Issue 115, August 2008
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Issue 106, May 2006
37 th Lunar and Planetary Science Conference THE CONFERENCE IN REVIEW Attendance at the 37th Lunar and Planetary Science Conference (LPSC) set yet another record for this conference, with 1546 participants from 24 countries attending the meeting held at the South Shore Harbour Resort and Conference Center in League City, Texas, on March 13–17, 2006 (see inset for attendance statistics). Rearrangement of the confi guration of the meeting rooms, along with additional overfl ow seating, allowed conference organizers and staff to accommodate the marked increase in attendance, thereby being able to maintain the current meeting venue and hence the low registration fee, which enables the high number of student attendees. LPSC continues to be recognized among the international science community as the most important planetary conference in the world, and this year’s meeting substantiated the merit of that reputation. More than 1400 abstracts were submitted in consideration for presentation at the conference, and hundreds of planetary scientists and students attended both oral and poster sessions focusing on such diverse topics as the Moon, Mars, Mercury, and Venus; outer planets and satellites; meteorites; comets, asteroids, and other small bodies; Limpacts; interplanetary dust particles and presolar grains; origins of planetary systems; planetary formation and early evolution; and astrobiology. Sunday night’s registration and reception were again held at the Center for Advanced Space Studies, which houses the Lunar and Planetary Institute. Featured on Sunday night was an open house for the display of education and public outreach activities and programs. Highlights of the conference program, established by the program committee under the guidance of co-chairs Dr. -
Titan and Enceladus $1 B Mission
JPL D-37401 B January 30, 2007 Titan and Enceladus $1B Mission Feasibility Study Report Prepared for NASA’s Planetary Science Division Prepared By: Kim Reh Contributing Authors: John Elliott Tom Spilker Ed Jorgensen John Spencer (Southwest Research Institute) Ralph Lorenz (The Johns Hopkins University, Applied Physics Laboratory) KSC GSFC ARC Approved By: _________________________________ Kim Reh Dr. Ralph Lorenz Jet Propulsion Laboratory The Johns Hopkins University, Applied Study Manager Physics Laboratory Titan Science Lead _________________________________ Dr. John Spencer Southwest Research Institute Enceladus Science Lead Pre-decisional — For Planning and Discussion Purposes Only Titan and Enceladus Feasibility Study Report Table of Contents JPL D-37401 B The following members of an Expert Advisory and Review Board contributed to ensuring the consistency and quality of the study results through a comprehensive review and advisory process and concur with the results herein. Name Title/Organization Concurrence Chief Engineer/JPL Planetary Flight Projects Gentry Lee Office Duncan MacPherson JPL Review Fellow Glen Fountain NH Project Manager/JHU-APL John Niehoff Sr. Research Engineer/SAIC Bob Pappalardo Planetary Scientist/JPL Torrence Johnson Chief Scientist/JPL i Pre-decisional — For Planning and Discussion Purposes Only Titan and Enceladus Feasibility Study Report Table of Contents JPL D-37401 B This page intentionally left blank ii Pre-decisional — For Planning and Discussion Purposes Only Titan and Enceladus Feasibility Study Report Table of Contents JPL D-37401 B Table of Contents 1. EXECUTIVE SUMMARY.................................................................................................. 1-1 1.1 Study Objectives and Guidelines............................................................................ 1-1 1.2 Relation to Cassini-Huygens, New Horizons and Juno.......................................... 1-1 1.3 Technical Approach............................................................................................... -
Ralph Lorenz Johns Hopkins – Applied Physics Lab
