A Pencil-Beam Search for Distant TNOs at the ESO NTT 117 Hermann Boehnhardt, Olivier Hainaut, Catherine Delahodde, Richard West, Karen Meech, Brian
|
|
- Abigail Norris
- 5 years ago
- Views:
Transcription
1 Contents The Kuiper Belt: Overview 1 David Jewitt 1 Introduction 1 2 Things We Know About the Kuiper Belt 1 3 Things We Think We Know 4 4 Things We Would Like to Know 6 5 Acknowledgement 8 Physical Characteristics of Trans-Neptunian Objects and Centaurs 9 John K. Davies 1 Introduction 9 2 Sizes 10 3 Rotation Periods and Lightcurve Amplitudes 11 4 Colours 12 5 Spectroscopy 17 6 Discussion 19 7 Acknowledgements 20 References 21 Detection of Thermal Emission from 1993 SC - First Results. 25 Nicolas Thomas, Sonke Eggers, Wing-Huen Ip, Giinter Lichtenberg, Alan Fitzsimmons, Horst Uwe Keller, Jwan Williams, Gerhard Hahn, Heike Rauer 1 Introduction 25 2 ISOPHOT Observations 26 3 Reduction 26 4 Modelling 28 5 Results 28 6 Summary and Discussion 30 References 30 Physical Characteristics of Distant Comets 33 Dina Prialnik 1 Introduction 33 2 Modelling the Structure and Evolution of Comets 34 3 Radiogenic Heating of Comets 37 4 Early Evolution of Comets Due to Radiogenic Heating 40 5 Conclusion: Characteristics of Distant (New) Comets 46 References 47
2 VIII Optical Observations of Trans-Neptunian and Centaur Objects 51 M. Antonietta Barucci, Monica Lazzarin 1 Introduction 51 2 Observations 52 3 Results 52 4 Conclusions 54 References 55 Photometry Techniques Report of Splinter Meeting 57 Simon Green, Neil McBride 1 Introduction 57 2 Data Reduction Strategy 58 3 Photometric Calibration 59 4 Where to Next? 59 5 Note added in proof: What happened next? 60 Physical Observations of 1996 TO 6 e 61 Catherine E. Delahodde, Olivier R. Hainaut, Hermann Bohnhardt, Elisabetta Dotto, M. Antonietta Barucci, Richard M. West, Karen J. Meech 1 Introduction and Observations 61 2 Results 62 3 Discussion 62 References 63 TNO Color Survey with the VLT: Pilot Observations with the Science Verification Camera 65 Olivier R. Hainaut, Hermann Bohnhardt, Richard M. West, Catherine E. Delahodde, Karen J. Meech 1 Introduction and Observations 65 2 Results 67 3 Conclusion and Projects 68 References 68 Colours of Distant Solar System Bodies 71 Claes-Ingvar Lagerkvist, Mats Dahlgren, Andreas Ekholm, Johan Lagerros, Magnus Lundstrom, Per Magnusson, Johan Warell 1 Introduction 71 2 Observations and Data Reductions 71 3 Results 72 4 Acknowledgement 73 References 73
3 ' IX Comet Size Distributions and Distant Activity 75 Karen J. Meech, Olivier R. Hainaut, Brian G. Marsden 1 Introduction 75 2 Observing-Program 76 3 Size Determination Issues 76 4 Discussion and Results 78 References 79 Ion Irradiation of Minor Bodies in the Outer Solar System 81 Giovanni Strazzulla 1 Introduction 81 2 An Organic Crust? 81 3 Effects on Specific Species 83 References 85 Surveys of the Distant Solar System 87 Alan Fitzsimmons 1 Introduction 87 2 Pre-1992 Surveys QBi and Beyond 89 4 Magnitude Distribution 92 5 Mass Constraints 93 6 Orbital Distribution of TNOs 94 7 Conclusions 96 References 97 Dust Measurements in the Outer Solar System 99 Eberhard Gru'n, Harald Kru'ger, Markus Landgraf 1 Introduction 99 2 Spacecraft Observations Interstellar Dust Characteristics Dust Dynamics in the Edgeworth-Kuiper Belt Future Measurements 107 References 107 Simulations of Bias Effects in Kuiper Belt Surveys 109 Chadwick Trujillo 1 Introduction Maximum Likelihood Method The Primordial Kuiper Belt Scattered Kuiper Belt Objects Ill 5 Truncated Kuiper Belt Summary 114 References 115
4 X A Pencil-Beam Search for Distant TNOs at the ESO NTT 117 Hermann Boehnhardt, Olivier Hainaut, Catherine Delahodde, Richard West, Karen Meech, Brian Marsden 1 A Search-Included TNO Programme The Observation Strategy The Data Reduction The Results with a Short Discussion Our Plans for Doing Better 122 References 123 Does Pluto Affect the Trans-Neptunian Region? 125 Brett Gladman, Jean-Marc Petit, Martin Duncan 1 Introduction The Back-of-the-Envelope Calculation Numerical Calculation 126 References 127 Kiso EKBO &c Centaur Survey and the Design and Implementation of the Moving Object Detection Engine. 129 Daisuke Kinoshita, Naotaka Yamamoto, Tomohiko 'Sekiguchi, Shinsuke Abe, Junichi Watanabe 1 Introduction Kiso EKBO & Centaur Survey Automated Detection Software 130 References 130 Limitations of Numerical Modelling of Kuiper Belt Object Dynamics 131 Ryszard Gabryszewski \ 1 Introduction Calculations Results Conclusions 133 References 133 Future Investigations with New Facilities 135 Hermann Boehnhardt 1 MBOSS 2000 and Beyond: The Main Questions Wavelength Regions for Remote Detection: Visible, Near-IR and Sub-mm Windows The Classical Approach: Observations in the Visible and Near-IR from Earth MBOSS Observations with Special Means Far Infrared and Sub-mm Observations Space Mission: Pluto Express ALMA, NGST and OWL: An Outlook 148
