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Eric wrote:
I see articles where they have taken 2 pics of an object,(eg a comet or asteroid) and the movement from pic 1 to pic 2 is only a part of an inch as measured on the photos. How do they calculate the orbit of an object with so little information? I often wondered the same thing myself. Apparently initial orbital calculations for comets assume they're parabolic at least removing one degree of freedom from the calculations. Presumably initial calculations for asteroids are that they are in circular orbits. I understand that initial calculations aren't very accurate, but then the next thing you here is that they've found the object in photos from 100yrs back. Presumably you need total precision to get back like that. Hubble has just recovered a satellite of Uranus (Perfida ?) originally seen in Voyager II photos. How they can tell whether it's taken n orbits or (n+1) orbits in the intervening time I don't know. Joe -- Joseph Mack NA3T EME(B,D), FM05lw North Carolina jmack (at) wm7d (dot) net - azimuthal equidistant map generator at http://www.wm7d.net/azproj.shtml Homepage http://www.austintek.com/ It's GNU/Linux! |
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On Sun, 25 Dec 2005 20:27:19 GMT, mack wrote:
I often wondered the same thing myself. Apparently initial orbital calculations for comets assume they're parabolic at least removing one degree of freedom from the calculations. Presumably initial calculations for asteroids are that they are in circular orbits. See my reply to Eric. There is a method, developed by Olbers, that assumes a parabolic orbit. However, more general methods are usually used, and these produce orbital elements without any initial assumption about the type of orbit. That is, they simply produce the elements, which determine whether the orbit is parabolic, hyperbolic, or elliptical. I understand that initial calculations aren't very accurate, but then the next thing you here is that they've found the object in photos from 100yrs back. Presumably you need total precision to get back like that. The initial calculations can be very accurate- it depends on how large a section of the orbit the measurements are collected. One problem with interpolating back in time is that the effect of perturbations can become significant. Identifying an object in an old photo is usually one part calculation and one part luck. Objects are seldom exactly where they are calculated to be. Normal orbital elements assume a two-body system. That is usually a good approximation in the short term, but not over long periods. Hubble has just recovered a satellite of Uranus (Perfida ?) originally seen in Voyager II photos. How they can tell whether it's taken n orbits or (n+1) orbits in the intervening time I don't know. I'm not familiar with this specific case, but normally, the initial error in calculating the orbit is small enough that it would take a very long time before the positional uncertainty would become so large that you didn't even know which orbit you were in. _________________________________________________ Chris L Peterson Cloudbait Observatory http://www.cloudbait.com |
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