Hunting for Meteorites at the Bottom of the World

Team members gather to inspect and collect a meteorite being placed in a Teflon bag. Photo credit: M. Keiding, 2007

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Antarctica’s distinctive, unforgiving environment is truly unique. But add to that setting the otherworldly task of looking for meteorites — bits and pieces from the far reaches of our solar system that are strewn about Antarctica’s icy surface,– and Earth’s southern-most continent can provide a truly unparalleled scientific experience. “I had the privilege to explore a part of the world that few people get to,” said Dr. Lucy McFadden, a research professor in the astronomy department at the University of Maryland, College Park. She also is a scientist in the education and public outreach area for NASA’s Dawn mission that is traveling to study the asteroids Ceres and Vesta. McFadden had the opportunity to travel to Antarctica and spend over six weeks hunting for meteorites, specifically looking for meteorites from Ceres and Vesta. She shared her experiences recently in an online “webinar,” answering questions about her journey. “I love sharing my adventures,” she said. “My excitement about exploring the solar system was renewed because I had the opportunity to explore Earth as a planet.”

Although meteorites fall uniformly all over the Earth –estimates are between 30-80 tons a year, — most are in the form of dust. For the bigger rock-sized pieces, many fall in the ocean and those that fall on land can be buried by shifting terrain, broken down by chemical weathering, or are easily confused with Earth rocks. But Antarctica’s blue ice sheets are clear and barren, making it easy to spy a dark rock that’s likely a sample from space.

Aerial view of Antarctica.  Photo credit: L. McFadden 2008
Aerial view of Antarctica. Photo credit: L. McFadden 2008

However, there’s another reason Antarctica is such a great place to look for meteorites. “There’s something special about Antarctica. Meteorites collect in certain areas there,” McFadden said. “The ice sheets are always moving, and the meteorites move with them. But the rocks get trapped by the barriers of the mountains, and that’s where the meteorites are found. Once you get a meteorite up against a barrier, the constant blowing of the polar winds ablates the ice, and rocks effectively come to the surface.” Over periods of tens or hundreds of thousands of years, very significant concentrations can build up in these areas.

Since 1976, the U.S. National Science Foundation has supported an annual search for meteorites during the Antarctic summer, through a program called ANSMET, the Antarctic Search for Meteorites. McFadden was part of an eight-member meteorite hunting team in November 2007 to January 2008.

McMurdo Station. Photo credit: L. McFadden, 2008
McMurdo Station. Photo credit: L. McFadden, 2008

A C-17 cargo plane brought the team to Antarctica’s McMurdo Station. But one doesn’t just go out and start hunting for rocks without instructions on how to survive Antarctica’s harsh environment. The team underwent a week of training that included lessons on proper clothing. “I had to learn which coat to put on when, which hat and gloves to wear and be sure to have my boots on,” said McFadden. “It brought me back to kindergarten.” Also, learning snowmobile operation and repair is a must, as that would be their mode of transportation during their expeditions. “We were trained how to stay away from the crevasses in the ice and trained for rescue in case someone fell in,” she said.

A plane then brought the team, the snowmobiles, fuel and gear to their field site on the Miller Range to set up camp. They erected tents – their homes for six weeks, and had to chip ice to get water for drinking and cooking. Typical daytime temperature was about 20 degrees Fahrenheit (-6 C) when there wasn’t a storm.

High winds at field camp.  Photo credit: L. McFadden, 2007
High winds at field camp. Photo credit: L. McFadden, 2007

At 70 degrees south latitude, the Antarctic summer sun never set. But the surroundings were desolate, to say the least. The region is mountainous, but constantly snow and ice covered. “I felt a sense of vulnerability of us humans,” McFadden said. “This is not a hospitable environment.” She also worried about the possibility of getting lost in the barren landscape with few landmarks. But with them was a seasoned, expert guide, John Schutt.

So what’s the trick of finding meteorites in Antarctica? “We practiced around the camp first, and walked up to all the rocks in the area,” said McFadden. “There are other rocks on the ground from rockslides from the mountains, so you have to learn what the local rocks look like.” Dr. Ralph Harvey, the head of the ANSMET program taught the team the art of meteorite hunting.

