Civil War Bounties 1861-1865

Total Page:16

File Type:pdf, Size:1020Kb

Civil War Bounties 1861-1865 Chester County Civil War Bounties 1861-1865 Last Name First Name Middle Name Residence/To Age Rank Company Regiment/Unit Year Folder See/Page Record Cable John 21st PA Cavalry 1863‐1864 OS #5 5 Bounty List Cable John 21st PA Cavalry 1865 71 Bounty Volume Cabreza Miguel Willistown 19 1864 3 Receipts Cahill James East 27 45th 1864 26 Cahill, James Receipts Nottingham Cahill James East 1864 165 Bounty Nottingham Volume Cain George East 1864 165 Bounty Nottingham Volume Cain George East 22 5th PA Cavalry 1864 3 Receipts Nottingham Cain Samuel G 55th 1865 79 Bounty Volume Cain William Willistown 28 17 Bounty List Cain William U.S.C.T. 1864 125 Bounty Volume Cain William Willistown 1864 28 47 Bounty List Cain William Willistown 1864 190 Bounty Volume Cairnes William Honey Brook 1862 OS #3 4 1st Draft List Cake William J.B 1st PA Reserve 1863‐1864 OS #4 1 Bounty List Cake William J.1st Sergt. 1st Infantry P.R.C. 1863‐1864 OS #5 4 Bounty List Chester County Archives and Record Services, West Chester, PA 19380 Last Name First Name Middle Name Residence/To Age Rank Company Regiment/Unit Year Folder See/Page Record Cake William J.A 1st PA Reserves 1864 102 Bounty Volume Calahan John New Garden 28 29 Bounty List Calahan John New Garden 1864 162 Bounty Volume Calaman Charles W. U.S.C.T. 1864 125 Bounty Volume Calderwood John Private D 53rd 1863‐1864 OS #5 4 Bounty List Calderwood John D 53rd 1863‐1864 OS #4 4 Bounty List Calderwood John D 53rd 1865 84 Bounty Volume Caldwell John Drummer H 53rd 1863‐1864 OS #5 4 Bounty List Caldwell John C.H 53rd 1863‐1864 OS #4 5 Bounty List Caldwell John C.H 53rd 1865 85 Bounty Volume Caldwell Patrick West Chester 28 53 Bounty List Caldwell Patrick West Chester 1864 191 Bounty Volume Cale John East Vincent 1862 OS #3 7 1st Draft List Calhoon Alfred East Bradford 1864 133 Bounty Volume Callahan George East Vincent 18 1864 26 Riley, Thomas Receipts Callahan John East Coventry 1862 OS #3 2 1st Draft List Callahan John New Garden 1864 28 51 Bounty List Chester County Archives and Record Services, West Chester, PA 19380 Last Name First Name Middle Name Residence/To Age Rank Company Regiment/Unit Year Folder See/Page Record Callahan John C. Philadelphia 20Private B 29th 1865 3 Applicati ons Callahan John C.B 29th 1865 43 Bounty Volume Callen John 1864 94 Bounty Volume Calvert George P. 20th PA Cavalry 1863‐1864 OS #5 4 Bounty List Calvert George P. 20th PA Cavalry 1865 87 Bounty Volume Calvin John West Chester 1864 192 Bounty Volume Calvin Robert New London 1862 OS #3 13 1st Draft List Cam Clement J.B 11th PA Cavalry 1864 100 Bounty Volume Camelans James East Pikeland 34 1864 3 Receipts Camelans James East Pikeland 1864 173 Bounty Volume Cameron Nicholas F 55th 1863‐1864 OS #4 23 Bounty List Cameron Nicholas F 55th 1865 78 Bounty Volume Campbell Anthony C 55th 1863‐1864 OS #4 20 Bounty List Campbell Anthony C 55th 1865 75 Bounty Volume Campbell Archibald West 1862 OS #3 3 1st Draft Nottingham List Campbell Coleman South 1862 OS #3 11 1st Draft Coventry List Campbell Frank A. West 1864 174 Bounty