News in Focus NASA/JPL-CALTECH Perseverance Is Lowered Onto Mars’S Dusty Surface by a Rocket-Powered ‘Sky Crane’
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Mawrth Vallis, Mars: a Fascinating Place for Future in Situ Exploration
Mawrth Vallis, Mars: a fascinating place for future in situ exploration François Poulet1, Christoph Gross2, Briony Horgan3, Damien Loizeau1, Janice L. Bishop4, John Carter1, Csilla Orgel2 1Institut d’Astrophysique Spatiale, CNRS/Université Paris-Sud, 91405 Orsay Cedex, France 2Institute of Geological Sciences, Planetary Sciences and Remote Sensing Group, Freie Universität Berlin, Germany 3Purdue University, West Lafayette, USA. 4SETI Institute/NASA-ARC, Mountain View, CA, USA Corresponding author: François Poulet, IAS, Bâtiment 121, CNRS/Université Paris-Sud, 91405 Orsay Cedex, France; email: [email protected] Running title: Mawrth: a fascinating place for exploration 1 Abstract After the successful landing of the Mars Science Laboratory rover, both NASA and ESA initiated a selection process for potential landing sites for the Mars2020 and ExoMars missions, respectively. Two ellipses located in the Mawrth Vallis region were proposed and evaluated during a series of meetings (3 for Mars2020 mission and 5 for ExoMars). We describe here the regional context of the two proposed ellipses as well as the framework of the objectives of these two missions. Key science targets of the ellipses and their astrobiological interests are reported. This work confirms the proposed ellipses contain multiple past Martian wet environments of subaerial, subsurface and/or subaqueous character, in which to probe the past climate of Mars, build a broad picture of possible past habitable environments, evaluate their exobiological potentials and search for biosignatures in well-preserved rocks. A mission scenario covering several key investigations during the nominal mission of each rover is also presented, as well as descriptions of how the site fulfills the science requirements and expectations of in situ martian exploration. -
Columbus Crater HLS2 Hangout: Exploration Zone Briefing
Columbus Crater HLS2 Hangout: Exploration Zone Briefing Kennda Lynch1,2, Angela Dapremont2, Lauren Kimbrough2, Alex Sessa2, and James Wray2 1Lunar and Planetary Institute/Universities Space Research Association 2Georgia Institute of Technology Columbus Crater: An Overview • Groundwater-fed paleolake located in northwest region of Terra Sirenum • ~110 km in diameter • Diversity of Noachian & Hesperian aged deposits and outcrops • High diversity of aqueous mineral deposits • Estimated 1.5 km depth of sedimentary and/or volcanic infill • High Habitability and Biosignature Preservation Potential LZ & Field Station Latitude: 194.0194 E Longitude: 29.2058 S Altitude: +910 m SROI #1 RROI #1 LZ/HZ SROI #4 SROI #2 SROI #5 22 KM HiRISE Digital Terrain Model (DTM) • HiRISE DTMs are made from two images of the same area on the ground, taken from different look angles (known as a stereo-pair) • DTM’s are powerful research tools that allow researchers to take terrain measurements and model geological processes • For our traversability analysis of Columbus: • The HiRISE DTM was processed and completed by the University of Arizona HiRISE Operations Center. • DTM data were imported into ArcMap 10.5 software and traverses were acquired and analyzed using the 3D analyst tool. • A slope map was created in ArcMap to assess slope values along traverses as a supplement to topography observations. Slope should be ≤30°to meet human mission requirements. Conclusions Traversability • 9 out of the 17 traverses analyzed met the slope criteria for human missions. • This region of Columbus Crater is traversable and allows access to regions of astrobiological interest. It is also a possible access point to other regions of Terra Sirenum. -
Mars Helicopter/Ingenuity
