Mars 2020 Science Definition Team Report Frequently Asked Questions Q
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Mars Reconnaissance Orbiter Navigation Strategy for the Exomars Schiaparelli EDM Lander Mission
Jet Propulsion Laboratory California Institute of Technology Mars Reconnaissance Orbiter Navigation Strategy for the ExoMars Schiaparelli EDM Lander Mission Premkumar R. Menon Sean V. Wagner, David C. Jefferson, Eric J. Graat, Kyong J. Lee, and William B. Schulze AAS/AIAA Astrodynamics Specialist Conference San Antonio, Texas February 5–9, 2017 AAS Paper 17-337 © 2017 California Institute of Technology. Government Sponsorship Acknowledged. Mars Reconnaissance Orbiter Project Mars Reconnaissance Orbiter (Mission, Spacecraft and PSO) The Mars Reconnaissance Orbiter mission launched in August 2005 from the Cape Canaveral Air Force Station arriving at Mars in March 2006 started science operations in November 2006. MRO has completed 10 years since launch (50,000 orbits by Mar 2017) and to date has returned nearly 300 Terabytes of data. MRO Primary Science Orbit (PSO): • Sun-synchronous orbit ascending node at 3:00 PM ± 15 minutes Local Mean Solar Time (LMST) (daylight equatorial crossing) • Periapsis is frozen about the Mars South Pole • Near-repeat ground track walk (GTW) every 17-day, 211 orbit (short-term repeat) MRO targeting cycle, exact repeat after 4602 orbits. The nominal GTW is 32.45811 km West each 211 orbit cycle (maintained with periodic maneuvers). MRO Spacecraft: • Spacecraft Bus: 3-axis stabilized ACS system; 3-meter diameter High Gain Antenna; hydrazine propulsion system • Instrument Suite: HiRISE Camera, CRISM Imaging spectrometer, Mars Climate Sounder, Mars Color Imager, Context Camera, Shallow Subsurface Radar, Electra engineering payload (among other instrument payloads) 2/07/17 MRO support of ExoMars Schiaparelli Lander Overflight Relay PRM-3 4. MRO shall have good overflight pass geometry within the first 2 Sols after landing. -
Exomars Schiaparelli Direct-To-Earth Observation Using GMRT
TECHNICAL ExoMars Schiaparelli Direct-to-Earth Observation REPORTS: METHODS 10.1029/2018RS006707 using GMRT S. Esterhuizen1, S. W. Asmar1 ,K.De2, Y. Gupta3, S. N. Katore3, and B. Ajithkumar3 Key Point: • During ExoMars Landing, GMRT 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA, 2Cahill Center for Astrophysics, observed UHF transmissions and California Institute of Technology, Pasadena, CA, USA, 3National Centre for Radio Astrophysics, Pune, India Doppler shift used to identify key events as only real-time aliveness indicator Abstract During the ExoMars Schiaparelli separation event on 16 October 2016 and Entry, Descent, and Landing (EDL) events 3 days later, the Giant Metrewave Radio Telescope (GMRT) near Pune, India, Correspondence to: S. W. Asmar, was used to directly observe UHF transmissions from the Schiaparelli lander as they arrive at Earth. The [email protected] Doppler shift of the carrier frequency was measured and used as a diagnostic to identify key events during EDL. This signal detection at GMRT was the only real-time aliveness indicator to European Space Agency Citation: mission operations during the critical EDL stage of the mission. Esterhuizen, S., Asmar, S. W., De, K., Gupta, Y., Katore, S. N., & Plain Language Summary When planetary missions, such as landers on the surface of Mars, Ajithkumar, B. (2019). ExoMars undergo critical and risky events, communications to ground controllers is very important as close to real Schiaparelli Direct-to-Earth observation using GMRT. time as possible. The Schiaparelli spacecraft attempted landing in 2016 was supported in an innovative way. Radio Science, 54, 314–325. A large radio telescope on Earth was able to eavesdrop on information being sent from the lander to other https://doi.org/10.1029/2018RS006707 spacecraft in orbit around Mars. -
Digital Opportunity: a Review of Intellectual Property and Growth
