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Multiple Asteroid Systems: Dimensions and Thermal Properties from Spitzer Space Telescope and Ground-Based Observations*
Multiple Asteroid Systems: Dimensions and Thermal Properties from Spitzer Space Telescope and Ground-Based Observations* F. Marchisa,g, J.E. Enriqueza, J. P. Emeryb, M. Muellerc, M. Baeka, J. Pollockd, M. Assafine, R. Vieira Martinsf, J. Berthierg, F. Vachierg, D. P. Cruikshankh, L. Limi, D. Reichartj, K. Ivarsenj, J. Haislipj, A. LaCluyzej a. Carl Sagan Center, SETI Institute, 189 Bernardo Ave., Mountain View, CA 94043, USA. b. Earth and Planetary Sciences, University of Tennessee 306 Earth and Planetary Sciences Building Knoxville, TN 37996-1410 c. SRON, Netherlands Institute for Space Research, Low Energy Astrophysics, Postbus 800, 9700 AV Groningen, Netherlands d. Appalachian State University, Department of Physics and Astronomy, 231 CAP Building, Boone, NC 28608, USA e. Observatorio do Valongo/UFRJ, Ladeira Pedro Antonio 43, Rio de Janeiro, Brazil f. Observatório Nacional/MCT, R. General José Cristino 77, CEP 20921-400 Rio de Janeiro - RJ, Brazil. g. Institut de mécanique céleste et de calcul des éphémérides, Observatoire de Paris, Avenue Denfert-Rochereau, 75014 Paris, France h. NASA Ames Research Center, Mail Stop 245-6, Moffett Field, CA 94035-1000, USA i. NASA/Goddard Space Flight Center, Greenbelt, MD 20771, United States j. Physics and Astronomy Department, University of North Carolina, Chapel Hill, NC 27514, U.S.A * Based in part on observations collected at the European Southern Observatory, Chile Programs Numbers 70.C-0543 and ID 72.C-0753 Corresponding author: Franck Marchis Carl Sagan Center SETI Institute 189 Bernardo Ave. Mountain View CA 94043 USA [email protected] Abstract: We collected mid-IR spectra from 5.2 to 38 µm using the Spitzer Space Telescope Infrared Spectrograph of 28 asteroids representative of all established types of binary groups. -
Binary Minor Planets
ANRV273-EA34-03 ARI 17 April 2006 23:17 Binary Minor Planets Derek C. Richardson and Kevin J. Walsh Department of Astronomy, University of Maryland, College Park, Maryland 20740-2421; email: [email protected], [email protected] Annu. Rev. Earth Planet. Sci. Key Words 2006. 34:47–81 First published online as a asteroids, comets, evolution, origin, satellites Review in Advance on October 31, 2005 Abstract The Annual Review of A review of observations and theories regarding binary asteroids and binary trans- by University of Central Florida on 10/27/08. For personal use only. Earth and Planetary Science Neptunian objects [collectively, binary minor planets (BMPs)] is presented. To date, is online at earth.annualreviews.org these objects have been discovered using a combination of direct imaging, lightcurve analysis, and radar. They are found throughout the Solar System, and present a chal- doi: 10.1146/ Annu. Rev. Earth Planet. Sci. 2006.34:47-81. Downloaded from arjournals.annualreviews.org annurev.earth.32.101802.120208 lenge for theorists modeling their formation in the context of Solar System evolution. The most promising models invoke rotational disruption for the smallest, shortest- Copyright c 2006 by Annual Reviews. All rights lived objects (the asteroids nearest to Earth), consistent with the observed fast rotation reserved of these bodies; impacts for the larger, longer-lived asteroids in the main belt, con- 0084-6597/06/0530- sistent with the range of size ratios of their components and slower rotation rates; 0047$20.00 and mutual capture for the distant, icy, trans-Neptunian objects, consistent with their large component separations and near-equal sizes. -
Asteroid Regolith Weathering: a Large-Scale Observational Investigation
