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The Curiosity Rover: Robotic Geologist and Explorer
Presented by: Jordan Evans
May 21, 2013 6:30 p.m. – 8:00 p.m. Eastern time
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3 Introducing today’s presenters
Introducing today’s presenter…
Jordan Evans NASA’s Jet Propulsion Laboratory Pasadena, CA
4 Jet Propulsion Laboratory California Institute of Technology
The Curiosity Rover: Robotic Geologist and Explorer
Jordan Evans JPL/Caltech/NASA
5 @Jordan2Mars Brief Biography…
• Led the “Flight System” design, build, test, launch, and operations on the Mars Science Laboratory Project • Aerospace Engineering – San Diego State University and University of Maryland • Worked on both Aircraft and Spacecraft • Jazz Musician (Bass) • Bacon Maker • Science Advisor • Woodworker • Camper Restorer 6 Blaine Baggett Executive Manager, Office of Communications and Education Jet Propulsion Laboratory Pasadena, CA
7 Why Mars?
8 The wonderful future
From the 1956 book, The Exploration of Mars, by von Braun and Willy Ley, with paintings by Chesley Bonestell Mars Exploration is CHALLENGING
10 Did you watch Curiosity’s landing on the night of August 5th (PT)?
✔ Yes ✖ No
11 Did you watch Curiosity’s landing on the night of August 5th (PT)?
An estimated 50 million people watched the landing!
12 13 Only 50% of Mars landers launched have worked
USSR: Mars 2 1971 (crashed) USSR: Mars 3 1971 (landed, radio died) USSR: Mars 6 1973 (aero data, crashed?) USSR: Mars 7 1974 (missed Mars) US: Viking 1 1975 US: Viking 2 1975 USSR: Mars ‘96 (2) 1996 (failed launch) US: Mars Pathfinder 1996 US: Mars Polar Lander 1998 (crashed?) US: DS-2 Microprobes (2) 1998 (crashed?) EU/UK: Beagle II 2003 (crashed?) US: MER Spirit 2003 US: MER Opportunity 2003 US: Phoenix 2007 US: MSL Curiosity 2011 [launch dates] 14 Thousands of problems to solve.
15 Testing 17 More testing More testing More testing 2010 Finally, a real Mars Science Lab! Rover Packaging Ready for flight Ready for the fairing Encapsulation at KSC ATLAS V fairing Launch Complex 41 NASA/KSC Atlas V Careful …. MSL Launch: Nov 26, 2011 Does every Mars-faring nation use the same approach to get to Mars?
✔ Yes ✖ No
30 Does every Mars-faring nation use the same approach to get to Mars?
31 The mission …. Mission Overview
ENTRY, DESCENT, LANDING • Guided entry and powered “sky crane” descent • 20×25-km landing ellipse • Access to landing sites ±30° CRUISE/APPROACH latitude, <0 km elevation • 8.5-month cruise • 900-kg rover • Arrived August 5, 2012 SURFACE MISSION • Prime mission is one Mars year (687 days) LAUNCH • Latitude-independent and long- lived power source • Nov. 26, 2011 • Ability to drive out of landing • Atlas V (541) ellipse • 84 kg of science payload • Direct (uplink) and relayed (downlink) communication • Fast CPU and large data storage 33 Rover Family Portrait ChemCam (Chemistry) Mastcam APXS (Imaging) RAD (Chemistry) MAHLI (Radiation) (Imaging) REMS (Weather)
DAN (Subsurface Hydrogen)
Drill Scoop Brush Sieves
SAM (Chemistry CheMin MARDI and Isotopes) (Mineralogy) (Imaging) Curiosity’s Science Payload 35 What’s Under the Hood?
