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Arxiv:2003.06799V2 [Astro-Ph.EP] 6 Feb 2021
Thomas Ruedas1,2 Doris Breuer2 Electrical and seismological structure of the martian mantle and the detectability of impact-generated anomalies final version 18 September 2020 published: Icarus 358, 114176 (2021) 1Museum für Naturkunde Berlin, Germany 2Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany arXiv:2003.06799v2 [astro-ph.EP] 6 Feb 2021 The version of record is available at http://dx.doi.org/10.1016/j.icarus.2020.114176. This author pre-print version is shared under the Creative Commons Attribution Non-Commercial No Derivatives License (CC BY-NC-ND 4.0). Electrical and seismological structure of the martian mantle and the detectability of impact-generated anomalies Thomas Ruedas∗ Museum für Naturkunde Berlin, Germany Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany Doris Breuer Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany Highlights • Geophysical subsurface impact signatures are detectable under favorable conditions. • A combination of several methods will be necessary for basin identification. • Electromagnetic methods are most promising for investigating water concentrations. • Signatures hold information about impact melt dynamics. Mars, interior; Impact processes Abstract We derive synthetic electrical conductivity, seismic velocity, and density distributions from the results of martian mantle convection models affected by basin-forming meteorite impacts. The electrical conductivity features an intermediate minimum in the strongly depleted topmost mantle, sandwiched between higher conductivities in the lower crust and a smooth increase toward almost constant high values at depths greater than 400 km. The bulk sound speed increases mostly smoothly throughout the mantle, with only one marked change at the appearance of β-olivine near 1100 km depth. -
PROJECT PENGUIN Robotic Lunar Crater Resource Prospecting VIRGINIA POLYTECHNIC INSTITUTE & STATE UNIVERSITY Kevin T
PROJECT PENGUIN Robotic Lunar Crater Resource Prospecting VIRGINIA POLYTECHNIC INSTITUTE & STATE UNIVERSITY Kevin T. Crofton Department of Aerospace & Ocean Engineering TEAM LEAD Allison Quinn STUDENT MEMBERS Ethan LeBoeuf Brian McLemore Peter Bradley Smith Amanda Swanson Michael Valosin III Vidya Vishwanathan FACULTY SUPERVISOR AIAA 2018 Undergraduate Spacecraft Design Dr. Kevin Shinpaugh Competition Submission i AIAA Member Numbers and Signatures Ethan LeBoeuf Brian McLemore Member Number: 918782 Member Number: 908372 Allison Quinn Peter Bradley Smith Member Number: 920552 Member Number: 530342 Amanda Swanson Michael Valosin III Member Number: 920793 Member Number: 908465 Vidya Vishwanathan Dr. Kevin Shinpaugh Member Number: 608701 Member Number: 25807 ii Table of Contents List of Figures ................................................................................................................................................................ v List of Tables ................................................................................................................................................................vi List of Symbols ........................................................................................................................................................... vii I. Team Structure ........................................................................................................................................................... 1 II. Introduction .............................................................................................................................................................. -
South Pole-Aitken Basin
Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole. -
2010-2011 Science Planning Summaries
Find information about current Link to project web sites and USAP projects using the find information about the principal investigator, event research and people involved. number station, and other indexes. Science Program Indexes: 2010-2011 Find information about current USAP projects using the Project Web Sites principal investigator, event number station, and other Principal Investigator Index indexes. USAP Program Indexes Aeronomy and Astrophysics Dr. Vladimir Papitashvili, program manager Organisms and Ecosystems Find more information about USAP projects by viewing Dr. Roberta Marinelli, program manager individual project web sites. Earth Sciences Dr. Alexandra Isern, program manager Glaciology 2010-2011 Field Season Dr. Julie Palais, program manager Other Information: Ocean and Atmospheric Sciences Dr. Peter Milne, program manager Home Page Artists and Writers Peter West, program manager Station Schedules International Polar Year (IPY) Education and Outreach Air Operations Renee D. Crain, program manager Valentine Kass, program manager Staffed Field Camps Sandra Welch, program manager