5 References 149 A SUBARU Survey Project with Suprime-Cam 151 Jun-ichi Watanabe 1 Introduction Why the SUBARU Telescope? Expected Discovery Rate of the Edgeworth-Kuiper Belt Objects References 153 The PICOCAM Project at Pic du Midi 155 Francois Colas, Jean Eudes Arlot, Jerome Berthier, Agnes Fienga, Michael Gastineau, Daniel Hestroffer, Laurent Jorda, Jean Lecacheux 1 Description of PICOCAM Centaurs and KBO Research Comet Survey Conclusions 157 References 158 The Power of Pencil-Beam Searches for Trans-Neptunian Science 159 Brett Gladman 1 Introduction Going Deep Future Prospects 161 References 163 Astrometry of Outer Solar System Bodies - Experience with a Small Telescope and Future Plans 165 Jana Tichd, Milos Tichy, Zdenek Moravec 1 Follow-Up Astrometry at Klet' Recovery of Centaur 1997 CU Astrometry of 1996 TL The New Project KLENOT Acknowledgements 166 References 167 TNO Follow-Up Observations at the Saji Observatory 169 Atsushi Miyamoto, Hiroki Kosai, Takaaki Oribe 1 Saji Observatory and Its Instruments TNO Observations 169 Detection of the Small EKB Objects by Occupation with Corot 171 Frangoise Roques 1 Introduction Stellar Occultations to Explore the Solar System 171 XI
6 XII 3 The Kuiper Belt Exploration by Occultation Corot Conclusions 175 References, 175 Possible Mechanism of Cometary Outbursts 177 Subhon Ibadov References 177 The Uppsala-DLR Trojan Survey of the Preceding Lagrangian Cloud 179 Claes-Ingvar Lagerkvist, Stefano Mottola, Uri Carsenty, Gerhard Hahn, Andreas Doppler, Arno Gna'dig 1 Introduction Observations Astrometry Orbit Determination and Linkage Results Acknowledgements 184 References The Distant Satellites of Uranus and the Other Giant Planets 187 Brian G. Marsden, Gareth V. Williams, KaareAksnes 1 Introduction Initial Orbit Computations Multiple-Opposition Orbit Computations Discussion 190 References 191
Small Bodies of the Outer Solar System
Mem. S.A.It. Suppl. Vol. 5, 37 c SAIt 2004 Memorie della Supplementi Small Bodies of the Outer Solar System E. Dotto 1 and M.A. Barucci 2 1 INAF-Osservatorio Astronomico di Roma, Via Frascati 33, 00040
More informationMony a Mickle Maks a Muckle:
Noname manuscript No. (will be inserted by the editor) Mony a Mickle Maks a Muckle: Minor Body Observations with Optical Telescopes of All Sizes Colin Snodgrass Received: date / Accepted: date Abstract
More informationUniversity of Hawai'i at Mänoa
Ms. Mildred Garner Grants Officer NASA Goddard Space Flight Center Code 216 Greenbelt,MD 20771 University of Hawai'i at Mänoa SUBJECT: Progress Report, Grant NAG 5-4669 Dear Ms. Garner, Institute for Astronomy
More informationSUPPLEMENTARY INFORMATION
Supplemental Discussion Infrared spectroscopy We obtained near infrared reflectance spectra of 26 bright KBOs with NIRC, the nearinfrared imaging spectrograph on the W.M. Keck Telescope using standard
More informationTNO Modelling Aspects and First Radiometric Results from the TNOs are Cool! Project
TNO Modelling Aspects and First Radiometric Results from the TNOs are Cool! Project Michael Mommert German Aerospace Center (DLR) Institute of Planetary Research, Berlin Thermal/Thermophysical Modelling
More informationSBAG GOALS Origin of the Solar System Theme
SBAG GOALS Origin of the Solar System Theme Objective 1.2. Study small bodies to understand the origin of the Solar System Objective 1.1.2 Find and characterize new samples from small bodies Presented
More informationTransneptunian Binaries and Collision Families: Probes of our Local Dust Disk
Transneptunian Binaries and Collision Families: Probes of our Local Dust Disk Susan D. Benecchi, STScI Collaborators: Keith Noll, Will Grundy, Denise Stephens, Hal Levison, and the Deep Ecliptic Survey
More informationCONTENTS. vii. in this web service Cambridge University Press. Preface Acknowledgements. xiii xvi
