Thermal, Thermophysical, and Compositional Properties of the Moon Revealed by the Diviner Lunar Radiometer
|
|
- Delphia Summers
- 5 years ago
- Views:
Transcription
1 Thermal, Thermophysical, and Compositional Properties of the Moon Revealed by the Diviner Lunar Radiometer Benjamin T. Greenhagen Jet Propulsion Laboratory David A. Paige and the Diviner Science Team LEAG /23/12 Greenbelt, MD
2 The Moon is a model of airless solar system bodies but don t forget the infrared!
3 LRO Diviner Overview Observation Strategy Detectors Fields of view Primarily nadir pushbroom mapping Nine 21-element linear arrays of uncooled thermopile detectors Detector Geometric IFOV: 6.7 mrad in-track 3.4 mrad cross track 320 m on ground in track for 50 km altitude 160 m on ground cross track for 50 km altitude Swath Width (Center to center of extreme pixels): 67 mrad; 3.4 km on ground for 50 km altitude Normalized Response Wavenumber (cm-1) Wavelength (microns) Science Goals 1. Characterize the Moon s surface thermal environments: Daytime Nighttime Polar 2. Map properties of the lunar surface: Bulk thermal properties Rock abundance Composition 3. Characterize polar cold traps: Map cold trap locations and temperatures Assess potential lunar volatile resources Determine thermophysical properties
4 Examples of Diviner South Pole Coverage /27 9/20 11/13 1/7 2/28 Des. EQX Lon EQX Time-of-Day :00 Ascending EQX 18:00 12:00 6:00 Descending EQX 0:00 Enhancing diurnal and seasonal coverage is a prime goal of the LRO extended science mission
5 South Pole Temperature Summary Maps Maximum Temperature Average Temperature Minimum Temperature Diviner has observed the lunar poles with a wide range of local times Diviner Polar Resource Products: Which volatiles could be present Where to look for surface and near surface deposits after Paige et al., 2010; Science Paige et al., 2012
6 South Pole Temperature Depth to 1 mm water Summary ice Maps sublimation per BY Maximum Temperature Average Temperature Minimum Temperature Diviner has observed the lunar poles with a wide range of local times Diviner Polar Resource Products: Which volatiles could be present Where to look for surface and near surface deposits after Paige et al., 2010; Science Paige et al., 2012
7 Equatorial Daytime Coverage Ch 7 Brightness Temperature (K) Green Crater 133 E / 3.5 N
8 Equatorial Nighttime Coverage Ch 7 Brightness Temperature (K) Green Crater 133 E / 3.5 N
9 Diviner-revised Thermal Models Highlands: rougher, more scatter Maria: smoother, but with warm rocks Remarkably similar on average Diviner diurnal temperature data reveal effects of thermophysical properties, roughness, and rocks Data are consistent with a near-surface regolith in which density and temp-variable conductivity gradually increase in the upper ~20 cm (Vasavada et al., 2012; JGR-Planets) Leveraged eclipse observations to understand upper ~2 cm (Hayne et al., 2012)
10 Diviner Global Rock Abundance 0 Tycho (~100 Ma) Aristarchus (~170 Ma) Rock Concentration (0-0.05) 0 50 km Copernicus (~800 Ma) Bullialdus (>1100 Ma) Rock Concentration Rock abundance and regolith temperature map level 3 products available at the PDS Methodology and initial science results published at JGR-Planets (Bandfield et al., 2011) Regolith Temperature (Normalized for Local Time) Regolith Temperature (Normalized for Local Time and Latitude)
11 Tsiolkovskiy Crater Diviner Rocks over WAC Mosaic / DEM after Greenhagen et al., 2012; EPSC
12 LROC WAC Equatorial Cold Spots Nighttime Soil Temperature Colder than average nighttime temperatures associated with small, fresh craters No associated albedo or spectral signature Modeling indicates thicker than average highly insulating layer Deposits were likely emplaced via combination of granular and fluidized flow Mechanism is currently uncertain but could include mobilization of volatiles after Bandfield et al., 2012
13 Surface and Buried Rock Populations Surface Rock Fraction Buried Rock Depth 5% 10 cm Model Rock Abundance 2.5% Model Rock Depth 5 cm 0% 0 cm Copernicus Crater Diviner surface rock abundances match LROC NAC images of surface rocks but Mini-RF shows extended regions of blocky materials Radar observed blocky materials must be buried Diviner rock abundance and nighttime soil temperatures with thermal models are used to estimate the burial depth of extended blocky regions potential to constrain lunar burial / regolith formation rate after Ghent et al., 2012
