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|BILL HARTMANN'S SCIENCE RESEARCH PAGE|
My scientific research has general involved the origin and evolution of the planetary system and planetary surfaces. Special interests have included of evolution of surface features, craters, and interplanetary bodies. Career highlights:
|In 1962, I was lead author, with G. P. Kuiper, in the first recognition of multi-ring impact basins with concentric and radial structure on the moon, including the discovery of the Orientale basin bullseye on the east limb of the moon. Such basins have since been recognized on most cratered planets and satellites. This was first recognized on "rectified photos" in which telescopic photos of the moon were projected on a globe.
In 1965 I used crater counts on the moon and Earth to predict successfully that the lunar lava plains have an age of "about 3.6 x 109 years" (Icarus, 4:164). The date was confirmed five years later with Apollo samples from the moon. This work helped pioneer the usefulness of craters for interpreting planet surface ages; the 1966 Nininger Meteorite Award was shared for this work.
| Discovery of the Orientale Impact Basin. Drawing by William K. Hartmann from Earth-based photos showing multi-ring basin on the limb of the moon, as it appears from Earth. From Hartmann and Kuiper, 1962, Comm. Lunar and Planetary Lab. 1:51-66.
|In 1971-72 I was a co-I on the Mariner 9 mission which first mapped Mars in detail. With Bruce Murray, Carl Sagan, and others on the imaging team, we discovered Mars' dry river channels, volcanoes, and other features.||
Mariner 9 photo of a martian channel, Nirgal Vallis.
|In 1974-5, I was lead author, with D. R. Davis, of what has become the most widely accepted theory of the origin of the moon, by impact of giant planetesimal at the close of the planet-forming period. See PSI's Origin of the Moon page.||Diagram from Hartmann and Davis (Icarus, 1975) showing schematic history of growth of planetesimals near Earth's orbit. Our suggestion was that the 2nd-largest body grew to large size before hitting Earth, ejecting mantle material that formed the moon.|
|In the 1980s, I worked with D. P. Cruikshank, David Tholen, and others to carry out observations at Mauna Kea Observatory on the relationships of asteroids and comets, with D. P. Cruikshank, D. Tholen, and others. Our 2-color diagram of visual and infrared colors (right) showed the close spectroscopic relation of comets and outer solar system asteroids. Bright, icy satellites are in the lower left corner (bluish-white colors), while comets and carbonaceous types of asteroids ("C, P, and D" taxonomic types with brownish-black colors) fall in the upper right corner. We were probably the first to recognize that comets have similar black surface materials (4% reflectivity) to those on outer solar system asteroids. This proposal was controversial at the time, but confirmed a few years later by the Giotto probe at Halley's comet.||
2-color diagram relating comets to the sequence of colors of icy bodies and asteroid taxonomy of outer solar system. From this diagram we correctly predicted in 1985, prior to Halley's comet's arrival, that its nucleus has an albedo of 0.04. Cruikshank, Hartmann, and Tolen, Nature, 315: 122-124, 1985
|Our program also yielded proof that Trojan asteroid 624 Hektor was one of the largest highly elongated bodies in the solar system, and the discovery that "asteroid" 2060 Chiron had erupted and turned into a comet. Generally, our work aided the recognition that comets and asteroids could no longer be considered as independently as had been traditional. Asteroid 3341 was named "Hartmann" in recognition of the research on small bodies.
In 1997, I was named the first winner of the Carl Sagan Medal of the American Astronomical Society's Division of Planetary Sciences, for communication of science to the public.
I'm concentrating my research efforts on Mars Global Surveyor's new data from Mars, as part of my work with the MGS imaging team. The results show the importance of windblown dust in blanketing and shaping much of the topography at 10-meter scale. More discussion is given in PSI's Mars Global Surveyor page.
Models of 624 Hector. Is it an elongated single body (top), two strong rocky spearheaded bodies in contact (middle), or two weak rubble-pile objects elongated by rotationaly forces (bottom)?
Copyright William K. Hartmann