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 17
... observed motion of an asteroid such as Eros or Amor . This approach is known as the " dynamical method " for determining and the astronomical unit from asteroid observations because it is actually a determination of m + ‹ . Because μ ...
... observed motion of an asteroid such as Eros or Amor . This approach is known as the " dynamical method " for determining and the astronomical unit from asteroid observations because it is actually a determination of m + ‹ . Because μ ...
Seite 45
... observations were made from July 21 , 1969 , to July 27 , 1970 , using the Hale Observatories ' 1.52 m telescope at Mt. Wilson . A total of 26 objects was observed : 1 Ceres , 2 Pallas , 3 Juno , 4 Vesta , 5 Astraea , 6 Hebe , 7 Iris ...
... observations were made from July 21 , 1969 , to July 27 , 1970 , using the Hale Observatories ' 1.52 m telescope at Mt. Wilson . A total of 26 objects was observed : 1 Ceres , 2 Pallas , 3 Juno , 4 Vesta , 5 Astraea , 6 Hebe , 7 Iris ...
Seite 117
... observations of asteroids were made as early as 1935 by Calder ( 1935 ) . Calder already observed comparison stars , chosen for their proximity to the asteroid and for similarity in color and magnitude . The comparison star observations ...
... observations of asteroids were made as early as 1935 by Calder ( 1935 ) . Calder already observed comparison stars , chosen for their proximity to the asteroid and for similarity in color and magnitude . The comparison star observations ...
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