UHF Radio Thermal Fluid Loop Spacecraft Computers Rover Motor Controller
ChemMin Power Electronics & Batteries
X-Band Radio
SAM
36 The Complexity and Beauty of Curiosity
37 Entry, Descent, and Landing (EDL) How Did it Go?
38 39 40 41 Landing area
(photo taken by Mars Reconnaissance orbiter) Curiosity’s Descent stage
Before
After (photo taken by Mars Reconnaissance orbiter) (photos taken by Mars Reconnaissance orbiter)
44 EDL Performance Summary
Rover Cruise Stage Separation Separation Sky Crane Detail ERT: 10:14:34 PM All Times in ERT PDT Alt: 21.5 m Velo: 0.77 m/s Note: gnd solution Flyaway change of ~1m near Impact ERT: <10:32:40 PM rover sep CBMD Distance: 640 m Separation Mobility Note: Impact pattern may be different than expected ERT: 10:16:24 PM Entry Interface Deploy ERT: 10:24:33 PM Alt: 21.1 Delivery error: 0.013 deg FPA Parachute Deploy ERT: 10:28:53 PM Peak Heating Mach: 1.72 Touchdown ERT: Pending Deceleration: ~6 g’s ERT: 10:31:49 PM Qmax: Pending Note: Lower than Velo: 0.75 m/s expected parachute Lat/Lon: - Peak Deceleration inflation loads 4.5895°/137.4417° ERT: 10:17:44 PM Deceleration: ~12.2 g’s
Hypersonic Backshell Aero-maneuvering Separation Variance from Numb of bank reversals: 3 ERT: 10:30:51 prediction Heatshield Guidance performance: Separation Radar Altitude: 1670 m < 1 s Great ERT: 10:29:13 Ground Solution Velocity: 78.6 m/s Note: Possible tailwind/low Mach: Pending ERT: 10:29:21 Note: density during final 50-100 km Note: Separation Powered Descent 1-2 s FS Infrastructure Alt: 8.3 km of flight rates as expected, Duration: 37 Voltage at TD: 32.1 V Error (alt): 113.4 m no tumbling Fuel usage: 260 kg Comm: Great Error (velo): 0.7 Note: Fuel usage >2 s Prop: Good m/s was lower than Thermal: Good Note: Better range expected Mech: Good at lock-up and AVS/FSW: Good lower error than SECC: N/A expected ISAs: 52822, 52845, 53000 (see following) Sky Crane Flyaway
45 Gale Crater and Mount Sharp
46 24 47 Mt. Sharp
48 49 Curiosity’s Exploration and Science Since Landing
50 51 52 53 54 Looking North to Crater Rim
55 56 Timekeeping on Mars Timekeeping on Mars
Martian Day = “Sol” 1 Sol = 24h 39m 35s
Timekeeping on Mars
Martian Day = “Sol” 1 Sol = 24h 39m 35s
“Yestersol”
Timekeeping on Mars
Martian Day = “Sol” 1 Sol = 24h 39m 35s
“Yestersol”
“Tosol”
Timekeeping on Mars
Martian Day = “Sol” 1 Sol = 24h 39m 35s
“Yestersol”
“Tosol”
“Nextersol” “Morrowsol” “Sol-orrow” Timekeeping on Mars
Martian Day = “Sol” 1 Sol = 24h 39m 35s
“Yestersol”
“Tosol”
“Nextersol” “Morrowsol” “Sol-orrow” Recent Mars Weather
June
63 Ear-Popping Daily Pressure Changes
100 Pa swing is… 15% of Mars Pressure 0.15% of Earth Pressure
64 Driving!
65 Sol 24 Navcam: Bradbury Landing Site
66 Rover tracks
(photo taken by Mars Reconnaissance orbiter) Stretching Out the Arm for Contact Science on Rock Named “Jake Matijevic”
NASA/JPL- Caltech/MSSS Science Instruments at the End of Curiosity’s Robotic Arm
70 71 72
. --- . --. . .-- . --- J . --. P . .-- L Curiosity’s primary scientific goal is to explore and quantitatively assess a local region on Mars’ surface as a potential habitat for life, past or present • Biological potential • Geology and geochemistry • Role of water • Surface radiation
NASA/JPL-Caltech
Curiosity’s Science Objectives 77 ChemCam Laser
78 Target: Beechey (Sol 19) Power: 1 Gigawatt Shots per spot: 50
8 Before After cm( 3”) NASA/JPL- Caltech/LANL/CNES/IRAP/LPGN/CNRS ChemCam’s laser induced breakdown
79 spectrometer acquires a 5-spot raster 80 81 Remnants of Ancient Streambed on Mars
82 Atmospheric Gas SAM found that argon, Abundances rather than nitrogen is the Measured by SAM second most abundant gas SAM also found that Mars’ atmosphere is enriched in the heavy versions of isotopes, indicating that atmospheric loss has occurred
Methane has not been definitively detected
NASA/JPL-Caltech/Goddard
TLS uses infrared lasers and mirrors to measure the absorption of light by atmospheric gases
The SAM Tunable Laser Spectrometer and Mass
83 Spectrometer measure atmospheric composition Scoop and Delivery for Chemistry and Mineralogy
84 85 Sol 61: First Scoop!