14 Lunar Swirls 50 km Diviner CF Map of Reiner Gamma Feature Off-swirl CF Swirl CF Δ CF Reiner Gamma Airy Ingenii Marginis km CF Shift consistent with solar wind stand-off inhibiting space weathering. CF position not consistent with pure feldspar composition Night-time data reveal weak thermal anomaly thermal modeling is under way. after Glotch et al., 2012
15 Groundtruthing Diviner Data Measured Diviner CF values for each Apollo Site Strong Correlation between Diviner measured CF and some geochemical species (esp. Al 2 O and FeO) Illustrates sensitivity to plagioclase-mafic ratio; complementary to NIR datasets Apollo 15 2 km Al 2 O 3 wt% Apollo 11 Apollo 12 Apollo 14 Apollo 15 Apollo 16 Apollo 17 Apollo 17 2 km CF Position (μm) after Greenhagen et al., 2012; LPSC
16 Diviner observations of crater central peaks (after Song et al., 2012, JGR-Planets) Copernicus Crater. Colorized CF over WAC basemap Copernicus crater (above), E 9.6 N. Central peak CF value of 8.14µm. Northern wall feature CF value is 8.41µm. Eratosthenes crater (right), 348 E 13.5 N. Central peak CF value of 8.48µm, making it the most mafic composition sampled in the central peak survey. 6/135 craters with central peak composition more mafic than typical mare basalt. None that appear to be mantlesourced. Eratosthenes Crater. Colorized CF over WAC basemap
17 Some Additional Ongoing Investigations Constraining lunar heat flow by analyzing data for coldest permanently shadowed craters Investigating Diviner-constrained lunar permafrost locations with neutron data Investigating warmer, off-pole shadowed regions where ice pumping to subsurface may be enhanced Photometric and thermophysical studies using targeted emission phase function observations Understanding the effects of space weathering on Diviner data Compositional studies of a wide range of targets High silica, plagioclase, olivine, pyroclastics, etc. Studying the Earth as an exoplanet using Diviner Earth scans Laboratory experiments to aid the interpretation of Diviner data Incorporating other lunar datasets to enhance Diviner data analyses LOLA, LROC, Mini-RF, M3, Kaguya, Clementine, LP Producing enhanced maps and data products for PDS
18 Conclusions Diviner data are being used to understand in detail the lunar thermal environment and thermophysical and compositional properties The Diviner dataset will be important for future lunar landing site selections Thermal state Global diurnal and seasonal temperatures Polar Resources Potential volatile cold traps and species Thermophysical Properties Rock abundance and nighttime soil temperature Insulating layer thickness Constraints on buried rocks Composition Mineralogical diversity Plagioclase abundances and mixing
SWIRLS. Spectral and Thermophysical Properties of Lunar Swirls from the Diviner Lunar Radiometer Tim Glotch, Stony Brook University
SWIRLS Spectral and Thermophysical Properties of Lunar Swirls from the Diviner Lunar Radiometer Tim Glotch, Stony Brook University 1. Space Weathering FORMATION MECHANISMS Some swirls associated with strong
More informationLunar surface rock abundance and regolith fines temperatures derived from LRO Diviner Radiometer data
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116,, doi:10.1029/2011je003866, 2011 Lunar surface rock abundance and regolith fines temperatures derived from LRO Diviner Radiometer data Joshua L. Bandfield, 1 Rebecca
More informationOH/H 2 0 Enhancements associated with Some Silicic Volcanism as detected by M 3
OH/H 2 0 Enhancements associated with Some Silicic Volcanism as detected by M 3 Noah Petro LEAG Annual Meeting 2014 October 23, 2014 H/T Carlé Pieters, Rachel Klima, Brad Jolliff, Lillian Ostrach, Tim
More informationScientific Contributions of Lunar Robotic Precursor Missions
Scientific Contributions of Lunar Robotic Precursor Missions Paul D. Spudis Johns Hopkins University Applied Physics Laboratory paul.spudis@jhuapl.edu www.spudislunarresources.com Presentation to LEAG
More informationMini-RF: An Imaging Radar for the Moon. Ben Bussey The Johns Hopkins University Applied Physics Laboratory
Mini-RF: An Imaging Radar for the Moon Ben Bussey The Johns Hopkins University Applied Physics Laboratory Paul D. Spudis President s Commission on Implementation of United States Space Exploration Policy
More informationICE IN THE FAR-IR & DIVINER 3. Far-IR Subteam: Ben Greenhagen, Christopher Edwards, Dan McCleese Additional Contributions: Tim Schofield & Paul Hayne
ICE IN THE FAR-IR & DIVINER 3 Far-IR Subteam: Ben Greenhagen, Christopher Edwards, Dan McCleese Additional Contributions: Tim Schofield & Paul Hayne WHY FAR IR? ~45µm fundamental ice feature (e.g. Moore
More informationBackground Image: SPA Basin Interior; LRO WAC, NASA/GSFC/ASU
