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Frontiers in Astronomy and Space Sciences, 2022 Orbital systems are often self-organized and/or characterized by harmonic relations. Inspired by music theory, we rewrite the Geddes and King-Hele (QJRAS, 24, 10–13, 1983) equations for mirror symmetries among the distances of the planets of the Solar ...
Michael J. Bank, Nicola Scafetta
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Wide angle search for extrasolar planets by the transit method [PDF]
, 2008 The transit method is considered to be one of the most promising for discovering extrasolar planets. However, the method requires photometric precision of better than ∼ 1%.
Alsubai, Khalid
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Vestnik Samarskogo Gosudarstvennogo Tehničeskogo Universiteta. Seriâ: Fiziko-Matematičeskie Nauki, 2011 Databases of major planets coordinates are created on the basis of the numerical theory of movement of planets DE405. Numerical integration of the motion equations of small bodies of Solar system is realized using the received databanks. Extra efficiency
Vladimir P Radchenko, Dmitriy A Zausaev
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Ice On Planets of the Solar System [PDF]
Journal of Glaciology, 1984 AbstractSeveral aspects of space glaciology are considered in the paper. Estimates of the water content of the Earth, Mars, and the Galilean moons of Jupiter are corrected. A considerable proportion of the total amount of water in the solar system is localized near Jupiter; part of this water is contained as ice in glaciations, glacial caps, and ice ...
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The Possibility of Mirror Planet as Planet Nine in the Solar System
Universe, 2022 A series of dynamical anomalies in the orbits of distant trans-Neptunian objects points to a new celestial body (usually named Planet Nine) in the solar system. In this draft, we point out that a mirror planet captured from the outer solar system or formed in the solar system is also a possible candidate.
Pei Wang +4 more
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The Solar System Beyond The Planets [PDF]
, 2006 The Kuiper belt contains a vast number of objects in a flattened, ring-like volume beyond the orbit of Neptune. These objects are collisionally processed relics from the accretion disk of the Sun and, as such, they can reveal much about early conditions in the Solar system.
Delsanti, Audrey, Jewitt, David
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On the interaction between embedded planets and the corotation region of protoplanetary discs [PDF]
, 2015 PhDDisc material in the corotation region librates with respect to low-mass planets on horseshoe trajectories. The exchange of angular momentum associated with this libration gives rise to the non-linear corotation torque (the horseshoe drag).
Fendyke, Stephen
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Giant planet formation in the Solar System
IcarusThe formation of gas giants has greatly influenced the structure of our solar system while their evolution has played a crucial role in shaping its history. Consequently, the growth of Jupiter has been studied quite extensively. However, little attention has been paid to Saturn and the other giants in the outer solar system.Here we explore, through 𝑁 ...
Anuja Raorane +5 more
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The Fundamental Connections between the Solar System and Exoplanetary Science [PDF]
, 2021 Over the past several decades, thousands of planets have been discovered outside our Solar System. These planets exhibit enormous diversity, and their large numbers provide a statistical opportunity to place our Solar System within the broader context of
Kane, Stephen R. +19 more
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Main Belt Comets and other “Interlopers” in the Solar System
Universe, 2022 According to traditional ideas about the formation of the Solar System starting from a protoplanetary disk of gas and dust, a well-defined distribution of planets and minor bodies is expected: (a) volatile-poor rocky bodies (terrestrial planets and ...
Vincenzo Orofino
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