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Environmental Sciences Branch (ESB)

Cosmic Dust from the South Pole

Photo of micrometeorites

 

Micrometeorites collected from a well at the Amundsen-Scott South Pole station offer clues to

  • The composition of solar-system objects such as asteroids and comets
  • The baseline inputs to Earth's sediments and oceans from extraterrestrial sources

What are Micrometeorites?

  • Micrometeorites are submillimeter extraterrestrial particles that have survived atmospheric entry
  • They are fragments of asteroids, comets, Mars, and our moon.
  • They range from unmelted and partially melted particles that retain much of their original mineralogy to totally melted cosmic spherules, some of which have lost much of their mass by vaporization.
  • They are thought to contribute most of the extraterrestrial matter accreted by the Earth on ten million-year time scales.
  • Approximately 30,000 tons of cosmic dust enters Earth's atmosphere each year

The Problem:

  • Large collections of these materials are difficult to find due to destruction of particles by weathering and highly variable concentrating processes in terrestrial environments.

Microscopic view (320X) of cross-sections of micrometeorites
Cross-sections of micrometeorites.

The Approach:

  • The Antarctic provides a good, "clean" source of these particles. Micrometeorites that fell on the snow hundreds of years ago are now frozen in ice layers under the South Pole station.
  • The South Pole water well (SPWW) is a 24-m-diameter subsurface melt pool. As the pool melts downward, extraterrestrial particles liberated from the ice remain on the well bottom to form a concentrated, unbiased deposit of micrometeorites.
  • CRREL researchers designed and built a robot to suction and filter all 50- to 2,000-micrometer particles from the well bottom without bias for density, magnetic susceptibility, or shape.

Results to Date:

  • Researchers collected hundreds of thousands of cosmic spherules (melted micrometeorites) that fell to earth between 700 to 1100 and 1100 to 1500 AD.
  • Initial calculations indicate the flux of the particles onto the earth's surface is about 2700 tons per year. Thus, about 90% of the influx of cosmic dust evaporates during atmospheric entry.
  • Ongoing work includes determining the compositional distribution of the spherules and using this information to estimate weathering rates for spherules collected from deep-sea sediments that are millions of years old.

Supported by:

National Science Foundation

 

Points of Contact:

Susan Taylor, Research Physical Scientist
Environmental Sciences Branch
ERDC-CRREL, Hanover, NH 03755
(603) 646-4310
Susan.Taylor@erdc.usace.army.mil

James Lever
Mechanical and Military Engineering Branch
ERDC-CRREL, Hanover, NH 03755
(603) 646-4309
James.H.Lever@erdc.usace.army.mil

View more micrometeorite particles and a preliminary system for classifying the particles

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Last modification: 25 March 2002 (seh)