Mars Science Laboratory: Entry, Descent, and Landing System Performance
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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. -
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. -
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. -
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. -
Telephone Remarks to the National Aeronautics and Space
Aug. 13 / Administration of Barack Obama, 2012 Telephone Remarks to the National Aeronautics and Space Administration’s Mars Science Laboratory Team at the Jet Propulsion Laboratory in Pasade- na, California August 13, 2012 The President. Hello, everybody. not know before and laying the groundwork for Jet Propulsion Laboratory Director Charles an even more audacious undertaking in the fu- Elachi. Good morning, Mr. President. ture, and that’s a human mission to the Red The President. Who am I speaking with? Planet. Director Elachi. This is Charles Elachi, the I understand there’s a special Mohawk guy director of JPL. And we have a room full of the that’s working on the mission. [Laughter] He’s mission operation personnel. This is Curiosity been one of the many stars of the show last mission operation on Mars. Sunday night. And I, in the past, thought about The President. Well, it is great to talk to all getting a Mohawk myself—[laughter]—but my of you. And I just want you to know that we team keeps on discouraging me. And now that could not be more excited about what you’ve he’s received marriage proposals and thou- been doing. sands of new Twitter followers, I think that I’m Somebody asked me the other day whether going to go back to my team and see if it makes you’ve already found Martians. [Laughter] I sense. [Laughter] told them we have to give you a little bit of Director Elachi. That’s going to be the new time. But we know you’re all hard at work and fashion at JPL. -
Review of the Government Trade, Tourism and Investment Strategy
Foreword Creating more and better jobs is the Government’s first priority. As Ireland emerges from its financial assistance programme, the Government has set out the target of achieving full employment by 2020. This is a challenging goal, but one that we must achieve, if we are to ensure that there are opportunities for all our people to enjoy the dignity of work and improving living standards. To reach this objective, we are determined to redouble our efforts across all Departments and State agencies to enhance employment creation and economic growth. This review of Ireland’s Trade, Tourism and Investment Strategy is an integral part of that process. Since the Strategy was published in 2010, Ireland has been through a major financial and economic crisis, but is now moving back to a sustainable model of export-led economic growth. Export performance has been strong, and our State agencies, strongly supported by our Embassy network, have been successful both in building new markets, and in attracting inward investment. At this point in the Strategy, Enterprise Ireland expects to have achieved its end-2015 target of increasing client company exports by 33% by the end of 2013 and Bord Bia has reported record exports for the food sector. 2013 was also an outstanding success for the tourism sector, and there are now record numbers of people employed by IDA Ireland clients. We must now build on those achievements. The purpose of this review is to look again at our Strategy to create employment by increasing trade, tourism and attracting further inward investment. -
The Cassini-Huygens Mission Overview
SpaceOps 2006 Conference AIAA 2006-5502 The Cassini-Huygens Mission Overview N. Vandermey and B. G. Paczkowski Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 The Cassini-Huygens Program is an international science mission to the Saturnian system. Three space agencies and seventeen nations contributed to building the Cassini spacecraft and Huygens probe. The Cassini orbiter is managed and operated by NASA's Jet Propulsion Laboratory. The Huygens probe was built and operated by the European Space Agency. The mission design for Cassini-Huygens calls for a four-year orbital survey of Saturn, its rings, magnetosphere, and satellites, and the descent into Titan’s atmosphere of the Huygens probe. The Cassini orbiter tour consists of 76 orbits around Saturn with 45 close Titan flybys and 8 targeted icy satellite flybys. The Cassini orbiter spacecraft carries twelve scientific instruments that are performing a wide range of observations on a multitude of designated targets. The