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Posiolova LV, Lognonné P, Banerdt WB, Clinton J, Collins GS, Kawamura T, Ceylan S, Daubar IJ, Fernando B, Froment M, Giardini D, Malin MC, Miljković K, Stähler SC, Xu Z, Banks ME, Beucler É, Cantor BA, Charalambous C, Dahmen N, Davis P, Drilleau M, Dundas CM, Durán C, Euchner F, Garcia RF, Golombek M, Horleston A, Keegan C, Khan A, Kim D, Larmat C, Lorenz R, Margerin L, Menina S, Panning M, Pardo C, Perrin C, Pike WT, Plasman M, Rajšić A, Rolland L, Rougier E, Speth G, Spiga A, Stott A, Susko D, Teanby NA, Valeh A, Werynski A, Wójcicka N, Zenhäusern G. Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation. Science 2022; 378:412-417. [DOI: 10.1126/science.abq7704] [Citation(s) in RCA: 2] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Two >130-meter-diameter impact craters formed on Mars during the later half of 2021. These are the two largest fresh impact craters discovered by the Mars Reconnaissance Orbiter since operations started 16 years ago. The impacts created two of the largest seismic events (magnitudes greater than 4) recorded by InSight during its 3-year mission. The combination of orbital imagery and seismic ground motion enables the investigation of subsurface and atmospheric energy partitioning of the impact process on a planet with a thin atmosphere and the first direct test of martian deep-interior seismic models with known event distances. The impact at 35°N excavated blocks of water ice, which is the lowest latitude at which ice has been directly observed on Mars.
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Affiliation(s)
| | - P. Lognonné
- Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France
| | - W. B. Banerdt
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - J. Clinton
- Swiss Seismological Service, ETH Zurich, Zurich, Switzerland
| | - G. S. Collins
- Department of Earth Science and Engineering, Imperial College London, London, UK
| | - T. Kawamura
- Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France
| | - S. Ceylan
- Institute of Geophysics, ETH Zurich, Zurich, Switzerland
| | - I. J. Daubar
- Department of Earth, Environmental, and Planetary Sciences, Brown University, Providence, RI, USA
| | - B. Fernando
- Department of Earth Sciences, University of Oxford, Oxford, UK
| | - M. Froment
- Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France
- Earth and Environmental Sciences Division, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - D. Giardini
- Institute of Geophysics, ETH Zurich, Zurich, Switzerland
| | - M. C. Malin
- Malin Space Science Systems, San Diego, CA, USA
| | - K. Miljković
- Space Science and Technology Centre, School of Earth and Planetary Sciences, Curtin University, Perth, WA, Australia
| | - S. C. Stähler
- Institute of Geophysics, ETH Zurich, Zurich, Switzerland
| | - Z. Xu
- Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France
| | - M. E. Banks
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - É. Beucler
- Nantes Université, Université Angers, Le Mans Université, CNRS, UMR 6112, Laboratoire de Planétologie et Géosciences, Nantes, France
| | | | - C. Charalambous
- Department of Electrical and Electronic Engineering, Imperial College London, London, UK
| | - N. Dahmen
- Institute of Geophysics, ETH Zurich, Zurich, Switzerland
| | - P. Davis
- Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, USA
| | - M. Drilleau
- Institut Supérieur de l’Aéronautique et de l’Espace ISAE-SUPAERO, Toulouse, France
| | - C. M. Dundas
- U.S. Geological Survey, Astrogeology Science Center, Flagstaff, AZ, USA
| | - C. Durán
- Institute of Geophysics, ETH Zurich, Zurich, Switzerland
| | - F. Euchner
- Institute of Geophysics, ETH Zurich, Zurich, Switzerland
| | - R. F. Garcia
- Institut Supérieur de l’Aéronautique et de l’Espace ISAE-SUPAERO, Toulouse, France
| | - M. Golombek
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - A. Horleston
- School of Earth Sciences, University of Bristol, Bristol, UK
| | - C. Keegan
- Malin Space Science Systems, San Diego, CA, USA
| | - A. Khan
- Institute of Geophysics, ETH Zurich, Zurich, Switzerland
- Physik-Institut, University of Zurich, Zurich, Switzerland
| | - D. Kim
- Institute of Geophysics, ETH Zurich, Zurich, Switzerland
- Department of Geology, University of Maryland, College Park, MD, USA
| | - C. Larmat
- Earth and Environmental Sciences Division, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - R. Lorenz
- Johns Hopkins Applied Physics Laboratory, Laurel, MD, USA
| | - L. Margerin
- Institut de Recherche en Astrophysique et Planétologie, Université Toulouse III Paul Sabatier, CNRS, CNES, Toulouse, France
| | - S. Menina
- Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France
| | - M. Panning
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - C. Pardo
- Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France
| | - C. Perrin
- Nantes Université, Université Angers, Le Mans Université, CNRS, UMR 6112, Laboratoire de Planétologie et Géosciences, Nantes, France
| | - W. T. Pike
- Department of Electrical and Electronic Engineering, Imperial College London, London, UK
| | - M. Plasman
- Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Paris, France
| | - A. Rajšić
- Space Science and Technology Centre, School of Earth and Planetary Sciences, Curtin University, Perth, WA, Australia
| | - L. Rolland
- Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, IRD, Géoazur, Valbonne, France
| | - E. Rougier
- Earth and Environmental Sciences Division, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - G. Speth
- Malin Space Science Systems, San Diego, CA, USA
| | - A. Spiga
- Laboratoire de Météorologie Dynamique/IPSL, Sorbonne Université, CNRS, Ecole Normale Supérieure, PSL Research University, Ecole Polytechnique, Paris, France
| | - A. Stott
- Institut Supérieur de l’Aéronautique et de l’Espace ISAE-SUPAERO, Toulouse, France
| | - D. Susko
- Malin Space Science Systems, San Diego, CA, USA
| | - N. A. Teanby
- School of Earth Sciences, University of Bristol, Bristol, UK
| | - A. Valeh
- Malin Space Science Systems, San Diego, CA, USA
| | - A. Werynski
- Malin Space Science Systems, San Diego, CA, USA
| | - N. Wójcicka
