Complete Program
Tuesday Wednesday Poster Session Thursday Friday
Tuesday,
November 4, 2014
PLENARY SESSION I
9:30 a.m. / Building 34 -Conference
Room W150
9:30
a.m. Welcome
and Information
Brook Lakew, Associate Director
for Planning, Research and Development
Colleen
Hartman, Acting Director, Science and Exploration Directorate, NASA Goddard
Christopher
Scolese, Director, NASA Goddard Space Flight Center
Tuesday, November 4, 2014
REVIEWS OF INSTRUMENTS ON PAST MISSIONS
10:00 a.m. / Building 34 -Conference
Room W150
Chairs: S.
Feldman, (JPL)
B.
Lakew (GSFC)
10:00
a.m. Mather J. C. *
Planets, Asteroids, Comets,
Satellites, and KBO's: How You Can Use the JWST [#1015]
The James Webb Space Telescope (JWST) is planned for launch
in 2018. Its four instruments will provide cameras and spectrometers over the
full range from 0.6 to 28.5 µm, with coronagraphs and capabilities to observe
transiting exoplanets.
10:30
a.m. Zuber Maria T. Smith David E. *
Gravity Recovery and Interior
Laboratory: From Satellite-to-Satellite Ranging to High-Resolution Gravity of
the Moon [#1121]
The GRAIL Discovery mission provided a high accuracy, high
resolution gravity field of the Moon which is providing new insight into the
lunar crust and interior.
10:50
a.m. Yingst R. A. * Edgett K. S. Kennedy M. R. Minitti M. E. Ravine M. A.
Cameras on Landed Payload Robotic Arms
— MAHLI on Mars and Lessons Learned from One Mars Year
of Operations. [#1031]
The MSL MAHLI has proven to be robust, efficient in
operation, and flexible in the images and derivative products it yields. We
present an overview of the MAHLI investigation Primary Mission activities and
results, and key lessons learned thus far.
11:05
a.m. Yanamandra-Fisher P. A. *
Polarimetric Methods and Instrumentation for Solar
System Exploration [#1048]
Polarization is a complementary technique to imaging and spectrosocpy for remote sensing measurements of the solar
system and beyond. My talk will highlight inclusion of polarization as a
technique in future mission and ground-based instrumentation.
11:20
a.m. Fedorov A. * Barabash S. Lundin R.
Mars Express ion mass spectrometer for
Mars plasma environment. The lessons of the instrument design and
data analysis [#1146]
Looking forward to MAVEN data in the near future, we asking
ourselves what did we obtain and what did we miss with Mars Express plasma data
regarding the phenomenon of the martian
induced magnetosphere and the martian
ionosphere escape.
11:35
a.m. Nixon C. A. * Chan C. Y. Albright S. Gorius N. Brasunas J. et al.
The Cassini Composite Infrared
Spectrometer (CIRS): lessons learned in design and operations [#1144]
In this paper we discuss the various types of electrical
noises that arise in the Cassini CIRS instrument, as well as the prevention and
mitigation strategies that the team has developed to eliminate or minimize
the effects.
11:50
a.m. LUNCH BREAK
Tuesday, November 4, 2014
CONTRIBUTED TALKS ON EXITING AND
UPCOMING MISSIONS
1:00 p.m. / Building 34 -Conference
Room W150
Chairs: R.
Lorenz (APL)
C.
Milam (GSFC)
1:00
p.m. Bhardwaj A. *
Indian Mars Orbiter Mission [#1089]
The Mars Orbiter Mission (MOM) is the first interplanetary
mission of India launched by Indian Polar Satellite Launch Vehicle (PSLV-XL) on
5 November 2013. MOM will reach Mars on Sept. 24, 2014.
1:20
p.m. Senske D. * Prockter L. Pappalardo R. Paczkowski B. Vance S. et al.
Exploring Europa with the
Europa Clipper [#1019]
The Europa Clipper concept provides an efficient means to
explore Europa and investigate its habitability. The ability to evaluate sites for a
potential future lander would also be enabled by the Clipper.
1:40
p.m. Cable M. L. * Blaney D. L. Hibbitts C. A. Kim W. Murchie S. L. et al.
Retiring Risk with the Europa Short
Wavelength Infrared Spectrometer (ESWIRS) [#1044]
In preparation for an instrument proposal for the upcoming
Europa mission call, we have built and tested a Europa Short Wavelength
Infrared Spectrometer (ESWIRS) development model to retire risk in radiation
mitigation and planetary protection.
1:55
p.m. Thomas N. Spohn T. Lara L.-M. Christensen U. Seiferlin K. * et al.
The BepiColombo
Laser Altimeter [#1049]
The BepiColombo Laser Altimeter is
currently in flight model testing for launch in 2016. Novel aspects of the
instrument will be presented.
2:10
p.m. Yoshikawa M. * Kuninaka H. Inaba N. Tsuda Y. Hayabusa Project Team et al.
Hayabusa2, The New Challenge based on
the Lessons Learned of Hayabusa [#1050]
Hayabusa2, the follow-on mission of Hayabusa,
will be launched at the end of 2014. Hayabusa2 has been changed in many parts,
because we learned a lot from Hayabusa. In this
paper, Hayabusa2 mission is introduced in comparison with Hayabusa mission.
2:25
p.m. Jaumann R. * Bibring J. P. Glassmeier K. H. Grott M. Ho T. M. et al.
A Mobile Asteroide
Surface Scout (MASCOT for the Hayabusa 2 Mission [#1051]
MASCOT, will support JAXAÕs Hayabusa
2 mission to investigate the C-type asteroid 1999 JU3. Main objective is to
in-situ map the asteroidÕs geomorphology as well as the intimate structure,
texture, physical properties, and composition of the regolith.
2:40
p.m. COFFEE BREAK
3:10
p.m. Benna M. * Mahaffy P. R. Harpold D. King T.
Neutral and Ion Mass Spectrometers for
the Ladee and Maven Missions [#1056]
Two similar quadrupole mass
spectrometers, the Neutral Gas and Ion Mass Spectrometer (NGIMS) on MAVEN and
the Neutral Mass Spectrometer (NMS) on the LADEE Mission are described.
3:25
p.m. Ravine M. A. * Schaffner J. A. Caplinger M. A.
ECAM, a Modular Spaceflight Imaging
System—Case Studies [#1114]
MSSS has developed ECAM, a modular spaceflight imaging
system. There are current three
ECAM systems in development, including one which will fly on the OSIRIS-REx Mission.
3:40
p.m. Hurford T. A. * Mandell A. OPIS Team
Observatory for Planetary
Investigations from the Stratosphere (OPIS) [#1124]
The OPIS mission aims to demonstrate the usefulness of
balloon-borne observations for planetary science research.
4:00
p.m. Dickinson C. S. * Daly M. Barnouin O. Johnson C. Bierhaus B. et al.
THE OSIRIS-REx
LASER ALTIMETER (OLA) [#1142]
The OSIRIS-REx Laser Altimeter
(OLA) is a contribution of the Canadian Space Agency to the OSIRIS-REx Mission to return a sample from carbonaceous asteroid
(101955 Bennu. Operational scenarios and results of
EM testing will be presented.
Wednesday, November 5, 2014
PLENARY SESSION II
9:00 a.m. / Building 34 -Conference
Room W150
Chairs: M.
Grande (Aberystwyth U., UK)
C.
Nixon (GSFC)
9:00
a.m. Grotzinger J. P. * Science Team M. S. L.
Geologic, geochemical and mineralogic
framework for Aeolis Palus bedrock, and its relationship to Mt.
Sharp, Mars [#1135]
Curiosity's instruments have documented an impressive set of
sedimentary and igneous rock compositions, preserved as part of
fluvial-deltaic-lacustrine environment, indicating a habitable paleoenvironment
at Gale crater.
Wednesday,
November 5, 2014
INSTRUMENTATION FOR NEXT GENERATION
ORBITERS (I)
9:30 a.m. / Building 34 -Conference
Room W150
Chairs: M.
Grande (Aberystwyth U., UK)
C.
Nixon (GSFC)
9:30
a.m. Grasset O. * Altobelli N. Barabash S. Iess L. Jaumann R. et al.
The Jupiter Icy Moons Explorer
(JUICE): Complementarity Of The Payload In Addressing The Mission
Science Objectives. [#1141]
Invited Speaker.
9:50
a.m. Bergsrud C. M. * Straub J.
Using Space Solar Power Satellites to
Aid in Planetary Science Discovery and Exploration [#1000]
This paper presents an overview of the space solar power
satellite technology, and its
application to planetary science missions.