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 5-2019 Asteroid Regolith Weathering: A Large-Scale Observational Investigation Eric Michael MacLennan University of Tennessee, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Recommended Citation MacLennan, Eric Michael, "Asteroid Regolith Weathering: A Large-Scale Observational Investigation. " PhD diss., University of Tennessee, 2019. https://trace.tennessee.edu/utk_graddiss/5467 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Eric Michael MacLennan entitled "Asteroid Regolith Weathering: A Large-Scale Observational Investigation." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Geology. Joshua P. Emery, Major Professor We have read this dissertation and recommend its acceptance: Jeffrey E. Moersch, Harry Y. McSween Jr., Liem T. Tran Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Asteroid Regolith Weathering: A Large-Scale Observational Investigation A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Eric Michael MacLennan May 2019 © by Eric Michael MacLennan, 2019 All Rights Reserved. -
Expanding Band Parameter Analysis Methods for HED Meteorites and V-Type Asteroids
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Masters Theses Graduate School 5-2021 Expanding Band Parameter Analysis Methods for HED Meteorites and V-type Asteroids Noah Adm Haverkamp Frere University of Tennessee, Knoxville, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_gradthes Part of the Physical Processes Commons, and the The Sun and the Solar System Commons Recommended Citation Frere, Noah Adm Haverkamp, "Expanding Band Parameter Analysis Methods for HED Meteorites and V- type Asteroids. " Master's Thesis, University of Tennessee, 2021. https://trace.tennessee.edu/utk_gradthes/6217 This Thesis is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Masters Theses by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a thesis written by Noah Adm Haverkamp Frere entitled "Expanding Band Parameter Analysis Methods for HED Meteorites and V-type Asteroids." I have examined the final electronic copy of this thesis for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Master of Science, with a major in . Sean S. Lindsay, Major Professor We have read this thesis and recommend its acceptance: Andrew W. Steiner, Tony Mezzacappa Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Expanding Band Parameter Analysis Methods for HED Meteorites and V-type Asteroids A Thesis Presented for the Master of Science Degree The University of Tennessee, Knoxville Noah Adm Haverkamp Frere May 2021 Copyright © by Noah Adm Haverkamp Frere, 2021 All Rights Reserved. -
Multiple Asteroid Systems: Dimensions and Thermal Properties from Spitzer Space Telescope and Ground-Based Observations Q ⇑ F
Icarus 221 (2012) 1130–1161 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Multiple asteroid systems: Dimensions and thermal properties from Spitzer Space Telescope and ground-based observations q ⇑ F. Marchis a,g, , J.E. Enriquez a, J.P. Emery b, M. Mueller c, M. Baek a, J. Pollock d, M. Assafin e, R. Vieira Martins f, J. Berthier g, F. Vachier g, D.P. Cruikshank h, L.F. Lim i, D.E. Reichart j, K.M. Ivarsen j, J.B. Haislip j, A.P. LaCluyze j a Carl Sagan Center, SETI Institute, 189 Bernardo Ave., Mountain View, CA 94043, USA b Earth and Planetary Sciences, University of Tennessee, 306 Earth and Planetary Sciences Building, Knoxville, TN 37996-1410, USA c SRON, Netherlands Institute for Space Research, Low Energy Astrophysics, Postbus 800, 9700 AV Groningen, Netherlands d Appalachian State University, Department of Physics and Astronomy, 231 CAP Building, Boone, NC 28608, USA e Observatorio do Valongo, UFRJ, Ladeira Pedro Antonio 43, Rio de Janeiro, Brazil f Observatório Nacional, MCT, R. General José Cristino 77, CEP 20921-400 Rio de Janeiro, RJ, Brazil g Institut de mécanique céleste et de calcul des éphémérides, Observatoire de Paris, Avenue Denfert-Rochereau, 75014 Paris, France h NASA, Ames Research Center, Mail Stop 245-6, Moffett Field, CA 94035-1000, USA i NASA, Goddard Space Flight Center, Greenbelt, MD 20771, USA j Physics and Astronomy Department, University of North Carolina, Chapel Hill, NC 27514, USA article info abstract Article history: We collected mid-IR spectra from 5.2 to 38 lm using the Spitzer Space Telescope Infrared Spectrograph Available online 2 October 2012 of 28 asteroids representative of all established types of binary groups. -
(2000) Forging Asteroid-Meteorite Relationships Through Reflectance