Pikeland Volume Chester County Archives and Record Services, West Chester, PA 19380 Last Name First Name Middle Name Residence/To Age Rank Company Regiment/Unit Year Folder See/Page Record Campbell Frank A. West 1864 25 Daum, Receipts Pikeland Frederick Campbell George W. East Pikeland 27 186th 1864 3 Receipts Campbell George W. East Pikeland 1864 173 Bounty Volume Campbell James M. Birmingham 1864 133 Bounty Volume Campbell John C. Capt. 27 3 Bounty Whitcraft's List Campbell John C. East 1864 28 51 Bounty Nottingham List Campbell John C.A 29th 1865 41 Bounty Volume Campbell John C. West 23Corporal A 29th 1865 3 Applicati Nottingham ons Campbell Robert H. Capt. 27 3 Bounty Whitcraft's List Campbell Robert H. West 1864 174 Bounty Pikeland Volume Campbell Robert H. West 1864 25 Daum, Receipts Pikeland Frederick Campbell Robert W.B 43rd 1863 19 Bounty Volume Campbell Samuel F 55th 1863‐1864 OS #4 23 Bounty List Campbell Samuel Private D 1st Infantry P.R.C. 1863‐1864 OS #5 4 Bounty List Campbell Samuel D 1st PA Reserve 1863‐1864 OS #4 1 Bounty List Campbell Samuel D 1st PA Reserves 1864 102 Bounty Volume Campbell Samuel F 55th 1865 78 Bounty Volume Chester County Archives and Record Services, West Chester, PA 19380 Last Name First Name Middle Name Residence/To Age Rank Company Regiment/Unit Year Folder See/Page Record Campbell William D 192nd 1864 129 Bounty Volume Campbell William C. East 28 16 Bounty Nottingham List Campbell William C. East 1864 165 Bounty Nottingham Volume Cannon Henry Willistown 1864 190 Bounty Volume Cannon John New Garden 28 29 Bounty List Cannon John New Garden 1864 28 45 Bounty List Cannon John New Garden 1864 162 Bounty Volume Carbaugh Anderson F 55th 1865 78 Bounty Volume Carbough Anderson F 55th 1863‐1864 OS #4 22 Bounty List Cardell Arthur 31 1st Battalion 1864 3 Receipts Cardell Arthur West Chester 1864 192 Bounty Volume Carey Charles Sadsbury 28 52 Bounty List Carey Charles Sadsbury 1864 28 51 Bounty List Carey Charles Sadsbury 1864 177 Bounty Volume Carl Daniel G.Private F 105th 1863‐1864 OS #5 5 Bounty List Carl Daniel G. 105th 1864 121 Bounty Volume Carl Henry 50th 1863‐1864 OS #5 5 Bounty List Chester County Archives and Record Services, West Chester, PA 19380 Last Name First Name Middle Name Residence/To Age Rank Company Regiment/Unit Year Folder See/Page Record Carl Henry H 50th 1863‐1864 OS #4 9 Bounty List Carl Henry 50th 1864 119 Bounty Volume Carlen David U.S. Cavalry 1865 70 Bounty Volume Carlisle Theodore London 1862 OS #3 10 1st Draft Britain List Carlow David U.S. Cavalry 1863‐1864 OS #5 4 Bounty List Carman Henry Willistown 26 203rd 1864 3 Receipts Carman John L. Lionville J. W. 27 7 Bounty Hawley's List Carman John L. 1862 3 Receipts Carman Ringold Lionville J. W. 27 7 Bounty Hawley's List Carmhael John East 28 34 Bounty Marlborough List Carmhael John East 1864 158 Bounty Marlborough Volume Carmichael John East 1864 28 44 Bounty Marlborough List Carnes Robert C 47th 1863 28 Bounty Volume Carney George W.Sergeant I 51st 1863‐1864 OS #5 4 Bounty List Carney George W.I 51st 1863‐1864 OS #4 9 Bounty List Carney George W.F 51st 1864 110 Bounty Volume Carney Thompson 1863‐1864 OS #5 