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Slide 1Meteorite compositionSlide 3ChondritesChondrite groupsPeekskill MeteoriteAchondritesMartian MeteoritesIron MeteoritesStony-iron MeteoritesIdentifying a meteoriteSlide 12Meteorite/ Comet ImpactsChicxulub, Yucatan Peninsula, MexicoSlide 15Impact CratersMegatsunamisEnergy of an impactMaterials indicating Meteorite ImpactsDiaplectic GlassWhat Happens to minerals that are there but not melted?DiamondsQuartz PolymorphsMeteorite composition•Major groupings:–Stony meteorites•Chondrites•Achondrites–Iron meteorites•Octahedrites, hexahedrites, ataxites–Stony-iron meteorites•Pallasites•Mesosiderites•Chondrites •Carbonaceous chondrite class –CI chondrite (Ivuna-like) group –CM-CO chondrite (mini-chondrule) clan •CM chondrite (Mighei-like) group •CO chondrite (Ornans-like) group –CV-CK chondrite clan •CV chondrite (Vigarano-like) group –CV-oxA chondrite (oxidized, Allende-like) subgroup –CV-oxB chondrite (oxidized, Bali-like) subgroup –CV-red chondrite (reduced) subgroup •CK chondrite (Karoonda-like) group –CR chondrite clan •CR chondrite (Renazzo-like) group •CH chondrite (Allan Hills 85085-like) group •CB chondrite (Bencubbin-like) group –CBa chondrite subgroup –CBb chondrite subgroup •Ordinary chondrite class –H chondrite group –L chondrite group –LL chondrite group •Enstatite chondrite class –EH chondrite group –EL chondrite group •Other chondrite groups, not in one of the major classes –R chondrite (Rumuruti-like) group –K chondrite (Kakangari-like) grouplet (a grouplet is a provisional group with <5 members)Chondrites•Stony meteorites – most common meteorites and represent the oldest solids that are the building blocks of the solar system•Parent bodies were small-medium asteroids, not planetoids!•Contain up to 80% chondrules, which were freely floating molten drops in space•Few m to 1 cm spheres•Mostly olivine and pyroxene, also feldspathic glass or crystals with minor troilite (FeS), chromite, phosphates •15 groups of chondritesChondrite groups•Ordinary – make up 80% of the meteorites and 90% of chondritic meteorites, abundant chondrules, variable Fe-Ni lead to H, L, and LL chondrites•Carbonaceous chondrites –less the 5% of chondritic meteorites, few chondrules, more lithophile elements (Ca, Mg, K, Cr, Al, Cl,…), high levels of water and organic compounds - many types based on characteristic specimen•Enstatite Chondrites – 2% of chondritic meteorites, very chemically reduced – enstatite-rich chondrules and abundant metal and sulfide mineralsPeekskill MeteoritePeekskill Meteor: October 9, 1992. This famous fireball was seen and filmed across several eastern states. It broke up into many fragments, one of which hit the trunk of Michelle Knapp's 1980 Chevy Malibu. When Ms. Knapp investigated a crash sound outside her Peekskill, NY home, she discovered the damaged trunk and found a warm 12-kg meteorite lying beside the car. 12-kg Ordinary Chondritic meteoriteCar – $10KMeteorite – $75KAchondrites•Stony meteorite similar to terrestrial basalts or plutonic rocks, represent 8% of meteorites grouped on the basis of Fe/Mn and 17O/18O ratios characteristic of the parent body•2/3 of these meteorites are HED type, originating from one asteroid, Vesta 4 - there is a large impact crater observed on this asteroid•Also includes Martian and lunar meteoritesLunar Meteorite Allan Hills 81005 The Johnstown Diogenite.Martian Meteorites•All are igneous, lherzolitic to basaltic composition, and some contain hydrated carbonates and sulfates, evidence of liquid water•ALH84001 is 4.5 ga, contains carbonate veins 3.6 – 4 ga, Organic matter (PAH), aligned magnetite crystals, proposed nanofossils (careful!!) – very controversial…ALH84001Nahkla MeteoriteALH84001 – round carbonate grainsIron Meteorites•5% of meteorites, but 90% of the mass of recovered meteorites and all of the largest meteorites (66 tons is the record) - primarily composed of iron-nickel alloy intergrowths:–Kamacite – Fe-Ni alloy at 90:10 to 95:5 Fe:Ni–Taenite – Fe-Ni alloy at 80:20 to 45:65 Fe:Ni–Widmanstätten pattern – finely interweaved Kamacite and Taenite (Octahedrites)•Classified on Ni content: Ataxites>Octahedrites>HexahedritesStony-iron Meteorites•Mix of iron-nickel alloy and silicate minerals (mostly olivine), 1% of meteorites–Pallasites are thought to form a the core-mantle boundary of differentiated asteroids–Mesosiderite – equal parts metal alloy and silicate with a breccia textureIdentifying a meteorite•Fusion crust – dull black to dark brown, often soft, can be weathered to red (but can flake off)•Density – generally dense•Chondrules are specifically meteoritic•Never porous, but can be ‘dimpled’ with surface depressions•99% of meteorites are magnetic•Unusually high Ni content•Fusion crust forms on entry through the atmosphereMeteorite/ Comet Impacts•P/T space??Chicxulub, Yucatan Peninsula, Mexico•K/T event at 64.98 ma, formed from a 6-12 mile diameter asteroid impact (50 megaton blast)Barringer Meteor Crater, Arizona, formed from Canyon Diable MeteoriteImpact CratersClearwater lakes, Quebec – 36+26km diameter, 290 ma•Many famous impact craters, hundreds known on earth (why might there have been plenty more??)–Sudbury, Ontario (250km diameter, 1.85 ga)–Chesapeake Bay (90km diameter, 35 ma)–Manson, Iowa (35km, 74ma)–Barringer, Arizona (1.2km, 49 ka)–Serpent Mound, Ohio (8km, 320 ma)Megatsunamis•Meteorite impact in the ocean displaces huge quantities of water instantly•The Chixculub crater impact generated a megatsunami 150-300 feet highEnergy of an impact•Kinetic energy – going from very fast to stopping is a BIG change in energy•What happens to that energy??•Impactite – any mineral formed as a result of this impactShatter coneMaterials indicating Meteorite Impacts•Tektites•Glass formed from impactDiaplectic Glass•Glass formed through fusion of different minerals – not melted, but fused…What Happens to minerals that are there but not melted?•Shock Quartz•Lamellae retaining evidence of impactDiamonds•Very small diamonds can form from impacts and are found in meteorite impact craters around the world•Diamonds can also form in meteorites- these can be gray to black•Lonsdalite - Hexagonal allotrope of diamond, specific to meteorite impacts, thought to form from graphite in meteoritesQuartz


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UVM GEOL 110 - Meteorite composition

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