Exploding Asteroid Theory Gains Evidence

About 13,000 years ago, woolly mammoths roamed the North American continent and the first known human society in that region, known as the Clovis civilization, lived there as well. But geologic and archeological evidence shows they both suddenly disappeared, and scientists have long debated the mystery of the mass extinction of both animals and humans about 12,900 years ago. At that time, climatic history suggests the Ice Age should have been drawing to a close, but instead rapid climate change initiated an additional 1,300 years of glacial conditions. But scientists couldn’t agree on the cause of the sudden change in climate. However, about two years ago geophysicist Allen West proposed that an asteroid or comet exploded just above the earth’s surface at that time over modern-day Canada, sparking a massive shock wave and heat-generating event that set large parts of the northern hemisphere ablaze, setting the stage for the extinctions. Another scientist set out to prove West wrong, but ended up finding evidence to support the exploding asteroid/comet theory.

Ken Tankersley, Anthropology professor at the University of Cincinnati studied sites in Ohio and Indiana that offers the strongest support yet for the exploding comet/asteroid theory. Samples of diamonds, gold and silver found in the region have been conclusively sourced through X-ray diffractometry to have come from the diamond fields region of Canada.

Tankersley and West both believe the best scenario to explain the presence of these materials this far south is the kind of cataclysmic explosive event described by West’s theory. “We believe this is the strongest evidence yet indicating a comet impact in that time period,” says Tankersley.

Previously, geologists believed the deposits of the gems and precious metals were brought south from the Great Lakes region by glaciers. But they are found at a soil depth consistent with the time frame of the comet/asteroid event.

“My smoking gun to disprove (West) was going to be the gold, silver and diamonds,” Tankersley says. “But what I didn’t know at that point was a conclusion he had reached that he had not yet made public – that the likely point of impact for the comet wasn’t just anywhere over Canada, but located over Canada’s diamond-bearing fields. Instead of becoming the basis for rejecting his hypothesis, these items became the very best evidence to support it.”

Additional work is being done at the sites looking for iridium, micro-meteorites and nano-diamonds that bear the markers of the diamond-field region, which also should have been blasted by the impact into this region.

As Tankersley, West and additional scientists compile more data, they’ll be looking for more clues to help explain the history of our planet and its climate.

“The kind of evidence we are finding does suggest that climate change at the end of the last Ice Age was the result of a catastrophic event,” Tankersley says. “The ultimate importance of this kind of work is showing that we can’t control everything,” he says. “Our planet has been hit by asteroids many times throughout its history, and when that happens, it does produce climate change.”

Original Source: Science Daily

Satellites Keep an Eye on Wildfires Around the World

Wildfire season is underway in the northern hemisphere, and with hot and dry conditions in many areas this summer, fires have been plentiful. Regions affected include central Canada, California in the US, Southeastern Russia and Norway. While wildfires are a natural part of Earth’s environment when sparked by lightning strikes, these fires consume a million or more square kilometers per year. Wildfires can also be started from volcano eruptions, but humans also start many fires -sometimes accidentally, but mostly deliberately. Both NASA and ESA have Earth-watching satellites that have been keeping an eye on wildfires around the world. Above, the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite captured this natural-color image of wildfires in Central Canada, in the Saskatchewan and Manitoba Provinces on June 30, 2008. Places where the sensor detected actively burning fires are marked in red; a strong wind was blowing east-southeast and spreading thick plumes of gray-brown smoke.


Thunderstorms in California brought lightning but little rain, starting several wildfires. This natural-color image was captured by MODIS on July 2, 2008, and it shows the location of actively burning fires marked in red. The highest concentration of fires is in Northern California, where reportedly 68 uncontained large fires were burning as of July 3. Meanwhile, Southern California was battling the state’s two largest blazes, shown in the lower half of this image.

These false-color images of the Santa Lucia Range Mountains near Big Sur, California, was captured by Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA’s Terra satellite on June 29, 2008. Vegetation is red, naturally bare ground is tan, burned ground is charcoal colored, and smoke is light blue. Clouds over the Pacific Ocean to the southwest are bright bluish white. Over 120,000 acres have been burned by the two large wildfires in this area.


