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. |
Im Buch
Seite 48
... albedo . In this way systematic errors from many diverse sources are mitigated , but other errors are introduced . For example , error from the visible phase integral q for 4 Vesta is introduced if the result is interpreted as the Bond ...
... albedo . In this way systematic errors from many diverse sources are mitigated , but other errors are introduced . For example , error from the visible phase integral q for 4 Vesta is introduced if the result is interpreted as the Bond ...
Seite 49
... albedo to Phobos . Infrared observations of Phobos are extremely important . This control point will help to remove distortion in the radius and albedo scales due to differences in surface morphology between large and small asteroids ...
... albedo to Phobos . Infrared observations of Phobos are extremely important . This control point will help to remove distortion in the radius and albedo scales due to differences in surface morphology between large and small asteroids ...
Seite 111
... albedo is 0.40 . This high value is compatible with frost deposits but excludes aggregated cosmic - dust coatings ... albedo of 0.13 is similar to the case for the Moon and Mercury . For Pallas , some inconsistencies remain between ...
... albedo is 0.40 . This high value is compatible with frost deposits but excludes aggregated cosmic - dust coatings ... albedo of 0.13 is similar to the case for the Moon and Mercury . For Pallas , some inconsistencies remain between ...
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