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Planetary orbit

The masses of the planets so far discovered vary between about 0.02 and 18 Jupiter masses. There are also very large variations in the values of the semi-major axis of the planetary orbits. If the first two methods for the discovery of extrasolar planets are compared (Doppler and transit methods), Doyle et al. (2000) point out the following facts around 40,000 photons are required to determine the transit of an extrasolar planet across the star HD 209548 using a photometer. But detection of the same system using variations in radial velocity requires 10 million photons. [Pg.296]

More complicated numerical methods, such as the Runge-Kutta method, yield more accurate solutions, and for precisely formulated problems requiring accurate solutions these methods are helpful. Examples of such problems are the evolution of planetary orbits or the propagation of seismic waves. But the more accurate numerical methods are much harder to understand and to implement than is the reverse Euler method. In the following chapters, therefore, I shall show the wide range of interesting environmental simulations that are possible with simple numerical methods. [Pg.15]

The bottom ash was treated with 0.4 moles of PO (from industrial-grade phosphoric acid) per kg dry weight of ash. The scrubber residue was treated with 1.2 moles of PO per kg of scrubber residue. The vitrification dust was treated with 0.4 moles of PO3- per kg of residue. Process mixing in all cases used an LS of 0.4. Mixing was done for 10 minutes in a Hobart mixer using a tined paddle (108 rpm) with a planetary orbit (48 rpm). [Pg.455]

Newtons law of gravitation played that ideal role for planetary astronomy during the eighteenth century. Once a planetary orbit had been calculated, based on the ideal relation between a planet and the sun, any deviation from the calculated path was immediately seen as a challenge to the law and became a focus of concerned attention to seek an explanation, usually found in the gravitational effects of other planets. The most spectacular example of this was the discovery of the planet Neptune from the deviations in the orbit of Uranus. [Pg.20]

With the modern concept of a hydrogen atom we do not visualize the orbital electron traversing a simple planetary orbit. Rather, we speak of an atomic orbital, in which there is only a probability of finding the electron in a particular volume a given distance and direction from the nucleus. The boundaries of such an orbital are not distinct because there always remains a finite, even if small, probability of finding the electron relatively far from the nucleus. [Pg.151]

The idea that laws of nature should satisfy a principle of simplicity goes back at least to the Greek philosophers [436], The anthropomorphic concept that the engineering skill of a supreme creator should result in rules of least effort or of most efficient use of resources leads directly to principles characterized by mathematical extrema. For example, Aristotle (De Caelo) concluded that planetary orbits must be perfect circles, because geometrical perfection is embodied in these curves ... of lines that return upon themselves the line which bounds the circle is the shortest. That movement is swiftest which follows the shortest line . Hero of Alexandria ( Catoptrics) proved perhaps the first scientific minimum principle, showing that the path of a reflected ray of light is shortest if the angles of incidence and reflection are equal. [Pg.3]

The superiority of circular planetary orbits became almost a religious dogma in the Christian era, intimately tied to the idea of the perfection of God and of His creations. It was replaced by modem celestial mechanics only after centuries in which the concept of esthetic perfection of the universe was gradually superseded by a concept of esthetic perfection of a mathematical theory that could account for the... [Pg.3]

Figure 8.2 Logarithmic spiral with superimposed mean planetary orbits. The circles in blue define the orbits of inner planets on a larger (self-similarj scale. The divergence angle of 108° causes those planets at angles of 5 x 108° apart to lie on opposite sides of the spiral origin. These pairs are Neptune-Mars, Uranus-Earth, Saturn-Venus and Jupiter-Mercury. The hypothetical antipode of the asteroid belt, a second, unobserved group of unagglomerated fragments, has been swallowed up by the sun... Figure 8.2 Logarithmic spiral with superimposed mean planetary orbits. The circles in blue define the orbits of inner planets on a larger (self-similarj scale. The divergence angle of 108° causes those planets at angles of 5 x 108° apart to lie on opposite sides of the spiral origin. These pairs are Neptune-Mars, Uranus-Earth, Saturn-Venus and Jupiter-Mercury. The hypothetical antipode of the asteroid belt, a second, unobserved group of unagglomerated fragments, has been swallowed up by the sun...
Metal and metal oxide catalysts with this capability were reported in the 1980s. Several of these metals occur in widely distributed petroleum samples and are among the above listed as constituents of primordial Earth planetary orbit dust. In the metallic and compounded state some have the ability to catalyze hydrogenation of carbon to kerogen like high viscosity hydrocarbons. Kerogen, a heavier petroleumlike hydrocarbon mixture occurs in tar sands and porous shales (oil shale). Thus the question of conceivable prehistoric or more recent petroleum from methane generation must be considered. [Pg.931]

The first method, developed for the calculation of planetary orbits, has also found much application in the wave mechanics of the atom. The second method is sometimes physically less clear but in most cases this method leads with less calculation more rapidly and more accurately to the end in view than the former method. In the wave-mechanical treatment of molecules the variational method is indeed mainly used. [Pg.132]

Gerald D. Quinlan and Scott Tremaine, Symmetric Multistep Methods for the Numerical Integration of Planetary Orbits, The Astronomical Journal, 1990, 100(5), 1694-1700. [Pg.481]

General relativity and planetary orbits) The relativistic equation for the orbit of a planet around the sun is... [Pg.186]

What was it that determined that the planetary orbits would be spaced as they are ... [Pg.122]

The relative distances from the sun of the various planetary orbits are illustrated here, including the orbit of the asteroids (dotted line) between Mars and Jupiter. [Pg.209]

Typically, the two phases of the solvent system are mutually saturated by shaking in a separatory funnel. The chosen stationaiy phase is loaded into the coil in the absence of rotation. The sample is then injected as a solution in either one, or a mixture of both phases. Rotation is then started and the mobile phase is pumped into the coil. Some stationary phase will be displaced and the sample constituents will be separated and eluted in the order of their partition coefficients. Mass transfer of the solute is promoted by a train of dynamic mixing zones, generated by the planetary motion of the coil as it rotates on its own axis while traversing a planetary orbit."... [Pg.118]

Kepler s laws - The three laws of planetary motion, which established the elliptical shape of planetary orbits and the relation between orbital dimensions and the period of rotation. [Pg.107]


See other pages where Planetary orbit is mentioned: [Pg.230]    [Pg.341]    [Pg.82]    [Pg.195]    [Pg.202]    [Pg.203]    [Pg.6]    [Pg.69]    [Pg.70]    [Pg.101]    [Pg.193]    [Pg.222]    [Pg.25]    [Pg.123]    [Pg.931]    [Pg.931]    [Pg.932]    [Pg.308]    [Pg.332]    [Pg.40]    [Pg.202]    [Pg.187]    [Pg.530]    [Pg.49]    [Pg.20]    [Pg.452]    [Pg.257]    [Pg.195]    [Pg.284]    [Pg.644]    [Pg.225]   
See also in sourсe #XX -- [ Pg.15 , Pg.120 , Pg.149 ]

See also in sourсe #XX -- [ Pg.86 , Pg.187 ]




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Planetary

Planetary orbital changes

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