Digital Opportunity A Review of Intellectual Property and Growth An Independent Report by Professor Ian Hargreaves May 2011 Contents Page Foreword by Ian Hargreaves 01 Executive Summary 03 Chapter 1 Intellectual Property and Growth 10 Chapter 2 The Evidence Base 16 Chapter 3 The International Context 21 Chapter 4 Copyright Licensing: a Moment of Opportunity 26 Chapter 5 Copyright: Exceptions for the Digital Age 41 Chapter 6 Patents 53 Chapter 7 Designs 64 Chapter 8 Enforcement and Disputes 67 Chapter 9 SMEs and the IP Framework 86 Chapter 10 An Adaptive IP Framework 91 Chapter 11 Impact 97 Annex A Terms of Reference 101 Annex B Stakeholders Met during Review of IP and Growth 102 Annex C Call for Evidence Submissions 105 Annex D List of Supporting Documents 109 Foreword When the Prime Minister commissioned this review in November 2010, he did so in terms which some considered provocative. The Review was needed, the PM said, because of the risk that the current intellectual property framework might not be sufficiently well designed to promote innovation and growth in the UK economy. In the five months we have had to compile the Review, we have sought never to lose sight of David Cameron’s “exam question”. Could it be true that laws designed more than three centuries ago with the express purpose of creating economic incentives for innovation by protecting creators’ rights are today obstructing innovation and economic growth? The short answer is: yes. We have found that the UK’s intellectual property framework, especially with regard to copyright, is falling behind what is needed. -
Mars 2020 Radiological Contingency Planning
National Aeronautics and Space Administration Mars 2020 Radiological Contingency Planning NASA plans to launch the Mars 2020 rover, produce the rover’s onboard power and to Perseverance, in summer 2020 on a mission warm its internal systems during the frigid to seek signs of habitable conditions in Mars’ Martian night. ancient past and search for signs of past microbial life. The mission will lift off from Cape NASA prepares contingency response plans Canaveral Air Force Station in Florida aboard a for every launch that it conducts. Ensuring the United Launch Alliance Atlas V launch vehicle safety of launch-site workers and the public in between mid-July and August 2020. the communities surrounding the launch area is the primary consideration in this planning. The Mars 2020 rover design is based on NASA’s Curiosity rover, which landed on Mars in 2012 This contingency planning task takes on an and greatly increased our knowledge of the added dimension when the payload being Red Planet. The Mars 2020 rover is equipped launched into space contains nuclear material. to study its landing site in detail and collect and The primary goal of radiological contingency store the most promising samples of rock and planning is to enable an efficient response in soil on the surface of Mars. the event of an accident. This planning is based on the fundamental principles of advance The system that provides electrical power for preparation (including rehearsals of simulated Mars 2020 and its scientific equipment is the launch accident responses), the timely availability same as for the Curiosity rover: a Multi- of technically accurate and reliable information, Mission Radioisotope Thermoelectric Generator and prompt external communication with the (MMRTG). -
An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger Depauw University
DePauw University Scholarly and Creative Work from DePauw University Student research Student Work 2015 An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger DePauw University Follow this and additional works at: http://scholarship.depauw.edu/studentresearch Part of the Economics Commons, and the The unS and the Solar System Commons Recommended Citation Knappenberger, Clayton, "An Economic Analysis of Mars Exploration and Colonization" (2015). Student research. Paper 28. This Thesis is brought to you for free and open access by the Student Work at Scholarly and Creative Work from DePauw University. It has been accepted for inclusion in Student research by an authorized administrator of Scholarly and Creative Work from DePauw University. For more information, please contact [email protected]. An Economic Analysis of Mars Exploration and Colonization Clayton Knappenberger 2015 Sponsored by: Dr. Villinski Committee: Dr. Barreto and Dr. Brown Contents I. Why colonize Mars? ............................................................................................................................ 2 II. Can We Colonize Mars? .................................................................................................................... 11 III. What would it look like? ............................................................................................................... 16 A. National Program ......................................................................................................................... -
