Dr. Faith Vilas is the 2019 recipient of the Whipple Award, the highest honor given by the Planetary Sciences section of AGU. During her more than 40 year career, Dr. Vilas has pioneered remote sensing of the solar system, pushing its capabilities through instrument design and expert observations of a variety of targets. Dr. Vilas studies the surface composition of airless bodies including asteroids, moons, and the planet Mercury. She has made ground-based visible wavelength spectroscopy her focus and has excelled in pulling out small but telling spectral features in the reflectance spectra of these airless bodies.
Examples of her groundbreaking work include her analysis of subtle absorption features in reflectance spectra of low-albedo (presumed primitive) asteroids. In particular, this includes a feature centered near 0.7 micron, which is caused by the action of aqueous alteration—evidence of water’s action throughout history in the asteroid belt. She showed that Galileo broadband data of the Moon exhibited the 0.7-micron feature, indicative of an aqueous alteration product near high southern latitude craters—an initial detection of lunar hydration, well before later reports based on infrared spectral features.
Vilas’s dedication to planetary science is also reflected in her contributions to the field in the form of service to the community. Examples include serving as the NASA Discovery Program Scientist; program director for planetary astronomy at the National Science Foundation; chief scientist of the NASA Planetary Data System; the inaugural NASA Small Bodies Assessment Group (SBAG) chair; chair of the American Astronomical Society Division for Planetary Sciences; and vice chair and chair of the Detection and Characterization Sub-committee on the 2009 National Academies’ study on near-Earth object detection, characterization, mitigation, Defending Planet Earth.
The impact of Dr. Vilas’s work in these areas cannot be overstated.
—Amanda Hendrix, Planetary Science Institute, Colorado
Space weathering effects on the rocky S‐class asteroids are well understood. However, on the low‐albedo C‐complex asteroids, such...