title: Drilling systems for extraterrestrial subsurface exploration.
abstract: Drilling consists of 2 processes: breaking the formation with a bit and removing the drilled cuttings. In rotary drilling, rotational speed and weight on bit are used to control drilling, and the optimization of these parameters can markedly improve drilling performance. Although fluids are used for cuttings removal in terrestrial drilling, most planetary drilling systems conduct dry drilling with an auger. Chip removal via water-ice sublimation (when excavating water-ice-bound formations at pressure below the triple point of water) and pneumatic systems are also possible. Pneumatic systems use the gas or vaporization products of a high-density liquid brought from Earth, gas provided by an in situ compressor, or combustion products of a monopropellant. Drill bits can be divided into coring bits, which excavate an annular shaped hole, and full-faced bits. While cylindrical cores are generally superior as scientific samples, and coring drills have better performance characteristics, full-faced bits are simpler systems because the handling of a core requires a very complex robotic mechanism. The greatest constraints to extraterrestrial drilling are (1) the extreme environmental conditions, such as temperature, dust, and pressure; (2) the light-time communications delay, which necessitates highly autonomous systems; and (3) the mission and science constraints, such as mass and power budgets and the types of drilled samples needed for scientific analysis. A classification scheme based on drilling depth is proposed. Each of the 4 depth categories (surface drills, 1-meter class drills, 10-meter class drills, and deep drills) has distinct technological profiles and scientific ramifications.
authors.affiliation: Honeybee Robotics Spacecraft Mechanisms Corporation, New York, NY 10001, USA. zacny@honeybeerobotics.com
authors.forename: K
authors.initials: K
authors.lastname: Zacny
authors.forename: Y
authors.initials: Y
authors.lastname: Bar-Cohen
authors.forename: M
authors.initials: M
authors.lastname: Brennan
authors.forename: G
authors.initials: G
authors.lastname: Briggs
authors.forename: G
authors.initials: G
authors.lastname: Cooper
authors.forename: K
authors.initials: K
authors.lastname: Davis
authors.forename: B
authors.initials: B
authors.lastname: Dolgin
authors.forename: D
authors.initials: D
authors.lastname: Glaser
authors.forename: B
authors.initials: B
authors.lastname: Glass
authors.forename: S
authors.initials: S
authors.lastname: Gorevan
authors.forename: J
authors.initials: J
authors.lastname: Guerrero
authors.forename: C
authors.initials: C
authors.lastname: McKay
authors.forename: G
authors.initials: G
authors.lastname: Paulsen
authors.forename: S
authors.initials: S
authors.lastname: Stanley
authors.forename: C
authors.initials: C
authors.lastname: Stoker
mesh_terms: D005118:Extraterrestrial Environment / Q000737:chemistry*; D007834:Lasers; D018535:Mars; D012371:Robotics; D012987:Soil / Q000032:analysis; D013026:Space Flight / Q000295:instrumentation*; D014465:Ultrasonics; D014481:United States; D018557:United States National Aeronautics and Space Administration
chemical_list: D012987:Soil