It details how it can drive lower costs and discusses prospective cost
savings in the context of two example missions.
10:05
a.m. Korth H. * Strohbehn K. Kitching J.
Miniature Absolute Scalar Magnetometer
Based on the Rubidium Isotope 87Rb [#1016]
Presented is a low-resource, miniaturized, absolute scalar
magnetometer based on the isotope 87Rb, which has a mass of <500 g and uses
0.5 W of power, while maintaining sensitivity comparable to present
state-of-the-art absolute magnetometers.
10:20
a.m. Mariani G. * Kenyon M.
Radiometric Mapping of Europa:
Challenges of Building a Radiation-Hardened, Uncooled, Far-Infrared
Thermal Imager [#1017]
Thermopile technology integrated with state-of-the-art
readout chips provides a far-infrared, uncooled, radiation-hardened, thermal
imaging solution to conduct accurate radiometric measurements of Europa.
10:35
a.m. Darrach M. * Farley K. Madzunkov S. Nikolic D. Niedholdt E. et al.
Mass Analyzer for Real-time
Investigation of Neutrals at Europa (MARINE) [#1018]
Presented herein is a summary of the Mass Analyzer for
Real-time Investigation of Neutrals at Europa (MARINE). MARINE new mass analyzer for analysis
the exospheres of planets, moons, and primitive bodies, such as found at Europa
or Enceladus.
10:50
a.m. COFFEE BREAK
11:10
a.m. Griggs C. E. * Paik H. J. Moody M. V. Han S. C. Rowlands D. D. et al.
Levitated Superconducting Gravity
Gradiometer for Planetary Missions [#1021]
We are developing an accurate tensor superconducting gravity
gradiometer for planetary missions. A new and innovative design gives a
sensitivity < 1 mE Hz^(–1/2) in the measurement band 1 mHz to 0.1 Hz
for a device with a baseline just over 10 cm.
11:25
a.m. Chattopadhyay G. * Reck T. J. Tang A. Jung-Kubiak C. Lee C. et al.
Silicon Micromachined High-Resolution
Terahertz Spectroscopic Instrument for Planetary Missions [#1022]
Using newly developed silicon micromachining technology we
are developing a low-mass and highly integrated state-of-the-art terahertz
radiometer/spectrometer instrument for planetary orbiter missions to Mars,
Venus, Titan, and the Galilean moons.
11:40
a.m. Sternovsky Z. * Gruen E. Horanyi M. Kempf S. Maute K. et al.
Hyperdust: Advanced instrument for the
in-situ detection and chemical analysis of cosmic dust particles [#1023]
The Hyperdust instrument is developed for future missions
for the composition and trajectory analysis of interstellar and interplanetary
particles, as well as surface composition analysis of airless
planetary objects.
11:55
a.m. Lingenauber K. * Hussmann H. Michaelis H. Oberst J. Kobayashi M. et al.
The Ganymede Laser Altimeter (GALA) on
ESA's JUICE mission: Overview of the Instrument Design. [#1029]
ESA's Jupiter Icy Moons Explorer (JUICE) will launch in 2022
and arrive at Jupiter in 2029. The Ganymede Laser Altimeter (GALA) will focus
on geodetic and geophysical investigations of the icy satellites Europa,
Callisto and Ganymede.
12:10
p.m. LUNCH BREAK
Wednesday, November 5, 2014
INSTRUMENTS ON FUTURE MARS LANDERS (I)
9:30 a.m. / Building 34- Conference
Room W120 A&B
Chairs: R.
Jaumann (DLR, Germany)
C.
Stahle (GSFC)
9:30
a.m. Mahaffy P. R. * Arevalo R. Brinckerhoff W. B. Caartwright J. A. Conrad P. G. et al.
AGES: A Noble Gas Mass Spectrometer
for Future in Situ Cosmic Radiation Exposure Age and K-Ar
Chronology Investigations [#1028]
The AGES mass spectrometer proposed for a future Mars, Lunar,
asteroid, or Phobos mission provides definitive in situ measurements of
cosmogenically and radiogenically produced noble gases to implement in situ
chronology investigations.
9:45
a.m. Sinclair J. A. * Wilson E. L. Irwin P. G. J. Calcutt S.
Detecting trace species in the Martian
atmosphere with a gas correlation filter radiometer [#1038]
We present the potential of a gas correlation radiometer in
detecting trace gases in the Martian atmosphere, such as methane and sulphur
dioxide. These species would serve
as tracers of geological, and perhaps biological activity on Mars.
10:00
a.m. Schmitz N. * Jaumann R. Coates A. J. Griffiths A. D. Leff C. E. et al.
PanCam on the ExoMars 2018 Rover: A
Stereo, Multispectral and High-Resolution Camera System to Investigate the
Surface of Mars [#1053]
The ExoMars rover will carry a Panoramic Camera System
("PanCam") being designed to obtain high-resolution colour and wide-angle
multi-spectral stereoscopic panoramic images from the rover mast.
10:15
a.m. Yu H. * Garnero E. Fouch M.
Molecular Electronic Transducers Based
Micro-Seismometers for Planetary Exploration [#1055]
A Molecular Electronic Transducers based micro seismometers
are under development, which are robust (orientation independent and high shock
tolerant) with low power, low mass, and relatively low cost and can be deployed
flexibly across a broad range.
10:30
a.m. Lorenz R. D. *
Micropower Instrumentation Needs for
an RHU-powered Mars Mini-Network Mission [#1062]
A network of affordable Mars landers ("MASER") able to
operate year-round is enabled by a radioisotope heater units (RHU) power system
(~200mWe) Continuous seismic
and wind measurements require new instrument designs able to operate
on ~50mW.
11:50
a.m. COFFEE BREAK
11:05
a.m. Rafkin S. C. R. * Banfield D. Nowicki K. Silver J. Dissly R.
An Instrument to Measure Turbulent
Fluxes in the Atmosphere of Mars and Other Planets [#1063]
A newly developed instrument capable of simultaneously
measuring turbulent fluxes in planetary atmospheres has been developed. The focus to date has been for Mars, but
can be adapted to other atmospheres such as Venus, Titan, and gas or
ice giants.
11:20
a.m. Arruego I. *
A Roadmap for the Development of
Miniature Instrumentation for Mars Exploration. [#1068]
We report on a 10-year initiative to set up a number of
resources for the development of miniature instruments for Planetary
Exploration. Thanks to it, we are involved in 2 Mars exploration missions: Mars
MetNet Lander and ExoMars 2016 EDM.
11:35
a.m. Olcott Marshall A. Marshall C. P. *
Challenges facing Raman spectroscopy
on Mars: Lessons from an Earth based analog [#1070]
Here we explore the best excitation wavelength ranging from
UV, Vis, and NIR for Raman analysis of samples from a Mars analog.
11:50
a.m. Apestigue V. * Jiménez J. J. Martsínez J. Álvarez F. J. Rivas J. et al.
DREAMS-SIS: A Miniature Instrument for
the Measurement of Atmospheric Optical Depth on ExoMars2016 EDM. [#1075]
The DREAMS-SIS sensor, a miniature photometer that will be
part of the DREAMS payload package on board ExoMars 2016 EDM, is presented. We
report on the design, development, calibration and qualification processes, as
well as present status.
12:05
p.m. LUNCH BREAK
Wednesday, November 5, 2014
INSTRUMENTATION FOR NEXT GENERATION
ORBITERS (II)
1:15 p.m. / Building 34 -Conference
Room W150
Chairs: C.
Webster (JPL)
S.
Milam (GSFC)
1:15
p.m. Dougherty M. K. * the J-MAG Team
J-MAG : The Magnetometer instrument
on JUICE [#1030]
The JUICE magnetometer instrument, J-MAG, will
be described.
1:35
p.m. André N. * Fedorov A. Paschalidis N. Sittler E. C. Jr. Cooper J. F.
PASTELS: an Innovative Rad-Hard,
Low-Mass Spectrometer for Electron and Negative Ion Characterization in
Planetary Environments(Europa, comets, Enceladus, Titan, ...) [#1032]
The Particle Analyzers for Suprathermal and Thermal
ELectronegative Species (PASTELS) consist of a compact, low mass, highly
capable sensor based on a design carefully optimized for the plasma and radiation
environment encountered around Europa.
1:50
p.m. Carter L. M. * Rincon R. F. Neish C. D.
SESAR: A Digital Beamforming
Polarimetric SAR for Near-Surface Imaging [#1033]
We discuss development of an advanced digital beamforming
radar instrument concept that can be used to image near-surface geology such as
potential ice layers and volcanic and sedimentary stratigraphy.