With extremely hot weather conditions in Europe, Norway experienced its biggest forest fire in the last half century in June. ESA’s Envisat satellite images were used in the fire’s aftermath to get an overview of the damaged area for authorities and insurance companies. The Envisat Advanced Synthetic Aperture Radar (ASAR) image shows the burned area as a red cluster in the image center.

The fires (red dots) visible along the shoreline of Russia’s Khabarovsk Province at the upper left of this image are only a few of the forest fires responsible for the river of smoke spreading eastward over the Sea of Okhotsk and the Kamchatka Peninsula on July 2, 2008. This natural-color image of the area was captured by MODIS on NASA’s Aqua satellite. Like this image, many images area developed daily from orbiting satellites to to provide up-to-date satellite images of the Earth’s landmasses in near real time. The MODIS Rapid Response Team provides these images, many times with a few hours of being collected. This system is valuable resource for the international fire monitoring community, who use the images to track fires.

News sources: NASA’s Earth Observatory Natural Hazards site, ESA’s Observing the Earth site

“Starlight Zone” Interview Now Online

The interview that I (Nancy) did with the “Starlight Zone” radio show from station 2NUR FM in Newcastle, Australia back on June 19 is now online (or just listen below). It’s only five minutes long, so if you need a short diversion to your day…. We talked about the concept of a one-way trip to Mars and the Phoenix mission.

Col Maybury, who does the show was a very fun guy to talk with. Check out all the past interviews he’s done with various “spacey” people on 2NUR’s “Starlight Zone” website.

G’day!

Theory of Relativity Passes Another Test

Einstein’s theory of General Relativity has been around for 93 years, and it just keeps hanging in there. With advances in technology has come the ability to put the theory under some scrutiny. Recently, taking advantage of a unique cosmic coincidence, as well as a pretty darn good telescope, astronomers looked at the strong gravity from a pair of superdense neutron stars and measured an effect predicted by General Relativity. The theory came through with flying colors.

Einstein’s 1915 theory predicted that in a close system of two very massive objects, such as neutron stars, one object’s gravitational tug, along with an effect of its spinning around its axis, should cause the spin axis of the other to wobble, or precess. Studies of other pulsars in binary systems had indicated that such wobbling occurred, but could not produce precise measurements of the amount of wobbling.

“Measuring the amount of wobbling is what tests the details of Einstein’s theory and gives a benchmark that any alternative gravitational theories must meet,” said Scott Ransom of the National Radio Astronomy Observatory.

The astronomers used the National Science Foundation’s Robert C. Byrd Green Bank Telescope (GBT) to make a four-year study of a double-star system unlike any other known in the Universe. The system is a pair of neutron stars, both of which are seen as pulsars that emit lighthouse-like beams of radio waves.

“Of about 1700 known pulsars, this is the only case where two pulsars are in orbit around each other,” said Rene Breton, a graduate student at McGill University in Montreal, Canada. In addition, the stars’ orbital plane is aligned nearly perfectly with their line of sight to the Earth, so that one passes behind a doughnut-shaped region of ionized gas surrounding the other, eclipsing the signal from the pulsar in back.

Animation of double pulsar system

The eclipses allowed the astronomers to pin down the geometry of the double-pulsar system and track changes in the orientation of the spin axis of one of them. As one pulsar’s spin axis slowly moved, the pattern of signal blockages as the other passed behind it also changed. The signal from the pulsar in back is absorbed by the ionized gas in the other’s magnetosphere.

The pair of pulsars studied with the GBT is about 1700 light-years from Earth. The average distance between the two is only about twice the distance from the Earth to the Moon. The two orbit each other in just under two and a half hours.

“A system like this, with two very massive objects very close to each other, is precisely the kind of extreme ‘cosmic laboratory’ needed to test Einstein’s prediction,” said Victoria Kaspi, leader of McGill University’s Pulsar Group.

Theories of gravity don’t differ significantly in “ordinary” regions of space such as our own Solar System. In regions of extremely strong gravity fields, such as near a pair of close, massive objects, however, differences are expected to show up. In the binary-pulsar study, General Relativity “passed the test” provided by such an extreme environment, the scientists said.

“It’s not quite right to say that we have now ‘proven’ General Relativity,” Breton said. “However, so far, Einstein’s theory has passed all the tests that have been conducted, including ours.”