B. L. Jolliff1, C. K. Shearer2, N. E. Petro3, D. A. Papanastassiou,4 Y. Liu,4 and L. Alkalai4 1Dept. of Earth & Planetary Sciences, Washington University, St. Louis, MO 2Institute of Meteoritics, University
More informationMicrowave brightness temperature features of lunar craters: observation from Chang E-1 mission
Microwave brightness temperature features of lunar s: observation from Chang E-1 mission Guo-Ping Hu Ke Chen Wei Guo Qing-Xia Li Hong-Yan Su Microwave brightness temperature features of lunar s: observation
More informationGlobal regolith thermophysical properties of the Moon from the Diviner Lunar Radiometer Experiment
Global regolith thermophysical properties of the Moon from the Diviner Lunar Radiometer Experiment Paul O. Hayne 1,*, Joshua L. Bandfield 2, Matthew A. Siegler 3, Ashwin R. Vasavada 1, Rebecca R. Ghent
More informationConstellation Program Office Tier 1 Regions of Interest for Lunar Reconnaissance Orbiter Camera (LROC) Imaging
Constellation Program Office Tier 1 Regions of Interest for Lunar Reconnaissance Orbiter Camera (LROC) Imaging Regions of Interest listed in alphabetical order ( no priority implied) East longitudes represented
More informationSTUDIES of the lunar regolith layer might provide the physical
384 IEEE GEOSCIENCE AND REMOTE SENSING LETTERS, VOL. 12, NO. 2, FEBRUARY 2015 Inversion of Dielectric Properties of the Lunar Regolith Media With Temperature Profiles Using Chang e Microwave Radiometer
More informationDetection of Adsorbed Water and Hydroxyl on the Moon
Detection of Adsorbed Water and Hydroxyl on the Moon Roger N. Clark U. S. Geological Survey, MS 964, Box 25046 Federal Center, Denver CO 80227, USA. E-mail: rclark@usgs.gov Data from the Visual and Infrared
More informationproviding 100-m per pixel resolution in nine ~1.0 µm wide infrared bands centered from
Supporting Text The THEMS instrument consists of separate infrared and visible imagers providing 100-m per pixel resolution in nine ~1.0 µm wide infrared bands centered from 6.78 to 14.88 µm, and 18-m
More informationLuna Resource / Glob Missions: Starting list of potential landing sites
Luna Resource / Glob Missions: Starting list of potential landing sites A.T. Basilevsky, A.M. Abdrakhimov, M.A. Ivanov, R.O. Kuzmin, E.N. Slyuta Vernadsky Institute of Geochemistry & Analytical Chemistry,
More informationLEAG Illumination Modeling at the Lunar Poles and its Benefits to Exploration and Science Investigations
LEAG 2015 2015.10.21 Illumination Modeling at the Lunar Poles and its Benefits to Exploration and Science Investigations Erwan Mazarico and J.B. Nicholas NASA GSFC Erwan Mazarico - LEAG - October 21, 2015
More informationThe Final Minute: Results from the LCROSS Solar Viewing NIR Spectrometer
The Final Minute: Results from the LCROSS Solar Viewing NIR Spectrometer Anthony Colaprete NASA Ames Research Center, Moffett Field, CA, Anthony.Colaprete-1@nasa.gov KISS: New Approaches to Lunar Ice Detection
More informationUncertainties: Limitations of Martian Granular Material Remote Sensing
Uncertainties: Limitations of Martian Granular Material Remote Sensing Albert F. C. Haldemann Jet Propulsion Laboratory, California Institute of Technology. albert.f.haldemann@jpl.nasa.gov More Data, Better
More informationIron and Titanium: Important Elements. posted October 20, References:
1 of 6 posted October 20, 1997 Moonbeams and Elements Written by G. Jeffrey Taylor Hawai'i Institute of Geophysics and Planetology To determine how a planetary body formed and evolved, we must determine
More informationDust in the Atmosphere of Mars 2017 (LPI Contrib. No. 1966)
Dust in the Atmosphere of Mars 2017 (LPI Contrib. No. 1966) MARS CLIMATE SOUNDER (MCS) OBSERVATIONS OF MARTIAN DUST A DECADE-LONG RECORD. D. M. Kass1, D. J. McCleese1, A. Kleinböhl1, J. T. Schofield1 and
More informationLyman Alpha Mapping Project (LAMP) Volatile Studies: PSR Water Frost, Lunar Atmosphere, and LCROSS Plume Observations
Lyman Alpha Mapping Project (LAMP) Volatile Studies: PSR Water Frost, Lunar Atmosphere, and LCROSS Plume Observations Kurt Southwest Research Inst. Nov. 17, 2009 THE LAMP TEAM: G.R. Gladstone, S. A. Stern,
More informationMoon and Mercury 3/8/07
The Reading Assignment Chapter 12 Announcements 4 th homework due March 20 (first class after spring break) Reminder about term paper due April 17. Next study-group session is Monday, March 19, from 10:30AM-12:00Noon
More informationMULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version E of the exam. Please fill in (E). A) This
More informationMULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.
ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version B of the exam. Please fill in (B). A) This
More informationLittle Learners Activity Guide
LUNAR RECONNAISSANCE ORBITER CAMERA Little Learners Activity Guide Learn about the Moon with puzzles, coloring, and fun facts! Mare Imbrium Mare Serenitatis Mare Tranquillitatis Oceanus Procellarum Mare
More informationToday. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week
Today Terrestrial Planet Atmospheres (continued) Events Homework DUE Review next time? Exam next week Planetary Temperature A planet's surface temperature is determined by the balance between energy from
More informationMalapert Mountain: A Recommended Site for a South Polar Outpost
For presentation at the Rutgers Symposium on Lunar Settlements, June 4-8, 2007 Malapert Mountain: A Recommended Site for a South Polar Outpost Paul. D. Lowman Jr. Goddard Space Flight Center, Code 698
More informationLRO-LOLA: Measurements of Lunar Altimetry and Surface Conditions
LRO-LOLA: Measurements of Lunar Altimetry and Surface Conditions David E. Smith, MIT Maria T. Zuber, MIT Gregory A. Neumann, GSFC Erwan Mazarico, GSFC and the LOLA Science Team Lunar-Glob Mission International
More informationSOLAR WIND VOLATILE PRESERVATION. Samantha R. Jacob Department of Geology and Geophysics University of Hawai i at Mānoa Honolulu, HI ABSTRACT
SOLAR WIND VOLATILE PRESERVATION Samantha R. Jacob Department of Geology and Geophysics University of Hawai i at Mānoa Honolulu, HI 96822 ABSTRACT Because the Moon has a negligible atmosphere and magnetosphere,
More informationarxiv: v1 [astro-ph.ep] 18 May 2016
Simulations of Particle Impact at Lunar Magnetic Anomalies and Comparison with Spectral Observations Erika Harnett Department of Earth and Space Science, University of Washington,Seattle, WA 98195-13,
More informationLunar Science from Chandrayaan-1 Data: An Indian Perspective
Lunar Science from Chandrayaan-1 Data: An Indian Perspective Introduction: During the last four decades, India has achieved a successful space based Earth Observation (EO) program, and has achieved noteworthy
More informationThe latitude dependence of dielectric breakdown on the Moon
The latitude dependence of dielectric breakdown on the Moon Andrew Jordan1,2, T. J. Stubbs3,2, J. K. Wilson1,2, P. O. Hayne4, N. A. Schwadron1,2, H. E. Spence1,2 and N. R. Izenberg5 EOS Space Science Center,
More informationLRO and the ESMD/SMD Partnership Lessons Learned. John Keller LRO Project Scientist
LRO and the ESMD/SMD Partnership Lessons Learned John Keller LRO Project Scientist LRO and the ESMD/SMD Partnership LRO is a highly successful mission of both exploration and science ESMD (Exploration
More informationTerrestrial Atmospheres
Terrestrial Atmospheres Why Is There Air? An atmosphere is a layer of gas trapped by the gravity of a planet or moon. Here s Earth s atmosphere viewed from orbit: Why Is There Air? If atoms move faster
More informationConstellation Program Office Tier 2 Regions of Interest for Lunar Reconnaissance Orbiter Camera (LROC) Imaging
Constellation Program Office Tier 2 Regions of Interest for Lunar Reconnaissance Orbiter Camera (LROC) Imaging Regions of Interest listed in alphabetical order ( no priority implied) East longitudes represented
More informationLatitudinal Enrichment of Hydrogen in the Lunar Polar Regions: Constraints on Hydrogen Mobility
Latitudinal Enrichment of Hydrogen in the Lunar Polar Regions: Constraints on Hydrogen Mobility W. V. Boynton, G. F. Droege, K. Harshman, M. A. Schaffner, I. G. Mitrofanov, T. P. McClanahan, and the LEND
More informationLunar Exploration Requirements and Data Acquisition Architectures
Lunar Exploration Requirements and Data Acquisition Architectures J. Plescia P. Spudis B. Bussey Johns Hopkins University / Applied Physics Laboratory 2005 International Lunar Conference The Vision and
More informationTHE EXOMARS CLIMATE SOUNDER (EMCS) INVESTIGATION.
