Space Science Reviews最新文献

{"title":"Characterization of the Surfaces and Near-Surface Atmospheres of Ganymede, Europa and Callisto by JUICE.","authors":"Federico Tosi, Thomas Roatsch, André Galli, Ernst Hauber, Alice Lucchetti, Philippa Molyneux, Katrin Stephan, Nicholas Achilleos, Francesca Bovolo, John Carter, Thibault Cavalié, Giuseppe Cimò, Emiliano D'Aversa, Klaus Gwinner, Paul Hartogh, Hans Huybrighs, Yves Langevin, Emmanuel Lellouch, Alessandra Migliorini, Pasquale Palumbo, Giuseppe Piccioni, Jeffrey J Plaut, Frank Postberg, François Poulet, Kurt Retherford, Ladislav Rezac, Lorenz Roth, Anezina Solomonidou, Gabriel Tobie, Paolo Tortora, Cecilia Tubiana, Roland Wagner, Eva Wirström, Peter Wurz, Francesca Zambon, Marco Zannoni, Stas Barabash, Lorenzo Bruzzone, Michele Dougherty, Randy Gladstone, Leonid I Gurvits, Hauke Hussmann, Luciano Iess, Jan-Erik Wahlund, Olivier Witasse, Claire Vallat, Rosario Lorente","doi":"10.1007/s11214-024-01089-8","DOIUrl":"10.1007/s11214-024-01089-8","url":null,"abstract":"<p><p>We present the state of the art on the study of surfaces and tenuous atmospheres of the icy Galilean satellites Ganymede, Europa and Callisto, from past and ongoing space exploration conducted with several spacecraft to recent telescopic observations, and we show how the ESA JUICE mission plans to explore these surfaces and atmospheres in detail with its scientific payload. The surface geology of the moons is the main evidence of their evolution and reflects the internal heating provided by tidal interactions. Surface composition is the result of endogenous and exogenous processes, with the former providing valuable information about the potential composition of shallow subsurface liquid pockets, possibly connected to deeper oceans. Finally, the icy Galilean moons have tenuous atmospheres that arise from charged particle sputtering affecting their surfaces. In the case of Europa, plumes of water vapour have also been reported, whose phenomenology at present is poorly understood and requires future close exploration. In the three main sections of the article, we discuss these topics, highlighting the key scientific objectives and investigations to be achieved by JUICE. Based on a recent predicted trajectory, we also show potential coverage maps and other examples of reference measurements. The scientific discussion and observation planning presented here are the outcome of the JUICE Working Group 2 (WG2): \"<i>Surfaces and Near-surface Exospheres of the Satellites, dust and rings</i>\".</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 5","pages":"59"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11310297/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141917449","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Advanced Methods for Analyzing in-Situ Observations of Magnetic Reconnection.","authors":"H Hasegawa, M R Argall, N Aunai, R Bandyopadhyay, N Bessho, I J Cohen, R E Denton, J C Dorelli, J Egedal, S A Fuselier, P Garnier, V Génot, D B Graham, K J Hwang, Y V Khotyaintsev, D B Korovinskiy, B Lavraud, Q Lenouvel, T C Li, Y-H Liu, B Michotte de Welle, T K M Nakamura, D S Payne, S M Petrinec, Y Qi, A C Rager, P H Reiff, J M Schroeder, J R Shuster, M I Sitnov, G K Stephens, M Swisdak, A M Tian, R B Torbert, K J Trattner, S Zenitani","doi":"10.1007/s11214-024-01095-w","DOIUrl":"10.1007/s11214-024-01095-w","url":null,"abstract":"<p><p>There is ample evidence for magnetic reconnection in the solar system, but it is a nontrivial task to visualize, to determine the proper approaches and frames to study, and in turn to elucidate the physical processes at work in reconnection regions from in-situ measurements of plasma particles and electromagnetic fields. Here an overview is given of a variety of single- and multi-spacecraft data analysis techniques that are key to revealing the context of in-situ observations of magnetic reconnection in space and for detecting and analyzing the diffusion regions where ions and/or electrons are demagnetized. We focus on recent advances in the era of the Magnetospheric Multiscale mission, which has made electron-scale, multi-point measurements of magnetic reconnection in and around Earth's magnetosphere.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 6","pages":"68"},"PeriodicalIF":9.8,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11369046/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142133806","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Geologic Constraints on the Formation and Evolution of Saturn's Mid-Sized Moons.","authors":"Alyssa Rose Rhoden, Sierra N Ferguson, William Bottke, Julie C Castillo-Rogez, Emily Martin, Michael Bland, Michelle Kirchoff, Marco Zannoni, Nicolas Rambaux, Julien Salmon","doi":"10.1007/s11214-024-01084-z","DOIUrl":"10.1007/s11214-024-01084-z","url":null,"abstract":"<p><p>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.