Physical Studies of Minor Planets, Ausgabe 267Tom Gehrels Scientific and Technical Information Office, National Aeronautics and Space Administration [available from National Technical Information Service, Springfield, Va.], 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."--p. viii. |
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Seite 16
The orbital elements just considered are those of the Earth-Moon barycenter,
while Earth itself moves about this barycenter in accordance with the Moon's
orbital revolutions around Earth. Consequently, the geocentric position of any
asteroid ...
The orbital elements just considered are those of the Earth-Moon barycenter,
while Earth itself moves about this barycenter in accordance with the Moon's
orbital revolutions around Earth. Consequently, the geocentric position of any
asteroid ...
Seite 88
The contrary claim by Widorn (1964) and others is largely based on a fortuitous
empirical relationship obtained by plotting 0 against p for the Moon and some of
the large planets. Jupiter and Venus are intrinsically bright (huge p) and have ...
The contrary claim by Widorn (1964) and others is largely based on a fortuitous
empirical relationship obtained by plotting 0 against p for the Moon and some of
the large planets. Jupiter and Venus are intrinsically bright (huge p) and have ...
Seite 477
The Eros Asteroids and the Early History of the Moon The asteroids may also
contribute in another respect to the clarification of the early history of the Moon.
Some of the Eros asteroids come very close to Earth with reasonably low
velocities.
The Eros Asteroids and the Early History of the Moon The asteroids may also
contribute in another respect to the clarification of the early history of the Moon.
Some of the Eros asteroids come very close to Earth with reasonably low
velocities.
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Inhalt
ASTROMETRIC OBSERVATIONS | 3 |
THE WORK AT THE MINOR PLANET CENTER | 9 |
HISTORICAL NOTES | 18 |
58 weitere Abschnitte werden nicht angezeigt.
Andere Ausgaben - Alle anzeigen
Häufige Begriffe und Wortgruppen
39 Laetitia accretion albedo amplitude Anders Apollo Apollo 11 Apollo asteroids approximately asteroid belt astrometry Astron Astrophys axis brightness Brouwer Ceres chondrites collisional color cometary comets corrections density determined diameter discussed distance Dohnanyi Dollfus dust Earth ecliptic effect equation Eros erosive families Figure flyby fragments function Gehrels Geophys Houten Icarus impact infrared interplanetary Jetstream Jupiter km/s Kuiper larger libration lightcurve longitude magnitude Mars mass distribution material measurements meteor meteorites meteoroid Minor Planets mission Moon motion NASA negative branch number of asteroids numbered asteroids objects Observatory observed obtained optical orbital elements Pallas parent bodies particles percent perihelion perturbations phase angle phase coefficient Photometric planetary planetoids plotted pole radar radius range relative rotation sample satellites scattering semimajor axis solar nebula solar system space spacecraft spectral reflectivity stars streams telescope Trojans variation velocity Vesta wavelength Zodiacal Light
Bibliografische Informationen
| Titel | Physical Studies of Minor Planets, Ausgabe 267 Band 267 von NASA SP Physical studies of minor planets |
| Herausgeber | Tom Gehrels |
| Mitwirkende Personen | International Astronomical Union. Colloquium |
| Verlag | Scientific and Technical Information Office, National Aeronautics and Space Administration [available from National Technical Information Service, Springfield, Va.], 1972 |
| Länge | 687 Seiten |
| Zitat exportieren | BiBTeX EndNote RefMan |