4 Bounty List Chester County Archives and Record Services, West Chester, PA 19380 Last Name First Name Middle Name Residence/To Age Rank Company Regiment/Unit Year Folder See/Page Record Carney Thompson 1864 92 Bounty Volume Carpenter David A 43rd 1863 23 Bounty Volume Carpenter David 44A 43rd 1863 OS #1 1 Descripti ve Carpenter John 1863‐1864 OS #5 5 Bounty List Carpenter John 1864 96 Bounty Volume Carpenter T. West Chester Capt. Otley's 27 4 Bounty Company List Carpenter William C. Independent 1865 51 Bounty Continental Troop Volume Carpenter William C. West 24Sergeant Continental 1865 3 Applicati Brandywine Independent ons Carr Clement J. Tredyffrin 28 26 Bounty List Carr Clement J.E 11th PA Cavalry 1863‐1864 OS #4 10 Bounty List Carr Clement J.Sergeant B 11th PA Volunteer 1863‐1864 OS #5 4 Bounty Cavalry List Carr Henry Franklin 28 25 Bounty List Carr Henry Franklin 1864 147 Bounty Volume Carr Henry Franklin 1864 28 48 Bounty List Carr McClees Tredyffrin 28 26 Bounty List Carr Morton C. Tredyffrin 28 26 Bounty List Carr Richard West Chester 28 53 Bounty List Chester County Archives and Record Services, West Chester, PA 19380 Last Name First Name Middle Name Residence/To Age Rank Company Regiment/Unit Year Folder See/Page Record Carr Richard West 28 28 Bounty Fallowfield List Carr Richard West 1864 28 51 Bounty Fallowfield List Carr Richard West Chester 1864 191 Bounty Volume Carr Richard West Chester 1864 28 47 Bounty List Carr William West ChesterPrivate West Chester Rifles OS #2 1 Muster Roll Carr William K. Pennsbury 28 42 Bounty List Carr William K. Pennsbury 1864 171 Bounty Volume Carr William K. Pennsbury 1864 28 48 Bounty List Carrington Edwin T. West 1864 161 Bounty Nantmeal Volume Carrington Edwin T. West 25I 45th U.S.C.T. 1864 3 Receipts Nantmeal Carroll Dennis 1863‐1864 OS #5 5 Bounty List Carroll Dennis 1864 99 Bounty Volume Carson John Phoenixville, 1864 25 Horan, Receipts South Ward Thomas Carson Michael Phoenixville, 28 54 Bounty South List Carson Michael Phoenixville 1864 28 51 Bounty List Carson Uriah D 192nd 1864 129 Bounty Volume Carson William Pennsbury 28 42 Bounty List Chester County Archives and Record Services, West Chester, PA 19380 Last Name First Name Middle Name Residence/To Age Rank Company Regiment/Unit Year Folder See/Page Record Carson William Pennsbury 1864 28 49 Bounty List Carson William Pennsbury 1864 171 Bounty Volume Carter Andrew Private 1863‐1864 OS #5 4 Bounty List Carter Andrew 1864 95 Bounty Volume Carter Francis E 97th 1863‐1864 OS #4 14 Bounty List Carter Francis E 97th 1864 114 Bounty Volume Carter George H. Tredyffrin 28 33 Bounty List Carter George H. Tredyffrin 1864 178 Bounty Volume Carter George W. Tredyffrin 1864 28 47 Bounty List Carter John Lower Oxford 20 5th PA Cavalry186425Howell, Receipts James Carter John Lower Oxford 20 5th PA Cavalry 1864 26 Smith, Receipts William Carter John Lower Oxford 1864 169 Bounty Volume Carter John J.C 43rd 1863 16 Bounty Volume Carter Joseph Phoenixville, 28 54 Bounty South List Carter Joseph Phoenixville 1864 28 49 Bounty List Carter Patrick West ChesterPrivate West Chester Rifles OS #2 1 Muster Roll Carter William Henry J.
