Resource Prospector Drill

Similar documents
Drilling: How do we access subsurface on Mars

Drilling Into Mars PLD

International Planetary Probes Workshop (IPPW) June 2018 Surface and Subsurface Sampling Drills for Life Detection on Ocean Worlds

HEOMD Overview March 16, 2015

The SPE Foundation through member donations and a contribution from Offshore Europe

Advanced Miniature Linear Ion Trap Mass Spectrometer (LITMS) for Space Applications

InSight Spacecraft Launch for Mission to Interior of Mars

7th ESA Workshop on Advanced Space Technologies for Robotics and Automation 'ASTRA 2002' ESTEC, Noordwijk, The Netherlands, November 19-21, 2002

DARPA Lunar Study: Reducing the technical risk associated with lunar resource utilization and lunar surface presence

Ice on Land! Who: Dr. Waleed Abdalati University of Colorado. Where: Greenland Ice Sheet and glaciers around the world.

Lunar Discovery and Exploration program

Scientific Contributions of Lunar Robotic Precursor Missions

Lunar Exploration Requirements and Data Acquisition Architectures

Robotic Site Survey for ISRU

Technology Goals for Small Bodies

A thermal model for analysis and control of drilling in icy formations on Mars

Field Testing of K10 with HYDRA at NASA Ames Research Center

NASA Announces Mars 2020 Rover Payload to Explore the Red Planet as Never Before Mission Plans

A Physical, Chemical, Isotopic and Astrobiology Instrumentation Package

Expanding Science with SmallSats/CubeSats

Mars Sample Return (MSR) Mission BY: ABHISHEK KUMAR SINHA

LUNAR ICY SOIL SAMPLING

Asteroid Sample Return and the Path to Exploration of Near-Earth Space* By Dante S. Lauretta 1

Environmental Effects on Lunar Base Designs. Anja Garcia Center for Structures in Extreme Environment

Thermal Wadis: Using Regolith for Thermal Energy Management

Investigation of diamond-impregnated drill bit wear while drilling under Earth and Mars conditions

Exercise 1: Earth s Moon

Laboratory drilling under Martian conditions yields unexpected results

NASA: BACK TO THE MOON

Planet 2. Planet 1 Gas Giant. Planet 3. Earth

Mars Science Laboratory - Overview Mars Express Conference

By Charis Smith, Cassie Scruggs, Erol Chandler, & Shawna Fox Anderson

Appendix D. Thermal Modelling of Luna 27 Landing Site. Hannah Rana Vito Laneve Philipp Hager Thierry Tirolien (ESA/ESTEC, The Netherlands)

Conducting Subsurface Surveys for Water Ice using Ground Penetrating Radar and a Neutron Spectrometer on the Lunar Electric Rover Never Stop

PROSPECT: ESA s Package for Resource Observation and In-Situ Prospecting for Exploration, Commercial Exploitation and Transportation

Terrestrial Atmospheres

Presentation to the NAC Planetary Science Subcommittee June 7, 2007

Astrobiology in the inner Solar System

Oil and natural gas on Mars

Lecture 27: Is There Life on Mars?

Earth s Atmosphere About 10 km thick

The Main Point. Basic Properties of Mars. Observations. Lecture #19: Mars

The Moon: Stepping Stone to the Planets

Arctic Mars Analogue Svalbard Expedition An Astrobiology (ASTEP) funded testing program

Low Cost Enceladus Sample Return Mission Concept

Life in the Solar System

Exploring the Moon & Asteroids: A Synergistic Approach

Edwin Ethridge, NASA, Marshall Space Flight Center, EM40 William Kaukler, University of Alabama, Huntsville

Lunar Oxygen Production and Metals Extraction Using Ionic Liquids

Update to LEAG Annual Meeting, 11/16/09 Barbara A. Cohen J. A. Bassler, D. W. Harris, L. Hill, M. S.

