Seasonal Seismic Activity on Mars, V 3.1.5, Last Saved 15/02/2021 16:44:00 ZENODO Documentation Copy

Total Page:16

File Type:pdf, Size:1020Kb

Seasonal Seismic Activity on Mars, V 3.1.5, Last Saved 15/02/2021 16:44:00 ZENODO Documentation Copy Knapmeyer et al., Seasonal Seismic Activity on Mars, v 3.1.5, last saved 15/02/2021 16:44:00 ZENODO documentation copy Seasonal Seismic Activity on Mars M. Knapmeyera, S. C. Stählerb, I. Daubarc, F. Forgetd, A. Spigad, T. Pierrond, M. van Drielb, D. Banfielde, E. Haubera, M. Grotta, N. Müllera, C. Perrinp, A. Jacobf, A. Lucasf, B. Knapmeyer-Endrung, C. Newmanh, M. P. Panningi, R. C. Weberj, F. J. Calefi, M. Böseb,r, S. Ceylanb, C. Charalambousk, J. Clintonr, N. Dah- menb, D. Giardinib, A. Horlestonl, T. Kawamuraf, A. Khanb, G. Mainsantq, M. Plasmanf, M. Lemmonn, R. Lorenzo, W. T. Pikek, J.-R. Scholzm, P. Lognonnéf, B. Banerdti Corresponding Author: Martin Knapmeyer DLR Institute for Planetary Research Rutherfordstr. 2 12489 Berlin [email protected] phone: 0049-30-67055394 Affiliations: a Institute of Planetary Research, DLR, Rutherfordstr. 2, 12489 Berlin, Germany. b Institute of Geophysics, ETH Zürich, Sonneggstrasse 5, 8092 Zürich, Switzerland c Department of Earth, Environmental, and Planetary Sciences, Brown University, Campus Box 1846, Provi- dence, RI 02912-1846, USA d Laboratoire de Météorologie Dynamique / Institut Pierre Simon Laplace (LMD/IPSL), Sorbonne Université, Centre National de la Recherche Scientifique (CNRS), École Polytechnique, École Normale Supérieure, France e Cornell University, Cornell Center for Astrophysics and Planetary Science, Ithaca, NY, 14853, USA f Université de Paris, Institut de physique du globe de Paris, CNRS, F-75005 Paris, France g Bensberg Observatory, University of Cologne, Vinzenz-Pallotti-Str. 26, 51429 Bergisch Gladbach, Germany h Aeolis Research, 333 N Dobson Road, Unit 5, Chandler AZ 85224-4412, USA i Jet Propulsion Laboratory, California Institute of Technology; 4800 Oak Grove Dr., M/S 183-301, Pasadena, CA 91109, USA j NASA MSFC, NSSTC Mail Code ST13, 320 Sparkman Drive, Huntsville, AL 35805, USA k Department of Electrical and Electronic Engineering, Imperial College London, South Kensington Campus, London, SW7 2AZ, United Kingdom l School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol BS8 1RJ, UK m Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany n Space Science Institute, 4765 Walnut Street, Suite B, Boulder, CO 80301, USA o Johns Hopkins Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA p Laboratoire de Planétologie et Géodynamique, UMR6112, OSUNA UMS3271, Univ. Nantes, Univ. Angers, CNRS, 2 rue de la Houssinière, BP 92208, 44322 Nantes Cedex 3, France q Institut Supérieur de l'Aéronautique et de l'Espace SUPAERO, 10 Avenue Edouard Belin, 31400 Toulouse, France r Swiss Seismological Service (SED), ETH Zurich, Sonneggstr. 