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This lecture from esys 150 explores the impacts of space objects on earth, focusing on comets and asteroids. Topics include the last major impact, the likelihood of future catastrophic events, impact scars on earth and the moon, sources of extraterrestrial debris, and environmental effects. Students will learn about meteoroids, meteors, meteorites, asteroids, and comets, as well as the rates of meteoroid influx and known impacts on earth.
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When was the last major space object impact? Are we likely to have a catastrophic rendezvous with a space object in the near future? IMAPCT SCARS AND SPACE OBJECTS (ABBOTT Ch 17) (F1) Introduction Earth moves through space occupied by comets and asteroids on different paths. Could a comet or asteroid destroy the human race? (F2 17.1) Impact Scars Earth dynamic so scars wiped out. Not a good place to look. Moon dead. Huge Number impact scars. By 3.9 Ba impacts died down (F3 17.2) Lunar Maria – dark colored, flood basalts 3.8 -3.2 Ba, few impact scars Sources of Extraterrestrial Debris Meteoroids Pieces of asteroids or comets orbiting the Sun. (F4) Meteor Debris fragmented asteroids/comets hits atmosphere creates meteor in Atmosphere. Meteorite becomes meteorite on ground, two types Irons – metallic, stones – made of rocks Stony more common entering atmosphere but more irons found Asteroids 9 planets orbit around sun, 4 inner rocky, 5 outer gaseous hydrogen and helium Asteroids rocky and metallic. Max diameters 933 km. Form in belts in space between Mars and Jupiter (F5 17.5) When asteroids collide, major collision, debris goes into gap Attraction from Jupiter that gives eccentric orbit. (F6 17.8) Clusters of asteroids have orbits that intersect the orbits of Earth and Mars Comets Divided into short and long period (F7) Short period in Kuiper Belt – a flattened disc from near Neptune to 50 Astronomical Units beyond sun and earth have orbits < 200 years. Long period in Oort cloud (dirty snowballs) – a spherical cloud of objects going out far beyond solar system, many millions of them. Comets essentially dirty snowballs. Have wildly eccentric orbits and a few come near to sun. (F8) Tail from sublimation to vapor, gives off gases. Gases pushed out by solar wind. Most only 15 km diameter. Have to be > 350 tons to burst through atmosphere Halley’s Comet comes every ~ 76 years. (F9 17.10 & 17.11) Ices contain carbon products and C, H, O and N in same ratio as human body Rates of Meteoroid Influx Meteoroids 100,000 enter earth’s Atmos. every day. Atmos. protects earth. Burn up. (F10 17.12) Cosmic dust Smallest meteorites 0.001 mm settle as cosmic dust. Shooting stars Incoming debris with 1mm diameter flame out as shooting stars Meteorites Debris weighing more than 1 gm falls onto earth’s surface. Outer surface burned off. Creates sonic boom KNOWN IMPACTS ON EARTH
Crater-Forming Objects greater than 350 tons, big ones hit near original speed, 164 world wide 57 in Canada and the US. (F11 17.20) Meteor Crater. Ar. World’s classic crater, on Colorado Plateau. 1 km wide crater, 185 m deep, rim 60 m high (F12 17.16) Evidence 1 Crater steep sided and closed. 2 Rim created by uplifting sedimentary strata. 3 Little hills outside inverted rock sequence. 4 Huge blocks limestone outside crater. 5 Crater holds 265 m shattered rock. 6 Numerous iron nickel meteorites in the area. 7 Very high T/P minerals, fused sand grains and shatter cones. No volcanic material nearby/No solution features. 30 m diameter meteorite, 50,000 years ago. Cretaceous/Tertiary Boundary Event Evidence Gubio, It. K & T have two very different assemblages (F13) Boundary well exposed, consist of clay layer Iridium 300 * normal Iridium is an iron loving element and goes with Iron into core But has a high % in iron-nickel meteorites. Iridium found everywhere on earth in clays at K/T boundary Clays have composition different from other clays, need Asteroid component Find shocked quartz and sandstone spherules indicating melting Site All round Caribbean evidence for nearby impact, Circular gravity structure Yucatan. PEMEX drill holes recover shattered rocks. 80 km inner ring. 195 km outer ring. (F14 17.24a) Angle Impact Gravity structures open to NW, low angle, Huge cloud over N America (F15 17.24b) ENVIRONMENTAL EFFECTS OF IMPACTS Crater-Forming Process Energy depends on size and speed. Objects > 350 tons impact at 30km/sec (F16 17.17a,b) 1 Shock so great meteoroid and crater rock vaporized, center of crater melted. 2 Release following shock wave causes floor in crater rise. (F17 17.17c,d) 3 Fractures walls fail, slide into crater, making it wider and shallower. The explosion creates the crater, thus always circular. Problems for Life from Impacts (F18 17.25) Earthquake Extrapolating up from nuclear explosions, K/T impact magnitude 11. Fires Local wild fires as result of Fireball Acid Rain Nitrogen oxides fall as acid rain from atmosphere Dust/soot block out the sunlight Warming after dust and soot settles greenhouse effect from CO 2 and Methane released K/T impact into limestone released lots of CO 2 , 10o^ C warming. EVENTS OF THE TWENTIETH CENTURY Biggest Event 20th^ Century Tunguska, Sib. 1908 Fireball exploded 8 km above ground. Heard 1000 km away