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Geologic Constraints on the Formation and Evolution of Saturn's Mid-Sized Moons. 土星中型卫星形成和演化的地质制约因素。
IF 9.1 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Pub Date : 2024-01-01 Epub Date: 2024-07-17 DOI: 10.1007/s11214-024-01084-z
Alyssa Rose Rhoden, Sierra N Ferguson, William Bottke, Julie C Castillo-Rogez, Emily Martin, Michael Bland, Michelle Kirchoff, Marco Zannoni, Nicolas Rambaux, Julien Salmon

Saturn's mid-sized icy moons have complex relationships with Saturn's interior, the rings, and with each other, which can be expressed in their shapes, interiors, and geology. Observations of their physical states can, thus, provide important constraints on the ages and formation mechanism(s) of the moons, which in turn informs our understanding of the formation and evolution of Saturn and its rings. Here, we describe the cratering records of the mid-sized moons and the value and limitations of their use for constraining the histories of the moons. We also discuss observational constraints on the interior structures of the moons and geologically-derived inferences on their thermal budgets through time. Overall, the geologic records of the moons (with the exception of Mimas) include evidence of epochs of high heat flows, short- and long-lived subsurface oceans, extensional tectonics, and considerable cratering. Curiously, Mimas presents no clear evidence of an ocean within its surface geology, but its rotation and orbit indicate a present-day ocean. While the moons need not be primordial to produce the observed levels of interior evolution and geologic activity, there is likely a minimum age associated with their development that has yet to be determined. Uncertainties in the populations impacting the moons makes it challenging to further constrain their formation timeframes using craters, whereas the characteristics of their cores and other geologic inferences of their thermal evolutions may help narrow down their potential histories. Disruptive collisions may have also played an important role in the formation and evolution of Saturn's mid-sized moons, and even the rings of Saturn, although more sophisticated modeling is needed to determine the collision conditions that produce rings and moons that fit the observational constraints. Overall, the existence and physical characteristics of Saturn's mid-sized moons provide critical benchmarks for the development of formation theories.

土星的中型冰卫星与土星内部、土星环以及它们之间有着复杂的关系,这种关系可以通过它们的形状、内部结构和地质学表现出来。因此,对其物理状态的观测可以为卫星的年龄和形成机制提供重要的制约因素,进而帮助我们了解土星及其星环的形成和演变过程。在此,我们将介绍中型卫星的陨石坑记录,以及这些记录在制约卫星历史方面的价值和局限性。我们还讨论了对这些卫星内部结构的观测约束,以及从地质学角度推断出的这些卫星在不同时期的热预算。总体而言,这些卫星(除米马斯卫星外)的地质记录包括高热流时代、短期和长期的地表下海洋、伸展构造和大量陨石坑的证据。奇怪的是,米马斯的表面地质中没有海洋的明显证据,但它的自转和轨道却表明有现今的海洋。虽然这些卫星不一定是原始的,就能产生观测到的内部演化和地质活动水平,但它们的发展可能有一个最低年龄,这个年龄还有待确定。由于撞击卫星的种群存在不确定性,因此利用陨石坑来进一步确定它们的形成时间具有挑战性,而卫星内核的特征以及对其热演化的其他地质推断可能有助于缩小其潜在历史的范围。破坏性碰撞也可能在土星中型卫星甚至土星环的形成和演化过程中发挥了重要作用,不过还需要更复杂的建模来确定产生符合观测约束条件的土星环和卫星的碰撞条件。总之,土星中型卫星的存在和物理特征为形成理论的发展提供了关键基准。
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引用次数: 0
Editorial to the Topical Collection: Solar and Stellar Dynamos: a New Era 专题集编辑:太阳和恒星动力:一个新时代
IF 10.3 2区 物理与天体物理 Q1 Earth and Planetary Sciences Pub Date : 2023-12-21 DOI: 10.1007/s11214-023-01037-y
Manfred Schüssler, Robert Cameron, Paul Charbonneau, M. Dikpati, Hideyuki Hotta, Leonid Kitchatinov
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引用次数: 0
Sedimentary Processes on Venus 金星上的沉积过程
IF 10.3 2区 物理与天体物理 Q1 Earth and Planetary Sciences Pub Date : 2023-12-01 DOI: 10.1007/s11214-023-01033-2
Lynn M. Carter, M. S. Gilmore, R. Ghail, Paul K. Byrne, S. Smrekar, Terra M. Ganey, N. Izenberg
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引用次数: 1
Initial on-Orbit Results from the GOES-18 Spacecraft Science Magnetometer GOES-18 航天器科学磁强计的初步在轨结果
IF 10.3 2区 物理与天体物理 Q1 Earth and Planetary Sciences Pub Date : 2023-12-01 DOI: 10.1007/s11214-023-01032-3
P. Loto’aniu, A. Davis, A. Jarvis, M. Grotenhuis, F. J. Rich, S. Califf, F. Inceoglu, A. Pacini, H. J. Singer
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引用次数: 0
