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 229
... present terrestrial planets and the asteroids ) and Mmax = 1.0M . With these values for the masses and V = 0.02 km / s , N ( ∞ ) = 3508 for pp = 5.5 g / cm3 and 3269 for pp = 3.6 g / cm3 ; whereas for V = 0.04 km / s , N ( ∞ ) = 1752 ...
... present terrestrial planets and the asteroids ) and Mmax = 1.0M . With these values for the masses and V = 0.02 km / s , N ( ∞ ) = 3508 for pp = 5.5 g / cm3 and 3269 for pp = 3.6 g / cm3 ; whereas for V = 0.04 km / s , N ( ∞ ) = 1752 ...
Seite 258
... present alined state . We wish to present a different interpretation of the peculiar alinement phenomenon . We will present directly below calculations showing that at least a few major impacts should have taken place on the large ...
... present alined state . We wish to present a different interpretation of the peculiar alinement phenomenon . We will present directly below calculations showing that at least a few major impacts should have taken place on the large ...
Seite 448
... present ; it is conceivable that in the outer solar system there are additional unobservable families of small bodies of some kind . However , it seems most fruitful to give first consideration to known classes of bodies , rather than ...
... present ; it is conceivable that in the outer solar system there are additional unobservable families of small bodies of some kind . However , it seems most fruitful to give first consideration to known classes of bodies , rather than ...
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