MESSENGER's Science Team consists of experts
in all fields of planetary science, brought together by their
ability
to complete the science investigations conducted by MESSENGER. The team is divided into four disciplinary
groups: (1) Geochemistry, (2) Geology, (3) Geophysics, and (4)
Atmosphere and Magnetosphere, with each team member given responsibility for
implementation of a particular part of the mission's science plan.
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Mario H. Acuña
NASA Goddard Space Flight Center
An expert in planetary magnetic fields who was involved in many space missions, Mario Acuña contributed to the development of the Magnetometer
(MAG) and the analysis of MAG observations from MESSENGER's first two flybys of Mercury. The MESSENGER team was deeply saddened by Mario's death on 4 March 2009. His contributions to the mission continue.
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Brian J. Anderson
The Johns Hopkins University Applied Physics Laboratory
Brian Anderson specializes in the dynamics of space plasmas and planetary magnetic fields. He will provide scientific direction to the operation of the Magnetometer (MAG) instrument in orbit and lead aspects of the scientific analysis of its data to identify and quantify magnetospheric contributions to the observations and to recover the structure of Mercury's internal magnetic field. Member of the Atmosphere and Magnetosphere Group. |
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Daniel N. Baker
University of Colorado
Daniel Baker is an expert on the interactions among
planetary magnetic fields, atmospheres, and the solar wind.
He will lead the characterization of magnetospheric processes
using Magnetometer (MAG), Mercury Atmospheric and Surface Composition
Spectrometer (MASCS), and Energetic Particle and Plasma Spectrometer
(EPPS) data. Member of the Atmosphere and Magnetosphere Group. |
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Mehdi Benna
NASA Goddard Space Flight Center
Mehdi Benna specializes in plasma physics and planetary magnetosphere dynamics. He will develop models for Mercury’s magnetospheric structure and participate in the analysis of charged particle and magnetic field measurements from the Energetic Particle and Plasma Spectrometer (EPPS) and the Magnetometer (MAG). Member of the Atmosphere and Magnetosphere Group. Selected as a Participating Scientist in 2007. |
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David T. Blewett
The Johns Hopkins University Applied Physics Laboratory
David Blewett specializes in remote sensing and geological studies of the Moon and Mercury. He will use the detailed spectral information provided by the Mercury Atmospheric and Surface Composition Spectrometer (MASCS) to define spectral parameters that can be mapped using images collected by the Mercury Dual Imaging System (MDIS). Member of the Geochemistry and Geology Groups. Selected as a Participating Scientist in 2007. |
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William V. Boynton
University of Arizona
William Boynton's background spans many disciplines of planetary
science. He is a pioneer in compositional analysis from gamma-ray spectroscopy. He aided in the development
of the Gamma-Ray and Neutron Spectrometer (GRNS) and X-Ray
Spectrometer (XRS), and he will lead the analysis of geochemical remote sensing measurements. Member of the Geochemistry Group. |
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Nancy L. Chabot
The Johns Hopkins University Applied Physics Laboratory
Nancy Chabot is the Instrument Scientist for the Mercury Dual Imaging System (MDIS) and contributes to the development of the mission's imaging campaigns. She leads MDIS-based scientific investigations of Mercury's polar, radar-bright, ice-bearing craters. She is chair of the Geology Group. |
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Clark R. Chapman
Southwest Research Institute
Clark Chapman is an expert on impact cratering and has been
involved in studies of asteroids, Mercury, the Moon, and the
satellites
of Jupiter. He
will lead the analysis of Mercury's crater record and participate
in
the analysis of Mercury Dual Imaging System (MDIS) and Mercury
Atmospheric and Surface Composition Spectrometer (MASCS) spectral
observations.
Member of the Geology Group. |
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Andrew F. Cheng
The Johns Hopkins University Applied Physics Laboratory
Andrew Cheng studies planetary magnetospheres and how they interact
with surfaces and atmospheres. He will lead the analysis of
how Mercury's magnetosphere and surface interact, using Magnetometer
(MAG), Energetic Particle and Plasma Spectrometer (EPPS), and
Mercury Atmospheric and Surface Composition Spectrometer (MASCS)
data. Member of the Atmosphere and Magnetosphere Group. |
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Brett W. Denevi
The Johns Hopkins University Applied Physics Laboratory
Brett Denevi studies the geology and composition of the Moon, Mercury, and asteroids using multispectral imaging and spectroscopy. Along with analyzing Mercury's crustal evolution, she provides scientific direction to the operation of the Mercury Dual Imaging System (MDIS). She is deputy chair of the Geology Group. |
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Deborah L. Domingue
Planetary Science Institute
Deborah Domingue's area of expertise is in the study of planetary surfaces through remote sensing data. She will lead the analysis of Mercury's
photometric properties as a geological mapping tool and will participate in
the geological and geochemical interpretation of surface images and
spectrometry. Member of the Geology and Geochemistry Groups. |
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Larry G. Evans
Computer Sciences Corporation and NASA Goddard Space Flight Center
Larry Evans is an expert in gamma-ray and X-ray spectroscopy of planetary surfaces. He will utilize data returned by MESSENGER's Gamma-Ray and Neutron Spectrometer (GRNS) to infer the surface elemental composition of Mercury. He is the chair of the Geochemistry Group. Selected as a Participating Scientist in 2007. |
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William C. Feldman
Planetary Science Institute
William Feldman is one
of the world's leading experts in planetary neutron spectrometry.
