4. rock shattered and deformed
5. process of impact differentiates impact craters from those produced by other processes
7. craters on Mars and Moon have been subject of detailed study
8. Shoemaker-Levy impact with Jupiter, 1994
III. Mass extinctions
A. Mass extinction characterized by sudden loss of large numbers of plants and animals relative to
number of new species added
2. many hypotheses for causes of mass extinctions
4. Other possible impact-related extinctions include the terminal Pleistocene megafauna
extinctions (see A Closer Look: Possible Extraterrestrial Impact 12,900 years ago)
B. Late Cretaceous: K-T boundary mass extinction
1. 10-kilometer diameter comet or asteroid impacted Yucatan Peninsula
3. history of K-T impact hypothesis is one of intrigue, suspense, rivalries, and cooperation
5. impact crater discovered through pattern of cenotes on Yucatan Peninsula
6. impact caused vaporization of limestone bedrock, creating acid rain, and ejected dust into
atmosphere, causing mass extinction
IV. Minimizing the impact hazard
A. Risk related to impacts
2. smaller objects (few tens of millions): regionally catastrophic if in populated area
a. called Tunguska-type events
4. if Tunguska event is typical, an urban area is likely to be destroyed every few tens of thousands
of years
5. tremendous statistical variability in predicting likelihood and type of future impacts
B. Minimizing the impact hazard
1. identification of near-Earth objects (see A Closer Look: Near-Earth Objects).
2. an estimated 20 million extraterrestrial objects are in near-Earth orbit
a. only 4% are likely to penetrate atmosphere and create a crater
b. 50% are structurally weak and prone to explode at high altitudes
3. options to avoid or minimize hazard are limited
a. escape from effects of large comet or asteroid impact with Earth is unlikely
b. blowing apart an identified object would likely increase the hazard