Physical Studies of Minor PlanetsScientific and Technical Information Office, National Aeronautics and Space Administration, 1972 - 687 Seiten " ... Some papers and discussions included in this book even though they were not presented at the meeting. In some respects, therefore, the book is independent of the colloquium. Several papers had been invited long beforehand with the request to publish them as review papers. The lack of a modern textbook on minor planets is keenly felt, and the proceedings of this meeting, with these additions, should provide a good reference book."--Page viii. |
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Seite 284
... collisional processes and their sum for two different average collisional velocities , as indicated . The population index of the crushed fragments during each collision n is taken to be the experimental value 1.8 . The value of a at ...
... collisional processes and their sum for two different average collisional velocities , as indicated . The population index of the crushed fragments during each collision n is taken to be the experimental value 1.8 . The value of a at ...
Seite 439
... collisional destruction ; e.g. , 107 yr . However , there is good reason to believe that the destruction lifetime is indeed on this order . Dohnanyi ( 1969 ) has reexamined the problem using an improved mass distribution function and ...
... collisional destruction ; e.g. , 107 yr . However , there is good reason to believe that the destruction lifetime is indeed on this order . Dohnanyi ( 1969 ) has reexamined the problem using an improved mass distribution function and ...
Seite 457
... collisional destruction will be to cut off the high exposure age " tail " on figure 5 and bring the calculated results into even better agreement with the observed data . For asteroidal sources , the effect is greater because for ...
... collisional destruction will be to cut off the high exposure age " tail " on figure 5 and bring the calculated results into even better agreement with the observed data . For asteroidal sources , the effect is greater because for ...
Inhalt
ASTROMETRIC OBSERVATIONS | 3 |
THE WORK AT THE MINOR PLANET CENTER | 9 |
DIAMETER MEASUREMENTS OF ASTEROIDS 25 | 25 |
Urheberrecht | |
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accretion albedo Alfvén Anders Apollo Apollo 12 Apollo asteroids asteroid belt asteroid families Astron Astrophys axis brightness Brouwer Ceres chondrites collisional collisions cometary comets counterglow craters curve density determined diameter discussed distance Dohnanyi Dollfus Earth ecliptic effect equation Eros families Figure flyby fragments function Gehrels Geophys gravity heliocentric Houten Icarus impact interplanetary dust iron meteorites jetstream Jupiter km/s Kuiper launch libration lightcurve longitude lunar magnitude Mars Mars-crossing asteroids mass distribution material measurements meteor meteoroid minor planets mission Moon NASA number of asteroids numbered asteroids objects Observatory observed obtained orbital elements Pallas parent bodies particles percent perihelion perturbations phase angle phase coefficient photometric planetary planetoids polarization pole propulsion radius range relative rotation sample satellites scattering semimajor axis solar nebula solar system space spacecraft stream surface target telescope trajectory Trojans velocity Vesta wavelength Whipple Zodiacal Light