THE EXOMARS CLIMATE SOUNDER (EMCS) INVESTIGATION. J. T. Schofield, D. M. Kass, A. Kleinböhl, D. J. McCleese, M. A. Allen, M. C. Foote, M. Jeganathan, Jet Propulsion Laboratory, California Institute of
More informationThe Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds
Chapter 10 Lecture The Cosmic Perspective Seventh Edition Planetary Atmospheres: Earth and the Other Terrestrial Worlds Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics
More informationLunar Precursor Robotics Program
National Aeronautics and Space Administration SCIENCE & MISSION SYSTEMS Lunar Precursor Robotics Program Michael J. Wargo, Sc.D. Chief Lunar Scientist for Exploration Systems Larry Hill LRO Mission Manager
More informationTechnologies for Transparency Dynamic Open Data Publishing with Open APIs
International Open Government Data Conference Technologies for Transparency Dynamic Open Data Publishing with Open APIs Kendall Clark, Cofounder and Managing Principal, Clark & Parsia LLC Dan Melton, Ph.D.,
More informationVenus Surface Thermal Emission Observed by VIRTIS on Venus Express
Venus Surface Thermal Emission Observed by VIRTIS on Venus Express N. Müller, J. Helbert, G. Hashimoto, C. Tsang, S. Erard, G. Piccioni, P. Drossart The VIRTIS-VEX Team Near Infrared Spectral Windows Highlands
More informationLunar Exploration Analysis Group. Report to the Planetary Science Subcommittee. 31 March 2015
Lunar Exploration Analysis Group Report to the Planetary Science Subcommittee 31 March 2015 LEAG Executive Committee Clive Neal Chair Samuel Lawrence Vice Chair James Carpenter Jasper Halekas Steve Mackwell
More informationLRO observations of morphology and surface roughness of volcanic cones and lobate lava flows in the Marius Hills
JOURNAL OF GEOPHYSICAL RESEARCH: PLANETS, VOL. 118, 615 634, doi:10.1002/jgre.20060, 2013 LRO observations of morphology and surface roughness of volcanic cones and lobate lava flows in the Marius Hills
More informationUV-V-NIR Reflectance Spectroscopy
UV-V-NIR Reflectance Spectroscopy Methods and Results A. Nathues Naturally-occurring inorganic substances with a definite and predictable chemical composition and physical properties Major groups: Silicates
More informationGale Crater Observations of Relevance to Planetary Protection
Gale Crater Observations of Relevance to Planetary Protection Ashwin Vasavada MSL Project Scientist 12/8/15 This document has been reviewed and determined not to contain export controlled technical data.
More informationLETTERS. High-resolution subsurface water-ice distributions on Mars. Joshua L. Bandfield 1
Vol 447 3 May 7 doi:10.1038/nature05781 LETTERS High-resolution subsurface water-ice distributions on Mars Joshua L. Bandfield 1 Theoretical models indicate that water ice is stable in the shallow subsurface
More informationComposition of the Moon's Crust
1 of 7 posted December 10, 2004 Composition of the Moon's Crust --- New empirical calibrations of Lunar Prospector and Clementine data yield improved global maps of Th, K, and FeO. The movie of the Moon,
More informationTesting polar spots of water-rich permafrost on the Moon: LEND observations onboard LRO
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117,, doi:10.1029/2011je003956, 2012 Testing polar spots of water-rich permafrost on the Moon: LEND observations onboard LRO I. Mitrofanov, 1 M. Litvak, 1 A. Sanin,
More informationChapter Introduction Lesson 1 Earth s Motion Lesson 2 Earth s Moon Lesson 3 Eclipses and Tides Chapter Wrap-Up. Jason Reed/Photodisc/Getty Images
Chapter Introduction Lesson 1 Earth s Motion Lesson 2 Earth s Moon Lesson 3 Eclipses and Tides Chapter Wrap-Up Jason Reed/Photodisc/Getty Images What natural phenomena do the motions of Earth and the Moon
More informationThermal removal from near infrared imaging spectroscopy data of the Moon
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116,, doi:10.1029/2010je003751, 2011 Thermal removal from near infrared imaging spectroscopy data of the Moon Roger N. Clark, 1 Carlé M. Pieters, 2 Robert O. Green,
More informationMSL Landing Site Analysis for Planetary Protection
MSL Landing Site Analysis for Planetary Protection Ashwin R. Vasavada MSL Deputy Project Scientist Jet Propulsion Laboratory, California Institute of Technology NASA Planetary Protection Subcommittee May
More informationWed. Oct. 04, Makeup lecture time? Will Friday noon work for everyone? No class Oct. 16, 18, 20?
