliosphere and the local interstellar medium.

The IBEX mission just completed the first global maps of these protective layers called the heliosphere through a new technique that uses neutral atoms like light to image the interactions between electrically charged and neutral atoms at the distant reaches of our Sun’s influence, far beyond the most distant planets. It is here that the solar wind, which continually emanates from the Sun at millions of miles per hour, slams into the magnetized medium of charged particles, atoms and dust that pervades the galaxy and is diverted around the system. The interaction between the solar wind and the medium of our galaxy creates a complex host of interactions, which has long fascinated scientists, and is thought to shield the majority of harmful galactic radiation that reaches Earth and fills the solar system.

“The magnetic fields of our galaxy may change the protective layers of our solar system that regulate the entry of galactic radiation, which affects Earth and poses hazards to astronauts,” says Nathan Schwadron of Boston University’s Center for Space Physics and the lead for the IBEX Science Operations Center at BU.

Each six months, the IBEX mission, which was launched on October 18, 2008, completes its global maps of the heliosphere. The first IBEX maps are strikingly different than any of the predictions, which are now forcing scientists to reconsider their basic assumptions of how the heliosphere is created.

“The most striking feature is the ribbon that appears to be controlled by the magnetic field of our galaxy,” says Schwadron.

Although scientists knew that their models would be tested by the IBEX measurements, the existence of the ribbon is “remarkable” says Geoffrey Crew, a Research Scientist at MIT and the Software Design Lead for IBEX. “It suggests that the galactic magnetic fields are much stronger and exert far greater stresses on the heliosphere than we previously believed.”

The discovery has scientists thinking carefully about how different the heliosphere could be than they expected.

“It was really surprising that the models did not generate features at all like the ribbon we observed,” says Christina Prested, a BU graduate student working on IBEX. “Understanding the ribbon in detail will require new insights into the inner workings of the interactions at the edge of our Sun’s influence in the galaxy.”

Adds Schwadron,”Any changes to our understanding of the heliosphere will also affect how we understand the astrospheres that surround other stars. The harmful radiation that leaks into the solar system from the heliosphere is present throughout the galaxy and the existence of astrospheres may be important for understanding the habitability of planets surrounding other stars.”

IBEX is the latest in NASA’s series of low-cost, rapidly developed Small Explorers space missions. Southwest Research Institute in San Antonio, Texas, leads and developed the mission with a team of national and international partners. NASA’s Goddard Space Flight Center in Greenbelt, Md., manages the Explorers Program for NASA’s Science Mission Directorate in Washington.

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The first all-sky maps developed by NASA’s Interstellar Boundary Explorer (IBEX) spacecraft, the initial mission to examine the global interactions occurring at the edge of the solar system, suggest that the galactic magnetic fields had a far greater impact on Earth’s history than previously conceived, and the future of our planet and others may depend, in part, on how the galactic magnetic fields change with time.


“The IBEX results are truly remarkable, with emissions not resembling any of the current theories or models of this never-before-seen region,” says Dr. David J. McComas, IBEX principal investigator and assistant vice president of the Space Science and Engineering Division at Southwest Research Institute. “We expected to see small, gradual spatial variations at the interstellar boundary, some 10 billion miles away. However, IBEX is showing us a very narrow ribbon that is two to three times brighter than anything else in the sky.”

A “solar wind” of charged particles continuously travels at supersonic speeds away from the Sun in all directions. This solar wind inflates a giant bubble in interstellar space called the heliosphere — the region of space dominated by the Sun’s influence in which the Earth and other planets reside. As the solar wind travels outward, it sweeps up newly formed “pickup ions,” which arise from the ionization of neutral particles drifting in from interstellar space. IBEX measures energetic neutral atoms (ENAs) traveling at speeds of roughly half a million to two and a half million miles per hour. These ENAs are produced from the solar wind and pick-up ions in the boundary region between the heliosphere and the local interstellar medium.

The IBEX mission just completed the first global maps of these protective layers called the heliosphere through a new technique that uses neutral atoms like light to image the interactions between electrically charged and neutral atoms at the distant reaches of our Sun’s influence, far beyond the most distant planets. It is here that the solar wind, which continually emanates from the Sun at millions of miles per hour, slams into the magnetized medium of charged particles, atoms and dust that pervades the galaxy and is diverted around the system. The interaction between the solar wind and the medium of our galaxy creates a complex host of interactions, which has long fascinated scientists, and is thought to shield the majority of harmful galactic radiation that reaches Earth and fills the solar system.

“The magnetic fields of our galaxy may change the protective layers of our solar system that regulate the entry of galactic radiation, which affects Earth and poses hazards to astronauts,” says Nathan Schwadron of Boston University’s Center for Space Physics and the lead for the IBEX Science Operations Center at BU.

Each six months, the IBEX mission, which was launched on October 18, 2008, completes its global maps of the heliosphere. The first IBEX maps are strikingly different than any of the predictions, which are now forcing scientists to reconsider their basic assumptions of how the heliosphere is created.

“The most striking feature is the ribbon that appears to be controlled by the magnetic field of our galaxy,” says Schwadron.

Although scientists knew that their models would be tested by the IBEX measurements, the existence of the ribbon is “remarkable” says Geoffrey Crew, a Research Scientist at MIT and the Software Design Lead for IBEX. “It suggests that the galactic magnetic fields are much stronger and exert far greater stresses on the heliosphere than we previously believed.”

The discovery has scientists thinking carefully about how different the heliosphere could be than they expected.

“It was really surprising that the models did not generate features at all like the ribbon we observed,” says Christina Prested, a BU graduate student working on IBEX. “Understanding the ribbon in detail will require new insights into the inner workings of the interactions at the edge of our Sun’s influence in the galaxy.”

Adds Schwadron,”Any changes to our understanding of the heliosphere will also affect how we understand the astrospheres that surround other stars. The harmful radiation that leaks into the solar system from the heliosphere is present throughout the galaxy and the existence of astrospheres may be important for understanding the habitability of planets surrounding other stars.”

IBEX is the latest in NASA’s series of low-cost, rapidly developed Small Explorers space missions. Southwest Research Institute in San Antonio, Texas, leads and developed the mission with a team of national and international partners. NASA’s Goddard Space Flight Center in Greenbelt, Md., manages the Explorers Program for NASA’s Science Mission Directorate in Washington.

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