Original News Source: Jodrell Bank Observatory

MESSENGER Provides New Insights on Mercury

mercury_plains..Credit: NASA/JHUAP/Arizona State University

Data from the MESSENGER spacecraft’s first flyby of Mercury in January of 2008 are now turning into science results. Several scientists discussed their findings at a press conference today highlighting the MErcury Surface, Space ENvironment, GEochemistry, and Ranging mission, the first spacecraft to visit Mercury since NASA’s Mariner 10 made three flyby passes in 1974 and 1975. Among the findings, scientists discovered volcanism has played a more extensive role in shaping the surface of Mercury than previously thought. MESSENGER data has also identified and mapped surface rock units that
correspond to lava flows, volcanos, and other geological features, showing an apparent planet-wide iron deficiency in Mercury’s surface rocks. Additionally, other instruments made the first observations about the surface and atmospheric composition of the closest world to the sun.

“We have now imaged half of the part of Mercury that was never seen by Mariner 10,” says Mark S. Robinson of Arizona State University, lead author of s study on composition variations in Mercury’s surface rocks using their multispectral colors. “The picture is still incomplete, but we’ll get the other half on October 6th.”

MESSENGER will make two more Mercury flybys (October 6, 2008 and September 29, 2009) before
going into orbit around the planet, March 18, 2011.

MESSENGER’s big-picture finding, says Robinson, is the widespread role played by volcanism. While impact craters are common, and at first glance Mercury still resembles the Moon, much of the planet has been resurfaced through volcanic activity.

“For example, according to our color data the Caloris impact basin is completely filled with smooth plains material that appears volcanic in origin,” Robinson explains. “In shape and form these deposits are very similar to the mare basalt flows on the Moon. But unlike the Moon, Mercury’s smooth plains are low in iron, and thus represent a relatively unusual rock type.”

Mercury’s surface also has a mysterious, widespread low-reflective material Robinson says, “It’s an important and widespread rock that occurs deep in the crust as well as at the surface, yet it has very little ferrous iron in its silicate minerals.”

Another experiment measured the charged particles in the planet Mercury’s magnetic field, which enabled the first observations about the surface and atmospheric composition of Mercury. “We now know more about what Mercury’s made of than ever before,” said Thomas Zurbuchen, a professor at the University of Michigan. “Holy cow, we found way more than we expected!”

Zurbuchen is project leader of the Fast Imaging Plasma Spectrometer (FIPS), a soda can-sized sensor on board the MESSENGER spacecraft.

FIPS detected silicon, sodium, sulfur and even water ions around Mercury. Ions are atoms or molecules that have lost electrons and therefore have an electric charge.

Because of the quantities of these molecules that scientists detected in Mercury’s space environment, they surmise that they were blasted from the surface or exosphere by the solar wind. The solar wind is a stream of charged particles emanating from the sun. It buffets Mercury, which is 2/3 closer to the sun than the Earth, and it causes particles from Mercury’s surface and atmosphere to sputter into space. FIPS measured these sputtered particles.

Mercury and MESSENGER form the subject of 11 papers in a special section devoted to the January flyby in the July 4, 2008, issue of the scientific journal Science.

News Sources: University of Arizona, MESSENGER site

International Group Studies Mars Sample Return Mission

Until humans can actually set foot on the Red Planet, the next best thing would be a sample return mission, to bring Martian soil samples back to Earth. A sample return would exponentially increase our knowledge and understanding Mars and its environment. And in order to pull off a mission of this magnitude, international cooperation might be required, and in fact, may be preferred. The International Mars Exploration Working Group (IMEWG), organized an international committee to study an international architecture for a Mars Sample Return (MSR) mission concept. After several months of collective work by scientists and engineers from several countries worldwide, the “iMARS” group is ready to publish the outcome of its deliberations and the envisioned common architecture for a future international MSR mission, and they will discuss their findings at an international conference on July 9 and 10 in France.

The conference will be held at the Auditorium of the Bibliothèque Nationale de France in Paris, and will bring together members of the scientific and industrial communities as well as representatives of space agencies around the world to discuss the status and prospects for Mars exploration over the coming decades. Attendees will have the opportunity to hear the current international thinking on Mars Sample Return and to interact with key players in the global endeavor of exploring and understanding Mars.