Forging Asteroid-Meteorite Relationships through Reflectance Spectroscopy by Thomas H. Burbine Jr. B.S. Physics Rensselaer Polytechnic Institute, 1988 M.S. Geology and Planetary Science University of Pittsburgh, 1991 SUBMITTED TO THE DEPARTMENT OF EARTH, ATMOSPHERIC, AND PLANETARY SCIENCES IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN PLANETARY SCIENCES AT THE MASSACHUSETTS INSTITUTE OF TECHNOLOGY FEBRUARY 2000 © 2000 Massachusetts Institute of Technology. All rights reserved. Signature of Author: Department of Earth, Atmospheric, and Planetary Sciences December 30, 1999 Certified by: Richard P. Binzel Professor of Earth, Atmospheric, and Planetary Sciences Thesis Supervisor Accepted by: Ronald G. Prinn MASSACHUSES INSTMUTE Professor of Earth, Atmospheric, and Planetary Sciences Department Head JA N 0 1 2000 ARCHIVES LIBRARIES I 3 Forging Asteroid-Meteorite Relationships through Reflectance Spectroscopy by Thomas H. Burbine Jr. Submitted to the Department of Earth, Atmospheric, and Planetary Sciences on December 30, 1999 in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy in Planetary Sciences ABSTRACT Near-infrared spectra (-0.90 to ~1.65 microns) were obtained for 196 main-belt and near-Earth asteroids to determine plausible meteorite parent bodies. These spectra, when coupled with previously obtained visible data, allow for a better determination of asteroid mineralogies. Over half of the observed objects have estimated diameters less than 20 k-m. Many important results were obtained concerning the compositional structure of the asteroid belt. A number of small objects near asteroid 4 Vesta were found to have near-infrared spectra similar to the eucrite and howardite meteorites, which are believed to be derived from Vesta. -
The Compositional Diversity of Non-Vesta Basaltic Asteroids
The compositional diversity of non-Vesta basaltic asteroids The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Leith, Thomas B. et al. "The compositional diversity of non-Vesta basaltic asteroids." Icarus 295 (October 2017): 61-73 © 2017 Elsevier As Published http://dx.doi.org/10.1016/j.icarus.2017.05.007 Publisher Elsevier BV Version Author's final manuscript Citable link https://hdl.handle.net/1721.1/127640 Terms of Use Creative Commons Attribution-NonCommercial-NoDerivs License Detailed Terms http://creativecommons.org/licenses/by-nc-nd/4.0/ The compositional diversity of non-Vesta basaltic asteroids Thomas B. Leitha,b, Nicholas A. Moskovitza, Rhiannon G. Maynec, Francesca E. DeMeod, Driss Takire, Brian J. Burta,d, Richard P. Binzeld, Dimitra Pefkoud aLowell Observatory, Flagstaff, AZ, 86001, USA bHarvard-Smithsonian Center for Astrophysics, Cambridge, MA, 02138, USA cMonnig Meteorite Collection, Texas Christian University, Fort Worth, TX, 76129, USA dMassachusetts Institute of Technology, Cambridge, MA, 02139, USA eAstrogeology Science Center, United States Geological Survey, Flagstaff, AZ, 86001, USA Abstract We present near-infrared (0.78-2.45 µm) reflectance spectra for nine middle and outer main belt (a > 2:5 AU) basaltic asteroids. Three of these objects are spectrally distinct from all classifications in the Bus-DeMeo system and could represent spectral end members in the existing taxonomy or be representatives of a new spectral type. The remainder of the sample are classified as V- or R- type. All of these asteroids are dynamically detached from the Vesta collisional family, but are too small to be intact differentiated parent bodies, implying that they originated from differentiated planetesimals which have since been destroyed or ejected from the solar system. -
Applying Machine Learning to Asteroid Classification Utilizing Spectroscopically Derived Spectrophotometry Kathleen Jacinda Mcintyre
University of North Dakota UND Scholarly Commons Theses and Dissertations Theses, Dissertations, and Senior Projects January 2019 Applying Machine Learning To Asteroid Classification Utilizing Spectroscopically Derived Spectrophotometry Kathleen Jacinda Mcintyre Follow this and additional works at: https://commons.und.edu/theses Recommended Citation Mcintyre, Kathleen Jacinda, "Applying Machine Learning To Asteroid Classification Utilizing Spectroscopically Derived Spectrophotometry" (2019). Theses and Dissertations. 2474. https://commons.und.edu/theses/2474 This Thesis is brought to you for free and open access by the Theses, Dissertations, and Senior Projects at UND Scholarly Commons. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of UND Scholarly Commons. For more information, please contact [email protected]. APPLYING MACHINE LEARNING TO ASTEROID CLASSIFICATION UTILIZING SPECTROSCOPICALLY DERIVED SPECTROPHOTOMETRY by Kathleen Jacinda McIntyre Bachelor oF Science, University oF Florida, 2011 Bachelor oF Arts, University oF Florida, 2011 A Thesis Submitted to the Graduate Faculty of the University oF North Dakota in partial fulfillment oF the reQuirements for the degree oF Master oF Science Grand Forks, North Dakota May 2019 ii PERMISSION Title ApPlying Machine Learning to Asteroid ClassiFication Utilizing SPectroscoPically Derived SPectroPhotometry DePartment Space Studies Degree Master oF Science In Presenting this thesis in Partial fulfillment of the reQuirements for a graduate degree From the University of North Dakota, I agree that the library of this University shall make it Freely available For insPection. I Further agree that permission For extensive copying For scholarly purposes may be granted by the professor Who suPervised my thesis Work, or in his absence, by the ChairPerson of the department of the dean of the School of Graduate Studies. -
Cumulative Index to Volumes 1-45
The Minor Planet Bulletin Cumulative Index 1 Table of Contents Tedesco, E. F. “Determination of the Index to Volume 1 (1974) Absolute Magnitude and Phase Index to Volume 1 (1974) ..................... 1 Coefficient of Minor Planet 887 Alinda” Index to Volume 2 (1975) ..................... 1 Chapman, C. R. “The Impossibility of 25-27. Index to Volume 3 (1976) ..................... 1 Observing Asteroid Surfaces” 17. Index to Volume 4 (1977) ..................... 2 Tedesco, E. F. “On the Brightnesses of Index to Volume 5 (1978) ..................... 2 Dunham, D. W. (Letter regarding 1 Ceres Asteroids” 3-9. Index to Volume 6 (1979) ..................... 3 occultation) 35. Index to Volume 7 (1980) ..................... 3 Wallentine, D. and Porter, A. Index to Volume 8 (1981) ..................... 3 Hodgson, R. G. “Useful Work on Minor “Opportunities for Visual Photometry of Index to Volume 9 (1982) ..................... 4 Planets” 1-4. Selected Minor Planets, April - June Index to Volume 10 (1983) ................... 4 1975” 31-33. Index to Volume 11 (1984) ................... 4 Hodgson, R. G. “Implications of Recent Index to Volume 12 (1985) ................... 4 Diameter and Mass Determinations of Welch, D., Binzel, R., and Patterson, J. Comprehensive Index to Volumes 1-12 5 Ceres” 24-28. “The Rotation Period of 18 Melpomene” Index to Volume 13 (1986) ................... 5 20-21. Hodgson, R. G. “Minor Planet Work for Index to Volume 14 (1987) ................... 5 Smaller Observatories” 30-35. Index to Volume 15 (1988) ................... 6 Index to Volume 3 (1976) Index to Volume 16 (1989) ................... 6 Hodgson, R. G. “Observations of 887 Index to Volume 17 (1990) ................... 6 Alinda” 36-37. Chapman, C. R. “Close Approach Index to Volume 18 (1991) .................. -
Lightcurve Study of V-Type Asteroids Matt on Winski
University of North Dakota UND Scholarly Commons Theses and Dissertations Theses, Dissertations, and Senior Projects January 2017 Lightcurve Study Of V-Type Asteroids Matt oN winski Follow this and additional works at: https://commons.und.edu/theses Recommended Citation Nowinski, Matt, "Lightcurve Study Of V-Type Asteroids" (2017). Theses and Dissertations. 2301. https://commons.und.edu/theses/2301 This Thesis is brought to you for free and open access by the Theses, Dissertations, and Senior Projects at UND Scholarly Commons. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of UND Scholarly Commons. For more information, please contact [email protected]. LIGHTCURVE STUDY OF V‐TYPE ASTEROIDS by Matthew Clarke Nowinski B.S. Aerospace Engineering, Virginia Tech, 1991 M.S. Mechanical Engineering, Virginia Tech, 1993 Ph.D. Mechanical Engineering, EPFL, 1999 A Thesis Submitted to the Graduate Faculty of the University of North Dakota in partial fulfillment of the requirements for the degree of Master of Science Grand Forks, North Dakota December 2017 PERMISSION Title: Lightcurve Study Of V‐Type Asteroids Department: Space Studies Degree : Master of Science In presenting this thesis in partial fulfillment of the requirements for a graduate degree from the University of North Dakota, I agree that the library of this University shall make it freely available for inspection. I further agree that permission for extensive copying for scholarly purposes may be granted by the professor who supervised my thesis work or in his absence, by the chairperson of the department or the dean of Graduate School. It is understood that any copying or publication or other use of this thesis or part thereof for financial gain shall not be allowed without my written permission. -
