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 83
... surface is extremely complicated . Ideally , one wishes to know for each angle of illumination and each angle of observation what parts of the surface are both illuminated and seen . The surface can be specified statistically in terms ...
... surface is extremely complicated . Ideally , one wishes to know for each angle of illumination and each angle of observation what parts of the surface are both illuminated and seen . The surface can be specified statistically in terms ...
Seite 86
... surface of figure 1 , B = 0.032 mag / deg for Q = 0 in figure 3 . For a scattering law of type ( 1 ) , the geometric albedo p of the model planet is independent of Q. Thus , for the above model , it can be concluded that- ( 1 ) Large ...
... surface of figure 1 , B = 0.032 mag / deg for Q = 0 in figure 3 . For a scattering law of type ( 1 ) , the geometric albedo p of the model planet is independent of Q. Thus , for the above model , it can be concluded that- ( 1 ) Large ...
Seite 95
... surface is found on small grained powders oxidized by ferreous limonite or goethite . New laboratory measurements were conducted to prepare the simulation of the asteroidal surfaces . Samples of the lunar surface returned to Earth ...
... surface is found on small grained powders oxidized by ferreous limonite or goethite . New laboratory measurements were conducted to prepare the simulation of the asteroidal surfaces . Samples of the lunar surface returned to Earth ...
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