Prototyping an Onboard Scheduler for the Mars 2020 Rover
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Mars Reconnaissance Orbiter
Chapter 6 Mars Reconnaissance Orbiter Jim Taylor, Dennis K. Lee, and Shervin Shambayati 6.1 Mission Overview The Mars Reconnaissance Orbiter (MRO) [1, 2] has a suite of instruments making observations at Mars, and it provides data-relay services for Mars landers and rovers. MRO was launched on August 12, 2005. The orbiter successfully went into orbit around Mars on March 10, 2006 and began reducing its orbit altitude and circularizing the orbit in preparation for the science mission. The orbit changing was accomplished through a process called aerobraking, in preparation for the “science mission” starting in November 2006, followed by the “relay mission” starting in November 2008. MRO participated in the Mars Science Laboratory touchdown and surface mission that began in August 2012 (Chapter 7). MRO communications has operated in three different frequency bands: 1) Most telecom in both directions has been with the Deep Space Network (DSN) at X-band (~8 GHz), and this band will continue to provide operational commanding, telemetry transmission, and radiometric tracking. 2) During cruise, the functional characteristics of a separate Ka-band (~32 GHz) downlink system were verified in preparation for an operational demonstration during orbit operations. After a Ka-band hardware anomaly in cruise, the project has elected not to initiate the originally planned operational demonstration (with yet-to-be used redundant Ka-band hardware). 201 202 Chapter 6 3) A new-generation ultra-high frequency (UHF) (~400 MHz) system was verified with the Mars Exploration Rovers in preparation for the successful relay communications with the Phoenix lander in 2008 and the later Mars Science Laboratory relay operations. -
Refactoring the Curiosity Rover's Sample Handling Architecture on Mars
Refactoring the Curiosity Rover's Sample Handling Architecture on Mars Vandi Verma Stephen Kuhn (abstracting the shared development effort of many) The research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Copyright 2018 California Institute of Technology. U.S. Government sponsorship acknowledged. Introduction • The Mars Science Laboratory (“MSL”) hardware was architected to enable a fixed progression of activities that essentially enforced a campaign structure. In this structure, sample processing and analysis conflicted with any other usage of the robotic arm. • Unable to stow the arm and drive away • Unable to deploy arm instruments for in-situ engineering or science • Unable to deploy arm instruments or mechanisms on new targets • Sampling engineers developed and evolved a refactoring of this architecture in order to have it both ways Turn the hardware into a series of caches and catchments that could service all arm orientations. Enable execution of other arm activities with one “active” sample Page 2 11/18/20preserved such that additional portions could be delivered. The Foundational Risk Page 3 11/18/20 The Original Approach Page 4 11/18/20 Underpinnings of the original approach • Fundamentally, human rover planners simply could not keep track of sample in CHIMRA as it sluiced, stick- slipped, fell over partitions, pooled in catchments, etc. Neither could we update the Flight Software to model this directly. • But, with some simplifying abstraction of sample state and preparation of it into confined regimes of orientation, ground tools could effectively track sample. Rover planners’ use of Software Simulator was extended to enforce a chain of custody in commanded orientation, creating a faulted breakpoint upon violation that could be used to fix it. -
The Journey to Mars: How Donna Shirley Broke Barriers for Women in Space Engineering
The Journey to Mars: How Donna Shirley Broke Barriers for Women in Space Engineering Laurel Mossman, Kate Schein, and Amelia Peoples Senior Division Group Documentary Word Count: 499 Our group chose the topic, Donna Shirley and her Mars rover, because of our connections and our interest level in not only science but strong, determined women. One of our group member’s mothers worked for a man under Ms. Shirley when she was developing the Mars rover. This provided us with a connection to Ms. Shirley, which then gave us the amazing opportunity to interview her. In addition, our group is interested in the philosophy of equality and we have continuously created documentaries that revolve around this idea. Every member of our group is a female, so we understand the struggles and discrimination that women face in an everyday setting and wanted to share the story of a female that faced these struggles but overcame them. Thus after conducting a great amount of research, we fell in love with Donna Shirley’s story. Lastly, it was an added benefit that Ms. Shirley is from Oklahoma, making her story important to our state. All of these components made this topic extremely appealing to us. We conducted our research using online articles, Donna Shirley’s autobiography, “Managing Martians”, news coverage from the launch day, and our interview with Donna Shirley. We started our research process by reading Shirley’s autobiography. This gave us insight into her college life, her time working at the Jet Propulsion Laboratory, and what it was like being in charge of such a barrier-breaking mission. -