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 5","pages":"55"},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11255024/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141736325","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Strong Lensing by Galaxies.","authors":"A J Shajib, G Vernardos, T E Collett, V Motta, D Sluse, L L R Williams, P Saha, S Birrer, C Spiniello, T Treu","doi":"10.1007/s11214-024-01105-x","DOIUrl":"10.1007/s11214-024-01105-x","url":null,"abstract":"<p><p>Strong gravitational lensing at the galaxy scale is a valuable tool for various applications in astrophysics and cosmology. Some of the primary uses of galaxy-scale lensing are to study elliptical galaxies' mass structure and evolution, constrain the stellar initial mass function, and measure cosmological parameters. Since the discovery of the first galaxy-scale lens in the 1980s, this field has made significant advancements in data quality and modeling techniques. In this review, we describe the most common methods for modeling lensing observables, especially imaging data, as they are the most accessible and informative source of lensing observables. We then summarize the primary findings from the literature on the astrophysical and cosmological applications of galaxy-scale lenses. We also discuss the current limitations of the data and methodologies and provide an outlook on the expected improvements in both areas in the near future.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"220 8","pages":"87"},"PeriodicalIF":9.8,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11549236/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142627960","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Editorial to the Topical Collection: Solar and Stellar Dynamos: a New Era","authors":"Manfred Schüssler, Robert Cameron, Paul Charbonneau, M. Dikpati, Hideyuki Hotta, Leonid Kitchatinov","doi":"10.1007/s11214-023-01037-y","DOIUrl":"https://doi.org/10.1007/s11214-023-01037-y","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"2 4","pages":""},"PeriodicalIF":10.3,"publicationDate":"2023-12-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138948388","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Sedimentary Processes on Venus","authors":"Lynn M. Carter, M. S. Gilmore, R. Ghail, Paul K. Byrne, S. Smrekar, Terra M. Ganey, N. Izenberg","doi":"10.1007/s11214-023-01033-2","DOIUrl":"https://doi.org/10.1007/s11214-023-01033-2","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":" 3","pages":""},"PeriodicalIF":10.3,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138611218","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Initial on-Orbit Results from the GOES-18 Spacecraft Science Magnetometer","authors":"P. Loto’aniu, A. Davis, A. Jarvis, M. Grotenhuis, F. J. Rich, S. Califf, F. Inceoglu, A. Pacini, H. J. Singer","doi":"10.1007/s11214-023-01032-3","DOIUrl":"https://doi.org/10.1007/s11214-023-01032-3","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":" 4","pages":""},"PeriodicalIF":10.3,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138615982","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"The Terminal Tracking Camera System on the NASA Lucy Trojan Asteroid Discovery Mission","authors":"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","doi":"10.1007/s11214-023-01030-5","DOIUrl":"https://doi.org/10.1007/s11214-023-01030-5","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"493 4","pages":""},"PeriodicalIF":10.3,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139012989","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"Origin and Evolution of Jupiter’s Trojan Asteroids","authors":"W. Bottke, Raphael Marschall, David Nesvorný, D. Vokrouhlický","doi":"10.1007/s11214-023-01031-4","DOIUrl":"https://doi.org/10.1007/s11214-023-01031-4","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":" 12","pages":""},"PeriodicalIF":10.3,"publicationDate":"2023-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"138614869","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

{"title":"The Lucy Long Range Reconnaissance Imager (L’LORRI)","authors":"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","doi":"10.1007/s11214-023-01028-z","DOIUrl":"https://doi.org/10.1007/s11214-023-01028-z","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":"49 9","pages":"1-53"},"PeriodicalIF":10.3,"publicationDate":"2023-11-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139206633","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}