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 xix
... TROJAN ASTEROIDS There are also accumulations at 1 : 1 and these are referred to as the Trojans . Sixteen members of the Trojans are definitely known and many others are suspected . The large number of Trojans and their asteroidlike ...
... TROJAN ASTEROIDS There are also accumulations at 1 : 1 and these are referred to as the Trojans . Sixteen members of the Trojans are definitely known and many others are suspected . The large number of Trojans and their asteroidlike ...
Seite 173
... TROJANS These are asteroids moving near the lagrangian points L4 and L5 of the Sun - Jupiter system . There are 15 numbered Trojans , but at fainter magnitudes than the limit of the ephemeris they are very numerous ; it was shown that ...
... TROJANS These are asteroids moving near the lagrangian points L4 and L5 of the Sun - Jupiter system . There are 15 numbered Trojans , but at fainter magnitudes than the limit of the ephemeris they are very numerous ; it was shown that ...
Seite 185
... Trojan in the PLS is 6.5 . It follows that the Trojans contribute little to the linear part of the phase function , and heavily to the opposition effect . It is , therefore , surprising that most Trojans yielded negative residuals with ...
... Trojan in the PLS is 6.5 . It follows that the Trojans contribute little to the linear part of the phase function , and heavily to the opposition effect . It is , therefore , surprising that most Trojans yielded negative residuals with ...
Inhalt
ASTROMETRIC OBSERVATIONS | 3 |
THE WORK AT THE MINOR PLANET CENTER | 9 |
DIAMETER MEASUREMENTS OF ASTEROIDS | 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 curve density determined diameter discussed distance Dohnanyi Dollfus Earth ecliptic effect ephemerides equation Eros families Figure flyby fragments function Gehrels Geophys gravitational 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 meteoroids 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 PHYSICAL STUDIES planetary planetoids polarization pole propulsion radius range rotation sample satellites scattering semimajor axis solar nebula solar system space spacecraft stream STUDIES OF MINOR surface trajectory Trojans velocity Vesta wavelength Whipple Zodiacal Light