“How Did Those Rocks Get Up There? Exploring Lake Smerdyachee, Russia” Earth2Class Workshops for...
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Transcript of “How Did Those Rocks Get Up There? Exploring Lake Smerdyachee, Russia” Earth2Class Workshops for...
““How Did Those Rocks Get Up There? How Did Those Rocks Get Up There? Exploring Lake Smerdyachee, Russia”Exploring Lake Smerdyachee, Russia”
Earth2Class Workshops for TeachersEarth2Class Workshops for TeachersLamont-Doherty Earth ObservatoryLamont-Doherty Earth ObservatoryOriginally presented 18 April 2015Originally presented 18 April 2015
Presented byPresented by
Dr. Dallas AbbottDr. Dallas Abbott
LDEO Research Scientist LDEO Research Scientist
Dallas has shared her research and data about impacts of asteroids, meteorites, and other extraterrestrial objects with us since 2002. Her studies have taken her to many parts of the world, from Australia and New Zealand to the Hudson River and the continental shelf off NJ/NY.
Today, she’ll discuss ongoing work in an area about 140 km east of Moscow, Lake Smerdyachee.
Some important concepts about impact cratersSome important concepts about impact craters
Form when a bollide (meteorite, asteroid Form when a bollide (meteorite, asteroid or comet) collides with a solid object or comet) collides with a solid object (planet or moon)(planet or moon)
Easily seen on our Moon, Mercury, and Easily seen on our Moon, Mercury, and Mars, where weathering and erosion are Mars, where weathering and erosion are slow slow
Often hard to recognize on Earth because Often hard to recognize on Earth because of the effects of weathering and erosionof the effects of weathering and erosion
Meteor Crater (Barringer Crater) in Meteor Crater (Barringer Crater) in Arizona was among the first recognizedArizona was among the first recognized
http://cass.jsc.nasa.gov/images/scraters/scraters_S10.gif
Impact craters on land have been known and studied for many years. This STS-9 image of Manicouagan Crater in northern Canada shows the remains of a collision estimated to have taken place 215 million years ago. It’s about 85 km in diameter.
http://antwrp.gsfc.nasa.gov/apod/ap001213.html
Many other craters have subsequently been Many other craters have subsequently been identified, especially by remote sensingidentified, especially by remote sensing
Approximately 190 are confirmed, with Approximately 190 are confirmed, with many other suspectedmany other suspected
Mostly within the stable cratons of North Mostly within the stable cratons of North America, Africa, Australia, and EuropeAmerica, Africa, Australia, and Europe
Earth’s greater gravitation pull probably Earth’s greater gravitation pull probably means it has been hit more, but water, means it has been hit more, but water, atmospheric weathering, and plate atmospheric weathering, and plate tectonics have destroyed or hidden many tectonics have destroyed or hidden many impact sitesimpact sites
High velocities at which meteoroids collide High velocities at which meteoroids collide with Earth explain the great effects from with Earth explain the great effects from
even small objectseven small objects
Velocities range between 11.2 km/sec Velocities range between 11.2 km/sec (escape velocity from Earth) and 72 km/sec (escape velocity from Earth) and 72 km/sec (orbital velocity of Earth plus escape (orbital velocity of Earth plus escape velocity of solar system)velocity of solar system)
Kinetic Energy released is proportional to Kinetic Energy released is proportional to square of velocitysquare of velocity
Effects is that meteorites are, gram for Effects is that meteorites are, gram for gram, more than 100x as powerful as TNT!gram, more than 100x as powerful as TNT!