86 What did Curiosity discover in the Rocknest Sand Dune?
A. A habitable environment conducive to microbial life B. Mars dust and sand dunes are a global phenomenon and aren’t necessarily habitable C. The “Rocknest Monster”
87 Gases SAM and released CheMin during SAM analyses experiments of Rocknest
Sand composed of unaltered basaltic NASA/JPL- Caltech/Ames minerals, NASA/JPL- similar to soils Caltech/MSSSNASA/JPL- on Mars Caltech/Goddard
Also evidence for water, sulfates, carbonates, and X-ray potentially perchlorates diffraction pattern from
88 CheMin
How far across SDSU would Curiosity have travelled in the 9 months thus far? How far across SDSU would Curiosity have travelled in the 9 months thus far?
Aztec Center Current Position ✖ Sols 55-100
Sol Sol Sol 120 43 39 MSL Rotary-Percussive Drill in Testbed at JPL Heading into Yellowknife Bay
NASA/JPL- Caltech/MSSS
94 NASA/JPL-Caltech/MSSS Postcards from Yellowknife Bay 95 NASA/JPL-Caltech ChemCam Remote Micro- Imager
NASA/JPL- Caltech/LANL/CNES/IRAP/ LPGNantes/CNRS/LGLyon/Planet- Terre ChemCam spectra from sol 125 “Crest” and 135 “Rapitan” “Sheepbed” rocks contain 1 to 5-mm fractures filled with calcium sulfate minerals that precipitated from fluids at low to moderate temperatures 96 NASA/JPL-Caltech/MSSS Spherules Suggest Water Percolation
97
NASA/JPL- Caltech/LANL/CNES/IRAP/LPG Nantes/CNRS 101 Drilling at John Klein: A “Goldmine” of Info
102 Drilling at John Klein: A “Goldmine” of Info
Wet Neutral pH Energy Gradients (Oxidation) Mildly Salty Key Chemicals (C,H,N,O,P,S)
103 Drilling at John Klein: A “Goldmine” of Info
Wet Neutral pH Energy Gradients (Oxidation) Mildly Salty Key Chemicals (C,H,N,O,P,S)
Conditions Favorable for Life!
104 105
“Cumberland” – Curiosity’s Second Drill Target What’s Next for Curiosity?
108 Curiosity’s Ultimate Goal: Mount Sharp
NASA/JPL-Caltech/Univ. of 109 Arizona 110 NASA/JPL- Caltech/MSSS 111 NASA/JPL- Caltech/MSSS Layers, Canyons, and Buttes of Mount Sharp
112 This boulder is the size of Curiosity
Layers, Canyons, and Buttes of Mount Sharp
113 114 Questions?
115 Introducing today’s presenters
Thanks to today’s presenter!
Jordan Evans NASA’s Jet Propulsion Laboratory Pasadena, CA
116 Thank you to the sponsor of tonight’s web seminar—1 of 6
Thank you to the sponsor of tonight’s web seminar:
This web seminar contains information about programs, products, and services offered by third parties, as well as links to third-party websites. The presence of a listing or such information does not constitute an endorsement by NSTA of a particular company or organization, or its programs, products, or services. 117 Thank you to NSTA administration—2 of 6
National Science Teachers Association David Evans, Ph.D., Executive Director Zipporah Miller, Associate Executive Director, Conferences and Programs
NSTA Web Seminar Team Al Byers, Ph.D., Assistant Executive Director, e-Learning and Government Partnerships Brynn Slate, Manager, Web Seminars, Online Short Courses, and Symposia Jeff Layman, Technical Coordinator, Web Seminars, SciGuides, and Help Desk
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