Wed. Oct. 04, 2017 Reading: For Friday: Bugiolacchi et al. 2008 Laurence et al. 1998" Makeup lecture time? Will Friday noon work for everyone? No class Oct. 16, 18, 20? Today: Finish Lunar overview (from
More informationRecent Reflec(vity Results. Paul G. Lucey University of Hawaii Greg Neumann NASA Goddard Space Flight Center
Recent Reflec(vity Results Paul G. Lucey University of Hawaii Greg Neumann NASA Goddard Space Flight Center LOLA Lunar Orbiter Laser Al(meter 2 LOLA on LRO 3 4 5 What LOLA measures: Normal Albedo Surface
More informationChapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure
Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric
More informationChapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds
Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric
More informationChapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds
Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds What is an atmosphere? 10.1 Atmospheric Basics Our goals for learning:! What is an atmosphere?! How does the greenhouse effect warm
More informationA) usually less B) dark colored and rough D) light colored with a smooth surface A) transparency of the atmosphere D) rough, black surface
1. Base your answer to the following question on the diagram below which shows two identical houses, A and B, in a city in North Carolina. One house was built on the east side of a factory, and the other
More informationN. A. Schwadron, J. K. Wilson, M. D. Looper, A. P. Jordan, H. E. Spence, J. B. Blake, A. W. Case, Y. Iwata, J. C. Kasper, W. M. Farrell, D. J.
Signatures of Volatiles in the CRaTER Proton Albedo N. A. Schwadron, J. K. Wilson, M. D. Looper, A. P. Jordan, H. E. Spence, J. B. Blake, A. W. Case, Y. Iwata, J. C. Kasper, W. M. Farrell, D. J. Lawrence,
More informationJet Propulsion Laboratory California Institute of Technology
Broadband InfraRed Compact High-resolution Exploration Spectrometer: Lunar Volatile Dynamics for the Lunar Ice Cube Mission P.E. Clark, CalTech/Jet Propulsion Laboratory, Science PI B. Malphrus, Morehead
More informationPROSPECT: ESA s Package for Resource Observation and In-Situ Prospecting for Exploration, Commercial Exploitation and Transportation
PROSPECT: ESA s Package for Resource Observation and In-Situ Prospecting for Exploration, Commercial Exploitation and Transportation E. Sefton-Nash, J. Carpenter and the PROSPECT Team LRO/LROC/ASU Lunar
More informationChapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds. What is an atmosphere? Planetary Atmospheres
Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds What is an atmosphere? Planetary Atmospheres Pressure Composition Greenhouse effect Atmospheric structure Color of the sky 1 Atmospheres
More informationThe Moon's Dark, Icy Poles
1 of 5 posted June 4, 2003 The Moon's Dark, Icy Poles --- Permanently shadowed regions on the Moon--where frozen water could be trapped--are more abundant and more widely distributed than originally thought.
More informationChapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds
Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric
More informationStas Barabash 1 Yoshifumi Futaana 1 and the SELMA Team. Swedish Institute of Space Physics Kiruna, Sweden. DAP, Boulder, January, 2017
Stas Barabash 1 Yoshifumi Futaana 1 and the SELMA Team 1 Swedish Institute of Space Physics Kiruna, Sweden DAP, Boulder, January, 2017 1 SELMA core team 2 SELMA main scientific questions SELMA (Surface,
More informationLunar Ice Cube Orbiter: Lunar Water Dynamics via a First Generation Deep Space CubeSat
Lunar Ice Orbiter: Lunar Water Dynamics via a First Generation Deep Space Sat P.E. Clark, CalTech/Jet Propulsion Laboratory, Science PI B. Malphrus, Morehead State University, PI NASA/GSFC Payload: D.
More informationThe Surprising Lunar Maria
1 of 5 posted June 23, 2000 The Surprising Lunar Maria Written by G. Jeffrey Taylor Hawai'i Institute of Geophysics and Planetology The lunar maria, the dark, smooth areas on the Moon, formed when lava
More informationMoon 101. Bellaire High School Team: Rachel Fisher, Clint Wu, Omkar Joshi
Moon 101 Bellaire High School Team: Rachel Fisher, Clint Wu, Omkar Joshi Part I Formation of the Moon Planetary Formation In the solar nebula, dust particles coalesced to form smaller planetesimals and
More informationAccessing the Lunar Poles for Human Exploration Missions
B. KENT JOOSTEN NASA Lyndon B. Johnson Space Center Houston, Texas The National Vision for Space Exploration calls for an American return to the Moon in preparation for the human exploration of Mars and
More informationWhat is there in thee, moon, That thou shouldst move My heart so potently? By John Keats