5, 8092 Zurich, Switzerland page 1 of 2 Knapmeyer et al., Seasonal Seismic Activity on Mars, v 3.1.5, last saved 15/02/2021 16:44:00 ZENODO documentation copy About this Document This document contains the paper highlights, graphical abstract, main manuscript, and supplemental information of the paper "Seasonal Seismic Activity on Mars" as submitted to Earth and Planetary Science Letters on 15. February 2021. Highlights: • InSight SEIS finds seasonal variations of "High Frequency" type Marsquake occurrence • Likely driving forces are solar illumination, solar tides, or the CO2 ice cycle • No relation to the orbital periods of Phobos and related tides is found Graphical Abstract page 2 of 2 Knapmeyer et al., Seasonal Seismic Activity on Mars, v 3.1.209, last saved 15/02/2021 09:46:00 For submission to EPSL 1 Seasonal Seismic Activity on Mars 2 M. Knapmeyera, S. C. Stählerb, I. Daubarc, F. Forgetd, A. Spigad, T. Pierrond, M. van Drielb, D. Banfielde, 3 E. Haubera, M. Grotta, N. Müllera, C. Perrinp, A. Jacobf, A. Lucasf, B. Knapmeyer-Endrung, C. Newmanh, 4 M. P. Panningi, R. C. Weberj, F. J. Calefi, M. Böseb,r, S. Ceylanb, C. Charalambousk, J. Clintonr, N. Dah- 5 menb, D. Giardinib, A. Horlestonl, T. Kawamuraf, A. Khanb, G. Mainsantq, M. Plasmanf, M. Lemmonn, R. 6 Lorenzo, W. T. Pikek, J.-R. Scholzm, P. Lognonnéf, B. Banerdti 7 Corresponding Author: 8 Martin Knapmeyer 9 DLR Institute for Planetary Research 10 Rutherfordstr. 2 11 12489 Berlin 12 [email protected] 13 phone: 0049-30-67055394 14 Affiliations: 15 a Institute of Planetary Research, DLR, Rutherfordstr. 2, 12489 Berlin, Germany. 16 b Institute of Geophysics, ETH Zürich, Sonneggstrasse 5, 8092 Zürich, Switzerland 17 c Department of Earth, Environmental, and Planetary Sciences, Brown University, Campus Box 1846, Provi- 18 dence, RI 02912-1846, USA 19 d Laboratoire de Météorologie Dynamique / Institut Pierre Simon Laplace (LMD/IPSL), Sorbonne Université, 20 Centre National de la Recherche Scientifique (CNRS), École Polytechnique, École Normale Supérieure, France 21 e Cornell University, Cornell Center for Astrophysics and Planetary Science, Ithaca, NY, 14853, USA 22 f Université de Paris, Institut de physique du globe de Paris, CNRS, F-75005 Paris, France 23 g Bensberg Observatory, University of Cologne, Vinzenz-Pallotti-Str. 26, 51429 Bergisch Gladbach, Germany 24 h Aeolis Research, 333 N Dobson Road, Unit 5, Chandler AZ 85224-4412, USA 25 i Jet Propulsion Laboratory, California Institute of Technology; 4800 Oak Grove Dr., M/S 183-301, Pasadena, 26 CA 91109, USA 27 j NASA MSFC, NSSTC Mail Code ST13, 320 Sparkman Drive, Huntsville, AL 35805, USA 28 k Department of Electrical and Electronic Engineering, Imperial College London, South Kensington Campus, 29 London, SW7 2AZ, United Kingdom 30 l School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol BS8 1RJ, UK 31 m Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany page 1 of 39 Knapmeyer et al., Seasonal Seismic Activity on Mars, v 3.1.209, last saved 15/02/2021 09:46:00 For submission to EPSL 32 n Space Science Institute, 4765 Walnut Street, Suite B, Boulder, CO 80301, USA 33 o Johns Hopkins Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA 34 p Laboratoire de Planétologie et Géodynamique, UMR6112, OSUNA UMS3271, Univ. Nantes, Univ. Angers, 35 CNRS, 2 rue de la Houssinière, BP 92208, 44322 Nantes Cedex 3, France 36 q Institut Supérieur de l'Aéronautique et de l'Espace SUPAERO, 10 Avenue Edouard Belin, 31400 Toulouse, 37 France 38 r Swiss Seismological Service (SED), ETH Zurich, Sonneggstr. 