The Comet's Tale
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Observational Constraints on Surface Characteristics of Comet Nuclei
Observational Constraints on Surface Characteristics of Comet Nuclei Humberto Campins ([email protected] u) Lunar and Planetary Laboratory, University of Arizona Yanga Fernandez University of Hawai'i Abstract. Direct observations of the nuclear surfaces of comets have b een dicult; however a growing number of studies are overcoming observational challenges and yielding new information on cometary surfaces. In this review, we fo cus on recent determi- nations of the alb edos, re ectances, and thermal inertias of comet nuclei. There is not much diversity in the geometric alb edo of the comet nuclei observed so far (a range of 0.025 to 0.06). There is a greater diversity of alb edos among the Centaurs, and the sample of prop erly observed TNOs (2) is still to o small. Based on their alb edos and Tisserand invariants, Fernandez et al. (2001) estimate that ab out 5% of the near-Earth asteroids have a cometary origin, and place an upp er limit of 10%. The agreement between this estimate and two other indep endent metho ds provide the strongest constraint to date on the fraction of ob jects that comets contribute to the p opulation of near-Earth asteroids. There is a diversity of visible colors among comets, extinct comet candidates, Centaurs and TNOs. Comet nuclei are clearly not as red as the reddest Centaurs and TNOs. What Jewitt (2002) calls ultra-red matter seems to be absent from the surfaces of comet nuclei. Rotationally resolved observations of b oth colors and alb edos are needed to disentangle the e ects of rotational variability from other intrinsic qualities. -
Ice& Stone 2020
Ice & Stone 2020 WEEK 41: OCTOBER 4-10 Presented by The Earthrise Institute # 41 Authored by Alan Hale This week in history OCTOBER 4 5 6 7 8 9 10 OCTOBER 4, 2020: The main-belt asteroid (1679) Nevanlinna will occult the 7th-magnitude star HD 224945 in Pisces. The predicted path of the occultation crosses Newfoundland, part of the Maritime Provinces of Canada, the northeastern through the south-central U.S. (including Houston, Texas), north-central Mexico (including the northern regions of Monterrey, Nuevo Leon), and the southern Pacific Ocean. OCTOBER 4 5 6 7 8 9 10 OCTOBER 7, 2008: Twenty hours after its discovery by Richard Kowalski during the course of the Mount Lemmon Survey in Arizona, the tiny asteroid 2008 TC3 enters Earth’s atmosphere above Sudan, explodes, and drops meteorite fragments – the Almahata Sitta meteorite – on the Nubian Desert. This is the first instance of an impacting asteroid being discovered in space while still inbound to an impact, and it is the subject of this week’s “Special Topics” presentation. OCTOBER 7, 2009: Astronomers using the Infrared Telescope Facility in Hawaii announce that the surface of the large main-belt asteroid (24) Themis appears to be completely covered with water ice. The significance of this discovery is discussed in a previous “Special Topics” presentation. OCTOBER 4 5 6 7 8 9 10 OCTOBER 8, 1769: Comet Messier C/1769 P1 passes through perihelion at a heliocentric distance of 0.123 AU. This was the brightest comet discovered by the 18th-Century French comet hunter Charles Messier and is a previous “Comet of the Week.” OCTOBER 4 5 6 7 8 9 10 OCTOBER 9, 1933: A brief but strong “storm” of Draconid meteors is seen over Europe. -
Photometric Study of Two Near-Earth Asteroids in the Sloan Digital Sky Survey Moving Objects Catalog
