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. |
Im Buch
Seite 181
These perturbations cause a bias in the eccentricities that has an approximately
sinusoidal dependence on the longitude of perihelion and an amplitude of 0.05.
This causes the average perihelion distance of 1.9 AU to have peak variations of
...
These perturbations cause a bias in the eccentricities that has an approximately
sinusoidal dependence on the longitude of perihelion and an amplitude of 0.05.
This causes the average perihelion distance of 1.9 AU to have peak variations of
...
Seite 198
This preference for mean anomalies near M = 0°, clearly borne out by the PLS
catalog, should be reflected in the orbital elements as a maximum occurrence of
the perihelion longitude m = \, or about 0° to 30°, and a minimum at m = A + 180°,
...
This preference for mean anomalies near M = 0°, clearly borne out by the PLS
catalog, should be reflected in the orbital elements as a maximum occurrence of
the perihelion longitude m = \, or about 0° to 30°, and a minimum at m = A + 180°,
...
Seite 209
(2) The PLS was taken in the direction of the perihelion of Jupiter's orbit. (3)
Asteroids are usually discovered near perihelion. In his figure 1, Kresák shows
that, indeed, there is a pronounced asymmetry in the distribution of perihelia for ...
(2) The PLS was taken in the direction of the perihelion of Jupiter's orbit. (3)
Asteroids are usually discovered near perihelion. In his figure 1, Kresák shows
that, indeed, there is a pronounced asymmetry in the distribution of perihelia for ...
Seite 351
—Distribution of the longitude of the perihelion in 647 stream orbits. (a) Number. (
b) Percentage. overall distribution (fig. 2(a)) is symmetric with respect to a
weighted mean longitude of perihelion m = 12°5, which agrees closely with the ...
—Distribution of the longitude of the perihelion in 647 stream orbits. (a) Number. (
b) Percentage. overall distribution (fig. 2(a)) is symmetric with respect to a
weighted mean longitude of perihelion m = 12°5, which agrees closely with the ...
Seite 416
The relative stability of their orbits, in particular the fact that the perihelion
distances cannot for at least a millennium have had significantly larger values
than now, means that these two comets have long been subject to strong solar
radiation, ...
The relative stability of their orbits, in particular the fact that the perihelion
distances cannot for at least a millennium have had significantly larger values
than now, means that these two comets have long been subject to strong solar
radiation, ...
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Andere Ausgaben - Alle anzeigen
Häufige Begriffe und Wortgruppen
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
Bibliografische Informationen
| Titel | Physical Studies of Minor Planets Ausgabe 12 von International Astronomical Union Colloquium Band 267 von NASA SP |
| Herausgeber | Tom Gehrels |
| Mitwirkende | International Astronomical Union, National Science Foundation (U.S.), United States. National Aeronautics and Space Administration, International Astronomical Union. Colloquium |
| Verlag | Scientific and Technical Information Office, National Aeronautics and Space Administration, 1972 |
| Original von | University of California |
| Digitalisiert | 30. Jan. 2009 |
| Länge | 687 Seiten |
| Zitat exportieren | BiBTeX EndNote RefMan |