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JRS: In article , seen in
news:sci.space.policy, Henry Spencer posted at Sun, 15 Feb 2004 23:04:56 :- In article , Dr John Stockton wrote: A close encounter with a planet can split a rubble pile into a pair of rubble piles, by tidal interaction. (In fact, one of the points offered in support of the rubble-pile hypothesis is precisely that we see a suspiciously large number of double asteroids, which ought to be fairly rare unless there is some specific mechanism that creates them.) Why a pair of rubble piles? Half a rubble pile is still a rubble pile, and should itself be split (ignoring the presumably improbable case of an encounter virtually tangent to the Roche limit). If memory serves -- I didn't pay close attention to the details -- the two-way split of a rubble pile is a non-trivial interaction between tidal forces and the rotation of the original rubble pile, and generally does not involve further splitting of the resulting two piles. Multi-way splits of fragile bodies are certainly possible, as witness SL9, but they generally don't leave the fragments in orbit around each other. OK, I can easily enough believe that if the spin rate gives a centrifugal effect non-negligible in comparison with surface gravity, then the break-up will occur at a greater distance, and that the subsequent distribution of angular momentum from spin into spin + spin + orbital will leave the new spins insufficient for further break-up. "The satellite is here assumed not to be spinning." is now added to my Roche material in gravity3.htm. -- © John Stockton, Surrey, UK. Turnpike v4.00 MIME. © Web URL:http://www.merlyn.demon.co.uk/ - FAQqish topics, acronyms & links; some Astro stuff via astro.htm, gravity0.htm; quotes.htm; pascal.htm; &c, &c. No Encoding. Quotes before replies. Snip well. Write clearly. Don't Mail News. |
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