On a related note, interesting article in the Sept 18 Science about "An Anomamous Basaltic Meteorite from the Innermost Main Belt"
Briefly (ha!) the fireball was detected by the Desert Fireball Network in Australia on 20 July 2007, and based on the path, not only was the unusual pre impact orbit determined, but 2 pieces (150 and 174g) were recovered. The object was luminous from 62.8 km to 29.6 km in height along it's 65 km long path.The authors calculated the largest fragments were in the range of 100 to 250 g, so searched along the flight path where objects of that size would have wound up. (Heavier objects travel further, lighter ones not as far, so based on the speed you can roughly predict how far a mass of a certain size will travel.) The two recovered pieces were 97 meters south and 29 meters north of the projected path center line.
Turns out the orbit was an Aten orbit (earth crossing but with a < 1 AU) with perihelion inside Venus' orbit and aphelion just outside of earth's.
It was close to a V-type asteroid (which are in general believe to be derived from Vesta, whch was at one point a completely molten, hence differentiated asteroid) but there were overal important differnces which indicate it is a nearly unique type. First it has 3 different distinct grain sizes (unlike the typical eucrite). The finest grains are close in O isotopic ratios to a class called angrites (n=3) and a meteorite called Ibitira (brazil 1957). But only one other recovered meteorite came close to the bulk comosition, Asuka-881349 (Queen Maud Land Antarcita, 1988).
They projected the orbit backwards, finding a close approach to Venus in 2001 and earlier close approches to earth. (The orbital period would have been ~ 300 days). Using a numerical model they determined the most likely source region was the innermost asteroid belt with 98% probability. There was a 72% chance it came form the Saturnian v6 secular resonance, 26% that it came from many small Jupiter mean motion resonances in the inner belt, and 2% that it came from the Jupiter 3:1 motion resonance. The outer main belt (>2.8 AU) and Jupiter family comets were ruled out as possible sources.
So that's two meteorites with known orbits discovered in the last 2 years based on observations; 2008 TC3 in the sudan based on pre impact NEO detection, and this from a fireball network.
I'll try and find an online link.
MW