“When you find a field of rocks, you have to look closely and separate out the regular rocks from meteorites,” McFadden said. Most meteorites are black because they have a fusion crust: a thin glassy rind that forms on meteorites when they are coming through the atmosphere. The friction heats them up and the outside of the meteorite melts just a little.

“We looked at each rock,” said McFadden. “If we thought we found a meteorite, we waved our arms and everyone would come over and look. If we determined it was a meteorite, we would pick it up with tongs and put it in a Teflon bag and mark it. Then we planted a flag where we found a meteorite. It was very satisfying to look back where we’d been and see all the flags.”

Flags marking meteorite finds.  credit: M. Keiding and ANSMET 2007-2008.
Flags marking meteorite finds. credit: M. Keiding and ANSMET 2007-2008.

They followed a certain procedure to make notes on each meteorite, take pictures, note the position of each sample with a Global Positioning System monitor, and then wrap the meteorites in a certain way and put them in backpacks. “It was a big process to catalogue and account for all of them,” McFadden said.

At the end of the day they collected all the rocks from the backpacks and put them in bags in a specialized container to keep them cold. This would avoid contamination from any snow that might be attached to the rocks, until they are brought to Johnson Space Center where they are catalogued and then distributed to scientists around the world.

A large meteorite found by the team. Photo credit: ANSMET 2007 Case Western Reserve University
A large meteorite found by the team. Photo credit: ANSMET 2007 Case Western Reserve University

Each of the meteorites tells a story about the processes of the early solar system. Scientists who study meteorites can find clues to the conditions as our solar system evolved, and find out more about the asteroids, moons and planets the meteorites originate from. Meteorites represent a “free” sample return mission for scientists.

The team didn’t do any scientific analysis out in the field, just collected the samples for transport to the laboratories in Houston. But that doesn’t mean they didn’t examine the rocks!

The team found lots of carbonaceous chondrites with very irregular and jagged shapes, some that may have come from the Moon, and others with a green mineral called olivine that may have come from Mars. One meteorite found made the team think of the famous ALH 84001 meteorite found in the Allan Hills region of Antarctica, that made headlines in 1996 when it was announced that the meteorite may contain evidence for traces of life from Mars. “We wondered if this one meteorite was related to ALH 84001,” said McFadden. But the team won’t know the answer until geochemical analyses are performed.

As for her search for samples from Ceres and Vesta, McFadden said, “I think we might have been successful in finding samples from Vesta, but I was really interested in looking for samples from Ceres. However, I wasn’t really sure what I was looking for. As far as we know we don’t have samples from Ceres.”

Small meteorite. Photo credit: ANSMET 2007 Case Western Reserve University
Small meteorite. Photo credit: ANSMET 2007 Case Western Reserve University

How do scientists know a meteorite came from a specific asteroid? “The whole study of meteoritics addresses that through laboratory studies of many different attributes of rocks,” said McFadden. “We know we have rocks in our meteorite collection from Vesta because about one in every seven meteorites we find has characteristics, or spectral signature, that matches Vesta as viewed through a telescope. We look at Vesta and see a huge impact basin that the meteorites probably came from.”

But Ceres is a different matter. “We don’t know much about Ceres,” she said. “The spectral signature of Ceres doesn’t match anything we have in the meteorite collection. But maybe they’ll find one in the samples we brought back or eventually find one on a future expedition.”

Snowmobiles, the vehicle of choice for Antarctic meteorite hunting. Photo credit: L. McFadden, 2007
Snowmobiles, the vehicle of choice for Antarctic meteorite hunting. Photo credit: L. McFadden, 2007

With stormy periods when they had to huddle in their tents, McFadden’s team had 22 full days of meteorite searching, and eight half days. They went out at 9:00 am, returning at 5:00 pm. “We had six guys and two women,” said McFadden. It’s different for each expedition. We didn’t know each other before hand, but we worked well together. We had this common experience and we had to look out for each other. But it was also very lonely; there wasn’t that much opportunity to interact. We were exhausted each night.”

