Pub Date : 2024-02-01DOI: 10.1007/s11214-023-01036-z
I. J. Daubar, A. Hayes, G. C. Collins, K. L. Craft, J. Rathbun, J. R. Spencer, D. Y. Wyrick, M. Bland, A. G. Davies, C. M. Ernst, S. M. Howell, E. J. Leonard, A. McEwen, J. M. Moore, C. B. Phillips, L. Prockter, L. Quick, J. Scully, J. Soderblom, S. M. Brooks, M. Cable, M. E. Cameron, K. Chan, C. J. Chivers, M. Choukroun, C. Cochrane, S. Diniega, A. Dombard, C. M. Elder, C. Gerekos, C. Glein, T. Greathouse, C. Grima, M. Gudipati, K. P. Hand, C. Hansen, P. Hayne, M. Hedman, K. Hughson, X. Jia, J. Lawrence, H. Meyer, K. Miller, R. Parekh, G. W. Patterson, D. Persaud, S. Piqueux, K. Retherford, K. Scanlan, P. Schenk, B. Schmidt, D. Schroeder, G. Steinbrügge, A. Stern, G. Tobie, P. Withers, D. A. Young, B. Buratti, H. Korth, D. Senske, R. Pappalardo
{"title":"Planned Geological Investigations of the Europa Clipper Mission","authors":"I. J. Daubar, A. Hayes, G. C. Collins, K. L. Craft, J. Rathbun, J. R. Spencer, D. Y. Wyrick, M. Bland, A. G. Davies, C. M. Ernst, S. M. Howell, E. J. Leonard, A. McEwen, J. M. Moore, C. B. Phillips, L. Prockter, L. Quick, J. Scully, J. Soderblom, S. M. Brooks, M. Cable, M. E. Cameron, K. Chan, C. J. Chivers, M. Choukroun, C. Cochrane, S. Diniega, A. Dombard, C. M. Elder, C. Gerekos, C. Glein, T. Greathouse, C. Grima, M. Gudipati, K. P. Hand, C. Hansen, P. Hayne, M. Hedman, K. Hughson, X. Jia, J. Lawrence, H. Meyer, K. Miller, R. Parekh, G. W. Patterson, D. Persaud, S. Piqueux, K. Retherford, K. Scanlan, P. Schenk, B. Schmidt, D. Schroeder, G. Steinbrügge, A. Stern, G. Tobie, P. Withers, D. A. Young, B. Buratti, H. Korth, D. Senske, R. Pappalardo","doi":"10.1007/s11214-023-01036-z","DOIUrl":"https://doi.org/10.1007/s11214-023-01036-z","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":10.3,"publicationDate":"2024-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139892197","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}
Pub Date : 2024-01-28DOI: 10.1007/s11214-024-01049-2
M. Ćuk, M. El Moutamid, Giacomo Lari, Marc Neveu, F. Nimmo, Benoit Noyelles, A. Rhoden, M. Saillenfest
{"title":"Long-Term Evolution of the Saturnian System","authors":"M. Ćuk, M. El Moutamid, Giacomo Lari, Marc Neveu, F. Nimmo, Benoit Noyelles, A. Rhoden, M. Saillenfest","doi":"10.1007/s11214-024-01049-2","DOIUrl":"https://doi.org/10.1007/s11214-024-01049-2","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":10.3,"publicationDate":"2024-01-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140491088","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}
Pub Date : 2024-01-23DOI: 10.1007/s11214-024-01047-4
A. S'anchez-Lavega, T. del Río-Gaztelurrutia, A. Spiga, J. Hern'andez-Bernal, E. Larsen, D. Tirsch, A. Cardesín-Moinelo, P. Machado
{"title":"Dynamical Phenomena in the Martian Atmosphere Through Mars Express Imaging","authors":"A. S'anchez-Lavega, T. del Río-Gaztelurrutia, A. Spiga, J. Hern'andez-Bernal, E. Larsen, D. Tirsch, A. Cardesín-Moinelo, P. Machado","doi":"10.1007/s11214-024-01047-4","DOIUrl":"https://doi.org/10.1007/s11214-024-01047-4","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":10.3,"publicationDate":"2024-01-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140498101","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}
Pub Date : 2024-01-22DOI: 10.1007/s11214-024-01045-6
T. Cavalié, J. Lunine, O. Mousis, R. Hueso
{"title":"The Deep Oxygen Abundance in Solar System Giant Planets, with a New Derivation for Saturn","authors":"T. Cavalié, J. Lunine, O. Mousis, R. Hueso","doi":"10.1007/s11214-024-01045-6","DOIUrl":"https://doi.org/10.1007/s11214-024-01045-6","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":10.3,"publicationDate":"2024-01-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139606370","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}