2:05
p.m. Lindeman M. A. * Kleinsasser A. W. Bumble B. Day P. K. Holmes W. A.
YBCO Kinetic Inductance Bolometers for
Hyperspectral Imaging of Cold Planetary Objects [#1042]
We are developing kinetic inductance bolometers to function
in hyperspectral imaging instruments for the characterization of the surfaces
of cold planetary bodies of the outer solar system in the mid to far
infrared bands.
2:20
p.m. Sittler E. C. Jr. * Cooper J. F. Paschalidis N. MacDonald E. A. Ali A. et al.
Advanced Ion Mass Spectrometer for
Giant Planet Ionospheres, Magnetospheres and Moons [#1043]
The Advanced Ion Mass Spectrometer is designed to measure
elemental, isotopic, and simple molecular composition abundances of 1 eV to 25
keV ions in the 1 – 60 amu mass range at mass resolution M/?M <= 60
within penetrating radiation environments.
2:35
p.m. Brageot E. C. * Drouin B. J. Kenyon M. E. Paige D. A. Johnson W. R.
Designing Visible Through FAR Infrared
Remote-Sending Instruments Based On A New Generation Of Thermopiles [#1126]
We present the capabilities of three different
multi-spectral visible to far-IR radiometers for Trojan Tour and Rendezvous,
Europa Clipper and Earth thermal climate sounding using the new generation of
uncooled thermopile arrays developed at JPL.
2:50
p.m. Goldsten J. O. * Maurer R. H. Mauk B. H.
ERM: An engineering radiation monitor
for high dose missions [#1105]
Missions to the moons of Jupiter must handle extreme
radiation environments. Given these can be very dynamic, mission planners,
spacecraft operators, and scientists can all benefit from a radiation monitor
that provides dose and charging rate data.
3:05
p.m. COFFEE BREAK
Wednesday, November 5, 2014
INSTRUMENTS ON FUTURE MARS LANDERS (II)
1:15 p.m. / Building 34 -Conference
Room W120 A&B
Chairs: P.
Beauchamp (JPL)
M.
Trainer (GSFC)
1:15
p.m. Vago J. L. * Witasse O. Rodionov D. ExoMars Team
Searching for Traces of Life with the
ExoMars Rover [#1132]
This presentation will concentrate on the ExoMars rover
mission (including science objectives, instrumen- tation, and upcoming
milestones), as well as briefly report on the progress achieved toward the
identifica- tion of suitable landing sites.
1:35
p.m. Steininger H. * Goesmann F. Raulin F. Brinckerhoff W. B. MOMA Team
Detecting Organics with the Mars
Organic Molecule Analyzer (MOMA) on the
2018 ExoMars Rover [#1098]
The Mars Organic Molecule Analyzer (MOMA) is a combined
pyrolysis gas chromatograph mass spectrometer (GC-MS) and laser desorption mass
spectrometer (LD-MS). It will be the key instrument of the ESA Roscosmos
ExoMars 2018 mission.
1:50
p.m. Elliott H. M. * Renno N. O. Preston R. A. Ruf C. S. Oudrhiri K. et al.
A Ground-Penetrating Radar and
Radiometer to Study the Shallow Subsurface of Mars and Other Solar
System Bodies [#1082]
An overview of the Mars Radar and Radiometry Sub-surface
Investigation (MARRSI), a novel type of sci-entific instrument that makes dual
use of the radio communication systems to studying the shallow subsurface of
planetary bodies.
2:05
p.m. Neumann G. A. * Garvin J. B. Blair J. B. Bufton J. L. Coyle D. B.
Lidar Imaging of Topography with
Millimeter Ranging Precision for Proximity Science and Operations from Rovers
or Spacecraft [#1076]
A new class of lidar sensor has been developed for measuring
local topography at millimeter vertical scales for 3-D assessment of context
geology and accurate navigation and positioning of surface assets for
sample acquisition.
2:20
p.m. Cho Y. * Kameda S. Miura Y. N. Miyamoto H. Sugita S.
An In-Situ K-Ar Isochron Dating System
for a Mars Rover Mission [#1157]
We propose an in-situ K-Ar isochron dating system for a
future Mars rover.
2:35
p.m. Lambert J. L. * Wang A. Cooper J. B.
Shifted-Excitation Raman Spectroscopic
Methodologies Developed for the Compact Integrated Raman
Spectrometer (CIRS) [#1136]
Experimental results demonstrating two methods of
fluorescence suppression are presented using fluorescent PAH's and minerals
samples. Both methods use a temperature-tuned green laser that is integrated
with the Compact Integrated Raman Spectrometer.
2:50
p.m. END OF SESSION
Wednesday, November 5, 2014
INSTRUMENTATION FOR NEXT GENERATION
ORBITERS (III)
1:15 p.m. / Building 34 -Conference
Room W150
Chairs: C.
Webster (JPL)
S.
Milam (GSFC)
3:35
p.m. Abshire J. B. * Smith M. D. Riris H. Sun X. Gentry B. M. et al.
MARLI: MARs LIdar for global climate
measurements from orbit [#1057]
We are developing a multifunctional atmospheric lidar
(MARLI) for Mars orbit. The lidar
approach is to simultaneously measure atmospheric backscatter and
depolarization profiles, wind profiles, and range from a near-polar
circular orbit.
3:50
p.m. Desai M. I. * Ogasawara K. Ebert R. W. Allegrini F. McComas D. J. et al.
Next Generation Plasma and Particle
Instrumentation for Planetary Missions [#1060]
This talk will focus on novel, miniaturized instrument
concepts for plasma and particle measurements on upcoming missions such as the
Europa Clipper, Enceladus Orbiter, Trojan Tour and Rendezvous, Uranus
Pathfinder etc.
4:05
p.m. Barabash S. * Brandt P. C. Wurz P. Team PEP.
Particle Environment Package (PEP) for
the ESA JUICE Mission [#1065]
PEP is a suite of six sensors that together provide
comprehensive in-situ and remote measurements of particle and plasma
environments of the Jovian system and its moons over nine decades of energy
from <0.001 eV to >1 MeV.
4:20
p.m. Kraft R. P. * Kenter A. T. Murray S. S. Martindale A. Pearson J. et al.
A High Speed, Radiation Hard X-ray
Imaging Spectrometer for Planetary Investigations [#1084]
We present a concept for a X-ray imaging spectrometer using
CMOS sensors and a microchannel plate optics. It could determine the composition of
the surface of the Galilean moons and airless rocky bodies, and the properties
of magnetospheric plasmas.
4:35
p.m. Miller T. C. * Kleinfelder S. Barwick S. Besson D. Connolly A. et al.
PRIDE – Passive Radio Ice Depth
Experiment - An Instrument to Measure Outer Planet Lunar Ice Depths from Orbit
using Neutrinos. [#1088]
We describe a low mass, low power passive instrument to
measure the thickness of the ice shell on ice moons, by making use of RF
signals from high energy neutrinos.
This update includes results from the first quarter of a 2014 NIAC Phase
1 grant.
4:50
p.m. Quilligan G. * Aslam S. Lakew B. DuMonthier J. Katz R. et al.
A 0.18µM CMOS Thermopile Readout ASIC
Immune to 50 Mrad (Si) Total Ionizing Dose and Single Event Latchup to
174 MeV-cm2/mg. [#1096]
A 180nm CMOS multi-channel digitizer (MCD) ASIC for a
thermopile readout was tested for radiation hardness. The chip was found to be immune to
single event latchup (SEL) and total ionizing dose (TID) at 174 MeV-cm2/mg and
50 Mrad (Si) respectively.
5:05
p.m. Wrbanek J. D. * Wrbanek S. Y. Fralick G. C. Clark P. E. McNeil R. R.
Compact Full-Field Ion Detector System
for SmallSats beyond LEO [#1103]
Under development by NASA GRC, the Compact Full-field Ion
Detector System is designed to be capable of being flown on a wide variety of
deep space platforms to provide multi-directional, comprehensive measurements
of ions in space environments.
5:20
p.m. END OF ORAL SESSION
Wednesday, November 5, 2014
POSTER SESSION
5:30 p.m. / Building 34 Gallery I
Contributed posters on existing and upcoming missions
(MESSENGER,
OSIRIS-Rex, Rosetta, Hayabusa 2, Mangalyaan/Indian
Mars Orbiter mission, JUICE, Europa Clipper, ExoMars,
MAVEN, LADEE, ...)
Schmidt W. Laitinen T. J較vinen R. Polkko J. Harri A.-M.