CONTENTS Preface Acknowledgements xiii xvi 1 Earth and sky 1 1.1 Planet Earth 1 1.2 The Earth s magnetosphere 6 1.3 Aurorae 8 1.4 Visually observing aurorae 10 1.5 Other methods of observing aurorae 16
More informationA Survey of the Trans-Neptunian Region
Next Generation Space Telescope Ad-Hoc Science Working Group Design Reference Mission Proposal Program contacts: Philip D. Nicholson, Brett J. Gladman Scientific category: SOLAR SYSTEM Instruments: OPT/CAM,
More informationWater Ice on the Satellite of Kuiper Belt Object 2003 EL61
Water Ice on the Satellite of Kuiper Belt Object 2003 EL61 K.M Barkume, M.E. Brown, and E.L. Schaller Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125
More informationASTEROIDS, COMETS, AND TRANS-NEPTUNIAN OBJECTS:
ASTEROIDS, COMETS, AND TRANS-NEPTUNIAN OBJECTS: SMALL BODIES IN THE SOLAR SYSTEM Rosemary E. Pike ASIAA TIARA Summer School 2018 On the Origins of the Solar System SMALL BODIES IN THE SOLAR SYSTEM Formation
More informationReceived 2002 July 22; accepted 2002 November 20
The Astronomical Journal, 125:1554 1558, 2003 March # 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. ESO LARGE PROGRAMME ON PHYSICAL STUDIES OF TRANS-NEPTUNIAN OBJECTS
More informationTransneptunian objects. Minor bodies in the outer Solar System. Transneptunian objects
Transneptunian objects Minor bodies in the outer Solar System Planets and Astrobiology (2016-2017) G. Vladilo Around 1980 it was proposed that the hypothetical disk of small bodies beyond Neptune (called
More informationFuture Ground-Based Solar System Research: a Prospective Workshop Summary
Earth Moon Planet (2009) 105:391 396 DOI 10.1007/s11038-009-9318-7 Future Ground-Based Solar System Research: a Prospective Workshop Summary H. Boehnhardt Æ H. U. Käufl Received: 31 January 2009 / Accepted:
More informationReport to Planetary Science Decadal Survey Primitive Bodies Panel. Perspectives from the Previous PBP Experience,
Report to Planetary Science Decadal Survey Primitive Bodies Panel Perspectives from the Previous PBP Experience, 2001-2002 Primitive Bodies Panel Meeting, Sept. 9, 2009, Washington, DC Dale Cruikshank
More informationPluto Data: Numbers. 14b. Pluto, Kuiper Belt & Oort Cloud. Pluto Data (Table 14-5)
14b. Pluto, Kuiper Belt & Oort Cloud Pluto Pluto s moons The Kuiper Belt Resonant Kuiper Belt objects Classical Kuiper Belt objects Pluto Data: Numbers Diameter: 2,290.km 0.18. Earth Mass: 1.0. 10 22 kg
More informationTNOs are Cool: A Survey of the Transneptunian Region. (39 members, 19 institutes, 9 countries)
TNOs are Cool: A Survey of the Transneptunian Region MPE Garching The TNOs-are-Cool Team (39 members, 19 institutes, 9 countries) Overview OT KP with 370 hours ( 15% executed) PACS and SPIRE photometric
More informationPluto. Sentinel of the Outer Solar System
Pluto Sentinel of the Outer Solar System Orbiting at the edge of the outer Solar System, Pluto is an intriguing object in astronomy. Since the fascinating events surrounding its discovery, it has helped
More informationOrbital Structure and Dynamical Evolution of. TNOs. Patryk Sofia Lykawka ( )
Orbital Structure and Dynamical Evolution of TNOs Patryk Sofia Lykawka ( ) patryksan@gmail.com Outline I: Introduction and motivation II: III: IV: Dynamical stability and planet migration Stable TNO populations
More informationThe Large Synoptic Survey Telescope
The Large Synoptic Survey Telescope Philip A. Pinto Steward Observatory University of Arizona for the LSST Collaboration 17 May, 2006 NRAO, Socorro Large Synoptic Survey Telescope The need for a facility
More informationThe Planet Pluto. & Kuiper Belt. The Search for PLANET X Pluto Discovered. Note how Pluto Moved in 6 days. Pluto (Hades): King of the Underworld
X The Planet Pluto & Kuiper Belt Updated May 9, 2016 The Search for PLANET X Recall Neptune was predicted from observed changes in orbit of Uranus Lowell & Pickering suggest small changes in Neptune s
More informationTHE KUIPER BELT: OVERVIEW
THE KUIPER BELT: OVERVIEW David Jewitt Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA e-mail jewitt@ifa.hawaii.edu web www.ifa.hawaii.edu/faculty/jewitt Paper on the web at www.ifa.hawaii.edu/faculty/jewitt/papers/eso
More informationAsteroid/Comet/Meteor Reading Homework Instructions: Read pages and answer the following questions.