A Mars Sample Return mission would use robotic systems and a Mars ascent rocket to collect and send samples of Martian rocks, soils, and atmosphere to Earth for detailed chemical and physical analysis. Researchers on Earth could measure chemical and physical characteristics much more precisely than they could by via remote control. On Earth, they would have the flexibility to make changes as needed for intricate sample preparation, instrumentation, and analysis if they encountered unexpected results. In addition, for decades to come, the collected Mars rocks could yield new discoveries as future generations of researchers apply new technologies in studying them.

Keynote speakers at the upcoming conferencewill are Steve Squyres of Cornell University, principal investigator under the MER mission, and Jean-Pierre Bibring of the Institut d’Astrophysique Spatiale, principal investigator for a key instrument on Mars Express.

Interested in attending? Check out their website

Original News Source: ESA

Explosive Spacewalk?

Explosive bolts that help detach the Russian Soyuz capsule from the International Space Station may be the source of the problems the spacecraft has encountered during the last two landings. Investigative space journalist and Jim Oberg at MSNBC, who is one of the best experts on the inner workings of the Russian space program recently wrote a very interesting article detailing Russian engineers’ plans to fix the problem: have two Russian cosmonauts conduct a spacewalk on July 10 to remove one of the explosive bolts and bring it inside the space station. The bolts, Oberg says, packs twice the explosive force of an M-80 firecracker when ignited, and the cosmonauts will be handling the bolts directly during what will be a very delicate, if not dramatic, operation.

Oberg reports that Russian space engineers say the bolts at one particular location failed to work properly during each of the two previous Soyuz landings, in October 2007 and then in April 2008. As a result, in each case the landing capsule was twisted out of proper orientation and underwent excess heating on unshielded surfaces before tearing loose from the propulsion module and falling to Earth.

NASA has scheduled a press briefing on July 8 to discuss the spacewalk, but Oberg uncovered details about the spacewalk from status reports and discussions with NASA engineers. The engineers in Houston said that, to their knowledge, no such pyrotechnic device has ever been brought into the space station in its 10-year history.

There are five pairs of explosive bolts that break the connections between the spacecraft’s crew capsule and its propulsion module during descent. Russian experts told NASA at one particular location, position 5, apparently failed to fire during both previous Soyuz descents, preventing a clean separation.

The two cosmonauts, station commander Sergey Volkov and flight engineer Oleg Konenenko will remove the position 5 bolt and place it in a shielded safety canister that was brought to the ISS on the last shuttle mission in May for this spacewalk. So obviously, the plan for this spacewalk has been in the works for quite some time.

Russians engineers assured NASA that the remaining four latches will be adequate to hold the two modules together during any other maneuvers in space.

Check out Jim’s article for more details.

Next TEGA “Bake” Could Be Last for Phoenix

The “vibrating” done to get the first Mars arctic soil sample into Phoenix’s TEGA (Thermal and Evolved Gas Analyzer) oven may have caused a short circuit that could happen again the next time the oven is used, perhaps with fatal results. A team of engineers and scientists assembled to assess TEGA after a short circuit was discovered in the instrument, and came to a fairly disheartening conclusion. “Since there is no way to assess the probability of another short circuit occurring, we are taking the most conservative approach and treating the next sample to TEGA as possibly our last,” said Peter Smith, Phoenix’s principal investigator. Therefore, the Phoenix team is doing everything they can to assure the next sample delivered to TEGA will be ice-rich.

The short circuit was believed to have been caused when TEGA’s oven number four was vibrated repeatedly over the course of several days to break up clumpy soil so that it could get inside the oven. Delivery to any TEGA oven involves a vibration action, and turning on the vibrator in any oven will cause oven number 4 to vibrate as well, which could cause a short.

A sample taken from the trench called “Snow White” that was in Phoenix’s robotic arm’s scoop earlier this week likely has dried out, so the soil particles are to be delivered to the lander’s optical microscope on Thursday. If material remains in the scoop, the rest will be deposited in the Wet Chemistry Laboratory, possibly early on Sunday.

The mission teams will mark the Independence Day holiday with a planned “stand down” from Thursday morning, July 3, to Saturday evening, July 5. A skeleton crew at the University of Arizona in Tucson, at NASA’s Jet Propulsion Laboratory in Pasadena, Calif., and Lockheed Martin Space Systems in Denver, Colo., will continue to monitor the spacecraft and its instruments over the holiday period.

