MAHLI on Mars: lessons learned operating a geoscience camera on a landed payload robotic arm

Abstract. The Mars Hand Lens Imager (MAHLI) is a 2-megapixel, color camera with resolution as high as 13.9 µm pixel−1. MAHLI has operated successfully on the Martian surface for over 1150 Martian days (sols) aboard the Mars Science Laboratory (MSL) rover, Curiosity. During that time MAHLI acquired images to support science and science-enabling activities, including rock and outcrop textural analysis; sand characterization to further the understanding of global sand properties and processes; support of other instrument observations; sample extraction site documentation; range-finding for arm and instrument placement; rover hardware and instrument monitoring and safety; terrain assessment; landscape geomorphology; and support of rover robotic arm commissioning. Operation of the instrument has demonstrated that imaging fully illuminated, dust-free targets yields the best results, with complementary information obtained from shadowed images. The light-emitting diodes (LEDs) allow satisfactory night imaging but do not improve daytime shadowed imaging. MAHLI's combination of fine-scale, science-driven resolution, RGB color, the ability to focus over a large range of distances, and relatively large field of view (FOV), have maximized the return of science and science-enabling observations given the MSL mission architecture and constraints.

[1]  Kenneth S. Edgett,et al.  The Mars Science Laboratory APXS calibration target: Comparison of Martian measurements with the terrestrial calibration , 2014 .

[2]  K. Herkenhoff,et al.  MAHLI After Dark: Nighttime Mars Hand Lens Imager Observations Under LED Illumination , 2014 .

[3]  M. Saccoccio,et al.  The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Science Objectives and Mast Unit Description , 2012 .

[4]  K. Herkenhoff,et al.  Mars Hand Lens Imager (MAHLI) Observations at the Pahrump Hills Field Site, Gale Crater , 2015 .

[5]  Luther W. Beegle,et al.  Collecting Samples in Gale Crater, Mars; an Overview of the Mars Science Laboratory Sample Acquisition, Sample Processing and Handling System , 2012 .

[6]  E. Sebastián,et al.  REMS: The Environmental Sensor Suite for the Mars Science Laboratory Rover , 2012 .

[7]  A. Yingst,et al.  A Habitable Fluvio-Lacustrine Environment at Yellowknife Bay, Gale Crater, Mars , 2014, Science.

[8]  Reg G. Willson,et al.  Curiosity’s Mars Hand Lens Imager (MAHLI) Investigation , 2012 .

[9]  R. V. Morris,et al.  Curiosity at Gale Crater, Mars: Characterization and Analysis of the Rocknest Sand Shadow , 2013, Science.

[10]  R. Anderson,et al.  Mars Science Laboratory Mission and Science Investigation , 2012 .

[11]  A. Knoll,et al.  Stratigraphy and sedimentology of a dry to wet eolian depositional system, Burns formation, Meridiani Planum, Mars , 2005 .

[12]  Reg G. Willson,et al.  Supplement (.zip file to download) to PRE-PRINT Edgett et al. - Curiosity’s robotic arm-mounted Mars Hand Lens Imager (MAHLI): Characterization and calibration status , 2015 .

[13]  R. E. Arvidson,et al.  Deposition, exhumation, and paleoclimate of an ancient lake deposit, Gale crater, Mars , 2015, Science.

[14]  Linda C. Kah,et al.  Diagenetic origin of nodules in the Sheepbed member, Yellowknife Bay formation, Gale crater, Mars , 2014 .

[15]  Linda C. Kah,et al.  MAHLI at the Rocknest sand shadow: Science and science‐enabling activities , 2013 .

[16]  N. Bridges,et al.  Transverse Aeolian Ridges (TARs) as Megaripples: Rover Encounters at Meridiani Planum, Gusev, and Gale , 2014 .

[17]  D. D. Des Marais,et al.  Biosignature Preservation and Detection in Mars Analog Environments , 2017, Astrobiology.

[18]  Won S. Kim,et al.  Test and validation of the Mars Science Laboratory Robotic Arm , 2013, 2013 8th International Conference on System of Systems Engineering.

[19]  R. Aileen Yingst,et al.  TERRAIN ASSESSMENT IN GALE CRATER FROM SOL 0-500 USING ORBITAL THERMAL INERTIA AND IN SITU VISIBLE DATA , 2014 .

[20]  R. Wiens,et al.  Overview of the Mars Science Laboratory mission: Bradbury Landing to Yellowknife Bay and beyond , 2014 .

[21]  N. Bridges,et al.  The ChemCam Instrument Suite on the Mars Science Laboratory (MSL) Rover: Body Unit and Combined System Tests , 2012 .

[22]  Dawn Y Sumner,et al.  Preservation of martian organic and environmental records: final report of the Mars biosignature working group. , 2011, Astrobiology.

[23]  K. Edgett,et al.  MSL‐APXS titanium observation tray measurements: Laboratory experiments and results for the Rocknest fines at the Curiosity field site in Gale Crater, Mars , 2014 .

[24]  E. A. Guinness,et al.  Ancient Aqueous Environments at Endeavour Crater, Mars , 2014, Science.

[25]  R. C. Wiens,et al.  Martian Fluvial Conglomerates at Gale Crater , 2013, Science.

[26]  C. Wentworth A Scale of Grade and Class Terms for Clastic Sediments , 1922, The Journal of Geology.

[27]  B. A. Cohen,et al.  A Test of Two Field Methods: Determining Best Practices in Reconnoitering Sites for Habitability Potential Using a Semi-Autonomous Rover , 2015 .

[28]  P. Conrad,et al.  The Mars Science Laboratory Organic Check Material , 2012 .