Pg. 62 SOME INTERESTING STUFF ABOUT IMPACTS When we look at the Moon we see the record of impacts on its surface. Moon formed nearly 4.5 billion ya (YEARS AGO) intense impacts till 3.9 billion ya From space debris - earth must have been equally impacted. Only a few impact craters (astroblems) survive - why? Plate tectonics destroys them. Moon has no plate tectonics Astro =star and blema =wound fancy term for impact crater IS IT STILL HAPPENING TODAY? YES - Shooting stars, meteor showers. If hit earth= meteorite PG. 62-63 WHERE DOES SPACE DEBRIS COME FROM? 1. Asteroids-small bodies orbiting the sun a) Asteroid Belt - between inner and outer planets orbit the Sun b) small (< 600 mi diameter) rocky metallic and icy mass c) If all came together would create a planet only about 1/2 size of Moon d) may have been the 10th planet but gravity of Jupiter so strong could not combine to make that planet-interfered with suns gravity causes “conflict” and too energetic field for accretion to occur PG. 62-63 WHERE DOES SPACE DEBRIS COME FROM? 1. Asteroids-small bodies orbiting the sun e) rarely collide but when do may cause orbital path to change and likely they could collide with planets f) Apollo and Amor asteroid groups’ orbits intersect Earth’s orbit- possibility of collision ND pg. 457 fig. 16.7 PG. 62-63 WHERE DOES SPACE DEBRIS COME FROM? 1. Asteroids-small bodies orbiting the sun ADD NEAR-Shoemaker Space Craft Near Earth Asteroid Rendezvous-NEAR=asteroids that come within 121 million miles of Earth Spent about a year orbiting and collecting images and data WHY? Landed on Eros just to see if they could. WHY? PG. 62-63 WHERE DOES SPACE DEBRIS COME FROM? 1. Asteroids-small bodies orbiting the sun g) recently determined that they are numerous small bodies (Ida and Dactyl) weakly held together not always one solid piece Could be Could ALSO be h) they may be able to absorb large amounts of energy without being destroyed - so much for destroying an asteroid on a collision path!-Could explain this Pg. 63 2. Comets a) ice and rock debris - see tail as frozen outer portion turns to vapor producing gasses and dust. Tail lines up with solar wind so always away from the Sun DEMO b) small - up to 10 mi diameter c) trillions of them out there - most in Oort cloud Pg. 63 2. Comets ADD Kuiper Belt Oort Cloud Contain short-period orbit comets<200years Contain long-period orbit comets>200 years Flattened disk image link Spherical image link Comets are “dirty snowballs” Comets are “dirty snowballs” Pg. 63 2. Comets d.) many have eccentric orbits which bring them closer to Sun (and Earth) and then track far outside Neptune’s orbit e.) Halley’s comet is most famous - last visit 1986 ~76 year return interval Pg. 63 LOTS OF METEOROIDS GET TO EARTH 1.Up to 100 billion meteoroids enter Earth’s atmosphere EVERY 24 hoursWhat happens to them? 2.Most are small - and most burn up – shooting stars are burning meteoroids (< 1mm in size) a) burn due to atmospheric friction b) some deflected back to space c) hit Earth’s atmosphere is like hitting a solid (water is deadly if you jump from great heights) This causes destruction on impact with the atmosphere. Pg. 63 LOTS OF METEOROIDS GET TO EARTH 3.If large enough (>.04 ounce) when hit the ground we call them meteorites Can create a sonic boom when enter atmosphere hear on Earth if meteoroid is > basketball size! Oh yeah, and can cause injuries if fall on you YOU HAVE GOT TO BE KIDDING ME 1954 an 8.5 lb. meteorite crashed through woman’s House bounced off several walls and hit her. Doesn’t happen often but when it does BIG global impact Pg. 64 IMPACT SITES METEOR CRATER, AZ - Barringer Crater Near Winslow AZ Crater is 0.6 miles wide and 600 feet deep with a rim rising 100-200 feet. Why an impact site? How do we know? Evidence? 1) 2) 3) 4) 5) steep-sides and closed rim rocks tilted back inverted stratigraphy (rock layers) huge blocks of rock outside or crater crater floor is shattered 6) meteorite material collected from floor 7) high Temp. and high Pressure - fused sand (tektites) and shatter cones and shatter cone in situ 8) What else could make a round circular crater-like thingy? volcano and solution cavity (subsidence) but no evidence for either DRAWING/DEMO BEFORE AND AFTER SUBSIDENCE/SINKHOLE Age- 50,000 years old Meteorite 130 feet across Trees leveled, wildfires and dust darkened sky. Rock material vaporized by heat energy. Twice energy as Mt.St. Helen’s eruption. Pg. 65 K/T (Cretaceous/Tertiary) Event (dinos die) 1) 2) 3) 4) 5) 6) Evidence in clays at boundary – iridium actual plot shocked quartz grains melted sand spherules - tektites microscopic diamonds commonly in meteorites fire layers-post impact fires ratio of iridium/osmium similar to meteorites basically the same idea as #1 Impact Site - Chicxulub off Yucatan Tsunami sediments related to Chicxulub found in Mexico, TX and NJ and Carolinas! Another link Pg. 65 An Ancient Impact site in Chesapeake Bay Evidence: Presence of tektites shape- defined by ejecta and seismic data Age: 35.5 million years old EFFECT: caused a topographic low= rivers drained toward Pg. 65 Tunguska, Siberia 1980 1) meteorite exploded 5 miles above ground WHY?-probably icy and stoney NOT metallic 2) Blast heard over 600 miles away!! 3) 37 miles away a person burned and thrown 7 feet in air by blast 4) people 300 miles away knocked down 5) fires seen 12 miles away 6) Forest leveled about 80 million of them 7) overall very nasty - luckily no one lived close to the area! CONSIDER THIS: What if it would have happened over a highly populated area Meteor was between 165-100 feet in diameter Pg. 65 COULD THIS HAPPEN TODAY - sure First Remember NEAR-Shoemaker project WHAT ARE WE DOING ABOUT IT? NASA has 3 funded programs to address NEO - near earth objects ADD SIMPLY: they are cataloguing and assessing any potentially dangerous asteroids/meteors Things we could do… 1.) shoot it with a nuclear warhead. problems? 2.) Use focused solar energy to nudge out of the way. 3.) Towing/pushing with space craft. Problems? THE TRUTH: Early Detection is key. Interesting Article QUIZ CHECK THE LECTURE PAGE FOR REVIEW QUESTIONS