“The stand down is a chance for our team to rest, but Phoenix won’t get a holiday,” Smith said. The spacecraft will be operating from pre-programmed science commands, taking atmospheric readings and panoramas and other images.

Once the sample is delivered to the chemistry experiment, Smith said the highest priority will be obtaining the ice-rich sample and delivering it to TEGA’s oven number zero.

The Phoenix team will conduct tests and trial runs so the instruments can deliver the icy sample quickly, in order to avoid sublimation of materials during the delivery process, so the solid ice doesn’t vaporize.

Original News Source: Phoenix News

Where In The Universe Challenge #10

I’ve been enjoying a few lazy days of summer relaxing by a lake. The weather has been perfect, the lake is clear and warm, the food and drinks plentiful; a perfect vacation. But I finally realized (late in the day) today is Wednesday, and its time for another “Where In The Universe” challenge. So, here’s an image, and your mission is to guess where in the universe this picture was taken. You get extra points for guessing the spacecraft that is responsible for the image, too. So take your time, maybe put your feet up and grab a cold beverage on this warm day and ponder this image for awhile. No peeking below for the answer until you’ve made your guess.

When I first saw this image, I thought for sure it was a picture of some icy planetary surface or body of water. But actually, its not ice at all. This is Lake Erie, in the United States, and the image was taken on May 28th, 2006 at about noon local time, on a nice summer day. The sun is just at the right angle that causes a glint off the water, giving it an icy appearance. The image shows features on the surface of Lake Erie, about 50 kilometers (30 miles) west of Cleveland, Ohio.

The image shows V-shaped wakes of small water craft, as well as broad patterns of larger craft, probably large freighters carrying cargo, that displace and disturb more water during passage. These larger wakes are aligned with the direct course between Detroit and Cleveland (not shown in the image). Some of the broad, ill-defined swaths of light and dark (aligned from lower left to upper right) are streaks of wind-roughened water, which reflect the Sun differently.

This image was taken by an astronaut on board the International Space Station with a Kodak 760C digital camera using an 800 mm lens. They are provided by the ISS Crew Earth Observations experiment and the Image Science & Analysis Group, Johnson Space Center.

So, where ever you are, you can now enjoy gazing at a lake, just like I’ve been doing all week. My lake is a lot smaller than Lake Erie, though. But, enjoy!

Learn more about this image at NASA’s Earth Observatory site.

GLAST Powers Up

The GLAST (Gamma-ray Large Area Space Telescope) spacecraft blasted off on June 11, 2008, and after acclimating to the cold reaches of space, the instruments on board are now powering up and have sent back signals to Earth indicating that all systems are operational. Meanwhile back on Earth, several bases of operations for the telescope are gearing up for processing data from the various instruments.

The Large Area Telescope (LAT), one of two instruments aboard GLAST has sent back data to Stanford Linear Accelerator Center’s Instrument Science Operations Center (ISOC) where it will be monitored, processed, and distributed to the rest of the science team worldwide. The observatory is commanded from the Mission Operations Center (MOC) at NASA Goddard Space Flight Center, and during the present initial on-orbit commissioning phase is staffed by a team from across the mission.

Manager Rob Cameron said, “Powering up the LAT has been even smoother than we had hoped. Everything has worked well-in fact, it’s going great. We’re already receiving high-quality data that we
can use to get the instrument ready for the best science return.”

Peter Michelson, of Stanford University, spokesperson and principal investigator for the LAT collaboration, said, “We’re off to a great start and we’re looking forward to a new view of our universe once science operations begin.”

GLAST will explore the most extreme, high energy environments in the universe, and seek answers to questions about dark matter, supermassive black hole systems, pulsars, and the origin of cosmic rays. It also will study the mystery of gamma-ray bursts.

VIDEO of GLAST and gamma rays from pulsars

After the 60-day checkout and initial calibration period, the project will begin science operations in earnest. The LAT will perform a full-sky survey for the first year of the mission and will rapidly respond to gamma-ray bursts detected by both GLAST instruments.

NASA’s GLAST mission has been developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.

Original News Source: NASA’s GLAST Site