Water equivalent hydrogen estimates from the first 200 sols of Curiosity's traverse (Bradbury Landing to Yellowknife Bay): Results from the Dynamic Albedo of Neutrons (DAN) passive mode experiment

C. G. Tate, J. Moersch, I. Jun, D. W. Ming, I. Mitrofanov, M. Litvak, A. Behar, W. V. Boynton, L. Deflores, D. Drake, B. Ehresmann, F. Fedosov, D. Golovin, Craig Hardgrove, K. Harshman, D. M. Hassler, A. S. Kozyrev, R. Kuzmin, D. Lisov, A. MalakhovR. Milliken, M. Mischna, M. Mokrousov, S. Nikiforov, A. B. Sanin, R. Starr, A. Varenikov, A. Vostrukhin, C. Zeitlin

Research output: Contribution to journalArticle

10 Citations (Scopus)

Abstract

The Dynamic Albedo of Neutrons (DAN) experiment on the Mars Science Laboratory (MSL) rover Curiosity is designed to detect neutrons to determine hydrogen abundance within the subsurface of Mars (Mitrofanov, I.G. et al. [2012]. Space Sci. Rev. 170, 559-582. http://dx.doi.org/10.1007/s11214-012-9924-y; Litvak, M.L. et al. [2008]. Astrobiology 8, 605-613. http://dx.doi.org/10.1089/ast.2007.0157). While DAN has a pulsed neutron generator for active measurements, in passive mode it only measures the leakage spectrum of neutrons produced by the Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) and Galactic Cosmic Rays (GCR). DAN passive measurements provide better spatial coverage than the active measurements because they can be acquired while the rover is moving. Here we compare DAN passive-mode data to models of the instrument's response to compositional differences in a homogeneous regolith in order to estimate the water equivalent hydrogen (WEH) content along the first 200 sols of Curiosity's traverse in Gale Crater, Mars. WEH content is shown to vary greatly along the traverse. These estimates range from 0.5. ±. 0.1. wt.% to 3.9. ±. 0.2. wt.% for fixed locations (usually overnight stops) investigated by the rover and 0.6. ±. 0.2. wt.% to 7.6. ±. 1.3. wt.% for areas that the rover has traversed while continuously acquiring DAN passive data between fixed locations. Estimates of WEH abundances at fixed locations based on passive mode data are in broad agreement with those estimated at the same locations using active mode data. Localized (meter-scale) anomalies in estimated WEH values from traverse measurements have no particular surface expression observable in co-located images. However at a much larger scale, the hummocky plains and bedded fractured units are shown to be distinct compositional units based on the hydrogen content derived from DAN passive measurements. DAN passive WEH estimates are also shown to be consistent with geologic models inferred from other MSL instruments, which indicate that fluvial/lacustrine activity occurred at certain locations (e.g., Yellowknife Bay).

Original languageEnglish (US)
Pages (from-to)102-123
Number of pages22
JournalIcarus
Volume262
DOIs
StatePublished - Dec 1 2015
Externally publishedYes

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landing
albedo
hydrogen
neutrons
estimates
Mars
water
experiment
Mars craters
regolith
thermoelectric generators
cosmic ray
exobiology
crater
leakage
radionuclide
plains
anomaly
mars
generators

Keywords

  • Cosmic rays
  • Mars
  • Mars, surface

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Water equivalent hydrogen estimates from the first 200 sols of Curiosity's traverse (Bradbury Landing to Yellowknife Bay) : Results from the Dynamic Albedo of Neutrons (DAN) passive mode experiment. / Tate, C. G.; Moersch, J.; Jun, I.; Ming, D. W.; Mitrofanov, I.; Litvak, M.; Behar, A.; Boynton, W. V.; Deflores, L.; Drake, D.; Ehresmann, B.; Fedosov, F.; Golovin, D.; Hardgrove, Craig; Harshman, K.; Hassler, D. M.; Kozyrev, A. S.; Kuzmin, R.; Lisov, D.; Malakhov, A.; Milliken, R.; Mischna, M.; Mokrousov, M.; Nikiforov, S.; Sanin, A. B.; Starr, R.; Varenikov, A.; Vostrukhin, A.; Zeitlin, C.

In: Icarus, Vol. 262, 01.12.2015, p. 102-123.

