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Where Are the Distant Worlds? Star Maps
W here Are the Distant Worlds? Star Maps Abo ut the Activity Whe re are the distant worlds in the night sky? Use a star map to find constellations and to identify stars with extrasolar planets. (Northern Hemisphere only, naked eye) Topics Covered • How to find Constellations • Where we have found planets around other stars Participants Adults, teens, families with children 8 years and up If a school/youth group, 10 years and older 1 to 4 participants per map Materials Needed Location and Timing • Current month's Star Map for the Use this activity at a star party on a public (included) dark, clear night. Timing depends only • At least one set Planetary on how long you want to observe. Postcards with Key (included) • A small (red) flashlight • (Optional) Print list of Visible Stars with Planets (included) Included in This Packet Page Detailed Activity Description 2 Helpful Hints 4 Background Information 5 Planetary Postcards 7 Key Planetary Postcards 9 Star Maps 20 Visible Stars With Planets 33 © 2008 Astronomical Society of the Pacific www.astrosociety.org Copies for educational purposes are permitted. Additional astronomy activities can be found here: http://nightsky.jpl.nasa.gov Detailed Activity Description Leader’s Role Participants’ Roles (Anticipated) Introduction: To Ask: Who has heard that scientists have found planets around stars other than our own Sun? How many of these stars might you think have been found? Anyone ever see a star that has planets around it? (our own Sun, some may know of other stars) We can’t see the planets around other stars, but we can see the star. -
C a L E N D a R F O R 2019
Small Astronomy Calendar for Amateur Astronomers Year III 2021 Let’s welcome our 2021 Small Astronomy Calendar Edition made by our Intergalactic Astronomy Educators Fellowship (IGAEF)’s team. In 2021, many amateur astronomers asked for calculations for more specific geographical locations. This year we added new useful calculated positions and coordinates for everyone in the world to use. You should check this calendar every month, specifically the lunar occultations pages for your observation point. There are many interesting and unique events that might not happen every year, because of the different parameters of the Moon orbit. Our hope is to fulfill your expectations. We would like to receive suggestions and feedback. You can find the editor’s email in the last page of the calendar. We appreciate your support and we are looking forward to having a good observational year, and a better and more complete calendar for this first year of a new decade. Index 3 - Calendar for 2021 4 – What is the Intergalactic Astronomy Educators Fellowship (IGAEF) 5 - Time Zones and Universal Time 6 - Phases of the Moon 2021 7 – Physical Ephemeris for the Moon 2021 10 - Local Time (EST) of MOONRISE 2021 11 - Local Time (EST) of MOONSET 2021 12 - Local time (EST) of planets rise and set 2021 15 - Diary of Astronomical Phenomena 2021 21 - Lunar eclipses 23 - Solar Eclipses 25 - Meteor Showers for 2021 26 – 2021 UPCOMING COMETS 27 - Satellites of Jupiter 2021 36 – Mutual Events of Jupiter Satellites 2021 39 - Julian Day Number, Apparent Sidereal Time, Obliquity -
Coalescence and Particle Self-Assembly of Inkjet-Printed Colloidal Drops
