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 84
... calculated in this way for a surface with Q > 0 will be less than that found when Q = 0 at all phase angles a > 0. We will , in fact , have the following relationship : ( α , 2 ) = ( α , 0 ) Σ ( α , 2 ) ( 7 ) where ( α , Q ) is a ...
... calculated in this way for a surface with Q > 0 will be less than that found when Q = 0 at all phase angles a > 0. We will , in fact , have the following relationship : ( α , 2 ) = ( α , 0 ) Σ ( α , 2 ) ( 7 ) where ( α , Q ) is a ...
Seite 136
... calculated from the previously approximated pole , Stobbe found ( amin DB , the observed variation in the time of arrival of the minimum due to change in phase . Using the assumed pole positions , he determined ( a ' min DR , the calculated ...
... calculated from the previously approximated pole , Stobbe found ( amin DB , the observed variation in the time of arrival of the minimum due to change in phase . Using the assumed pole positions , he determined ( a ' min DR , the calculated ...
Seite 450
... calculated from those orbits terminating with Earth impact . Comparison of the calculated and observed data showed that none of these sources yielded data that agreed with the observed data . In fact , it was shown that only an initial ...
... calculated from those orbits terminating with Earth impact . Comparison of the calculated and observed data showed that none of these sources yielded data that agreed with the observed data . In fact , it was shown that only an initial ...
Inhalt
ASTROMETRIC OBSERVATIONS | 3 |
THE WORK AT THE MINOR PLANET CENTER | 9 |
DIAMETER MEASUREMENTS OF ASTEROIDS | 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 curve density determined diameter discussed distance Dohnanyi Dollfus Earth ecliptic effect ephemerides equation Eros families Figure flyby fragments function Gehrels Geophys gravitational 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 meteoroids 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 PHYSICAL STUDIES planetary planetoids polarization pole propulsion radius range rotation sample satellites scattering semimajor axis solar nebula solar system space spacecraft stream STUDIES OF MINOR surface trajectory Trojans velocity Vesta wavelength Whipple Zodiacal Light