Name Date Block: Due Date: Asteroid/Comet/Meteor Reading Homework Instructions: Read pages 333-358 and answer the following questions. Page 333 1. What are 4 examples of minor bodies in our solar system?
More informationPROBING THE SURFACE COMPOSITION OF TRANSNEPTUNIAN OBJECTS WITH JWST/NIRSPEC. P. Ferruit & A. Guilbert Lepoutre
PROBING THE SURFACE COMPOSITION OF TRANSNEPTUNIAN OBJECTS WITH JWST/NIRSPEC P. Ferruit & A. Guilbert Lepoutre Trans-Neptunian Objects (TNOs) ~1600 known TNOs and Centaurs (between Jupiter & Neptune). Sub-populations
More informationAstronomy & Astrophysics manuscript no. (will be inserted by hand later) BVRI Photometry of 27 Kuiper Belt Objects with ESO/Very Large Telescope? A.C.
Astronomy & Astrophysics manuscript no. (will be inserted by hand later) BVRI Photometry of 27 Kuiper Belt Objects with ESO/Very Large Telescope? A.C. Delsanti, 1;2 H. Boehnhardt, 1 L. Barrera, 3 K.J.
More informationAST 105. Overview of the Solar System
AST 105 Overview of the Solar System Scale of the Solar System Earth Voyager 1, 1991, distance = 4 billion miles Recap: The Solar System in Scale If the Solar System were the size of a football
More informationSolar Systems Near and Far - ALMA View
Solar Systems Near and Far - ALMA View Bryan Butler National Radio Astronomy Observatory Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very
More informationPLATO. revealing the interior of planets and stars completing the age of planet discovery for Earth-sized planets constraining planet formation
PLATO PLAnetary Transits and Oscillations of Stars revealing the interior of planets and stars completing the age of planet discovery for Earth-sized planets constraining planet formation The PLATO Consortium:
More informationToday. Next time. Emission & Absorption lines measuring elemental abundances. Doppler Effect. Telescopes technology to measure with
Today Emission & Absorption lines measuring elemental abundances Doppler Effect measuring motion Telescopes technology to measure with Solar System Overview what s out there? Next time Homework 3 Due Chemical
More informationPluto, the Kuiper Belt, and Trans- Neptunian Objects
Pluto, the Kuiper Belt, and Trans- Neptunian Objects 1 What about Pluto? Pluto used to be considered a planet Pluto is one of a large number of Trans-Neptunian Objects, not even the largest one! Discovery
More informationLaboratory Simulations of Space Weathering Effects Giovanni Strazzulla INAF Osservatorio Astrofisico di Catania, Italy
Laboratory Simulations of Space Weathering Effects Giovanni Strazzulla INAF Osservatorio Astrofisico di Catania, Italy gianni@oact.inaf.it http://web.ct.astro.it/weblab/ 1 NNNNNNNN kev-mev ions ELECTRONS
More informationLecture Outlines. Chapter 14. Astronomy Today 7th Edition Chaisson/McMillan Pearson Education, Inc.
Lecture Outlines Chapter 14 Astronomy Today 7th Edition Chaisson/McMillan Chapter 14 Solar System Debris Units of Chapter 14 14.1 Asteroids What Killed the Dinosaurs? 14.2 Comets 14.3 Beyond Neptune 14.4
More informationSmall Bodies in the Outer Solar System
Frank N. Bash Symposium 2005: New Horizons in Astronomy ASP Conference Series, Vol. 352, 2006 S. J. Kannappan, S. Redfield, J. E. Kessler-Silacci, M. Landriau, and N. Drory Small Bodies in the Outer Solar
More informationObservational Cosmology Journal Club May 14, 2018; Ryohei Nakatani
Observational Cosmology Journal Club May 14, 2018; Ryohei Nakatani 1. Haze heats Pluto s atmosphere yet explains its cold temperature Xi Zhang, Darrell F. Strobel & Hiroshi Imanaka; Nature, 551, 352, (2017)
More informationHST Observations of Planetary Atmospheres
HST Observations of Planetary Atmospheres John T. Clarke Boston University Hubble Science Legacy 3 April 2002 Venus - Near-UV images reveal cloud motions and winds - UV spectra track SO 2 composition,
More informationThe Kuiper Belt Electronic Newsletter CONTENTS
Issue No. 56 January 2008 DISTAN T EKOs The Kuiper Belt Electronic Newsletter Edited by: Joel Wm. Parker ekonews@boulder.swri.edu www.boulder.swri.edu/ekonews CONTENTS News & Announcements... 1 Abstracts
More informationSynergies between and E-ELT
Synergies between and E-ELT Aprajita Verma & Isobel Hook 1) E- ELT Summary 2) E- ELT Project Status 3) Parameter space 4) Examples of scientific synergies The World s Biggest Eye on the Sky 39.3m diameter,
More informationASTRONOMY AND ASTROPHYSICS. Physical properties of TNO 1996 TO 66. Lightcurves and possible cometary activity
Astron. Astrophys. 356, 1076 1088 (2000) Physical properties of TNO 1996 TO 66 Lightcurves and possible cometary activity ASTRONOMY AND ASTROPHYSICS O.R. Hainaut 1, C.E. Delahodde 1, H. Boehnhardt 1, E.