5, 8092 Zurich, Switzerland 39 page 2 of 39 Knapmeyer et al., Seasonal Seismic Activity on Mars, v 3.1.209, last saved 15/02/2021 09:46:00 For submission to EPSL 40 Abstract 41 The activity of High Frequency (HF) marsquakes, as recorded by InSight at Homestead Hollow, Elysium 42 Planitia, increased after about 퐿푆 = 33°, and ceased almost completely by 퐿푆 = 187°, following an ap- 43 parently seasonal variation with a peak rate near aphelion. We define seismic rate models based on the 44 declination of the Sun, annual solar tides, and the annual CO2 cycle as measured by atmospheric pres- 45 sure. Evaluation of Akaike weights and evidence ratios shows that the declination of the Sun is the most 46 likely, and the CO2 cycle the least likely driver of this seismic activity, although the discrimination is weak, 47 and the occurrence of a few events in August 2020 is in favor for a triggering by CO2 ice load. We also 48 show that no periodicity related to Phobos’ orbit is present in the HF event sequence. Event rate fore- 49 casts are presented to allow further discrimination of candidate mechanisms from future observations. 50 Keywords: 51 Mars 52 Elysium Planitia 53 InSight 54 Seasonal Seismic Activity 55 Phobos 56 page 3 of 39 Knapmeyer et al., Seasonal Seismic Activity on Mars, v 3.1.209, last saved 15/02/2021 09:46:00 For submission to EPSL 57 1. Introduction 58 NASA’s InSight (Interior exploration using Seismic Investigations, Geodesy, and Heat Transport) mis- 59 sion, launched in May 2018, landed at a site in the western part of Elysium Planitia, about 500 km to the 60 north of the dichotomy boundary. The landing site is 1500 km west of Cerberus Fossae, which was sus- 61 pected to be seismically active by Taylor et al. (2013). After the touchdown on 26. Nov. 2018, deploy- 62 ment of the seismometer experiment SEIS (Seismic Experiment for Interior Structure; Lognonné et al., 63 2019, 2020) was completed on sol 70 (the 70th Martian day of the mission). SEIS started continuous re- 64 cording on sol 73 (09. Feb. 2019), and reached full performance on sol 85 (21. Feb. 2019, Banerdt et al., 65 2020). With the exception of a downtime from 28. Aug. 2019 to 18. Sep. 2019 (sol 267 to 288; due to a 66 minor problem in power management, which was extended to three weeks duration by the solar con- 67 junction), and a few smaller data losses due to downlink interruptions, SEIS has been recording seismic 68 data continuously ever since. 69 Estimates of the seismic activity of Mars published prior to the InSight mission basically assumed that 70 marsquakes would occur in the same fashion as earthquakes: according to a Gutenberg-Richter distribu- 71 tion in size, and randomly in time (Phillips, 1991, Knapmeyer et al., 2006, Taylor et al., 2013, Plesa et al., 72 2018, and references therein). A certain class of events (High Frequency (HF) and 2.4Hz events, the latter 73 being small HF events visible only by their excitation of an ambient resonance at 2.4 Hz, Clinton et al., 74 2020), however exhibits an occurrence rate that appears variable in time, as shown in Figure 1 (which we 75 first mentioned in Giardini et al., 2020). We interpret the timing of these events as result of a nonsta- 76 tionary Poisson process (supplemental text S6), and compare it with several time-varying processes in 77 order to identify what might drive the nonstationarity.