They did have opportunities for recreation such as skiing, playing games or reading books. One particularly nice day they made a couch from snow and sat outside for awhile. Planes occasionally brought re-supply of food, letters, and other supplies. They were in Antarctica for Christmas, so they decorated and had a potluck supper. “The isolation and cold weather got to us after awhile, but we loved our time out there,” McFadden said. “We looked forward to going home, but we had a tremendous experience. We all appreciated the beauty of Antarctica.”

Aerial view near McFadden's field camp in the Miller Range. Photo credit: M. Keiding, 2007
Aerial view near McFadden's field camp in the Miller Range. Photo credit: M. Keiding, 2007

Their expedition found 710 meteorites, some as small as a little finger nail (about 1.0 x 0.5 x 0.5 cm) 3a), and others about 8 pounds and too big to hold in one hand (about 25 cm x 15 cm x 12).
“We had good hunting,” she said. “It wasn’t a record. Some days we wanted to keep going, but our guide had to keep us in check and keep us safe. In that climate you do have to stop and take care of yourself.”

Over the more than 25 years of these expeditions, over 26,000 meteorites have been found, expanding the volume of extraterrestrial materials that can be studied here on Earth to provide a context for our remote sensing explorations out in the solar system, such as the Dawn mission. “My experience searching for meteorites inspired me to continue trying to understand the meteorites themselves and pair that with my exploration with the Dawn spacecraft that is searching out in the solar system,” said McFadden.

And now another team of scientists is preparing to return to Antarctica in November this year to continue the hunt.

Dr. Lucy McFadden, Dawn Co-Investigator and Education and Public Outreach (E/PO) lead Photo credit: M. Keiding, 2007
Dr. Lucy McFadden, Dawn Co-Investigator and Education and Public Outreach (E/PO) lead Photo credit: M. Keiding, 2007

McFadden responded to the question of why teams keep going back every year to look for meteorites. “There is the potential to find new types of meteorites. In 2006, they found a type of meteorite that had never been seen before. They believe it’s from another body in our solar system that was probably the size of the moon, but its isotopic signature is decidedly different from the moon or Mars. So we have indeed found evidence of planetesimals that are new to us that are out there in the asteroid belt. That’s very exciting and that keeps us going.”

More information:
McFadden’s article on the Dawn website.
McFadden’s video “webinar” presentation.

“Find a Meteorite” online activity
Dawn Mission website
Dawn Mission Education website

Solving the Asteroid – Meteorite Puzzle

Meteorites. Credit: NASA

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Astronomers studying ways to deal with incoming near-Earth asteroids (NEA) that might be on a collision course with our planet want to know in detail what these space rocks are made of. The better they “know the enemy” the better they can come up with ways to destroy or change the course of NEAs. Since we’ve only studied a couple of asteroids up close with spacecraft, the best way to learn more about the composition of asteroids should be fairly easy: just look at meteorites that fall to Earth, which are small chunks of asteroids. But in doing so, researchers discovered quite a huge discrepancy. The vast majority of asteroids that whiz by Earth are of a type that matches only a tiny fraction of the meteorites that most frequently hit our planet. This difference has had astronomer scratching their heads. But a team of researchers has now found what it believes is the answer to the puzzle. The smaller rocks that most often fall to Earth, it seems, come straight in from the main asteroid belt out between Mars and Jupiter, rather than from the near-Earth asteroid population.

The researchers studied the spectral signatures of near-Earth asteroids and compared them with spectra obtained on Earth from the thousands of meteorites found on Earth. But the more they looked, the more they found that most NEAs — about two-thirds of them — match a specific type of meteorites called LL chondrites, which only represent about 8 percent of meteorites.

“Why do we see a difference between the objects hitting the ground and the big objects whizzing by?” asked Richard Binzel, a professor from MIT. “It’s been a headscratcher.” As the effect became gradually more and more noticeable as more asteroids were analyzed, “we finally had a big enough data set that the statistics demanded an answer. It could no longer be just a coincidence.”

Way out in the main belt, the population is much more varied, and approximates the mix of types that is found among meteorites. But why would the things that most frequently hit us match this distant population better than it matches the stuff that’s right in our neighborhood?

An obscure effect that was discovered long ago was recently recognized as a significant factor in moving asteroids around and putting them on a fast track towards the inner solar system, called the Yarkovsky effect.

