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The zonal winds on the surfaces of giant planets vary with latitude. Jupiter and Saturn, for example, have several bands of alternating eastward (prograde) and westward (retrograde) jets relative to the angular velocity of their global…

天体物理学 · 物理学 2009-11-13 Gary A. Glatzmaier , Martha Evonuk , Tamara M. Rogers

Neutron stars (NSs) are compact objects that host the densest forms of matter in the observable universe, providing unique opportunities to study the behaviour of matter at extreme densities. While precision measurements of NS masses…

广义相对论与量子宇宙学 · 物理学 2025-12-18 Huanchen Hu , Paulo C. C. Freire

Recent measurements of Jupiter's gravitational moments by the Juno spacecraft and seismology of Saturn's rings suggest that the primordial composition gradients in the deep interior of these planets have persisted since their formation. One…

地球与行星天体物理 · 物理学 2023-11-08 J. R. Fuentes , Evan H. Anders , Andrew Cumming , Bradley W. Hindman

Restriction on the neutron-antineutron oscillation time in vacuum is obtained from latest SNO data on the deuteron stability, $\tau_D\,>\,3.01^.10^{31}$ years. Calculation performed within the quantum field theory based diagram technique…

高能物理 - 唯象学 · 物理学 2015-06-03 Vladimir Kopeliovich , Irina Potashnikova

The absence of plate tectonics and the young surface age (0.3-1 billion years) of Venus have led to diverse geodynamic models for Venus. The energetics of the Venusian interior drive these models; however, the lack of direct constraints on…

地球与行星天体物理 · 物理学 2025-07-14 Javier Ruiz , Alberto Jiménez-Díaz , Isabel Egea-González , Ignacio Romeo , Jon F. Kirby , Pascal Audet

Venus Express provided a long-term monitoring of Venus atmosphere. Several works focused on the dynamics of the upper cloud visible on the day-side in ultraviolet images sensitive to the 65-70 km altitude and in the lower cloud level (50 km…

地球与行星天体物理 · 物理学 2024-01-31 Ricardo Hueso , Javier Peralta , Itziar Garate-Lopez , Tatyana V. Bandos , Agustin Sanchez-Lavega

AIMS: An alternative to the traditional method for modeling kinematics of the Earth's rotation is proposed. The purpose of developing the new approach is to provide a self-consistent and simple description of the Earth's rotation in a way…

天体物理学 · 物理学 2009-11-11 L. Petrov

We have analyzed new and archival time series spectra taken six years apart during transits of the hot Jupiter WASP-33 b, and spectroscopically resolved the line profile perturbation caused by the Rossiter-McLaughlin effect. The motion of…

地球与行星天体物理 · 物理学 2015-09-29 Marshall C. Johnson , William D. Cochran , Andrew Collier Cameron , Daniel Bayliss

The relativistic perihelion precession due to the three-body interaction is derived. We consider a hierarchical coplanar three-body system, such as the Sun, Jupiter and Saturn, in which both the secondary object as the largest planet…

广义相对论与量子宇宙学 · 物理学 2012-03-26 Kei Yamada , Hideki Asada

An exact expression for the rate of dragging of inertial frames (Lense-Thirring (LT) precession) in a general stationary spacetime, is derived without invoking the weak field approximation. This expression, when used for the Kerr metric,…

广义相对论与量子宇宙学 · 物理学 2013-04-29 Chandrachur Chakraborty , Parthasarathi Majumdar

The recovery of cosmic ray protons of energy ~150-250 MeV/nuc in solar cycle #23 from 2004 to 2010 has been followed at the Earth using IMP, ACE and balloon data and also at V2 between 74-92 AU and at V1 beyond the heliospheric termination…

地球物理 · 物理学 2011-11-11 W. R. Webber , F. B. McDonald , P. R. Higbie , B. Heikkila

We have carried out a new photometric V,Rc study of 12 protoplanetary nebulae, objects in the short-lived transition between the AGB and PN phases of stellar evolution. These had been the subjects of an earlier study, using data from…

太阳与恒星天体物理 · 物理学 2022-11-09 Bruce J. Hrivnak , Wenxian Lu , William C. Bakke , Peyton J. Grimm

Neptune has brightened by more than 10% during the past several decades. We report on the analysis of published Johnson-Cousins B and V magnitudes dating back to 1954 along with new U, B, V, R, Rc, I and Ic photometry that we recorded…

地球与行星天体物理 · 物理学 2016-04-05 Richard W. Schmude , Ronald E. Baker , Jim Fox , Bruce A. Krobusek , Hristo Pavlov , Anthony Mallama

We investigate the evolution of rigidly and differentially rotating protoneutron stars (PNSs) during the first twenty seconds of their life. We solve the equations describing stationary axisymmetric configurations in general relativity…

天体物理学 · 物理学 2007-05-23 Loic Villain , Jose A. Pons , Pablo Cerda-Duran , Eric Gourgoulhon

Recent observations of FRB 20220529 reveal significant variation and a partial reversal in its rotation measure (RM), suggesting the presence of a dynamically evolving magnetized environment, which could be caused by the orbital motion of…

高能天体物理现象 · 物理学 2026-01-07 Ze-Xin Du , Yun-Wei Yu , Aming Chen , Chen-Hui Niu , Jia-Heng Zhang

We report the results of a long campaign of time-series photometry on the nova-like variable UX Ursae Majoris during 2015. It spanned 150 nights, with ~1800 hours of coverage on 121 separate nights. The star was in its normal `high state'…

Binary black-hole systems are expected to be important sources of gravitational waves for upcoming gravitational-wave detectors. If the spins are not colinear with each other or with the orbital angular momentum, these systems exhibit…

广义相对论与量子宇宙学 · 物理学 2016-08-07 Serguei Ossokine , Michael Boyle , Lawrence E. Kidder , Harald P. Pfeiffer , Mark A. Scheel , Béla Szilágyi

We fit an isothermal oscillatory density model of Neptune's protoplanetary disk to the surviving regular satellites and its innermost ring and we determine the radial scale length of the disk, the equation of state and the central density…

地球与行星天体物理 · 物理学 2019-03-05 Dimitris M. Christodoulou , Demosthenes Kazanas

Precision radial velocity (RV) measurements of the Sun-like dwarf 14 Herculis published by Naef et. al (2004), Butler et. al (2006) and Wittenmyer et al (2007) reveal a Jovian planet in a 1760 day orbit and a trend indicating the second…

天体物理学 · 物理学 2009-11-13 K. Gozdziewski , C. Migaszewski , M. Konacki

Sulfur dioxide is a radiatively and chemically important trace gas in the atmosphere of Venus and its abundance at the cloud-tops has been observed to vary on interannual to decadal timescales. This variability is thought to come from…

地球与行星天体物理 · 物理学 2020-11-02 Pushkar Kopparla , Ashwin Seshadri , Takeshi Imamura , Yeon Joo Lee