Coalescence and Particle Self-assembly of Inkjet-printed Colloidal Drops A Thesis Submitted to the Faculty of Drexel University by Xin Yang in partial fulfillment of the requirements for the degree of Doctor of Philosophy December 2014 ii © Copyright 2014 Xin Yang. All Rights Reserved. iii Acknowledgements I would like to thank my advisor Prof. Ying Sun. During the last 3 years, she supports and guides me throughout the course of my Ph.D. research with her profound knowledge and experience. Her dedication and passion for researches greatly encourages me in pursuing my career goals. I greatly appreciate her contribution to my growth during my Ph.D. training. I would like to thank my parents, my girlfriend, my colleagues (Brandon, Charles, Dani, Gang, Dong-Ook, Han, Min, Nate, and Viral) and friends (Abraham, Mahamudur, Kewei, Patrick, Xiang, and Yontae). I greatly appreciate Prof. Nicholas Cernansky, Prof. Bakhtier Farouk, Prof. Adam Fontecchio, Prof. Frank Ji, Prof. Alan Lau, Prof. Christopher Li, Prof. Mathew McCarthy, and Prof. Hongseok (Moses) Noh for their critical assessments and positive suggestions during my candidacy exam, proposal and my defense. I also appreciate the financial supports of National Science Foundation (Grant CAREER-0968927 and CMMI-1200385). iv TABLE OF CONTENTS LIST OF TABLES ............................................................................................................ vii LIST OF FIGURES ......................................................................................................... viii -
The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile. -
00E the Construction of the Universe Symphony
The basic construction of the Universe Symphony. There are 30 asterisms (Suites) in the Universe Symphony. I divided the asterisms into 15 groups. The asterisms in the same group, lay close to each other. Asterisms!! in Constellation!Stars!Objects nearby 01 The W!!!Cassiopeia!!Segin !!!!!!!Ruchbah !!!!!!!Marj !!!!!!!Schedar !!!!!!!Caph !!!!!!!!!Sailboat Cluster !!!!!!!!!Gamma Cassiopeia Nebula !!!!!!!!!NGC 129 !!!!!!!!!M 103 !!!!!!!!!NGC 637 !!!!!!!!!NGC 654 !!!!!!!!!NGC 659 !!!!!!!!!PacMan Nebula !!!!!!!!!Owl Cluster !!!!!!!!!NGC 663 Asterisms!! in Constellation!Stars!!Objects nearby 02 Northern Fly!!Aries!!!41 Arietis !!!!!!!39 Arietis!!! !!!!!!!35 Arietis !!!!!!!!!!NGC 1056 02 Whale’s Head!!Cetus!! ! Menkar !!!!!!!Lambda Ceti! !!!!!!!Mu Ceti !!!!!!!Xi2 Ceti !!!!!!!Kaffalijidhma !!!!!!!!!!IC 302 !!!!!!!!!!NGC 990 !!!!!!!!!!NGC 1024 !!!!!!!!!!NGC 1026 !!!!!!!!!!NGC 1070 !!!!!!!!!!NGC 1085 !!!!!!!!!!NGC 1107 !!!!!!!!!!NGC 1137 !!!!!!!!!!NGC 1143 !!!!!!!!!!NGC 1144 !!!!!!!!!!NGC 1153 Asterisms!! in Constellation Stars!!Objects nearby 03 Hyades!!!Taurus! Aldebaran !!!!!! Theta 2 Tauri !!!!!! Gamma Tauri !!!!!! Delta 1 Tauri !!!!!! Epsilon Tauri !!!!!!!!!Struve’s Lost Nebula !!!!!!!!!Hind’s Variable Nebula !!!!!!!!!IC 374 03 Kids!!!Auriga! Almaaz !!!!!! Hoedus II !!!!!! Hoedus I !!!!!!!!!The Kite Cluster !!!!!!!!!IC 397 03 Pleiades!! ! Taurus! Pleione (Seven Sisters)!! ! ! Atlas !!!!!! Alcyone !!!!!! Merope !!!!!! Electra !!!!!! Celaeno !!!!!! Taygeta !!!!!! Asterope !!!!!! Maia !!!!!!!!!Maia Nebula !!!!!!!!!Merope Nebula !!!!!!!!!Merope -
THE STAR FORMATION NEWSLETTER an Electronic Publication Dedicated to Early Stellar Evolution and Molecular Clouds
THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stellar evolution and molecular clouds No. 193 — 13 Jan 2009 Editor: Bo Reipurth ([email protected]) Abstracts of recently accepted papers [O i] sub-arcsecond study of a microjet from an intermediate mass young star: RY Tau V. Agra-Amboage1, C. Dougados1, S. Cabrit2, P.J.V. Garcia3,4,1 and P. Ferruit5 1 Laboratoire d’Astrophysique de l’Observatoire de Grenoble, UMR 5521 du CNRS, 38041 Grenoble C´edex 9, France 2 LERMA, Observatoire de Paris, UMR 8112 du CNRS, 61 Avenue de l’Observatoire, 75014 Paris, France 3 Departamento de Engenharia Fisica,Faculdade de Engenharia,Universidade do Porto, 4200-465 Porto, Portugal 4 Centro de Astrofisica, Universidade do Porto, Porto, Portugal 5 CRAL, Observatoire de Lyon, 9 Av. Charles Andr´e, F-69230 St. Genis Laval, France E-mail contact: Catherine.Dougados at obs.ujf-grenoble.fr High-resolution studies of microjets in T Tauri stars (cTTs) reveal key information on