Recommended publications
  • Scientific Rationale and Requirements for a Global Seismic Network on Mars
    SCIENTIFIC RATIONALE AND REQUIREMENTS FOR A GLOBAL SEISMIC NETWORK ON MARS MARS Model AR 90 EARTH 180 (NASA-CR-188806) SCIENTIFIC RATIONALE AND N92-14949 REQUIREMENTS FOR A GLOBAL SEISMIC NETWORK ON MARS (Lunar and Planetary Inst.) 48 p CSCL 03B Unclas G3/91 0040098 LPI Technical Report Number 91-02 LUNAR AND PLANETARY INSTITUTE 3303 NASA ROAD 1 HOUSTON TX 77058-4399 LPI/TR-91-02 SCIENTIFIC RATIONALE AND REQUIREMENTS FOR A GLOBAL SEISMIC NETWORK ON MARS Sean C. Solomon, Don L. Anderson, W. Bruce Banerdt, Rhett G. Butler, Paul M. Davis, Frederick K. Duennebier, Yosio Nakamura, Emile A. Okal, and Roger J. Phillips Report of a Workshop Held at Morro Bay, California May 7-9, 1990 Lunar and Planetary Institute 3303 NASA Road 1 Houston TX 77058 LPI Technical Report Number 91-02 LPI/TR-91-02 Compiled in 1991 by the LUNAR AND PLANETARY INSTITUTE The Institute is operated by Universities Space Research Association under Contract NASW-4574 with the National Aeronautics and Space Administration. Material in this document may be copied without restraint for library, abstract service, educational, or personal research purposes; however, republication of any portion requires the written permission of the authors as well as appropriate acknowledgment of this publication. This report may be cited as: Solomon S. C. et al. (1991) Scientific Rationale and Requirements far a Global Seismic Network on Mars. LPI Tech. Rpt. 91-02, Lunar and Planetary Institute, Houston. 51 pp. This report is distributed by: ORDER DEPARTMENT Lunar and Planetary Institute 3303 NASA Road 1 Houston TX 77058-4399 Mail order requestors will be invoiced for the cost of shipping and handling.
    [Show full text]
  • Bibliographyof Space Books Andarticlesfrom Non
    https://ntrs.nasa.gov/search.jsp?R=19800016707N 2020-03-11T18:02:45+00:00Zi_sB--rM-._lO&-{/£ 3 1176 00167 6031 HHR-51 NASA-TM-81068 ]9800016707 BibliographyOf Space Books And ArticlesFrom Non-AerospaceJournals 1957-1977 _'C>_.Ft_iEFERENC_ I0_,'-i p,,.,,gvi ,:,.2, , t ,£}J L,_:,._._ •..... , , .2 ,IFER History Office ...;_.o.v,. ._,.,- NASA Headquarters Washington, DC 20546 1979 i HHR-51 BIBLIOGRAPHYOF SPACEBOOKS AND ARTICLES FROM NON-AEROSPACE JOURNALS 1957-1977 John J. Looney History Office NASA Headquarters Washlngton 9 DC 20546 . 1979 For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D.C. 20402 Stock Number 033-000-0078t-1 Kc6o<2_o00 CONTENTS Introduction.................................................... v I. Space Activity A. General ..................................................... i B. Peaceful Uses ............................................... 9 C. Military Uses ............................................... Ii 2. Spaceflight: Earliest Times to Creation of NASA ................ 19 3. Organlzation_ Admlnlstration 9 and Management of NASA ............ 30 4. Aeronautics..................................................... 36 5. BoostersandRockets............................................ 38 6. Technology of Spaceflight....................................... 45 7. Manned Spaceflight.............................................. 77 8. Space Science A. Disciplines Other than Space Medicine ....................... 96 B. Space Medicine ..............................................119 C.