Pub Date : 2024-01-19DOI: 10.1007/s11214-023-01017-2
D. Gershman, S. Fuselier, Ian J. Cohen, D. L. Turner, Yi-Hsin Liu, Li‐Jen Chen, T. Phan, Julia Stawarz, G. DiBraccio, A. Masters, Robert W. Ebert, Weijie Sun, Yuki Harada, M. Swisdak
{"title":"Magnetic Reconnection at Planetary Bodies and Astrospheres","authors":"D. Gershman, S. Fuselier, Ian J. Cohen, D. L. Turner, Yi-Hsin Liu, Li‐Jen Chen, T. Phan, Julia Stawarz, G. DiBraccio, A. Masters, Robert W. Ebert, Weijie Sun, Yuki Harada, M. Swisdak","doi":"10.1007/s11214-023-01017-2","DOIUrl":"https://doi.org/10.1007/s11214-023-01017-2","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":10.3,"publicationDate":"2024-01-19","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"139612846","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}
Pub Date : 2024-01-17DOI: 10.1007/s11214-024-01046-5
Emma K. Dahl, N. Rowe-Gurney, Glenn S. Orton, S. Brueshaber, R. Cosentino, C. Palotai, Ram B. Sankar, K. Sayanagi
{"title":"Atmospheric Science Questions for a Uranian Probe","authors":"Emma K. Dahl, N. Rowe-Gurney, Glenn S. Orton, S. Brueshaber, R. Cosentino, C. Palotai, Ram B. Sankar, K. Sayanagi","doi":"10.1007/s11214-024-01046-5","DOIUrl":"https://doi.org/10.1007/s11214-024-01046-5","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":10.3,"publicationDate":"2024-01-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140505127","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}
Pub Date : 2024-01-08DOI: 10.1007/s11214-024-01041-w
P. Saha, D. Sluse, Jenny Wagner, L. Williams
{"title":"Essentials of Strong Gravitational Lensing","authors":"P. Saha, D. Sluse, Jenny Wagner, L. Williams","doi":"10.1007/s11214-024-01041-w","DOIUrl":"https://doi.org/10.1007/s11214-024-01041-w","url":null,"abstract":"","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":10.3,"publicationDate":"2024-01-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140512435","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}
Pub Date : 2024-01-01Epub Date: 2024-02-05DOI: 10.1007/s11214-024-01044-7
Sherry H Suyu, Ariel Goobar, Thomas Collett, Anupreeta More, Giorgos Vernardos
Strong gravitational lensing and microlensing of supernovae (SNe) are emerging as a new probe of cosmology and astrophysics in recent years. We provide an overview of this nascent research field, starting with a summary of the first discoveries of strongly lensed SNe. We describe the use of the time delays between multiple SN images as a way to measure cosmological distances and thus constrain cosmological parameters, particularly the Hubble constant, whose value is currently under heated debates. New methods for measuring the time delays in lensed SNe have been developed, and the sample of lensed SNe from the upcoming Rubin Observatory Legacy Survey of Space and Time (LSST) is expected to provide competitive cosmological constraints. Lensed SNe are also powerful astrophysical probes. We review the usage of lensed SNe to constrain SN progenitors, acquire high-z SN spectra through lensing magnifications, infer SN sizes via microlensing, and measure properties of dust in galaxies. The current challenge in the field is the rarity and difficulty in finding lensed SNe. We describe various methods and ongoing efforts to find these spectacular explosions, forecast the properties of the expected sample of lensed SNe from upcoming surveys particularly the LSST, and summarize the observational follow-up requirements to enable the various scientific studies. We anticipate the upcoming years to be exciting with a boom in lensed SN discoveries.