University of North Dakota UND Scholarly Commons Theses and Dissertations Theses, Dissertations, and Senior Projects January 2020 Photometric Study Of Two Near-Earth Asteroids In The Sloan Digital Sky Survey Moving Objects Catalog Christopher James Miko Follow this and additional works at: https://commons.und.edu/theses Recommended Citation Miko, Christopher James, "Photometric Study Of Two Near-Earth Asteroids In The Sloan Digital Sky Survey Moving Objects Catalog" (2020). Theses and Dissertations. 3287. https://commons.und.edu/theses/3287 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]. PHOTOMETRIC STUDY OF TWO NEAR-EARTH ASTEROIDS IN THE SLOAN DIGITAL SKY SURVEY MOVING OBJECTS CATALOG by Christopher James Miko Bachelor of Science, Valparaiso University, 2013 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 August 2020 Copyright 2020 Christopher J. Miko ii Christopher J. Miko Name: Degree: Master of Science This document, submitted in partial fulfillment of the requirements for the degree from the University of North Dakota, has been read by the Faculty Advisory Committee under whom the work has been done and is hereby approved. ____________________________________ Dr. Ronald Fevig ____________________________________ Dr. Michael Gaffey ____________________________________ Dr. Wayne Barkhouse ____________________________________ Dr. Vishnu Reddy ____________________________________ ____________________________________ This document is being submitted by the appointed advisory committee as having met all the requirements of the School of Graduate Studies at the University of North Dakota and is hereby approved. -
NASA Ames Jim Arnold, Craig Burkhardt Et Al
The re-entry of artificial meteoroid WT1190F AIAA SciTech 2016 1/5/2016 2008 TC3 Impact October 7, 2008 Mohammad Odeh International Astronomical Center, Abu Dhabi Peter Jenniskens SETI Institute Asteroid Threat Assessment Project (ATAP) - NASA Ames Jim Arnold, Craig Burkhardt et al. Michael Aftosmis - NASA Ames 2 Darrel Robertson - NASA Ames Next TC3 Consortium http://impact.seti.org Mission Statement: Steve Larson (Catalina Sky Survey) “Be prepared for the next 2008 TC3 John Tonry (ATLAS) impact” José Luis Galache (Minor Planet Center) Focus on two aspects: Steve Chesley (NASA JPL) 1. Airborne observations of the reentry Alan Fitzsimmons (Queen’s Univ. Belfast) 2. Rapid recovery of meteorites Eileen Ryan (Magdalena Ridge Obs.) Franck Marchis (SETI Institute) Ron Dantowitz (Clay Center Observatory) Jay Grinstead (NASA Ames Res. Cent.) Peter Jenniskens (SETI Institute - POC) You? 5 NASA/JPL “Sentry” early alert October 3, 2015: WT1190F Davide Farnocchia (NASA/JPL) Catalina Sky Survey: Richard Kowalski Steve Chesley (NASA/JPL) Marco Michelli (ESA NEOO CC) 6 WT1190F Found: October 3, 2015: one more passage Oct. 24 Traced back to: 2013, 2012, 2011, …, 2009 Re-entry: Friday November 13, 2015 10.61 km/s 20.6º angle Bill Gray 11 IAC + UAE Space Agency chartered commercial G450 Mohammad Odeh (IAC, Abu Dhabi) Support: UAE Space Agency Dexter Southfield /Embry-Riddle AU 14 ESA/University Stuttgart 15 SETI Institute 16 Dexter Southfield team Time UAE Camera Trans-Lunar Insertion Stage Leading candidate (1/13/2016): LUNAR PROSPECTOR T.L.I.S. Launch: January 7, 1998 UT Lunar Prospector itself was deliberately crashed on Moon July 31, 1999 Carbon fiber composite Spin hull thrusters Titanium case holds Amonium Thiokol Perchlorate fuel and Star Stage 3700S HTPB binder (both contain H) P.I.: Alan Binder Scott Hubbard 57-minutes later: Mission Director Separation of TLIS NASA Ames http://impact.seti.org 30 . -
ISTS-2017-D-074ⅠISSFD-2017-074
A look at the capture mechanisms of the “Temporarily Captured Asteroids” of the Earth By Hodei URRUTXUA1) and Claudio BOMBARDELLI2) 1)Astronautics Group, University of Southampton, United Kingdom 2)Space Dynamics Group, Technical University of Madrid, Spain (Received April 17th, 2017) Temporarily captured asteroids of the Earth are a newly discovered family of asteroids, which become naturally captured in the vicinity of the Earth for a limited time period. Thus, during the temporary capture these asteroids are in energetically favorable condi- tions, which makes them appealing targets for space missions to asteroids. Despite their potential interest, their capture mechanisms are not yet fully understood, and basic questions remain unanswered regarding the taxonomy of this population. The present work looks at gaining a better understanding of the key features that are relevant to the duration and nature of these asteroids, by analyzing patterns and extracting conclusions from a synthetic population of temporarily captured asteroids. Key Words: Asteroids, temporarily captured asteroids, capture