More informationarxiv:astro-ph/ v1 20 Dec 1999
POPULATION OF THE SCATTERED KUIPER BELT 1 Chadwick A. Trujillo Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822 arxiv:astro-ph/9912428v1 20 Dec 1999 chad@ifa.hawaii.edu David C. Jewitt
More informationASTRONOMY FINAL EXAM REVIEW
ASTRONOMY 2013-2014 NAME: DATE: ASTRONOMY FINAL EXAM REVIEW PERIOD: Energy in the Universe: Light and Matter (Chapter 5) 1. What are the wavelengths of the electromagnetic spectrum? Order them from longest
More informationHerschel and Planck: ESA s New Astronomy Missions an introduction. Martin Kessler Schloss Braunshardt 19/03/2009
Herschel and Planck: ESA s New Astronomy Missions an introduction Martin Kessler Schloss Braunshardt 19/03/2009 Missions in Operations Rosetta Hubble Integral Newton Mars Express SOHO Ulysses Cluster Venus
More informationarxiv:astro-ph/ v1 29 May 2004
Photometry of Irregular Satellites of Uranus and Neptune Tommy Grav 1 Harvard-Smithsonian Center for Astrophysics, MS51, 60 Garden Street, Cambridge MA 02138 arxiv:astro-ph/0405605v1 29 May 2004 tgrav@cfa.harvard.edu
More information(1,2), E. (1), T. (3), P. (1,4), P. (5), C. (6), T. (7), M. (8), E. (3), D. (1), J.
TNOs are Cool: A survey of the trans-neptunian region. Results from the combined Herschel PACS and SPIRE observations of 9 bright targets at 70-500 μm. S. Fornasier (1,2), E. Lellouch (1), T. Müller (3),
More informationPlanetary Perturbations on the 2 : 3 Mean Motion Resonance with Neptune
PASJ: Publ. Astron. Soc. Japan 54, 493 499, 2002 June 25 c 2002. Astronomical Society of Japan. Planetary Perturbations on the 2 : 3 Mean Motion Resonance with Neptune Tetsuharu FUSE Subaru Telescope,
More informationVisible spectroscopic and photometric survey of Jupiter Trojans: final results on dynamical families.
arxiv:0704.0350v1 [astro-ph] 3 Apr 2007 Visible spectroscopic and photometric survey of Jupiter Trojans: final results on dynamical families. Fornasier S. 1,2, Dotto E. 3, Hainaut O. 4, Marzari F. 5, Boehnhardt
More informationWhy is this important to scientists, and why is it important to you as a teacher or parent of a child who wants to know how many planets there are?
11 October 2006 On Wednesday, August 16, 2006, the International Astronomical Union (IAU) announced a proposed definition of a planet. A significantly revised version of this definition was passed by the
More informationComets and KBO's. Comets. Halley's Comet. Far outside the orbit of Neptune are an overwhelming number of small icy bodies
Comets and KBO's Far outside the orbit of Neptune are an overwhelming number of small icy bodies The Kuiper belt is a ring of icy material located in the plane of the Solar System Comets were known and
More informationVisible and infrared photometry of Kuiper Belt objects: searching for evidence of trends
Available online at www.sciencedirect.com R Icarus 161 (2003) 501 510 www.elsevier.com/locate/icarus Visible and infrared photometry of Kuiper Belt objects: searching for evidence of trends Neil McBride,
More informationSmallest Kuiper Belt Object Ever Detected
National Aeronautics and Space Administration Smallest Kuiper Belt Object Ever Detected Taken from: Hubble 2009: Science Year in Review Produced by NASA Goddard Space Flight Center and the Space Telescope
More informationForming the Kuiper Belt by the Outward Transport of Objects During Neptune s Migration
Forming the Kuiper Belt by the Outward Transport of Objects During Neptune s Migration Harold F. Levison and Alessandro Morbidelli Southwest Research Institute, Boulder, CO 80302, USA Observatoire de la
More informationEarth-Based Support for the New Horizons Kuiper Extended Mission. Richard Binzel Alan Stern John Spencer 2016 DPS Meeting, Pasadena October18 th 2016
Earth-Based Support for the New Horizons Kuiper Extended Mission Richard Binzel Alan Stern John Spencer 2016 DPS Meeting, Pasadena October18 th 2016 Agenda Introduction to New Horizons Kuiper Belt Extended
More informationUsing Spitzer to Observe the Solar System
Using Spitzer to Observe the Solar System Sean Carey Spitzer Science Center 47 th DPS meeting 09 November 2015 SJC - 1 Spitzer Space Telescope NASA s Infrared Great Observatory Launched on 25 August 2003
More informationThe Collisional Evolution of Small Bodies in the Solar System
The Collisional Evolution of Small Bodies in the Solar System David P. O'Brien* Planetary Science Institute Tucson, AZ Invited Review CD '07 Alicante, Spain * with Don Davis, Scott Kenyon and Benjamin
More information> Nuno Peixinho. > Alain Doressoundiram >>> CORRELATIONS BETWEEN COLORS AND ORBITAL PARAMETERS
>>> CORRELATIONS BETWEEN COLORS AND ORBITAL PARAMETERS > Nuno Peixinho > Alain Doressoundiram Grupo de Astrofísica U. C. Observatório Astronómico U. C. Universidade de Coimbra Multicolor Photometry of
