490 Veritas is a carbonaceous Veritasianasteroid, which may have been involved in one of the more massive asteroid-asteroid collisions of the past 100 million years. It was discovered by German astronomerMax Wolf atHeidelberg Observatory on 3 September 1902.
With a diameter of more than 100 kilometers, Veritas is the largest member and namesake of theVeritas family, a mid-sizedasteroid family of carbonaceous asteroids in theouter main-belt, that formed recently approximately8.5±0.5 million years ago.[2][7]: 8, 23 David Nesvorný of theSouthwest Research Institute inBoulder traced the orbits of these bodies back in time, and calculated that they formed in a collision of a body at least 150 km in diameter with a smaller asteroid. Veritas and Undina would have been the largest fragments of that collision which caused a "late Miocene dust shower". The family consists of more than a thousand known members including1086 Nata,2428 Kamenyar and2934 Aristophanes.
Substantiating Nesvorný's estimate,Kenneth Farleyet al. found evidence in sea-floor sediments of a fourfold increase in the amount ofcosmic dust reaching Earth's surface, which began 8.2 million years ago and tapered off over the next million and a half years. This is one of the largest increases in dust deposits of the past 100 million years.[8]
The suspected Veritas collision would have been too far fromJupiter for the fragments to have been slung into a collision course with Earth. However,solar radiation would have caused the resulting dust to drift inward to Earth orbit over a time span consistent with the record of dust in theocean sediment.
Today continuing collisions among Veritas-family asteroids are estimated to send five thousand tons of cosmic dust to Earth each year, 15% of the total.