What is there in thee, moon, That thou shouldst move My heart so potently? By John Keats The most popular view about how the moon formed was that a space object collided with the Earth. The material that
More informationEarth Science final exam study guide (Semester 2)
Earth Science final exam study guide (Semester 2) Chapter 22: astronomy, sun-earth-moon system Define the following vocabulary and answer the questions that follow Earth-Sun-Moon 1. Define nebula: 2. Identify
More informationMian Abbas, Jim Spann, Andre LeClair NASA Marshall Space Flight Center, Huntsville, AL
Lunar Dust Distributions From So Infrared Absorption Measurement With a Fourier Transform Spectrometer Mian Abbas, Jim Spann, Andre LeClair NASA Marshall Space Flight Center, Huntsville, AL John Brasunas,
More informationAgenda. Chapter 7. The Earth s Moon. The Moon. Surface Features. Magnificent Desolation. The Moon
Chapter 7 The 1 Agenda Announce: Project Part II due Tue No class next Thursday...Tgiving break! No class 12/14 (last day) Spectral Lines Lab due Pass Back Test 2 Discuss grades NYT article on gamma ray
More informationMineralogical and Geomorphological Mapping of western central part of Mare Tranquillitatis using Hyperspectral Imager onboard Chandrayaan-1
Mineralogical and Geomorphological Mapping of western central part of Mare Tranquillitatis using Hyperspectral Imager onboard Chandrayaan-1 Henal V. Bhatt 1, Paras M. Solanki 2, Mamta Chauhan 3 Geology
More informationPreliminary Scientific Results of Chang E-1 Lunar Orbiter:BasedonPayloadsDetectionData in the First Phase
0254-6124/2008/28(5)-361 09 Chin. J. Space Sci. Ouyang Ziyuan, Jiang Jingshan, Li Chunlai, Sun Huixian, Zou Yongliao, Liu Jianzhong, Liu Jianjun, Zhao Baochang, Ren Xin, Yang Jianfeng, Zhang Wenxi, Wang
More informationPTYS/ASTR Section 2 - Spring 2007 Practice Exam 2
PTYS/ASTR 206 - Section 2 - Spring 2007 Practice Exam 2 Note: The exam is scheduled for Thursday, March 29, 2007. It will be held in-class; you will have 75 minutes to finish the exam, though many of you
More informationVIRTIS-Venus Express
VIRTIS-Venus Express - G. Piccioni, P. Drossart and the VIRTIS-VenusX Team Scientific Team Members by Countries I (1) (PI) Total 14 F (2) PO ES RU NL US D UK P Total (PI) 10 1 2 2 1 2 5 2 1 (1) G. Piccioni,
More informationChapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Pearson Education, Inc.
Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric
More informationWater and Hydrogen Resources on the Moon, Mercury, and Mars*
Water and Hydrogen Resources on the Moon, Mercury, and Mars* William Ambrose 1 Search and Discovery Article #70166 (2014)** Posted August 11, 2014 *Adapted from oral presentation at AAPG Annual Convention
More informationGeological Setting of the Luna Glob Candidate Landing Site Region in the Northern High Latitudes: Characterization from LOLA and Related Data
Geological Setting of the Luna Glob Candidate Landing Site Region in the Northern High Latitudes: Characterization from LOLA and Related Data A.M. Abdrakhimov, A.T. Basilevsky, M.A. Ivanov, Vernadsky Institute,
More informationThe Moon. Tides. Tides. Mass = 7.4 x 1025 g = MEarth. = 0.27 REarth. (Earth 5.5 g/cm3) Gravity = 1/6 that of Earth
The Moon Mass = 7.4 x 1025 g = 0.012 MEarth Radius = 1738 km = 0.27 REarth Density = 3.3 g/cm3 (Earth 5.5 g/cm3) Gravity = 1/6 that of Earth Dark side of the moon We always see the same face of the Moon.
More informationKorean Pathfinder Lunar Orbiter (KPLO) Status Update
Korean Pathfinder Lunar Orbiter (KPLO) Status Update LEAG 2017 Oct 10, 2017 Gwanghyeok Ju KPLO Program Office KARI (Korea Aerospace Research Institute) 1 Agenda 2 Korean Lunar Program Overview Technology
More informationSupplementary Figure 1 Panoramic view of four sites (CE-0005, CE-0006, CE-0007, and CE-0008) measured by APXS and VNIS. Images (a), (b), and (d) were
Supplementary Figure 1 Panoramic view of four sites (CE-0005, CE-0006, CE-0007, and CE-0008) measured by APXS and VNIS. Images (a), (b), and (d) were acquired by the Panoramic Camera at the CE3-0007 site,
More informationExploring the Moon & Asteroids: A Synergistic Approach
Exploring the Moon & Asteroids: A Synergistic Approach Clive R. Neal Dept. Civil Eng. & Geological Sci. University of Notre Dame Notre Dame, IN 46556, USA neal.1@nd.edu Perspective Perspective SCIENCE
More informationThe Moon. A look at our nearest neighbor in Space! Free powerpoints at
The Moon A look at our nearest neighbor in Space! Free powerpoints at http://www.worldofteaching.com What is the Moon? A natural satellite One of more than 96 moons in our Solar System The only moon of
