NASA ADVISORY COUNCIL Planetary Sciences Subcommittee
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Mars Exploration: an Overview of Indian and International Mars Missions Nayamavalsa Scariah1, Dr
Taurian Innovative Journal/Volume 1/ Issue 1 Mars exploration: An overview of Indian and International Mars Missions NayamaValsa Scariah1, Dr. Mili Ghosh2, Dr.A.P.Krishna3 Birla Institute of Technology, Mesra, Ranchi Abstract- Mars is the fourth planet from the sun. It is 1. Introduction also known as red planet because of its iron oxide content. There are lots of missions have been launched to Mars is also known as red planet, because of the mars for better understanding of our neighboring planet. reddish iron oxide prevalent on its surface gives it a There are lots of unmanned spacecraft including reddish appearance. It is the fourth planet from sun. orbiters, landers and rovers have been launched into mars since early 1960. Sputnik was the first satellite The term sol is used to define duration of solar day on launched in 1957 by Soviet Union. After seven failure Mars. A mean Martian solar day or sol is 24 hours 39 missions to Mars, Mariner 4 was the first satellite which minutes and 34.244 seconds. Many space missions to reached the Martian orbiter successfully. The Viking 1 Mars have been planned and launched for Mars was the first lander reached on Mars on 1975. India exploration (Table:1) but most of them failed without successfully launched a spacecraft, Mangalyan (Mars completing the task specially in early attempts th Orbiter Mission) on 5 November, 2013, with five whereas some NASA missions were very payloads to Mars. India was the first nation to successful(such as the twin Mars Exploration Rovers, successfully reach Mars on its first attempt. -
+ New Horizons
Media Contacts NASA Headquarters Policy/Program Management Dwayne Brown New Horizons Nuclear Safety (202) 358-1726 [email protected] The Johns Hopkins University Mission Management Applied Physics Laboratory Spacecraft Operations Michael Buckley (240) 228-7536 or (443) 778-7536 [email protected] Southwest Research Institute Principal Investigator Institution Maria Martinez (210) 522-3305 [email protected] NASA Kennedy Space Center Launch Operations George Diller (321) 867-2468 [email protected] Lockheed Martin Space Systems Launch Vehicle Julie Andrews (321) 853-1567 [email protected] International Launch Services Launch Vehicle Fran Slimmer (571) 633-7462 [email protected] NEW HORIZONS Table of Contents Media Services Information ................................................................................................ 2 Quick Facts .............................................................................................................................. 3 Pluto at a Glance ...................................................................................................................... 5 Why Pluto and the Kuiper Belt? The Science of New Horizons ............................... 7 NASA’s New Frontiers Program ........................................................................................14 The Spacecraft ........................................................................................................................15 Science Payload ...............................................................................................................16 -
LAURA KERBER Jet Propulsion Laboratory [email protected] 4800 Oak Grove Dr
LAURA KERBER Jet Propulsion Laboratory [email protected] 4800 Oak Grove Dr. Pasadena, CA __________________________________________________________________________________________ Education September 2006-May 2011 Brown University, Providence, RI PhD, Geological Sciences (May 2011) MS, Engineering, Fluid Mechanics (May 2011) MS, Geological Sciences (May 2008) August 2002-May 2006 Pomona College, Claremont, CA Major: Planetary Geology/Space Science Minor: Mathematics May 2002 Graduated Cherry Creek High School, Greenwood Village, Colorado, highest honors Research Experience and Roles September 2014- Present Jet Propulsion Laboratory, Research Scientist PI of Discovery Mission Concept Moon Diver Deputy Project Scientist, 2001 Mars Odyssey Yardang formation and distribution on Mars and Earth Ongoing development of end-to-end Martian sulfur cycle model, including microphysical processes, photochemistry, and interaction with the surface Measurement of wind over complex surfaces Microscale wind and erosion processes in cold polar deserts Science liaison to the Mars Program Office, Next Mars Orbiter (NeMO) Member of 2015 NeMO SAG Member of 2015 ICE-WG (In-situ resource utilization and civil engineering HEOMD working group) Science lead on several internal formulation studies, including a “Many MERs to Mars” concept study; “RSL Exploration with the Axel Extreme Terrain Robot” strategic initiative; “Autonomous Recognition of Signs of Life” spontaneous RTD; Moon Diver Instrument Trade Study; etc. Lead of Citizen Scientist “Planet Four: -