the jet collimation and launching mechanism, but only a handful of systems have been mapped so far. We perform a detailed study of the microjet from the 2 M⊙ young star RY Tau, to investigate the influence of its higher stellar mass and claimed close binarity on jet properties. Spectro-imaging observations of RY Tau were obtained in [O i]λ6300 with resolutions of 0.4′′ and 135 km s−1, using the integral field spectrograph OASIS at the Canada-France-Hawaii Telescope. Deconvolved images reach a resolution of 0.2′′. The blueshifted jet is detected within 2′′ of the central star. -
Bernard Mombo Kissui
Demography, population dynamics, and the human-lion conflicts: lions in the Ngorongoro Crater and the Maasai steppe, Tanzania A Thesis Submitted to the Faculty of the Graduate School of the University of Minnesota By Bernard Mombo Kissui In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy Craig Packer, Adviser May, 2008 Acknowledgements The success of the work presented in this thesis could not have been possible without the support and assistance from many people. I would particularly like to acknowledge Craig Packer, whom I have worked with for nearly ten years now, initially as a field research assistant on the Serengeti Lion Project and later as my advisor at the University of Minnesota . I am grateful for his guidance through the development and writing stages of the thesis. I acknowledge my advisory committee: Claudia Neuhauser, Steve Polasky and Sandy Weisberg for their guidance and supervision. I am particularly grateful to Sandy Weisberg for his tireless advice in statistical analysis throughout the writing process. I acknowledge the financial support from many organizations that made this study possible. I would like to particularly thank the McArthur Fellowship Program at the Interdisciplinary Center for the study of Global Change (ICGC) and the EEB department, University of Minnesota for making it possible for me to initially join the doctorate program and for continuous support through the program. To AWF’s Charlotte Conservation Fellowship Program; WCS Kaplan Award Program for Wildcat Conservation; Lincoln Park Zoo’s Field Conservation Funds, and to Woodland Park Zoo I am grateful for supporting my field research in the Maasai steppe. -
July OBSERVER(220Dpi)
THE OBSERVER OF THE TWIN CITY AMATEUR ASTRONOMERS Volume 45, Number 7 July 2020 INSIDE THIS ISSUE: 1«Editor’s Choice: Image of the Month – Messier 27 2«President’s Note 2«NCRAL’s Season Messier Mini Marathons 3«Calendar of Astronomical Events – July 2020 3«New & Renewing Members/Dues Blues/E-Mail List 4«This Month’s Phases of the Moon 4«This Month’s Solar Phenomena 4«AstroBits – News from Around the TCAA 6«Waynesville Observatory Use Policy Statement 7«CDK 24” Telescope Coming Online at WO 7«Celestron NexStar 11” Telescope Donated to TCAA 8«TCAA Image Gallery 9«Maintenance Work at Waynesville Observatory 10«Did You Know? 11«TCAA Active on Facebook 11«July 2020 with Jeffrey L. Hunt 23«Renewing Your TCAA Membership 23«Online Public Talks for 2020 24«TCAA Treasurer’s Report as of June 26, 2020 The TCAA is an affiliate of the Astronomical League as well as its North Central Region. For more information about the TCAA, be certain to visit the TCAA website at http://www.tcaa.us/ Visit http://www.astroleague.org for additional information about the Astronomical League and its EDITOR’S CHOICE: IMAGE OF THE MONTH – MESSIER 27 numerous membership benefits, including observing programs. This image of M27 (Dumbbell Nebula) was taken by Scott and Emily Wade and Deva Chatrathi. Scott writes, “Here’s an image of M27 Also, visit the NCRAL website at that was captured on the evenings of 6/23 (Emily & Scott) and 6/25 http://ncral.wordpress.com for in- (Deva & Scott) using the CDK 17” telescope with the QHY600 formation about our North Central camera and RGB filters. -