    [Show full text]
  • Massachusetts Inst. of Thch.) 666 P HC A9NATIF A0L AEOA, CSCD 03F Unclas
    lo2 to the " NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Contract NAS9-12334 -APOLLOPASSIVE SEISMICEXPERIMENT PARTICIPATION 'I NASA-CR-151882) LUNAR SEISMOLOGY: THE 1479-17782 INTERNAL STRUCTURE ORHE LOt Ph. Thesis (Massachusetts Inst. of Thch.) 666 p HC A9NATIF A0L AEOA, CSCD 03f Unclas 1 Januarya-19-12 -o 3.0 September .1978 G3/91' 1351 0 M. Nafi Toksbz- Principal Investigator Department of Earth and Planetar SciencesO Massachusetts Institute of Technology Cambridge, Massachusetts 02139 LUNAR SEISMOLOGY: THE INTERNAL STRUCTURE OF THE MOON by -Neal Rodney Goins Submitted to the Department of-Earth -and Planetary Sciences on May 24,.1978, in parti&l .flfillment of the requirements for the degree of Doctor of Philosophy.. ABSTRACT, A primary goal of-the Apollo missions was the exploration and scientific study of the moon. The nature of the lunar interior is of particular interest for comparison with the earth and in studying comparative planetology. The principal experiment designed to study the lunar interior was the passive seismic experiment (PSE) included as part of the science package on missions 12, 14, 15, and 16. Thus seis­ mologists were provided with a uniqueopportunity ta study the seismicity and seismic characteristics of a second planetary 'bdy and ascertain if analysis methods developed on earth could illuminate the structure of the lunar interior. The lunar seismic data differ from terrestrial data in three major respects. First, the seismic sources are much smaller than on earth, so that no significant information has -been yet obtained for the 4v/ry deep lunar interior. Second, a strong, high Q scattering layer exists on the surface of the moon, resulting in very emergent seismic arrivals, long ringing-codas that obscure secondary (later arriving)-phases., and 'the-destruction of coherent dispersed surface wave trains.
    [Show full text]
  • The Moon and Eclipses
    Lecture 10 The Moon and Eclipses Jiong Qiu, MSU Physics Department Guiding Questions 1. Why does the Moon keep the same face to us? 2. Is the Moon completely covered with craters? What is the difference between highlands and maria? 3. Does the Moon’s interior have a similar structure to the interior of the Earth? 4. Why does the Moon go through phases? At a given phase, when does the Moon rise or set with respect to the Sun? 5. What is the difference between a lunar eclipse and a solar eclipse? During what phases do they occur? 6. How often do lunar eclipses happen? When one is taking place, where do you have to be to see it? 7. How often do solar eclipses happen? Why are they visible only from certain special locations on Earth? 10.1 Introduction The moon looks 14% bigger at perigee than at apogee. The Moon wobbles. 59% of its surface can be seen from the Earth. The Moon can not hold the atmosphere The Moon does NOT have an atmosphere and the Moon does NOT have liquid water. Q: what factors determine the presence of an atmosphere? The Moon probably formed from debris cast into space when a huge planetesimal struck the proto-Earth. 10.2 Exploration of the Moon Unmanned exploration: 1950, Lunas 1-3 -- 1960s, Ranger -- 1966-67, Lunar Orbiters -- 1966-68, Surveyors (first soft landing) -- 1966-76, Lunas 9-24 (soft landing) -- 1989-93, Galileo -- 1994, Clementine -- 1998, Lunar Prospector Achievement: high-resolution lunar surface images; surface composition; evidence of ice patches around the south pole.
    [Show full text]
  • WILLIAM MAURICE EWING May 12, 1906-May 4, 1974
    NATIONAL ACADEMY OF SCIENCES WILLIAM MAURICE Ew ING 1906—1974 A Biographical Memoir by ED W A R D C . B ULLARD Any opinions expressed in this memoir are those of the author(s) and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 1980 NATIONAL ACADEMY OF SCIENCES WASHINGTON D.C. WILLIAM MAURICE EWING May 12, 1906-May 4, 1974 BY EDWARD C. BULLARD* CHILDHOOD, 1906-1922 ILLIAM MAURICE EWING was born on May 12, 1906 in W Lockney, a town of about 1,200 inhabitants in the Texas panhandle. He rarely used the name William and was always known as Maurice. His paternal great-grandparents moved from Kentucky to Livingston County, Missouri, at some date before 1850. Their son John Andrew Ewing, Maurice's grandfather, fought for the Confederacy in the Civil War; while in the army he met two brothers whose family had also come from Kentucky to Missouri before 1850 and were living in De Kalb County. Shortly after the war he married their sister Martha Ann Robinson. Their son Floyd Ford Ewing, Maurice's father, was born in Clarkdale, Mis- souri, in 1879. In 1889 the family followed the pattern of the times and moved west to Lockney, Texas. Floyd Ewing was a gentle, handsome man with a liking for literature and music, whom fate had cast in the unsuitable roles of cowhand, dryland farmer, and dealer in hardware and farm implements. Since he kept his farm through the *This memoir is a corrected and slightly amplified version of one published by the Royal Society in their Biographical Memoirs (21:269-311, 1975).
