Maps of subsurface hydrogen from the High Energy Neutron Detector, Mars Odyssey

I. Mitrofanov; D. Anfimov; A. Kozyrev; M. Litvak; A. Sanin; V. Tret'yakov; A. Krylov; V. Shvetsov; W. Boynton; C. Shinohara; D. Hamara; R. S. Saunders

doi:10.1126/science.1073616

Maps of subsurface hydrogen from the High Energy Neutron Detector, Mars Odyssey

I. Mitrofanov
, D. Anfimov
, A. Kozyrev
, M. Litvak
, A. Sanin
, V. Tret'yakov
, A. Krylov
, V. Shvetsov
, W. Boynton
, C. Shinohara
, D. Hamara
, R. S. Saunders

Lunar and Planetary Lab

Research output: Contribution to journal › Article › peer-review

359 Scopus citations

Abstract

After 55 days of mapping by the High Energy Neutron Detector onboard Mars Odyssey, we found deficits of high-energy neutrons in the southern highlands and northern lowlands of Mars. These deficits indicate that hydrogen is concentrated in the subsurface. Modeling suggests that water ice-rich layers that are tens of centimeters in thickness provide one possible fit to the data.

Original language	English (US)
Pages (from-to)	78-81
Number of pages	4
Journal	Science
Volume	297
Issue number	5578
DOIs	https://doi.org/10.1126/science.1073616
State	Published - Jul 5 2002

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title = "Maps of subsurface hydrogen from the High Energy Neutron Detector, Mars Odyssey",

abstract = "After 55 days of mapping by the High Energy Neutron Detector onboard Mars Odyssey, we found deficits of high-energy neutrons in the southern highlands and northern lowlands of Mars. These deficits indicate that hydrogen is concentrated in the subsurface. Modeling suggests that water ice-rich layers that are tens of centimeters in thickness provide one possible fit to the data.",

author = "I. Mitrofanov and D. Anfimov and A. Kozyrev and M. Litvak and A. Sanin and V. Tret'yakov and A. Krylov and V. Shvetsov and W. Boynton and C. Shinohara and D. Hamara and Saunders, \{R. S.\}",

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language = "English (US)",

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TY - JOUR

T1 - Maps of subsurface hydrogen from the High Energy Neutron Detector, Mars Odyssey

AU - Mitrofanov, I.

AU - Anfimov, D.

AU - Kozyrev, A.

AU - Litvak, M.

AU - Sanin, A.

AU - Tret'yakov, V.

AU - Krylov, A.

AU - Shvetsov, V.

AU - Boynton, W.

AU - Shinohara, C.

AU - Hamara, D.

AU - Saunders, R. S.

PY - 2002/7/5

Y1 - 2002/7/5

N2 - After 55 days of mapping by the High Energy Neutron Detector onboard Mars Odyssey, we found deficits of high-energy neutrons in the southern highlands and northern lowlands of Mars. These deficits indicate that hydrogen is concentrated in the subsurface. Modeling suggests that water ice-rich layers that are tens of centimeters in thickness provide one possible fit to the data.

AB - After 55 days of mapping by the High Energy Neutron Detector onboard Mars Odyssey, we found deficits of high-energy neutrons in the southern highlands and northern lowlands of Mars. These deficits indicate that hydrogen is concentrated in the subsurface. Modeling suggests that water ice-rich layers that are tens of centimeters in thickness provide one possible fit to the data.

UR - https://www.scopus.com/pages/publications/18444418833

UR - https://www.scopus.com/pages/publications/18444418833#tab=citedBy

U2 - 10.1126/science.1073616

DO - 10.1126/science.1073616

M3 - Article

C2 - 12040089

AN - SCOPUS:18444418833

SN - 0036-8075

VL - 297

SP - 78

EP - 81

JO - Science

JF - Science

IS - 5578

ER -

Maps of subsurface hydrogen from the High Energy Neutron Detector, Mars Odyssey

Abstract

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