dynamics, asteroid retrieval. Acronyms system. Asteroid 2006 RH120 is so far the only known mem- ber of this population, though statistical studies by Granvik et TCA : Temporarily captured asteroids al.12) support the evidence that such objects are actually com- TCO : Temporarily captured orbiters mon companions of the Earth, and thus it is expected that an TCF : Temporarily captured fly-bys increasing number of them will be found as survey technology improves.13) 1. Introduction During their temporary capture phase these asteroids are technically orbiting the Earth rather than the Sun, since their The origin of planetary satellites in the Solar System has Earth-binding energy is negative. -
Comet Section Observing Guide
Comet Section Observing Guide 1 The British Astronomical Association Comet Section www.britastro.org/comet BAA Comet Section Observing Guide Front cover image: C/1995 O1 (Hale-Bopp) by Geoffrey Johnstone on 1997 April 10. Back cover image: C/2011 W3 (Lovejoy) by Lester Barnes on 2011 December 23. © The British Astronomical Association 2018 2018 December (rev 4) 2 CONTENTS 1 Foreword .................................................................................................................................. 6 2 An introduction to comets ......................................................................................................... 7 2.1 Anatomy and origins ............................................................................................................................ 7 2.2 Naming .............................................................................................................................................. 12 2.3 Comet orbits ...................................................................................................................................... 13 2.4 Orbit evolution .................................................................................................................................... 15 2.5 Magnitudes ........................................................................................................................................ 18 3 Basic visual observation ........................................................................................................ -
Stargazer Vice President: James Bielaga (425) 337-4384 Jamesbielaga at Aol.Com P.O
1 - Volume MMVII. No. 1 January 2007 President: Mark Folkerts (425) 486-9733 folkerts at seanet.com The Stargazer Vice President: James Bielaga (425) 337-4384 jamesbielaga at aol.com P.O. Box 12746 Librarian: Mike Locke (425) 259-5995 mlocke at lionmts.com Everett, WA 98206 Treasurer: Carol Gore (360) 856-5135 janeway7C at aol.com Newsletter co-editor: Bill O’Neil (774) 253-0747 wonastrn at seanet.com Web assistance: Cody Gibson (425) 348-1608 sircody01 at comcast.net See EAS website at: (change ‘at’ to @ to send email) http://members.tripod.com/everett_astronomy nearby Diablo Lake. And then at night, discover the night sky like EAS BUSINESS… you've never seen it before. We hope you'll join us for a great weekend. July 13-15, North Cascades Environmental Learning Center North Cascades National Park. More information NEXT EAS MEETING – SATURDAY JANUARY 27TH including pricing, detailed program, and reservation forms available shortly, so please check back at Pacific Science AT 3:00 PM AT THE EVERETT PUBLIC LIBRARY, IN Center's website. THE AUDITORIUM (DOWNSTAIRS) http://www.pacsci.org/travel/astronomy_weekend.html People should also join and send mail to the mail list THIS MONTH'S MEETING PROGRAM: [email protected] to coordinate spur-of-the- Toby Smith, lecturer from the University of Washington moment observing get-togethers, on nights when the sky Astronomy department, will give a talk featuring a clears. We try to hold informal close-in star parties each month visualization presentation he has prepared called during the spring, summer, and fall months on a weekend near “Solar System Cinema”. -
The Comet's Tale