    [Show full text]
  • Apollo 17 Press
    7A-/ a NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Washington. D . C . 20546 202-755-8370 FOR RELEASE: Sunday t RELEASE NO: 72-220K November 26. 1972 B PROJECT: APOLLO 17 (To be launched no P earlier than Dec . 6) R E contents 1-5 6-13 U APOLLC 17 MISSION OBJECTIVES .............14 LAUNCH OPERATIONS .................. 15-17 COUNTDOWN ....................... 18-21 Launch Windows .................. 20 3 Ground Elapsed Time Update ............ 20-21 LAUNCH AND MISSION PROFILE .............. 22-32 Launch Events .................. 24-26 Mission Events .................. 26-28 EVA Mission Events ................ 29-32 APOLLO 17 LANDING SITE ................ 33-36 LUNAR SURFACE SCIENCE ................ 37-55 S-IVB Lunar Impact ................ 37 ALSEP ...................... 37 K SNAP-27 ..................... 38-39 Heat Flow Experiment ............... 40 Lunar Ejecta and Meteorites ........... 41 Lunar Seismic Profiling ............. 41-42 I Lunar Atmospheric Composition Experiment ..... 43 Lunar Surface Gravimeter ............. 43-44 Traverse Gravimeter ............... 44-45 Surface Electrical Properties 45 I-) .......... T Lunar Neutron Probe ............... 46 1 Soil Mechanics .................. 46-47 Lunar Geology Investigation ........... 48-51 Lunar Geology Hand Tools ............. 52-54 Long Term Surface Exposure Experiment ...... 54-55 -more- November 14. 1972 i2 LUNAR ORBITAL SCIENCE ............... .5 6.61 Lunar Sounder ................. .5 6.57 Infrared Scanning Radiometer ......... .5 7.58 Far-Ultraviolet Spectrometer ..........5
    [Show full text]
  • Sources of Extraterrestrial Rare Earth Elements: to the Moon and Beyond
    resources Article Sources of Extraterrestrial Rare Earth Elements: To the Moon and Beyond Claire L. McLeod 1,* and Mark. P. S. Krekeler 2 1 Department of Geology and Environmental Earth Sciences, 203 Shideler Hall, Miami University, Oxford, OH 45056, USA 2 Department of Geology and Environmental Earth Science, Miami University-Hamilton, Hamilton, OH 45011, USA; [email protected] * Correspondence: [email protected]; Tel.: 513-529-9662; Fax: 513-529-1542 Received: 10 June 2017; Accepted: 18 August 2017; Published: 23 August 2017 Abstract: The resource budget of Earth is limited. Rare-earth elements (REEs) are used across the world by society on a daily basis yet several of these elements have <2500 years of reserves left, based on current demand, mining operations, and technologies. With an increasing population, exploration of potential extraterrestrial REE resources is inevitable, with the Earth’s Moon being a logical first target. Following lunar differentiation at ~4.50–4.45 Ga, a late-stage (after ~99% solidification) residual liquid enriched in Potassium (K), Rare-earth elements (REE), and Phosphorus (P), (or “KREEP”) formed. Today, the KREEP-rich region underlies the Oceanus Procellarum and Imbrium Basin region on the lunar near-side (the Procellarum KREEP Terrain, PKT) and has been tentatively estimated at preserving 2.2 × 108 km3 of KREEP-rich lithologies. The majority of lunar samples (Apollo, Luna, or meteoritic samples) contain REE-bearing minerals as trace phases, e.g., apatite and/or merrillite, with merrillite potentially contributing up to 3% of the PKT. Other lunar REE-bearing lunar phases include monazite, yittrobetafite (up to 94,500 ppm yttrium), and tranquillityite (up to 4.6 wt % yttrium, up to 0.25 wt % neodymium), however, lunar sample REE abundances are low compared to terrestrial ores.
