Notes
Slide Show
Outline
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FOSSIL METEORITES
  • Channon Visscher
  • EPSc 571
  • Fall 2003
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Outline
  • Definition and overview


  • Current inventory of fossil meteorites


  • Importance of fossil meteorites


  • Where to look for them
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What is a fossil meteorite?
  • Meteorite with ancient terrestrial age
  • Buried in sediment after fall event
  • Incorporated into geologic record


  • Not considered fossil meteorites:
    • Meteorites embedded in ice (e.g. Antarctica)
    • Objects associated with craters
    • Cosmic spherules, tektites, etc.
    • Objects found in surface sediments(?)
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Micrometeorites, etc.
  • Small (sub-mm) objects that survive atmospheric entry
    • If totally melted: cosmic spherules
    • Typically iron, stony, or glassy
  • Large numbers collected from deep sea sediments, etc.
    • Large age range: kyr to several hundred Ma
    • Present flux of ~30,000 tons per year
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Catalogue of fossil meteorites
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Fossil meteorites: Irons
  • Most recognizable; High Ni contents
  • Oxidized partially or completely into limonite, etc.
  • May preserve some of original structure


  • Surface finds
    • Technically not “fossil”, but shown to have old terrestrial ages
    • Ider (3.1 Ma), Tamarugal (2.7 Ma) (53Mn/10Be)
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Fossil meteorites: Stones
  • More difficult to preserve, recognize
  • Original meteorite structures may be present
  • Original minerals usually replaced by diagenitic minerals (e.g. limestone chondrules)
  • Chromite as a meteoritic marker (Schmitz et al. 2001):
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Brunflo (Sweden)
  • Polished slab of Ordivician limestone
  • Found in 1952, recognized 1979
  • 463 Ma terrestrial age; probably H-L chondrite



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Österplana (Sweden)
  • systematic search (1992-present) in limestone quarry
  • 40 meteoritic objects recovered so far
  • 480 Ma terrestrial age; probably L chondrites
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Österplana (Sweden)
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K-T boundary
  • 2.5 mm meteorite found in K-T boundary clays
  • Original minerals replaced by hematite and clay
  • 65 Ma, maybe a carbonaceous chondrite
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Importance of fossil meteorites
  • Has flux changed over geologic time?
  • Flux: ~28,000 objects > 0.1 kg per year on Earth (Halliday et al. 1989)


  • Quantity – higher/lower flux in the past?
    • Österplana suggests 10-100X higher flux
    • asteroidal breakup of L-type parent body?

  • Quality – similar distribution of groups?
    • Irons are better preserved/more recognizable
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Where to look
  • Coals, shales, limestones, sandstones, clay deposits, evaporites
  • Slow accumulation over long time period
  • Favorable conditions for preservation


  • Ongoing systematic searches:
    • Swedish quarries
    • PA and WY coal mines


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Fossil Meteorites in Missouri?
  • Relatively rapid accumulation rates (~15 cm/kyr)
  • 75 million tons of limestone products per year


  • limestone: 2700 kg m3
  • 75 million tons = 25 m thick deposit over 1 km2
  • 25 m = 170,000 years of accumulation


  • With present flux, can expect ~10 meteorites > 0.1 kg processed each year in Missouri