Low Power Solutions for Rosetta Instruments: Finnish
Contributions to an Exciting Project [#1037]
The
Finnish Meteorological Institute (FMI) provided hardware or software for five
different instruments and for one system device onboard Rosetta satellite and
for an instrument and a system device onboard the Philae lander.
Mottola S. Michaelis H. Bresch W. Jaumann R. Arnold G. et al.
ROLIS, A Close-up Look at the Surface of 67P. [#1058]
ROLIS
is the descent/close-up imager onboard Philae, the Rosetta lander. The
experiment objectives and the instrument capabilities are described.
Caplinger M. A. Ravine M. A. Hansen C. J.
Junocam: the challenges of adding an imaging
system to the Juno Mission [#1073]
Junocam was added to the
Juno Mission during Phase A. To
limit cost, a camera design from MSL was adapted to the Juno requirements. There were numerous challenges in doing
so, all of which were successfully surmounted.
Fletcher Z. J. McMichael R. Cheng A. F. Hibbitts C. A.
BOPPS
Infrared Camera. [#1123]
The
abstract describes a balloon-borne planetary imager which
will fly one month before the workshop to observe the comet Siding Spring along
with the Mars spacecraft MRO and MAVEN and the Curiosity rover.
Instrumentation for in-situ analysis missions
(Venus
in-situ Explorer, Titan Lake Lander, ...)
Palomba E. Longobardo A. Dirri F. Zampetti E. Biondi D. et al.
VISTA: A Micro-Ther,mogravimeter
to Measure Water and Organics Content in Planetary Environment [#1052]
The
presentation focuses on the VISTA instrument (developed by a consortium of
Italian institues), its large field of planetary
applications, its technical characteristics and the functional and performance
tests performed.
Li X. Getty S. A. Grubisic A. Brinckerhoff W. B. Cornish T. et al.
New Developments in Reversible-Polarity Laser
Time-of-Flight Mass Spectrometry for Future In Situ Planetary Missions [#1067]
A
reversible polarity laser desorption/ionization time-of-flight mass
spectrometer incorporating curved field reflectron,
and pulsed pin ion gate has been developed.Data
from this analyzer is shown to have advanced analytical capabilities.
Trainer M. G. Mahaffy P. R. Brinckerhoff W. B. Johnson N. M. Glaze L. S.
Investigating the Origin and Evolution of Venus with In
Situ Mass Spectrometry [#1083]
Measurement of noble gas abundances on
Venus remain
a high priority for planetary science. This can be accomplished as part of an
atmospheric investigation using flight-proven technology and demonstrated
enrichment techniques.
Yingst R. A. Ravine M. A. Bartley J. K. Cohen B. A. Edgett K. S.
et
al.
Hawkeye:
Deciphering Lithologic Clues Remotely and
Rapidly from Stationary and Mobile Platforms. [#1094]
Hawkeye,
a mast-mounted, 2-megapixel RGB color camera with a focusable macro lens, is a
simple, heritage-rich investigation that provides hand lens scale lithology
from actionable distances, maximizing the efficiency of landed or
roving vehicles.
Szopa C. Buch A. Coll P. Cabane M. Coscia D. et al.
Gas chromatography to characterize the molecular
composition of extraterrestrial environments [#1110]
We
present results obtained these two last decades with GCMS instrumentation,
using compact GC systems. Are also presented recent developments on
miniaturized GC components to be used in the future in science payloads with
limited ressources.
Uckert K. Chanover N. J. Getty S. Grubisic A. Li X. et al.
Using IR Spectroscopy To Optimize Organic Detection With
A Two-Step Laser Desorption/Ionization Time-of-Flight Mass Spectrometer [#1113]
We
explore the dependence of the IR desorption laser wavelength of a two step
laser desorption/ionization time-of-flight mass spectrometer on the strength of
IR absorption features of organically doped sulfates to optimize the detection
of organic species.
Chanover N. J. Uckert K. Voelz D. G. Boston P. J.
The Development and Field Testing of the Portable
Acousto-optic Tunable Filter Spectrometer for Astrobiology [#1139]
We
present the first field observations of cave environments using a portable
reflectance spectrometer sensitive between 1.6-3.6 ?m. We will present a suite of PASA spectra
in order to demonstrate its efficacy as a tool for biomarker detection.
Sultana M. Adkins-Reick R. Stern J. C.
Graphene
Chemical Sensor Array for in situ Chemical Analysis [#1156]
We
are developing highly sensitive, selective and low resource graphene
chemical sensor arrays for in situ detection of trace gases and volatile
organics. The versatile nature makes these sensors suitable for both orbiters
and landed missions.
POSTER SESSION
5:30 p.m. / Building 34 Gallery II
Instrumentation for next generation orbiters
(Io,
Mars 2020, TGO/ExoMars, ESA/JUICE, Europa Clipper
mission, Enceladus, Trojan Tour and Rendezvous, ...)
Schmitz N. Palumbo P. Jaumann R. Della Corte V. Zusi M. et al.
JANUS on JUICE: A Camera to Investigate Ganymede,
Europa, Callisto and the Jovian System. [#1054]
ESA's
JUICE mission will carry the camera system JANUS, an optical camera to study
global, regional and local morphology and processes on the Jovian moons, and to
perform mapping of the Moon's surfaces and the clouds on Jupiter.
Cadu A. Devoto P. Louarn P. Sauvaud J. A.
Grazing Incidence Time-of-Flight Mass Spectrometer:
Prototype Results and Possible Improvements [#1064]
We
designed a complete time-of-flight mass spectrometer prototype for space plasma
instrumentation, using grazing incidence MCP to replace usual carbon foil for
electron emission. We present the first results and possibilities
of improvements.
Westlake J. H. Kasper J. C. Rymer A. M. Case A. W. Stevens M. L. et al.
The Influence of Magnetospheric
Plasma on Magnetic Sounding of Europaユs Interior Oceans: Plasma Instrumentation
for the Europa Clipper Mission. [#1081]
We
present instrumentation designed for operation on the Europa Clipper
spacecraft, consisting of Faraday cup sensors, that can
pro-vide the high quality plasma measurements that are crucial to the success
of a Europa magnetic sounding experiment.
Brown A. -D. Aslam S. Barrentine E. M. Mikula V. Schmidt A. et al.
Micromachined
Thermopile Arrays with Novel Thermoelectric Materials [#1091]
We
have fabricated and characterized novel thermopile detectors, which use micromachined 2 micron-thick Si legs to thermally isolate
the hot and cold thermocouple regions.
Hibbitts C. A. Boldt J. D. Liang S. X. Edens W. K. Kelly M. A. et al.
Uncooled Thermal Infrared Camera Development
at JHU-APL [#1107]
We
will present our development effort for a ~ megapixel uncooled TIR camera and
some results from an aircraft test flight.
Parsons A. M. Boynton W. V. Evans L. G. Hamara D. Harshman K. et al.
Orbital High Purity Germanium (HPGe)
Composition Measurements of Carbonaceous Asteroids [#1111]
HPGe gamma ray
spectrometers have very successfully mapped the subsurface bulk elemental
compositions of Mars and Mercury.
This powerful technique can also be applied to determine the subsurface
bulk elemental compositions of carbonaceous asteroids.
Bloser P. F. Schwadron N. Bancroft C. Legere J. Ryan J. et al.
Dose Spectra from Energetic Particles and
Neutrons (DoSEN) [#1115]
DoSEN combines two
advanced complementary radiation detection concepts with fundamental advantages
over traditional dosimetry. DoSEN
measures energy and charge distribution of energetic particles in a way not
possible with current dosimeters.
MacDonald E. A. Funsten H. O. Larsen B. A. Reeves G. D. Skoug R. M. et al.
A High TRL Low Resource "2 in 1" Concept for Magnetospheric Plasma Mass Spectrometry for High Radiation
Planetary Environments [#1128]
A High TRL Low Resource "2 in
1" Concept for Magnetospheric Plasma Mass
Spectrometry for High Radiation Planetary Environments, based on the HOPE
instrument flown on the Van Allen Probes.
Glenn J.
High-J CO as a Probe of Warm Molecular Gas in
Galaxies: Herschel Evidence for
Feedback and the Need for Future Far-Infrared Spectroscopy [#1002]
High-J
CO observations of LIRGs revealed a warm component of molecular gas that
carries ~90% of the CO luminosity. High resolution FIR
observations will be required to characterize ISM feedback and understand
consequences for galaxy evolution.
MacEwen H. A.
In-space Infrastructures: Synergisms Among Disciplines
in Astrophysics [#1004]
Addresses
in-space infrastructures to assist in the assembly and servicing of large space
telescopes in general, and is intended to enhance interactions among the FAR-IR
community, and the space community at large (e.g., human exploration).