Recommended publications
  • March 21–25, 2016
    FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk,
    [Show full text]
  • The Multiplexed Squid Tes Array at Ninety Gigahertz (Mustang)
    University of Pennsylvania ScholarlyCommons Publicly Accessible Penn Dissertations Spring 2011 The Multiplexed Squid Tes Array at Ninety Gigahertz (Mustang) Phillip M. Korngut University of Pennsylvania, [email protected] Follow this and additional works at: https://repository.upenn.edu/edissertations Part of the External Galaxies Commons, and the Instrumentation Commons Recommended Citation Korngut, Phillip M., "The Multiplexed Squid Tes Array at Ninety Gigahertz (Mustang)" (2011). Publicly Accessible Penn Dissertations. 317. https://repository.upenn.edu/edissertations/317 This paper is posted at ScholarlyCommons. https://repository.upenn.edu/edissertations/317 For more information, please contact [email protected]. The Multiplexed Squid Tes Array at Ninety Gigahertz (Mustang) Abstract The Multiplexed SQUID/TES Array at Ninety Gigahertz (MUSTANG) is a bolometric continuum imaging camera designed to operate at the Gregorian focus of the 100m Green Bank Telescope (GBT) in Pocahontas county, West Virginia. The combination of the GBT's large collecting area and the 8x8 array of transition edge sensors at the heart of MUSTANG allows for deep imaging at 10'' resolution at 90GHz. The MUSTANG receiver is now a facility instrument of the National Radio Astronomy Observatory available to the general astronomical community. The 3.3mm continuum passband is useful to access a large range of Galactic and extra-Galactic astrophysics. Sources with synchrotron, free-free and thermal blackbody emission can be detected at 3.3mm. Of particular interest is the Sunyaev Zel'dovich effect in clusters of galaxies, which arises from the inverse Compton scattering of CMB photons off hot electrons in the intra-cluster medium. In the MUSTANG band, the effect is observationally manifested as an artificial decrement in power on the sky in the direction of the cluster.
    [Show full text]
  • GRAIL Gravity Observations of the Transition from Complex Crater to Peak-Ring Basin on the Moon: Implications for Crustal Structure and Impact Basin Formation
    Icarus 292 (2017) 54–73 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus GRAIL gravity observations of the transition from complex crater to peak-ring basin on the Moon: Implications for crustal structure and impact basin formation ∗ David M.H. Baker a,b, , James W. Head a, Roger J. Phillips c, Gregory A. Neumann b, Carver J. Bierson d, David E. Smith e, Maria T. Zuber e a Department of Geological Sciences, Brown University, Providence, RI 02912, USA b NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA c Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, MO 63130, USA d Department of Earth and Planetary Sciences, University of California, Santa Cruz, CA 95064, USA e Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA 02139, USA a r t i c l e i n f o a b s t r a c t Article history: High-resolution gravity data from the Gravity Recovery and Interior Laboratory (GRAIL) mission provide Received 14 September 2016 the opportunity to analyze the detailed gravity and crustal structure of impact features in the morpho- Revised 1 March 2017 logical transition from complex craters to peak-ring basins on the Moon. We calculate average radial Accepted 21 March 2017 profiles of free-air anomalies and Bouguer anomalies for peak-ring basins, protobasins, and the largest Available online 22 March 2017 complex craters. Complex craters and protobasins have free-air anomalies that are positively correlated with surface topography, unlike the prominent lunar mascons (positive free-air anomalies in areas of low elevation) associated with large basins.
    [Show full text]
  • Geological Mapping of Lunar Crater Lalande: Topographic Configuration, Morphology and Cratering Process
    The International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, Volume XLII-3/W1, 2017 2017 International Symposium on Planetary Remote Sensing and Mapping, 13–16 August 2017, Hong Kong GEOLOGICAL MAPPING OF LUNAR CRATER LALANDE: TOPOGRAPHIC CONFIGURATION, MORPHOLOGY AND CRATERING PROCESS B. Li a, b*, Z.C. Ling a, J. Zhanga, J. Chen a, C.Q. Liu a, X.Y. Bi a a Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment; Institute of Space Sciences, Shandong University, Weihai, China. - [email protected] b Key Laboratory of Lunar and Deep Space Exploration, Beijing, China. Commission VI, WG VI/4 KEY WORDS: Crater Lalande, Geological mapping, Low-relief bulges, Cratering process, Elevation differences ABSTRACT: Highland crater Lalande (4.45°S, 8.63°W; D=23.4 km) is located on the PKT area of the lunar near side, southeast of Mare Insularum. It is a complex crater in Copernican era and has three distinguishing features: high silicic anomaly, highest Th abundance and special landforms on its floor. There are some low-relief bulges on the left of crater floor with regular circle or ellipse shapes. They are ~250 to 680 m wide and ~30 to 91 m high with maximum flank slopes >20°. There are two possible scenarios for the formation of these low-relief bulges which are impact melt products or young silicic volcanic eruptions. According to the absolute model ages of ejecta, melt ponds and hummocky floor, the ratio of diameter and depth, similar bugle features within other Copernican-aged craters and lack of volcanic source vents, we hypothesized that these low-relief bulges were most consistent with an origin of impact melts during the crater formation instead of small and young volcanic activities occurring on the crater floor.
