TL;DR: An interpretative synthesis of current knowledge on the moon and the terrestrial planets is presented, emphasizing the impact of recent lunar research (using Apollo data and samples) on theories of planetary morphology and evolution.
Abstract: An interpretative synthesis of current knowledge on the moon and the terrestrial planets is presented, emphasizing the impact of recent lunar research (using Apollo data and samples) on theories of planetary morphology and evolution. Chapters are included on the exploration of the solar system; geology and stratigraphy; meteorite impacts, craters, and multiring basins; planetary surfaces; planetary crusts; basaltic volcanism; planetary interiors; the chemical composition of the planets; the origin and evolution of the moon and planets; and the significance of lunar and planetary exploration. Photographs, drawings, graphs, tables of quantitative data, and a glossary are provided.
TL;DR: In this article, the authors show that the empirical relationship between the interplanetary field strength and the frequency of the waves in the observer's rest frame, derived originally from ground-based pulsation studies, and later, in situ, is approximately true at all the planets.
Abstract: We can extend our understanding of collisionless shocks by comparing their behaviour in a variety of plasma conditions at several different planets. One property of such shocks is the occurrence of upstream magnetohydrodynamic waves associated with particle beams accelerated at these shocks, and flowing back towards the Sun1. We report here observations of one of these classes of wave at Mercury, Venus, Earth and Jupiter. First, we show that the empirical relationship between the interplanetary field strength and the frequency of the waves in the observer's rest frame, derived originally from ground-based pulsation studies, and later, in situ, is approximately true at all the planets. Second, the observed frequencies are consistent with resonance with beams of ions of essentially the same energy at each of the planets. This observation is consistent with Sonnerup's2 geometrical model of ion reflection at collisionless shocks. The universality of this ion acceleration mechanism in the Solar System suggests that like acceleration occurs in similar astrophysical systems outside our Solar System and thus may provide a source of acceleration for cosmic rays.
TL;DR: The study of planets as physical objects goes back to the early 17th century, when Galileo discovered Jupiter's four main satellites and initiated the observations that led to Huyghens' discovery of Saturn's rings.
Abstract: The study of planets as physical objects goes back to the early 17th century, when Galileo discovered Jupiter's four main satellites and initiated the observations that led to Huyghens' discovery of Saturn's rings. But systematic work in planetary science is a comparatively recent development which has accompanied the rise of modern geophysics and astrophysics.
TL;DR: In this paper, it was shown that the earth is not in chemical equilibrium, and that it still retains vestiges of its heterogeneous growth in spite of prolonged convection and volcanism, and enough information remains in meteorites to show that the solar nebula was chemically inhomogeneous and did not develop under physical and chemical equilibrium.
Abstract: It is pointed out that enough information remains in meteorites to show that the solar nebula was chemically inhomogeneous, and that it did not develop under physical and chemical equilibrium. It is found that the earth is not in chemical equilibrium, and that it still retains vestiges of its heterogeneous growth in spite of prolonged convection and volcanism. The present investigation has the aim to unify simple ideas into a comprehensive, complex scheme for heterogeneous growth of the planets and parent bodies of meteorites. A scheme is considered for the conversion of dust and gas in the solar nebula into the present population of bodies. Attention is given to possible processes for the growth and development of planetesimals from dust via clouds, the major episodes in the development of the solar system, the relation of meteorites to a solar nebula with monotonic variation of temperature and oxidation state, the significance of meteorite properties, the composition of the inner planets, and the development of the earth.
TL;DR: In this paper, the Pioneer Vernus Orbiter plasma analyzer was used during passages through the Venus solar wind wake in June 1979, detecting frequent, episodic disappearances of the plasma.
Abstract: Observations by the Pioneer Vernus Orbiter plasma analyzer during passages through the Venus solar wind wake in June 1979 are reported. The spacecraft traveled 8-12 Venus radii behind the planet from the sun, detecting frequent, episodic disappearances of the plasma. The disappearance occurred inside the magnetotail, indicating a tattered, filamentary extension of the solar wind cavity. Positive oxygen ions were observed inside and outside of the magnetotail on some days, and were absent on others. The data indicate that the cavity contracts during high solar wind dynamic pressure, although the presence of 0(+) ions is not correlated well with the solar wind dynamic pressure. The most intense bursts originated from a flux of 10 million ions/sq cm per sec, with an 0(+) kinetic energy estimated to be 100,000-1,000,000 K.
TL;DR: A summary of all the telescopic observations of the clouds in Saturn's atmosphere made prior to the Voyager encounters with the planet can be found in this article, where a possible subatmospheric origin for the GWS is proposed, in which it is due to a temporary and local anisotropy in the internal heat source (a hot spot in the deeper atmosphere).
TL;DR: In this article, the authors studied the factors that affect the linear stability of a periodic planetary orbit in the plane and proved that planetary systems with two planets describing nearly circular orbits in the same direction are linearly stable and no perturbation exists which destroys the stability unless a resonance of the form 1/3, 3/5, 5/7,... among the orbits of the planets occurs.