National Aeronautics and Space Administration Mars Helicopter/Ingenuity When NASA’s Perseverance rover lands on February 18, 2021, it will be carrying a passenger onboard: the first helicopter ever designed to fly in the thin Martian air. The Mars Helicopter, Ingenuity, is a small, or as full standalone science craft carrying autonomous aircraft that will be carried to instrument payloads. Taking to the air would the surface of the Red Planet attached to the give scientists a new perspective on a region’s belly of the Perseverance rover. Its mission geology and even allow them to peer into is experimental in nature and completely areas that are too steep or slippery to send independent of the rover’s science mission. a rover. In the distant future, they might even In the months after landing, the helicopter help astronauts explore Mars. will be placed on the surface to test – for the first time ever – powered flight in the thin The project is solely a demonstration of Martian air. Its performance during these technology; it is not designed to support the experimental test flights will help inform Mars 2020/Perseverance mission, which decisions relating to considering small is searching for signs of ancient life and helicopters for future Mars missions, where collecting samples of rock and sediment in they could perform in a support role as tubes for potential return to Earth by later robotic scouts, surveying terrain from above, missions. This illustration shows the Mars Helicopter Ingenuity on the surface of Mars. Key Objectives Key Features • Prove powered flight in the thin atmosphere of • Weighs 4 pounds (1.8 kg) Mars. -
Implications for Mars 2020 Strategic Planning. J.I
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 1515.pdf CHARACTERIZING THE STRATIGRAPHY OF THE NILI PLANUM REGION OUTSIDE JEZERO CRATER: IMPLICATIONS FOR MARS 2020 STRATEGIC PLANNING. J.I. Simon1, E.L. Scheller2, S. Holm- Alwmark3, K.C. Benison4, T. Bosak5, A.J. Brown6, L.E. Mayhew7, D.L. Shuster8, V. Sun9, B.P. Weiss5, N.R. Williams9, and the Mars 2020 Science Team. 1NASA JSC, TX ([email protected]), 2Caltech, CA, 3University of Copenhagen, Denmark, 4West Virginia University, WV, 5MIT, MA, 6Plancius Research, MD, 7University of Colorado Boulder, CO, 8UC Berkeley, CA, 9JPL/Caltech, CA. Introduction: The Mars 2020 team has developed plans for exploration and sample collection of the Nili On delta Planum region outside Jezero crater (Fig. 1) for the Near delta Far east possibility of an extended mission. This extended mission would follow and complement the exploration Sample of Jezero, as it expands investigations of the regional depots/ stratigraphy [1-2] to new settings and would likely Start extend the accessible geology ~1-2 billion years Areas in compared to the primary mission. This area has common representative units of Nili Fossae and the Nili Planum regions [3-6], including the canonical Noachian Basement, Olivine-carbonate Unit, Mafic Cap Unit, and putative younger fluvial-lacustrine deposits and presumably spans Pre-Noachian/Early Noachian to Figure 1: Region and suggested extended mission rover paths Hesperian time [1-4]. This stratigraphy likely records outside Jezero crater. Color coding indicate 3 paths that afford high prior surface and subsurface aqueous environments, priority science and sampling objectives in Nili Planum. -
Mineralogy of the Martian Surface
EA42CH14-Ehlmann ARI 30 April 2014 7:21 Mineralogy of the Martian Surface Bethany L. Ehlmann1,2 and Christopher S. Edwards1 1Division of Geological & Planetary Sciences, California Institute of Technology, Pasadena, California 91125; email: [email protected], [email protected] 2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 Annu. Rev. Earth Planet. Sci. 2014. 42:291–315 Keywords First published online as a Review in Advance on Mars, composition, mineralogy, infrared spectroscopy, igneous processes, February 21, 2014 aqueous alteration The Annual Review of Earth and Planetary Sciences is online at earth.annualreviews.org Abstract This article’s doi: The past fifteen years of orbital infrared spectroscopy and in situ exploration 10.1146/annurev-earth-060313-055024 have led to a new understanding of the composition and history of Mars. Copyright c 2014 by Annual Reviews. Globally, Mars has a basaltic upper crust with regionally variable quanti- by California Institute of Technology on 06/09/14. For personal use only. All rights reserved ties of plagioclase, pyroxene, and olivine associated with distinctive terrains. Enrichments in olivine (>20%) are found around the largest basins and Annu. Rev. Earth Planet. Sci. 2014.42:291-315. Downloaded from www.annualreviews.org within late Noachian–early Hesperian lavas. Alkali volcanics are also locally present, pointing to regional differences in igneous processes. Many ma- terials from ancient Mars bear the mineralogic fingerprints of interaction with water. Clay minerals, found in exposures of Noachian crust across the globe, preserve widespread evidence for early weathering, hydrothermal, and diagenetic aqueous environments. Noachian and Hesperian sediments include paleolake deposits with clays, carbonates, sulfates, and chlorides that are more localized in extent. -