Sorensen P. H. Davis B. J. Kline-Schoder R. J. Morrison R. L.
An Ultra-Compact, High-Accuracy Star Tracker [#1013]
Creare's Ultra Compact Star
Tracker is estimated to have mass less than 650 g, volume less than 400 cm3,
and consume less than 0.5 W of power, while providing estimated attitude
accuracy of 1 arc second in pitch and yaw and 10 arc seconds in roll.
Technology for in-situ analysis and sample return
(Lunar,
Mars, Comet surface (i.e. ROsetta), NEOs (i.e.
OSIRIS-Rex), ...)
John K. K. Abell P. A. Graham L. D.
Surface Investigations of Asteroids: Science
Justification and the Need for Instrument Development [#1118]
There
is very limited knowledge about the surface of asteroids. There is a lack of scientific data on
the properties of regolith and a lack of instrumentation to characterize the
surface. Surface interaction is key
in order to obtain ground truth.
Clark P. E. Farrand W. Scheld D. Martin J. Dreyer C.
MIA: Miniature In-Situ Analyzer for Mars, the Moon
or Asteroids [#1026]
We
are developing MIA, a next-generation in-situ geochemical, mineralogical, and petrological analysis tool requiring no sample preparation,
combining XRF and XRD instruments with a compact X-ray source, and dual
CCD detectors.
Segal N. R. E. Osinski G. R. Dietrich P. Tornabene L. L. Coulter A. B. et al.
Demonstrating TEMMI: A Three-Dimensional Exploration
Multispectral Microscopic Imager on Geologic Materials. [#1095]
Demonstration
of the capabilities of the Three-Dimensional Exploration Multispectral
Microscopic Imager (TEMMI)on geologically relevant
materials. TEMMI has three different operating modes: 2D colour,
3D and Ultraviolet (UV), including multispectral.
Lim L. F. Getty S. A. Kotecki C. A. Southard A. E. Gaskin J.
A Miniature Electron Probe for In Situ
Elemental Microanalysis [#1106]
The
Mini-EPMA is an adaptation of the standard laboratory technique of electron
probe microanalysis (EPMA) to a flight instrument suitable for a lander or
rover mission.
Wei J. Wang A. Goetz W. Cornor K.
Quantification of Fluorescence Emission from
Extraterrestrial Materials [#1112]
Quantification
of fluorescence emissions from Martian meteorites, carbonaceous condrites and terrestrial samples were obtained from a
fluorescence microscope.
Wei J. Wang A. Lu Y. Connor K. Bradley A.
Detection Limits of Biomarkers by Micro-Beam 532 nm
Laser Raman Spectrometry (LRS) [#1117]
We
present detection limits of biosmarkers by micro-beam
532 nm laser Raman spectrometry.
Beaty D. W. Liu Y.
Planning for the Earth-Based Instruments and Associated
Sample Preparation Procedures Needed to Achieve the Scientific Objectives
of MSR. [#1122]
Now
that NASA has selected the instruments for the M-2020 sample-collecting rover,
the attention of the instrument-planning/building community needs to shift in
part to the instruments needed to evaluate the samples if they are returned
to Earth.
POSTER
SESSION
5:30
p.m. / Building 34 Gallery III
Instruments on future Mars landers
(ExoMars, Mars 2020 & beyond, ...)
Polkko J. Kahanpää H. Harri A-M. Genzer M. Nikkanen T. et al.
Atmospheric Pressure & Humidity Instrument
Technologies for Planetary Landers [#1035]
Finnish
Meteorological Institute has provided meteorological pressure & humidity
instruments for several planetary landing missions. Flown instruments on
successful missions are presented as well as those under development for coming
Mars missions.
Southard A. E. Adachi T. Brown G. Gonnsen Z. Johnson C. et al.
High speed and accurate pressure measurement with a mems pressure gauge from 100 to 0.1 mtorr
in support of MOMA-MS [#1059]
We
demonstrate an approach to improve response time of a transistor can sized,
300-600 microWatt pirani
pressure gauge and demonstrate its readiness for use in the MOMA ion trap
mass spectrometer.
Blake D. F. Sarrazin P. Bristow T.
Mapping alpha-particle X-ray Fluorescence
Spectrometer (Map-X) [#1080]
Map-X
is an arm-based imaging XRF spectrometer.
It utilizes a radioisotope fluorescent source, an X-ray オ-pore Optic
(MPO) and an X-ray sensitive CCD to record postage stamp - sized element maps
and XRF spectra of ground-selected ROI.
Fries M. Bhartia R. Beegle L. Burton A. Ross A. et al.
The Calibration Target for the Mars 2020 SHERLOC
Instrument: Multiple Science Roles for Future Manned and Unmanned
Mars Exploration [#1093]
The
SHERLOC instrument is a deep-UV Raman/fluorescence instrument selected for the
Mars 2020 rover instrument suite. SHERLOCユs calibration target includes space
suit materials and meteorite samples to serve multiple SMD and HEOMD
science roles.
Brinckerhoff W. Danell R.
van Amerom F.
Pinnick V. Li X. et al.
Development of a Linear Ion Trap Mass Spectrometer
(LITMS) Investigation for Future Planetary Surface Missions [#1109]
We
present an overview of the LITMS investigation under development with support
of the Maturation of Instruments for Solar System Exploration (MatISSE) program.
Pinnick V. T. Buch A. Grand N. Humeau O. van Amerom F. H. W. et al.
Mars Organic Molecule Analyzer: Performance of the Gas
Chromatography-Mass Spectrometry Mode of Operation. [#1119]
The
Mars Organic Molecule Analyzer, a key analytical tool aboard the 2018 ExoMars Rover, is a combined pyrolysis gas chromatography
and laser desorption mass spectrometer.
This report focuses on the current performance of the
GC-MS interface.
Grubisic A. van Amerom F. H. W. Danell R. M. Pinnick V. T. Arevalo R. D. et al.
Mars Organic Molecule Analyzer: Performance of Laser
Desorption Ionization Linear Ion Trap Mass Spectrometer [#1120]
Performance
characteristics of the laser desorption ionization mode of the Engineering Test
Unit of Mars Organic Molecule Analyzer Linear Ion Trap Mass Spectrometer
is demonstrated.
Rodriguez-Manfredi J. A. de la Torre M. Bridges N. T. Conrad P. G. Ferri F. et al.
MEDA, An Environmental And Meteorological Package For
The MARS 2020 Mission. [#1125]
This
abstract describes MEDA, the environmental instrument recently selected as part
of the Mars2020's scientific payload, its goals and concept.
Blagojevic B. Trainer M. G. Pavlov A. A. Prasad C. R.
Bio-Indicator Lidar Instrument
for NASA Planetary Missions [#1140]
We
propose a novel planetary Astrobiology instrument based on a real-time
technique of remote detection and discrimination of any bio-signatures
dispersed in the ground-level planetary atmosphere.
CubeSats concepts for planetary missions
Clark P. E. Dichmann D. Folta D. Lo M. Staehle R. et al.
MOLO: MiniMoon Orbiting
Lagrange Observatory [#1025]
The
MiniMoon Orbiting Lagrange Observatory (MOLO) is an
operationally complex, multi-platform Cubesat concept
involving 'targets-of-opportunity' encounters with incoming minimoons
via Lagrange Points.
Sittler E. C. Jr. Paschalidis N. Cooper J. F. Zesta E. Ali A. et al.
Development of Ion and Neutral Mass Spectrometers (INMS)
for Heliophysics and Planetary Missions [#1041]
High
Precision Electric Gate (HPEG) that can provide precision electric gate ~ 1 ns
time resolution, and also acts as a velocity filter. It can provide miniature
and lower power ion neutral mass spectrometers for CubeSat applications.
Leiter R. Himwich Z. Natarajan A. Rosenthall J.
SPACE for Cubesats: Small
Payloads and Advanced Concepts for Exploration Early Mission Design Tool [#1027]
The
SPACE tool separates the design process of a CubeSat
mission into selection of an instrument or payload and selection of
various subsystems.
Kobayashi M. Ishimaru R.
Dust Monitoring Instrument on CubeSat
for Small Body Mission [#1071]
we describe a concept idea of dust
monitoring by CubeSat probe dispatched from the main
spacecraft in small body mission.
Collier M. R. Sibeck D. G. Porter F. S.
Soft X-ray Instrumentation for Planetary Exploration:
Current Status and Future Potential [#1079]
Solar
wind charge exchange (SWCX) operates at all solar system objects with
atmospheres/exospheres. SWCX generates X-rays that can be used to image
characteristic density structures, so spacecraft can map out the boundaries
surrounding these bodies.
