Meteorite impacts Comparativ e energies No human in

Meteorite impacts Comparativ e energies No human in

Meteorite impacts Comparativ e energies No human in past 1,000 years has been killed by a meteorite

Direct observations of meteorite impacts Tunguska, Siberia, 30 June 1908a big bang above the Earths surface Shoemaker-Levy 9, July 1994 impacts hitting Jupiter

Direct observations of meteorite impacts In 1954, a 5-kg meteorite crashed through a house in Alabama the object bounced off a radio and hit the owner in the head Effects upon children

Indirect evidence of meteorite impacts Preserved craters on the continents, mainly the oldest parts (shields) Lac cratre in northern Qubec is a simple crater its rim diameter is 3.4 km, it is 250 m

deep, and it is 1.4 Ma in age Location map of some impact craters seen at the surface Lac cratre Meteor crater in Arizona is another

simple crater showing rim ejecta Manicouagan The Manicouagan crater in Qubec is a spectacular example of a complex crater Its original rim has been removed by erosionthe current diameter is 100 km It has an uplifted central core and outer rings, which are

filled by a lake Its age - 210 Ma - coincides approximately with a large extinction at the end of the Triassic period Manicouagan St. Lawrence River

Central uplift Asteroids and the Asteroid Belt The Asteroid Belt lies between Mars and Jupiterthere are about 4,000 objects As asteroids collide

with one another, they fragment and send pieces into near-Earth orbits Asteroids Asteroids are rocky fragments (diameter 10m to 1000 km) which

either: failed to consolidate into a planet, or represent remnants of a fragmented planet Asteroids Metallic: some stony types are strong and hard and may hit the

Earth. Weak, friable types likely will explode in the atmosphere at high altitudes. Comets Comets come from the far reaches of the Solar System (outer solar system, kuiper Belt and in the Oort Cloud). They mainly consist of frozen water, carbon dioxide, or

both with admixed small rock fragments and dust, thus are referred to as dirty icebergs or dirty snowballs They have highly elongate, elliptical orbits which bring them close to the Sun Comets The tail of the comet is produced as

ices melt and gases and dust particles are shed from the object. Generally explode in the atmosphere at high altitudes. Comet West, 9 March 1976

Comet P/Shoemaker-Levy 9, July 1994 This comet was first detected on 24 March 1993 It was broken apart by a close pass to Jupiter

on 7 July 1992 Hubble image, 1 July 1993 The sequence of events The collision of the comet with Jupiter occurred over several days, 16-22 July 1994

It was the first collision of 2 solar system bodies ever observed At least 20 fragments hit Jupiter at speeds of 60 km/second Energies Fragment A struck with energy equivalent to 225,000 megatons of TNT, the plume rising to

1000 km Fragment G was the biggie, with 6,000,000 megatons TNT energy and a plume rising to 3,000 km Fragment G (and K, L) created dark impact sites whose diameters were at least that of Earths radius

Other definitions Meteor: light through the sky. Most meteors are destroyed in Earths atmosphere. Meteoroid: matter revolving around the Sun or any object in planetary space too small to be called an asteroid or a comet Meteorite: a meteoroid which reaches the surface of the Earth without being vaporized

Stony meteorites (94% of all meteorites) Two types: Chondritescontain chondrulesthey are very old and primitive

Achondritesno chondrules Photo of a carbonaceous chondrite (carbon-bearing) Types of meteorites derived from asteroids

Achondrites have a metallic core and stony silicate mantle Metallic core As asteroids fragment, both

metallic and silicate pieces are produced Stony silicate mantle Iron meteorites These consist of nearly pure

metallic nickel and iron This photo shows an iron meteorite named ARISPE Stony-iron meteorites These are a mixture of

the previous two types Often they are fragmental, suggestive of violent processes This stony-iron meteorite is named ESTHER

Impact events 1. Probabilities 2. Nature of the event 3. Consequences 4. Mitigation 1. Probabilities of a collision What are the chances of a large meteorite

hitting Earth? As of 2003, ~700 objects with diameters > 1 km known to have orbits which intersect that of Earth And 30 new objects are discovered each year, with the search only 8% complete! Probabilities - Zebrowski

Zebrowski shows that, on average, collisions of 1 kmdiameter objects occur every 250,000 years Such an impact is sufficient to wipe out most of the human

population From Zebrowski (1997) Probabilities - Courtillot Is Zebrowskis estimate too high? Courtillot suggests it is

about 1 Ma between events In any case, you can see that these events are both very rare and very destructive From Courtillot (1999)

2. Nature of the event Impact cratering is an important process in the history of Earth and other planets 107 to 109 kg of meteoritic flux strikes Earth each year, mostly in the form of

dust Impact events The cratering process is very rapid Since the objects travel so fast (4-40 km/second), a huge amount of energy is transferred upon impact

Cratering A blanket of ejecta is dispersed around the crater rock is fractured, crushed, and broken In large impact events, the rock can even be vaporized (depending on the type of rock)

Cratering (continued) Very high pressures are reached, resulting in shock metamorphism (pressure-temperature increases) After the initial compression comes decompression, which may cause the rock to melt

