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 177
... elements , all of the above studies looked for clusterings of the semimajor axis a , the proper eccentricities e ' , and proper inclinations i ' . The calculation of proper elements involves using a theory of secular perturbations to ...
... elements , all of the above studies looked for clusterings of the semimajor axis a , the proper eccentricities e ' , and proper inclinations i ' . The calculation of proper elements involves using a theory of secular perturbations to ...
Seite 200
... elements and the osculating elements , a random distribution in ẞ implies a prevalence of certain values of π . The resulting direction of maximum concentration of the osculating perihelia depends on the semimajor axis a . In the outer ...
... elements and the osculating elements , a random distribution in ẞ implies a prevalence of certain values of π . The resulting direction of maximum concentration of the osculating perihelia depends on the semimajor axis a . In the outer ...
Seite 337
... elements a , e , and i . Brouwer ( 1951 ) , who restudied this problem using the proper elements , has added several new families . Arnold ( 1969 ) introduced computer methods in the classification of families and found additional ...
... elements a , e , and i . Brouwer ( 1951 ) , who restudied this problem using the proper elements , has added several new families . Arnold ( 1969 ) introduced computer methods in the classification of families and found additional ...
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