Space phySicS Seminar Ralph Lorenz Johns Hopkins – Applied Physics Lab Sailing the Seas of Titan, Saturn's Earth-Like Moon Thursday, September 19, 2013 725 Commonwealth Ave. Refreshments at 3:30pm in CAS 500 Talk begins at 4:00pm in CAS 502 Abstract: Oceanography is no longer just an Earth Science. The ongoing NASA/ESA Cassini mission - still making exciting discoveries 10 years after its arrival in the rich Saturnian system - has found that three seas of liquid hydrocarbons adorn Saturn’s giant, frigid moon Titan. Titan was already exotic, having a thick, organic-rich atmosphere, and a diverse landscape with mountains, craters, river channels and vast fields of sand dunes, but these seas, and hundreds of lakes, present a new environment (low gravity, dense atmosphere, hydrocarbon liquid) in which to explore familiar and important physical processes such as air:sea heat and moisture exchange, wind- driven currents and waves, etc. Moreover, Titan’s seas (notably the two largest ones, Kraken Mare and Ligiea Mare, about 1000km and 400km across, respectively) offer an appealing and accessible target for future Titan exploration. This talk will review the latest findings from Cassini, and its prospects for new discoveries as we move towards Titan’s northern summer solstice in 2017, and the opportunities for future exploration which might include (as at Mars) orbiters and landers, but also vehicles that can exploit Titan’s environment such as balloons or airplanes. The most affordable near-term prospect for in-situ exploration is a capsule to float in the seas of Titan, where after splashdown it would drift in the winds to make a traverse across the sea, measuring the liquid composition and turbidity, studying conditions with cameras and meteorological instruments, and exploring the seabed with a depth sounder. -
Titan a Moon with an Atmosphere
TITAN A MOON WITH AN ATMOSPHERE Ashley Gilliam Earth 450 – Satellites of Jupiter and Saturn 4/29/13 SATURN HAS > 60 SATELLITES, WHY TITAN? Is the only satellite with a dense atmosphere Has a nitrogen-rich atmosphere resembles Earth’s Is the only world besides Earth with a liquid on its surface • Possible habitable world Based on its size… Titan " a planet in its o# $ght! R = 6371 km R = 2576 km R = 1737 km Ch$%iaan Huy&ns (1629-1695) DISCOVERY OF TITAN Around 1650, Huygens began building telescopes with his brother Constantijn On March 25, 1655 Huygens discovered Titan in an attempt to study Saturn’s rings Named the moon Saturni Luna (“Saturns Moon”) Not properly named until the mid-1800’s THE DISCOVERY OF TITAN’S ATMOSPHERE Not much more was learned about Titan until the early 20th century In 1903, Catalan astronomer José Comas Solà claimed to have observed limb darkening on Titan, which requires the presence of an atmosphere Gerard P. Kuiper (1905-1973) José Comas Solà (1868-1937) This was confirmed by Gerard Kuiper in 1944 Image Credit: Ralph Lorenz Voyager 1 Launched September 5, 1977 M"sions to Titan Pioneer 11 Launched April 6, 1973 Cassini-Huygens Images: NASA Launched October 15, 1997 Pioneer 11 Could not penetrate Titan’s Atmosphere! Image Credit: NASA Vo y a &r 1 Image Credit: NASA Vo y a &r 1 What did we learn about the Atmosphere? • Composition (N2, CH4, & H2) • Variation with latitude (homogeneously mixed) • Temperature profile Mesosphere • Pressure profile Stratosphere Troposphere Image Credit: Fulchignoni, et al., 2005 Image Credit: Conway et al. -
DAVINCI: Deep Atmosphere Venus Investigation of Noble Gases, Chemistry, and Imaging Lori S
DAVINCI: Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging Lori S. Glaze, James B. Garvin, Brent Robertson, Natasha M. Johnson, Michael J. Amato, Jessica Thompson, Colby Goodloe, Dave Everett and the DAVINCI Team NASA Goddard Space Flight Center, Code 690 8800 Greenbelt Road Greenbelt, MD 20771 301-614-6466 Lori.S.Glaze@ nasa.gov Abstract—DAVINCI is one of five Discovery-class missions questions as framed by the NRC Planetary Decadal Survey selected by NASA in October 2015 for Phase A studies. and VEXAG, without the need to repeat them in future New Launching in November 2021 and arriving at Venus in June of Frontiers or other Venus missions. 