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 187
... ECLIPTIC PLANE T. KIANG Dunsink Observatory Ireland For examining the steady - state distribution of asteroids in the direction perpendicular to the ecliptic plane ( the z distribution ) , we shall assume all orbits to be circular ...
... ECLIPTIC PLANE T. KIANG Dunsink Observatory Ireland For examining the steady - state distribution of asteroids in the direction perpendicular to the ecliptic plane ( the z distribution ) , we shall assume all orbits to be circular ...
Seite 261
... ecliptic ? ( We will ignore Vesta because its free precession time will be very long as a result of its sphericity and any precession it may have will not be observable . ) Because the ecliptic is , in some sense , defined by the ...
... ecliptic ? ( We will ignore Vesta because its free precession time will be very long as a result of its sphericity and any precession it may have will not be observable . ) Because the ecliptic is , in some sense , defined by the ...
Seite 380
... ecliptic . Model calculations indicate that the polarization is a more sensitive discriminant than the intensity in determining the optical properties and size distribution of the dust particles . The maximum observed polarization Pmax ...
... ecliptic . Model calculations indicate that the polarization is a more sensitive discriminant than the intensity in determining the optical properties and size distribution of the dust particles . The maximum observed polarization Pmax ...
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