NASA's Mars 2020 Perseverance Rover Gets Balanced 21 April 2020
NASA's Mars 2020 Perseverance rover gets balanced 21 April 2020 minimize friction that could affect the accuracy of the results, the table's surface sits on a spherical air bearing that essentially levitates on a thin layer of nitrogen gas. To determine center of gravity relative to the rover's z-axis (which extends from the bottom of the rover through the top) and y-axis (from the rover's left to right side), the team slowly rotated the vehicle back and forth, calculating the imbalance in its mass distribution. NASA's Perseverance rover is moved during a test of its mass properties at Kennedy Space Center in Florida. The image was taken on April 7, 2020. Credit: NASA/JPL-Caltech With 13 weeks to go before the launch period of NASA's Mars 2020 Perseverance rover opens, final preparations of the spacecraft continue at the Kennedy Space Center in Florida. On April 8, the This image of the Perseverance Mars rover was taken at assembly, test and launch operations team NASA's Kennedy Space Center on April 7, 2020, during a completed a crucial mass properties test of the test of the vehicle's mass properties. Credit: NASA/JPL- rover. Caltech Precision mass properties measurements are essential to a safe landing on Mars because they help ensure that the spacecraft travels accurately Just as an auto mechanic places small weights on throughout its trip to the Red Planet—from launch a car tire's rim to bring it into balance, the through its entry, descent and landing. Perseverance team analyzed the data and then added 13.8 pounds (6.27 kilograms) to the rover's On April 6, the meticulous three-day process chassis. -
Margie Burns
Gumbo ~ The Grail Connection ~ February 2008 MEMBER GIVING ANALYSIS 2007 The 2007 Member Giving figures are in. Here’s a snapshot of how we ended the year. TOTAL 2007 MEMBER DONATIONS = $ 149,475 Reflects donations to: » The National Office » Grailville » Cornwall » Development Loan forgiveness » “Other” donations/in kind services through National Office Does not include $3,950 from U.S. members in other countries # OF MEMBERS GIVING All member categories = 144 of 242 (59.5%) Active & Wider Grail = 125 of 201 (62%) Emerita donations = $32,283 Development Loan Forgiveness = $ 22,375 Donated Salary / WIST training fees = $ 11,000 $ 33,375 MEMBER DONATIONS TO: National Office = $ 71,855 Grailville = $ 24,030 Cornwall = $ 19,240 A SPECIAL THANK YOU! TO ALL WHO FORGAVE THE LOANS THEY MADE TO THE GRAIL IN THE 1990S FOR THE ESTABLISHMENT OF A DEVELOPMENT OFFICE! 1 GENERAL ASSEMBLY 2008: JUNE 23-29 SCENARIO PLANNING FOR THE FUTURE OF THE GRAIL ~ Judith Blackburn ~ for the Council Preparation for this year’s General Assembly is now underway, and a packet of scenarios depicting the Grail of the future has been distributed to members. All of the scenarios are based on the simple fact that the Grail is not now operating on a sustainable model. Your job is to help discern how we might downsize or re-focus. Times have changed. We no longer recruit women who are able or willing to donate their working lives to the Grail. At the same time we have many ongoing obligations to each other, to our properties, and to the Grail itself. One of our strengths has been how comprehensive our programming has been, but at this juncture we MUST either simplify or scale back our operations. -
(PLEXIL) for Executable Plans and Command Sequences”, International Symposium on Artificial Intelligence, Robotics and Automation in Space (Isairas), 2005
V. Verma, T. Estlin, A. Jónsson, C. Pasareanu, R. Simmons, K. Tso, “Plan Execution Interchange Language (PLEXIL) for Executable Plans and Command Sequences”, International Symposium on Artificial Intelligence, Robotics and Automation in Space (iSAIRAS), 2005 PLAN EXECUTION INTERCHANGE LANGUAGE (PLEXIL) FOR EXECUTABLE PLANS AND COMMAND SEQUENCES Vandi Verma(1), Tara Estlin(2), Ari Jónsson(3), Corina Pasareanu(4), Reid Simmons(5), Kam Tso(6) (1)QSS Inc. at NASA Ames Research Center, MS 269-1 Moffett Field CA 94035, USA, Email:[email protected] (2)Jet Propulsion Laboratory, M/S 126-347, 4800 Oak Grove Drive, Pasadena CA 9110, USA , Email:[email protected] (3) USRA-RIACS at NASA Ames Research Center, MS 269-1 Moffett Field CA 94035, USA, Email:[email