On October 13, 2002, the NEAT asteroid survey discovered an apparently unusual asteroid using the 1.2m Oschin Schmidt Telescope at the Palomar Mountain Observatory. The object, then only known by it's temporary designation SYJ9ARB, was confimed less than 20 hours later by Kyle Smalley and Mitch Glaze at Powell Observatory. They found the asteroid sailing trough the Great Andromeda Galaxy, Messier 31. Of course, the proximity is only an illusion: While the asteroid was only about seven light minutes away when the image was taken, the galaxy is a world of it's own, in about 2.5 million light years distance.
These and some additional observations published on MPEC 2002-U03, confirmed that SYJ9ARB, which is now designated as 2002 TS190, has a unusual Mars-approaching orbit, which is nearly circular, but highly inclined (47°) to the ecliptic.
Asteroid 2002 TS190, imaged on October 14, 2002, by Kyle Smalley and Mitch Glaze, Powell Observatory, Louisburg, Kansas, U.S.A. Fifteen images, each a 45 second exposure, taken with a Apogee AP-8 CCD (funded by NASA OSS Grant) on a 0.75m Newtonian reflector, were stacked with Astrometrica for this view. (Click on the image to see the full resolution one megapixel image.) While the asteroid, shining at only 20mag, is hardly visible in this image, stacking the same images and compenasting for the asteroids motion of 2"/minute brings out the faint interloper, as shown in the inset.