A veteran of the Lunar Prospector, Mars Observer, and Mars
Odyssey missions, he provided the conceptual design for and
contributed to the calibration of the neutron spectrometer
sensor on the Gamma-Ray and Neutron Spectrometer (GRNS) instrument,
and he will lead the analysis of data from that sensor. Member
of the Geochemistry Group. |
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Robert W. Gaskell
Planetary Science Institute
Robert Gaskell is an expert in determining high-resolution shape and topography from stereo-photoclinometry data. He will use images acquired by the Mercury Dual Imaging System (MDIS) to derive information on the shape, topography, and internal structure of Mercury. Member of the Geology Group. Selected as a Participating Scientist in 2007. |
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Jeffrey J. Gillis-Davis
University of Hawaii
Jeffrey Gillis-Davis specializes in using remote sensing data to study the geological evolution of the terrestrial planets. On the MESSENGER team, he will investigate the origin of Mercury's intercrater and smooth plains deposits through an integration of MESSENGER data sets. Member of the Geology and Geophysics Groups. Selected as a Participating Scientist in 2007. |
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George Gloeckler
University of Michigan and University of Maryland
George Gloeckler is an expert in the solar wind and other space
plasmas, and he has been
involved in numerous space missions. He helped to develop the
Energetic Particle and Plasma Spectrometer (EPPS) and will
lead the analysis of its plasma measurements. Member of the Atmosphere
and Magnetosphere Group. |
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Robert E. Gold
The Johns Hopkins University Applied Physics Laboratory
Robert Gold is an expert in space plasmas. He
will participate in analysis of charged particle measurements
from the Energetic Particle and Plasma Spectrometer (EPPS). Member of the Atmosphere and Magnetosphere Group. |
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Steven A. Hauck, II
Case Western Reserve University
Steven Hauck's areas of expertise are planetary geophysics and tectonics. He will synthesize MESSENGER data sets to infer the internal structure and evolution of Mercury. Member of the Geophysics Group. Selected as a Participating Scientist in 2007. |
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James W. Head
III Brown University
James Head is an expert in planetary morphology, volcanism,
and tectonics with a long history in numerous planetary missions, beginning with Apollo. He will lead the
analysis of volcanic features and age relations among different
rock units. Member of the Geology Group. |
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Jörn Helbert
Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt
Jörn Helbert investigates planetary surfaces through infrared spectroscopy and thermal and physical modeling. Along with contributing to the study of Mercury's surface, he will work to develop cross-calibration strategies between MESSENGER and the Venus Express and BepiColombo missions of the European Space Agency. Member of the Geochemistry and Geology Groups. Selected as a Participating Scientist in 2007. |
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Kevin C. Hurley
University of California, Berkeley
Kevin Hurley's area of expertise is the field of cosmic gamma-ray bursts. On the MESSENGER team, he will fold observations from the Gamma-Ray and Neutron Spectrometer (GRNS) into an interplanetary network of cosmic gamma-ray burst detectors. Member of the Geochemistry Group. Selected as a Participating Scientist in 2007. |
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Catherine L. Johnson
University of British Columbia and Planetary Science Institute
Catherine Johnson is an expert in planetary magnetic and gravity fields. On the MESSENGER team, she will contribute to an understanding of Mercury's internal magnetic field. She is the deputy chair of the Geophysics Group. Selected as a Participating Scientist in 2007. |
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Rosemary M. Killen
NASA Goddard Space Flight Center
Rosemary Killen is an expert in the field of planetary atmospheres. She will integrate MESSENGER data to understand Mercury's exosphere, including its composition, variability, and interaction with the solar wind. Member of the Atmosphere and Magnetosphere Group. Selected as a Participating Scientist in 2007. |
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Stamatios M. Krimigis
The Johns Hopkins University Applied Physics Laboratory and
Academy of Athens
Stamatios Krimigis is an expert in solar, interplanetary, and magnetospheric
plasma physics and has been involved in numerous space missions.