THE COMET’S TALE Journal of the Comet Section of the British Astronomical Association Number 33, 2014 January Not the Comet of the Century 2013 R1 (Lovejoy) imaged by Damian Peach on 2013 December 24 using 106mm F5. STL-11k. LRGB. L: 7x2mins. RGB: 1x2mins. Today’s images of bright binocular comets rival drawings of Great Comets of the nineteenth century. Rather predictably the expected comet of the century Contents failed to materialise, however several of the other comets mentioned in the last issue, together with the Comet Section contacts 2 additional surprise shown above, put on good From the Director 2 appearances. 2011 L4 (PanSTARRS), 2012 F6 From the Secretary 3 (Lemmon), 2012 S1 (ISON) and 2013 R1 (Lovejoy) all Tales from the past 5 th became brighter than 6 magnitude and 2P/Encke, 2012 RAS meeting report 6 K5 (LINEAR), 2012 L2 (LINEAR), 2012 T5 (Bressi), Comet Section meeting report 9 2012 V2 (LINEAR), 2012 X1 (LINEAR), and 2013 V3 SPA meeting - Rob McNaught 13 (Nevski) were all binocular objects. Whether 2014 will Professional tales 14 bring such riches remains to be seen, but three comets The Legacy of Comet Hunters 16 are predicted to come within binocular range and we Project Alcock update 21 can hope for some new discoveries. We should get Review of observations 23 some spectacular close-up images of 67P/Churyumov- Prospects for 2014 44 Gerasimenko from the Rosetta spacecraft. BAA COMET SECTION NEWSLETTER 2 THE COMET’S TALE Comet Section contacts Director: Jonathan Shanklin, 11 City Road, CAMBRIDGE. CB1 1DP England. Phone: (+44) (0)1223 571250 (H) or (+44) (0)1223 221482 (W) Fax: (+44) (0)1223 221279 (W) E-Mail: [email protected] or [email protected] WWW page : http://www.ast.cam.ac.uk/~jds/ Assistant Director (Observations): Guy Hurst, 16 Westminster Close, Kempshott Rise, BASINGSTOKE, Hampshire. -
THE GREAT CHRIST COMET CHRIST GREAT the an Absolutely Astonishing Triumph.” COLIN R
“I am simply in awe of this book. THE GREAT CHRIST COMET An absolutely astonishing triumph.” COLIN R. NICHOLL ERIC METAXAS, New York Times best-selling author, Bonhoeffer The Star of Bethlehem is one of the greatest mysteries in astronomy and in the Bible. What was it? How did it prompt the Magi to set out on a long journey to Judea? How did it lead them to Jesus? THE In this groundbreaking book, Colin R. Nicholl makes the compelling case that the Star of Bethlehem could only have been a great comet. Taking a fresh look at the biblical text and drawing on the latest astronomical research, this beautifully illustrated volume will introduce readers to the Bethlehem Star in all of its glory. GREAT “A stunning book. It is now the definitive “In every respect this volume is a remarkable treatment of the subject.” achievement. I regard it as the most important J. P. MORELAND, Distinguished Professor book ever published on the Star of Bethlehem.” of Philosophy, Biola University GARY W. KRONK, author, Cometography; consultant, American Meteor Society “Erudite, engrossing, and compelling.” DUNCAN STEEL, comet expert, Armagh “Nicholl brilliantly tackles a subject that has CHRIST Observatory; author, Marking Time been debated for centuries. You will not be able to put this book down!” “An amazing study. The depth and breadth LOUIE GIGLIO, Pastor, Passion City Church, of learning that Nicholl displays is prodigious Atlanta, Georgia and persuasive.” GORDON WENHAM, Adjunct Professor “The most comprehensive interdisciplinary of Old Testament, Trinity College, Bristol synthesis of biblical and astronomical data COMET yet produced. -
Three Decades of Small-Telescope Science
Three Decades of Small-Telescope Science A Report on the 2011 Society for Astronomical Sciences 30th Annual Sym- posium on Telescope Science Robert K. Buchheim For three decades, the Society for Astronomical Sciences has supported small telescope sci- ence, encouraged amateur research, and facilitated pro-am collaboration. On May 24-26, more than one hundred participants in the 30th anniversary SAS Symposium heard presentations cov- ering a wide range of astronomical topics, reaching from the laboratory to the distant cosmos. From Planets to Galaxies Sky & Telescope Editor-in-Chief Bob Naeye opened the technical session with a review of the amateur contributions to exoplanet discovery