Thanks to movies like "Armageddon" and "Deep Impact", we all are aware of asteriods and comets and how they can crash into the Earth, causing death, destruction and doom for life here. (Actually, I knew this stuff even before such movies.) But the planet has had numerous near-misses over the years, and we think nothing of it--which is okay, of course. But the other day I was asked by my nephew about the moon's effects on the Earth's tides, and it just occurred to me that even a near miss by an object that is massive enough could cause serious problems for our world through its gravitational forces alone. My question is, how massive would such an object have to be before being a threat? For example, say a white dwarf star (or some other such star) goes supernova, and in the process throws out a fragment of white dwarf matter. How massive would that fragment have to be to cause gravitational chaos for the planet? I know it wouldn't have to be big; how massive would it need to be?
2007-06-06
09:47:19
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5 answers
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asked by
Mr James
1
in
Science & Mathematics
➔ Astronomy & Space