Educator's Guide
EDUCATOR’S GUIDE ABOUT THE FILM Dear Educator, “ROVING MARS”is an exciting adventure that This movie details the development of Spirit and follows the journey of NASA’s Mars Exploration Opportunity from their assembly through their Rovers through the eyes of scientists and engineers fantastic discoveries, discoveries that have set the at the Jet Propulsion Laboratory and Steve Squyres, pace for a whole new era of Mars exploration: from the lead science investigator from Cornell University. the search for habitats to the search for past or present Their collective dream of Mars exploration came life… and maybe even to human exploration one day. true when two rovers landed on Mars and began Having lasted many times longer than their original their scientific quest to understand whether Mars plan of 90 Martian days (sols), Spirit and Opportunity ever could have been a habitat for life. have confirmed that water persisted on Mars, and Since the 1960s, when humans began sending the that a Martian habitat for life is a possibility. While first tentative interplanetary probes out into the solar they continue their studies, what lies ahead are system, two-thirds of all missions to Mars have NASA missions that not only “follow the water” on failed. The technical challenges are tremendous: Mars, but also “follow the carbon,” a building block building robots that can withstand the tremendous of life. In the next decade, precision landers and shaking of launch; six months in the deep cold of rovers may even search for evidence of life itself, space; a hurtling descent through the atmosphere either signs of past microbial life in the rock record (going from 10,000 miles per hour to 0 in only six or signs of past or present life where reserves of minutes!); bouncing as high as a three-story building water ice lie beneath the Martian surface today. -
NUCLEAR SAFETY LAUNCH APPROVAL: MULTI-MISSION LESSONS LEARNED Yale Chang the Johns Hopkins University Applied Physics Laboratory
ANS NETS 2018 – Nuclear and Emerging Technologies for Space Las Vegas, NV, February 26 – March 1, 2018, on CD-ROM, American Nuclear Society, LaGrange Park, IL (2018) NUCLEAR SAFETY LAUNCH APPROVAL: MULTI-MISSION LESSONS LEARNED Yale Chang The Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Rd, Laurel, MD 20723 240-228-5724; [email protected] Launching a NASA radioisotope power system (RPS) trajectory to Saturn used a Venus-Venus-Earth-Jupiter mission requires compliance with two Federal mandates: Gravity Assist (VVEJGA) maneuver, where the Earth the National Environmental Policy Act of 1969 (NEPA) Gravity Assist (EGA) flyby was the primary nuclear safety and launch approval (LA), as directed by Presidential focus of NASA, the U.S. Department of Energy (DOE), the Directive/National Security Council Memorandum 25. Cassini Interagency Nuclear Safety Review Panel Nuclear safety launch approval lessons learned from (INSRP), and the public alike. A solid propellant fire test multiple NASA RPS missions, one Russian RPS mission, campaign addressed the MPF finding and led in part to two non-RPS launch accidents, and several solid the retrofit solid propellant breakup systems (BUSs) propellant fire test campaigns since 1996 are shown to designed and carried by MER-A and MER-B spacecraft have contributed to an ever-growing body of knowledge. and the deployment of plutonium detectors in the launch The launch accidents can be viewed as “unplanned area for PNH. The PNH mission decreased the calendar experiments” that provided real-world data. Lessons length of the NEPA/LA processes to less than 4 years by learned from the nuclear safety launch approval effort of incorporating lessons learned from previous missions and each mission or launch accident, and how they were tests in its spacecraft and mission designs and their applied to improve the NEPA/LA processes and nuclear NEPA/LA processes. -
Mars Science Laboratory: Curiosity Rover Curiosity’S Mission: Was Mars Ever Habitable? Acquires Rock, Soil, and Air Samples for Onboard Analysis