Event Numbering System Integrated System Science Dr. Lisa Clough, program manager Institution Index USAP Station and Ship Indexes Amundsen-Scott South Pole Station McMurdo Station Palmer Station RVIB Nathaniel B. Palmer ARSV Laurence M. Gould Special Projects ODEN Icebreaker Event Number Index Technical Event Index Deploying Team Members Index Project Web Sites: 2010-2011 Find information about current USAP projects using the Principal Investigator Event No. Project Title principal investigator, event number station, and other indexes. Ainley, David B-031-M Adelie Penguin response to climate change at the individual, colony and metapopulation levels Amsler, Charles B-022-P Collaborative Research: The Find more information about chemical ecology of shallow- USAP projects by viewing individual project web sites. -
2020-2021 Science Planning Summaries
Project Indexes Find information about projects approved for the 2020-2021 USAP field season using the available indexes. Project Web Sites Find more information about 2020-2021 USAP projects by viewing project web sites. More Information Additional information pertaining to the 2020-2021 Field Season. Home Page Station Schedules Air Operations Staffed Field Camps Event Numbering System 2020-2021 USAP Field Season Project Indexes Project Indexes Find information about projects approved for the 2020-2021 USAP field season using the USAP Program Indexes available indexes. Astrophysics and Geospace Sciences Dr. Robert Moore, Program Director Project Web Sites Organisms and Ecosystems Dr. Karla Heidelberg, Program Director Find more information about 2020-2021 USAP projects by Earth Sciences viewing project web sites. Dr. Michael Jackson, Program Director Glaciology Dr. Paul Cutler, Program Director More Information Ocean and Atmospheric Sciences Additional information pertaining Dr. Peter Milne, Program Director to the 2020-2021 Field Season. Integrated System Science Home Page TBD Station Schedules Antarctic Instrumentation & Research Facilities Air Operations Dr. Michael Jackson, Program Director Staffed Field Camps Education and Outreach Event Numbering System Ms. Elizabeth Rom; Program Director USAP Station and Vessel Indexes Amundsen-Scott South Pole Station McMurdo Station Palmer Station RVIB Nathaniel B. Palmer ARSV Laurence M. Gould Special Projects Principal Investigator Index Deploying Team Members Index Institution Index Event Number Index Technical Event Index Other Science Events Project Web Sites 2020-2021 USAP Field Season Project Indexes Project Indexes Find information about projects approved for the 2020-2021 USAP field season using the Project Web Sites available indexes. Principal Investigator/Link Event No. -
Systematics and Consequences of Comet Nucleus Outgassing Torques
Systematics and Consequences of Comet Nucleus Outgassing Torques David Jewitt1;2 1Department of Earth, Planetary and Space Sciences, UCLA, 595 Charles Young Drive East, Los Angeles, CA 90095-1567 2Department of Physics and Astronomy, University of California at Los Angeles, 430 Portola Plaza, Box 951547, Los Angeles, CA 90095-1547 [email protected] Received ; accepted Revised 2021 March 17 arXiv:2103.10577v1 [astro-ph.EP] 19 Mar 2021 { 2 { ABSTRACT Anisotropic outgassing from comets exerts a torque sufficient to rapidly change the angular momentum of the nucleus, potentially leading to rotational instability. Here, we use empirical measures of spin changes in a sample of comets to characterize the torques and to compare them with expectations from a sim- ple model. Both the data and the model show that the characteristic spin-up timescale, τs, is a strong function of nucleus radius, rn. Empirically, we find that the timescale for comets (most with perihelion 1 to 2 AU and eccentricity ∼0.5) 2 varies as τs ∼ 100rn, where rn is expressed in kilometers and τs is in years. The −2 fraction of the nucleus surface that is active varies as fA ∼ 0:1rn . We find that the median value of the dimensionless moment arm of the torque is kT = 0.007 (i.e. ∼0.7% of the escaping momentum torques the nucleus), with weak (<3σ) −3 2 evidence for a size dependence kT ∼ 10 rn. Sub-kilometer nuclei have spin- up timescales comparable to their orbital periods, confirming that outgassing torques are quickly capable of driving small nuclei towards rotational disrup- tion. -
On the Effect of Magnetospheric Shielding on the Lunar Hydrogen Cycle O
