Asteroids IIIWilliam Frederick Bottke Two hundred years after the first asteroid was discovered, asteroids can no longer be considered mere points of light in the sky. Spacecraft missions, advanced Earth-based observation techniques, and state-of-the-art numerical models are continually revealing the detailed shapes, structures, geological properties, and orbital characteristics of these smaller denizens of our solar system. This volume brings together the latest information obtained by spacecraft combined with astronomical observations and theoretical modeling, to present our best current understanding of asteroids and the clues they reveal for the origin an,d evolution of the solar system. This collective knowledge, prepared by a team of more than one hundred international authorities on asteroids, includes new insights into asteroid-meteorite connections, possible relationships with comets, and the hazards posed by asteroids colliding with Earth. The book's contents include reports on surveys based on remote observation and summaries of physical properties; results of in situ exploration; studies of dynamical, collisional, cosmochemical, and weathering evolutionary processes; and discussions of asteroid families and the relationships between asteroids and other solar system bodies. Two previous Space Science Series volumes have established standards for research into asteroids. Asteroids III carries that tradition forward in a book that will stand as the definitive source on its subject for the next decade. |
Contents
The Asteroids III Perspective | 3 |
Giuseppe Piazzi and the Discovery of Ceres | 17 |
Asteroid Orbit Computation | 27 |
NearEarth Asteroid Search Programs | 43 |
Analysis and Potential Impact Detection | 55 |
Observational Selection Effects in Asteroid Surveys | 71 |
Binzel R P 3 255 | 86 |
The Comparison of SizeFrequency Distributions of Impact Craters and Asteroids | 89 |
Asteroid Geology from Galileo and NEAR Shoemaker Data | 329 |
Mission Summary | 351 |
The 2001 Perspective | 367 |
Implications | 379 |
The Effect of Yarkovsky Thermal Forces on the Dynamical Evolution of Asteroids and Meteoroids | 395 |
Asteroidal Dust | 423 |
Laboratory Experiments and Scaling Laws | 443 |
Asteroid Interiors | 459 |
Origin and Evolution of NearEarth Objects | 101 |
Asteroid Masses and Densities | 103 |
Asteroid Rotations | 113 |
Cheng A F 351 | 121 |
Asteroid Photometric and Polarimetric Phase Effects | 123 |
Asteroid Models from Diskintegrated Data | 135 |
Geissler P E 527 | 149 |
Asteroid Radar Astronomy | 151 |
Howell E S 235 | 166 |
VisibleWavelength Spectroscopy of Asteroids | 169 |
Spectroscopic Properties of Asteroid Families | 180 |
Mineralogy of Asteroids | 183 |
Jopek T J 645 | 202 |
Asteroids in the Thermal Infrared | 205 |
725 | 208 |
Observations from Orbiting Platforms | 216 |
Lagerros J S V | 217 |
Larsen J 71 | 233 |
The Astronomical Record | 235 |
633 | 249 |
Physical Properties of NearEarth Objects | 255 |
Physical Properties of Trojan and Centaur Asteroids | 268 |
Asteroids Do Have Satellites | 289 |
Müller T G 219 | 310 |
Cratering on Asteroids from Galileo and NEAR Shoemaker | 315 |
Asteroid Density Porosity and Structure | 485 |
Evidence and Evolution | 500 |
S 331 | 512 |
Spin Rate Changes Tumbling Rotation States and Binary Asteroids | 517 |
J | 524 |
The Fate of Asteroid Ejecta | 527 |
Stokes G H 45 | 541 |
Collisional Evolution of SmallBody Populations | 545 |
Thermal Evolution Models of Asteroids | 559 |
367 485 | 571 |
The Smallest Terrestrial Planet | 573 |
Asteroid Space Weathering and Regolith Evolution | 585 |
The Determination of Asteroid Proper Elements | 603 |
Asteroid Family Identification | 613 |
Asteroid Meteoroid Streams | 645 |
Their Number and Identification | 653 |
Evolution of Comets into Asteroids | 669 |
Chronology of Asteroid Accretion and Differentiation | 687 |
Meteorite Evidence for the Accretion and Collisional Evolution of Asteroids | 697 |
Primordial Excitation and Depletion of the Main Belt | 708 |
Origin and Evolution of Trojan Asteroids | 725 |
Dealing with the Impact Hazard | 739 |
Asteroid Data Archiving in the Planetary Data System | 757 |
Color Section following page | 774 |
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Asteroids III William F. Bottke,Alberto Cellino,Paolo Paolicchi,Richard P. Binzel Limited preview - 2002 |
Common terms and phrases
253 Mathilde absorption features albedo Arizona aster asteroid belt asteroid families Asteroids III W. F. astrometry Astron Astrophys band Barucci Bell J. F. binary binary asteroids Binzel R. P. Ceres Chapman C. R. collisions comets composition craters curve density detection determined diameter distribution effect ejecta Eros Gaffey M. J. Gaspra Gehrels Harris A. W. Hudson R. S. Icarus images impact infrared Lebofsky lightcurve Lunar and Planetary main-belt asteroids mass Mathilde meteorites minerals Muinonen near-Earth asteroids NEAS NEOS objects oids optical orbit ordinary chondrites Ostro S. J. parameters parent body perturbation phase angles photometric polarimetric polarization Pravec pyroxene regolith resonances rotation S-type S-type asteroids sample Šarounová satellites scattering Science shape Shoemaker solar system space weathering spacecraft spectral spectrum surface telescope teroids thermal Tholen tion Toutatis Tucson Univ Vesta Veverka W. F. Bottke Jr wavelength Yeomans D. K. Zappalŕ Zellner