    [Show full text]
  • Lunar Seismology: an Update on Interior Structure Models
    Space Science Reviews manuscript No. (will be inserted by the editor) Lunar seismology: An update on interior structure models Raphael F. Garcia · Amir Khan · M´elanie Drilleau · Ludovic Margerin · Taichi Kawamura · Daoyuan Sun · Mark A. Wieczorek · Attilio Rivoldini · Ceri Nunn · Renee C. Weber · Angela G. Marusiak · Philippe Lognonn´e · Yosio Nakamura · Peimin Zhu Received: date / Accepted: date R. F. Garcia (corresponding author) Institut Sup´erieurde l'A´eronautiqueet de l'Espace (ISAE-SUPAERO), Universit´ede Toulouse, 10 Ave E. Belin 31400 Toulouse, France Tel.: +33-561338114 E-mail: [email protected] Institut de Recherche en Astrophysique et Plan´etologie,C.N.R.S., Universit´ede Toulouse, 14 Ave E. Belin, 31400 Toulouse, France A. Khan Institute of Geophysics, ETH Z¨urich, Switzerland. M. Drilleau Universit de Paris, Institut de physique du globe de Paris, CNRS, F-75005 Paris, France L. Margerin Institut de Recherche en Astrophysique et Plan´etologie,C.N.R.S., Universit´ede Toulouse, 14 Ave E. Belin, 31400 Toulouse, France T. Kawamura Institut de Physique du Globe de Paris, Paris, France D. Sun Laboratory of Seismology and Physics of Earths Interior, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China CAS Center for Excellence in Comparative Planetology, Hefei, China M. A. Wieczorek Universit´eC^oted'Azur, Observatoire de la C^oted'Azur, CNRS, Laboratoire Lagrange, Nice, France A. Rivoldini Observatoire Royal de Belgique, 3 Avenue Circulaire, 1050 Bruxelles, Belgique C. Nunn Jet Propulsion Laboratory - California Institute of Technology, Pasadena, U.S.A and Ludwig Maximilian University, Munich, Germany R. C.
    [Show full text]
  • Jet Propulsion Laboratory Publications Collection
    Jet Propulsion Laboratory Publications Collection Paul Silbermann 1999 National Air and Space Museum Archives 14390 Air & Space Museum Parkway Chantilly, VA 20151 [email protected] https://airandspace.si.edu/archives Table of Contents Collection Overview ........................................................................................................ 1 Administrative Information .............................................................................................. 1 Historical Note ................................................................................................................ 1 Citations........................................................................................................................... 2 Series Organization.......................................................................................................... 2 Scope and Content Note ................................................................................................ 2 Names and Subjects ...................................................................................................... 3 Container Listing ............................................................................................................. 4 Series 1: Combined Bimonthly Summaries, 1947-1954........................................... 4 Series 2: 1- Prefix Publications, 1950-1952............................................................. 7 Series 3: 4- Prefix Publications, 1947-1949............................................................
