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Defending Planet Earth

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Presentation on theme: "Defending Planet Earth"— Presentation transcript:

1 Defending Planet Earth
Review from Goddard Symposium Mike A’Hearn

2 Chixculub Every Myears Goddard Symposium

3 Airburst of oblique impactor
Tunguska Airburst of oblique impactor 5-30 Mtons of TNT ( Pj) m diameter impactor Everything flattened over >2000 km2 Possibly one every 200 years 1927 vs. 2008 Goddard Symposium

4 Size Distribution & Frequency
Goddard Symposium

5 From Space vs. from Earth
Finding Them From Space vs. from Earth Earth-trailing orbit is fastest From Earth’s surface is cheapest IR vs. Visible IF! In space, IR seems better Goal of G. E. Brown survey 90% of >140m Goddard Symposium

6 Kill Curves Goddard Symposium

7 Annual Deaths LP Comets ignored ~10%, not important
LP Comets ignored ~50% Whoops! Goddard Symposium

8 Mitigation (per NRC) 4 approaches depending on circumstances
Civil defense (evacuation, sheltering, first aid, etc. Up to 50m diameter? Slow Push-Pull (tug, solar heating, albedo change, gravity tractor, et al.) Needs decades to operate (plus time to build, etc.) Max size m diameter Gravity tractor closest to ready and least dependent on properties of NEO Kinetic Impacts (Super Deep Impact) sensitive to porosity of top meters to tens of meters momentum transfer efficiency not known much wider range of applicability (max size 1 to 1.5 km, shorter warning for small ones) Nuclear blast standoff blast best works up to 10 km and relatively short warning Goddard Symposium

9 Mitigation Applicability
Goddard Symposium

10 Don Quixote-like mission
What Next? Don Quixote-like mission a rendezvous spacecraft at a small NEO followed by a large impactor biggest gain in knowledge directly related to mitigation Guess $1.5G; Good for international collaboration Gravity tractor demonstration fewer unknowns other than engineering second priority Apophis a possible target but any small NEO will do Can’t predict which might need to be used first Small NEO is by far the most likely Warning time very uncertain but short warnings are likely at ~100m diameter or less Goddard Symposium

11 Research Needs Momentum transfer Warning times
Tails of orbital distribution NEO properties - spin & shape, multiplicity, & especially porosity and density lots for science but not so much for hazard mitigation hence radar programs at Arecibo and Goldstone Physics of airbursts search strategy - death plunge vs. full survey Effects of the wide range of NEO properties on the mitigation strategy tsunami generation NEO disruption Goddard Symposium

12 Incomplete Mitigation
Risk of incomplete mitigation could lead to paranoia or even retaliation Risk of retaliation could lead to total inaction Requires official, working level close cooperation Goddard Symposium

13 Insurance prevents destruction rather than compensating to rebuild
Bottom Line Insurance prevents destruction rather than compensating to rebuild How much insurance do we want? Goddard Symposium

14 Backup Slides


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