protected] (4)QSS Inc. at NASA Ames Research Center, MS 269-1 Moffett Field CA 94035, USA, Email:[email protected] (5)Robotics Institute, Carnegie Mellon University, Pittsburgh PA 15213, USA, Email:[email protected] (6)IA Tech Inc., 10501Kinnard Avenue, Los Angeles, CA 9002, USA, Email: [email protected] ABSTRACT this task since it is impossible for a small team to manually keep track of all sub-systems in real time. Space mission operations require flexible, efficient and Complex manipulators and instruments used in human reliable plan execution. In typical operations command missions must also execute sequences of commands to sequences (which are a simple subset of general perform complex tasks. Similarly, a rover operating on executable plans) are generated on the ground, either Mars must autonomously execute commands sent from manually or with assistance from automated planning, Earth and keep the rover safe in abnormal situations. -
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. -
Real-Time Fault Detection and Situational Awareness for Rovers: Report on the Mars Technology Program Task
Real-time Fault Detection and Situational Awareness for Rovers: Report on the Mars Technology Program Task Richard Dearden, Thomas Willeke Frank Hutter fRIACS, QSS Group Inc.g / NASA Ames Research Center Fachbereich Informatik M.S. 269-3, Moffett Field, CA 94035, USA Technische Universitat¨ Darmstadt, Germany fdearden,[email protected] [email protected] Reid Simmons, Vandi Verma Sebastian Thrun Carnegie Mellon University Computer Science Department, Stanford University Pittsburg, PA 15213, USA 353 Serra Mall, Gates Bldg 154 freids,[email protected] Stanford, CA 94305, USA [email protected] Abstract— An increased level of autonomy is critical for 1. INTRODUCTION meeting many of the goals of advanced planetary rover mis- This paper reports the results from a study done as part of sions such as NASA’s 2009 Mars Science Lab. One impor- NASA’s Mars Technology Program entitled “Real-time Fault tant component of this is state estimation, and in particular Detection and Situational Awareness for Rovers”. The main fault detection on-board the rover. In this paper we describe goal of this project was to develop and demonstrate a fault- the results of a project funded by the Mars Technology Pro- detection technology capable of operating on-board a Mars gram at NASA, aimed at developing algorithms to meet this rover in real-time. requirement. We describe a number of particle filtering-based algorithms for state estimation which we have demonstrated Fault diagnosis is a critical task for autonomous operation of successfully on diagnosis problems including the K-9 rover systems such as spacecraft and planetary rovers. -
Insight Spacecraft Launch for Mission to Interior of Mars
InSight Spacecraft Launch for Mission to Interior of Mars InSight is a robotic scientific explorer to investigate the deep interior of Mars set to launch May 5, 2018. It is scheduled to land on Mars November 26, 2018. It will allow us to better understand the origin of Mars. First Launch of Project Orion Project Orion took its first unmanned mission Exploration flight Test-1 (EFT-1) on December 5, 2014. It made two orbits in four hours before splashing down in the Pacific. The flight tested many subsystems, including its heat shield, electronics and parachutes. Orion will play an important role in NASA's journey to Mars. Orion will eventually carry astronauts to an asteroid and to Mars on the Space Launch System. Mars Rover Curiosity Lands After a nine month trip, Curiosity landed on August 6, 2012. The rover carries the biggest, most advanced suite of instruments for scientific studies ever sent to the martian surface. Curiosity analyzes samples scooped from the soil and drilled from rocks to record of the planet's climate and geology. Mars Reconnaissance Orbiter Begins Mission at Mars NASA's Mars Reconnaissance Orbiter launched from Cape Canaveral August 12. 2005, to find evidence that water persisted on the surface of Mars. The instruments zoom in for photography of the Martian surface, analyze minerals, look for subsurface water, trace how much dust and water are distributed in the atmosphere, and monitor daily global weather. Spirit and Opportunity Land on Mars January 2004, NASA landed two Mars Exploration Rovers, Spirit and Opportunity, on opposite sides of Mars. -
Determining Mineralogy on Mars with the Chemin X-Ray Diffractometer the Chemin Team Logo Illustrating the Diffraction of Minerals on Mars
