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Models of the Sun's long-term evolution suggest that its luminosity was substantially reduced 2-4 billion years ago, which is inconsistent with substantial evidence for warm and wet conditions in the geological records of both ancient Earth…

地球与行星天体物理 · 物理学 2018-12-19 Christopher Spalding , Woodward W. Fischer , Gregory Laughlin

Solar quasi-biennial oscillations with period range 0.6 to 4 years, are prominent in records of solar activity. Here we show that the 1.6 year quasi-biennial oscillation in solar activity has the exceptional feature of phase inversion…

太阳与恒星天体物理 · 物理学 2021-10-27 Ian R. Edmonds

In future geocentric space-based gravitational-wave observatory missions, eclipses due to passing through the Moon's and Earth's shadows can negatively impact the sciencecraft's thermal stability and steady power supply. The occurrence…

广义相对论与量子宇宙学 · 物理学 2021-02-17 Bobing Ye , Xuefeng Zhang , Yanwei Ding , Yunhe Meng

Planetary systems with multiple transiting planets are beneficial for understanding planet occurrence rates and system architectures. Although we have yet to find a solar system analogue, future surveys may detect multiple terrestrial…

地球与行星天体物理 · 物理学 2026-01-12 Bethlee Lindor , Eric Agol

The possibility to detect circumbinary planets and to study stellar magnetic fields through eclipsing time variations (ETVs) in binary stars has sparked an increase of interest in this area of research. We revisit the connection between…

太阳与恒星天体物理 · 物理学 2022-07-20 Felipe H. Navarrete , Petri J. Käpylä , Dominik R. G. Schleicher , Carolina A. Ortiz , Robi Banerjee

We report a calculation of time-dependent quasi-geostrophic core flows for 1940-2010. Inverting recursively for an ensemble of solutions, we evaluate the main source of uncertainties, namely the model errors arising from interactions…

地球物理 · 物理学 2016-03-01 N Gillet , D Jault , C. C. Finlay

Planets with masses between 0.1 - 10 M_earth are believed to host dense atmospheres. These atmospheres can play an important role on the planet's spin evolution, since thermal atmospheric tides, driven by the host star, may counterbalance…

地球与行星天体物理 · 物理学 2014-08-05 Diana Cunha , Alexandre C. M. Correia , Jacques Laskar

The Total Solar Irradiance varies over a solar cycle of 11 years and maybe over cycles with longer period. Is the solar diameter variable over time too? We introduce a new method to perform high resolution astrometry of the solar diameter…

太阳与恒星天体物理 · 物理学 2012-02-20 Andrea Raponi , Costantino Sigismondi , Konrad Guhl , Richard Nugent , Andreas Tegtmeier

Astronomical (or Milankovi\'c) forcing of the Earth system is key to understanding rhythmic climate change on time scales >~ 10 kyr. Paleoceanographic and paleoclimatological applications concerned with past astronomical forcing rely on…

地球与行星天体物理 · 物理学 2024-05-03 Richard E. Zeebe , Margriet L. Lantink

The search of a rational explanation of eclipses pervades the beginnings of philosophical and scientific thought. Within this intellectual frame, the knowledge of the "saros cycle" (a cycle of 18 years, 10 or 11 days and 1/3 of a day that…

物理学史与哲学 · 物理学 2013-04-30 Roberto Casazza , Alejandro Gangui

Climate model evaluation plays a crucial role in ensuring the accuracy of climatological predictions. However, existing statistical evaluation methods often overlook time misalignment of events in a system's evolution, which can lead to a…

统计方法学 · 统计学 2025-04-29 Robert C. Garrett , Trevor Harris , Zhuo Wang , Bo Li

Earth-like planets in the habitable zone of low-mass stars undergo strong tidal effects that modify their spin states. These planets are expected to host dense atmospheres that can also play an important role in the spin evolution. On one…

地球与行星天体物理 · 物理学 2024-10-02 E. F. S. Valente , A. C. M. Correia , P. Auclair-Desrotour , M. Farhat , J. Laskar

The coupled evolution of the magnetic field and the flow at the Earth's core mantle boundary is modeled within the 1900.0-2014.0 time period. To constraint the dynamical behavior of the system with a core field model deriving from direct…

Context: The Solar System giant planets harbour a wide variety of moons. Moons around exoplanets are plausibly similarly abundant, even though most of them are likely too small to be easily detectable with modern instruments. Moons are…

地球与行星天体物理 · 物理学 2026-01-28 Yubo Su , Melaine Saillenfest

The equilibrium rotation of tidally evolved "Earth-like" extra-solar planets is often assumed to be synchronous with their orbital mean motion. The same assumption persisted for Mercury and Venus until radar observations revealed their true…

天体物理学 · 物理学 2008-08-08 Alexandre C. M. Correia , Benjamin Levrard , Jacques Laskar

In order to test planetary accretion and differentiation scenarios, we integrated a multistage core-mantle differentiation model with N-body accretion simulations. Impacts between embryos and planetesimals result in magma ocean formation…

Geological data show that, early in its history, the Earth had a large-scale magnetic field with an amplitude comparable to the one of the present geomagnetic field. However, its origin remains enigmatic and various mechanisms have been…

地球物理 · 物理学 2026-02-24 Jérémie Vidal , David Cébron

We report the empirical detection of a multi-planet quasi-commensurability in the Solar System and identify an anomalous exclusion that may bear on the dynamical history of Uranus. An exhaustive search identifies T* = 420,403 days (approx.…

地球与行星天体物理 · 物理学 2026-04-10 Carlos Baiget Orts

Aims. Particles ejected from the lunar surface via hypervelocity impacts form a torus between the Earth and the Moon. According to our previous study (Yang et al., A\&A, 659, A120), among them about $2.3\times10^{-4}\,\mathrm{kg/s}$…

地球与行星天体物理 · 物理学 2025-07-22 Kun Yang , Yu Jiang , Youpeng Liang , Xiaodong Liu