The Terminal Tracking Camera System on the NASA Lucy Trojan Asteroid Discovery Mission 美国国家航空航天局露西特洛伊小行星发现任务的终端跟踪摄像系统
IF 10.3 2区 物理与天体物理 Q1 Earth and Planetary Sciences Pub Date : 2023-12-01 DOI: 10.1007/s11214-023-01030-5
J. F. Bell, Y. Zhao, E. Cisneros, M. Beasley, C. Olkin, M. Caplinger, M. Ravine, J. Schaffner, M. J. Clark, J. Shamah, P. Faiks, S. Mottola, C. Adam, E. Lessac-Chenen, B. Bos
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引用次数: 0
Origin and Evolution of Jupiter’s Trojan Asteroids 木星特洛伊小行星的起源与演变
IF 10.3 2区 物理与天体物理 Q1 Earth and Planetary Sciences Pub Date : 2023-12-01 DOI: 10.1007/s11214-023-01031-4
W. Bottke, Raphael Marschall, David Nesvorný, D. Vokrouhlický
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引用次数: 0
The Lucy Long Range Reconnaissance Imager (L’LORRI) 露西远程侦察成像仪(L'LORRI)
IF 10.3 2区 物理与天体物理 Q1 Earth and Planetary Sciences Pub Date : 2023-11-30 DOI: 10.1007/s11214-023-01028-z
H. A. Weaver, J. P. Wilson, S. Conard, J. D. Adams, S. Begley, J. Burgum, E. H. Darlington, N. Dello Russo, R. Hacala, S. London, M. F. Morgan, G. Murphy, T. Nelson, A. Shah, J. Spencer, H. Taylor, T. Boehmer, L. Burke, C. Drabenstadt, C. Henry, S. Ling, C. Porter, J. Yin
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引用次数: 0
Tunable Laser Spectrometers for Planetary Science 行星科学用可调谐激光光谱仪
IF 10.3 2区 物理与天体物理 Q1 Earth and Planetary Sciences Pub Date : 2023-11-22 DOI: 10.1007/s11214-023-01023-4
Christopher R. Webster, Amy E. Hofmann, P. Mahaffy, S. Atreya, Christopher H. House, Amy A. Simon, James B. Garvin
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引用次数: 0
Planetary Radio Interferometry and Doppler Experiment (PRIDE) of the JUICE Mission JUICE 飞行任务的行星无线电干涉测量和多普勒实验(PRIDE)
IF 10.3 2区 物理与天体物理 Q1 Earth and Planetary Sciences Pub Date : 2023-11-07 DOI: 10.1007/s11214-023-01026-1
Leonid I. Gurvits, G. Cimò, D. Dirkx, V. Pallichadath, Alexander Akins, Nicolas Altobelli, T. Bocanegra-Bahamon, Stephanie M. Cazaux, Patrick Charlot, D. Duev, Marie S. Fayolle, J. Fogasy, Sándor Frey, V. Lainey, G. Calves, K. Perger, Sergey V. Pogrebenko, N. M. M. Said, C. Vallat, B. Vermeersen, Pieter N.A.M. Visser, Kuo-Nung Wang, Konrad Willner
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引用次数: 0
HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence 太阳风:一个多点,多尺度的任务,以表征湍流
2区 物理与天体物理 Q1 Earth and Planetary Sciences Pub Date : 2023-11-03 DOI: 10.1007/s11214-023-01019-0
Kristopher G. Klein, Harlan Spence, Olga Alexandrova, Matthew Argall, Lev Arzamasskiy, Jay Bookbinder, Theodore Broeren, Damiano Caprioli, Anthony Case, Benjamin Chandran, Li-Jen Chen, Ivan Dors, Jonathan Eastwood, Colin Forsyth, Antoinette Galvin, Vincent Genot, Jasper Halekas, Michael Hesse, Butler Hine, Tim Horbury, Lan Jian, Justin Kasper, Matthieu Kretzschmar, Matthew Kunz, Benoit Lavraud, Olivier Le Contel, Alfred Mallet, Bennett Maruca, William Matthaeus, Jonathan Niehof, Helen O’Brien, Christopher Owen, Alessandro Retinò, Christopher Reynolds, Owen Roberts, Alexander Schekochihin, Ruth Skoug, Charles Smith, Sonya Smith, John Steinberg, Michael Stevens, Adam Szabo, Jason TenBarge, Roy Torbert, Bernard Vasquez, Daniel Verscharen, Phyllis Whittlesey, Brittany Wickizer, Gary Zank, Ellen Zweibel
Abstract HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in plasmas throughout the universe. This will be accomplished by making simultaneous measurements at nine spacecraft with separations spanning magnetohydrodynamic and sub-ion spatial scales in a variety of near-Earth plasmas. In this paper, we describe the scientific background for the HS investigation, the mission goals and objectives, the observatory reference trajectory and instrumentation implementation before the start of Phase B. Through multipoint, multiscale measurements, HS promises to reveal how energy is transferred across scales and boundaries in plasmas throughout the universe.
摘要:HelioSwarm (HS)是美国宇航局太阳物理部门的一项中型探测器任务,旨在探索控制等离子体湍流物理的动态三维机制,等离子体湍流是发生在太阳层和整个宇宙等离子体中的普遍过程。这将通过在9个航天器上同时进行测量来完成,这些航天器在各种近地等离子体中具有跨越磁流体动力学和亚离子空间尺度的分离。在本文中,我们描述了HS研究的科学背景、任务目标和目的、天文台参考轨迹和b阶段开始前的仪器实施。通过多点、多尺度测量,HS有望揭示整个宇宙中等离子体中能量如何跨尺度和边界转移。
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引用次数: 3
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