Exploring the Solar System From the Ends of the Earth
The best meteorites are found in … Antarctica.
We’ve been to the moon and just about everywhere on Earth. So
what’s left to discover? In September, Future Tense is publishing a
series of articles in response to the question, “Is exploration dead?” Read more about modern-day exploration of the sea, space, land, and more unexpected areas.
Traditionally, when we think of exploring the solar system, we
conjure up images of spacecraft that cost billions of dollars and
traverse millions of miles to reach other worlds. We almost never stop
to think that pieces of these other worlds may actually traverse
millions of miles to reach us free of cost.
Fragments of asteroidal and planetary bodies in our solar system have
been falling to Earth throughout the course of its 4.6 billion-year
history. While there is some loss of this material from frictional
heating in the atmosphere as the fragments fall to Earth, larger pieces
do make it to the surface as meteorites (not to be confused with
meteors, which represent only the light and sound phenomenon associated
with the fall of a space rock through the Earth’s atmosphere).
Scientists have used these pieces to push back the limits of our
understanding of how and when our solar system and the planets in it
were formed.
Meteorites fall everywhere on Earth with equal probability, but there
are places where they are more easily found because the geology and the
environmental conditions allow these fallen rocks to be preserved for
up to millions of years. In fact, some of the best meteorite-hunting
grounds are in the cold deserts of Antarctica. The cold and dry
conditions keep these rocks from space from being weathered and eroded
away. Other factors unique to Antarctica are in play, too, and they
serve to actively concentrate meteorites in certain areas called
“stranding surfaces.” These surfaces are typically found in ice fields
near the Transantarctic Mountains. Here, the movement of the ice sheets
toward the Antarctic coastlines pushes them up against the mountains. At
the same time, the high-speed, gravitationally driven Katabatic winds
ablate away the surface of this ice to expose meteorites that had
previously fallen on the ice sheets and been carried along with them.
What results is a treasure trove of meteorites: Often dozens or even
hundreds can be found in an area the size of a football field. There are
no other places on Earth where such concentrations of relatively
well-preserved meteorites have been found. We have discovered that the
southernmost continent is a uniquely excellent place to hunt for space
rocks. And this discovery was made rather serendipitously.
In 1973, William Cassidy, a professor of geology and planetary
science at the University of Pittsburgh, was attending a conference and
happened to hear a talk about meteorites that a team of Japanese
glaciologists had found in the Antarctic during a field trip in 1969.
The scientists had apparently uncovered nine meteorites in a relatively
small area—50 square kilometers. This would not have been terribly
surprising if all these rocks had been of the same kind, which would
have suggested that they came from a single meteorite fall. However,
these nine meteorites represented five different types.
Something clicked for Cassidy: This meant that there was some sort of
meteorite concentration mechanism operating in such areas in
Antarctica. It then took him a few years to convince the National
Science Foundation that it was worth funding an expedition to the white
continent to hunt and collect meteorites, but he eventually managed to
do it. This is how the U.S. Antarctic Search for Meteorites, or ANSMET,
program came into being in 1976, and it has since been hugely
successful. In the last 37 years, more than 20,000 meteorite specimens
have been collected in Antarctica by the ANSMET program. This represents
many more meteorites than were ever recovered throughout the world in
the 500 years prior. Parallel collection efforts by the Japanese and
Europeans inspired by ANSMET have similarly resulted in the recovery of
thousands more meteorites. The amazing thing is that total cost of this
entire enterprise of collecting meteorites in Antarctica, by the
combined efforts of the Americans, Japanese and Europeans for well over
three decades, has been less than the cost of a NASA Discovery mission—a
class of mission described by former NASA Administrator Daniel Goldin
as a “faster, better, cheaper” way of exploring the solar system.
The contribution of the Antarctic meteorite collection effort to
planetary science, and to scientific knowledge in general, cannot be
overstated. The new and unique meteorite samples collected from this
effort over the years have literally allowed scientists working in
laboratories here on Earth to explore the far reaches of the solar
system. Indeed, these meteorites represent fragments of other worlds
that are unlikely to be visited by any spacecraft in the near future,
much less by a sample return mission that might bring back materials
from them.
For example, one of the most significant developments enabled by the
Antarctic meteorite collection effort has been the recognition that
although the majority of meteorites originated on asteroids, a small
fraction have originated on Mars and the moon, thus providing us with
the ability to study the origin and evolution of these planetary bodies.
The first meteorites for which Martian and lunar origins were
established beyond reasonable doubt (named EETA 79001 and ALHA 81005,
respectively) were recovered in Antarctica within the first five years
of the ANSMET program. Given that it could be many years before we are
able to return to the moon or to get a sample back from Mars, the
Antarctic has taken on a special significance as the potential source of
new and interesting planetary materials for scientific investigations.
On a more personal note, I will vouch for the fact that a trip to the
ice to collect precious fragments of other worlds can be exhilirating
and perhaps even life-changing. It is the knowledge that one is doing
one’s part in contributing to the grand scientific enterprise. It is
being immersed every single day, for weeks at a time, in the astounding
beauty of a uniquely majestic place on our Earth where not too many
humans have ever set foot. It is knowing that the meteorites being
collected are each a piece of another place in our solar system where no
human may ever set foot.
More from Slate’s series on the future of exploration: Is the ocean the real final frontier, or is manned sea exploration dead? Why are the best meteorites found in Antarctica? Can humans reproduce on interstellar journeys? Why are we still looking for Atlantis? Why do we celebrate the discovery of new species but keep destroying their homes? Who will win the race to claim the melting Arctic—conservationists or profiteers? Why don’t travelers ditch Yelp and Google in favor of wandering? What can exploring Google’s Ngram Viewer teach us about history? How did a 1961 conference jump-start the serious search for extraterrestrial life? Why are liminal spaces—where urban areas meet nature—so beautiful?
The author participated in the 1992-1993 and the 2012-2013 field
seasons of the ANSMET program, which is operated through Case Western
Reserve University with support from NSF, NASA, and the Smithsonian
Institution. This article arises from Future Tense, a collaboration
among Arizona State University, the New America Foundation, and Slate. Future Tense explores the ways emerging technologies affect society, policy, and culture. To read more, visit the Future Tense blog and the Future Tense home page. You can also follow us on Twitter.
Meenakshi Wadhwa is director of the Center for Meteorite Studies at Arizona State University and participates in the Antarctic Search for Meteorites program.
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