Ejecta blanket Broken rock fracturing

Simple craters are basically simple bowls With time, the ejecta blanket outside the crater is eroded melt Central uplift

Complex craters are generated by rebound of the central core This core, as it decompresses, may melt There are about 200 large, well-preserved impact

craters worldwideBUT>>200 impact events during Earths history This map shows both SURFACE and SUB-SURFACE examples Consequences of a large impact event

These would apply for an object of about 1 km or larger Actually, you may not want to hear the list of death and destruction (or maybe you do)... Consequences 1

A base surge, similar to a volcanic pyroclastic flow, will be generated by the impact For a terrestrial impact, rock will be pulverized and/or vaporized, sending up huge amounts of dust into the stratosphere

Consequences 2 For an oceanic impact: huge amounts of water will be vaporized Global tsunamis will be generated, which will ravage the Earths coastlines Consequences 3

In the short term, global wildfires will be generated by the impact event These fires will burn uncontrollably across the globe, sending more soot, dust, and gas into the stratosphere Consequences 4 All this suspended dust and soot will cause global winter and global darkness

Acid rains will fall Crops will fail catastrophically The end result will be MASS EXTINCTIONS Consequences 5 One last interesting point: The impact likely will trigger devastating quakes around the globe, especially where

tectonic stresses are high (i.e., plate margins) Volcanism (flood basalts) may occur on the opposite side of the globe from the impact, as a result of shock waves travelling through the center of the Earth From Murck et al. (1996)

Mitigation The problem is the possibility of little or no warning There are proposals to use nuclear weapons and satellites to shoot down or destroy such killer objects For further edification, rent Armegeddon from Blockbuster (1998)

Good subject for a paper ! Two case studies Tunguska 1908, Russia The Cretaceous-Tertiary extinction, 65 Ma

Tunguska, Russia, 30 June 1908 Something big seems to have exploded in the atmosphere The exact cause is uncertain, but we

suspect a comet or a meteor Aerial view of Tunguska Natural Reserve What happened? The objects entry appeared to be at

an angle of 30-35 The object shattered in a series of explosions at about 8 km altitude

Tree blowdown from the explosions; Note parallel alignment of the trees Big fires In the central region, forests flashed to fires which burned

for weeks a herd of 600700 reindeer was incinerated Aligned trees Trees were felled in a radial sense

About 2,000 km2 were flattened by the blasts What happened? Our best scientific guess is that it was part of a comet 20-60

meters in diameter no crater was found and no meteoritic debris has been found Felled trees aligned parallel to each other

Area of devastation superimposed on a map or Rome. Yellow=charred trees; Green=felled trees The lack of a crater suggests disintegration above the surface

of the Earth The lack of solid debris implies a comet rather than an asteroid A global view

Soot from the fires circled the globe, producing spectacular sunrises and sunsets for months afterward The Tunguska event was the largest known comet/asteroid event in the history of civilization Impact events and mass

extinctions In the Phanerozoic (570-0 Ma), there have been two great extinctions of fauna and flora: 1) end of the Permian Period at about 250 Ma 2) end of the Cretaceous Period at 65 Ma These extinctions serve to divide geologic time in the Phanerozoic into three main eras

The Cretaceous-Tertiary (KT) extinction at 65 Ma End of the dinosaurs and other species In fact, about two-thirds of all species wiped out 80% of all individuals killed off Thereafter, mammals took over What caused the extinction?

The two main theories are: (1) a meteorite impact (2) flood basalt volcanism Some important questions Was the extinction of the dinosaurs rapid or prolonged? Or both? In other words, prolonged followed by

abrupt? Did a meteorite impact trigger volcanism? Note location of the Chicxulub crater to the Deccan basalts Was it a meteorite? Evidence for meteorite impact

High iridium at the K-T boundary Unique to the K-T boundary? 9 parts per billion (ppb) Ir in clay at the boundary Background in area <<1 ppb Earths crust < 0.1 ppb Some metallic meteorites ~500 ppb Iridium and the dinosaurs

The high iridium is coincident with the disappearance of the dinosaurs, as seen in the fossil record No dinosaur fossils above the K-T boundary, whereas there are lots below, as old as 165 Ma The iridium

The iridium may have come from impact of a metallic meteorite Circulation and settling of Ir-rich dust would result in global distribution of Ir at the K-T boundary Global effects

The atmospheric dust and gas from the impact event would cause global cooling (compare with nuclear winter) Global wildfires also would have been ignited by the fireball Other meteorite evidence

Spherulesthese represent melt droplets dispersed globally from the impact Shocked quartz this requires high pressures

Shocked quartz under the microscope The impact crater Located in the Yucatan Peninsula of Mexico, it is called Chicxulub It is completely buried, and was located

by petroleum geologists The size of the crater implies a meteorite about 10 km in diameter Chicxulu b crater Approx 300 km

Some incidental facts Many of the rocks associated with Chicxulub are evaporite sedimentary rocks (gypsum, anhydrite, etc.) containing sulfur (CaSO4) This sulfur may have been vaporized to produce sulfate aerosols in the atmosphere, contributing to global cooling