Abstract: The factors which affect the linear stability of a periodic planetary orbit in the plane are studied. It is proved that planetary systems with two planets describing nearly circular orbits in the same direction are linearly stable and no perturbation exists which destroys the stability, unless a resonance of the form 1/3, 3/5, 5/7, ... among the orbits of the planets occurs. This latter resonant case is always unstable. Retrograde motion is always linearly stable. Planetary systems with three or more planets in nearly circular orbits in the same direction are proved to be unstable, in the sense that a Hamiltonian perturbation always exists which destroys the stability. The generation of instability in the case of three or more planets is not only due to the existence of resonances, as in the case of two planets, but also to the nonexistence of integrals of motion, apart from the energy and angular momentum integrals. It is also proved that planetary systems with nearly elliptic orbits of the planets are unstable.
TL;DR: In this article, the authors propose that polar wandering, induced by the intrinsic response of the viscoelastic planet to such cryospheric forcings, may be the underlying cause for the termination of the present ice age epoch.
Abstract: Recent geological evidence1,2 suggests that several degrees of true polar wandering have occurred since the mid-Pliocene. This rotational instability is supported by dynamical calculations3 of the spin axis of a layered viscoelastic Earth, which has been subjected to the periodic forcings characteristic of the late Cenozoic ice age. We propose here that polar wandering, induced by the intrinsic response of the viscoelastic planet to such cryospheric forcings, may be the underlying cause for the termination of the present ice age epoch.
TL;DR: In this paper, the authors compared Triton and Pluto in terms of their similar brightness and current distance of 30 AU from the sun, and showed that both are high albedo objects.
Abstract: The Neptune satellite Triton and the planet Pluto, whose diameter and albedo must be estimated by indirect methods, invite comparative study because of their similar brightness and current distance of 30 AU from the sun. IR spectroscopy has detected methane on both objects. Upper limits are given for the thermal IR emission from these objects which allow the determination of significant upper diameter limits. It is also demonstrated that both are high albedo objects, excluding the possibility that Triton is the largest planetary satellite and consistent with the small Pluto dimensions deduced from other data
TL;DR: In this paper, the influence of resonance perturbations due to the gravitational field of an oblate planet on its satellite whose motion is commensurable with rotation of the planet has been investigated.
Abstract: The influence of resonance perturbations due to the gravitational field of an oblate planet on its satellite whose motion is commensurable with rotation of the planet has been investigated. It has been shown that in special case of the critical inclination or circular orbit the Lagrange equations can be integrated for all resonance terms simultaneously. The method is applied to the investigation of the motion of the 12-hour communication and navigation satellites of the ‘Molniya’ and ‘Navstar’ type. The computations has been performed by the use of four models of the geopotential.
TL;DR: In this article, radio maps with a resolution of 1.5 arcsec were made of Saturn at 1.3, 2, and 6 cm. The inclination of the ring plane was -5.4 deg.
TL;DR: In this article, the authors attempt to draw an integrated picture of the atmospheric evolutionary process being careful to define the outstanding problems, differentiate theory from fact, and to emphasize the strengths and weaknesses of a priori and a posteriori approaches to these problems.
TL;DR: In this article, the authors reviewed the observations and the probable natures of the five known satellites of Uranus, including Titania and Oberon, and estimated the properties of the satellites from their surface geometric albedos, assumed mean densities and dynamics yield radii in the range 160-520 km.
Abstract: Observations and the probable natures of the five known satellites of Uranus are reviewed. Photographic, photoelectric and CCD photometry of the satellites since 1961, although in agreement within experimental error, is not as mutually consistent as may be expected, and broadband JHK photometry falls in a portion of the J-H, H-K color diagram difficult to interpret. Spectrophotometry in the range 0.3-1.1 microns taken on two separate occasions is inconsistent, with only the relatively neutral reflectances of Titania and Oberon regarded as well established. Near-infrared spectrophotometry has revealed the presence of water ice or frost on the satellite surfaces, possibly in a very pure state, with spectra most similar to Ganymede. Estimations of the properties of the satellites from their surface geometric albedos, assumed mean densities and dynamics yield radii in the range 160-520 km, albedos on the order of 0.5 and densities of about 1.3 g/cu cm, similar to the icy Saturn satellites. The satellites are also believed to have formed after the event that caused the planet to tilt to its present obliquity.
TL;DR: In this paper, the effect of the oblateness of the Earth on the motion of the Moon and the indirect effect of planets was investigated. But the effect was not considered.
Abstract: Perturbations in the motion of the Moon are computed for the effect by the oblateness of the Earth and for the indirect effect of planets. Based on Delaunay's analytical solution of the main problem, the computations are performed by a method of Fourier series operation. The effect of the oblateness of the Earth is obtained to the second order, partly adopting an analytical evaluation. Both in longitude and latitude are found a few terms whose coefficient differs from the current lunar ephemeris based on Brown's theory by about 0″.01. While, concerning the indirect effect of planets, several periodic terms in the current ephemeris seem to have errors reaching 0″.05.
TL;DR: In this paper, the origin of the solar system is considered along with the formation of the planets, the evolution of the planet, the surfaces of solid planets, and the atmosphere of the Earth.
