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

An Experiment to Test Panspermia

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One of most intriguing, and controversial, theories astrobiology is the concept of Panspermia. This idea proposes that life on Earth might have began on another planet, or maybe even out in interstellar space. Scientists have discovered just how hardy microbial life can be, surviving long journeys in the vacuum, cold, and radiation of space. Now an experiment has been devised to see how well microbes can withstand reentry through the Earth’s atmosphere.

The experiment, designed by Professor John Parnell from the University of Aberdeen, involves bolting a Scottish rock to the outside of an ESA research spacecraft. When the Foton M3 mission launches on Friday, September 14th, microbes in the rock will enjoy the acceleration of liftoff, 12 days of microgravity and vacuum, and then re-entry through the Earth’s atmosphere.

“The objective behind this is to look at the rock’s behaviour when it is exposed during re-entry through the Earth’s atmosphere – when temperatures are extreme. This will tell us something about the likelihood of life being transferred between planets on meteorites.

“The Orkney rock is a very robust material but it will be interesting to see if organic matter in the rock is robust enough to survive the harsh conditions endured during re-entering the Earth’s atmosphere.”

In theory, asteroid strikes in the past excavated material on other planets, hurling microbe-laden rocks into interplanetary space. The rocks would then act as lifeboats, carrying the microbes to other planets. More importantly, they should protect the bacteria as the rock plunges into the atmosphere.

This experiment will help discover if there’s anything to this idea. Bacteria might just be hardy enough to survive the complete journey from planet to planet.

Original Source:Univ. Of Aberdeen

Aurigid Meteor Shower, September 1

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What a fantastic month for skywatching. On August 12th, we’ve got the Perseid meteor shower. On August 28th there’ll be a total lunar eclipse. And on September 1st, there might be another meteor shower to enjoy: the Aurigids.

Unlike the dependable Perseids, the Aurigid meteor shower is unpredictable. They’re a stream of particles left behind by Comet Kiess (C/1911 N1). This is a long period comet that has only visited the inner solar system twice within the last two thousand years. Its last visit is believed to have been 83 BC.

On September 1, 2007, the Earth will pass through the dusty trail left behind by Comet Kiess, and it might be a spectacular show. Or it might be a non-event.

“We have so little experience with ancient debris from long-period comets,” notes Bill Cooke of NASA’s Meteoroid Environment Office (MEO) at the Marshall Space Flight Center. “Almost anything could happen—from a fizzle to a beautiful meteor shower.”

Astronomers have predicted that the peak of the shower will occur at approximately 1136 UTC (7:36 am EDT), and last for about 2 hours. It should be visible to observers in Western North America, the Pacific, and Eastern Asia.

One prediction calculated that there could be as many as 100 meteors an hour. That’s pretty good, but not at meteor storm levels, like the Leonids. One unique attribute about the Aurigids is that they leave a brilliant blue-green streak in the sky. Scientists think this might be because Comet Kiess is such a long period comet, spending much of its time in the darkness of the outer Solar System, its particles are relatively untouched by the Sun

So, I can’t guarantee anything. But the weather should still be warm on September 1st. School hasn’t started, and many of you will be looking for an excuse to enjoy the night sky with your friends and family.

Now you’ve got something to do. Go see the Aurigid meteors.

Original Source: NASA Science

Asteroid Vesta Formed Quickly, and Early

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Asteroid 4 Vesta is the second largest asteroid in the Solar System, stuck between the orbits of Mars and Jupiter. It was fully formed early on, turning solid and crystallizing within 10 million years of the Solar System’s formation. How do scientists know this? They’ve found a little piece of it right here on Earth. A Vesta meteorite discovered in Antarctica that tells the history of the early Solar System.

A study is being led by researchers from the University of Toronto. Their subject is a volcanic meteorite discovered in Antarctica during a recent survey. The space rock contains tiny zircon crystals that match the chemical makeup of Asteroid Vesta. It belongs to a class of objects called eucrites – meteorites that formed from volcanic activity.

Scientists believe that Vesta was quickly heated, and then melted into a metallic and silcate core, similar to the process that happened here on Earth billions of years ago. The radioactive decay from abundant minerals in the early Solar System was thought to provide the energy for this process.

Based on their analysis, this meteorite – and therefore Vesta – was once boiling rock that quickly turned solid and crystallized. This change, from liquid to solid happened within 10 million years of the Solar System’s formation. This information gives scientists clues about how our own planet solidified out of the Solar System’s protoplanetary disk.

Original Source:University of Toronto News Release

Another Reminder, Go See the Perseids

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My favourite meteor show is less than 2 weeks away now, so I wanted to give you all another gentle reminder to get organized and make sure that you’re able to enjoy the Perseid meteors this year – the shower will be peaking on the night of August 12, and into the next morning. It’s going to be a special event because the shower coincides with a new moon. The sky will be at its darkest, and the meteors will be at their brightest.

The shower gets its name because they will appear to originate from the constellation of Perseus. Don’t worry about finding the constellation, though, just lay on your back and stare up, you’ll see them.

On the evening of August 12, the first thing you’ll want to do is head outside shortly after sunset. If you’re lucky, you’ll see “earthgrazers”. These are some of the most beautiful meteors that you’ll see in the whole evening. Then settle down, find some satellites, and wait for the show to really get going. It you’ve got the stamina, the best viewing will happen in the early dawn hours of Monday, August 13th. At that point, you could be seeing a few dozen every hour.

To really get the best experience out of this, travel away from the lights of the city. Here in Vancouver, we need to get about 50 km away to start seeing the Milky Way above our heads. We’ve got a dark sky park in a suburb called Abbotsford that’s perfect.

So get organized. Book the evening with your friends, map out where you’re going to go. Bring hot drinks, warm clothes, and a comfortable place to sit back and enjoy the show.

And if you’re interested, Pamela and I recorded an episode of Astronomy Cast dealing with meteors and meteor showers, so you can listen in the car before you reach your viewing spot.

Enjoy, and let me know how it goes.

Set Your Calendar for the 2007 Perseids: August 12th

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My absolute favourite meteor shower every year is the Perseids. They’re not the most spectacular meteors of the year, but the weather’s nice and warm here in Canada. We always head back home to Hornby Island to visit the family at Perseid time to enjoy them with nice dark skies. We keep the kids awake as long as possible, and then lay back on a mattress, enjoying the sky show.

And this year’s going to be a great one: no moon.

That’s right, there’s going to be a new moon on Sunday, August 12th, the exact same time that the Perseid shower is peaking. Without the glare of the Moon, the meteors will be at their brightest. But to really enjoy the show, you’ll want to head outside your city, away from the glare.

Like all meteor showers, the Perseids get their name from the constellation the meteors originate from. The constellation is in the northeast. As soon as it starts to get dark, you should start seeing meteors streaking across overhead. It’ll probably just be a couple every minute, but by early morning, when the shower is peaking, you could even see a few dozen a minute.

And as a special bonus, Mars is going to be in the sky as well. It’ll appear to be a bright red star also in the northeast.

I want you to organize something for the Perseids this year. Gather together some great friends, head somewhere dark, and plan to enjoy a great show. Put it on your calendar right now.

Promise?

Original Source: NASA