Physical Studies of Minor PlanetsTom Gehrels Scientific 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 93
It has been suggested (Gehrels and Teska, 1963) that simultaneous polarization
and brightness measurements can be used to decide conclusively to what extent
the short-period brightness fluctuations of asteroids are due to changes in ...
It has been suggested (Gehrels and Teska, 1963) that simultaneous polarization
and brightness measurements can be used to decide conclusively to what extent
the short-period brightness fluctuations of asteroids are due to changes in ...
Seite 95
PHYSICAL STUDIES OF ASTEROIDS BY POLARIZATION OF THE LIGHT
AUDOU//V DOLLFUS Observatoire de Paris Curves of polarization are available
at present for asteroids Vesta, Ceres, Pallas, Iris, Flora, and Icarus. These curves
are ...
PHYSICAL STUDIES OF ASTEROIDS BY POLARIZATION OF THE LIGHT
AUDOU//V DOLLFUS Observatoire de Paris Curves of polarization are available
at present for asteroids Vesta, Ceres, Pallas, Iris, Flora, and Icarus. These curves
are ...
Seite 96
POLARIZATION MEASUREMENTS AVAILABLE ON ASTEROIDS The first curves
of polarization on asteroids were derived in France by B. Lyot (1934). He used a
photographic polarimeter attached to the 100 cm reflector of Meudon ...
POLARIZATION MEASUREMENTS AVAILABLE ON ASTEROIDS The first curves
of polarization on asteroids were derived in France by B. Lyot (1934). He used a
photographic polarimeter attached to the 100 cm reflector of Meudon ...
Seite 104
LABORATORY POLARIZATION STUDIES RELEVANT TO ASTEROID
PROBLEMS For the purpose of interpreting the asteroid's polarization curves, we
are developing, at Meudon Observatory, a program of laboratory measurements
on ...
LABORATORY POLARIZATION STUDIES RELEVANT TO ASTEROID
PROBLEMS For the purpose of interpreting the asteroid's polarization curves, we
are developing, at Meudon Observatory, a program of laboratory measurements
on ...
Seite 380
Ingham and Jameson (1968) and Jameson (1970) observed the brightness and
polarization at 510 nm in regions away from the ecliptic. Model calculations
indicate that the polarization is a more sensitive discriminant than the intensity in
...
Ingham and Jameson (1968) and Jameson (1970) observed the brightness and
polarization at 510 nm in regions away from the ecliptic. Model calculations
indicate that the polarization is a more sensitive discriminant than the intensity in
...
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albedo angle Apollo appears approach approximately assumed asteroid belt asteroids Astron bodies brightness calculated Ceres chondrites close collisions cometary comets compared complete considered constant corrections curve density depends determined diameter direction discussed distance distribution dust Earth effect electric elements equation Eros estimate families field Figure fragments function Gehrels given Icarus impact important included increase indicate interplanetary Jupiter known larger less light lightcurve limit lunar magnitude Mars mass material mean measurements meteorites minor planets mission Moon motion NASA objects observed obtained opposition orbits origin particles percent period phase photometry polarization position possible present probably problem properties radius range REFERENCES reflectivity relation relative rotation sample scattering selection shown similar smaller solar solar system space spacecraft stream suggested surface velocity Vesta