More informationMoon Obs #1 Due! Moon visible: early morning through afternoon. 6 more due June 13 th. 15 total due June 25 th. Final Report Due June 28th
Moon Obs #1 Due! Moon visible: early morning through afternoon 6 more due June 13 th 15 total due June 25 th Final Report Due June 28th Our Solar System Objectives Overview of what is in our solar system
More informationSurvey of the Solar System. The Sun Giant Planets Terrestrial Planets Minor Planets Satellite/Ring Systems
Survey of the Solar System The Sun Giant Planets Terrestrial Planets Minor Planets Satellite/Ring Systems Definition of a dwarf planet 1. Orbits the sun 2. Is large enough to have become round due to the
More informationSmall Body Science Issues. Joe Nuth, lead SBAG
Small Body Science Issues Joe Nuth, lead SBAG joseph.a.nuth@nasa.gov Organization of Outline We have a broad range of objects that fall under our purview. However, to some extent, (more for some objects,
More informationTrans-Neptunian Objects
Fakulteta za Matematiko in Fiziko Univerza v Ljubljani Trans-Neptunian Objects Mirko Kokole Mentor: Prof. Dr. Tomaž Zwitter May 1, 2005 Abstract In the last decade our view of the Solar system changed
More informationUniverse Now. 5. Minor planets and other small bodies in the Solar System
Universe Now 5. Minor planets and other small bodies in the Solar System An overview of the known Solar System The Sun 4 terrestrial planets: Mercury, Venus, Earth, Mars 4 Jovian planets: Jupiter, Saturn,
More informationThe Shape Distribution of Kuiper Belt Objects
The Shape Distribution of Kuiper Belt Objects Jane Luu MIT Lincoln Laboratory Pedro Lacerda Leiden Observatory, University of Leiden June 23, 2003 Abstract. If we assume that the periodic brightness variations
More informationCometary Science. Jessica Sunshine. Department of Astronomy University of Maryland
Cometary Science Jessica Sunshine Department of Astronomy University of Maryland Slide 1 Major Cometary Goals: Last Decadal Survey Building Blocks of the Solar System Where in the solar system are the
More informationColors of Minor Bodies in the Outer Solar System,
A&A 389, 641 664 (2002) DOI: 10.1051/0004-6361:20020431 c ESO 2002 Astronomy & Astrophysics Colors of Minor Bodies in the Outer Solar System, A statistical analysis O. R. Hainaut 1 and A. C. Delsanti 1,2
More information7. Our Solar System. Planetary Orbits to Scale. The Eight Planetary Orbits
7. Our Solar System Terrestrial & Jovian planets Seven large satellites [moons] Chemical composition of the planets Asteroids & comets The Terrestrial & Jovian Planets Four small terrestrial planets Like
More informationSimultaneous visible-near IR photometric study of Kuiper Belt Object surfaces with the ESO/Very Large Telescopes
A&A 417, 1145 1158 (2004) DOI: 10.1051/0004-6361:20034182 c ESO 2004 Astronomy & Astrophysics Simultaneous visible-near IR photometric study of Kuiper Belt Object surfaces with the ESO/Very Large Telescopes
More informationSpitzer Space Telescope Calibration Strategy: The Use of Asteroids
Spitzer Space Telescope Calibration Strategy: The Use of Asteroids 1, J. Stansberry 2, C. Engelbracht 2, M. Blaylock 2, A. Noriega-Crespo 1 2004 December 3 Herschel Calibration Workshop, Leiden, The Netherlands
More informationThe Main Point. Planetary Ring Systems
Lecture #31: Satellites and Rings II Ring Systems Overview of rings: Jupiter, Saturn, Uranus, Neptune. What are rings made of? How do they form? Reading: Chapter 11.3. The Main Point All of the giant planets
More informationConsiderations on the magnitude distributions of the Kuiper belt and of the Jupiter Trojans
Considerations on the magnitude distributions of the Kuiper belt and of the Jupiter Trojans Morbidelli Alessandro, Harold Levison, William Bottke, Luke Dones, David Nesvorny To cite this version: Morbidelli
More informationSolar System Working Group. 6th Meeting -----
Solar System Working Group 6th Meeting ----- F. Mignard 1 Attendants - Alberto CELLINO - Aldo DELL'ORO -Marco DELBO - Enrico GERLACH - Daniel HESTROFFER - Sergei KLIONER - Claes-Ingvar LAGERKVIST -ValeryLAINEY
More informationA FIRST LOOK AT THE DAMOCLOIDS
The Astronomical Journal, 129:000 000, 2005 January # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. A FIRST LOOK AT THE DAMOCLOIDS David Jewitt 1 Institute for Astronomy,
More informationAssessment Vocabulary Instructional Strategies
Inner Planets and the similarities for each of the inner planets? (Mercury, Venus, Earth, and Mars - such as Size, atmosphere, moons/rings, ) What are the unique characteristics and details of each of
More informationEvidence for an extended scattered disk.