He will lead the analysis of Energetic Particle and Plasma Spectrometer
(EPPS) data to characterize the interaction of Mercury's magnetosphere
with the solar wind. Member of the Atmosphere and Magnetosphere Group. |
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Haje Korth
The Johns Hopkins University Applied Physics Laboratory
Haje Korth specializes in the magnetic field and plasma environment of Mercury's magnetosphere resulting from the interaction of the magnetized planet with the solar wind. He is also the instrument scientist for the Magnetometer (MAG) and deputy chair of the Atmosphere and Magnetosphere Group. |
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David J. Lawrence
The Johns Hopkins University Applied Physics Laboratory
David Lawrence is an expert in gamma-ray and neutron spectroscopy and determining planetary compositions by remote sensing. Utilizing data from the Gamma-Ray and Neutron Spectrometer (GRNS), he will investigate Mercury's composition and geology. He is the deputy chair of the Geochemistry Group. Selected as a Participating Scientist in 2007. |
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Jean-Luc Margot
University of California, Los Angeles
Jean-Luc Margot is interested in the dynamics, geophysics, and geodesy of solid planets. He is an expert on high-precision measurements of planetary rotation. His investigation will combine MESSENGER data and ground-based radar data to characterize the interior of Mercury. Member of the Geophysics Group. Selected as a Participating Scientist in 2007. |
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William E. McClintock
University of Colorado
William McClintock is an expert in upper planetary atmospheres and specializes in their measurement using ultraviolet spectroscopy.
He led the development of the Mercury Atmospheric and Surface Composition Spectrometer (MASCS) and will lead the analysis of its measurements of atmospheric composition. Member of the Atmosphere and Magnetosphere Group and Geochemistry Group. |
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Timothy J. McCoy
Smithsonian Institution National Museum of Natural History
Tim McCoy is an expert in the study of meteorites, the mineralogy and chemistry of planetary materials, and X-ray and gamma-ray spectroscopy. As a member of the MESSENGER team, he will contribute to mapping and interpreting the mineralogy of Mercury's surface. Member of the Geochemistry Group. Selected as a Participating Scientist in 2007.
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Ralph L. McNutt Jr.
The Johns Hopkins University Applied Physics Laboratory
Ralph McNutt has been involved in a broad range of space physics research and is a pioneer in solar neutrino research. He will participate in the analysis of Mercury's surface composition using X-Ray Spectrometer (XRS) and Gamma-Ray and Neutron Spectrometer (GRNS) data. Member of the Atmosphere and Magnetosphere Group and Geochemistry Group. |
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Scott L. Murchie
The Johns Hopkins University Applied Physics Laboratory
Scott Murchie studies the surface composition of Mars, asteroids, and the Moon using imaging and spectroscopy. He led development of the Mercury Dual Imaging System (MDIS) and contributes to the mission imaging strategy, and he will participate in the analysis of MDIS and Mercury Atmospheric and Surface Composition Spectrometer (MASCS) spectral measurements of Mercury's surface. Member of the Geochemistry and Geology Groups. |
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Jürgen Oberst
Institute for Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt
Jürgen Oberst is an expert in planetary geodesy. He will contribute to the determination of topography from stereo imaging as well as to geodesy and cartography. Member of the Geology and Geophysics Groups. Selected as a Participating Scientist in 2007. |
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David A. Paige
University of California, Los Angeles
David Paige studies the polar regions of terrestrial planets. He will assist in MESSENGER's exploration of the polar regions of Mercury, particularly the identification of permanently shadowed areas that have the possibility for hosting water ice. Member of the Geochemistry, Geology, and Geophysics Groups. Selected as a Participating Scientist in 2007. |
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Stanton J. Peale
University of California, Santa Barbara
Stanton Peale is a leading expert on planetary dynamics. He developed the technique by which MESSENGER will measure the size and state of Mercury's core. He will lead the interpretation of Mercury Laser Altimeter (MLA) measurements of Mercury's rotation and libration. Member of the Geophysics Group. |
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Roger J. Phillips
Southwest Research Institute
Roger Phillips studies planetary tectonics and crustal structure
using geophysical techniques. He will lead the analysis of topography,
tectonics, and interior dynamics using Mercury Dual Imaging
System (MDIS), Mercury Laser Altimeter (MLA), and Radio Science (RS) data. He is the chair of the Geophysics Group. |
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Louise M. Prockter
The Johns Hopkins University Applied Physics Laboratory
Louise Prockter has an extensive background in planetary geology and geophysics. Along with providing scientific direction to the operation of the Mercury Dual Imaging System (MDIS), she will analyze MDIS images to gain insight into the geological evolution of Mercury, particularly the role of impact melting during the formation of large basins and the contribution of impact melts to smooth plains deposits. Member of the Geology Group. |
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Michael E. Purucker
Raytheon at Planetary Geodynamics Lab, NASA Goddard Space Flight Center
