The Blurring Distinction Between Asteroids and Comets
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Jjmonl 1712.Pmd
alactic Observer John J. McCarthy Observatory G Volume 10, No. 12 December 2017 Holiday Theme Park See page 19 for more information The John J. McCarthy Observatory Galactic Observer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky Technical Support It is through their efforts that the McCarthy Observatory Bob Lambert has established itself as a significant educational and recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Route Mike Chiarella Roger Moore Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Doug Delisle Marc Polansky Cecilia Detrich Joe Privitera Dirk Feather Monty Robson Randy Fender Don Ross Louise Gagnon Gene Schilling John Gebauer Katie Shusdock Elaine Green Paul Woodell Tina Hartzell Amy Ziffer In This Issue "OUT THE WINDOW ON YOUR LEFT"............................... 3 REFERENCES ON DISTANCES ................................................ 18 SINUS IRIDUM ................................................................ 4 INTERNATIONAL SPACE STATION/IRIDIUM SATELLITES ............. 18 EXTRAGALACTIC COSMIC RAYS ........................................ 5 SOLAR ACTIVITY ............................................................... 18 EQUATORIAL ICE ON MARS? ........................................... -
1. Some of the Definitions of the Different Types of Objects in the Solar
1. Some of the definitions of the different types of objects in has the greatest orbital inclination (orbit at the the solar system overlap. Which one of the greatest angle to that of Earth)? following pairs does not overlap? That is, if an A) Mercury object can be described by one of the labels, it B) Mars cannot be described by the other. C) Jupiter A) dwarf planet and asteroid D) Pluto B) dwarf planet and Kuiper belt object C) satellite and Kuiper belt object D) meteoroid and planet 10. Of the following objects in the solar system, which one has the greatest orbital eccentricity and therefore the most elliptical orbit? 2. Which one of the following is a small solar system body? A) Mercury A) Rhea, a moon of Saturn B) Mars B) Pluto C) Earth C) Ceres (an asteroid) D) Pluto D) Mathilde (an asteroid) 11. What is the largest moon of the dwarf planet Pluto 3. Which of the following objects was discovered in the called? twentieth century? A) Chiron A) Pluto B) Callisto B) Uranus C) Charon C) Neptune D) Triton D) Ceres 12. If you were standing on Pluto, how often would you see 4. Pluto was discovered in the satellite Charon rise above the horizon each A) 1930. day? B) 1846. A) once each 6-hour day as Pluto rotates on its axis C) 1609. B) twice each 6-hour day because Charon is in a retrograde D) 1781. orbit C) once every 2 days because Charon orbits in the same direction Pluto rotates but more slowly 5. -
Alexandre Amorim -.:: GEOCITIES.Ws
Alexandre Amorim (org) 2 3 PREFÁCIO O Boletim Observe! é uma iniciativa da Coordenação de Observação Astronômica do Núcleo de Estudo e Observação Astronômica “José Brazilício de Souza” (NEOA-JBS). Durante a reunião administrativa do NEOA-JBS em maio de 2010 foi apresentada a edição de Junho de 2010 para apreciação dos demais coordenadores do Núcleo onde houve aprovação unânime em usar o Boletim Observe! como veículo de informação das atividades e, principalmente, observações astronômicas. O Boletim Observe! é publicado mensalmente em formato eletrônico ou impresso separadamente, prezando pela simplicidade das informações e encorajando os leitores a observar, registrar e publicar os eventos astronômicos. Desde a sua primeira edição o Boletim Observe! conta com a colaboração espontânea de diversos astrônomos amadores e profissionais. Toda edição do Observe! do mês de dezembro é publicado um índice dos artigos do respectivo ano. Porém, desde aquela edição de Junho de 2010 foram publicados centenas de artigos e faz-se necessário consultar assuntos que foram tratados nas edições anteriores do Observe! e seus respectivos autores. Para isso publicaremos anualmente esse Índice de Assuntos, permitindo a consulta rápida dos temas abordados. Florianópolis, 1º de dezembro de 2018 Alexandre Amorim Coordenação de Observação Astronômica do NEOA-JBS 4 Ano I (2010) Nº 1 – Junho 2010 Eclipse da Lua em 26 de junho de 2010 Amorim, A. Júpiter sem a Banda Equatorial Sul Amorim, A. Conjunção entre Júpiter e Urano Amorim, A. Causos do Avelino Alves, A. A. Quem foi Eugênia de Bessa? Amorim, A. Nº 2 – Julho 2010 Aprendendo a dimensionar as distâncias angulares no céu Neves, M. -