Evidence for an extended scattered disk. arxiv:astro-ph/0103435v1 27 Mar 2001 B. Gladman 1, M. Holman 2, T. Grav 3, J. Kavelaars 4, P. Nicholson 5, K. Aksnes 3, J-M. Petit 1 1 Observatoire de la Côte d
More informationPHYSICAL CHARACTERIZATION OF THE BINARY EDGEWORTH KUIPER BELT OBJECT 2001 QT 297
PHYSICAL CHARACTERIZATION OF THE BINARY EDGEWORTH KUIPER BELT OBJECT 2001 QT 297 DAVID J. OSIP Observatories of the Carnegie Institution of Washington, Las Campanas Observatory S. D. KERN 1 and J. L. ELLIOT
More informationPolarimetry in Planetary Science A Step Forward with the VLT and a Need for the ELTs
Earth Moon Planet (2009) 105:95 100 DOI 10.1007/s11038-009-9321-z Polarimetry in Planetary Science A Step Forward with the VLT and a Need for the ELTs H. Boehnhardt Æ G. P. Tozzi Æ M. Sterzik Æ S. Bagnulo
More informationComet Measurement Techniques. Karen Meech Institute for Astronomy Session 27 1/18/05
Comet Measurement Techniques Karen Meech Institute for Astronomy Session 27 1/18/05 Image copyright, R. Wainscoat, IfA Image courtesy K. Meech Techniques Summary Imaging & Detectors Photometry Deep Imaging
More informationAstronomy 405 Solar System and ISM
Astronomy 405 Solar System and ISM Lecture 14 Comets February 15, 2013 Dynamics of Comet Tails Gas (ion) tails - interact with the solar wind - point away from the Sun. Dust tails - pushed by radiation
More informationPueo-Nui Workshop Solar System Observations
Pueo-Nui Workshop Solar System Observations Christophe Dumas NASA / Jet Propulsion Laboratory Background information Pueo-Nui expected performances Strehl of ~ 92% at K band (on bright sources) Strehl
More informationBenefits of Infrared. The Spitzer Space Telescope. Instruments/Components of Spitzer. Cryostat. Infrared Telescope
The Spitzer Space Telescope Benefits of Infrared IR can reveal objects that don't emit visible light IR provides different information than visible light IR is better than visible for viewing cold objects
More informationOverview. Hubble Pluto Satellite Search Team reporting the discovery to the New Horizons Science Team on November 2, 2005 at the Kennedy Space Center
The discovery of two new satellites of Pluto Overview Max Mutchler Space Telescope Science Institute mutchler@stsci.edu New Horizons Educator Workshop 16 January 2006 Hubble s Advanced Camera; Discovery
More informationExploring and Understanding the Primitive Bodies of the Solar System: Progress Report from the Primitive Bodies Panel of the Decadal Survey
Exploring and Understanding the Primitive Bodies of the Solar System: Progress Report from the Primitive Bodies Panel of the Decadal Survey J. VEVERKA, H. MCSWEEN AND THE PRIMITIVE BODIES PANEL AGU MEETING
More informationTNOs are Cool: A Survey of the Transneptunian Region. (37 members, 19 institutes, 9 countries)
TNOs are Cool: A Survey of the Transneptunian Region Thomas Müller & MPE Garching The TNOs-are-Cool Team (37 members, 19 institutes, 9 countries) Overview OT KP with 370 hours PACS and SPIRE photometric
More informationPostcards from the Edge. JJ Kavelaars
Postcards from the Edge JJ Kavelaars Extra-Extra... HR 8799 in the sub-mm HR 8799 (Marios et al.) Spectra! (Janson, et al.) Background... Glencoe District High School GDHS Some personal info... Show your
More informationThe search for Planet X Lowell Observatory, Flagstaff, Arizona. Overview. Andy Lubenow
The discovery of two new satellites of Pluto Max Mutchler Space Telescope Science Institute Open Night 3 January 2006 Andy Lubenow 1956-2005 Hubble Pluto Satellite Search Team reporting the discovery to
More informationarxiv: v1 [astro-ph.ep] 13 Feb 2015
Astronomy & Astrophysics manuscript no. peixinho+2015 c ESO 2016 November 16, 2016 Reanalyzing the visible colors of Centaurs and KBOs: what is there and what we might be missing. Nuno Peixinho 1, Audrey
More information28-Aug-17. A Tour of Our Solar System and Beyond. The Sun
A Tour of Our Solar System and Beyond The Sun diameter = 1,390,000 km = 864,000 mi >99.8% of the mass of the entire solar system surface temperature 5800 C 600 x 10 6 tons H -> 596 x 10 6 tons He per second
More informationAstronomy 1 Winter Lecture 11; January
Astronomy 1 Winter 2011 Lecture 11; January 31 2011 Previously on Astro-1 Properties of the Planets: Orbits in the same plane and direction Inner planets are small and made of heavy elements Outer planets
