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 34
... Vesta allows the repetition of the approaches , which cause the perturba- tions by Vesta in the mean longitude of Arete to accumulate . Although the total effect of the attraction of Vesta is small and the observations have various ...
... Vesta allows the repetition of the approaches , which cause the perturba- tions by Vesta in the mean longitude of Arete to accumulate . Although the total effect of the attraction of Vesta is small and the observations have various ...
Seite 35
... Vesta . Leveau ( 1896 , 1910 ) derived a reliable and homogeneous set of 252 normal positions from 68 oppositions of Vesta for the interval from 1807 to 1904. He applied systematic corrections to the observations as far as he knew them ...
... Vesta . Leveau ( 1896 , 1910 ) derived a reliable and homogeneous set of 252 normal positions from 68 oppositions of Vesta for the interval from 1807 to 1904. He applied systematic corrections to the observations as far as he knew them ...
Seite 59
... Vesta to be that of certain basaltic achondrite meteorites ( Mg - rich orthopyroxene or pigeonite ) . This identification , of course , refers to the composition of the Vesta surface minerals that , because of their abundance and albedo ...
... Vesta to be that of certain basaltic achondrite meteorites ( Mg - rich orthopyroxene or pigeonite ) . This identification , of course , refers to the composition of the Vesta surface minerals that , because of their abundance and albedo ...
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