On the Effect of Magnetospheric Shielding on the Lunar Hydrogen Cycle O. J. Tucker1*, W. M. Farrell1, and A. R. Poppe2 1NASA Goddard Space Flight Center, Greenbelt, Md, USA. 2Space Sciences Laboratory, University of California, Berkeley, CA, USA *Corresponding author: Orenthal Tucker ([email protected]) NASA Goddard Space Flight Center, Magnetospheric Physics/Code 695, Greenbelt, MD 20771, USA Key Points: Low latitude nightside OH is depleted from waning gibbous to waxing crescent because of shielding when traversing the magnetotail. Low latitude dayside OH is decreased in the tail compared to out but the difference cannot be resolved with current observations. Magnetospheric shielding decreases the global H2 exosphere by an order of magnitude during the full Moon. 1 Abstract The global distribution of surficial hydroxyl on the Moon is hypothesized to be derived from the implantation of solar wind protons. As the Moon traverses the geomagnetic tail it is generally shielded from the solar wind, therefore the concentration of hydrogen is expected to decrease during full Moon. A Monte Carlo approach is used to model the diffusion of implanted hydrogen atoms in the regolith as they form metastable bonds with O atoms, and the subsequent degassing of H2 into the exosphere. We quantify the expected change in the surface OH and the H2 exosphere using averaged SW proton flux obtained from the Acceleration, Reconnection, Turbulence, and Electrodynamics of the Moon’s Interaction with the Sun (ARTEMIS) measurements. At lunar local noon there is a small difference less than ~10 ppm between the surface concentrations in the tail compared to out. -
5 Escape of Atmospheres to Space
5 Escape of Atmospheres to Space So far, our discussion of atmospheric evolution has circumstances: Jeans’ escape, where individual mol- concentrated on atmosphere and climate fundamentals. ecules evaporate into a collisionless exosphere, and Climate constrains possible life and, as we will see later hydrodynamic escape, which is a bulk outflow with a in this book, the way that climate is thought to have velocity driven by atmospheric heating that induces an evolved can explain many environmental differences upward pressure gradient force (e.g., Johnson et al., between Earth, Venus, and Mars. Climate is closely tied 2013d; Walker, 1982). (ii) Suprathermal (or nonthermal) to the composition of a planet’s atmosphere, which deter- escape is where individual atoms or molecules are mines the greenhouse effect. Consequently, to understand boosted to escape velocity because of chemical reactions how climate has changed over time, we must consider or ionic interactions. Finally, (iii) impact erosion is where how atmospheric composition has evolved. In turn, we atmospheric gases are expelled en masse as a result of must examine how atmospheric gases can be lost. large body impacts, such as the cumulative effect of Gases are lost at an atmosphere’s upper and lower asteroids hits. Of these three types, nonthermal escape is boundaries: the planet’s surface and interplanetary space. generally slow because if it were fast the molecules would In this chapter, we consider the latter. Studies of the Solar collide and the escape would be in the thermal category. System have shown that some bodies are vulnerable to Theory suggests that the two mechanisms that can most atmospheric escape (Hunten, 1990). -
An Innovative Solution to NASA's NEO Impact Threat Mitigation Grand
Final Technical Report of a NIAC Phase 2 Study December 9, 2014 NASA Grant and Cooperative Agreement Number: NNX12AQ60G NIAC Phase 2 Study Period: 09/10/2012 – 09/09/2014 An Innovative Solution to NASA’s NEO Impact Threat Mitigation Grand Challenge and Flight Validation Mission Architecture Development PI: Dr. Bong Wie, Vance Coffman Endowed Chair Professor Asteroid Deflection Research Center Department of Aerospace Engineering Iowa State University, Ames, IA 50011 email: [email protected] (515) 294-3124 Co-I: Brent Barbee, Flight Dynamics Engineer Navigation and Mission Design Branch (Code 595) NASA Goddard Space Flight Center Greenbelt, MD 20771 email: [email protected] (301) 286-1837 Graduate Research Assistants: Alan Pitz (M.S. 2012), Brian Kaplinger (Ph.D. 2013), Matt Hawkins (Ph.D. 2013), Tim Winkler (M.S. 2013), Pavithra Premaratne (M.S. 2014), Sam Wagner (Ph.D. 2014), George Vardaxis, Joshua Lyzhoft, and Ben Zimmerman NIAC Program Executive: Dr. John (Jay) Falker NIAC Program Manager: Jason Derleth NIAC Senior Science Advisor: Dr. Ronald Turner NIAC Strategic Partnerships Manager: Katherine Reilly Contents 1 Hypervelocity Asteroid Intercept Vehicle (HAIV) Mission Concept 2 1.1 Introduction ...................................... 2 1.2 Overview of the HAIV Mission Concept ....................... 6 1.3 Enabling Space Technologies for the HAIV Mission . 12 1.3.1 Two-Body HAIV Configuration Design Tradeoffs . 12 1.3.2 Terminal Guidance Sensors/Algorithms . 13 1.3.3 Thermal Protection and Shield Issues . 14 1.3.4 Nuclear Fuzing Mechanisms ......................... 15 2 Planetary Defense Flight Validation (PDFV) Mission Design 17 2.1 The Need for a PDFV Mission ............................ 17 2.2 Preliminary PDFV Mission Design by the MDL of NASA GSFC . -
19890006473.Pdf