2023, DAVINCI would be the first U.S. entry probe to target Venus’ atmosphere in 45 years. DAVINCI is designed to study The three major DAVINCI science objectives are: the chemical and isotopic composition of a complete cross- section of Venus’ atmosphere at a level of detail that has not • Atmospheric origin and evolution: Understand the been possible on earlier missions and to image the surface at origin of the Venus atmosphere, how it has evolved, optical wavelengths and process-relevant scales. and how and why it is different from the atmospheres of Earth and Mars. TABLE OF CONTENTS • Atmospheric composition and surface interaction: Understand the history of water on Venus and the 1. INTRODUCTION ....................................................... 1 chemical processes at work in the lower atmosphere. 2. MISSION DESIGN ..................................................... 2 • Surface properties: Provide insights into tectonic, 3. PAYLOAD ................................................................. 2 volcanic, and weathering history of a typical tessera 4. SUMMARY ................................................................ 3 (highlands) terrain. -
Scientific Observations with the Insight Solar Arrays: Dust, Clouds
Scientific Observations With the InSight Solar Arrays: Dust, Clouds, and Eclipses on Mars Ralph Lorenz, Mark Lemmon, Justin Maki, Donald Banfield, Aymeric Spiga, Constantinos Charalambous, Elizabeth Barrett, Jennifer Herman, Brett White, Samuel Pasco, et al. To cite this version: Ralph Lorenz, Mark Lemmon, Justin Maki, Donald Banfield, Aymeric Spiga, et al.. Scientific Obser- vations With the InSight Solar Arrays: Dust, Clouds, and Eclipses on Mars. Earth and Space Science, American Geophysical Union/Wiley, 2020, 7 (5), 10.1029/2019EA000992. hal-02872154 HAL Id: hal-02872154 https://hal.sorbonne-universite.fr/hal-02872154 Submitted on 17 Jun 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Distributed under a Creative Commons Attribution - NonCommercial - NoDerivatives| 4.0 International License RESEARCH ARTICLE Scientific Observations With the InSight Solar Arrays: 10.1029/2019EA000992 Dust, Clouds, and Eclipses on Mars Special Section: Ralph D. Lorenz1 , Mark T. Lemmon2 , Justin Maki3 , Donald Banfield4 , InSight at Mars 5,6 7 3 3 Aymeric Spiga -
EGU2018-19456-1, 2018 EGU General Assembly 2018 © Author(S) 2018
Geophysical Research Abstracts Vol. 20, EGU2018-19456-1, 2018 EGU General Assembly 2018 © Author(s) 2018. CC Attribution 4.0 license. DRAGONFLY: in situ exploration of Titan’s meteorology Scot Rafkin (1), Ralph Lorenz (2), Elizabeth Turtle (2), Jason Barnes (3), Melissa Trainer (4), Alice Le Gall (5), Juan Lora (6), Chris McKay (7), Claire Newman (8), Mark Panning (9), Kristin Sotzen (2), Tetsuya Tokano (10), Colin Wilson (11), and the Dragonfly Team (1) Southwest Research Institute, Boulder, CO, USA, (2) Johns Hopkins Applied Physics Lab., Laurel, MD, USA, (3) Univ. Idaho, Moscow, ID, USA, (4) NASA Goddard Space Flight Center, Greenbelt, MD, USA, (5) Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France, (6) Univ. California, Los Angeles, CA, USA, (7) NASA Ames Research Center, Moffett Field, CA, USA, (8) Aeolis Research, Pasadena, CA, USA, (9) Jet Propulsion Laboratory California Institute of Technology, Pasadena, CA, USA, (10) Inst. fur Geophysik und Meteorologie, Univ. Koln, Koln, Germany, (11) Oxford Univ., Oxford, UK Dragonfly is a rotorcraft lander mission currently in a Phase A study under NASA’s New Frontiers Program that would take advantage of Titan’s dense atmosphere and low gravity to visit a number of surface locations to study how far chemistry can progress in environments that provide key ingredients for life. This mission architecture also permits and demands investigation of Titan’s atmosphere. First, Dragonfly is a lander that will spend >2 Earth years on Titan’s surface, long enough to observe many diurnal cycles, atmospheric waves, and perhaps even some seasonal change. The DraGMet (Dragonfly Geophysics and Meteorology) instrument package includes measurement of wind speed and direction (using sensors on each of the four rotor pylons, to assure that one or more sensors are upwind of and thus unperturbed by the vehicle), temperature and pressure, and methane humidity. -
Newsletter 14-2 Published on Division for Planetary Sciences (