This effect causes asteroids to change their orbits as a result of the way they absorb the sun’s heat on one side and radiate it back later as they rotate around, which alters the object’s path. This effect acts much more strongly on the smallest objects, and only weakly on the larger ones.

So, for smaller sized space rocks– the kinds of things that end up as typical meteorites — the Yarkovsky effect plays a major role, moving them with ease from throughout the asteroid belt on to paths that can head toward Earth. For larger asteroids a kilometer or so across, the kind that we worry about as potential threats to the Earth, the effect is so weak it can only move them small amounts.

The new study is also good news for protecting the planet. One of the biggest problems in figuring out how to deal with an approaching asteroid, if and when one is discovered on a potential collision course, is that they are so varied. The best way of dealing with one kind might not work on another.

But now that this analysis has shown that the majority of near-Earth asteroids are of this specific type — stony objects, rich in the mineral olivine and poor in iron — it’s possible to concentrate most planning on dealing with that kind of object, Binzel says. “Odds are, an object we might have to deal with would be like an LL chondrite, and thanks to our samples in the laboratory, we can measure its properties in detail,” he says. “It’s the first step toward ‘know thy enemy’.”

News Source: MIT

Where Do Meteorites Come From?

If you’ve ever held a real meteorite in your hand, you probably wanted to know, “Where has this rock been in space and where did it come from?” Until now, no one has been able to definitively establish where the majority of meteorites found on Earth came from because of the changes that occur in meteorites after they are ejected from the asteroids they were originally part of. The most common type of meteorite found on Earth, about 75% of those identified, are chondrites, stony bits of space rocks that didn’t undergo any melting while out in space. Two astronomers say have determined that most of these meteorites come from the asteroid belt between Mars and Jupiter. Using the GEMINI telescope, they found that asteroids in that region are similar to chondrites found on Earth.

This discovery is the first observational match between the most common meteorites and asteroids in the main belt. It also confirms the role of space weathering in altering asteroid surfaces.

To find the parent asteroid of a meteorite, the astronomers compared the spectra of a meteorite specimen to those of asteroids. This is a difficult task because meteorites and their parent asteroids underwent different processes after the meteorite was ejected. In particular, surfaces of asteroids are known to be altered by a process called “space weathering”, which is probably caused by micrometeorite and solar wind action that changes the surface and spectra of asteroid surfaces.

Meteoroids are created, usually when there is a collision between asteroids. When an impact of a large asteroid occurs, the fragments broken off can follow the same orbit as the primary asteroid. These groups of fragments are called “asteroid families.” Until recently, most of the known asteroid families have been very old (they were formed 100 million to billions of years ago), and younger families are more difficult to detect because asteroid fragments are closer to each other.

In 2006, four new, extremely young asteroid families were identified, with an age ranging from 50,000 to 600,000 years. The astronomers, Thais Mothé-Diniz from Brazil and David Nesvorný from the US observed these asteroids, obtaining visible spectra. They compared the asteroids spectra to the spectra of an ordinary chondrite (the Fayetteville meteorite, shown in the top photo) and found they matched.

Identifying the parent asteroid of a meteorite is a unique tool when studying the history of our solar system because one can infer both the time of geological events (from the meteorite that can be analyzed through dating techniques) and their location in the solar system (from the location of the parent asteroid).

Meteorites are also a major tool for knowing the history of the solar system because their composition is a record of past geologic processes that occurred while they were still incorporated in the parent asteroid.

Original News Source: Astronomy and Astrophysics

Geologist Finds a Meteorite Crater in Google Earth

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Want to discover an impact crater, and even get it named after you? All you’ve got to do is spend a few (hundred) hours poring over images in Google Earth or Google Maps. That’s exactly what Geologist Arthur Hickman did, turning up a previously unknown impact crater when he was searching for iron ore in the mountains of West Australia.

While he was browsing through images on Google Earth, Hickman’s geology training helped him recognize the circular shape and raised rim of an impact crater. He sent a screenshot and coordinates to colleagues at Australian National University, and they confirmed that it’s a well-preserved meteor crater between 10,000 and 100,000 years old. And until now, totally unknown.

You can take a look at the crater for yourself on Google Maps.

