Don Quixote: An Asteroid that is a Living Comet
Friday, October 11, 2013
Science Update - A look at CfA discoveries from recent journals

Near Earth Objects (NEOs) are asteroids or comets whose orbits sometimes bring them close to the earth's orbit. An NEO could therefore someday collide with the Earth -- giving them considerably more parochial interest than most objects in astronomy. The 1908 Tunguska event, for example, that flattened over 2000 square kilometers in Russia was by some basic estimates caused by an asteroid only 60 meters in diameter. The asteroid that struck Siberia last spring (the Chelyabinsk meteor) was only about 40 meters in diameter. While it is relatively easy to detect an NEO in visible light by watching its movement across the sky from night to night, determining its size is more difficult. This is because the optical brightness of an NEO is the result of two factors, its size and its reflectivity. CfA astronomers have for several years been using the IRAC infrared camera on Spitzer to measure the infrared light emitted from NEOs, and modeling the flux to determine the reflectivity and thus the sizes of NEOs.

NEOs are thought to originate from collisional fragments of objects in the asteroid belt beyond the orbit of Mars, and over 10,000 NEOs are known today. Short-period comets can also be NEOs, Unlike the asteroids, these comets most likely originated in the Kuiper belt, a reservoir of icy bodies outside the orbit of Neptune. Their orbits are disturbed as a result of gravitational perturbations with the giant planets, and some end up as NEOs. As they get closer to the Sun these comets become active and produce comae and tails, as expected for comets, but the activity is significantly briefer than their orbital lifetimes near the Earth which are estimated to last tens of millions of years. As a result, it is very likely that the NEO population being studied includes a significant number of extinct comets. So far 160 of them have been identified.

The NEO asteroid Don Quixote was discovered in 1983, and infrared and optical measurements indicate that it is big: about 18.7 kilometers in size, making it the third largest known NEO. Its reflectivity, and its particular orbit, suggested to astronomers that it was actually an extinct comet. CfA astronomers Joe Hora and Howard Smith, together with a team of colleagues, used Spitzer to study it. Although it is so large and bright that it had already been measured in the infrared, the scientists wondered if the more sensitive Spitzer measurements could discern something about its putative cometary nature. After careful processing of the comet's image, which was so bright in the infrared that it virtually blinded the camera, the team discovered a tail to this comet extending about 100,000 kilometers. From the infrared color of the tail, the team also concluded that the infrared light is largely produced by carbon dioxide gas being emitted from the comet's surface at a rate of about 7000 liters per second. The result, besides highlighting the advantages of more sensitive observations of known bright asteroids, suggests that carbon dioxide ice can remain frozen in near-Earth space over a very long time.

Reference(s): 

"The Discovery of Cometary Activity in Near-Earth Asteroid (3552) Don Quixote," Michael Mommert, J. Hora, A. W. Harris, W. Reach, J. Emery, C. Thomas, M. Mueller, D. Cruikshank, D. Trilling, M. Delbo, and H. Smith, ApJ 2013 (in press)