A Multispectral Assessment of Complex Impact Craters on the Lunar Farside
Western University Scholarship@Western Electronic Thesis and Dissertation Repository 2-15-2013 12:00 AM A Multispectral Assessment of Complex Impact Craters on the Lunar Farside Bhairavi Shankar The University of Western Ontario Supervisor Dr. Gordon R. Osinski The University of Western Ontario Graduate Program in Planetary Science A thesis submitted in partial fulfillment of the equirr ements for the degree in Doctor of Philosophy © Bhairavi Shankar 2013 Follow this and additional works at: https://ir.lib.uwo.ca/etd Part of the Geology Commons, Geomorphology Commons, Physical Processes Commons, and the The Sun and the Solar System Commons Recommended Citation Shankar, Bhairavi, "A Multispectral Assessment of Complex Impact Craters on the Lunar Farside" (2013). Electronic Thesis and Dissertation Repository. 1137. https://ir.lib.uwo.ca/etd/1137 This Dissertation/Thesis is brought to you for free and open access by Scholarship@Western. It has been accepted for inclusion in Electronic Thesis and Dissertation Repository by an authorized administrator of Scholarship@Western. For more information, please contact [email protected]. A MULTISPECTRAL ASSESSMENT OF COMPLEX IMPACT CRATERS ON THE LUNAR FARSIDE (Spine title: Multispectral Analyses of Lunar Impact Craters) (Thesis format: Integrated Article) by Bhairavi Shankar Graduate Program in Geology: Planetary Science A thesis submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy The School of Graduate and Postdoctoral Studies The University of Western Ontario London, Ontario, Canada © Bhairavi Shankar 2013 ii Abstract Hypervelocity collisions of asteroids onto planetary bodies have catastrophic effects on the target rocks through the process of shock metamorphism. The resulting features, impact craters, are circular depressions with a sharp rim surrounded by an ejecta blanket of variably shocked rocks. -
304 Index Index Index
_full_alt_author_running_head (change var. to _alt_author_rh): 0 _full_alt_articletitle_running_head (change var. to _alt_arttitle_rh): 0 _full_article_language: en 304 Index Index Index Adamson, Robert (1821–1848) 158 Astronomische Gesellschaft 216 Akkasbashi, Reza (1843–1889) viiii, ix, 73, Astrolog 72 75-78, 277 Astronomical unit, the 192-94 Airy, George Biddell (1801–1892) 137, 163, 174 Astrophysics xiv, 7, 41, 57, 118, 119, 139, 144, Albedo 129, 132, 134 199, 216, 219 Aldrin, Edwin Buzz (1930) xii, 244, 245, 248, Atlas Photographique de la Lune x, 15, 126, 251, 261 127, 279 Almagestum Novum viii, 44-46, 274 Autotypes 186 Alpha Particle Spectrometer 263 Alpine mountains of Monte Rosa and BAAS “(British Association for the Advance- the Zugspitze, the 163 ment of Science)” 26, 27, 125, 128, 137, Al-Biruni (973–1048) 61 152, 158, 174, 277 Al-Fath Muhammad Sultan, Abu (n.d.) 64 BAAS Lunar Committee 125, 172 Al-Sufi, Abd al-Rahman (903–986) 61, 62 Bahram Mirza (1806–1882) 72 Al-Tusi, Nasir al-Din (1202–1274) 61 Baillaud, Édouard Benjamin (1848–1934) 119 Amateur astronomer xv, 26, 50, 51, 56, 60, Ball, Sir Robert (1840–1913) 147 145, 151 Barlow Lens 195, 203 Amir Kabir (1807–1852) 71 Barnard, Edward Emerson (1857–1923) 136 Amir Nezam Garusi (1820–1900) 87 Barnard Davis, Joseph (1801–1881) 180 Analysis of the Moon’s environment 239 Beamish, Richard (1789–1873) 178-81 Andromeda nebula xii, 208, 220-22 Becker, Ernst (1843–1912) 81 Antoniadi, Eugène M. (1870–1944) 269 Beer, Wilhelm Wolff (1797–1850) ix, 54, 56, Apollo Missions NASA 32, 231, 237, 239, 240, 60, 123, 124, 126, 130, 139, 142, 144, 157, 258, 261, 272 190 Apollo 8 xii, 32, 239-41 Bell Laboratories 270 Apollo 11 xii, 59, 237, 240, 244-46, 248-52, Beg, Ulugh (1394–1449) 63, 64 261, 280 Bergedorf 207 Apollo 13 254 Bergedorfer Spektraldurchmusterung 216 Apollo 14 240, 253-55 Biancani, Giuseppe (n.d.) 40, 274 Apollo 15 255 Biot, Jean Baptiste (1774–1862) 1,8, 9, 121 Apollo 16 240, 255-57 Birt, William R. -