This isn’t the first time a crater has been discovered using Google Earth. One was found in the Saharan Desert two years ago. That crater is 31 km (19 miles) across – much bigger than Meteor Crater in Arizona.

The newly named “Hickman Crater” measures 270 metres (885 feet) across, and is about 35 km north of Newman, Australia. The region was mapped by the Geological Survey of Western Australia about 20 years ago, but the crater went unnoticed until now.

Since large meteorites hit the Earth every few thousand years, and when you consider that the landscape is millions of years old, there are many regions hiding meteorite impacts.

They’re just waiting for you to find them.

Original Source: ScienceAlert

Peruvian Meteorite May Rewrite Impact Theories

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On September 15th of last year, a meteorite impacted the Earth near the town of Carancas in Peru. The story made worldwide headlines when hundreds of people who flocked to see the crater reported getting ill. As it turned out, there were no mysterious space illnesses plaguing the population; the super-hot meteorite likely vaporized arsenic-containing water that was near the surface of the impact site, and onlookers and investigators breathed in the noxious gas. The meteorite is again in the spotlight, though not for making people sick.

Researchers estimate from their analysis of the crater that the meteorite was of a rocky composition, and that it impacted the ground at a whopping 15,000 miles (24,150 kilometers) per hour. That is really fast for a stony meteorite! It is calculated to have been between .2 and 2 meters at the point of impact, and upwards of 3 meters when it entered the atmosphere.

“Normally with a small object like this, the atmosphere slows it down, and it becomes the equivalent of a bowling ball dropping into the ground. It would make a hole in the ground, like a pit, but not a crater. But this meteorite kept on going at a speed about 40 to 50 times faster than it should have been going.” said Peter Schultz, professor of geological sciences at Brown University, who presented the findings of his travels to the impact site at the 39th annual Lunar and Planetary Science Conference in Texas last week. Schultz collaborated on his research with a team of scientist from Brown University, Peru and Uruguay.

Stony meteorites – called chondrites – generally break up in the atmosphere and impact the ground at rather slow speeds. In fact, most of the objects that enter Earth’s atmosphere end up never hitting the ground because the gases are so thick that the heat caused by air compression vaporizes them.

Schultz and his team think the Carancas meteorite may have initially broken up and then reformed in such a way as to make it more aerodynamic, allowing it to bullet through the atmosphere instead of being braked by the friction with the gases in our atmosphere. As opposed to dissipating and burning up like other chondrites, the meteorite landed as one large chunk.

This contradicts the conventional theory that small, rocky asteroids either can’t impact at all, or create only small impact pits. If the new theory is correct, we may have to rethink the history and influence of meteorite impacts on the Earth, as well as consider what kind of damage they are capable of doing in the future.

Source: Brown University News Release

Meteorites Can Be Rich With the Ingredients of Life

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How did life arise on Earth? How did we get from rocks and water to the abundance and variety that we see today? Perhaps the raw ingredients for life, amino acids, were delivered to Earth by a steady bombardment of meteorites. Researchers have turned up space rocks with concentrations of amino acids 10x higher than previously measured, raising hopes that the early Solar System was awash in organic material.

The study was done by Marilyn Fogel of Carnegie’s Geophysical Laboratory and Conel Alexander of the Department of Terrestrial Magnetism with Zita Martins of Imperial College London and two colleagues, and will be published in Meteoritics and Planetary Science.

If you’re like me, the astronomy stuff’s fine, but the biology news is a little baffling (I forward the kids’ biology questions to my wife). Amino acids are organic molecules that form the backbone of proteins, which make much of life’s structures and drive chemical reactions in cells. Amino acids are naturally occurring, but they somehow came together to make the first proteins in the Earth’s early days.

The researchers took samples from three meteorites collected during recent expeditions to Antarctica. The meteorites are from a type called CR chondrites, which are through to contain ancient organic materials that date back to the earliest times of the Solar System. At one point, these meteorites were part of a larger “parent body”, which was later shattered by impacts.

One sample had few amino acids, but the other two had the highest concentration ever seen in primitive meteorites.