近年来，超新星（SNe）的强引力透镜和微透镜正在成为宇宙学和天体物理学的新探针。我们概述了这一新兴研究领域，首先总结了首次发现的强透镜超新星。我们介绍了如何利用多个 SN 图像之间的时间延迟来测量宇宙学距离，从而约束宇宙学参数，特别是哈勃常数，而哈勃常数的值目前正处于激烈的争论之中。测量有透镜自发彗星时间延迟的新方法已经开发出来，即将进行的鲁宾天文台时空遗留巡天（LSST）的有透镜自发彗星样本有望提供有竞争力的宇宙学约束。透镜SNE也是强大的天体物理探测器。我们回顾了利用透镜原核天体来约束原核天体的祖先、通过透镜放大获得高兹原核天体光谱、通过微透镜推断原核天体的大小以及测量星系中尘埃的性质。该领域目前面临的挑战是发现透镜原核的罕见性和难度。我们介绍了发现这些壮观爆炸的各种方法和正在进行的努力，预测了即将进行的巡天（尤其是 LSST）中预期的有透镜自发彗星样本的性质，并总结了进行各种科学研究所需的观测跟踪要求。我们预计，在接下来的几年里，有透镜SN的发现将是令人兴奋的。
{"title":"Strong Gravitational Lensing and Microlensing of Supernovae.","authors":"Sherry H Suyu, Ariel Goobar, Thomas Collett, Anupreeta More, Giorgos Vernardos","doi":"10.1007/s11214-024-01044-7","DOIUrl":"10.1007/s11214-024-01044-7","url":null,"abstract":"<p><p>Strong gravitational lensing and microlensing of supernovae (SNe) are emerging as a new probe of cosmology and astrophysics in recent years. We provide an overview of this nascent research field, starting with a summary of the first discoveries of strongly lensed SNe. We describe the use of the time delays between multiple SN images as a way to measure cosmological distances and thus constrain cosmological parameters, particularly the Hubble constant, whose value is currently under heated debates. New methods for measuring the time delays in lensed SNe have been developed, and the sample of lensed SNe from the upcoming Rubin Observatory Legacy Survey of Space and Time (LSST) is expected to provide competitive cosmological constraints. Lensed SNe are also powerful astrophysical probes. We review the usage of lensed SNe to constrain SN progenitors, acquire high-z SN spectra through lensing magnifications, infer SN sizes via microlensing, and measure properties of dust in galaxies. The current challenge in the field is the rarity and difficulty in finding lensed SNe. We describe various methods and ongoing efforts to find these spectacular explosions, forecast the properties of the expected sample of lensed SNe from upcoming surveys particularly the LSST, and summarize the observational follow-up requirements to enable the various scientific studies. We anticipate the upcoming years to be exciting with a boom in lensed SN discoveries.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11297109/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141890169","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}
Pub Date : 2024-01-01Epub Date: 2024-05-14DOI: 10.1007/s11214-024-01063-4
B M Walsh, K D Kuntz, S Busk, T Cameron, D Chornay, A Chuchra, M R Collier, C Connor, H K Connor, T E Cravens, N Dobson, M Galeazzi, H Kim, J Kujawski, C K Paw U, F S Porter, V Naldoza, R Nutter, R Qudsi, D G Sibeck, S Sembay, M Shoemaker, K Simms, N E Thomas, E Atz, G Winkert
The Lunar Environment heliospheric X-ray Imager (LEXI) is a wide field-of-view soft X-ray telescope developed to study solar wind-magnetosphere coupling. LEXI is part of the Blue Ghost 1 mission comprised of 10 payloads to be deployed on the lunar surface. LEXI monitors the dayside magnetopause position and shape as a function of time by observing soft X-rays (0.1-2 keV) emitted from solar wind charge-exchange between exospheric neutrals and high charge-state solar wind plasma in the dayside magnetosheath. Measurements of the shape and position of the magnetopause are used to test temporal models of meso- and macro-scale magnetic reconnection. To image the boundary, LEXI employs lobster-eye optics to focus X-rays to a microchannel plate detector with a 9.1 field of view.