About GRAS and ACP About Observing Plans Overall Plan Format
About GRAS and ACP Global Rent-a-Scope systems are based on a highly modified version of ACP, that we have customized in house. A number of key differences exist between the generic version and the GRAS version. Please review this document for the supported GRAS supported directives. About Observing Plans You can generate plans a number of ways: 1. One Click Image. If you are new to GRAS and ACP follow the “One Click Image” link, this will give you a menu of target currently visible from the observatory. You just click the target to start imaging it. 2. ACP can generate a simple plan via its web interface consisting of single target with multiple filters and exposure time, please see “Single Image” and “Color Series” links inside ACP. This plan will automatically start at the observatory. This is by far the easies way to get started with ACP. The plan it generates is called “last-plan-from-web.txt” and it can be download via the My Documents link inside ACP if you wish to view its contents. 3. GRAS has also implemented via its reservation system a Plan Generator which work the same way as point two. You can select a target, filters and exposure times. You can give you plan a name and it will save it. You can then use this plan via the Launch a Plan feature on the reservation system to start the plan at a given date and time. You can also start this plan manually via “Scripted Plan” link inside ACP. -
Gemini Observations of Active Asteroid 354P/LINEAR (2010 A2)
Gemini Observations of Active Asteroid 354P/LINEAR (2010 A2) Yoonyoung Kim, Masateru Ishiguro Seoul National University (Korea) Science & Evolution of Gemini Observatory 2018 Fisherman’s Wharf, San Francisco Contents • Overview • Active asteroids resulting from impacts • The case of 354P/LINEAR (2010 A2) • Concluding remark Overview “Small Solar System bodies are primitive, but...” Solar System Formation “Snow line” Credit: Univ. of Hawaii Primitive small bodies Kuiper Belt ~30-55 AU Oort Cloud ~104-105 AU Yeomans 2000 Primitive small bodies (easy to observe) are comets and asteroids Kuiper Belt ~30-55 AU Oort Cloud ~104-105 AU Yeomans 2000 but, primitive small bodies also evolved... by solar radiative heating by impacts NASA/JPL/Univ. of Maryland but, primitive small bodies also evolved... by solar radiative heating by impacts NASA/JPL/Univ. of Maryland Purpose of this study • We aim to figure out one of the major evolutionary processes in the Solar System (impacts) through observational studies of • Active asteroids resulting from impacts • The case of 354P/LINEAR (2010 A2) Comets Active Asteroids Active asteroids Dormant Comets Asteroids resulting from impacts : The case of 354P/LINEAR (2010 A2) Kim, Y., Ishiguro, M., et al. 2017, AJ Kim, Y., Ishiguro, M., & Lee, M. G. 2017, ApJL Background “Evidences of past impacts” Credit: D. Jewitt The case of (596) Scheila Ishiguro+2011 The case of 354P/2010 A2 Jewitt+2011 The case of 354P/2010 A2 The case of 354P/2010 A2 Previous modelings (Jewitt+10,13; Snodgrass+10; Hainaut+12; Agarwal+13; Kleyna+13) Jewitt+2013 Kleyna+2013 Observation 2010 Model Observation Agarwal+2013 Obs. -
Instrumental Methods for Professional and Amateur
Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, Francois Colas, Alain Klotz, Christophe Pellier, Jean-Marc Petit, Philippe Rousselot, et al. To cite this version: Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, et al.. Instru- mental Methods for Professional and Amateur Collaborations in Planetary Astronomy. Experimental Astronomy, Springer Link, 2014, 38 (1-2), pp.91-191. 10.1007/s10686-014-9379-0. hal-00833466 HAL Id: hal-00833466 https://hal.archives-ouvertes.fr/hal-00833466 Submitted on 3 Jun 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy O. Mousis, R. Hueso, J.-P. Beaulieu, S. Bouley, B. Carry, F. Colas, A. Klotz, C. Pellier, J.-M. Petit, P. Rousselot, M. Ali-Dib, W. Beisker, M. Birlan, C. Buil, A. Delsanti, E. Frappa, H. B. Hammel, A.-C. Levasseur-Regourd, G. S. Orton, A. Sanchez-Lavega,´ A. Santerne, P. Tanga, J. Vaubaillon, B. Zanda, D. Baratoux, T. Bohm,¨ V. Boudon, A. Bouquet, L. Buzzi, J.-L. Dauvergne, A. -
An Early Warning System for Asteroid Impact