More informationAstronomers Universe. More information about this series at
Astronomers Universe More information about this series at http://www.springer.com/series/6960 ThiS is a FM Blank Page John Wilkinson The Solar System in Close-Up John Wilkinson Castlemaine, Victoria Australia
More informationPost-perihelion observations of comet 1P/Halley
A&A 417, 1159 1164 (2004) DOI: 10.1051/0004-6361:20035658 c ESO 2004 Astronomy & Astrophysics Post-perihelion observations of comet 1P/Halley V: r h = 28.1 AU O. R. Hainaut 1, A. Delsanti 2, K. J. Meech
More information11th tri-annual CFHT User's Meeting. Brett Gladman, UBC, for the OSSOS collaboration
11th tri-annual CFHT User's Meeting Brett Gladman, UBC, for the OSSOS collaboration The OSSOS award Top-ranked LP from the 2nd 4-year round. Awarded 560 hours, evenly spread (70h/semseter) over 2013A-2016B
More informationON THE ORIGIN OF THE HIGH-PERIHELION SCATTERED DISK: THE ROLE OF THE KOZAI MECHANISM AND MEAN MOTION RESONANCES
ON THE ORIGIN OF THE HIGH-PERIHELION SCATTERED DISK: THE ROLE OF THE KOZAI MECHANISM AND MEAN MOTION RESONANCES RODNEY S. GOMES 1, TABARE GALLARDO 2, JULIO A. FERNA NDEZ 2 AND ADRIA N BRUNINI 3 1 GEA/OV/UFRJ
More informationIme annnfi 3ll i I am is Il im ow U * doif uo tm.i NO No m ini uudift u
REPORT DOCUMENTATION PAGE ramn Appmmld cmno 070 J-O18s hlow Iponu fu d i inom miflit 0 WMO au nnuwiu liii ins IUE IIIIIII'U NOE- r badi.. m Ia V f~ I law. noift a "Nimillon Ime annnfi 3ll i I am is Il
More informationIcarus. Considerations on the magnitude distributions of the Kuiper belt and of the Jupiter Trojans
Icarus 202 (2009) 30 35 Contents lists available at ScienceDirect Icarus www.elsevier.com/locate/icarus Considerations on the magnitude distributions of the Kuiper belt and of the Jupiter Trojans Alessandro
More informationKuiper Belt Objects Advanced Lab
Kuiper Belt Objects Advanced Lab Introduction To date, there are over 763 known Kuiper Belt Objects (KBOs), including Pluto and Charon, however, because they are so distant, faint, and relatively new to
More informationColors of Centaurs. Stephen C. Tegler Northern Arizona University. James M. Bauer Jet Propulsion Laboratory. William Romanishin University of Oklahoma
Tegler et al.: Colors of Centaurs 105 Colors of Centaurs Stephen C. Tegler Northern Arizona University James M. Bauer Jet Propulsion Laboratory William Romanishin University of Oklahoma Nuno Peixinho Grupo
More informationPolarimetry of asteroids
Polarimetry of asteroids Irina Belskaya Institute of Astronomy, V.N. Karazin Kharkiv National University, Ukraine In collaboration with: Stefano Bagnulo, Armagh Observatory, UK Sonia Fornasier, Observatoire
More informationA collective effort of many people active in the CU4 of the GAIA DPAC
A collective effort of many people active in the CU4 of the GAIA DPAC (D. Hestroffer, P. Tanga, J.M. Petit, J. Berthier, W. Thuillot, F. Mignard, M. Delbò,...) The impact of GAIA on Asteroid Science will
More informationCharacterization of the exoplanet host stars. Exoplanets Properties of the host stars. Characterization of the exoplanet host stars
Characterization of the exoplanet host stars Exoplanets Properties of the host stars Properties of the host stars of exoplanets are derived from a combination of astrometric, photometric, and spectroscopic
More informationAstronomy 1140 Quiz 4 Review
Astronomy 1140 Quiz 4 Review Anil Pradhan December 6, 2016 I The Outer Planets in General 1. How do the sizes, masses and densities of the outer planets compare with the inner planets? The outer planets
More information1. INTRODUCTION. THE ASTRONOMICAL JOURNAL, 121:1730È1735, 2001 March ( The American Astronomical Society. All rights reserved. Printed in U.S.A.
THE ASTRONOMICAL JOURNAL, 121:1730È1735, 2001 March ( 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A. ON THE SIZE DEPENDENCE OF THE INCLINATION DISTRIBUTION OF THE MAIN
More informationPLANETARY ASTRONOMY: MINOR PLANETS AND PLANET FORMATION.
PLANETARY ASTRONOMY: MINOR PLANETS AND PLANET FORMATION. J. KAVELAARS 1, B.J. GLADMAN 2, ALAN HILDEBRAND 3, W. C. FRASER 4, RALPH E. PUDRITZ 6, AND PAUL WIEGERT 7 SUMMARY Solar system studies of minor
More informationLight and Telescopes
Light and Telescopes Astronomy 1 Elementary Astronomy LA Mission College Spring F2015 Quotes & Cartoon of the Day We find them smaller and fainter, in constantly increasing numbers, and we know that we
More information