月球环境日光层 X 射线成像仪（LEXI）是为研究太阳风-磁层耦合而开发的宽视场软 X 射线望远镜。LEXI 是蓝幽灵 1 号任务的一部分，由 10 个有效载荷组成，将部署在月球表面。LEXI 通过观测外大气层中性物质和日侧磁鞘中高电荷态太阳风等离子体之间太阳风电荷交换发出的软 X 射线（0.1-2 千伏），监测日侧磁鞘位置和形状随时间的变化。对磁层顶形状和位置的测量用于检验中尺度和大尺度磁重联的时间模型。为了对边界进行成像，LEXI 采用了龙虾眼光学技术，将 X 射线聚焦到具有 9.1×∘9.1∘ 视场的微通道板探测器上。
{"title":"The Lunar Environment Heliophysics X-ray Imager (LEXI) Mission.","authors":"B M Walsh, K D Kuntz, S Busk, T Cameron, D Chornay, A Chuchra, M R Collier, C Connor, H K Connor, T E Cravens, N Dobson, M Galeazzi, H Kim, J Kujawski, C K Paw U, F S Porter, V Naldoza, R Nutter, R Qudsi, D G Sibeck, S Sembay, M Shoemaker, K Simms, N E Thomas, E Atz, G Winkert","doi":"10.1007/s11214-024-01063-4","DOIUrl":"https://doi.org/10.1007/s11214-024-01063-4","url":null,"abstract":"<p><p>The Lunar Environment heliospheric X-ray Imager (LEXI) is a wide field-of-view soft X-ray telescope developed to study solar wind-magnetosphere coupling. LEXI is part of the Blue Ghost 1 mission comprised of 10 payloads to be deployed on the lunar surface. LEXI monitors the dayside magnetopause position and shape as a function of time by observing soft X-rays (0.1-2 keV) emitted from solar wind charge-exchange between exospheric neutrals and high charge-state solar wind plasma in the dayside magnetosheath. Measurements of the shape and position of the magnetopause are used to test temporal models of meso- and macro-scale magnetic reconnection. To image the boundary, LEXI employs lobster-eye optics to focus X-rays to a microchannel plate detector with a 9.1<math><mmultiscripts><mo>×</mo><mprescripts></mprescripts><none></none><mo>∘</mo></mmultiscripts><msup><mn>9.1</mn><mo>∘</mo></msup></math> field of view.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":10.3,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11093736/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"140959508","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}
Pub Date : 2024-01-01Epub Date: 2024-06-17DOI: 10.1007/s11214-024-01079-w
S Birrer, M Millon, D Sluse, A J Shajib, F Courbin, S Erickson, L V E Koopmans, S H Suyu, T Treu
Multiply lensed images of a same source experience a relative time delay in the arrival of photons due to the path length difference and the different gravitational potentials the photons travel through. This effect can be used to measure absolute distances and the Hubble constant ( ) and is known as time-delay cosmography. The method is independent of the local distance ladder and early-universe physics and provides a precise and competitive measurement of . With upcoming observatories, time-delay cosmography can provide a 1% precision measurement of and can decisively shed light on the current reported 'Hubble tension'. This manuscript details the general methodology developed over the past decades in time-delay cosmography, discusses recent advances and results, and, foremost, provides a foundation and outlook for the next decade in providing accurate and ever more precise measurements with increased sample size and improved observational techniques.
同一光源的多重透镜图像在光子到达时会出现相对的时间延迟，这是由于光子经过的路径长度差异和重力势能不同造成的。这种效应可用于测量绝对距离和哈勃常数（H 0），被称为时间延迟宇宙学。这种方法不受本地距离阶梯和早期宇宙物理学的影响，可以精确地测量哈勃常数。通过即将建成的天文台，时间延迟宇宙学可以对 H 0 进行 1% 的精确测量，并对目前报道的 "哈勃张力 "做出决定性的解释。这篇手稿详细介绍了过去几十年来在时间延迟宇宙学方面发展起来的一般方法，讨论了最近的进展和结果，最重要的是为下一个十年提供了基础和展望，以便随着样本量的增加和观测技术的改进，提供更精确的测量结果。
{"title":"Time-Delay Cosmography: Measuring the Hubble Constant and Other Cosmological Parameters with Strong Gravitational Lensing.","authors":"S Birrer, M Millon, D Sluse, A J Shajib, F Courbin, S Erickson, L V E Koopmans, S H Suyu, T Treu","doi":"10.1007/s11214-024-01079-w","DOIUrl":"10.1007/s11214-024-01079-w","url":null,"abstract":"<p><p>Multiply lensed images of a same source experience a relative time delay in the arrival of photons due to the path length difference and the different gravitational potentials the photons travel through. This effect can be used to measure absolute distances and the Hubble constant ( <math><msub><mi>H</mi> <mn>0</mn></msub> </math> ) and is known as time-delay cosmography. The method is independent of the local distance ladder and early-universe physics and provides a precise and competitive measurement of <math><msub><mi>H</mi> <mn>0</mn></msub> </math> . With upcoming observatories, time-delay cosmography can provide a 1% precision measurement of <math><msub><mi>H</mi> <mn>0</mn></msub> </math> and can decisively shed light on the current reported 'Hubble tension'. This manuscript details the general methodology developed over the past decades in time-delay cosmography, discusses recent advances and results, and, foremost, provides a foundation and outlook for the next decade in providing accurate and ever more precise measurements with increased sample size and improved observational techniques.</p>","PeriodicalId":21902,"journal":{"name":"Space Science Reviews","volume":null,"pages":null},"PeriodicalIF":9.1,"publicationDate":"2024-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC11182856/pdf/","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141427666","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}
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