Bio-Preservation Potential of Sediment in Eberswalde Crater, Mars
Western Washington University Western CEDAR WWU Graduate School Collection WWU Graduate and Undergraduate Scholarship Fall 2020 Bio-preservation Potential of Sediment in Eberswalde crater, Mars Cory Hughes Western Washington University, [email protected] Follow this and additional works at: https://cedar.wwu.edu/wwuet Part of the Geology Commons Recommended Citation Hughes, Cory, "Bio-preservation Potential of Sediment in Eberswalde crater, Mars" (2020). WWU Graduate School Collection. 992. https://cedar.wwu.edu/wwuet/992 This Masters Thesis is brought to you for free and open access by the WWU Graduate and Undergraduate Scholarship at Western CEDAR. It has been accepted for inclusion in WWU Graduate School Collection by an authorized administrator of Western CEDAR. For more information, please contact [email protected]. Bio-preservation Potential of Sediment in Eberswalde crater, Mars By Cory M. Hughes Accepted in Partial Completion of the Requirements for the Degree Master of Science ADVISORY COMMITTEE Dr. Melissa Rice, Chair Dr. Charles Barnhart Dr. Brady Foreman Dr. Allison Pfeiffer GRADUATE SCHOOL David L. Patrick, Dean Master’s Thesis In presenting this thesis in partial fulfillment of the requirements for a master’s degree at Western Washington University, I grant to Western Washington University the non-exclusive royalty-free right to archive, reproduce, distribute, and display the thesis in any and all forms, including electronic format, via any digital library mechanisms maintained by WWU. I represent and warrant this is my original work, and does not infringe or violate any rights of others. I warrant that I have obtained written permissions from the owner of any third party copyrighted material included in these files. -
Nr. 64/1002 22.10.2015 EØS-Tillegget Til Den Europeiske Unions
Nr. 64/1002 EØS-tillegget til Den europeiske unions tidende 22.10.2015 KOMMISJONSVEDTAK 2015/EØS/64/27 av 17. august 2005 om innføring av eit register over stader som skal danne eit interkalibreringsnett i samsvar med europaparlaments- og rådsdirektiv 2000/60/EF [meldt under nummeret K(2005) 3140] (2005/646/EF)(*) KOMMISJONEN FOR DEI EUROPEISKE FELLESSKAPA fastsett ein framgangsmåte for å sikre at biologiske HAR — overvakingsresultat kan jamførast medlemsstatane imellom, ettersom dei utgjer ein sentral del av klassifiseringa av økologisk tilstand. Ein føresetnad for dette er at resultata av overvakings- og med tilvising til traktaten om skipinga av Det europeiske klassifiseringssystema i medlemsstatane vert jamførte fellesskapet, gjennom eit interkalibreringsnett som er samansett av overvakingsstader i kvar medlemsstat og i kvar økoregion i Fellesskapet. Direktivet krev at medlemsstatane i høveleg omfang samlar inn naudsynte opplysningar som gjeld dei stadene som inngår i interkalibrerings- med tilvising til europaparlaments- og rådsdirektiv 2000/60/ nettet, slik at det vert mogleg å vurdere om det EF av 23. oktober 2000 om fastsettelse av en ramme for nasjonale klassifiseringssystemet stemmer overeins fellesskapstiltak på området vannpolitikk(1), særleg nr. 1.4.1 med dei normative definisjonane i vedlegg V til direktiv vii) i vedlegg V til direktivet, og 2000/60/EF, og om klassifiseringssystema kan jamførast medlemsstatane imellom. ut frå desse synsmåtane: 1) Etter artikkel 4 nr. 1) bokstav a) ii) i direktiv 2000/60/ EF skal medlemsstatane, med atterhald for visse unntak, verne, betre og gjenopprette alle førekomstar av overflatevatn med sikte på å oppnå god overflatevas- stilstand seinast 15 år etter at direktivet tok til å gjelde, i samsvar med dei føresegnene som er fastsette i vedlegg V til direktivet. -
News in Focus GETTY Ahead of a Lockdown Imposed on 14 April, Migrant Workers Queue at a Railway Station to Leave the City of Mumbai, India