Newsletter 14-2 Published on Division for Planetary Sciences (https://dps.aas.org) Newsletter 14-2 Issue 14-2, January 22, 2014 +-----------------------------CONTENTS--------------------------------+ 1) NOTE FROM THE CHAIR 2) MESSAGE FROM THE FEDERAL RELATIONS SUBCOMMITTEE (FRS) CHAIR 3) REMINDER: CALL FOR DPS 2014 PRIZE NOMINATIONS 4) REMINDER : 2014 ONLINE MEMBERSHIP RENEWALS 5) CALL FOR MISSION CONCEPTS FOR THE LARGE-SIZE 'L2' MISSION OPPORTUNITY IN ESA'S SCIENCE PROGRAMME 6) DRAFT SOLICITATIONS OF SOME PSD R&A SOLICITATIONS FOR ROSES14 RELEASED TO PUBLIC 7) MARS CRITICAL DATA PRODUCTS PROGRAM (ROUND IX) 8) JOBS/POSITIONS OPPORTUNITIES 9) UPCOMING MEETINGS +---------------------------------------------------------------------+ 1---------1---------1---------1---------1---------1---------1---------1---------1 NOTE FROM THE CHAIR Washington DC may be currently covered in snow, but warm fuzzies abound here as a 2014 budget has passed into law (more details in the note below from the Federal Relations Subcommittee). Take a deep breath, and think about our DPS community’s successes. We’ve secured $1.3 Billion dollars to do planetary exploration. Our missions are healthy: Cassini, Curiosity, MESSENGER, JUNO, and more. ESA’s ROSETTA mission successfully reawakened from hibernation, ready to go comet hunting. Europa got a big boost with the news from the Hubble Space Telescope hinting at tidally-driven water geysers. What have you done to share this news with your family, your community, your representatives in Washington? Drop me a line; I’d like to share some of your stories. Regarding NASA’s R&A reorganization, please communicate your thoughts with the members of the Planetary Science Subcommittee (PSS), as well as the members of the various assessment groups (OPAG, SBAG, VEXAG, MEPAG, LEAG, etc). -
Titan Mare Explorer
TiME Titan Mare Explorer Titan Mare Explorer (TiME): Proxemy Research First Exploration of an Extraterrestrial Sea Ellen Stofan TiME Science . Discovery of lakes and seas in Titan’s northern hemisphere confirmed the expectation that liquid hydrocarbons exist . Detection of the presence of ethane in Ontario Lacus near the South Pole (Brown et al., 2008) . 2 distinct types of features- lakes and seas, likely 10’s, >100 m deep . Post-Cassini, major questions will remain on the chemistry of sea liquids, their role in the overall methane cycle, the origin of sea basins, and seasonal processes and variability TiME Proprietary Information/Competition Sensitive Titan’s methane cycle • Titan’s methane cycle is analogous to Earth’s hydrologic cycle, with meteorological working fluid existing in condensed phase on surface and within crust, cycling through the surface atmosphere system and transporting mass and energy TiME Proprietary Information/Competition Sensitive TiME Science Target •Target: Ligeia Mare (78°N, 250°W) –One of the largest seas identified to date on Titan, surface area ~100,000 km2 –Backup target- Kraken Mare TiME Proprietary Information/Competition Sensitive TiME Science Team .PI: Ellen Stofan (Proxemy Research) .Co-Is: .Jonathan Lunine (Univ. of Az.) - Deputy PI .Ralph Lorenz (APL)- Project Scientist .Oded Aharonson (CalTech) .Beau Bierhaus (LM) .Ben Clark (SSI) .Caitlin Griffith (Univ. Arizona) .Ari-Matti Harri (FMI) .Erich Karkoschka (Univ. Arizona) .Randy Kirk (USGS) .Paul Mahaffy (Goddard) .Claire Newman (Ashima Research) .Mike Ravine (MSSS) .Melissa Trainer (GSFC) .Elizabeth Turtle (APL) .Hunter Waite (SWRI) .Margaret Yelland (Univ. Southampton) .John Zarnecki (Open University) TiME Proprietary Information/Competition Sensitive TiME Science Goals and Objectives . -
Proquest Dissertations
