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Features of motion of macroscopic body in gravitational field in a space with noncommutativity of coordinates and noncommutativity of momenta are considered in general case when coordinates and momenta of different particles satisfy…

广义相对论与量子宇宙学 · 物理学 2018-10-17 Kh. P. Gnatenko , V. M. Tkachuk

Changes that occur on our planet can be tracked back to one of two energy sources: the sun and the Earth's internal energy. The motion of tectonic plates, volcanism, mountain building and the reshaping of our planet's surface over geologic…

地球与行星天体物理 · 物理学 2018-01-30 Johnny Seales , Adrian Lenardic

Lunar Laser Ranging (LLR) measurements are crucial for advanced exploration of the evolutionary history of the lunar orbit, the laws of fundamental gravitational physics, selenophysics and geophysics as well as for future human missions to…

广义相对论与量子宇宙学 · 物理学 2009-02-23 Sergei Kopeikin

Satellite formation is a natural by-product of planet formation. With the discovery of nu- merous extrasolar planets, it is likely that moons of extrasolar planets (exomoons) will soon be discovered. Some of the most promising techniques…

地球与行星天体物理 · 物理学 2017-01-10 Amy C. Barr

Earth has had oceans for nearly four billion years and Mars had lakes and rivers 3.5-3.8 billion years ago. However, it is still unknown whether water has ever condensed on the surface of Venus because the planet - now completely dry - has…

地球与行星天体物理 · 物理学 2021-10-19 Martin Turbet , Emeline Bolmont , Guillaume Chaverot , David Ehrenreich , Jeremy Leconte , Emmanuel Marcq

Rotation is a prominent feature of the Sun, and it plays a crucial role in the generation and dynamic evolution of solar magnetic fields. The daily composite time series of Ca II K plage areas from 1907 February 1 to 2023 December 31 is…

太阳与恒星天体物理 · 物理学 2025-12-18 N. B. Xiang , X. H. Zhao , L. H. Deng , F. Y. Li , M. Wan , S. Y. Qi

The past decade has seen major progress in our understanding of terrestrial planet formation. Yet key questions remain. In this review we first address the growth of 100 km-scale planetesimals as a consequence of dust coagulation and…

地球与行星天体物理 · 物理学 2018-12-05 Andre Izidoro , Sean N. Raymond

Migration of bodies under the gravitational influence of almost formed planets was studied, and probabilities of their collisions with the Earth and other terrestrial planets were calculated. Based on the probabilities, several conclusions…

地球与行星天体物理 · 物理学 2026-01-12 S. I. Ipatov

This article discusses the limits of the Anthropogenic Global Warming Theory advocated by the Intergovernmental Panel on Climate Change. A phenomenological theory of climate change based on the physical properties of the data themselves is…

地球物理 · 物理学 2010-05-31 Nicola Scafetta

We investigate the obliquity and spin period of Earth-Moon like systems after 4.5 Gyr of tidal evolution with various satellite masses and initial planetary obliquity and discuss their relations to the habitability of the planet. We find…

地球与行星天体物理 · 物理学 2015-06-11 R. Brasser , S. Ida , E. Kokubo

Seismic and geodynamic studies indicate that the boundary between the Earth's liquid outer core and solid mantle is not spherical, but is likely characterized by topography in the form of inverted mountains and valleys that have typical…

地球物理 · 物理学 2025-06-10 Tobias G. Oliver , Eric G. Blackman , John A. Tarduno , Michael A. Calkins

I derived an equation to describe the dependence of Moon orbit radius around the Earth. I obtained the radius changes with time according to a scaling equation, Moon orbit radius is proportional to power 2/5 of the Moon age. Using the…

科普物理 · 物理学 2018-02-09 Mikrajuddin Abdullah

In this brief report we discuss how continuous changes on the physical parameters that determine the weather conditions may lead to long term climate variability. This variability of the weather patterns are a response to continuous random…

地球与行星天体物理 · 物理学 2022-09-21 Orfeu Bertolami

Given the inexorable increase in the Sun's luminosity, Earth will exit the habitable zone in ~1 Gyr. There is a negligible chance that Earth's orbit will change during that time through internal Solar System dynamics. However, there is a…

地球与行星天体物理 · 物理学 2023-11-22 Sean N. Raymond , Nathan A. Kaib , Franck Selsis , Herve Bouy

We devise and exploit a data-driven, semi-empirical framework of galaxy formation and evolution, coupling it to recipes for planet formation from stellar and planetary science, to compute the cosmic planet formation rate, and the properties…

星系天体物理 · 物理学 2024-08-19 Andrea Lapi , Lumen Boco , Francesca Perrotta , Marcella Massardi

This paper investigates the motion of a small particle moving near the triangular points of the Earth-Moon system. The dynamics are modeled in the Hill restricted 4-body problem (HR4BP), which includes the effect of the Earth and Moon as in…

动力系统 · 数学 2024-02-29 Luke T. Peterson , Gavin Brown , Àngel Jorba , Daniel Scheeres

The null findings of the terrestrially conducted Michelson-Morley type experiments have been influential to determining which physical theory best fits reality. Here, we propose the use of parallax and ranging techniques of distance…

综合物理 · 物理学 2009-09-29 Akinbo Ojo

According to the generally accepted scenario, the last giant impact on the Earth formed the Moon and initiated the final phase of core formation by melting the Earth's mantle. A key goal of geochemistry is to date this event, but different…

地球与行星天体物理 · 物理学 2015-04-08 Seth A. Jacobson , Alessandro Morbidelli , Sean N. Raymond , David P. O'Brien , Kevin J. Walsh , David C. Rubie

The understanding of the solar magnetic coronal structure is tightly linked to the shape of open field regions, specifically coronal holes. A dynamically evolving coronal hole coincides with the local restructuring of open to closed…

Impacts that leave the Earth-Moon system with a large excess in angular momentum have recently been advocated as a means of generating a protolunar disc with a composition that is nearly identical to that of the Earth's mantle. We here…

地球与行星天体物理 · 物理学 2017-02-22 Julien Salmon , Robin M. Canup