The world this week News in focus GETTY Ahead of a lockdown imposed on 14 April, migrant workers queue at a railway station to leave the city of Mumbai, India. INDIA’S MASSIVE COVID SURGE PUZZLES SCIENTISTS The virus is spreading faster than ever before in India, despite previous high infection rates in megacities, which should have conferred some protection. By Smriti Mallapaty Delhi and Chennai had already been infected, Germany are also currently experiencing large leading some researchers to conclude that the outbreaks relative to their size, and nations he pandemic is sweeping through India worst of the pandemic was over in the country. including Brazil and the United States are at a pace that has staggered scientists. Researchers in India are now trying to pin- reporting infection rates of around 60,000– Daily case numbers have exploded point what is behind the unprecedented surge, 70,000 a day. But India’s daily totals are now since early March: the government which could be due to an unfortunate con- the highest recorded for any country, and have reported 352,991 new infections fluence of factors, including the emergence exceeded a peak of 300,000 cases seen in the Tnationally on 25 April. High numbers in India of particularly infectious variants, a rise in United States on 2 January. have also helped to drive daily global cases to un restricted social interactions, and low vac- COVID-19 case numbers started to drop in a high of 899,755 in the past week, breaking a cine coverage. Untangling the causes could India last September, after a high of around record set in January. -
Translitterering Och Alternativa Geografiska Namnformer
TRANSLITTERERING OCH ALTERNATIVA GEOGRAFISKA NAMNFORMER Version XX, 27 juli 2015, Stefan Nordblom 1 FÖRORD För många utländska egennamn, i första hand personnamn och geografiska namn, finns det på svenska väl etablerade namnformer. Om det inte finns någon sådan kan utländska egennamn dock vålla bekymmer vid översättning till svenska. Föreliggande material är tänkt att vara till hjälp i sådana situationer och tar upp fall av translitterering1 och transkribering2 samt exonymer3 . Problemen uppstår främst på grund av att olika språk har olika system för translitterering och transkribering från ett visst språk och på grund av att orter kan ha olika namn på olika utländska språk. Eftersom vi oftast översätter från engelska och franska innehåller sammanställningen även translittereringar och exonymer på engelska och franska (samt tyska). Man kan alltså i detta material göra en sökning på sådana namnformer och komma fram till den svenska namnformen. Om man t.ex. i en engelsk text träffar på det geografiska namnet Constance kan man söka på det namnet här och då få reda på att staden (i detta fall på tyska och) på svenska kallas Konstanz. Den efterföljande sammanställningen bygger i huvudsak på följande källor: Institutet för de inhemska språken (FI): bl.a. skriften Svenska ortnamn i Finland - http://kaino.kotus.fi/svenskaortnamn/ Iate (EU-institutionernas termbank) Nationalencyklopedin Nationalencyklopedins kartor Interinstitutionella publikationshandboken - http://publications.europa.eu/code/sv/sv-000100.htm Språkbruk (Tidskrift utgiven av Svenska språkbyrån i Helsingfors) Språkrådet© (1996). Publikation med rekommendationer i term- och språkfrågor som utarbetas av rådets svenska översättningsenhet i samråd med övriga EU-institutioner. TT-språket - info.tt.se/tt-spraket/ I de fall uppgifterna i dessa källor inte överensstämmer med varandra har det i enskilda fall varit nödvändigt att väga, välja och sammanjämka namnförslagen, varvid rimlig symmetri har eftersträvats. -
The Mars 2020 Candidate Landing Sites: a Magnetic Field Perspective
The Mars 2020 Candidate Landing Sites: A Magnetic Field Perspective The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Mittelholz, Anna et al. “The Mars 2020 Candidate Landing Sites: A Magnetic Field Perspective.” Earth and Space Science 5, 9 (September 2018): 410-424 © 2018 The Authors As Published http://dx.doi.org/10.1029/2018EA000420 Publisher American Geophysical Union (AGU) Version Final published version Citable link http://hdl.handle.net/1721.1/118846 Terms of Use Creative Commons Attribution-NonCommercial-NoDerivs License Detailed Terms http://creativecommons.org/licenses/by-nc-nd/4.0/ Earth and Space Science RESEARCH ARTICLE The Mars 2020 Candidate Landing Sites: A Magnetic 10.1029/2018EA000420 Field Perspective Key Points: • Mars 2020 offers the opportunity Anna Mittelholz1 , Achim Morschhauser2 , Catherine L. Johnson1,3, to acquire samples that record the Benoit Langlais4 , Robert J. Lillis5 , Foteini Vervelidou2 , and Benjamin P. Weiss6 intensity and direction of the ancient Martian magnetic field 1 • Laboratory paleomagnetic Department of Earth, Ocean and Atmospheric Sciences, The University of British Columbia, Vancouver, British Columbia, 2 3 measurements of returned samples Canada, GFZ German Research Center for Geosciences, Potsdam, Germany, Planetary Science Institute, Tucson, AZ, USA, can address questions about the 4Laboratoire de Planétologie et Geodynamique, UMR 6112 CNRS & Université de Nantes, Nantes, France, 5Space Science history of the -
Jan - Mar 2021 Volume 11 • Issue 1
National Aeronautics and Space Administration IT Talk Jan - Mar 2021 Volume 11 • Issue 1 Collaboration at NASA www.nasa.gov IT Talk Jan - Mar 2021 Volume 11 • Issue 1 In this Issue Office of the CIO NASA Headquarters 300 E Street SW Message From Washington, D.C. 20546 3 the NASA CIO Chief Information Officer Jeff Seaton (Acting) Editor & Publication Manager Eldora Valentine Graphic & Web Designer Michael Porterfield ICT SCRM Copy Editor 4 Takes a Village Meredith Isaacs IT Talk is an official publication of the Office of the Chief Information Officer Collaboration of the National Aeronautics and Space Administration, Headquarters, 6 at NASA Washington, D.C. It is published by the OCIO office for all NASA employees and external audiences. For distribution questions or to suggest a story idea, email: Remote Collaboration [email protected] Tools Support To read IT Talk online visit: www.nasa.gov/offices/ocio/ittalk 8 NASA’s Mission For more info on the OCIO: v www.nasa.gov/offices/ocio v inside.nasa.gov/ocio (Internal NASA network only) Communications www.nasa.gov/open/ v Program Hosts www.facebook.com/NASAcio 10 Webex Cheer Wall Message from the NASA CIO The COVID-19 pandemic highlights the importance of effective collaboration. Enhanced remote teamwork tools with the accelerated availability of Teams, train- ing sessions, Office 365 mobile applications, and the Teams Audio Conferencing service have allowed our Agency’s mission to successfully continue. Scientists and engineers have been able to collaborate with internal and external partners to develop research proposals, exchange ideas and observations, share data and analysis, and collaboratively develop scientific software applications. -
Deep Space Navigation
Deep Space Navigation NASA Technology Roadmaps Review Robotics, Communications, and Navigation Workshop 29 March 2011 Lincoln J. Wood Jet Propulsion Laboratory, California Institute of Technology Topics to be Covered • Information about speaker • General comments on roadmap • Comments on roadmap Section 2.1.4 • Radio metric tracking technologies • Frequency and timing technologies • Comments on roadmap section 2.1.6 • Communications technologies (brief overview) LJW - 2 Information about Speaker • Education – B.S., Cornell University, Engineering Physics – M.S., Ph.D., Stanford University, Aeronautics and Astronautics • With Jet Propulsion Laboratory, Caltech, since 1977 – Various program management, line management, and technical analysis responsibilities in space navigation and mission design – Currently, Principal Engineer, Mission Design & Navigation Section • Associate Editor of – Journal of Guidance, Control, and Dynamics, 1983-1990 – Journal of the Astronautical Sciences, 1980-1983 • Technical committee member – American Astronautical Society (AAS) Space Flight Mechanics Committee, 1980-1997; Chairman, 1993-1995 – AIAA Astrodynamics Technical Committee, 1985-1988; Chairman, 1986-1988 • Associate Fellow, AIAA; Senior Member, AAS and IEEE LJW - 3 Information about Speaker (Cont’d) • Author or coauthor of 70+ journal articles or conference papers on space navigation, trajectory optimization, or control theory • Pertinent recent publications include – Wood, L. J., “Interplanetary Navigation,” Encyclopedia of Aerospace Engineering, Vol. 5, edited by R. Blockley and W. Shyy, John Wiley & Sons, Ltd., Chichester, UK, 2010, pp. 3071-3084. – Wood, L. J., “The Evolution of Deep Space Navigation: 1989-1999,” in Advances in the Astronautical Sciences: The F. Landis Markley Astronautics Symposium, Vol. 132, edited by J. L. Crassidis, et al., Univelt, San Diego, 2008, pp. 877-898. – Wood, L.