Incidental facts (ctd.) Other rocks in the vicinity are limestones (CaCO3) Vaporization of evaporites and limestone would inject sulfur dioxide and carbon dioxide into the atmosphere Sulfur dioxide causes cooling, CO2 causes

warming Climate change Short-term global cooling from: Dust from impact Soot from wildfires Injection of sulfur

Longer-term global warming from: Injection of CO2 Age of Deccan volcanism Interestingly, the Deccan Traps recently have been dated at 63-67 Ma And most of the volcanism occurred during

a 500,000 year period at 65 Mawhich is the K-T boundary This is basically a geological instant in time Some concluding remarks: meteorites vs. volcanoes Ir from a meteorite? From the Earths mantle via eruptions? The iridium anomaly is found not only at the

K-T boundary, but also extends several meters on either side Has the Ir been redistributed from an originally thin layer at the K-T boundary? Or is it a record of more than a single event? Globally speaking... A meteorite impact into the Chicxulub

region would produce: dust from the impact soot from global fires sulfur gases from evaporite rocks CO2 from limestone Basaltic volcanic eruptions would produce abundant sulfur, and probably CO2 also

Points in favour of a meteorite High iridium global distribution of spherules global distribution of shocked quartz Points in favour of volcanic

eruptions The ecological crisis began 105 years before the Ir-rich horizon and appeared to continue for a period of time afterward (~105 years?) Other mass extinctions appear to show some correlation with flood basalt events

5 major extinctions during the Phanerozoic (570-0 Ma) End Ordovician, 440 Ma end Devonian, 350 Ma end Permian, 250 Ma (Paleozoic-Mesozoic boundary)

end Triassic, 200 Ma end Cretaceous, 65 Ma Cenozoic boundary) (K-T event) (Mesozoic- An interesting aside

The K-T extinction is the only one for which there is good evidence for a meteorite impact Meteorite impacts - readings Alvarez, W., 1997. T. Rex and the crater of doom. Princeton, Princeton University Press.

Alvarez, L.W., W. Alvarez, F. Asaro, H. Michel, 1980. Extraterrestrial cause for the Cretaceous-Tertiary extinction. Science, v. 208, pp. 1095-1108. Frankel, C., 1999. The end of the dinosaurs. Cambridge, Cambridge University Press. Grieve, R.A.F., 1990. Impact cratering on the Earth. Scientific American, v. 262, pp. 66-73.

Meteorite impacts - web Two general sites of interest: Shoemaker-Levy:

Canadian sites on terrestrial impact craters:

Recently Viewed Presentations

  • Facility Location - University of Kentucky

    Facility Location - University of Kentucky

    Facility Location Part 3 by Anita Lee-Post Break-even analysis Determine the fixed and variable costs for each location. Identify the indifference point for each pair of location alternatives. Identify the ranges of output for which each location has the lowest...
  • Title 1

    Title 1

    Two registers are used to keep track of the organization: rsp address of the top element on the stack rbp address of the first element in the current stack frame
  • 1.1 Silicon Crystal Structure - University of California ...

    1.1 Silicon Crystal Structure - University of California ...

    This is smaller than the rectangular depletion region underneath the gate, by the factor This is the factor by which the depletion charge Qdep is reduced from the ideal One can deduce from simple geometric analysis that VT Roll-Off: First-Order...
  • 12.215 Modern Navigation Thomas Herring (, MW 11:00-12:30

    12.215 Modern Navigation Thomas Herring ([email protected]), MW 11:00-12:30

    High quality receiver: noise about 10 cm Low cost receiver ($200): noise is a few meters (depends on surroundings and antenna) In general: C/A code pseudoranges are of similar quality to P(Y) code ranges. C/A can use narrowband tracking which...
  • Chapter 8 Erosional Forces - Suffolk City Public Schools

    Chapter 8 Erosional Forces - Suffolk City Public Schools

    Chapter 8 Erosional Forces Section 8-2 Glaciers ... Esker! 2 Types of Glaciers Continental glaciers cover 10% of the Earth, mostly near Antarctica and Greenland. The continental glaciers are huge masses of Ice and snow, and are thicker than some...
  • Haute Autorité de Coordination de la Lutte contre la Corruption

    Haute Autorité de Coordination de la Lutte contre la Corruption

    Programme d'actions (suite) Sensibilisation et communication en direction des citoyens Elaboration de la politique nationale de lutte anticorruption Mobilisation des partenaires pour le financement du plan d'action national Elaboration de la politique nationale de lutte anticorruption Processus en cours depuis...
  • Inside Out by: Francisco Jimenez

    Inside Out by: Francisco Jimenez

    "That sounds like a doozy, my friend." Sue Ellen said. "Let's see what we can do about this." Sam and Sue Ellen walked around Sam's farm, inspecting the land and talking about what they could do. That's when Sue Ellen...
  • Volume &amp; Surface Area - Arizona State University

    Volume & Surface Area - Arizona State University

    Example of volume units are cm3, cubic feet, cubic meters or inches3. Surface Area Surface area is the flat area on the surface of a three-dimensional object. What you do is compute the area of all the sides of an...