Encyclopedia of Physical Science and Technology, Volume 2Academic Press, 1992 - Physical sciences |
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Page 138
IV . Solar System Objects Although the known planets , moons , and other solar systems objects were first discovered and studied by the visible sunlight they reflect , the key to unlocking may secrets of the solar system lies in studies ...
IV . Solar System Objects Although the known planets , moons , and other solar systems objects were first discovered and studied by the visible sunlight they reflect , the key to unlocking may secrets of the solar system lies in studies ...
Page 139
... solar system ring structures may be a model for many astrophysi- cal processes . [ See PLANETARY SATELLITES , NATURAL . ] B. COMETS , SATELLITES , AND ASTEROIDS The chemical history of the solar system may be preserved in primitive ...
... solar system ring structures may be a model for many astrophysi- cal processes . [ See PLANETARY SATELLITES , NATURAL . ] B. COMETS , SATELLITES , AND ASTEROIDS The chemical history of the solar system may be preserved in primitive ...
Page 188
... solar system was formed 4.5 billion years ago , play a greater role in shap- ing their present appearance , and so the tiniest bodies in the solar system are the most useful cosmic fossils . The number of objects in the solar system ...
... solar system was formed 4.5 billion years ago , play a greater role in shap- ing their present appearance , and so the tiniest bodies in the solar system are the most useful cosmic fossils . The number of objects in the solar system ...
Contents
Guide to Using the Encyclopedia ix Atomic Physics | 339 |
Approximations and Expansions 1 Atomic Spectrometry | 357 |
Archaeological Geology 31 Atomic Spectroscopy | 381 |
Copyright | |
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absorption acid aldoses angular momentum approximation asbestos atmosphere atoms auroral BASIC battery black hole Boolean algebra carbon fibers catalyst cell chemical chrysotile clouds collision complex components concentration convection cross section curve density developed disaccharide disk distribution dust electron elements emission emitted energy engine equations example expert system flux function galaxies heat hydrogen hydroxyl groups infrared input interaction interstellar interstellar medium ionization ions mass material measurements mechanism ment metal molecular molecules monosaccharides neutron stars nucleophile observed oligosaccharides operator orbital oxidation oxygen parameter particles photons plume problem radiation reaction reactor region result saccharide solar solution space spectral spectroscopy spectrum speed spline stable stars stellar structure surface techniques telescope temperature Theorem thermal tion tive turbulence ture typical variable velocity vertical wave wavelength weight white dwarf wind