MEPAG Report to PSS 03-2016
Lisa Pratt, MEPAG Chair Report to PSS March 10-11, 2016 Mission Status Highlights • Curiosity is moving on from its several-month investigation of the Namib (part of Bagnold dunes) • MRO and ODY are stepping up observations as data rates increase – Both orbiters have started observing candidate sites (exploration zones) for humans on Mars • MER-B has survived winter and is exploring area where orbital data indicate clays • MAVEN has finished prime mission; special issue out with 59 papers reporting results • Foreign collaborations with ESA Mars Express and ExoMars MOMA continuing • 2020 Mars rover passed PDR review but has not gone through the Directorate or Agency Program Management Councils MEPAG Face-to-Face Meeting held March 2–3 • New MEPAG Chair: Jeff Johnson (JHU-APL) – Lisa Pratt moves to MEPAG Executive Committee – Nominations invited to fill vacancies on Goals Committee • Wide-Ranging Presentations and Discussion – Reports from PSD, MEP, and several space agencies • Including report from IMEWG iMARS coordination study – Overview of joint HEO-SMD activities • Successful first workshop for landing sites (Exploration Zones) for humans on Mars held October 2015 – MEPAG accepted two reports from its Science Analysis Groups • Science Objectives for Human Explorers on Mars (HSO-SAG) • Next Mars Orbiter (NEX-SAG) Next Mars Orbiter (1 of 3) MEPAG endorsed the NEX-SAG report which concluded: o z M’rs Prflitere utilizing Solar Electric Propulsion (SEP) and advanced telecom in a 5‑year mission in low Mars orbit, could provide exciting new science and resource identification A mission with SEP could have the capability for return of a cache of Mars samples to Earth vicinity as well as payload elements addressing high-priority resource and other science objectives o Return capability addresses the need to make progress on sample return, which is the Decadal Survey’s highest priority for flagship missions. -
Gao-21-306, Nasa
United States Government Accountability Office Report to Congressional Committees May 2021 NASA Assessments of Major Projects GAO-21-306 May 2021 NASA Assessments of Major Projects Highlights of GAO-21-306, a report to congressional committees Why GAO Did This Study What GAO Found This report provides a snapshot of how The National Aeronautics and Space Administration’s (NASA) portfolio of major well NASA is planning and executing projects in the development stage of the acquisition process continues to its major projects, which are those with experience cost increases and schedule delays. This marks the fifth year in a row costs of over $250 million. NASA plans that cumulative cost and schedule performance deteriorated (see figure). The to invest at least $69 billion in its major cumulative cost growth is currently $9.6 billion, driven by nine projects; however, projects to continue exploring Earth $7.1 billion of this cost growth stems from two projects—the James Webb Space and the solar system. Telescope and the Space Launch System. These two projects account for about Congressional conferees included a half of the cumulative schedule delays. The portfolio also continues to grow, with provision for GAO to prepare status more projects expected to reach development in the next year. reports on selected large-scale NASA programs, projects, and activities. This Cumulative Cost and Schedule Performance for NASA’s Major Projects in Development is GAO’s 13th annual assessment. This report assesses (1) the cost and schedule performance of NASA’s major projects, including the effects of COVID-19; and (2) the development and maturity of technologies and progress in achieving design stability. -
Calwater Field Studies Designed to Quantify the Roles of Atmospheric Rivers and Aerosols in Modulating U.S
CALWATER FIELD STUDIES DESIGNED TO QUANTIFY THE ROLES OF ATMOSPHERIC RIVERS AND AEROSOLS IN MODULATING U.S. WEST COAST PRECIPITATION IN A CHANGING CLIMATE BY F. M. RALPH, K. A. PRATHER, D. CAYAN, J. R. SPAckmAN, P. DEMOTT, M. DETTINGER, C. FAIRALL, R. LEUNG, D. ROSENFELD, S. RUTLEDGE, D. WALISER, A. B. WHITE, J. COrdEIRA, A. MARTIN, J. HELLY, AND J. INTRIERI A group of meteorologists, hydrologists, climate scientists, atmospheric chemists, and oceanographers have created an interdisciplinary research effort to explore the causes of variability of rainfall, flooding and water supply along the U.S. West Coast. alWater is a multiyear program of field cam- air pollution, aerosol chemistry, and climate. The paigns, numerical modeling experiments, and purpose of the CalWater workshop was threefold: 1) to C scientific analysis focused on phenomena that discuss key science gaps and the potential for lever- are key to the water supply and associated extremes aging long-term Hydrometeorology Testbed (HMT) (drought, flood) in the U.S. West Coast region. Table 1 data collection in California (Ralph et al. 2013), 2) to summarizes CalWater’s development timeline. The explore interest in the potential impacts of anthropo- results from CalWater are also relevant in many genic aerosols on California’s water supply, and 3) to other regions around the globe. CalWater began as build on the Suppression of Precipitation (SUPRECIP) a workshop at Scripps Institution of Oceanography experiment from 2005 to 2007 (Rosenfeld et al. 2008b) (SIO) in 2008 that brought -