Thursday, November 6, 2014
PLENARY SESSION III
9:00 a.m. / Building 34 -Conference
Room W150
Chairs: P.
Mahaffy (GSFC)
X.
Sun (GSFC)
9:00 a.m. Elphic R. C. * Hine B. P. Delory G. T. Noble S. Colaprete A. et al.
Lunar Science On
A ShoeString: The Adventures of LADEE [1164]
NASA's Lunar Atmosphere and Dust
Environment Explorer (LADEE) arrived at the Moon on Oct 6, 2013. It
demonstrated many firsts: deep-space demonstration of high-speed laser
communications; acquisition of all necessary science data in 100 days etc.
Thursday, November 6, 2014
INSTRUMENTATION FOR IN-SITU ANALYSIS
MISSIONS
9:30 a.m. / Building 34 -Conference
Room W150
Chairs: P.
Mahaffy (GSFC)
L.
Carter (GSFC)
9:30
a.m. Nagihara S. * Zacny K. Hedlund M. Taylor P. T.
Compact, Modular Heat Flow Probe for
the Lunar Geophysical Network Mission [#1011]
We report our progress in designing and testing prototypes
of a low-mass, low-power heat flow probe for possible use in the Lunar
Geophysical Network and other missions to the Moon.
9:45
a.m. Cohen B. A. * Devismes D. Miller J. S. Swindle T. D.
The Potassium-Argon Laser Experiment
(KArLE): In Situ Geochronology for Planetary Robotic Missions [#1040]
We are developing an in situ geochronology capability using
flight-heritage components. KArLE results show that for planetary samples older
than 2 Ga, precision will be ア100 Ma, sufficient to address a wide range of
high-priority science.
10:00
a.m. Stockton A. M. * Kim J. Willis P. A. Lillis R. Amundson R. et al.
The Mars Organic Analyzer:
Instrumentation and Methods for Detecting Trace Organic Molecules on Mars and
Elsewhere in our Solar System [#1045]
Mars Organic Analyzer was designed to give the Mars 2020
Mission capability to look for organic molecules, including amines, aldehydes,
ketones, organic acids, thiols and polycyclic aromatic hydrocarbons, in martian
samples with sub-ppb sensitivity.
10:15
a.m. Ehlmann B. L. * Mouroulis P. Van Gorp B. Blaney D. Rodriguez J. et al.
Microimaging VSWIR Spectroscopy
Instruments for Planetary Exploration: Measuring In-Situ Mineralogy, Ices,
Organics, and Linking to Remote Observation [#1046]
In situ microimaging VSWIR spectroscopy to assess mineralogy
and texture simultaneously with no surface prep, rapid measurement (<10min
scan for 140,000 discrete measurements), and high sensitivity to minerals has
been demonstrated with a prototype.
10:30
a.m. Willis P. A. * Mora M. F. Cable M. L. Stockton A. M. Williford K. H. et al.
Microfluidic Life Analyzer (MILA) [#1047]
MILA is a newly initiated planetary instrument development
effort funded under the NASA-PICASSO Program aimed at the analysis of organic
acids. Key measurement capabilities include amino acid chirality and carboxylic
acid chain length up to 30 atoms.
10:45
a.m. Peplowski P. N. * Goldsten J. O. Lawrence D. J.
COUGRS: A Low-Resouce Gamma-Ray
Spectrometer for Surface Science Investigations into Planetary Origins
and Evolution [#1061]
We present a new, lightweight, low-resource gamma-ray
spectrometer capable of making high-quality geochemical measurements on future
planetary landers.
11:00
a.m. COFFEE BREAK
11:20
a.m. Wang Alian. * Jolliff B. L. Lambert J. L. Menzies R. Hutchinson I. et al.
A Compact Integrated Raman
Spectrometer, CIRS, for Fine-Scale Mineralogy and Bio-Signature Detection in
Planetary Surface Explorations of Our Solar System. [#1090]
CIRS is a non-optical-fiber version of MMRS, with augmented
science capabilities. It combines a high-quality laser Raman spectrometer
(CIRS-LRS) with a Context Imager (CIRS-CI). CIRS development enables broad
applications for future missions.
11:35
a.m. Beauchamp P. M. * Hörst S. M. Yelle R. V. Cable M. L. Neidholdt E. L. et al.
Planetary Organics Detector (POD): A
High Resolution Mass Spectrometer System To Determine Composition
And Structure [#1129]
POD has high resolution tandem mass spectrometers and a cryogenic
sample handling system for analyzing gas, liquid, and solid samples to
distinguish between structural isomers and isobars, molecular formulas and ions
that have the same nominal mass.
11:50
a.m. Blaney D. L. * Murchie S. L. Green R. O. Mustard J. Ehlman B. et al.
Ultra Compact Imanging Spectrometer
(UCIS): Technology Maturaion and Applications for Mars, the Moon, and
Small bodies. [#1148]
The Ultra Compact Imaging Spectrometer (UCIS) is the first
imaging spectrometer compatible with being put on the mast of a lander or rover
that has been built using flight-proven components and can collect data on the
Moon, asteroids, or Mars.
12:05
p.m. Southard A. E. * Ferrance J. Elsila J. E. Espiritu A. M. Kotecki C. et al.
Liquid Chromatography-Mass
Spectrometry Interface for detection of extraterrestrial organics [#1155]
The OASIS (Organics Analyzer for Sampling Icy surfaces) is
being developed to do in situ detection of the organic content of icy bodies in
the solar system using liquid chromatography-mass spectrometry.
12:20
p.m. LUNCH BREAK
Thursday, November 6, 2014
INSTRUMENTATION FOR NEXT GENERATION
ORBITERS (IV)
9:30 a.m. / Building 34- Conference
Room W120 A&B
Chairs: M.
Grande (Aberystwyth U., UK)
X.
Sun (GSFC)
9:30
a.m. Tamppari L. K. * Spiers G.
A Doppler Wind LIDAR for Mars [#1127]
The winds on Mars are almost completely unknown, yet are
critical for understanding fundamental processes on Mars, and ensuring safe
landing of robotic and human spacecraft.
We are developing a Doppler LIDAR for Mars to be flown from orbit.
9:45
a.m. Asmar S. W. * Iess L. Folkner W. M. Simone L. Bolton S. J.
Advanced Radio Science Instrumentation
for the Juno, BepiColombo, and JUICE Missions [#1130]
Planetary interior structures are constrained via
gravitational field recovery. Radio Science techniques have utilized Doppler
tracking. Beyond X-band links, we have introduced Ka-band radios and improved
data quality by an order of magnitude.
10:00
a.m. James D. * Kemph S. Passe H. Sternovsky Z. Young J. et al.
Development and Characterization of a
New Dynode Multiplier for Missions to Harsh Radiation Environments [#1138]
An electron multiplier and its housing are being developed
for the SUrface Dust Analyzer instrument proposed on NASA's planned Europa
mission. This talk presents the
results of design, modeling, and testing in preparation for the
harsh environment.
10:15
a.m. Jones S. M. * Anderson M. S. Davies A. G. Kirby J. P.
Aerogel Dust Capture for In-Situ Mass
Spectrometry Analysis [#1143]
To demonstrate that aerogel dust capture can be used to
complement current methods of sample collection for in-situ mass spectrometry
(MS), impact tests and analyses with MS were conducted. PAHs were identified
from the dust captured in aerogel.
10:30
a.m. Kempf S. * Altobelli N. Brios C. Grün E. Hand K. et al.
SUDA: A Dust Mass Spectrometer for
Compositional Surface Mapping for a Mission to Europa [#1152]
SUDA is an impact mass spectrometer, which measures the
composition of ballistic dust particles from Europa's surface. The unique
compositional data enables SUDA to define and constrain the geological
activities on and below the moons' surface.
10:45
a.m. Sandor-Leahy S. * Miller H. Logan J. Flannery M. Folkman M.
Compact Thermal Imaging Spectrometer
for Planetary Science Applications [#1159]
NGAS has developed a novel, compact, low weight and power,
hyperspectral imaging spectrometer , which has key
features that make it particularly suitable for planetary science and uses a
compact optical design resulting in a single compact instrument package.
11:00
a.m. COFFEE BREAK
11:20
a.m. Gautam N.
Sherwin M. S. * Kawamura J. Karasik B. Focardi P. et al.
A Heterodyne Detector for Terahertz
Spectroscopy of Planets and Comets. [#1160]
Between 1 and 5 THz, molecular lines in cometary and
planetary atmospheres are dense and strong. We discuss the development of a
frequency-agile, nearly quantum-limited, heterodyne receiver for 1-5 THZ that
can be passively cooled.