“The amino acids probably formed within the parent body before it broke up,” says Alexander. “For instance. ammonia and other chemical precursors from the solar nebula, or even the interstellar medium, could have combined in the presence of water to make the amino acids. Then, after the break up, some of the fragments could have showered down onto the Earth and the other terrestrial planets. These same precursors are likely to have been present in other primitive bodies, such as comets, that were also raining material onto the early Earth. ”

So this points to the conclusion that the early Solar System was a much richer source of organic molecules than researchers previously believed. And the constant rain of amino acid-laden meteorites would have delivered this material to the primordial soup where life first emerged.

Exactly how the amino acids became the first proteins… that’s still one of the biggest mysteries in science.

Original Source: Carnegie Institution for Science News Release

Researchers Observe Extra-galactic Meteor

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The common belief is that all meteors come from inside our solar system. Most meteors are thought to be pieces of comet dust or fragments of asteroids that enter Earth’s atmosphere and burn up before they hit the ground, leaving a fiery trail we call “shooting stars.” But a recent observation might put a hole in the idea that these space rocks only come from the immediate vicinity of our solar system. A group of astronomers in Russia believe they observed a meteor of extragalactic origin.

On July 28, 2006, Victor Afanasiev from the Russian Academy of Sciences was making observations using a 6 meter telescope equipped with a multi-slit spectrometer. By chance, he observed the spectrum of a faint meteor as it burned up in the Earth’s atmosphere, and in looking at the data, found several anomalies. First was the speed at which the meteor was traveling. This meteor hit the atmosphere at about 300 kilometers per second, which is quite extraordinary. Only about 1% of meteors have velocities above 100 km/sec, and no previous meteor observations have yielded velocities of several hundred km/s. So where did this one come from?

Since the Earth moves around the galactic center at about 220 km/s, Afanasiev says the meteor’s origin cannot easily be explained by reference to the Milky Way. It appears that it came from the direction in which the Earth and the Milky Way is travelling towards the center of our local group of galaxies. “This fact leads us to conclude that we observed an intergalactic particle, which is at rest with respect to the mass centroid of the Local Group and which was ‘hit’ by the Earth,” Afanasiev and his team say in their paper.

Afanasiev also noted that the spectra of this meteor showed it was made of iron, magnesium, oxygen, iodine and nitrogen. These materials, particularly the metals, form inside stars. Additionally, spectral analysis showed features typical from the materials being strongly heated with the temperatures of 15000 – 20000K. Afanasiev says this differs widely from materials of terrestrial-type rocks and is suggestive of extrasolar or presolar materials.

Another difference was the size of the meteor. The researchers calculated that the meteor was several tens of a millimeter in size. This is two orders of magnitude larger than common interstellar dust grains in our galaxy. They estimated its size by integrating the equation of mass loss jointly with the equation of the variation of the density of the atmosphere. The research team noted that their size estimate, which they admit come from “rather coarse assumptions,” agrees with the expected parameters of the speed of interstellar meteors, which could be as high as 500 km/s.

The team subsequently made other observations to see if other meteors could perhaps be from outside our galaxy. In a total observing time of 34.5 hours during Oct-Nov 2006, they observed 246 meteors, 12 of which had velocity and direction to possibly have come from outside our galaxy.

Afanasiev and his team say there are many questions to be answered about their findings. For example, how metal-rich dust particles came to be in the extragalactic space, and why the sizes of extragalactic particles are larger by two orders of magnitude (and their masses greater by six orders of magnitude) than common meteors. Also, if extragalactic dust surrounds galaxies, could this be observed with infrared telescopes like the Spitzer Space Telescope? And is this dust spread out evenly in the universe or could it be found in clumps that might show up in the form of irregularities on the cosmic microwave background, observed by WMAP (Wilkinson Microwave Anisotropy Probe)?

With all our incredible observatories like Hubble, Spitzer, Chandra, etc, we have the opportunity to see outside of our galaxy. But now we have evidence that we actually might be interacting with extragalactic material as well.

Original News Source: Arxiv

When the Solar System Went from Dust to Mountains

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Astronomers are slowly piecing together the earliest phases of our Solar System’s history. At some point, tiny particles of dust clung together forming larger and larger boulders and eventually even mountain-sized chunks of rock. Researchers from UC Davis have pegged the date that this occurred to 4.568 billion years ago, give or take a few million years.