    [Show full text]
  • O Lunar and Planetary Institute Provided by the NASA Astrophysics Data System 414 LPS XXVII
    LPS XXVII THE COMPOSITION AND GEOLOGIC SETTING OF LUNAR FAR SIDE MARIA. Jeffrey J. illi is', & Paul D. ~~udis"', 1. Dept. of Geology and Geophysics, Rice University, Houston TX, 77005 2. Lunar and Planetary Institute, Houston Texas 77058. The dichotomy in the distribution of maria between the Earth facing side and the far side of the Moon has evoked many questions concerning the emplacement mechanisms, compositional variation, and source regions of lunar basalts. The near side maria have been well analyzed using a variety of Earth based, and lunar surface and satellite information. The Clementine mission has provided the first global mineralogical and chemical maps for the Moon. These data will allow us to gain knowledge of many lunar far side basalt deposits for the first time. Although the far side maria (Figure 1) represents only about 1% of the surface of the Moon [I], these deposits provide insight into the crustal evolution, thermal history, and the interior of the Moon. Information on the composition, age, and volume of mare deposits will further our understanding of these questions. We are now studying several data sets, including multi-spectral images, crater statistics, and altimetry, to reconstruct and understand lunar volcanic evolution. Ultravioletlvisible (UVVIS) image data provide information of the composition of mare deposits. Ratios 4151750 provide information of titanium content [2,4] and the 9501750 absorptions is correlated with the concentration of ~e~+and mafic minerals [2, 31. Crater statistics provide relative age determination, which can be used to estimate absolute ages. Knowing the range in ages of all the mare units on the far side will allow us to determine the duration of magmatism on the far side.
    [Show full text]
  • The Lassell Massif-A Silicic Lunar Volcano
    Icarus 273 (2016) 248–261 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus The Lassell massif—A silicic lunar volcano ∗ J.W. Ashley a, b , , M.S. Robinson a, J.D. Stopar a, T.D. Glotch c, B. Ray Hawke d, C.H. van der Bogert e, H. Hiesinger e, S.J. Lawrence a, B.L. Jollifff, B.T. Greenhagen g, T.A. Giguere d, D.A. Paige h a School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85281, USA b Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA c Department of Geosciences, Stony Brook University, Stony Brook, NY 11794, USA d Hawaii Institute of Geophysics and Planetology, School of Ocean and Earth Science and Technology, University of Hawaii, Honolulu, HI 96822, USA e Institut für Planetologie, Westfälische Wilhelms-Universität, Münster, Germany f Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63105, USA g Johns Hopkins University – Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA h Department of Earth and Space Sciences, University of California Los Angeles, Los Angeles, CA 90095, USA a r t i c l e i n f o a b s t r a c t Article history: Lunar surface volcanic processes are dominated by mare-producing basaltic extrusions. However, spec- Received 24 June 2014 tral anomalies, landform morphology, and granitic or rhyolitic components found in the Apollo sample Revised 20 November 2015 suites indicate limited occurrences of non-mare, geochemically evolved (Si-enriched) volcanic deposits. Accepted 14 December 2015 Recent thermal infrared spectroscopy, high-resolution imagery, and topographic data from the Lunar Re- Available online 30 December 2015 connaissance Orbiter (LRO) show that most of the historic “red spots” and other, less well-known loca- Keywords: tions on the Moon, are indeed silica rich (relative to basalt).