Methods to identify impact locations Methods to identify impact locations include:include:
Siderophile elements (esp. Ir, Os, and Pt) Siderophile elements (esp. Ir, Os, and Pt) in “impact melt rocks”in “impact melt rocks”
““Shock metamorphism” in “target rocks” Shock metamorphism” in “target rocks” and mineralsand minerals
““Shatter cones”Shatter cones”High-pressure mineral phases, such as High-pressure mineral phases, such as
stishovitestishovite ““Diaplectic glass” and tektites in “ejecta Diaplectic glass” and tektites in “ejecta
blankets”blankets”
Many craters or remnants have been Many craters or remnants have been recognized by the presence of rare elementsrecognized by the presence of rare elements
““Siderophile elements” such as Ir indicate Siderophile elements” such as Ir indicate that terrestrial clays have been mixed with that terrestrial clays have been mixed with extraterrestrial materialsextraterrestrial materials
One of the best studied is the subsurface One of the best studied is the subsurface Chicxulub structure in Mexico, widely Chicxulub structure in Mexico, widely accepted at the location of the Cretaceous-accepted at the location of the Cretaceous-Tertiary boundary eventTertiary boundary event
Not exposed at the surface, it has been identified through geophysical studies of the gravitational field. Located near 21°N 90°W, the structure has a diameter of ~250-280 km. Its age has been calculated at 64.98 ± 0.05 million years
http://cass.jsc.nasa.gov/images/scraters/scraters_S37.gif
Impact Craters are classified as Impact Craters are classified as “Simple” or “Complex”“Simple” or “Complex”
““Simple Craters” are relatively small, have Simple Craters” are relatively small, have a smooth bowl shape, and a a smooth bowl shape, and a depth:diameter ratio of 1:5 to 1:7depth:diameter ratio of 1:5 to 1:7
““Complex Craters” are largely and show Complex Craters” are largely and show the effect of gravitational collapse of the the effect of gravitational collapse of the walls to produce a central peak or peak walls to produce a central peak or peak ringring
Connections between impacts and Connections between impacts and mass extinctions provide evidence for mass extinctions provide evidence for the still-unproved theory that such the still-unproved theory that such events may be the “metronome that events may be the “metronome that sets the cadence for biological sets the cadence for biological evolution on Earth.” evolution on Earth.” (Koeberl and Sharpton)(Koeberl and Sharpton)
What might happen when an impact occurs What might happen when an impact occurs in the ocean? Tsunami!in the ocean? Tsunami!
A tsunami is a giant sea wave or series of waves A tsunami is a giant sea wave or series of waves caused by disruption of the ocean surfacecaused by disruption of the ocean surface
Most tsunamis are connected with earthquakes Most tsunamis are connected with earthquakes or volcanic eruptions, but some may be caused or volcanic eruptions, but some may be caused by meteorite or asteroid collisionsby meteorite or asteroid collisions
For more information about tsunamis, go to For more information about tsunamis, go to http://www.geophys.washington.edu/tsunami/welhttp://www.geophys.washington.edu/tsunami/welcome.html come.html
Where Are Impact Craters Found?Where Are Impact Craters Found?
The “Fount of All Wisdom” (Wikipedia) The “Fount of All Wisdom” (Wikipedia) provides tables of confirmed and suspected provides tables of confirmed and suspected impact cratersimpact craters
http://en.wikipedia.org/wiki/http://en.wikipedia.org/wiki/List_of_impact_craters_on_Earth List_of_impact_craters_on_Earth
Impact Lakes in RussiaImpact Lakes in Russia
Many lakes in the interior of RussiaMany lakes in the interior of Russia7 show unusual features and may be 7 show unusual features and may be
impact craters, rather than karst, glacial, or impact craters, rather than karst, glacial, or other featuresother features
Understanding origins involves combining Understanding origins involves combining field observation, laboratory investigations, field observation, laboratory investigations, and statistical analysesand statistical analyses
NASA’s Jet Propulsion Laboratory NASA’s Jet Propulsion Laboratory provides much more information provides much more information
about impact craters throughout the about impact craters throughout the solar system in their “Welcome to solar system in their “Welcome to
the Planets” web sitethe Planets” web site
http://pds.jpl.nasa.gov/planets/http://pds.jpl.nasa.gov/planets/
Excellent information and classroom Excellent information and classroom activities have been created by the activities have been created by the Hawai'i Space Grant College, Hawai'i Hawai'i Space Grant College, Hawai'i Institute of Geophysics and Institute of Geophysics and Planetology, University of Hawai'iPlanetology, University of Hawai'i
http://www.spacegrant.hawaii.edu/http://www.spacegrant.hawaii.edu/class_acts/CrateringDoc.htmlclass_acts/CrateringDoc.html
Selected URLs about Impact CratersSelected URLs about Impact Craters
For more information/classroom activities:For more information/classroom activities:
http://www.solarviews.com/eng/edu/http://www.solarviews.com/eng/edu/craters.htmcraters.htmThe Meteor Crater home page: The Meteor Crater home page: http://www.meteorcrater.com/http://www.meteorcrater.com/A Webquest about impact craters: A Webquest about impact craters: http://earthview.sdsu.edu/trees/impact.htmlhttp://earthview.sdsu.edu/trees/impact.html