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PTYS 214 – Spring2011

Announcements. PTYS 214 – Spring2011. Homework #7 available for download from the class website Due Tuesday, Mar. 29 Class website: http://www.lpl.arizona.edu/undergrad/classes/spring2011/Pierazzo_214 / Useful Reading: class website  “Reading Material”

sybill-jordan
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PTYS 214 – Spring2011

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  1. Announcements PTYS 214 – Spring2011 • Homework #7 available for download from the class website Due Tuesday, Mar. 29 • Class website: http://www.lpl.arizona.edu/undergrad/classes/spring2011/Pierazzo_214/ • Useful Reading:class website  “Reading Material” http://en.wikipedia.org/wiki/Near-Eart_object http://neo.jpl.nasa.gov/stats/ http://users.tpg.com.au/users/tps-seti/swaprock.html

  2. Extra Credit Presentation Sara Cohen Viktoriya Stoeva

  3. Where did the K/P impactor come from? Asteroids: small bodies that are made of rock - Located in the Asteroid Belt (between Mars and Jupiter) Comets: small bodies made of rock and ice (“dirty snowball”) - Located in the Oort Cloud and in the Kuiper Belt Jupiter Inner SS Outer SS

  4. Comets • Among the oldest bodies in the solar system • Origin: Kuiper Belt or Oort Cloud (outskirts of the Solar System) • Contain organic material • Very porous objects rich in ices We do not know a lot about them First samples: 2006 Stardust Mission! Comet dust resembles asteroid material Comet Wild 2

  5. A natural experiment:Impact of Comet SL9 HST, May 1994 • Comet Shoemaker-Levy 9 was torn into pieces as a result of a close approach to Jupiter in July 1992 • Discovered in 1993, it collided with Jupiter at a speed of 60 km/s (135,000 mi/hr!) during the third week of July 1994 Dark “scars” lasted for months Plumes thousands of km high! HST, July 27, 1994

  6. Known asteroids Jupiter’s orbit Ecliptic Near Earth Objects (NEOs) Main Belt Mars’ orbit

  7. Near Earth Objects (NEOs) Asteroids in the neighborhood of the Earth, called Near Earth Objects (or NEOs) NEOs rarely get close to Earth enough to be considered a major hazard

  8. But the possibility exists! Peekskill Meteor, 9 Oct. 1992 – 40 seconds of glory!

  9. NEOs are potentially hazardous Peekskill Meteorite

  10. June 30, 1908The Tunguska Event Early morning: A big fireball raced through the dawn sky over Siberia (Russia) It exploded in the atmosphere over the Tunguska region with an estimated force of 1,000 Hiroshima bombs - The atmospheric shock wave knocked people off their feet and broke windows up to 650 km (400 miles) away - For few weeks, night skies were so bright that one could read in their light

  11. Tunguska: No crater! 1927: The first expedition to the site found a region of scorched trees about 50 km across and no crater! - Most trees had been knocked down pointing away from the center (“ground zero”)

  12. What happened? • It was the airburst of a meteor 6 to 10 kilometers above the Earth's surface • Near ground zero, trees were knocked down by the shock wave produced by a large explosion, similar to the effects observed in atmospheric nuclear tests in the 1950s and 1960s • Alternate Explanation:the Tunguska event is the result of an exploding alien spaceship or an alien weapon going off to "save the Earth from an imminent threat" No evidence was ever found by UFO sympathizers…

  13. Asteroids Hazard Bolides (energy <5 MT; D< 30 m ) – no crater  Great fireworks display (“shooting stars”), no damage Small Impact (<15Mt; D< 50 m) – crater ~1 km  Damage similar to large nuclear bomb (city-destroyer)  Average interval for whole Earth: >1,000 years Local catastrophes (<10,000 MT; D<250 m) – crater ~10km  Destroys area equivalent to small country  Average interval for whole Earth: >100,000 years Global catastrophe (>106 MT; D>1 km) – crater >50 km  Global environmental damage, threatening civilization  Average interval for whole Earth: >1 million years 1 MT= 1 Mton TNT equivalent= 4.21015 J

  14. Terrestrial Impact Frequency year century Tunguska Meteor Crater Hiroshima 10,000 years Time million yr Global catastrophe (for human civilization) End-Cretaceous billion yr 0.01 1 100 10,000 million 100 million TNT equivalent yield (MT) 1 MT= 1 Mton TNT equivalent= 4.1861015 J

  15. Spaceguard Program In the United States it is funded by NASA Goal: Find 90% of NEAs with D > 1 km by the end of 2008 Mar. 16, 2011: 822 discovered (>85%) D>1 km

  16. Comparison with Other Risks Statistical risk of death from impacts:1 in a million per year (about 1:20,000 over a lifetime) Much less than auto accidents, shootings (in U.S.) Comparable with other natural hazards (earthquakes, floods) It is a different kind of risk! • Average interval between major impact disasters is larger than for any other hazard we face(millions years) • A single event can kill millions of people (and other living things) ! • Unique as major threat to civilization (comparable to a global nuclear war)

  17. Impact cratering is normally regarded as a destructive process, dangerous for life… … but is it always that way?

  18. Impacts eject material at high speed Could an impact eject material into space? Could it eject rocks with LIFE into space?

  19. Could microbes contained in ejected rocks be ejected alive? Near-surface rocks can be ejected at high speed without serious damage (low shock) YES! Nicholson et al. (2009) Bacterial spores survive hypervelocity launch by spallation: Implicatons for lithopanspermia, 27th Lunar Planet. Sci. Conf.

  20. Microbes could be transferred from one large body to another, but they must survive a host of hazards! • Launch • Space exposure • Landing

  21. Material ejected from planets in large impacts wanders around the solar system, rather than traveling directly from planet to planetReaching another planet may take tens of millions of years! Can life survive this long without nurishment?

  22. Spore-forming bacteria are tough Spore-forming bacteria Bacillus Subtilis survived a 6-years spaceflight, experiencing vacuum, cold, lack of water and radiation Dormant microbes may survive for tens of millions of years (can contamination really be ruled out?) Science 268 (1995) 1060-1064

  23. Some micro-organisms can tolerate a lot of cosmic radiation, but not much UV, so they have to hide in rocks Deinococcus Radiodurans Listed in The Guinness Book of World Records as the world’s toughest bacterium

  24. Surviving reentry and landing is difficult …yet meteorites contain fragile organic molecules like amino acids ! So, It is highly probable that viable microbes could be carried from Earth to Mars or vice versa

  25. Quiz Time !

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