    [Show full text]
  • Magmatic Volatiles (H, C, N, F, S, Cl) in the Lunar Mantle, Crust, and Regolith: Abundances, Distributions, Processes, and Reservoirs†K
    American Mineralogist, Volume 100, pages 1668–1707, 2015 THE SECOND CONFERENCE ON THE LUNAR HIGHLANDS CRUST AND NEW DIRECTIONS REVIEW Magmatic volatiles (H, C, N, F, S, Cl) in the lunar mantle, crust, and regolith: Abundances, distributions, processes, and reservoirs†k FRANCIS M. MCCUBBIN1,2,*, KATHLEEN E. VANDER KAADEN1,2, ROMAIN TARTÈSE3, RACHEL L. KLIMA4, YANG LIU5, JAMES MORTIMER3, JESSICA J. BARNES3,6, CHARLES K. SHEARER1,2, ALLAN H. TREIMAN7, DAVID J. LAWRENCE3, STEPHEN M. ELARDO1,2,8, DANA M. HURLEY3, JEREMY W. BOYCE9 AND MAHESH ANAND3,6 1Institute of Meteoritics, University of New Mexico, 200 Yale Blvd SE, Albuquerque, New Mexico 87131, U.S.A. 2Department of Earth and Planetary Sciences, University of New Mexico, 200 Yale Blvd SE, Albuquerque, New Mexico 87131, U.S.A. 3Planetary and Space Sciences, The Open University, Walton Hall, Milton Keynes, MK7 6AA, U.K. 4Planetary Exploration Group, Space Department, Johns Hopkins University Applied Physics Lab, Laurel, Maryland 20723, U.S.A. 5Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, U.S.A. 6Department of Earth Sciences, The Natural History Museum, Cromwell Road, London, SW7 5BD, U.K. 7Lunar and Planetary Institute, USRA, 3600 Bay Area Boulevard, Houston, Texas 77058, U.S.A. 8Geophysical Laboratory, Carnegie Institution of Washington, 5251 Broad Branch Road NW, Washington, D.C. 20015, U.S.A. 9Department of Earth and Space Sciences, University of California, Los Angeles, California 90095-1567, U.S.A. ABSTRACT Many studies exist on magmatic volatiles (H, C, N, F, S, Cl) in and on the Moon, within the last several years, that have cast into question the post-Apollo view of lunar formation, the distribution and sources of volatiles in the Earth-Moon system, and the thermal and magmatic evolution of the Moon.
    [Show full text]
  • Understanding the Lunar Surface and Space-Moon Interactions Paul Lucey1, Randy L
    Reviews in Mineralogy & Geochemistry Vol. 60, pp. 83-219, 2006 2 Copyright © Mineralogical Society of America Understanding the Lunar Surface and Space-Moon Interactions Paul Lucey1, Randy L. Korotev2, Jeffrey J. Gillis1, Larry A. Taylor3, David Lawrence4, Bruce A. Campbell5, Rick Elphic4, Bill Feldman4, Lon L. Hood6, Donald Hunten7, Michael Mendillo8, Sarah Noble9, James J. Papike10, Robert C. Reedy10, Stefanie Lawson11, Tom Prettyman4, Olivier Gasnault12, Sylvestre Maurice12 1University of Hawaii at Manoa, Honolulu, Hawaii, U.S.A. 2Washington University, St. Louis, Missouri, U.S.A. 3University of Tennessee, Knoxville, Tennessee, U.S.A. 4Los Alamos National Laboratory, Los Alamos, New Mexico, U.S.A. 5Smithsonian Institution, Washington D.C., U.S.A. 6Lunar and Planetary Laboratory, Univ. of Arizona, Tucson, Arizona, U.S.A. 7University of Arizona, Tucson, Arizona, U.S.A. 8Boston University, Cambridge, Massachusetts, U.S.A. 9Brown University, Providence, Rhode Island, U.S.A. 10University of New Mexico, Albuquerque, New Mexico, U.S.A. 11 Northrop Grumman, Van Nuys, California, U.S.A. 12Centre d’Etude Spatiale des Rayonnements, Toulouse, France Corresponding authors e-mail: Paul Lucey <[email protected]> Randy Korotev <[email protected]> 1. INTRODUCTION The surface of the Moon is a critical boundary that shapes our understanding of the Moon as a whole. All geologic mapping and remote sensing techniques utilize only the outermost portion of the Moon. Before leaving the Moon for study in our laboratories, all lunar samples that have been studied existed at or very near the surface. With the exception of the deeply probing geophysical techniques, our understanding of the interior of the Moon is derived from surficial, but not superficial, information, coupled with geologic reasoning.
