Title: Autonomous Drilling in Extreme Environments
1Autonomous Drillingin Extreme Environments
- Gregory A. Dorais
- NASA Ames Research Center
2Outline
- Background
- Motivation
- Challenges
- Current Efforts
- Candidate Architecture
3Background
Technical Areas
4Background Deep-hole Drilling
- 200m holes regularly drilled in China in 1100s
(In 1132, 4900 brine wells were registered in
Sichuan province alone) - Xinhai well drilled to 1001m in 1835
- First steam-powered drill rig is operational in
1856 - 12,261m hole was drilled in the Kola peninsula,
Russia, 1970 - 1989
5Background Deep-hole Drilling (cont.)
- Holes are generally either drilled or cored
- Holes can be lined or left unlined. Frequently
holes are only lined where needed. Liners can be
continuous or segmented. - Motor can be located on the surface or near the
bit. - Hole diameter can be constant or reduce with
depth. - Holes can be straight or vary directionally
- Semi-autonomous directional drilling is current
state-of-the art. Such drills can follow a
horizontal stratum less than 1m thick. - A variety of sensor measurements can be made
while drilling or down-hole when drilling stops
6Drilling Down-hole Science Sensors
Gamma Ray (U,Th,K) Spontaneous Potential Sonic De
nsity Neutron (scatter) Photoelectric
Absorption Neutron Activation (inelastic
capture) Galvanic Resistivity (laterolog) Inducti
on Resistivity Nuclear Magnetic Resonance
(NMR) Dielectric Electrical Borehole
Image Acoustic Borehole Image Video Image
? - yes ? - dont know X - no
Open Hole (fluid filled) Open Hole (air
filled) Steel Cased Hole Fiberglass Cased Hole
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Presented by Quinn Passey, Exxon-Mobil, at Mars
Drilling Feasibility Workshop, D. Beaty, S.
Miller, Houston, TX, 2/27/2001
7Background Extreme Environments
- Characteristics
- Temperature, e.g., Eros varies -150 to 100C
- Pressure
- Gravity
- Radiation
- Stability
- Accessibility
- Uncertainty
8Background Autonomy Robotics
- Deep Space 1 spacecraft
- Launched 10/98
- Technologies Flight Validated
- Remote Agent Autonomous Control System
Demonstration(model-based, goal-oriented),
included - Planner/Scheduler
- Mode Identification Recovery
- Reactive Executive
- Autonomous Navigation System
9Motivation
- Exploring Earths extremes doesnt appear to have
been or will be a driver of autonomous drilling
technology research (much less expensive to have
people nearby drill site). - Two primary drivers are
- Cost-efficient production holes, e.g., oil.
- Space exploration
- Moons Luna, Europa, Titan
- Planets Mars, Venus, Mercury
- Asteroids
- Comets
10Motivation (cont.)
- Space exploration includes
- Astrobiology organic molecules, extinct and
extant life - Geology composition, physical properties, and
age of strata - Climatology climate history and its effect on
crust - Lithospheric Rheology, e.g., volcanism, tectonics
- Search for resources, e.g., water, minerals
Graphic from Mars Drilling Feasibility Workshop,
Introduction, D. Beaty, S. Miller, Houston, TX,
2/27/2001
11Challenges
- Extreme is an relative term earth vs. space
extremes. Unclear how much more difficult
drilling in various space extreme environments
is. - Drill Platform mobility (multi-hole capability?)
- Small hole diameter (e.g., miniaturization of
sensors) - Low power and mass budgets (limits redundancy and
backup resources equipment) - Cuttings removal (dry?)
- Down-force application (weight-on-bit)
- Bottom Hole Assembly Cooling
- Bit control, localization, and telemetry
- Contamination of samples and hole walls
- Core removal and sample handling attempt to
maintain core temperature and pressure
12Challenges (cont.)
- COTS autonomous control systems mostly limited to
nominal operations - Resource Management
- Low power, significantly varies during day and
between days - Limited consumables, e.g., bits
- Stuck Equipment
- Mechanical Failure
- Self-maintenance, condition-based
- Autonomous recovery
- Unknown material in strata (e.g., risk of
pressurized/gaseous zones) - Hole Instability
- Hole stabilization (e.g., liners)
- Cave-in removal
13Drilling Hole-diameter Analysis
- A commercial drilling contractor, if asked to
drill a hole 5km deep in unknown terrain, would - bring in at least 50 tons of equipment
- use a prime mover with at least 50 kW of power
- producing a hole averaging perhaps 20 cm in
diameter. - The volume of this hole would be at about 160
cubic meters - the energy delivered to the rock face would about
50 Gj, - equivalent to over 17 kW for 100 eight hour days
of drilling. - This is vastly more mass and power than can be
landed on Mars in a near-term subsurface
exploration mission.