Gordon Woodcock Space Architecture Award 2020 Candidate: a Scott Howe
Gordon Woodcock Space Architecture Award 2020 Candidate: A Scott Howe To the AIAA Space Architecture Technical Committee, thank you very much for nominating me for this award. I feel humbled, and I’m sure there are many worthy candidates. I feel as though I have been busy in some distant corner of the field, but I am very pleased that Space Architecture has grown to what it is today. The following are my statements and comments as requested – please let me know if further information is needed. 1. Statement confirming you’ve been involved in the field for at least 10 years: I was at the impressionable age of 9 years old when Neil and Buzz walked on the moon and was interested in space ever since. However, the idea of working for NASA seemed way beyond my reach, and didn’t seem compatible with my desire to become an architect so I went straight into architecture. I worked in terrestrial architecture since 1978. A turning point came when I began working in Japan in 1988, and got involved with the folks doing robotic construction. I began considering the issue of large-scale construction using entirely autonomous, mechanized means, and in the late 1990’s was introduced to early AIAA Design Engineering Space Architecture WG efforts by Marc Cohen and Ted Hall. I submitted my first Space Architecture paper, discussing a robotic outpost construction system in 2000 and increased my involvement in AIAA after that. I became a full-time Space Architect in 2007 when I joined the NASA Jet Propulsion Laboratory and have been working on robotic construction for planetary surfaces, the design of outposts and habitats, and pressurized vehicles ever since that time. -
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. -
Coupled Chemistry-Meteorology/ Climate Modelling (CCMM): Status and Relevance for Numerical Weather Prediction, Atmospheric Pollution and Climate Research
GAW Report No. 226 WWRP 2016-1 WCRP Report No. 9/2016 Coupled Chemistry-Meteorology/ Climate Modelling (CCMM): status and relevance for numerical weather prediction, atmospheric pollution and climate research (Geneva, Switzerland, 23-25 February 2015) WEATHER CLIMATE WATER CLIMATE WEATHER WMO-No. 1172 GAW Report No. 226 WWRP 2016-1 WCRP Report No. 9/2016 Coupled Chemistry-Meteorology/ Climate Modelling (CCMM): status and relevance for numerical weather prediction, atmospheric pollution and climate research (Geneva, Switzerland, 23-25 February 2015) WMO-No. 1172 2016 WMO-No. 1172 © World Meteorological Organization, 2016 The right of publication in print, electronic and any other form and in any language is reserved by WMO. Short extracts from WMO publications may be reproduced without authorization, provided that the complete source is clearly indicated. Editorial correspondence and requests to publish, reproduce or translate this publication in part or in whole should be addressed to: Chairperson, Publications Board World Meteorological Organization (WMO) 7 bis, avenue de la Paix Tel.: +41 (0) 22 730 84 03 P.O. Box 2300 Fax: +41 (0) 22 730 80 40 CH-1211 Geneva 2, Switzerland E-mail: [email protected] ISBN 978-92-63-11172-2 NOTE The designations employed in WMO publications and the presentation of material in this publication do not imply the expression of any opinion whatsoever on the part of WMO concerning the legal status of any country, territory, city or area, or of its authorities, or concerning the delimitation of itsfrontiers or boundaries. The mention of specific companies or products does not imply that they are endorsed or recommended by WMO in preference to others of a similar nature which are not mentioned or advertised. -
The Supercam Instrument Suite on the NASA Mars 2020 Rover: Body Unit and Combined System Tests