    [Show full text]
  • The Distribution of Mg-‐Spinel Across the Moon and Constraints on Crustal
    Pieters 4776 Revision1: February 2014 The Distribution of Mg-Spinel across the Moon and Constraints on Crustal Origin Carle M. Pieters1 Kerri Donaldson Hanna1 Leah Cheek1 Deepak Dhingra1 Tabb Prissel1 Colin Jackson1 Daniel Moriarty1 Stephen Parman1 2 Lawrence A. Taylor 1Department of Geological Sciences, Brown University, Providence, RI 02912 USA 2Planetary Geosciences Institute; University of Tennessee, Knoxville, TN 37996 USA Submitted to American Mineralogist [special issue on Lunar Highland Crust (and Spinels?)] DATE: October 2013 REVISED: February 2014 1 Pieters 4776 Revision1: February 2014 1 Abstract 2 A robust assessment is made of the distribution and (spatially resolved) geologic context for 3 the newly identified rock type on the Moon, a Mg-spinel-bearing anorthosite (Pink-Spinel 4 Anorthosite, PSA). Essential criteria for confirmed detection of Mg-spinel using spectroscopic 5 techniques are presented and these criteria are applied to recent data from the Moon Mineralogy 6 Mapper. Altogether, 23 regions containing confirmed exposures of the new Mg-spinel rock type 7 are identified. All exposures are in highly feldspathic terrain and are small – a few hundred 8 meters - but distinct and verifiable, most resulting from multiple measurements. Each confirmed 9 detection is classified according to geologic context along with other lithologies identified in the 10 same locale. Confirmed locations include areas along the inner rings of four mascon basins, 11 knobs within central peaks of a few craters, and dispersed exposures within the terraced walls of 12 several large craters. Unexpected detections of Mg-spinel are also found at a few areas of 13 hypothesized non-mare volcanism. The small Mg-spinel exposures are shown to be global in 14 distribution, but generally associated with areas of thin crust.
    [Show full text]
  • Science Concept 3: Key Planetary Processes Are Manifested in the Diversity of Lunar Crustal Rocks
    Science Concept 3: Key Planetary Processes are Manifested in the Diversity of Lunar Crustal Rocks Science Concept 3: Key planetary processes are manifested in the diversity of crustal rocks Science Goals: a. Determine the extent and composition of the primary feldspathic crust, KREEP layer, and other products of differentiation. b. Inventory the variety, age, distribution, and origin of lunar rock types. c. Determine the composition of the lower crust and bulk Moon. d. Quantify the local and regional complexity of the current lunar crust. e. Determine the vertical extent and structure of the megaregolith. INTRODUCTION Formation and Evolution of the Moon The Moon is a unique environment, preserving crucial information about the early history and later evolution of the solar system. The lack of major surficial tectonic processes within the past few billion years or so, as well as the lack of significant quantities of surface water, have allowed for excellent preservation of the lithologies and geomorphological features that formed during the major planetary formation events. Fundamental discoveries during the Apollo program showed that the Moon is made up of a variety of volcanic and impact rock types that exhibit a particular range of chemical and mineralogical compositions. The key planetary processes conveyed by this diversity include planetary differentiation, volcanism, and impact cratering. Analysis of Apollo, Luna, and lunar meteoritic samples, as well as orbital data from a series of lunar exploration missions, generated geophysical models that strove to tell the story of the Moon. However, such models are restricted in the sense that they are based on information gathered from the samples that have so far been acquired.