An Early Warning System for Asteroid Impact John L. Tonry(1) ABSTRACT Earth is bombarded by meteors, occasionally by one large enough to cause a significant explosion and possible loss of life. It is not possible to detect all hazardous asteroids, and the efforts to detect them years before they strike are only advancing slowly. Similarly, ideas for mitigation of the danger from an impact by moving the asteroid are in their infancy. Although the odds of a deadly asteroid strike in the next century are low, the most likely impact is by a relatively small asteroid, and we suggest that the best mitigation strategy in the near term is simply to move people out of the way. With enough warning, a small asteroid impact should not cause loss of life, and even portable property might be preserved. We describe an \early warning" system that could provide a week's notice of most sizeable asteroids or comets on track to hit the Earth. This may be all the mitigation needed or desired for small asteroids, and it can be implemented immediately for relatively low cost. This system, dubbed \Asteroid Terrestrial-impact Last Alert System" (AT- LAS), comprises two observatories separated by about 100 km that simulta- neously scan the visible sky twice a night. Software automatically registers a comparison with the unchanging sky and identifies everything which has moved or changed. Communications between the observatories lock down the orbits of anything approaching the Earth, within one night if its arrival is less than a week. The sensitivity of the system permits detection of 140 m asteroids (100 Mton impact energy) three weeks before impact, and 50 m asteroids a week be- fore arrival. -
The Minor Planet Bulletin 44 (2017) 142
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 44, NUMBER 2, A.D. 2017 APRIL-JUNE 87. 319 LEONA AND 341 CALIFORNIA – Lightcurves from all sessions are then composited with no TWO VERY SLOWLY ROTATING ASTEROIDS adjustment of instrumental magnitudes. A search should be made for possible tumbling behavior. This is revealed whenever Frederick Pilcher successive rotational cycles show significant variation, and Organ Mesa Observatory (G50) quantified with simultaneous 2 period software. In addition, it is 4438 Organ Mesa Loop useful to obtain a small number of all-night sessions for each Las Cruces, NM 88011 USA object near opposition to look for possible small amplitude short [email protected] period variations. Lorenzo Franco Observations to obtain the data used in this paper were made at the Balzaretto Observatory (A81) Organ Mesa Observatory with a 0.35-meter Meade LX200 GPS Rome, ITALY Schmidt-Cassegrain (SCT) and SBIG STL-1001E CCD. Exposures were 60 seconds, unguided, with a clear filter. All Petr Pravec measurements were calibrated from CMC15 r’ values to Cousins Astronomical Institute R magnitudes for solar colored field stars. Photometric Academy of Sciences of the Czech Republic measurement is with MPO Canopus software. To reduce the Fricova 1, CZ-25165 number of points on the lightcurves and make them easier to read, Ondrejov, CZECH REPUBLIC data points on all lightcurves constructed with MPO Canopus software have been binned in sets of 3 with a maximum time (Received: 2016 Dec 20) difference of 5 minutes between points in each bin. -
Solar System in My Room Man
6 + 2055 WARNING: CHOKING HAZARD - Small parts/small ball(s). Not for children under 3 years. A word about Pluto... Since it was discovered in 1930, Pluto has been considered the ninth planet of our solar system. In 2006, at a large gathering of astronomers from around the world, it was agreed that objects in our solar system should be divided into three main categories: planets, dwarf planets, and small solar system bodies. A planet orbits only the Sun and nothing else; it is massive enough that its gravity makes it spherical; and its gravity is strong enough to keep the path of its orbit clear of other objects. There are officially eight planets in our solar system. A dwarf planet also orbits the Sun and is spherical, but its gravity is not strong enough to clear its orbital path of other objects. There are officially at least three dwarf planets in our solar system. A small solar system body is not massive enough to have gravity that can make it spherical, so its shape is irregular. Asteroids, comets and moons are in this category. There are many small solar system bodies. Therefore, with these new definitions of objects in our solar system, Pluto is no longer considered a planet. It is officially a dwarf planet (along with two others, Ceres and Eris). Ceiling Installing Batteries Mounting Plate Tool required - Small Phillips-head screwdriver 1. Use a Phillips-head screwdriver to remove the battery door. On/Off 2. Insert 3 “AA” batteries. Make sure the “+” and “-” ends are inserted correctly, as indicated in the battery compartment. -
The Search for Water Ice on Comets and Asteroids