Thursday, November 6, 2014
INTERPLANETARY LASER RANGING AND
COMMUNICATIONS
11:35 a.m. / Building 34- Conference
Room W120 A&B
Chairs: M.
Grande (Aberystwyth U., UK)
X.
Sun (GSFC)
11:35
a.m. Cornwell D. M. *
NASA's Optical Communications Program
for Future Planetary and Near-Earth Missions [#1010]
An overview of NASA's vibrant and wide-ranging optical
communications program to support future planetary and near-Earth missions will
be provided, based on the success of the laser communications demonstration
from the Moon on LADEE in 2013.
11:55
a.m. Dell'Angnello S. *
NASA-SSERVI and INFN Partnership
"SPRINGLETS":Solar system Payloads of laser
Retroreflectors of INfn for General reLativity,Exploration and planeTary Science [#1163]
A research partnership between INFN and NASA-SSERVI, the
NASA Solar System Exploration and Research Virtual Institute, to provide new
generation laser retroreflectors for precise positioning of the Moon, Mars and
the icy/rocky moons of Jupiter and Saturn.
12:10
p.m. END OF SESSION
LUNCH
BREAK
Thursday, November 6, 2014
MARS 2020 MISSION AND INSTRUMENTS
1:20 p.m. / Building 34 -Conference
Room W150
Chairs: A.
Bhardwaj (VSSC, India)
T.
Stubbs (GSFC)
1:20
p.m. Farley K. A. * Schulte M. D. Williford K. H.
Overview of the Mars 2020 Mission and
its Investigation Payload [#1133]
An overview of the investigations selected for the Mars 2020
rover mission.
1:40
p.m. Allwood A. C. * Clark B. Elam W. T. Flannery D. T. Grotzinger J. et al.
PIXL: Planetary Instrument for X-ray
Lithochemistry on Mars 2020 [#1104]
PIXL is a microfocus XRF instrument on the robotic arm of
the Mars 2020 rover. PIXL will be used to investigate abundances and
submillimeter-scale distribution of chemical elements in rocks and soils.
2:00
p.m. Hamran S.-E. *
Amundsen H. E. F. Carter L. Ghent R. Kohler J. et al.
The Ground Penetrating Radar RIMFAX on
the Mars 2020 Mission. [#1034]
The Radar Imager for Mars' sub-surFAce eXperiment (RIMFAX)
ground penetrating radar experiment for the Mars 2020 Rover will add a new
dimension to the rover's toolset by providing the capability to image the
shallow subsurface beneath the rover.
2:20
p.m. Wiens R. C. * Maurice S. Johnson J. R. Clegg S. M. Sharma S. K. et al.
The SuperCam Remote Sensing Suite for
Mars 2020: Co-Aligned LIBS, Raman, and Near-IR Spectroscopies, and
Color Micro-Imaging [#1086]
SuperCam/Mars2020 is a suite of 4 instruments: Laser Induced
Breakdown Spectroscopy (LIBS), Raman spectros-copy, visible and near-infrared
spectroscopy (VISIR), and high resolution color imaging, all co-aligned and at
micro-radian angular resolution.
2:40
p.m. Bell J. F. III * Maki J. N. Mehall G. L. Ravine M. A. Caplinger M. A.
Mastcam-Z: A Geologic, Stereoscopic,
and Multispectral Investigation on the NASA Mars-2020 Rover [#1151]
Here we describe the mast-mounted Mastcam-Z imaging system
on the Mars-2020 rover. We describe our geologic, atmospheric, and operational
science goals, as well as the basic functionality and predicted performance of
the cameras.
3:00
p.m. Beegle L. W. * Bhartia R. DeFlores L. White M. Asher S. et al.
SHERLOC: Scanning Habitable
Environments with Raman & Luminescence for Organics & Chemicals, an
Investigation for 2020 [#1078]
The SHERLOC investigation was recently selected for the Mars
2020 integrated payload. SHERLOC enables non-contact, spatially resolved, and
highly sensitivity detection and characterization of organics and minerals
on Mars.
3:20
p.m. Hecht M. H. * Rapp D. R. Hoffman J. A. The MOXIE TEAM
The Mars Oxygen ISRU
Experiment (MOXIE) [#1134]
Recently selected to fly on NASAユs Mars 2020 mission, MOXIE
is a 1% scale model of an oxygen processing plant that might support a human
expedition sometime in the 2030s. MOXIE will produce 22g/hr of O2 on Mars with
>99.6% purity during 50 sols.
3:40
p.m. END OF ORAL SESSION
GSFC
TOURS
Thursday, November 6, 2014
GSFC Tours
3:55 p.m.
3:55 p.m. |
Group A: Bus departs from Building 34 for Visitor Center, then returns to
Building 34 for Group B |
4:00 p.m. |
Group A:The Astrobiology Walk at the
Visitor Center Garden, Visitor Center Group B: Bus departs from Building 34 for Building 29, then returns to Visitor
Center for Group A |
4:10 p.m. |
Group B: James Webb Space Telescope Space Systems Development and Integration
Facility Clean Room and Building 29 |
4:30 p.m. |
Group A: Bus returns to Visitor Center for Group A, takes VIPs to Building 29 and
picks up Group B to take to Visitor Center |
4:40 p.m. |
Group A: James Webb Space Telescope Space Systems Development and Integration
Facility Clean Room and Building 29 Group B: Bus departs
from Building 29, for the Visitor Center |
4:50 p.m. |
Group B: The Astrobiology Walk at the Visitor Center, Garden, and Visitor Center |
5:15 p.m. |
Group A: bus picks up VIPs from Building 29, takes to Visitor Center Group B: already at Visitor Center |
5:20 p.m. |
Group A & B await hotel shuttles at Visitor Center, then depart center |
Friday, November 7, 2014
PLENARY SESSION IV
9:00 a.m. / Building 34 -Conference
Room W150
Chairs: C.
Webster (JPL)
C.
Nixon (GSFC)
9:00
a.m. C. J.
Alexander *
Humanity's First Attempt to Land on A
Comet, November 2014
Friday, November 7, 2014
TECHNOLOGY FOR IN-SITU ANALYSIS AND
SAMPLE RETURN (I)
9:30 a.m. / Building 34 -Conference
Room W150
Chairs: C.
Webster (JPL)
C.
Nixon (GSFC)
9:30
a.m. Zagarola M. V. * Hill R. W. Gagne J. R.
Ultra Low Power Cryo-Refrigerator
for Space [#1085]
Creare is currently working to develop an innovative type of cryocooler, an ultra-low power cryocooler
that utilizes a cryogenic heat sink.
We recently completed the demonstration of a technology demonstration
unit, which is the subject of this presentation.
9:45
a.m. Glavin D. P. * Tsou P. Anbar A. D. Baross J. Beegle L. W. et al.
Plume Collection Strategies for Future
Icy Body Sample Return Missions [#1012]
Sample return of plume materials from Enceladus will be
critical to the search for evidence of life on this potentially habitable
moon. Here we focus on sample
collector and containment technology development and testing needed for
future missions.
10:00
a.m. Webster C. R. * Christensen L. E. Flesch G. J. Forouhar S. Briggs R. et al.
Tunable Laser Spectrometers for
Space Science [#1066]
Tunable laser spectrometers have enjoyed a huge growth in
capability for space science: for planetary missions, the International Space
Station (ISS) cabin monitoring, and for In Situ Resource Utilization (ISRU) on
the Mars 2020 mission.
10:15
a.m. Izenberg N. R. *
FirefOx - An Oxygen Fugacity Sensor
for Venus [#1074]
FirefOx is a ceramic oxygen sensor designed for deep atmosphere,
near surface determination of the oxygen fugacity of Venus, and constraint of
stable surface mineralogy and gas chemistry.
10:30
a.m. Durga Prasad K. * Maniteja V. Murty S. V. S.
A Novel Approach for Precise
Temperature Measurement by Planetary Thermal Probes [#1014]
We have developed and tested a novel signal
conditioning scheme for precise RTD based temperature measurement by
Planetary thermal probes. This scheme would help in designing an optimised electronics for in situ planetary heat
flow measurements.
10:45
a.m. Gerasimov M. V. *
Gas-Analytic Package of the Russian
メLunar-Resourceモ mission [#1036]
Gas-analytic package of the Lunar-Resource mission is aimed
on comprehensive investigation of the inventory of volatiles in the polar regions regolith. It uses
pyrolysis-gas-chromatography-mass-spectrometry method and consists of
three instruments.
11:00
a.m. Hill S. W. * Hohlfeld E. M. Adams E. A. Liang S. X. Sharma A. et al.