Space Sci Rev (2021) 217:4 https://doi.org/10.1007/s11214-020-00777-5 The SuperCam Instrument Suite on the NASA Mars 2020 Rover: Body Unit and Combined System Tests RogerC.Wiens1 · Sylvestre Maurice2 · Scott H. Robinson1 · Anthony E. Nelson1 · Philippe Cais3 · Pernelle Bernardi4 · Raymond T. Newell1 · Sam Clegg1 · Shiv K. Sharma5 · Steven Storms1 · Jonathan Deming1 · Darrel Beckman1 · Ann M. Ollila1 · Olivier Gasnault2 · Ryan B. Anderson6 · Yves André7 · S. Michael Angel8 · Gorka Arana9 · Elizabeth Auden1 · Pierre Beck10 · Joseph Becker1 · Karim Benzerara11 · Sylvain Bernard11 · Olivier Beyssac11 · Louis Borges1 · Bruno Bousquet12 · Kerry Boyd1 · Michael Caffrey1 · Jeffrey Carlson13 · Kepa Castro9 · Jorden Celis1 · Baptiste Chide2,14 · Kevin Clark13 · Edward Cloutis15 · Elizabeth C. Cordoba13 · Agnes Cousin2 · Magdalena Dale1 · Lauren Deflores13 · Dorothea Delapp1 · Muriel Deleuze7 · Matthew Dirmyer1 · Christophe Donny7 · Gilles Dromart16 · M. George Duran1 · Miles Egan5 · Joan Ervin13 · Cecile Fabre17 · Amaury Fau11 · Woodward Fischer18 · Olivier Forni2 · Thierry Fouchet4 · Reuben Fresquez1 · Jens Frydenvang19 · Denine Gasway1 · Ivair Gontijo13 · John Grotzinger18 · Xavier Jacob20 · Sophie Jacquinod4 · Jeffrey R. Johnson21 · Roberta A. Klisiewicz1 · James Lake1 · Nina Lanza1 · Javier Laserna22 · Jeremie Lasue2 · Stéphane Le Mouélic23 · Carey Legett IV1 · Richard Leveille24 · Eric Lewin10 · Guillermo Lopez-Reyes25 · Ralph Lorenz21 · Eric Lorigny7 · Steven P. Love1 · Briana Lucero1 · Juan Manuel Madariaga9 · Morten Madsen19 · Soren Madsen13 -
Mars-Base-Camp-2028.Pdf
Mars Base Camp An Architecture for Sending Humans to Mars by 2028 A Technical Paper Presented by: Timothy Cichan Stephen A. Bailey Lockheed Martin Space Deep Space Systems, Inc. [email protected] [email protected] Scott D. Norris Robert P. Chambers Lockheed Martin Space Lockheed Martin Space [email protected] [email protected] Robert P. Chambers Joshua W. Ehrlich Lockheed Martin Space Lockheed Martin Space [email protected] [email protected] October 2016 978-1-5090-1613-6/17/$31.00 ©2017 IEEE Abstract—Orion, the Multi-Purpose Crew Vehicle, near term Mars mission is compelling and feasible, is a key piece of the NASA human exploration and will highlight the required key systems. architecture for beyond earth orbit (BEO). Lockheed Martin was awarded the contracts for TABLE OF CONTENTS the design, development, test, and production for Orion up through the Exploration Mission 2 (EM- 1. INTRODUCTION ..................................................... 2 2). Additionally, Lockheed Martin is working on 2. ARCHITECTURE PURPOSE AND TENETS ....................... 3 defining the cis-lunar Proving Ground mission 3. MISSION CAMPAIGN, INCLUDING PROVING GROUND architecture, in partnership with NASA, and MISSIONS ................................................................ 5 exploring the definition of Mars missions as the 4. MISSION DESCRIPTION AND CONCEPT OF OPERATIONS . 7 horizon goal to provide input to the plans for 5. ELEMENT DESCRIPTIONS ....................................... 13 human exploration of the solar system. This paper 6. TRAJECTORY DESIGN ............................................ 16 describes an architecture to determine the 7. SCIENCE ............................................................. 19 feasibility of a Mars Base Camp architecture 8. MARS SURFACE ACCESS FOR CREW ......................... 14 within about a decade. -
The Future of Mro/Hirise
49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 1301.pdf THE FUTURE OF MRO/HIRISE. A. S. McEwen1 and the HiRISE Science and Operations Team 1LPL, Univer- sity of Arizona ([email protected]). Introduction: The High Resolution Imaging Sci- we can help with PDS archival of any full-resolution, ence Experiment (HiRISE) [1-2] on the Mars Recon- high-quality DTMs. naisance Orbiter (MRO) [3-4] has been orbiting Mars More than 1,300 peer-reviewed publications with since 2006. The nominal mission ended in 2010, but “HiRISE” and “Mars” are found by NASA ADS full- MRO has continued science and relay operations, now text search (Fig. 1). A good sample of HiRISE-based in its 4th extended mission. Both the spacecraft and studies can be seen by searching for “HiRISE” in instrument have experienced a variety of anomalies LPSC abstracts; in 2017, there were 181 abstracts. and degradation over time, although the performance Most publications do not include HiRISE team mem- of both has been exceptional well past their originally bers as authors, so much of the community may be planned lifetimes. This presentation describes the ac- unaware of changes over time. complishments to date of HiRISE and prospects for the HiRISE image anomalies: There have been a future, with perhaps another decade of imaging. number of anomalies that affect image quality. HiRISE obtains the highest-resolution orbital im- Loss of CCDs. RED9 was lost in 2011, narrowing ages acquired of Mars, ranging from 25-35 cm/pixel the swath width. Fortunately there have been no fur- scale depending on MRO’s altitude and the off-nadir ther failures to date, but this remains a distinct possi- look angle.