M
mikeemmert
Guest
I have, since the initial post in this thread, simulated a number of flybys of binaries by Neptune. Patterns are beginning to sort themselves out. There are several poosible results of a flyby. The binary can remain intact if the velocity is too high, corresponding to a high inclination of the binaries' orbit around the Sun with respect to Neptune's, or a high eccentricity or having the wrong angle with respect to Neptune. The binary can separate without a capture. One object can be captured and the other flung out at a higher velocity, as I believe happened to Triton/Xena.<br /><br />A fourth possiblity is that the binary objects can collide. The collision itself is beyond the scope of my computer's programming, but work by others regarding such a collision of a Lagrange object with Earth indicates that the cores of the objects can merge and the mantles can form another object.<br /><br />With the parameters I was using (1.3 km/sec velocity approaching from 120,000,000 km away from Neptune, 20,000 km distance between the binary objects, 310,000 -560,000 km approach distance with speeds at closest approach of around 7 km/sec), the objects collided right about at 1000 meters per second, about the speed of a rifle bullet.<br /><br />I think such a collision resulted in a second pair of objects; Pluto and 2003 EL61 "Santa":<br /><br />http://64.233.167.104/search?q=cache:-Is9XpqwZXEJ:www.gps.caltech.edu/~mbrown/2003EL61/rabinowitz.pdf%202003%20EL61%20Arizona&hl=en<br /><br />Santa is a strange object whose discovery was announced at the end of July. The most striking feature of it is it's high density, about 3000 kg/cubic meter. This is in a region of icy bodies with low densities. Another strange characteristic of this thing is it's extremely rapid rate of spin. It's day is only 3.9 hours long.<br /><br></br>