Fuor and Exor Variables: a NIR High-Resolution Spectroscopic Survey Joseph Liskowsky Clemson University, [email protected]
Clemson University TigerPrints All Theses Theses 12-2010 FUor and EXor Variables: A NIR High-Resolution Spectroscopic Survey Joseph Liskowsky Clemson University, [email protected] Follow this and additional works at: https://tigerprints.clemson.edu/all_theses Part of the Astrophysics and Astronomy Commons Recommended Citation Liskowsky, Joseph, "FUor and EXor Variables: A NIR High-Resolution Spectroscopic Survey" (2010). All Theses. 977. https://tigerprints.clemson.edu/all_theses/977 This Thesis is brought to you for free and open access by the Theses at TigerPrints. It has been accepted for inclusion in All Theses by an authorized administrator of TigerPrints. For more information, please contact [email protected]. FUor and EXor Variables, a NIR High-Resolution Spectroscopic Survey A Thesis Presented to the Graduate School of Clemson University In Partial Fulfillment of the Requirements for the Degree Master of Science Physics and Astronomy by Joseph Paul Liskowsky Dec 2010 Accepted by: Dr. Sean Brittain, Committee Chair Dr. Dieter Hartmann Dr. Mark Leising Dr. Bradley Meyer Abstract To better understand the labyrinth of heating and cooling processes in YSOs (young stellar objects), we study systems where there exists a large variability in the heating of this gas due to accretion. This research project focuses on several classes of early young eruptable T-Tauri stars, namely the FUors, the EXors and the so-called FU Ori-like, which all have the property of large amplitude oscillations in accretion rate. Each of these categories may well represent specific stages in early low-mass stellar evolution. While these objects have specific spectroscopic and circumstellar diagnostics (as means of identification) our research suggests that there are at least several objects that defy (typical) classification. -
Upper Darby High School, 601 N Lansdowne Ave, Drexel Hill, PA
Basalt Thickness of Mare Tranquillitatis using Two Methods Upper Darby High School, 601 N Lansdowne Ave, Drexel Hill, PA Gutama Biru, Chris DeMott, Galen Farmer, Daniel Gordon, Isabel Hunt, Kenneth Lin, Thomas Nguyen, Zach Thornton, Vince Tran, Most Yeasmin PROBLEM ISOPACH MAPS The purpose of this experiment is to evaluate two methods of calculating basalt thickness in Mare Tranquillitatis. Figure 1 is the original isopach map used for reference. Figures 2 and 3 are isopach maps made using 3DField software. INTRODUCTION Lunar maria are large impact craters or basins that have been filled with basalt. While the Moon was still cooling, lava seeped into these basins through cracks, cooling to form the maria. This study compares two methods of determining the thickness of basalt in Mare Tranquillitatis: the Pre-Mare Crater Method and the Post- Figure 2. Pre-Mare Crater Isopach Mare Crater Method. The first method uses craters from before the mare was formed and the latter uses craters from after the mare was formed, as the names imply. Previous work ( De HONs map reference) has been conducted using these methods to Figure 1. Reference Map (DeHon 1974) calculate mare thickness; however the tools used to collect that data are outdated. The current study, conducted using data from the Lunar Reconnaissance Orbiter and Clementine camera, compares the two methods for determining mare thickness. The Pre-Mare Crater Method used craters that were formed inside the large impact basins before they filled with lava. By measuring the diameter of these craters, the original rim height can be estimated using a relationship defined by Pike (1974, 1977).