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> Just how do we test this >hypothesis. Ellis says rocks formed at the time of the P-T extinction may >contain "unusual isotopes" of common elements. Got to add those to your >list Erwin. Some guys just have all the luck! ;) Haven't read that paper yet, but I brought up the topic with an astrophysicist doing his dissertation on some aspect of supernovae. Here is his response: > There would be a few obvious effects of our being that close to a >supernova. Fossil Aluminum 26 would probably be the easiest to find. Just >how >close was the supposed supernova? My quick, back of the envelop, calculation >is >that a supernova 5 light years away would, to an earth-based observer, be >equivalent to a second sun. It would last for a few months. To get >catastrophic >effects you would have to get closer (The effects would go as r^-2). However, >I >would expect a supernova even this close to leave a pretty clear isotopic >record. >In particular, minerals containing alot of aluminum should contain excesses of >Magnesium 26. These should be deposited after the supernova (You need time to >get >here) but at most about 1Myr later (The lifetime of Al26). Of course, the >further >away the less Al26. I'm not sure about where the limiting distance would be >before we couldn't detect any. Thomas R. Holtz, Jr. tholtz@geochange.er.usgs.gov Vertebrate Paleontologist in Exile Phone: 703-648-5280 U.S. Geological Survey FAX: 703-648-5420 Branch of Paleontology & Stratigraphy MS 970 National Center Reston, VA 22092 U.S.A.
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