In-Situ Small Body Surface
Characterization Enabled by the Planetary Object Geophysical
Observer (POGO) [#1039]
The Planetary Object Geophysical Observer (POGO) is a self-contained,
fully autonomous ride along payload that is able to provide in-situ elemental
and compositional information of many different locations on a small
body surface.
11:15
a.m. COFFEE BREAK
11:35
a.m. Arevalo R. Jr. * Brinckerhoff W. B. Mahaffy P. R. van Amerom F. H. W. Danell R. M. et al.
It's a Trap! A review of MOMA and
other ion traps in space or under development [#1102]
Ion trap instruments have found a niche in planetary
missions that require small, versatile mass analyzers. Here, a review is
provided on the current state of ion trap technologies in flight and/or
under development.
11:55
a.m. Thangavelautham J. * Robinson M. Taits A. McKinney T. Amidan S. et al.
Flying, Hopping Pit-bots for Cave and
Lava Tube Exploration on the Moon and Mars [#1087]
In this paper we introduce a network of 3 kg, 0.30 m
diameter ball robots that can fly, hop and roll using an on board miniature
propulsion system in extreme environments such as caves and lava tubes on the
Moon and Mars.
12:10
p.m. Lawrence D. J. * Burks M. T. Goldsten J. O. Peplowski P. N. Beck A. W.
GeMini Plus: A Low Resource, High Precision
Gamma-Ray Spectrometer for Planetary Composition Measurements [#1092]
We discuss a new instrument called GeMini
Plus that can accomplish laboratory quality, high-precision gamma-ray
measurements with the type of low-resources needed for landed platforms as well
as resource-constrained orbital missions.
12:25
p.m. Harvey T. J. Hur-Diaz S. *
Asteroid Capture with a Structured
Netted Asteroid Retrieval Envelope (SNARE) [#1097]
We describe an innovative asteroid capture system concept
using CubeSats called the Structured Netted Asteroid
Retrieval Envelope (SNARE) as a viable and compelling solution to capturing a
small asteroid.
12:40
p.m. LUNCH BREAK
Friday, November 7, 2014
CUBESATS CONCEPTS FOR PLANETARY
MISSIONS
9:30 a.m. / Building 34 -Conference
Room W120 A&B
Chairs: S.
Feldman (JPL)
S.
Stahle (GSFC)
9:30
a.m. Baker J. D. *
Expanding Science and Innovation with CubeSat Instruments [#1150]
Imagine flying through the plumes above Europa and being
able to identify the composition of the ejecta
without risking your primary spacecraft. Today the first low cost deep space CubeSats, called INSPIRE have been developed and more are
on the way.
9:50
a.m. Farrell W. M. * MacDowall R. J. Folta D. Bradley D. Collier M. R. et al.
Terminator Double Layer Explorer (TerDLE): A Plasma Lunarcube Concept [#1072]
TerDLE will study the plasma expansion process at low altitudes
along the flank of the lunar plasma wake.
10:05
a.m. Castillo-Rogez J. C. Blacksberg J.
Feldman S. M. * Kahn C. L. Shapiro-Scharlotta A. A.
Small Instruments for Nano-Spacecraft
Applications - A Review [#1158]
This paper provides a review of the current state of the art
in small instruments that may be applicable to future missions involving
independent or deployable platforms in the 1-10 kg range.
10:20
a.m. Paine C. G. * Hayne P. O. Cohen B. A.
Lunar Flashlight: A 6U CubeSat Using Solar Sail Propulsion to Orbit the Moon and
Illuminate Permanently-Shadowed Regions in a Search for Water [#1131]
We describe a mission concept for a solar-sail—powered
CubeSat to orbit the moon, illuminate permanently shadowed
polar regions with sunlight reflected from the sail,
and quantify the presence of cold-trapped water ice using the
reflected spectrum.
10:35
a.m. Esper J. E. *
Cubesat Application for Planetary Entry
(CAPE) Missions: Micro-Reentry Capsule (MIRCA) [#1147]
The CAPE concept describes a high-performing Cubesat system which includes a propulsion module and
miniaturized technologies capable of surviving atmospheric entry heating. MIRCA
is CAPEユs first planetary entry probe flight prototype.
10:50 a.m. Cooper J. F. * Sturner S. J. Sittler E. C. Paschalidis N. Wesenberg R. P. et al.
Natural
Environmental Shielding Impacts on Electronics and Sensor Shielding Design for
Missions to Extreme Radiation Environments of the Europa and Ganymede [#1149]
Natural environmental
shielding impacts of Galilean moon bodies, surface topography, and magnetic
fields on spacecraft and sensor electronics are considered for orbiter, flyby,
and lander missions to extreme radiation environments of these moons.
11:05
a.m. END OF SESSION
Friday, November 7, 2014
TECHNOLOGY FOR IN-SITU ANALYSIS AND
SAMPLE RETURN (II)
1:40 p.m. / Building 34 -Conference
Room W150
Chairs: M.
Trainer (GSFC)
L.Carter (GSFC)
1:40
p.m. Noell A. C. * Lee M. C. Takano N. Elleman D. Hasenoehrl J. et al.
Astrobionibbler: Microfluidic Subcritical Water
Extraction of Organics from Planetary Samples [#1100]
Astrobionibbler is a microfluidic instrument meant for sample extraction
and concentration of organic molecules from solid powder samples. By
miniaturizing the extraction and concentration process it will enable a wide
range of wet chemical analysis.
1:55
p.m. Getty S. A. * Li X. Cornish T. Grubisic A. Uckert K. et al.
A Two-step Tandem Laser Time-of-Flight
Mass Spectrometer for the In Situ Study of the Surfaces of Primitive and Icy
Solar System Bodies [#1101]
Laser desorption/ionization time-of-flight mass spectrometry
offers compositional analysis of solid samples using an instrument that can be
made compact, low power, and lightweight for future in situ misions
to primitive bodies and icy moons.
2:10
p.m. Alerstam E. * Blacksberg J. Maruyama Y. Cochrane C. Rossman G. R.
A miniature time-resolved Raman
spectrometer for in situ planetary surface exploration [#1077]
We present a time-resolved Raman spectrometer (TRRS) for
planetary science as a means for identification and mapping of minerals even in
the presence of high background fluorescence.
2:25
p.m. Parsons A. M. * Evans L. G. Karunatillake S. McClanahan T. P. Moersch J. E. et al.
High Sensitivity Subsurface Elemental
Composition Measurements with PING [#1108]
The Probing In situ with Neutrons and Gamma rays (PING)
instrument will measure the bulk elemental composition of the subsurface of any
solid solar system body and is a versatile, effective tool for a host of in
situ scientific investigations.
2:40
p.m. Tulej M. * Riedo A. Neuland M. Wurz P.
LMS Instrument: Present State and
Perspectives for Element and Isotope Analysis of Planetary Materials [#1137]
The performance figures of a miniature laser abaltion/ionisation instrument
(LMS) are presented and its coupling with a miniature microscope-camera (CAMAM
suite) for additional complementary characterisation
of the planetary materials.
2:55
p.m. Rymer A. M. * Westlake J. H. Smith H. T. Strohbehn K. Bowen K.
ANIONS: Atmospheric Negative
ION Sensor. [#1099]
The importance and measurement of planetary atmospheric
negative ion chemistry.
3:10
p.m. Núñez J. I. * Adams E. Y. Koerner L. J. Murchie S. L.
Impact of Geometry on Element
Abundances from X-ray Fluorescence in Vacuum: Considerations for APXS
Measurements on Small Airless Bodies [#1145]
We present test results of a prototype APXS instrument under
vacuum to assess the impact of position geometry on element abundance
measurements using x-ray spectroscopy. Results have implications for in-situ
APXS measurements on asteroids or comets.
3:25
p.m. Roman M. J. * Malin M. C. Ravine M. A. Robinson M. S.
Strategies for unmanned lunar rovers:
Integration of teleoperation and autonomy based on
field testing [#1153]
We have carried out a series of rover field tests,
demonstrating multiple km of range with human-in-the-loop operation (with
lunar-appropriate latency) and (in separate tests) with
autonomous operation.
3:40
p.m. Anderson F. S. * Whitaker T. J. Levine J. L.
The Case For In-situ Dating with
Geologic Context for the Moon and Mars using the Chemistry, Organics, And
Dating EXperiment (codex) [#1161]
The Chemistry, Organics, and Dating Experiment can identify
evidence of non-terrestrial organics, and understand the history and duration
of events in the solar system, placing them both in context.
3:55
p.m. END OF ORAL SESSION