Spectral Diversity and Photometric Behavior of Main-Belt and Near-Earth Vestoids and (4) Vesta: a Study in Preparation for the Dawn Encounter ⇑ Michael D
Icarus 235 (2014) 60–74 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Spectral diversity and photometric behavior of main-belt and near-Earth vestoids and (4) Vesta: A study in preparation for the Dawn encounter ⇑ Michael D. Hicks a, , Bonnie J. Buratti a, Kenneth J. Lawrence a, John Hillier b, Jian-Yang Li c, Vishnu Reddy d, Stefan Schröder d, Andreas Nathues d, Martin Hoffmann d, Lucille Le Corre d, Rene Duffard e, Hai-Bin Zhao f, Carol Raymond a, Christopher Russell g, Thomas Roatsch h, Ralf Jaumann h, Heath Rhoades a, Deronda Mayes a, Tzitlaly Barajas i, Thien-Tin Truong i, James Foster i, Amanda McAuley i a Jet Propulsion Laboratory, California Inst. of Technology, 4800 Oak Grove Drive 183-501, Pasadena, CA 91109, USA b Grays Harbor College, 1620 Edward P Smith Drive, Aberdeen, WA 98520-7599, USA c Department of Astronomy, University of Maryland, College Park, MD 20742, USA d Max Planck Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany e Instituto de Astrofisica de Andalucia, CSIC, C/Bajo de Huetor, 50, Granada 18008, Spain f Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China g Institute of Geophysics and Planetary Physics, University of California Los Angeles, Los Angeles, CA 90024-1567, USA h Institute of Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt, Berlin 80302, Germany i California State University Los Angeles, State University Drive, Los Angeles, CA 90032, USA article info abstract Article history: In anticipation of the Dawn Mission to 4 Vesta, we conducted a ground-based campaign of Bessel BVRI filter Received 20 September 2012 photometry of five V-type near-Earth asteroids over a wide range of solar phase angles. -
AURA/NOAO ANNUAL PROJECT REPORT FY 2004 Submitted to the National Science Foundation Via Fastlane November 1, 2004
AURA/NOAO ANNUAL PROJECT REPORT FY 2004 Submitted to the National Science Foundation via FastLane November 1, 2004 Three-color composite image of spiral galaxy NGC4402 taken at the WIYN 3.5-meter telescope on Kitt Peak using the WIYN Tip-Tilt module, an adaptive optics device that uses a movable mirror to provide first-order compensation for the jittery motion of the incoming image caused by variable atmospheric conditions and telescope vibrations. NGC4402 is interacting with the intergalactic medium of the Virgo Cluster. Photo Courtesy: H. Crowl (Yale University) and WIYN/NOAO/AURA/NSF NATIONAL OPTICAL ASTRONOMY OBSERVATORY TABLE OF CONTENTS EXECUTIVE SUMMARY .........................................................................................................iii 1 SCIENTIFIC ACTIVITIES AND FINDINGS....................................................................1 1.1 NOAO Gemini Science Center, 1 A Luminous Lyman-α Emitting Galaxy at Redshift z=6.535, 1 Accretion Signatures in Massive Star Formation, 1 1.2 Cerro Tololo Inter-American Observatory (CTIO), 3 The Halo of Our Galaxy: Structured, Not Smooth, 3 Science with ISPI at the Blanco, 3 1.3 Kitt Peak National Observatory (KPNO), 4 2 THE NATIONAL GROUND-BASED O/IR OBSERVING SYSTEM ..............................6 2.1 The Gemini Telescopes, 6 Support of U.S. Gemini Users and Proposers, 6 Providing U.S. Scientific Input to Gemini, 7 U.S. Gemini Instrumentation Program, 7 2.2 CTIO Telescopes, 8 Blanco 4-Meter Telescope, 8 SOAR 4-m Telescope, 9 Blanco Instrumentation, 9 SOAR Instrumentation, 10 SMARTS Consortium and Other Small Telescopes, 10 2.3 KPNO Telescopes, 11 Performance Upgrades at WIYN, 11 New Instrument and Upgrades, 12 New Major Tenant for KPNO, 12 Site Protection, 13 2.4 Enhanced Community Access to the Independent Observatories, 13 MMT Observatory and the Hobby-Eberly Telescope, 13 W.