- Department of Earth Science and Engineering, Imperial College London, London, UK
| | - G. Zenhäusern
- Institute of Geophysics, ETH Zurich, Zurich, Switzerland
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Karamlou M, Asaria I, Barron J, Boutros P, Fisher V, Grandinetti R, Johnson J, Richard E, Susko D, Urrutia C, Woolsey B, Baumann R, Cottle J, Sweaney R, Wenzel M, Nusstein J, Hall D. Complications After Dental Sedation: A Myotonic Mystery Case Report. Anesth Prog 2022; 69:26-31. [PMID: 36534775 PMCID: PMC9773408 DOI: 10.2344/anpr-69-02-09] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/24/2021] [Accepted: 03/18/2022] [Indexed: 12/23/2022] Open
Abstract
Myotonic dystrophy (dystrophia myotonica; DM) is an uncommon progressive hereditary muscle disorder that can present with variable severity at birth, in early childhood, or most commonly as an adult. Patients with DM, especially type 1 (DM1), are extremely sensitive to the respiratory depressant effects of sedative-hypnotics, anxiolytics, and opioid agonists. This case report describes a 37-year-old male patient with previously undiagnosed DM1 who received dental care under minimal sedation using intravenous midazolam. During the case, the patient experienced 2 brief episodes of hypoxemia, the second of which required emergency intubation after propofol and succinylcholine and resulted in extended hospital admission. A lipid emulsion (Liposyn II 20%) infusion was given approximately 2 hours after the last local anesthetic injection due to slight ST elevation and suspicion of local anesthetic toxicity (LAST). Months after treatment, the patient suffered a fall resulting in a fatal traumatic brain injury. Complications noted in this case report were primarily attributed to the unknown diagnosis of DM1, although additional precipitating factors were likely present. This report also provides a basic review of the literature and clinical guidelines for managing myotonic dystrophy patients for dental care with local anesthesia, sedation, or general anesthesia.
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Affiliation(s)
- Milad Karamlou
- Former Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Iman Asaria
- Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Jaime Barron
- Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Petra Boutros
- Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Vincent Fisher
- Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Rachel Grandinetti
- Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Julian Johnson
- Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Emily Richard
- Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - David Susko
- Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Cristobal Urrutia
- Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Bryce Woolsey
- Chief Resident, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Ronald Baumann
- Former Assistant Professor and Attending, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - James Cottle
- Assistant Professor and Attending, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Richard Sweaney
- Assistant Professor and Attending, The Ohio State University College of Dentistry General Practice Residency Program, Columbus, Ohio
| | - Mark Wenzel
- Program Director and Hospital Attending, The Ohio State University College of Dentistry General Practice Residency Program and Wexner Medical Center, Columbus, Ohio
| | - John Nusstein
- Professor and Chair Division of Endodontics, The Ohio State University College of Dentistry, Columbus, Ohio
| | - David Hall
- Associate Professor and Hospital Attending, The Ohio State University College of Dentistry General Practice Residency Program and Wexner Medical Center, Columbus, Ohio
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Susko D, Karunatillake S, Kodikara G, Skok JR, Wray J, Heldmann J, Cousin A, Judice T. A record of igneous evolution in Elysium, a major martian volcanic province. Sci Rep 2017; 7:43177. [PMID: 28233797 PMCID: PMC5324095 DOI: 10.1038/srep43177] [Citation(s) in RCA: 11] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/25/2016] [Accepted: 01/22/2017] [Indexed: 11/30/2022] Open
Abstract
A major knowledge gap exists on how eruptive compositions of a single martian volcanic province change over time. Here we seek to fill that gap by assessing the compositional evolution of Elysium, a major martian volcanic province. A unique geochemical signature overlaps with the southeastern flows of this volcano, which provides the context for this study of variability of martian magmatism. The southeastern lava fields of Elysium Planitia show distinct chemistry in the shallow subsurface (down to several decimeters) relative to the rest of the martian mid-to-low latitudes (average crust) and flows in northwest Elysium. By impact crater counting chronology we estimated the age of the southeastern province to be 0.85 ± 0.08 Ga younger than the northwestern fields. This study of the geochemical and temporal differences between the NW and SE Elysium lava fields is the first to demonstrate compositional variation within a single volcanic province on Mars. We interpret the geochemical and temporal differences between the SE and NW lava fields to be consistent with primary magmatic processes, such as mantle heterogeneity or change in depth of melt formation within the martian mantle due to crustal loading.
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Affiliation(s)
- David Susko
- Department of Geology and Geophysics, Louisiana State University, Louisiana, USA
| | - Suniti Karunatillake
- Department of Geology and Geophysics, Louisiana State University, Louisiana, USA
| | - Gayantha Kodikara
- Department of Oceanography and Marine Geology, Faculty of Fisheries and Marine Sciences &Technology, University of Rahuna, Matara, Sri Lanka
| | | | - James Wray
- School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, GA, USA
| | | | - Agnes Cousin
- Institut de Recherche en Astrophysique et Planétologie, Toulouse, France
| | - Taylor Judice
- Department of Geology and Geophysics, Louisiana State University, Louisiana, USA
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