Presented by Brian Wilcox, JPL, at Mars Drilling
Feasibility Workshop, D. Beaty, S. Miller,
Houston, TX, 2/27/2001
14Comparison of Technology Challenges for Mars
YearDepth
Key for Technology Challenge 1 Greatest 8
Least
2014 missions assume successful 2007 mission
Chart from Technology Breakout Session, Mars
Drilling Feasibility Workshop, D. Beaty, S.
Miller, Houston, TX, 2/27/2001
152007 Smart Lander Mission Concept
- Conduct Significant
- Science
- Sub-surface drilling
- In-situ soil/rock analysis
- Atmospheric measurements
SURFACE MOBILITY
- Demonstrate Next-Generation
- Lander/Rover Capabilities
- Global access
- latitude range
- surface elevation
- rugged terrain
- Accurate/safe landing
- Go-to mobility
- Extended mission operations
GUIDED ENTRY
- Approach
- Strong, multi-
- disciplinary team
- NASA centers
- Industry
- Universities
- Early pre-project
- with extensive
- technology program
HAZARD DETECTION/AVOIDANCE
No strawman payload yet defined, examples of
possible experiments listed
ROBUST TOUCHDOWN SYSTEM
Presented by Sam Thurman, JPL, at Mars Drilling
Feasibility Workshop, D. Beaty, S. Miller,
Houston, TX, 2/27/2001
162007 Smart Lander/Rover Concept
1st Generation EDL System
N
Note that lower 1/3 of image is often shadowed
2nd Generation EDL System
99 dispersions shown
NOTE grid squares are 10 ? 10 km
- Target Crater in Elysium Planitia
- 36.7 N Lat., 252.3 W Lon.
- 10 km diameter
- Contains gully features
- Go-to Rover Traverse Capability
- Target site chosen for safety
- Rover capability employed to reach
- surface features of interest
Presented by Sam Thurman, JPL, at Mars Drilling
Feasibility Workshop, D. Beaty, S. Miller,
Houston, TX, 2/27/2001
17Pallet Landing System with Fixed Payload
Presented by Tom Rivellini, JPL, at Mars Drilling
Feasibility Workshop, D. Beaty, S. Miller,
Houston, TX, 2/27/2001
18Drill Concepts for 2007 Mission
- 2m drill on Rover (low risk, mobile)
- 20m Auger Drill (med. risk)
- 20-200m Coiled Tube Drill (med. risk)
- 300-500m Worm drill (high risk, no core samples)
19Sample Drill Algorithm
20Sensors for Drilling Control
- Weight-on-bit
- Rate-of-penetration
- Rotation Rate
- Bit Torque
- Temperature
- Bit Depth
- Core Length
- Bottom-Hole Assembly Lift Weight
- X, Y Translation
- 6-DOF Inertia
- Gas Pressure
- Multi-spectral Imager
- Gamma Ray
- Neutron/Density
21Candidate Architecture
On-board Control System
System Environment Models, Procedures,
Constraints, Heuristics
Drilling and Sample Analysis Experts
Declarative/ReactivePlanners
plan requests
Ground Control System
Communication Network
plans
Plan Runner
Plan/State Database
Communication Mgr.
Communication Mgr.
high-level commands
state/health
AdaptiveControllers
AdaptiveControllers
Autonomous Drilling Management System
Core Bore Hole Data Analysis System
low-level commands
Core Handling Module Sensors Actuators
State/Health Estimator
signals
Bottom Hole Assembly Sensors Actuators
signals
physics
physics
Resources, e.g., energy, consumables
Ground Operator
Principal Investigator
Hole Environment
Surface Environment
22Reference
- Report on the Mars Drilling Feasibility Workshop
of February 27-28, 2001, Lunar and Planetary
Institute, Houston, TX, eds. Dave Beaty and
Sylvia Miller, JPL.