Payloads. Andrew J. Ball Short Course on Small Satellites, IPPW-15 Boulder, CO, 9 June 2018

Image of the Moon from the Galileo Space Craft

Surface Observations Including from the 2012 Mars Curiosity Rover. Martian Atmosphere

CHARACTERIZING THE PERFORMANCE OF THE WHEEL ELECTROSTATIC SPECTROMETER

Lunar Cratering and Surface Composition

10/8/2013. Recent Results from Curiosity s SAM Instrument and Looking Ahead to MAVEN. Curiosity s Science Objectives. Curiosity s Science Payload

THE GAS GIANTS JUPITER VENUS MARS EARTH

NASA s Solar System Exploration Research Virtual Institute (SSERVI)

Lunar Precursor Robotics Program

Super Quiz. 4 TH Grade

In Situ Instruments for Small Body Exploration

Moon Express Advancing Commerce and Science

***Note: U.S. Citizenship is required of all participants (teacher and students).***

Advanced Probes for Planetary Surface and Subsurface Exploration

Europa Exploration: Challenges and Solutions

PSRD:: Cosmochemistry and Human Exploration

David Baxter. GK-12 Summer Research Program Brown University Oliver Hazard Perry Middle School NASA Explorer School

Iron and Titanium: Important Elements. posted October 20, References:

Plans for an International Lunar Network

Phobos/Deimos State of Knowledge in Preparation for Future Exploration

In Situ Instruments for Small Body Exploration

Detection of subsurface ice and water deposits on Mars with a mutual impedance probe

The Final Minute: Results from the LCROSS Solar Viewing NIR Spectrometer

Solar System. The Jovian Satellites. Regular vs. Irregular Satellites. Jovian satellites reside beyond the frost line

HERA MISSION & CM16 lessons learned

The Moon. Tidal Coupling Surface Features Impact Cratering Moon Rocks History and Origin of the Moon

The time period while the spacecraft is in transit to lunar orbit shall be used to verify the functionality of the spacecraft.

Mars Update. Presented by NASA/JPL Solar System Educator Don W. Brown

Mercury = Hermes Mythology. Planet Mercury, Element, Mercredi God of Commerce, Messenger God, guide to Hades Winged sandals and staff

Administrivia. Administrivia

1.2: Observing the Surfaces of Mars and Earth

Detection of Adsorbed Water and Hydroxyl on the Moon

Hermes Experiment Opportunities

COMMON THEMES IN PLANETARY SMALL BODIES RESEARCH (2018 UPDATE)

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week

High Speed Penetrator deployable mass spectrometers. Presented by Simon Sheridan The Open University on behalf of the UK Penetrator Consortium

Dive In What is an advantage of sending unmanned crafts to space?

ROSETTA: ESA's Comet Orbiter and Lander Mission. Hermann Boehnhardt Max-Planck Institute for Solar System Research Katlenburg-Lindau, Germany

Welcome! To The Restructured, Reconfigured, NASA Advisory Council!

Life and habitability in the Solar System and beyond: the Roadmap

What is there in thee, moon, That thou shouldst move My heart so potently? By John Keats

Overview of Lunar Science Objectives. Opportunities and guidelines for future missions.

Testing the Composition of Ganymede

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres

9. Moon, Mercury, Venus

Introduction to Formation Evaluation Abiodun Matthew Amao

Solar System. The Jovian Satellites. Regular vs. Irregular Satellites. Jovian satellites reside beyond the frost line

Italian Lunar Science Studies and Possible Missions a.k.a. The Moon: an Italian Approach. Angioletta Coradini Istituto Nazionale di Astrofisica

The Lunar polar Hydrogen Mapper (LunaH-Map) Mission

Rosetta. ESA s Comet Lander Mission. Andrew Morse. Open University. 3 May 2012 Keck Institute for Space Studies Pasadena

Transcription:

Resource Prospector Drill Kris Zacny, Honeybee Robotics zacny@honeybeerobotics.com Gale Paulsen, Honeybee Robotics Jackie Quinn, NASA KSC Jim Smith, NASA KSC Julie Kleinhenz, NASA GRC LEAG, 20-22 October 2015 Honeybee Robotics Spacecraft Mechanisms Corporation 398 W Washington Blvd., Suite 200, Pasadena, CA 91103 www.honeybeerobotics.com

