AMP
Home Astronomy Thinking small: Uncovering the secrets of micrometeorites

Thinking small: Uncovering the secrets of micrometeorites

0
Thinking small: Uncovering the secrets of micrometeorites


As I look down right into a Petri dish of sand by means of a binocular microscope, the bigger grains turn out to be obelisks, with smaller ones forming avenues between them. It’s a microscopic echo of the Chicago skyline that I can see by means of the window after I search for. I’m on the Subject Museum of Pure Historical past, residence to the Robert A. Pritzker Heart for Meteoritics and Polar Research. The museum has many giant objects: Dinosaurs, elephants, and a few very substantial meteorites. However at the moment, I’m considering small. The meteorites I’m on the lookout for are hidden within the sand beneath my microscope. Perhaps.

The sand is from the Sør Rondane Mountains in Antarctica, introduced right here by Maria Valdes, a analysis assistant on the Museum, who journeyed there with an expedition in quest of meteorites. They discovered a number of, together with an extra-large space rock weighing 16.7 kilos (7.6 kilograms). To discover a meteorite that large is a rarity; however for this specific venture, she wants one thing small: micrometeorites.

Cosmic origins

About 40,000 metric tons of extraterrestrial materials rain down on planet Earth yearly. We will usually see bits of it streaking by means of the evening sky as meteors. If any a part of a meteor survives its fiery descent by means of the environment to achieve Earth’s floor, we name it a meteorite. Typically these meteorites are comparatively giant: boulder-sized chunks of iron or small, blackened rocks. However a lot of the materials arrives right here within the type of micrometeorites, often lower than 0.04 inch (1 millimeter) in measurement.

Associated: Colorado town throws 100th birthday party for pet space rock

To meteoriticists, the scientists who research meteorites, these are cosmic messengers, carrying details about their origins within the solar system. Most meteorites originate in the primary belt, a area of rocky our bodies orbiting the sun between Mars and Jupiter. Over the course of time, a few of these collide and break up, flinging items of particles towards the internal solar system, the place their paths can intersect with Earth’s. Items from a single collision might land on our planet in broadly separated locations and at occasions tens of millions — and even lots of of tens of millions — of years aside. However they nonetheless have one factor in widespread: They preserve the traits of the asteroid they got here from, known as the father or mother physique.

Chromite is a mineral usually present in meteorites. A sturdy mixture of chromium and oxygen, it is ready to face up to the warmth of coming into the environment and lengthy durations of weathering on Earth’s floor. This makes it an excellent reminiscence financial institution for the properties of its father or mother physique. Although all samples of chromite are chemically the identical, the nuclear properties of the oxygen they comprise can differ. All oxygen atoms have eight protons, however they will have eight, 9, or 10 neutrons, ensuing within the isotopes we name oxygen-16, oxygen-17, and oxygen 18, respectively. Oxygen discovered on Earth consists of those isotopes within the ratio 99.76: 0.04: 0.20. In asteroids and meteorites, nonetheless, this ratio can differ. What’s extra, it may possibly differ between one father or mother physique and one other, permitting meteoriticists to affiliate a meteorite with its father or mother physique by measuring the ratio of the oxygen isotopes utilizing a mass spectrometer.

Over time, meteoriticists have assembled a document of isotopic ratios for various father or mother our bodies, so {that a} newly discovered meteorite will be checked towards it and its origin can usually be recognized. However Valdes sees a potential drawback with the method. What if a meteorite’s oxygen content material has been altered by its descent by means of our oxygen-rich environment? Small meteorites, which may be largely and even completely melted on the way in which down, can be particularly vulnerable to this. Her venture — the one which has me peering right into a Petri dish and poking sand grains with tweezers — is attempting out a unique method of figuring out the place meteoritic materials originated.

In addition to chromite, meteorites generally comprise minerals with calcium. Calcium additionally has a number of naturally occurring isotopes, so measuring its isotopic ratios gives another method for learning meteorites. “The strategy for isolating and measuring calcium isotopes is nicely established for meteorites,” says Valdes, however doing these measurements on micrometeorites is new.

Though the mass spectrometry for measuring oxygen isotopes largely spares the micrometeorite from harm, the calcium testing destroys it altogether. Meaning establishing the calcium ratios requires taking a look at a whole lot of micrometeorites. And poking by means of a whole lot of sand.

Grains of sand

So why go all the way in which to Antarctica to get sand? There’s loads of it proper exterior, by Lake Michigan. And it too comprises micrometeorites. Sadly, it additionally comprises the soot and slag of a number of centuries of human habitation. These particles can confuse the image. In my hunt for micrometeorites, I’m on the lookout for objects the dimensions of a grain of sand, however that don’t seem like sand. With the microscopic particles of civilization is combined in, it’s much more like on the lookout for a needle in a haystack.

The Sør Rondane mountain vary of Antarctica, nonetheless, remains to be a pristine location basically uncontaminated by human exercise. In its sand, micrometeorites usually tend to stand out. “It’s nonetheless like on the lookout for a needle,” says Valdes, “however no less than there’s no haystack.”

The shapes I’m on the lookout for are spheres, not needles. When stony particles shoots by means of the environment, the frictional warmth melts its floor, making a blackened crust a couple of millimeter thick. If the article itself is only some millimeters throughout, then it’d soften completely by means of. When this occurs, the molten materials assumes probably the most aerodynamic form that it may possibly: a sphere. And that helps it stand out from the blocklike sand grains I’m trying by means of.

In truth, I see one that appears form of spherical. Push it with the tweezers. Nope, not a sphere. Preserve trying.

After a number of days within the lab, I’d plucked 15 roundish objects from the Antarctic sand and positioned them fastidiously on epoxy pads in plastic pattern instances. I doubt that every one of them are actually micrometeorites. Actually, I can’t swear that any of them are. Valdes tells me that they must be examined with a scanning electron microscope to find out what they’re.

I hope I discovered no less than just a few micrometeorites, however even when I didn’t, there’s nonetheless loads of sand left.



Source link

NO COMMENTS

LEAVE A REPLY

Please enter your comment!
Please enter your name here

Exit mobile version