Research output: Contribution to journalArticle

Tate, CG, Moersch, J, Jun, I, Ming, DW, Mitrofanov, I, Litvak, M, Behar, A, Boynton, WV, Deflores, L, Drake, D, Ehresmann, B, Fedosov, F, Golovin, D, Hardgrove, C, Harshman, K, Hassler, DM, Kozyrev, AS, Kuzmin, R, Lisov, D, Malakhov, A, Milliken, R, Mischna, M, Mokrousov, M, Nikiforov, S, Sanin, AB, Starr, R, Varenikov, A, Vostrukhin, A & Zeitlin, C 2015, 'Water equivalent hydrogen estimates from the first 200 sols of Curiosity's traverse (Bradbury Landing to Yellowknife Bay): Results from the Dynamic Albedo of Neutrons (DAN) passive mode experiment', Icarus, vol. 262, pp. 102-123. https://doi.org/10.1016/j.icarus.2015.09.002
Tate, C. G. ; Moersch, J. ; Jun, I. ; Ming, D. W. ; Mitrofanov, I. ; Litvak, M. ; Behar, A. ; Boynton, W. V. ; Deflores, L. ; Drake, D. ; Ehresmann, B. ; Fedosov, F. ; Golovin, D. ; Hardgrove, Craig ; Harshman, K. ; Hassler, D. M. ; Kozyrev, A. S. ; Kuzmin, R. ; Lisov, D. ; Malakhov, A. ; Milliken, R. ; Mischna, M. ; Mokrousov, M. ; Nikiforov, S. ; Sanin, A. B. ; Starr, R. ; Varenikov, A. ; Vostrukhin, A. ; Zeitlin, C. / Water equivalent hydrogen estimates from the first 200 sols of Curiosity's traverse (Bradbury Landing to Yellowknife Bay) : Results from the Dynamic Albedo of Neutrons (DAN) passive mode experiment. In: Icarus. 2015 ; Vol. 262. pp. 102-123.
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abstract = "The Dynamic Albedo of Neutrons (DAN) experiment on the Mars Science Laboratory (MSL) rover Curiosity is designed to detect neutrons to determine hydrogen abundance within the subsurface of Mars (Mitrofanov, I.G. et al. [2012]. Space Sci. Rev. 170, 559-582. http://dx.doi.org/10.1007/s11214-012-9924-y; Litvak, M.L. et al. [2008]. Astrobiology 8, 605-613. http://dx.doi.org/10.1089/ast.2007.0157). While DAN has a pulsed neutron generator for active measurements, in passive mode it only measures the leakage spectrum of neutrons produced by the Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) and Galactic Cosmic Rays (GCR). DAN passive measurements provide better spatial coverage than the active measurements because they can be acquired while the rover is moving. Here we compare DAN passive-mode data to models of the instrument's response to compositional differences in a homogeneous regolith in order to estimate the water equivalent hydrogen (WEH) content along the first 200 sols of Curiosity's traverse in Gale Crater, Mars. WEH content is shown to vary greatly along the traverse. These estimates range from 0.5. ±. 0.1. wt.{\%} to 3.9. ±. 0.2. wt.{\%} for fixed locations (usually overnight stops) investigated by the rover and 0.6. ±. 0.2. wt.{\%} to 7.6. ±. 1.3. wt.{\%} for areas that the rover has traversed while continuously acquiring DAN passive data between fixed locations. Estimates of WEH abundances at fixed locations based on passive mode data are in broad agreement with those estimated at the same locations using active mode data. Localized (meter-scale) anomalies in estimated WEH values from traverse measurements have no particular surface expression observable in co-located images. However at a much larger scale, the hummocky plains and bedded fractured units are shown to be distinct compositional units based on the hydrogen content derived from DAN passive measurements. DAN passive WEH estimates are also shown to be consistent with geologic models inferred from other MSL instruments, which indicate that fluvial/lacustrine activity occurred at certain locations (e.g., Yellowknife Bay).",
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T1 - Water equivalent hydrogen estimates from the first 200 sols of Curiosity's traverse (Bradbury Landing to Yellowknife Bay)

T2 - Results from the Dynamic Albedo of Neutrons (DAN) passive mode experiment

AU - Tate, C. G.

AU - Moersch, J.

AU - Jun, I.

AU - Ming, D. W.

AU - Mitrofanov, I.

AU - Litvak, M.

AU - Behar, A.

AU - Boynton, W. V.

AU - Deflores, L.

AU - Drake, D.

AU - Ehresmann, B.

AU - Fedosov, F.

AU - Golovin, D.

AU - Hardgrove, Craig

AU - Harshman, K.

AU - Hassler, D. M.

