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 86
... wavelength , unless Þ ( a ) has a wavelength dependence . But because it is assumed that the particles of the model surface are opaque and large compared to the wavelength , the wavelength dependence of ( a ) will be small . SOME ...
... wavelength , unless Þ ( a ) has a wavelength dependence . But because it is assumed that the particles of the model surface are opaque and large compared to the wavelength , the wavelength dependence of ( a ) will be small . SOME ...
Seite 88
... wavelength in the UBV region of the spectrum , this slight decrease in ẞ with increasing wavelength may perhaps be attributed to the increased importance of the small , multiply scattered component at long wavelengths , as suggested ...
... wavelength in the UBV region of the spectrum , this slight decrease in ẞ with increasing wavelength may perhaps be attributed to the increased importance of the small , multiply scattered component at long wavelengths , as suggested ...
Seite 383
... wavelength bands can provide direct information on the effects of Earth's atmosphere . Such observations should be ... wavelength will not fit at another wavelength . In PHYSICAL PROPERTIES OF THE INTERPLANETARY DUST 383.
... wavelength bands can provide direct information on the effects of Earth's atmosphere . Such observations should be ... wavelength will not fit at another wavelength . In PHYSICAL PROPERTIES OF THE INTERPLANETARY DUST 383.
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 craters curve density determined diameter discussed distance Dohnanyi Dollfus Earth ecliptic effect Ephemeris 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