(PhysOrg.com) -- A remarkable discovery was made by astronomers on 12 December 2010: an asteroid named Scheila had changed its appearance and looked more like a comet, complete with bright tail. An international team of scientists have used innovative modeling techniques to support the idea that the cause was another object impacting Scheila, ejecting material from the asteroid. The lead scientist of this study, Fernando Moreno of the Instituto de Astrofísica de Andalucía in Granada, Spain, will present the groups theory complete with up-to-date and refined estimates of impact date and size on Friday 7th October in Nantes, France at the joint meeting of the European Planetary Science Congress and the American Astronomical Societys Division for Planetary Sciences.
Asteroid are rocks that primarily circle the Sun between the orbits of Mars and Jupiter. In contrast, comets tend to have highly elliptical orbits taking them from the frozen extreme edges of our Solar System to within distances so close to the Sun that solar radiation causes material in the comet to vaporize and stream out, forming the characteristic tails. That an asteroid was observed with a comet-like tail puzzled astronomers and required some inventive modeling to explain.
Moreno and his team charted the brightness of Scheilas tail, noting how it dipped over the course of several weeks. They reached the conclusion that this unconventional tail was caused by another object smashing into Scheila and causing pieces to be blasted off.
Explains Moreno, The model we used involves a very large number of particles ejected from Scheila. We took into account gravity from the Sun, pressure radiation on the ejected particles, and Scheila´s gravity, which has a strong effect on the particles in its vicinity owing to its large mass.
It was initially thought that the impact event occurred between 11 November and 3 December 2010; further analysis to be presented at the EPSC-DPS Joint Meeting has now resulted in the date being refined to on or within three days of 27 November 2010. In addition, the latest calculations have dramatically increased the estimated size of the impactor, from 36m in diameter to 60 180m.
Moreno elaborates on how his team came to this conclusion: We applied a scaling law that uses impact velocity to indicate the mass of the impactor and ejected material. We know the impact should be about 5 kilometres per second because thats the average velocity of asteroids in the Main Belt. Using this number we predicted both the ejection velocity of the particles (50 to 80 metres per second) and the size of the impactor.
The model created correlates closely with observations taken over four days in December using the IAC-80 telescope on the Observatorio de Izaña, Tenerife, the 1.23 metre telescope of Calar Alto Observatory, and the 0.1-m telescope of the New Mexico Skies Observatory.
Scheila itself is fairly large as asteroids go at around 110 kilometres across, but it evidently felt the smaller objects punch.
Explore further: Heavy metal frost? A new look at a Venusian mystery