AU - Kozyrev, A. S.

AU - Kuzmin, R.

AU - Lisov, D.

AU - Malakhov, A.

AU - Milliken, R.

AU - Mischna, M.

AU - Mokrousov, M.

AU - Nikiforov, S.

AU - Sanin, A. B.

AU - Starr, R.

AU - Varenikov, A.

AU - Vostrukhin, A.

AU - Zeitlin, C.

PY - 2015/12/1

Y1 - 2015/12/1

N2 - The Dynamic Albedo of Neutrons (DAN) experiment on the Mars Science Laboratory (MSL) rover Curiosity is designed to detect neutrons to determine hydrogen abundance within the subsurface of Mars (Mitrofanov, I.G. et al. [2012]. Space Sci. Rev. 170, 559-582. http://dx.doi.org/10.1007/s11214-012-9924-y; Litvak, M.L. et al. [2008]. Astrobiology 8, 605-613. http://dx.doi.org/10.1089/ast.2007.0157). While DAN has a pulsed neutron generator for active measurements, in passive mode it only measures the leakage spectrum of neutrons produced by the Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) and Galactic Cosmic Rays (GCR). DAN passive measurements provide better spatial coverage than the active measurements because they can be acquired while the rover is moving. Here we compare DAN passive-mode data to models of the instrument's response to compositional differences in a homogeneous regolith in order to estimate the water equivalent hydrogen (WEH) content along the first 200 sols of Curiosity's traverse in Gale Crater, Mars. WEH content is shown to vary greatly along the traverse. These estimates range from 0.5. ±. 0.1. wt.% to 3.9. ±. 0.2. wt.% for fixed locations (usually overnight stops) investigated by the rover and 0.6. ±. 0.2. wt.% to 7.6. ±. 1.3. wt.% for areas that the rover has traversed while continuously acquiring DAN passive data between fixed locations. Estimates of WEH abundances at fixed locations based on passive mode data are in broad agreement with those estimated at the same locations using active mode data. Localized (meter-scale) anomalies in estimated WEH values from traverse measurements have no particular surface expression observable in co-located images. However at a much larger scale, the hummocky plains and bedded fractured units are shown to be distinct compositional units based on the hydrogen content derived from DAN passive measurements. DAN passive WEH estimates are also shown to be consistent with geologic models inferred from other MSL instruments, which indicate that fluvial/lacustrine activity occurred at certain locations (e.g., Yellowknife Bay).

AB - The Dynamic Albedo of Neutrons (DAN) experiment on the Mars Science Laboratory (MSL) rover Curiosity is designed to detect neutrons to determine hydrogen abundance within the subsurface of Mars (Mitrofanov, I.G. et al. [2012]. Space Sci. Rev. 170, 559-582. http://dx.doi.org/10.1007/s11214-012-9924-y; Litvak, M.L. et al. [2008]. Astrobiology 8, 605-613. http://dx.doi.org/10.1089/ast.2007.0157). While DAN has a pulsed neutron generator for active measurements, in passive mode it only measures the leakage spectrum of neutrons produced by the Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) and Galactic Cosmic Rays (GCR). DAN passive measurements provide better spatial coverage than the active measurements because they can be acquired while the rover is moving. Here we compare DAN passive-mode data to models of the instrument's response to compositional differences in a homogeneous regolith in order to estimate the water equivalent hydrogen (WEH) content along the first 200 sols of Curiosity's traverse in Gale Crater, Mars. WEH content is shown to vary greatly along the traverse. These estimates range from 0.5. ±. 0.1. wt.% to 3.9. ±. 0.2. wt.% for fixed locations (usually overnight stops) investigated by the rover and 0.6. ±. 0.2. wt.% to 7.6. ±. 1.3. wt.% for areas that the rover has traversed while continuously acquiring DAN passive data between fixed locations. Estimates of WEH abundances at fixed locations based on passive mode data are in broad agreement with those estimated at the same locations using active mode data. Localized (meter-scale) anomalies in estimated WEH values from traverse measurements have no particular surface expression observable in co-located images. However at a much larger scale, the hummocky plains and bedded fractured units are shown to be distinct compositional units based on the hydrogen content derived from DAN passive measurements. DAN passive WEH estimates are also shown to be consistent with geologic models inferred from other MSL instruments, which indicate that fluvial/lacustrine activity occurred at certain locations (e.g., Yellowknife Bay).

KW - Cosmic rays

KW - Mars

KW - Mars, surface

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