Physical Studies of Minor PlanetsTom Gehrels Scientific 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 80
Tom Gehrels. understanding the physical implications of this quantity (which I will
denote by 3) can be divided into two parts: (1) To adequately describe the
scattering properties of an individual small element of the surface of a typical
asteroid ...
Tom Gehrels. understanding the physical implications of this quantity (which I will
denote by 3) can be divided into two parts: (1) To adequately describe the
scattering properties of an individual small element of the surface of a typical
asteroid ...
Seite 83
THE EFFECTS OF LARGE-SCALE ROUGHNESS: MACROSCOPIC
SHADOWING Unfortunately, the general problem of shadowing on a randomly
rough two-dimensional surface is extremely complicated. Ideally, one wishes to
know for each ...
THE EFFECTS OF LARGE-SCALE ROUGHNESS: MACROSCOPIC
SHADOWING Unfortunately, the general problem of shadowing on a randomly
rough two-dimensional surface is extremely complicated. Ideally, one wishes to
know for each ...
Seite 86
mag/deg, Hence, because over the same interval of phase angles, slab = 0.026
mag/deg for the surface of figure 1, 3 = 0.032 mag/deg for Q = 0 in figure 3. For a
scattering law of type (1), the geometric albedo p of the model planet is ...
mag/deg, Hence, because over the same interval of phase angles, slab = 0.026
mag/deg for the surface of figure 1, 3 = 0.032 mag/deg for Q = 0 in figure 3. For a
scattering law of type (1), the geometric albedo p of the model planet is ...
Seite 88
Mercury and the Moon are intrinsically dark (low p) and have rough dark surfaces
(high 6). Thus one can arrive at the unfounded conclusion that 3 must always be
inversely correlated with p, which in the case of dark surfaces certainly need ...
Mercury and the Moon are intrinsically dark (low p) and have rough dark surfaces
(high 6). Thus one can arrive at the unfounded conclusion that 3 must always be
inversely correlated with p, which in the case of dark surfaces certainly need ...
Seite 95
Laboratory simulations had already proved that the Moon's surface behaves like
a powder of pulverized basalts; the recent confirmation by direct exploration is
proving the significance of the method for remote determination of the surface ...
Laboratory simulations had already proved that the Moon's surface behaves like
a powder of pulverized basalts; the recent confirmation by direct exploration is
proving the significance of the method for remote determination of the surface ...
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Inhalt
| 3 | |
| 9 | |
| 25 | |
| 33 | |
| 41 | |
| 51 | |
| 67 | |
| 79 | |
| 353 | |
| 363 | |
| 377 | |
| 389 | |
| 395 | |
| 407 | |
| 413 | |
| 423 | |
| 91 | |
| 117 | |
| 133 | |
| 141 | |
| 147 | |
| 155 | |
| 165 | |
| 173 | |
| 183 | |
| 197 | |
| 211 | |
| 225 | |
| 239 | |
| 247 | |
| 257 | |
| 263 | |
| 297 | |
| 305 | |
| 315 | |
| 319 | |
| 327 | |
| 337 | |
| 429 | |
| 447 | |
| 461 | |
| 473 | |
| 479 | |
| 489 | |
| 503 | |
| 513 | |
| 527 | |
| 539 | |
| 561 | |
| 567 | |
| 577 | |
| 585 | |
| 595 | |
| 607 | |
| 623 | |
| 633 | |
| 639 | |
| 649 | |
| 661 | |
Andere Ausgaben - Alle anzeigen
Häufige Begriffe und Wortgruppen
albedo angle Apollo appears approach approximately assumed asteroid belt asteroids Astron bodies brightness calculated Ceres chondrites close collisions cometary comets compared complete considered constant corrections curve density depends determined diameter direction discussed distance distribution dust Earth effect electric elements equation Eros estimate families field Figure fragments function Gehrels given Icarus impact important included increase indicate interplanetary Jupiter known larger less light lightcurve limit lunar magnitude Mars mass material mean measurements meteorites minor planets mission Moon motion NASA objects observed obtained opposition orbits origin particles percent period phase photometry polarization position possible present probably problem properties radius range REFERENCES reflectivity relation relative rotation sample scattering selection shown similar smaller solar solar system space spacecraft stream suggested surface velocity Vesta
Bibliografische Informationen
| Titel | Physical Studies of Minor Planets Ausgabe 12 von International Astronomical Union Colloquium Band 267 von NASA SP |
| Herausgeber | Tom Gehrels |
| Mitwirkende | International Astronomical Union, National Science Foundation (U.S.), United States. National Aeronautics and Space Administration, International Astronomical Union. Colloquium |
| Verlag | Scientific and Technical Information Office, National Aeronautics and Space Administration, 1972 |
| Original von | University of California |
| Digitalisiert | 30. Jan. 2009 |
| Länge | 687 Seiten |
| Zitat exportieren | BiBTeX EndNote RefMan |