Abstract: The origin of the solar systems is considered along with the formation of the planets, the evolution of the planets, the surfaces of solid planets, and the atmosphere of the planets. A description is provided of the various planets of the solar system. It is pointed out that Mercury was little known until March 1974 when the Mariner 10 spacecraft made the first of its three flybys of that body. In the case of Venus, the Pioneer mission to Venus by NASA in 1978 provided a breakthrough concerning a knowledge of the solid body hidden beneath the clouds. The characteristics of the planet earth are discussed together with information about the moon. A shaded relief map of Mars illustrates the geographic features of this planet. The map was produced with the aid of Mariner 9 photographs. Maps of the Jovian system based on photographs provided by space missions are also presented, and the Saturnian system is discussed, taking into account major satellites and rings of Saturn.
TL;DR: In this paper, it was shown that two previously unidentified, yet conspicuous gaps in Saturn's rings lie at distances corresponding to 2/3 and 4/3 of the planet's rotation period, and that these gaps can be produced in a ring of large bodies or small uncharged particles by a nonaxisymmetric gravitational field.
Abstract: Evidence is presented that two previously unidentified, yet conspicuous gaps in Saturn's rings lie at distances corresponding to 2/3 and 4/3 of the planet's rotation period. Gaps such as these can be produced in a ring of large bodies or small uncharged particles by a nonaxisymmetric gravitational field (both of the above can be associated with the l = m = 3 harmonic), a fact that is relevant to models of planetary interiors.
TL;DR: In this paper, the origin of the solar system is considered along with the formation of the planets, the evolution of the planet, the surfaces of solid planets, and the atmosphere of the Earth.
Abstract: The origin of the solar systems is considered along with the formation of the planets, the evolution of the planets, the surfaces of solid planets, and the atmosphere of the planets. A description is provided of the various planets of the solar system. It is pointed out that Mercury was little known until March 1974 when the Mariner 10 spacecraft made the first of its three flybys of that body. In the case of Venus, the Pioneer mission to Venus by NASA in 1978 provided a breakthrough concerning a knowledge of the solid body hidden beneath the clouds. The characteristics of the planet earth are discussed together with information about the moon. A shaded relief map of Mars illustrates the geographic features of this planet. The map was produced with the aid of Mariner 9 photographs. Maps of the Jovian system based on photographs provided by space missions are also presented, and the Saturnian system is discussed, taking into account major satellites and rings of Saturn.
TL;DR: In this paper, a new solution for the planetary perturbations of the Moon is built in the frame of ELP 2000, using Bretagnon's planetary theories, and achieved at the first order.
Abstract: A new solution for the planetary perturbations of the Moon is being built in the frame of ELP 2000, using Bretagnon's planetary theories, and achieved at the first order. It contains the two actions commonly distinguished: direct and indirect. The internal precision of computation is 2×10−6 arcsec. First-order planetary perturbations, in the direct case (Venus & Mars), have been compared to Standaert's solution. The major discrepancy reaches 70 cm in the longitude of Venus. Perturbations of the second order with respect to planetary masses, have been undertaken and illustrations are given. Finally, new values for the perigee and node motions are proposed.
TL;DR: The regular satellites of Jupiter and Saturn are generally believed to have accreted within cooling circumplanetary nebulae as mentioned in this paper, where small silicate bodies are lost into the planet by gas drag before ice can condense.
Abstract: The regular satellites of Jupiter and Saturn are generally believed to have accreted within cooling circumplanetary nebulae. Small silicate bodies are lost into the planet by gas drag before ice can condense. Larger silicate protosatellites survive by exerting tidal torques on the gas, clearing low-density “tunnels” around their orbits. The nebula is thus divided into series of gas rings depleted in silicates. Cooling eventually allows ice condensation, yielding another generation of icy bodies. Collisional accretion of these objects accounts for stochastic density variations of Saturn’s inner satellites. High dynamic pressure may have prevented accretion in the inner part of the Jovian nebula; J5 may be an ablated remnant of a larger body.
TL;DR: An updated study of Uranus interior models using current information about the planet's gravity field and rotation rate is presented in this article, where the most plausible model, both from the point of view of recent data and cosmogony, has a central core of iron and magnesium silicates, an outer envelope of liquid water, methane, and ammonia, and a deep "atmosphere" of almost four earth masses of hydrogen, helium and methane.
Abstract: An updated study is presented of Uranus interior models using current information about the planet's gravity field and rotation rate The most plausible model, both from the point of view of recent data and cosmogony, has a central core of iron and magnesium silicates, an outer envelope of liquid water, methane, and ammonia, and a deep 'atmosphere' of almost four earth masses of hydrogen, helium, and methane The 'atmosphere' contains a gravitationally nonnegligible amount of methane - about 40% by mass All plausible models are most consistent with a rotation period of 15 to 16 hours
TL;DR: The mass loss from planetary protoatmospheres is in the order of 10 −2 -10 −4 parts of the planetary mass for the terrestrial planets and about 10 −7 −10 −8 parts for the giant planets as mentioned in this paper.