National Aeronautics and Space Administration Mars Science Laboratory: Curiosity Rover www.nasa.gov Curiosity’s Mission: Was Mars Ever Habitable? acquires rock, soil, and air samples for onboard analysis. Quick Facts Curiosity is about the size of a small car and about as Part of NASA’s Mars Science Laboratory mission, Launch — Nov. 26, 2011 from Cape Canaveral, tall as a basketball player. Its large size allows the rover Curiosity is the largest and most capable rover ever Florida, on an Atlas V-541 to carry an advanced kit of 10 science instruments. sent to Mars. Curiosity’s mission is to answer the Arrival — Aug. 6, 2012 (UTC) Among Curiosity’s tools are 17 cameras, a laser to question: did Mars ever have the right environmental Prime Mission — One Mars year, or about 687 Earth zap rocks, and a drill to collect rock samples. These all conditions to support small life forms called microbes? days (~98 weeks) help in the hunt for special rocks that formed in water Taking the next steps to understand Mars as a possible and/or have signs of organics. The rover also has Main Objectives place for life, Curiosity builds on an earlier “follow the three communications antennas. • Search for organics and determine if this area of Mars was water” strategy that guided Mars missions in NASA’s ever habitable for microbial life Mars Exploration Program. Besides looking for signs of • Characterize the chemical and mineral composition of Ultra-High-Frequency wet climate conditions and for rocks and minerals that ChemCam Antenna rocks and soil formed in water, Curiosity also seeks signs of carbon- Mastcam MMRTG • Study the role of water and changes in the Martian climate over time based molecules called organics. -
Challenges and Opportunities for Bone Health
Challenges and opportunities for bone health *Han-sung Kim1 1 Department of Biomedical Engineering & Institute of Medical Engineering, Yonsei University & Yonsei-Fraunhofer medical device lab Space mission One Man One Way Trip(2020) SpaceX Dragon, 2018년 50대 부부 화성 우주인 프로젝트 화성 개척 우주인 모집 2022년 Space Exploration Technologies Corp., USA Inspiration Mars Foundation, USA Mars One, Netherlands Spaceship2, Whiteknight2 The Spaceship company, USA H-IIB F4, (2013.8.4 예정) Curiosity (12.8.6) 선저우 神舟 호 귀환 Naro 3 13.1.30 ( ) 9 Epsilon-1, (2013.8.22 예정) (12.6.29) Diane Byerly, Ph.D. NASA Johnson Space Center Houston, TX Human Mars Mission Flight Profile Transit out: 161 days Mars Departure Jan. 24, 2022 Mars surface stay: 573 days Return: 154 days 3 Earth Departure 1 Jan. 20, 2020 Mars Arrival June 30, 2020 2 4 Earth Arrival June 26, 2022 Earth Orbit At least 2years Mars Orbit Piloted Trajectories Stay on Mars Surface are need!! Bone Loss in Space Bone Loss Bone Remodeling Bone Bone formation resorbtion Bone formation Normal bone Bone resorbtion Bone Bone formation resorbtion Bone Bone resorbtion formation Bone Loss in Space unloading Bed rest Animal experiment Cell experiment Hind-limb suspenstion Denervation 3D Clinostat Unloading Animal Model (Sciatic Nerve Neurectomy) Co-research with KARI Unloading animal model from sciatic nerve neurectomy Sciatic nerve neurectomy In-vivo micro-CT (Skyscan 1076) Ko et al. (2011), J Biomech Eng Circadian Rhythms Induced night shift by regulation of light Increased accumulation of ADT may lead to child obesity, adult disease Bone loss may leads to increase fracture risk and inhibit growth of bone Disturbance of circadian rhythms Pharmacotherapy Suppress Bone resorption Recovery Whole body vibration (non pharmacotherapy) Liver damage, stomach hemorrhage Muscle pain Hard to apply to patients and elders Vertigo, vomitWe and indigestionneed to develop alternative therapies capable of overcoming the limitation. -
MARS 2020, CANDIDATES LANDING SITES, EXOMARS and THEIR RELATIONSHIP to MARS SAMPLE RETURN 10:25 A.M
2nd International Mars Sample Return 2018 (LPI Contrib. No. 2071) sess303.pdf Thursday, April 26, 2018 MARS 2020, CANDIDATES LANDING SITES, EXOMARS AND THEIR RELATIONSHIP TO MARS SAMPLE RETURN 10:25 a.m. Forum This session will present a status report on the Mars 2020 sample-caching rover, its candidate landing sites, the Exomars rover mission, and the relationship of all of these to Mars Sample Return. Chairs: Victoria Hipkin (Canadian Space Agency, Canada) Briony Horgan (Purdue University, USA) 10:25 a.m. Williford K. * *Jet Propulsion Laboratory, California Institute of Technology, USA The NASA Mars 2020 Rover Mission The NASA Mars 2020 rover mission will explore an astrobiologically relevant site to characterize its geology, evaluate past habitability, seek signs of ancient life, and assemble a returnable cache of samples. An overview of technical capabilities and scientific strategy in development will be presented with a focus on the role envisioned for Mars 2020 in a possible Mars sample return campaign. 