Huygens probe carried six additional instruments that provided in-situ sampling of the atmosphere and surface of Titan. The multi-national nature of this mission poses significant challenges in the area of flight operations. This paper will provide an overview of the mission, spacecraft, organization and flight operations environment used for the Cassini-Huygens Mission. It will address the operational complexities of the spacecraft and the science instruments and the approach used by Cassini- Huygens to address these issues. I. The Mission Saturn has fascinated observers for over 300 years. The only planet whose rings were visible from Earth with primitive telescopes, it was not until the age of robotic spacecraft that questions about the Saturnian system’s composition could be answered. -
Mars Exploration Entry, Descent and Landing Challenges1,2
Mars Exploration Entry, Descent and Landing Challenges1,2 Robert D. Braun Robert M. Manning Georgia Institute of Technology Jet Propulsion Laboratory Atlanta, GA 30332-0150 California Institute of Technology (404) 385-6171 Pasadena, CA 91109 [email protected] (818) 393-7815 [email protected] Abstract—The United States has successfully landed five interesting locations within close proximity (10’s of m) of robotic systems on the surface of Mars. These systems all pre-positioned robotic assets. These plans require a had landed mass below 0.6 metric tons (t), had landed simultaneous two order of magnitude increase in landed footprints on the order of hundreds of km and landed at sites mass capability, four order of magnitude increase in landed below -1 km MOLA elevation due the need to perform accuracy, and an entry, descent and landing operations entry, descent and landing operations in an environment sequence that may need to be completed in a lower density with sufficient atmospheric density. Current plans for (higher surface elevation) environment. This is a tall order human exploration of Mars call for the landing of 40-80 t that will require the space qualification of new EDL surface elements at scientifically interesting locations within approaches and technologies. close proximity (10’s of m) of pre-positioned robotic assets. This paper summarizes past successful entry, descent and Today, robotic exploration systems engineers are struggling landing systems and approaches being developed by the with the challenges of increasing landed mass capability to 1 robotic Mars exploration program to increased landed t while improving landed accuracy to 10’s of km and performance (mass, accuracy and surface elevation). -
Mars Reconnaissance Orbiter's High Resolution Imaging Science
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112, E05S02, doi:10.1029/2005JE002605, 2007 Click Here for Full Article Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HiRISE) Alfred S. McEwen,1 Eric M. Eliason,1 James W. Bergstrom,2 Nathan T. Bridges,3 Candice J. Hansen,3 W. Alan Delamere,4 John A. Grant,5 Virginia C. Gulick,6 Kenneth E. Herkenhoff,7 Laszlo Keszthelyi,7 Randolph L. Kirk,7 Michael T. Mellon,8 Steven W. Squyres,9 Nicolas Thomas,10 and Catherine M. Weitz,11 Received 9 October 2005; revised 22 May 2006; accepted 5 June 2006; published 17 May 2007. [1] The HiRISE camera features a 0.5 m diameter primary mirror, 12 m effective focal length, and a focal plane system that can acquire images containing up to 28 Gb (gigabits) of data in as little as 6 seconds. HiRISE will provide detailed images (0.25 to 1.3 m/pixel) covering 1% of the Martian surface during the 2-year Primary Science Phase (PSP) beginning November 2006. Most images will include color data covering 20% of the potential field of view. A top priority is to acquire 1000 stereo pairs and apply precision geometric corrections to enable topographic measurements to better than 25 cm vertical precision. We expect to return more than 12 Tb of HiRISE data during the 2-year PSP, and use pixel binning, conversion from 14 to 8 bit values, and a lossless compression system to increase coverage. HiRISE images are acquired via 14 CCD detectors, each with 2 output channels, and with multiple choices for pixel binning and number of Time Delay and Integration lines. -
Finalprogram-V1.Pdf