The evolution of the Solar System is believed to have gone through several distinct stages. The first stage occurred when tiny particles of interstellar dust linked up, created boulders, and leading up to the mountain-sized rocks.

In the second stage, these mountains collected into about 20 Mars-sized objects. In the third and final stage, these mini-planets smashed into one another, eventually leading to the large planets we have today. The dates of the second and third stages are fairly well known, but the timing of the first stage has largely been a mystery.

To get an idea of when that first stage took place, researchers from UC Davis analyzed a particular kind of meteorite, called carbonaceous chondrites. These represent some of the oldest material in the Solar System.

They found that the meteorites have very stable ratios of certain elements, which can allow them to be dated. Since the rocks never got large enough to heat up from radioactive decay, they’re cosmic sediments from the early Solar System.

The UC Davis researchers estimated the timing of their formation to 4.568 billion years ago, ranging from 910,000 years earlier or 1.17 million years later.

“We’ve captured a moment in history when this material got packed together,” said Qing-zhu Yin, assistant professor of geology.

The work is published in the Dec. 20 issue of Astrophysical Journal Letters.

Original Source: UC Davis News Release

Tunguska Meteoroid’s Cousins Found?

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It’s a cosmic whodunit: a meteorite exploded in the air near a remote part of Russia called Tunguska in 1908, and the meteorite that caused the event all but disappeared. Where did it come from? Was it an asteroid or part of a comet? Astronomers have taken up the case, using mathematical simulations to track down the perpetrator. They even think they might even know a few of its siblings.

Tadeusz J. Jopek and his team at the Astronomical Observatory UAM in Poland – in collaboration with the Observatoire de la Côte d’Azur in France – looked for the possible origins of the Tunguska meteor by essentially running the explosion backwards, and mathematically simulating where the parent object of the event would have been before the impact.

By taking the existing forensic evidence of the impact to estimate the velocity and impact angle of the Tunguska meteorite, the team was able to simulate the possible orbit and speed of the object before it hit the earth. In doing this, they created 3311 virtual “particles” as possible origins of the object.

They then analyzed the orbits of near-earth objects that lie in the most likely region for the past 20,000 years to find possible matches with their simulated particles. It is still unclear exactly where the Tunguska meteor came from, and there are over 130 suspects.

“We believe that TCB originated as the result of a breakup of a single body : a comet or an asteroid. In our study we concluded that it is more probable that it was an asteroid. We cannot point to which one; instead we have found several candidates for the Tunguska parent, and the asteroid 2000 WK63 is an example of it,” Dr. Tadeusz said.

This is a hard case to solve indeed, as there remains little physical evidence of the original object near Tunguska, and the only tools astronomers have to work with are mathematical and statistical simulations. The question still remains whether the parent was a comet or asteroid, and indeed if the near-earth object it came from has been discovered yet.

“Such statistical conclusion gives no absolute sure [sic] that one of the presently known asteroids was indeed the Tunguska cosmic body parent. Therefore it is possible that still, the real Tunguska parent body is undiscovered.” Dr. Tadeusz said.

Source: Earth, Moon, and Planets Journal

2007 Perseid Meteor Shower Didn’t Disappoint

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So, did you heed my advice? Did you set aside Sunday evening to head out with friends and family to enjoy the Perseid meteor shower. Here in Vancouver, we had cloudy skies into the evening. But on a hunch, I set my alarm for 4 am, when the shower was at its height. What a treat.

My kids were disappointed that the sky was clouded over, and we wouldn’t be able to see the meteors Sunday evening. But incredibly, the sky cleared up over night, and it was perfectly clear when I checked outside at 4 am. So, I woke up the kids and we laid out on the back deck and watched for meteors as the skies started to brighten up. I was able to see quite a few before the rising Sun started to brighten the skies too much. All in all, it was great to see.

I’m really looking forward to the next big event: the total lunar eclipse on August 28, 2007. I can’t stress it enough. If you live in the Western North America, the Pacific, or Asia please try and make an event of this eclipse. It’s going to be great.

The European Space Agency has an interesting article about some of the science that happened during the meteor shower, as well as some tests of new equipment that could eventually be used to observer meteors… from space.

Source: ESA News Release