    [Show full text]
  • 太空|TAIKONG 国际空间科学研究所 - 北京 ISSI-BJ Magazine No
    太空|TAIKONG 国际空间科学研究所 - 北京 ISSI-BJ Magazine No. 10 June 2018 LUNAR AND PLANETARY SEISMOLOGY IMPRINT FOREWORD 太空 | TAIKONG In the last few years, during different planetary seismology. Especially ISSI-BJ Magazine meetings, discussions took place on since although the data available possible international cooperation dates back from the Apollo missions on planetary science, especially in the 70s, and there are several Address: No.1 Nanertiao, in the field of lunar seismology. papers reviewing past results on Zhongguancun, Haidian District, These discussions were related lunar seismology, the ISSI-BJ forum, Beijing, China to the possibility of joint scientific however, was rather to focus on the Postcode: 100190 experiments on Chinese lunar prospects of new science and future Phone: +86-10-62582811 Website: www.issibj.ac.cn missions or European space projects. programs, as there is still much It was subsequently suggested that to do in terms of new science. In Authors the scientists who are interested this sense, the proposed topic has in this topic should have closer a very high added value for ISSI- Philippe Lognonné (IPGP, France), Wing Huen Ip (NCU, GIA, Taiwan), contacts to pave the way for future BJ, especially with the success of Yosio Nakamura (UTIG, USA), collaboration when the opportunities Chang’e-3, and even more for the Wang Yanbin (SESS, PKU, China), Mark Wieczorek (LAGRANGE/ arise. With this in mind, the ISSI-BJ future Chinese Lunar/Planetary OCA, France) Executive Director, Prof. Maurizio missions, which may consider having William Bruce Banerdt (JPL/ Falanga, has been invited to visit Prof. such instruments onboard. The ISSI- Caltech, USA), Raphael Garcia Ip Wing Huen at the National Central BJ Science committee members (ISAE/SUPAERO, France), Patrick Gaulme (MPS/MPG, Germany), University, and, subsequently, he have positively recommended the Jan Harms (GSSI, Italy), Heiner visited Prof.
    [Show full text]
  • Humanity and Space
    P a g e | 1 HUMANITY AND SPACE AN INTERACTIVE QUALIFYING PROJECT SUBMITTED TO THE WORCESTER POLYTECHNIC INSTITUTE In Partial Fulfillment for the Degree of Bachelor Science By James Miguel Costello Nicola Richard DiLibero III George Howard Merry Submitted to: Professor Mayer Humi P a g e | 2 CONTENTS Abstract ......................................................................................................................................................... 3 Executive Summary ...................................................................................................................................... 4 Introduction.................................................................................................................................................... 6 Moon Base .................................................................................................................................................. 13 Background ......................................................................................................................................... 13 Introduction .......................................................................................................................................... 15 Why Go Back? .................................................................................................................................... 16 Lunar Radiation ................................................................................................................................... 19 Lunar Base
    [Show full text]
  • The Lunar Moho and the Internal Structure of the Moon: a Geophysical Perspective
    Tectonophysics 609 (2013) 331–352 Contents lists available at ScienceDirect Tectonophysics journal homepage: www.elsevier.com/locate/tecto Review Article The lunar moho and the internal structure of the Moon: A geophysical perspective A. Khan a,⁎, A. Pommier b, G.A. Neumann c, K. Mosegaard d a Institute of Geochemistry and Petrology, Swiss Federal Institute of Technology, Zürich, Switzerland b School of Earth and Space Exploration, Arizona State University, Tempe, USA c NASA Goddard Space Flight Center, Greenbelt, MD, USA d Department of Informatics and Mathematical Modelling, Technical University of Denmark, Lyngby, Denmark article info abstract Article history: Extraterrestrial seismology saw its advent with the deployment of seismometers during the Apollo missions Received 2 May 2012 that were undertaken from July 1969 to December 1972. The Apollo lunar seismic data constitute a unique Received in revised form 7 February 2013 resource being the only seismic data set which can be used to infer the interior structure of a planetary Accepted 14 February 2013 body besides the Earth. On-going analysis and interpretation of the seismic data continues to provide con- Available online 24 February 2013 straints that help refine lunar origin and evolution. In addition to this, lateral variations in crustal thickness (~0–80 km) are being mapped out at increasing resolution from gravity and topography data that have Keywords: Lunar seismology and continue to be collected with a series of recent lunar orbiter missions. Many of these also carry onboard Crustal thickness multi-spectral imaging equipment that is able to map out major-element concentration and surface mineral- Lunar structure and composition ogy to high precision.
    [Show full text]