Characterizing transiting extrasolar giant planets: On companions, rings, and love handles Item Type text; Dissertation-Reproduction (electronic) Authors Barnes, Jason Wayne Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 01/10/2021 05:33:59 Link to Item http://hdl.handle.net/10150/290019 NOTE TO USERS This reproduction is the best copy available. UMI CHARACTERIZING TRANSITING EXTRASOLAR GIANT PLANETS: ON COMPANIONS, RINGS, AND LOVE HANDLES by Jason Wayne Barnes A Dissertation Submitted to the Faculty of the DEPARTMENT OF PLANETARY SCIENCES In Partial Fulfillment of the Requirements For the Degree of DOCTOR OF PHILOSOPHY In the Graduate College THE UNIVERSITY OF ARIZONA 2 0 0 4 UMI Number: 3131584 INFORMATION TO USERS The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleed-through, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyright material had to be removed, a note will indicate the deletion. UMI UMI Microform 3131584 Copyright 2004 by ProQuest Information and Learning Company. All rights reserved. This microform edition is protected against unauthorized copying under Title 17, United States Code. ProQuest Information and Learning Company 300 North Zeeb Road P.O. -
The Planetary Report December Solstice 2011 Volume 31, Number 5
THE PLANETARY REPORT DECEMBER SOLSTICE 2011 VOLUME 31, NUMBER 5 www.planetary.org REMEMBERING THE YEAR IN PICTURES NEW (OLD) VENUS IMAGES C POLITICAL ACTION 2011 UPDATE C SHOEMAKER GRANT RECIPIENTS SNAPSHOTS FROM SPACE EMILY STEWART LAKDAWALLA blogs at planetary.org/blog. New images, old camera 1975 was a good-looking year for Venus VENERA 9 BECAME THE FIRST ARTIFICIAL satellite of Venus, and its lander was the first to photograph Venus’ surface, on October 20, 1975. One of its two cameras, a line-scanner that rotated in order to build a complete image, returned two views of a rock-strewn hillside. The scanner was angled from the spacecraft’s body, so this panorama shows the horizon at its edges and the Images: Russian Academy of Sciences/Don Mitchell Sciences/Don of Academy Russian Images: ground in front of the lander at its center. This view was reconstructed by Don Mitchell from data on tapes exchanged between the Soviet Union and Brown University. More recently, digital data have become available online, and Mitchell used those data to reconstruct a view of Venus (at right) captured by the Venera 9 orbiter on December 11, 1975. For more Venera photos, visit Mitchell’s website at MENTALLANDSCAPE.COM. —Emily Stewart Lakdawalla LEARN MORE ABOUT THIS IMAGE PLANETARY.ORG/SNAPSHOTS DIS COVER MORE ABOUT AMATEUR IMAGE PROCESSING PLANETARY.ORG/PROGRAMS/PROJECTS/AMATEUR SEE MORE EVERY DAY! PLANETARY.ORG/BLOG CONTACT US The Planetary Society 85 South Grand Avenue Pasadena, CA 91105-1602 General Calls: 626-793-5100 E-mail: [email protected] Internet: planetary.org 2 THE PLANETARY REPORT C DECEMBER SOLSTICE 2011 SNAPSHOTS FROM SPACE CONTENTS DECEMBER SOLSTICE 2011 The Year in Pictures Stunning photography of breakthroughs 6 in space science from the the past year. -
COPYRIGHT NOTICE: Ralph Lorenz and Jacqueline Mitton: Titan Unveiled Is Published by Princeton University Press and Copyrighted, © 2008, by Princeton University Press
COPYRIGHT NOTICE: Ralph Lorenz and Jacqueline Mitton: Titan Unveiled is published by Princeton University Press and copyrighted, © 2008, by Princeton University Press. All rights reserved. No part of this book may be reproduced in any form by any electronic or mechanical means (including photocopying, recording, or information storage and retrieval) without permission in writing from the publisher, except for reading and browsing via the World Wide Web. Users are not permitted to mount this file on any network servers. Follow links for Class Use and other Permissions. For more information send email to: [email protected] 1. The Lure of Titan On July 1, 2004, the Cassini spacecraft arrived at Saturn after a journey from Earth lasting almost seven years. At 6.8 m in length, this monstrous robotic explorer was the largest western spacecraft ever to be dispatched on an interplanetary mission. Its battery of scientific instruments was designed to return images and data not only from the giant planet itself and its spectacular ring system, but also from members of Saturn’s family of over fifty moons. Foremost in interest among the diverse collection of icy worlds in orbit around Saturn was Titan, a body so special, so intri guing in its own right that Cassini carried with it a detachable package of instruments—named the Huygens probe—that would parachute through Titan’s atmosphere to observe its surface. By any reckoning, Titan is an unusual moon. It is 5,150 km across— nearly 50 percent bigger than our own Moon and 6 percent larger than Mercury.