10:45 a.m. Schulte M. * Meyer M. Grant J. Golombek M. *NASA Headquarters, USA The Mars 2020 Rover Mission Landing Site Candidates [#6026] The number of suitable landing sites for the Mars 2020 rover mission has been narrowed to three leading candidates: Jezero Crater, NE Syrtis, and Columbia Hills. Each offers geologic settings with the potential for preservation of biosignatures. 11:00 a.m. Vago J. L. * Svedhem H. Sefton-Nash E. Kminek G. Ruesch O. Haldemann A. F. C. Rodionov D. ExoMars Science Working Team *European Space Agency ExoMars Contributions to Mars Sample Return [#6021] Each of the two ExoMars missions has the potential to make discoveries that could inform and perhaps influence our collective strategy for a future Mars Sample Return mission. -
Exploration of Mars by the European Space Agency 1
Exploration of Mars by the European Space Agency Alejandro Cardesín ESA Science Operations Mars Express, ExoMars 2016 IAC Winter School, November 20161 Credit: MEX/HRSC History of Missions to Mars Mars Exploration nowadays… 2000‐2010 2011 2013/14 2016 2018 2020 future … Mars Express MAVEN (ESA) TGO Future ESA (ESA- Studies… RUSSIA) Odyssey MRO Mars Phobos- Sample Grunt Return? (RUSSIA) MOM Schiaparelli ExoMars 2020 Phoenix (ESA-RUSSIA) Opportunity MSL Curiosity Mars Insight 2020 Spirit The data/information contained herein has been reviewed and approved for release by JPL Export Administration on the basis that this document contains no export‐controlled information. Mars Express 2003-2016 … First European Mission to orbit another Planet! First mission of the “Rosetta family” Up and running since 2003 Credit: MEX/HRSC First European Mission to orbit another Planet First European attempt to land on another Planet Original mission concept Credit: MEX/HRSC December 2003: Mars Express Lander Release and Orbit Insertion Collission trajectory Bye bye Beagle 2! Last picture Lander after release, release taken by VMC camera Insertion 19/12/2003 8:33 trajectory Credit: MEX/HRSC Beagle 2 was found in January 2015 ! Only 6km away from landing site OK Open petals indicate soft landing OK Antenna remained covered Lessons learned: comms at all time! Credit: MEX/HRSC Mars Express: so many missions at once Mars Mission Phobos Mission Relay Mission Credit: MEX/HRSC Mars Express science investigations Martian Moons: Phobos & Deimos: Ionosphere, surface, -
Inventory of CO2 Available for Terraforming Mars
PERSPECTIVE https://doi.org/10.1038/s41550-018-0529-6 Inventory of CO2 available for terraforming Mars Bruce M. Jakosky 1,2* and Christopher S. Edwards3 We revisit the idea of ‘terraforming’ Mars — changing its environment to be more Earth-like in a way that would allow terres- trial life (possibly including humans) to survive without the need for life-support systems — in the context of what we know about Mars today. We want to answer the question of whether it is possible to mobilize gases present on Mars today in non- atmospheric reservoirs by emplacing them into the atmosphere, and increase the pressure and temperature so that plants or humans could survive at the surface. We ask whether this can be achieved considering realistic estimates of available volatiles, without the use of new technology that is well beyond today’s capability. Recent observations have been made of the loss of Mars’s atmosphere to space by the Mars Atmosphere and Volatile Evolution Mission probe and the Mars Express space- craft, along with analyses of the abundance of carbon-bearing minerals and the occurrence of CO2 in polar ice from the Mars Reconnaissance Orbiter and the Mars Odyssey spacecraft. These results suggest that there is not enough CO2 remaining on Mars to provide significant greenhouse warming were the gas to be emplaced into the atmosphere; in addition, most of the CO2 gas in these reservoirs is not accessible and thus cannot be readily mobilized. As a result, we conclude that terraforming Mars is not possible using present-day technology. he concept of terraforming Mars has been a mainstay of sci- Could the remaining planetary inventories of CO2 be mobi- ence fiction for a long time, but it also has been discussed from lized and emplaced into the atmosphere via current or plausible 1 a scientific perspective, initially by Sagan and more recently near-future technologies? Would the amount of CO2 that could T 2 by, for example, McKay et al.