and research through monitoring of transits and micro-lensing events. R. Jay GaBany described his participation as an astro-imager in the search for evidence of galactic mergers. His exquisite deep images taken with his 24-inch telescope displayed the di- verse patterns of star streams that can be left behind when a dwarf galaxy is disrupted and ab- sorbed by a larger galaxy. He also noted that not all faint structures are evidence of galactic mergers: the faint ”loop” structure near M-81 is actually foreground “galactic cirrus” in our own Milky Way masquerading as a faux tidal loop. Education and Outreach Several papers related to education and outreach were presented. Debra Ceravolo applied her expertise in the generation and perception of colors, to describe a new method of merging narrow-band (e.g. Hα) and broad-band (e.g. RGB) images into a natural-color image that displays enhanced detail without glaring false colors. -
Oort Cloud and Scattered Disc Formation During a Late Dynamical Instability in the Solar System ⇑ R
Icarus 225 (2013) 40–49 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Oort cloud and Scattered Disc formation during a late dynamical instability in the Solar System ⇑ R. Brasser a, , A. Morbidelli b a Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 106, Taiwan b Departement Lagrange, University of Nice – Sophia Antipolis, CNRS, Observatoire de la Côte d’Azur, Nice, France article info abstract Article history: One of the outstanding problems of the dynamical evolution of the outer Solar System concerns the Received 11 January 2012 observed population ratio between the Oort cloud (OC) and the Scattered Disc (SD): observations suggest Revised 21 January 2013 that this ratio lies between 100 and 1000 but simulations that produce these two reservoirs simulta- Accepted 11 March 2013 neously consistently yield a value of the order of 10. Here we stress that the populations in the OC Available online 2 April 2013 and SD are inferred from the observed fluxes of new long period comets (LPCs) and Jupiter-family comets (JFCs), brighter than some reference total magnitude. However, the population ratio estimated in the sim- Keywords: ulations of formation of the SD and OC refers to objects bigger than a given size. There are multiple indi- Origin, Solar System cations that LPCs are intrinsically brighter than JFCs, i.e. an LPC is smaller than a JFC with the same total Comets, Dynamics Planetary dynamics absolute magnitude. When taking this into account we revise the SD/JFC population ratio from our sim- ulations relative to Duncan and Levison (1997), and then deduce from the observations that the size-lim- þ54 ited population ratio between the OC and the SD is 44À34. -
Abstract Volume
T I I II I II I I I rl I Abstract Volume LPI LPI Contribution No. 1097 II I II III I • • WORKSHOP ON MERCURY: SPACE ENVIRONMENT, SURFACE, AND INTERIOR The Field Museum Chicago, Illinois October 4-5, 2001 Conveners Mark Robinbson, Northwestern University G. Jeffrey Taylor, University of Hawai'i Sponsored by Lunar and Planetary Institute The Field Museum National Aeronautics and Space Administration Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Contribution No. 1097 Compiled in 2001 by LUNAR AND PLANETARY INSTITUTE The Institute is operated by the Universities Space Research Association under Contract No. NASW-4574 with the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication .... This volume may be cited as Author A. B. (2001)Title of abstract. In Workshop on Mercury: Space Environment, Surface, and Interior, p. xx. LPI Contribution No. 1097, Lunar and Planetary Institute, Houston. This report is distributed by ORDER DEPARTMENT Lunar and Planetary institute 3600 Bay Area Boulevard Houston TX 77058-1113, USA Phone: 281-486-2172 Fax: 281-486-2186 E-mail: order@lpi:usra.edu Please contact the Order Department for ordering information, i,-J_,.,,,-_r ,_,,,,.r pA<.><--.,// ,: Mercury Workshop 2001 iii / jaO/ Preface This volume contains abstracts that have been accepted for presentation at the Workshop on Mercury: Space Environment, Surface, and Interior, October 4-5, 2001.