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 16
... 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 is also a function of the so - called constant of ...
... 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 is also a function of the so - called constant of ...
Seite 88
... Moon and some of the large planets . Jupiter and Venus are intrinsically bright ( large p ) and have cloud decks in which multiple scattering is important ( low ẞ ) . Mercury and the Moon are intrinsically dark ( low p ) and have rough ...
... Moon and some of the large planets . Jupiter and Venus are intrinsically bright ( large p ) and have cloud decks in which multiple scattering is important ( low ẞ ) . Mercury and the Moon are intrinsically dark ( low p ) and have rough ...
Seite 364
... Moon libration clouds , m1 is Earth , m2 is the Moon , and the dust clouds are near L4 and L5 . See van de Kamp ( 1964 ) or Szebehely ( 1967 ) for further discussion . counterglow was due to a collection of dust around the L3 libration ...
... Moon libration clouds , m1 is Earth , m2 is the Moon , and the dust clouds are near L4 and L5 . See van de Kamp ( 1964 ) or Szebehely ( 1967 ) for further discussion . counterglow was due to a collection of dust around the L3 libration ...
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