More informationNASA Lunar Science Activities. Lunar Science and Exploration
NASA Lunar Science Activities Lunar Science and Exploration James L. Green Director, Planetary Sciences Division Science Directorate Mission Directorate NASA In NASA s James Science L. Green Mission Presented
More informationMay 15, Lunar Reconnaissance Orbiter (LRO) Instrument Thermal Balance and Thermal Vacuum Direction. Rev. (Initial) j Mission
j Mission Lunar Reconnaissance Orbiter (LRO) Report Title Instrument Thermal Balance and Thermal Vacuum Direction Date May 15, 2006 Revision Rev. (Initial) Prepared By: Charles Baker LRO Thermal Lead Scope/Purpose:
More informationGeneral Comments about the Atmospheres of Terrestrial Planets
General Comments about the Atmospheres of Terrestrial Planets Mercury Very little atmosphere Contents: vaporized micrometeorites, solar wind Sky is black Venus Very thick (10% density of water), dense
More informationToday. Events. Terrestrial Planet Atmospheres (continued) Homework DUE
Today Terrestrial Planet Atmospheres (continued) Events Homework DUE Sources of Gas Outgassing from volcanoes 2014 Pearson Education, Inc. Evaporation of surface liquid; sublimation of surface ice (cometary
More informationOutline. Planetary Atmospheres. General Comments about the Atmospheres of Terrestrial Planets. General Comments, continued
Outline Planetary Atmospheres Chapter 10 General comments about terrestrial planet atmospheres Atmospheric structure & the generic atmosphere Greenhouse effect Magnetosphere & the aurora Weather & climate
More informationM-Type asteroids: primitive, metallic, or both?
Artist s concept of mission to (16) Psyche NASA/JPL-Caltech M-Type asteroids: primitive, metallic, or both? Zoe A. Landsman 1 Collaborators: J. Emery 2, H. Campins 1 1 University of Central Florida, Orlando,
More informationChandrayaan Mission Objectives and future lunar programs
Chandrayaan Mission Objectives and future lunar programs CHANDRAYAAN -I Paul Spudis, channeling J. N. Goswami Principal Scientist, Chandrayaan-1 Mission The Clementine & Lunar Prospector Missions to Moon
More informationDana Felberg Steven Hester David Nielsen Zach Weddle Jack Williams
Dana Felberg Steven Hester David Nielsen Zach Weddle Jack Williams To identify key features on the lunar surface near the Apollo 11 Landing site in the Mare Tranquillitatis. Apollo 11 launched: 16 July
More informationNEXT STEPS ON THE MOON REPORT OF THE SPECIFIC ACTION TEAM
NEXT STEPS ON THE MOON REPORT OF THE SPECIFIC ACTION TEAM Specific Action Team Charter SAT commissioned by Science Mission Directorate, Planetary Science Division Assess lunar missions needed to address
More informationNational Science Olympiad 2014 Division B: Solar System May 17th 2014
National Science Olympiad 2014 Division B: Solar System May 17th 2014 Sponsored by the University of Texas Institute for Geophysics Team Number: Team Name: Questions 1-24 refer to the images in Image Set
More informationREVISED COORDINATES FOR APOLLO HARDWARE
REVISED COORDINATES FOR APOLLO HARDWARE R. V. Wagner *, E. J. Speyerer, K. N. Burns, J. Danton, M.S. Robinson Lunar Reconnaissance Orbiter Camera, School of Earth and Space Exploration, Arizona State University,
More informationMARS CLIMATE DATABASE VERSION 4.3 VALIDATION DOCUMENT - DRAFT -
MARS CLIMATE DATABASE VERSION 4.3 VALIDATION DOCUMENT - DRAFT - E. Millour, F. Forget (LMD, Paris) May 2008 1. Introduction This document presents comparisons between available data and outputs of the
More informationMercury = Hermes Mythology. Planet Mercury, Element, Mercredi God of Commerce, Messenger God, guide to Hades Winged sandals and staff
Mercury = Hermes Mythology Planet Mercury, Element, Mercredi God of Commerce, Messenger God, guide to Hades Winged sandals and staff Mercury s Orbit Mercury never seen more than 28 from the sun Revolves/orbits
More informationHow Can radar See? Introduction to radar Imaging
How Can radar See? Introduction to radar Imaging Teacher Guide Purpose To understand the complexities of radar imaging, this series of activities will cover some basic concepts of the electromagnetic spectrum.
More informationChapter 22 Exam Study Guide
Chapter 22 Exam Study Guide Name: Hour: Date: Multiple Choice Identify the choice that best completes the statement or answers the question. Write the letter that best answers the question or completes
More informationRationale of NASA Lunar Precursor Robotic Program (LPRP) for the VSE
Rationale of NASA Lunar Precursor Robotic Program (LPRP) for the VSE (vs. I don t need nuthin but a map) Jeff Plescia, Ben Bussey, Paul Spudis, Tony Lavoie Applied Physics Laboratory, Johns Hopkins University
More information