Michael Purucker is an expert in planetary magnetic fields. He will contribute to the co-estimation and interpretation of Mercury's internal and external magnetic fields. Member of the Atmosphere and Magnetosphere Group. Selected as a Participating Scientist in 2007. |
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Mark S. Robinson
Arizona State University
Mark Robinson is an expert in planetary surface morphology and specializes in image analysis and stereogrammetry. He will lead the development of global image products and the analysis of Mercury Dual Imaging System (MDIS) and Mercury Atmospheric and Surface Composition Spectrometer (MASCS) spectral measurements of the surface. Member of the Geochemistry and Geology Groups. |
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David Schriver
University of California, Los Angeles
David Schriver is a specialist in the simulation of space plasma physics phenomena. On the MESSENGER team, he will conduct global hybrid simulations of solar wind interaction with Mercury's magnetosphere. Member of the Atmosphere and Magnetosphere Group. Selected as a Participating Scientist in 2007. |
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James A. Slavin
University of Michigan
James Slavin is a leading expert on planetary magnetospheres and how they interact with atmospheres and the solar wind. He shared in the development of the Magnetometer (MAG) and will lead the analysis of the magnetospheric magnetic field measurements. He is a member of the Atmosphere and Magnetosphere Group. |
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Ann L. Sprague
University of Arizona
Ann Sprague is an expert in Mercury's exosphere and surface mineralogy. On the MESSENGER team, she will investigate the sources of elements measured in Mercury's exosphere and surface to probe the formation and evolution of the planet. Member of the Atmosphere and Magnetosphere Group and the Geochemistry Group. Selected as a Participating Scientist in 2007. |
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David E. Smith
Massachusetts Institute of Technology
David Smith studies the structure and dynamics of solar system objects
and specializes in techniques using gravity and laser ranging
measurements. He led the development of the Mercury Laser
Altimeter (MLA) and the Radio Science (RS) investigation, and he will lead the integration
of the two sets of measurements. Member of the Geophysics Group. |
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Richard D. Starr
The Catholic University of America
Richard Starr is an expert in X-ray and gamma-ray spectroscopy. He will contribute to the elemental analysis of Mercury’s surface with the MESSENGER geochemistry instrument suite. Member of the Geochemistry Group. Selected as a Participating Scientist in 2007. |
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Robert G. Strom
University of Arizona
Robert Strom is one of the founders of modern planetary geology and is an expert in surface morphology, particularly the effects of impact cratering. He has been studying Mercury since Mariner 10. He will lead the analysis of Mercury's geologic history and will participate in the analysis of Mercury Atmospheric and Surface Composition Spectrometer (MASCS) spectral measurements of the surface. Member of the Geology Group.
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Jacob I. Trombka
NASA Goddard Space Flight Center
Jacob Trombka is a leading expert on the study of planetary surface composition using X-rays and gamma-rays. He participated in the development of the X-Ray Spectrometer (XRS) and Gamma-Ray and Neutron Spectrometer (GRNS) and will share in the analysis of their measurements. Member of the Geochemistry Group. |
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Ronald J. Vervack, Jr.
The Johns Hopkins University Applied Physics Laboratory
Ron Vervack specializes in the study of planetary atmospheres using remote sensing data. He will participate in the planning and analysis of the observations of the exosphere as well as the modeling needed to understand Mercury's complex exospheric system. He is the chair of the Atmosphere and Magnetosphere Group. Selected as a Participating Scientist in 2007. |
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Faith Vilas
Planetary Science Institute
Faith Vilas is an expert in the study of the surface compositions of airless planetary bodies. She will lead the analysis of MESSENGER data to characterize space weathering on Mercury's surface. Member of the Geochemistry and Geology Groups. Selected as a Participating Scientist in 2007. |
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Thomas R. Watters
Smithsonian Institution National Air and Space Museum
Thomas Watters is an expert in the field of planetary tectonics and tectonic landforms. He will contribute to the analysis of Mercury's tectonic features using images obtained from the Mercury Dual Imaging System (MDIS) and topographic data obtained from the Mercury Laser Altimeter (MLA). Member of the Geology Group. Selected as a Participating Scientist in 2007. |
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Maria T. Zuber
Massachusetts Institute of Technology
Maria Zuber studies the structure and tectonics of solid solar system objects and specializes in using gravity and laser altimetry measurements to determine interior structure and evolution. She is leading the analysis of the Mercury Laser Altimeter (MLA) data. Member of the Geophysics Group. |
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Thomas H. Zurbuchen
University of Michigan
Thomas Zurbuchen is an expert in space plasmas and the space environment. He will provide scientific direction to the operation of the Fast Imaging Plasma Spectrometer (FIPS) and will lead aspects of the scientific analysis of FIPS data toward an understanding of Mercury's charged particle environment, particularly the distribution of plasma ions near Mercury and the implications for magnetosphere–solar wind interaction. Member of the Atmosphere and Magnetosphere Group. |