Determining Mineralogy on Mars with the CheMin X-Ray Diffractometer The CheMin team logo illustrating the diffraction of minerals on Mars. Robert T. Downs1 and the MSL Science Team 1811-5209/15/0011-0045$2.50 DOI: 10.2113/gselements.11.1.45 he rover Curiosity is conducting X-ray diffraction experiments on the The mineralogy of the Martian surface of Mars using the CheMin instrument. The analyses enable surface is dominated by the phases found in basalt and its ubiquitous Tidentifi cation of the major and minor minerals, providing insight into weathering products. To date, the the conditions under which the samples were formed or altered and, in turn, major basaltic minerals identi- into past habitable environments on Mars. The CheMin instrument was devel- fied by CheMin include Mg– Fe-olivines, Mg–Fe–Ca-pyroxenes, oped over a twenty-year period, mainly through the efforts of scientists and and Na–Ca–K-feldspars, while engineers from NASA and DOE. Results from the fi rst four experiments, at the minor primary minerals include Rocknest, John Klein, Cumberland, and Windjana sites, have been received magnetite and ilmenite. CheMin and interpreted. The observed mineral assemblages are consistent with an also identifi ed secondary minerals formed during alteration of the environment hospitable to Earth-like life, if it existed on Mars. basalts, such as calcium sulfates KEYWORDS: X-ray diffraction, Mars, Gale Crater, habitable environment, CheMin, (anhydrite and bassanite), iron Curiosity rover oxides (hematite and akaganeite), pyrrhotite, clays, and quartz. These secondary minerals form and INTRODUCTION persist only in limited ranges of temperature, pressure, and The Mars rover Curiosity landed in Gale Crater on August ambient chemical conditions (i.e. -
Moxtek in Space Again – Mars Perseverance Rover Landing 2021 Feb 9, 2021
Moxtek in Space Again – Mars Perseverance Rover Landing 2021 Feb 9, 2021 MOXTEK, Inc. Orem, UT [email protected] MOXTEK (Orem, UT) is excited to celebrate the landing of the Perseverance rover in the Mars Jezero crater on February 18th 2021. This landing will be watched by many people around the world with anticipation as this new high‐tech rover is delivered to our red planet neighbor. Moxtek employees will also be anxiously watching as this rover, with three Moxtek products, prepares for a safe landing. Please celebrate this landing with us on February 18th @ 1:55pm MST (Utah time). The Perseverance rover, developed by NASA’s Jet Propulsion Laboratory (JPL), includes seven important instruments intended to explore and seek evidence of past life on Mars. One of these instruments, the Planetary Instrument for X‐ray Lithochemistry (PIXL), is a compact x‐ray fluorescence (XRF) spectrometer mounted at the end of the rover’s robotic arm and is designed to provide accurate identification of the elemental composition of rock and soil on Mar’s surface. The PIXL system uses three Moxtek components including a miniature x‐ray tube and two DuraBeryllium x‐ray detector windows. NASA/JPL chose Moxtek x‐ray windows because of their exceptional dependability in harsh and remote environments and chose the Moxtek x‐ray tube because of its compact design, rigidity, and low‐power consumption. The Moxtek x‐ray tube was specifically designed to couple directly to an x‐ray polycapillary optic, developed by X‐ ray Optical Systems (XOS), for the purpose of elemental mapping. Moxtek’s x‐ray tube and window enable the PIXL system to provide increased spatial resolution and improved measurement sensitivity. -
Mars Insight Launch Press Kit
Introduction National Aeronautics and Space Administration Mars InSight Launch Press Kit MAY 2018 www.nasa.gov 1 2 Table of Contents Table of Contents Introduction 4 Media Services 8 Quick Facts: Launch Facts 12 Quick Facts: Mars at a Glance 16 Mission: Overview 18 Mission: Spacecraft 30 Mission: Science 40 Mission: Landing Site 53 Program & Project Management 55 Appendix: Mars Cube One Tech Demo 56 Appendix: Gallery 60 Appendix: Science Objectives, Quantified 62 Appendix: Historical Mars Missions 63 Appendix: NASA’s Discovery Program 65 3 Introduction Mars InSight Launch Press Kit Introduction NASA’s next mission to Mars -- InSight -- will launch from Vandenberg Air Force Base in California as early as May 5, 2018. It is expected to land on the Red Planet on Nov. 26, 2018. InSight is a mission to Mars, but it is more than a Mars mission. It will help scientists understand the formation and early evolution of all rocky planets, including Earth. A technology demonstration called Mars Cube One (MarCO) will share the launch with InSight and fly separately to Mars. Six Ways InSight Is Different NASA has a long and successful track record at Mars. Since 1965, it has flown by, orbited, landed and roved across the surface of the Red Planet. None of that has been easy. Only about 40 percent of the missions ever sent to Mars by any space agency have been successful. The planet’s thin atmosphere makes landing a challenge; its extreme temperature swings make it difficult to operate on the surface. But if a spacecraft survives the trip, there’s a bounty of science to be collected.