Front Cover Image: Top Right: The Mars Science laboratory Curiosity Rover successfully landed in Gale Crater on August 6, 2012. Credit: NASA /Jet Propulsion Laboratory. Upper Middle: The Dragon spacecraft became the first commercial vehicle in history to successfully attach to the International Space Station May 25, 2012. Credit: Space Exploration Technologies (SpaceX). Lower Middle: The Dawn Spacecraft enters orbit about asteroid Vesta on July 16, 2011. Credit: Orbital Sciences Corporation and NASA/Jet Propulsion Laboratory, California Institute of Technology. Lower Right: GRAIL-A and GRAIL-B spacecraft, which entered lunar orbit on December 31, 2011 and January 1, 2012, fly in formation above the moon. Credit: Lockheed Martin and NASA/Jet Propulsion Laboratory, California Institute of Technology. Lower Left: The Dawn Spacecraft launch took place September 27, 2007. Credit: Orbital Sciences Corporation and NASA/Jet Propulsion Laboratory, California Institute of Technology. Program sponsored and provided by: 23 rd AAS / AIAA Space Flight Mechanics Meeting Page 1 Table of Contents Registration ..................................................................................................................................... 4 Schedule of Events .......................................................................................................................... 5 Conference Center Layout .............................................................................................................. 7 Special Events ................................................................................................................................ -
Burkhard Bilger a New Era in Mars Exploration the New Yorker
Burkhard Bilger: A New Era in Mars Exploration : The New Yorker http://www.newyorker.com/reporting/2013/04/22/130422fa_fact_b... A REPORTER AT LARGE THE MARTIAN CHRONICLERS A new era in planetary exploration. by Burkhard Bilger APRIL 22, 2013 Print More Share Close Reddit Linked In Email The view from inside Gale Crater, the landing place of the rover Curiosity. Eight months after touching down safely, the rover has already found an ancient lake bed laced with carbon, hydrogen, nitrogen, oxygen, phosphorus, and sulfur—the building blocks of life. here once were two planets, new to the galaxy Tand inexperienced in life. Like fraternal twins, they were born at the same time, about four and a half billion years ago, and took roughly the same shape. Both were blistered with volcanoes and etched with watercourses; both circled the same yellow dwarf star—close enough to be 1 of 21 5/2/13 11:32 AM Burkhard Bilger: A New Era in Mars Exploration : The New Yorker http://www.newyorker.com/reporting/2013/04/22/130422fa_fact_b... warmed by it, but not so close as to be blasted to a cinder. Had an alien astronomer swivelled his telescope toward them in those days, he might have found them equally promising—nurseries in the making. They were large enough to hold their gases close, swaddling themselves in atmosphere; small enough to stay solid, never swelling into gaseous giants. They were “Goldilocks planets,” our own astronomers would say: just right for life. The rest is prehistory. On Earth, the volcanoes filled the air with water vapor and carbon dioxide. -
Curiosity Sets Down Safely on Mars Six-Wheeled Robot Now Set to Begin Its Multi-Year Mission at Gale Crater
NATURE | BREAKING NEWS Curiosity sets down safely on Mars Six-wheeled robot now set to begin its multi-year mission at Gale Crater. Eric Hand 06 August 2012 PASADENA, CALIFORNIA “It’s the wheel! It’s the wheel!” NASA/JPL-Caltech Ready to roll: Curiosity's first glimpse from Gale The jubilant shout was heard over cheers and exclamations as team members with Crater. NASA’s Mars Science Laboratory — also known as Curiosity — watched the first image from their spacecraft flash up on a control room screen here at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, just minutes after it landed. The picture capped off a dramatic descent sequence that deposited the rover on the surface of Mars at 10:32 p.m. Pacific daylight time on 5 August. Although not a beautiful image — it was shot through a lens cover by the rover’s rear hazard camera — the picture was enough to show one of Curiosity’s wheels resting firmly on the Martian soil. Off in the distance, the curving horizon beckons. After an 8-month journey, Curiosity survived its violent, 7-minute fall through the thin atmosphere of Mars before touching down with a speed of less than 1 metre per second, the softest landing in Mars exploration history. The feat proved that the mission's wickedly complicated landing system was as robust as advertised. The 900-kilogram rover touched down at the bottom of Gale Crater, a 154-kilometre-wide pit the size of Kuwait, where it will begin its search for past habitable environments.