1. ASPECTS OF LITHOSPHERIC EVOLUTION ON VENUS II. THERMAL AND COLLISIONAL HISTORIES OF CHONDRITE PARENT BODIES Robert E. Grimm B.A., University of Tennessee (1 983) SUBMITTED TO THE DEPARTMENT OF EARTH, ATMOSPHERIC, AND PLANETARY SCIENCES IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY October 1988 0 Massachusetts Institute of Technology 1988 Signature of Author Department of Earth, Atmospheric, and Planetary Sciences Certified by Sean C. Solomon Thesis Supervisor Accepted by Theodore R. Madden Chairman, Department Committee LhASA-CR-le4568) PA69 1: ASEIC'IS CP N 8 9- 1f 8 4 4 I~!ZBOSP€IER~C€VCLt!IION GN VELC5. FAET 2: 1EERtlAL AhD CCLLIEICNAL HI5'lCE1EE GP CIICNDSiI'IE FAbENI tOlj1IS Ph.C. Skesis Dnclas (tassachusettr lngt- cf Tech.) 229 p G3/91 0178596 2 1. ASPECTS OF LITHOSPHERIC EVOLUTION ON VENUS II. THERMAL AND COLLISIONAL HISTORIES OF CHONDRITE PARENT BODIES Robert E. Grimm Submitted to the Department of Earth, Atmospheric, and Planetary Sciences on October 25, 1988, in partial fulfillment of the requirements of the Degree of Doctor of Philosophy in Geophysics ABSTRACT This thesis consists of two principal sections which address the geological evo- lution of distinctly different kinds of solar system objects. Venus, the second largest of the terrestrial planets, has been observed over the past decade by orbital radars on both American and Soviet spacecraft. These surface measurements provide clues to the structure and evolution of the lithosphere. The parent bodies of chon- dritic meteorites, thought to resemble asteroids, represent the other end of the size spectrum of terrestrial objects. -
Surface Properties of Asteroids from Mid-Infrared Observations and Thermophysical Modeling
Dissertation zur Erlangung des akademischen Grades Doktor der Naturwissenschaften (doctor rerum naturalium) Surface Properties of Asteroids from Mid-Infrared Observations and Thermophysical Modeling Dipl.-Phys. Michael M¨uller 2007 Eingereicht und verteidigt am Fachbereich Geowissenschaften der Freien Universit¨atBerlin. Angefertigt am Institut f¨ur Planetenforschung des Deutschen Zentrums f¨urLuft- und Raumfahrt e.V. (DLR) in Berlin-Adlershof. arXiv:1208.3993v1 [astro-ph.EP] 20 Aug 2012 Gutachter Prof. Dr. Ralf Jaumann (Freie Universit¨atBerlin, DLR Berlin) Prof. Dr. Tilman Spohn (Westf¨alische Wilhems-Universit¨atM¨unster,DLR Berlin) Tag der Disputation 6. Juli 2007 In loving memory of Felix M¨uller(1948{2005). Wish you were here. Abstract The subject of this work is the physical characterization of asteroids, with an emphasis on the thermal inertia of near-Earth asteroids (NEAs). Thermal inertia governs the Yarkovsky effect, a non-gravitational force which significantly alters the orbits of asteroids up to ∼ 20 km in diameter. Yarkovsky-induced drift is important in the assessment of the impact hazard which NEAs pose to Earth. Yet, very little has previously been known about the thermal inertia of small asteroids including NEAs. Observational and theoretical work is reported. The thermal emission of aster- oids has been observed in the mid-infrared (5{35 µm) wavelength range using the Spitzer Space Telescope and the 3.0 m NASA Infrared Telescope Facility, IRTF; techniques have been established to perform IRTF observations remotely from Berlin. A detailed thermophysical model (TPM) has been developed and exten- sively tested; this is the first detailed TPM shown to be applicable to NEA data. -
Hls-Ug-001 Human Landing System Lunar Thermal Analysis Guidebook
HLS-UG-001 BASELINE RELEASE National Aeronautics and EFFECTIVE DATE: JANUARY 04, 2021 Space Administration HUMAN LANDING SYSTEM LUNAR THERMAL ANALYSIS GUIDEBOOK Publicly Available: Release to Public Websites Requires Approval of Chief, Office of Primary Responsibility, and approval via the Scientific and Technical Information (STI) process, if applicable The electronic version is the official approved document. Verify this is the correct version before use. Human Landing System Lunar Thermal Analysis Guidebook January 2021 Revision: Baseline Release Document No: HLS-UG-01 Effective Date: January 04, 2021 Page: 1 of 147 Title: Human Landing System Lunar Thermal Analysis Guidebook REVISION AND HISTORY PAGE Revision Change Effective Description No. No. Date - HLS- Baseline Release (Reference HCB.07.01.2020) 01/04/2021 C0064 The electronic version is the official approved document. Verify this is the correct version before use. Human Landing System Lunar Thermal Analysis Guidebook January 2021 Revision: Baseline Release Document No: HLS-UG-01 Effective Date: January 04, 2021 Page: 2 of 147 Title: Human Landing System Lunar Thermal Analysis Guidebook TABLE OF CONTENTS SECTION PAGE 1.0 INTRODUCTION ................................................................................................. 10 PURPOSE ........................................................................................................... 10 SCOPE ................................................................................................................ 10 CHANGE