    [Show full text]
  • Listing of Preserved Farms
    New Jersey Farmland Preservation Program Permanently Preserved Farmland by County Per State Original Total State Acre Cost Type of Date County Municipality Owner Acres Cost Cost Total Share Acquisition Closed Cost Percent Atlantic Buena Boro Castellari, Doug & Maria 34.8700 181,324.00 181,324.00 5,200.00 100.00% SADC EP 11/14/2002 Atlantic Buena Boro Castellari, Edward G. & Lucy R. 18.1320 99,726.00 99,726.00 5,500.00 100.00% SADC EP 03/26/2002 Atlantic Buena Boro Consalo Farms Inc. II 33.5060 136,805.00 136,805.00 4,083.00 100.00% SADC EP 02/19/2009 Atlantic Buena Boro Consalo, Vincent Jr. I 66.3850 262,685.45 262,685.45 3,957.00 100.00% SADC EP 02/19/2009 Atlantic Buena Boro John, Jack Baylis 19.0210 35,545.01 35,545.01 1,868.72 100.00% SADC Pine EP 05/26/2004 Atlantic Buena Boro Ralph Donato 88.5000 283,200.00 169,200.00 3,200.00 59.75% SADC Pine EP 03/24/2003 Atlantic Buena Vista Twp. Galbiati, Arnold 57.7710 380,806.80 380,806.80 6,591.66 100.00% SADC EP 06/30/2009 Atlantic Egg Harbor Twp. (Erickson) Fleming, George & Cynthia 62.3510 195,600.00 195,600.00 3,137.08 100.00% SADC EP 07/21/2011 Atlantic Egg Harbor Twp. Handson, Arthur L. 131.6250 191,756.25 191,756.25 1,456.84 100.00% SADC EP 11/30/2010 Atlantic Folsom Boro Eckhardt, George J.
    [Show full text]
  • ANNUAL REPORT Fiscal Year 2009
    DEPARTMENT OF DEFENSE ANNUAL REPORT Fiscal Year 2009 Maj. Gen. Robert G.F. Lee Adjutant General 3949 Diamond head Road, Honolulu, Hawaii 96816-4495 (808) 733-4246 / 733-4238 Fax Website: www.hawaii.gov/dod Dear Governor Lingle: It is my privilege to present the State of Hawaii, Department of Defense Annual Report for FY09. The Hawaii Army National Guard performed its federal and state missions to the highest standards during the 29th Infantry Brigade Combat Team’s deployment to Kuwait and Iraq and during recovery RSHUDWLRQVIROORZLQJÁRRGLQJKHUHDWKRPH The Hawaii Air National Guard moved into new roles and missions, standing up an Air Operations *URXSDQGDQHZ,QWHO6TXDGURQ$LU*XDUGSHUVRQQHODOVRFRQWULEXWHGWRÁRRGUHFRYHU\HIIRUWVDVZHOODV 0HGLFDO,QQRYDWLYH5HDGLQHVVWUDLQLQJEHQHÀWWLQJQHHG\+DZDLLUHVLGHQWV State Civil Defense established the Governor’s Interagency Volcano Task Force to investigate the effects of increased volcanic emissions while continuing to improve the processes for preventing and/or mitigating future disasters. 7KH2IÀFHRI9HWHUDQV6HUYLFHVKHOGLWVDQQXDO9HWHUDQV'D\DQG0HPRULDO'D\FHUHPRQLHVDWWKH Hawaii State Veterans Cemetery, while overseeing the burial and care of more than 3,000 grave sites there. The Youth Challenge Academy graduated two more classes, bringing to more than 2,700 cadets who’ve EHQHÀWWHGIURPWKHSURJUDP ,WKDVEHHQDQKRQRUDQGSULYLOHJHWRKDYHVHUYHGDVWKH6WDWH$GMXWDQW*HQHUDODVZHPRYHLQWRWKHÀQDO year of your administration. Sincerely, ROBERT G.F.LEE Major General Hawaii Army National Guard Adjutant General HAPPY 373RD – Retired Command Sgt. Maj. James Reis, Pfc. Amber Sevidal and Master Sgt. Francis Hapenny representing the retirees, and, the youngest and oldest active Hawaii National Guard members at the 373rd National Guard birthday ball are assisted by Command Chief Master Sgt. Denise M. Jelinski-Hall, the senior enlisted advisor, to cut the birthday cake at the Ihilani Resort on Dec 12, 2009.
    [Show full text]