UNIVERSIDAD COMPLUTENSE DE MADRID FACULTAD DE CIENCIAS FÍSICAS TESIS DOCTORAL The Search for water ice on Comets and Asteroids La búsqueda de hielo de agua en Cometas y Asteroides MEMORIA PARA OPTAR AL GRADO DE DOCTOR PRESENTADA POR Laurence O’Rourke DIRECTOR Michael Küppers Madrid © Laurence O’Rourke, 2021 UNIVERSIDAD COMPLUTENSE DE MADRID FACULTAD DE CIENCIAS FÍSICAS TESIS DOCTORAL La búsqueda de hielo de agua en Cometas y Asteroides MEMORIA PARA OPTAR AL GRADO DE DOCTOR PRESENTADA POR Laurence O’Rourke DIRECTOR Dr. Michael Küppers The Search for water ice on Comets and Asteroids La búsqueda de hielo de agua en Cometas y Asteroides TESIS DOCTORAL LAURENCE O’ROURKE Departamento de Física de la Tierra y Astrofísica Facultad de Ciencias Físicas Universidad Complutense de Madrid A thesis submitted for the degree of Doctor en Astrofisica September 2020 Director: Dr. Michael Küppers Tutor: Prof. David Montes Gutiérrez Dedication I would like to dedicate this thesis to my wife Cristina & our children David and Paulina, and to my parents, Laurence and Rita (neé Curley) O’Rourke, who have both passed away but who would no doubt have been very proud of me for this achievement. Acknowledgements This work has been possible thanks to the great support and help provided by my PhD director Michael Küppers and by my UCM tutor, David Montes Gutiérrez. The published papers presented, provide an excellent overview of the significant collaborations I have had across the planetary science community with nearly 50 different co-authors represented in the papers. Their professionalism, expertise and friendship were vital to ensure that the papers I wrote were at the highest level. -
The Castalia Mission to Main Belt Comet 133P/Elst-Pizarro C
The Castalia mission to Main Belt Comet 133P/Elst-Pizarro C. Snodgrass, G.H. Jones, H. Boehnhardt, A. Gibbings, M. Homeister, N. Andre, P. Beck, M.S. Bentley, I. Bertini, N. Bowles, et al. To cite this version: C. Snodgrass, G.H. Jones, H. Boehnhardt, A. Gibbings, M. Homeister, et al.. The Castalia mission to Main Belt Comet 133P/Elst-Pizarro. Advances in Space Research, Elsevier, 2018, 62 (8), pp.1947- 1976. 10.1016/j.asr.2017.09.011. hal-02350051 HAL Id: hal-02350051 https://hal.archives-ouvertes.fr/hal-02350051 Submitted on 28 Aug 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Distributed under a Creative Commons Attribution| 4.0 International License Available online at www.sciencedirect.com ScienceDirect Advances in Space Research 62 (2018) 1947–1976 www.elsevier.com/locate/asr The Castalia mission to Main Belt Comet 133P/Elst-Pizarro C. Snodgrass a,⇑, G.H. Jones b, H. Boehnhardt c, A. Gibbings d, M. Homeister d, N. Andre e, P. Beck f, M.S. Bentley g, I. Bertini h, N. Bowles i, M.T. Capria j, C. Carr k, M. -
Colours of Minor Bodies in the Outer Solar System II - a Statistical Analysis, Revisited
Astronomy & Astrophysics manuscript no. MBOSS2 c ESO 2012 April 26, 2012 Colours of Minor Bodies in the Outer Solar System II - A Statistical Analysis, Revisited O. R. Hainaut1, H. Boehnhardt2, and S. Protopapa3 1 European Southern Observatory (ESO), Karl Schwarzschild Straße, 85 748 Garching bei M¨unchen, Germany e-mail: [email protected] 2 Max-Planck-Institut f¨ur Sonnensystemforschung, Max-Planck Straße 2, 37 191 Katlenburg- Lindau, Germany 3 Department of Astronomy, University of Maryland, College Park, MD 20 742-2421, USA Received —; accepted — ABSTRACT We present an update of the visible and near-infrared colour database of Minor Bodies in the outer Solar System (MBOSSes), now including over 2000 measurement epochs of 555 objects, extracted from 100 articles. The list is fairly complete as of December 2011. The database is now large enough that dataset with a high dispersion can be safely identified and rejected from the analysis. The method used is safe for individual outliers. Most of the rejected papers were from the early days of MBOSS photometry. The individual measurements were combined so not to include possible rotational artefacts. The spectral gradient over the visible range is derived from the colours, as well as the R absolute magnitude M(1, 1). The average colours, absolute magnitude, spectral gradient are listed for each object, as well as their physico-dynamical classes using a classification adapted from Gladman et al., 2008. Colour-colour diagrams, histograms and various other plots are presented to illustrate and in- vestigate class characteristics and trends with other parameters, whose significance are evaluated using standard statistical tests.