Defending Planet Earth Review from Goddard Symposium Mike A’Hearn mahearn@mac.com
Chixculub Every 50-100 Myears 7-13-11 Goddard Symposium
Airburst of oblique impactor Tunguska Airburst of oblique impactor 5-30 Mtons of TNT (20-130 Pj) 30-100m diameter impactor Everything flattened over >2000 km2 Possibly one every 200 years 1927 vs. 2008 7-13-11 Goddard Symposium
Size Distribution & Frequency 7-13-11 Goddard Symposium
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 7-13-11 Goddard Symposium
Kill Curves 7-13-11 Goddard Symposium
Annual Deaths LP Comets ignored ~10%, not important LP Comets ignored ~50% Whoops! 7-13-11 Goddard Symposium
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 300-600 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 7-13-11 Goddard Symposium
Mitigation Applicability 7-13-11 Goddard Symposium
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 7-13-11 Goddard Symposium
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 7-13-11 Goddard Symposium
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 7-13-11 Goddard Symposium
Insurance prevents destruction rather than compensating to rebuild Bottom Line Insurance prevents destruction rather than compensating to rebuild How much insurance do we want? 7-13-11 Goddard Symposium
Backup Slides