Background: The Resource Prospector (RP) Goal: ISRU demo: Prospecting for volatiles, extraction of O2 from lunar regolith Instruments: 1. The Neutron Spectrometer Subsystem (NSS) 1. Localizing elevated H2 concentration 2. The Drill Subsystem 1. Capture samples from up to 1 m 3. The Near InfraRed Volatiles Spectrometer Subsystem (NIRVSS) 1. Characterize hydrocarbons, mineralogical context for the site, nature of water ice 4. The Oxygen and Volatile Extraction Node (OVEN) Subsystem 1. Evolve the volatiles in sample by heating and transfer to LAVA 2. Demo hydrogen reduction process (H2 reacts with iron oxide to produce water) 5. The Lunar Advanced Volatiles Analysis (LAVA) Subsystem 1. quantities and species of volatiles via GC/MS 2. Water Droplet Demonstration (WDD) Andrews et al., 2014 2

The Drill Subsystem: Background The Icebreaker drill Developed for acquisition of Ice/Ice Cemented Ground at the Mars Poles 1 m depth, 10 kg Tested in Antarctica, Arctic, Greenland Tested in Mars Chamber TRL 5/6 Goal: Turn Mars drill into Lunar drill Courtesy NASA Mars vs Moon Drill Mars: Planetary Protection Perchlorate in Ice (freezing point depression) Sticky Sample (Relative humidly up to 100%) Full autonomy (long communication delay) Moon Extreme Temperatures (40K 400K) Hard Vacuum (Ice sublimation >106 K) Teleop/supervised autonomy 3

Drilling Approaches SONIC ULTRA SONIC PERCUSSIVE ROTARY 40 kg Lander Rover 40 kg 10 kg 12 kg Final Selection: ROTARY-PERCUSSIVE 4

Complexity Sampling Trades 1. Embedded Sensor Step 1: Drill Step 2: Analyze 2. Sniffer Step 1: Drill Step 2: Acquire Sample Step 3: Analyze 3. Sampling Auger Step 1: Drill Step 2: Transfer Cuttings Step 3: Analyze 4. Bit Sampler Step 1: Drill Step 2: Pull Out Step 3: Transfer Cuttings Step 4: Analyze 5. Core Step 1: Drill Step 2: Break-off core Step 3: Capture Core Step 4: Pull out Step 5: Eject core Step 6: Process core Step 7: Analyze Science Payoff

1 st bite 2 nd bite Bite Sampling Concept Drill to 1 meter in short (~ 10 cm) bites Preserve stratigraphy in bites More accurate strength measurement of subsurface Lower risk ( graceful failure ) if stuck at 60 cm, 5 bites done Time for analysis while drill in safe place (above the hole) Time for subsurface to cool down Brush Brush

Implementation of Bite Sampling 2. Retract auger with captured cuttings NIR Spectrometer 1. Drill Bites into icebearing material Ice Bearing Material 3. Inspect cuttings with Infrared Sensor and Camera. If ice bearing material is detected, proceed to next step. Otherwise continue taking Bites 4. Rotate and retract auger to deliver ice-bearing material still within sampling system 7

Tests at NASA GRC Background: Soil: NU-LHT-3M with 4-5 water wt%, Vibratory compacted to ~1.5 g/cc Temp: -140 C to 90 C Chamber P: ~10^-6 torr Crucible T: -85 C to 50 C (+10 C) Goal: 1. Capture sample from 40 50 cm 2. Deliver to crucible 3. Seal

Cameras 9

Drill holes and crucible 7 12 8 11 10 9 Stuck Drill Test

Results Water wt% = function(temperature) Can preserve all water if T kept low Kleinhenz et al. 2015, AIAA SciTech

Drill Data Bit T was dropping during drilling because soil T was lower with depth Approx. 10 min to capture 10 cm bite

Drill Data Drilling Power ~20 Watt (percussion hardly ever used) Weight on Bit < 30 N Left drill in a hole for 45 min no problem

Drill tests at JSC. Controls in Pasadena. 14

Strength of Material from Drilling SE Strength value from drilling telemetry Drilling in three known sandstones and FJS-1 Extrapolating UCS of FJS-1 based on SE of FJS1 and the three sandstones UCS ~ 48 MPa Strength value from UCS tests UCS=43 MPa, std=11 MPa Error Dave Cole, CRREL 15

Acknowledgements NASA Small Business Innovation Research NASA Advanced Exploration Systems NASA Astrobiology Science and Technology for Exploring Planets 16

Thank You! Honeybee Robotics Spacecraft Mechanisms Corporation 398 W Washington Blvd., Suite 200, Pasadena, CA 91103 www.honeybeerobotics.com