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1 the Comets of Caroline Herschel (1750-1848)
Inspiration of Astronomical Phenomena, INSAP7, Bath, 2010 (www.insap.org) 1 publication: Culture and Cosmos, Vol. 16, nos. 1 and 2, 2012 The Comets of Caroline Herschel (1750-1848), Sleuth of the Skies at Slough Roberta J. M. Olson1 and Jay M. Pasachoff2 1The New-York Historical Society, New York, NY, USA 2Hopkins Observatory, Williams College, Williamstown, MA, USA Abstract. In this paper, we discuss the work on comets of Caroline Herschel, the first female comet-hunter. After leaving Bath for the environs of Windsor Castle and eventually Slough, she discovered at least eight comets, five of which were reported in the Philosophical Transactions of the Royal Society. We consider her public image, astronomers' perceptions of her contributions, and the style of her astronomical drawings that changed with the technological developments in astronomical illustration. 1. General Introduction and the Herschels at Bath Building on the research of Michael Hoskini and our book on comets and meteors in British art,ii we examine the comets of Caroline Herschel (1750-1848), the first female comet-hunter and the first salaried female astronomer (Figure 1), who was more famous for her work on nebulae. She and her brother William revolutionized the conception of the universe from a Newtonian one—i.e., mechanical with God as the great clockmaker watching over its movements—to a more modern view—i.e., evolutionary. Figure 1. Silhouette of Caroline Herschel, c. 1768, MS. Gunther 36, fol. 146r © By permission of the Oxford University Museum of the History of Science Inspiration of Astronomical Phenomena, INSAP7, Bath, 2010 (www.insap.org) 2 publication: Culture and Cosmos, Vol. -
Project Pan-STARRS and the Outer Solar System
Project Pan-STARRS and the Outer Solar System David Jewitt Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822 ABSTRACT Pan-STARRS, a funded project to repeatedly survey the entire visible sky to faint limiting magnitudes (mR ∼ 24), will have a substantial impact on the study of the Kuiper Belt and outer solar system. We briefly review the Pan- STARRS design philosophy and sketch some of the planetary science areas in which we expect this facility to make its mark. Pan-STARRS will find ∼20,000 Kuiper Belt Objects within the first year of operation and will obtain accurate astrometry for all of them on a weekly or faster cycle. We expect that it will revolutionise our knowledge of the contents and dynamical structure of the outer solar system. Subject headings: Surveys, Kuiper Belt, comets 1. Introduction to Pan-STARRS Project Pan-STARRS (short for Panoramic Survey Telescope and Rapid Response Sys- tem) is a collaboration between the University of Hawaii's Institute for Astronomy, the MIT Lincoln Laboratory, the Maui High Performance Computer Center, and Science Ap- plications International Corporation. The Principal Investigator for the project, for which funding started in the fall of 2002, is Nick Kaiser of the Institute for Astronomy. Operations should begin by 2007. The science objectives of Pan-STARRS span the full range from planetary to cosmolog- ical. The instrument will conduct a survey of the solar system that is staggering in power compared to anything yet attempted. A useful measure of the raw survey power, SP , of a telescope is given by AΩ SP = (1) θ2 where A [m2] is the collecting area of the telescope primary, Ω [deg2] is the solid angle that is imaged and θ [arcsec] is the full-width at half maximum (FWHM) of the images { 2 { produced by the telescope. -
Ice & Stone 2020
Ice & Stone 2020 WEEK 17: APRIL 19-25, 2020 Presented by The Earthrise Institute # 17 Authored by Alan Hale This week in history APRIL 19 20 21 22 23 24 25 APRIL 20, 1910: Comet 1P/Halley passes through perihelion at a heliocentric distance of 0.587 AU. Halley’s 1910 return, which is described in a previous “Special Topics” presentation, was quite favorable, with a close approach to Earth (0.15 AU) and the exhibiting of the longest cometary tail ever recorded. APRIL 20, 2025: NASA’s Lucy mission is scheduled to pass by the main belt asteroid (52246) Donaldjohanson. Lucy is discussed in a previous “Special Topics” presentation. APRIL 19 20 21 22 23 24 25 APRIL 21, 2024: Comet 12P/Pons-Brooks is predicted to pass through perihelion at a heliocentric distance of 0.781 AU. This comet, with a discussion of its viewing prospects for 2024, is a previous “Comet of the Week.” APRIL 19 20 21 22 23 24 25 APRIL 22, 2020: The annual Lyrid meteor shower should be at its peak. Normally this shower is fairly weak, with a peak rate of not much more than 10 meteors per hour, but has been known to exhibit significantly stronger activity on occasion. The moon is at its “new” phase on April 23 this year and thus the viewing circumstances are very good. COVER IMAGE CREDIT: Front and back cover: This artist’s conception shows how families of asteroids are created. Over the history of our solar system, catastrophic collisions between asteroids located in the belt between Mars and Jupiter have formed families of objects on similar orbits around the sun. -
Symposium on Telescope Science
Proceedings for the 26th Annual Conference of the Society for Astronomical Sciences Symposium on Telescope Science Editors: Brian D. Warner Jerry Foote David A. Kenyon Dale Mais May 22-24, 2007 Northwoods Resort, Big Bear Lake, CA Reprints of Papers Distribution of reprints of papers by any author of a given paper, either before or after the publication of the proceedings is allowed under the following guidelines. 1. The copyright remains with the author(s). 2. Under no circumstances may anyone other than the author(s) of a paper distribute a reprint without the express written permission of all author(s) of the paper. 3. Limited excerpts may be used in a review of the reprint as long as the inclusion of the excerpts is NOT used to make or imply an endorsement by the Society for Astronomical Sciences of any product or service. Notice The preceding “Reprint of Papers” supersedes the one that appeared in the original print version Disclaimer The acceptance of a paper for the SAS proceedings can not be used to imply or infer an endorsement by the Society for Astronomical Sciences of any product, service, or method mentioned in the paper. Published by the Society for Astronomical Sciences, Inc. First printed: May 2007 ISBN: 0-9714693-6-9 Table of Contents Table of Contents PREFACE 7 CONFERENCE SPONSORS 9 Submitted Papers THE OLIN EGGEN PROJECT ARNE HENDEN 13 AMATEUR AND PROFESSIONAL ASTRONOMER COLLABORATION EXOPLANET RESEARCH PROGRAMS AND TECHNIQUES RON BISSINGER 17 EXOPLANET OBSERVING TIPS BRUCE L. GARY 23 STUDY OF CEPHEID VARIABLES AS A JOINT SPECTROSCOPY PROJECT THOMAS C. -
Blood-Horse Directory
THE PAMPLEMOUSSE gr/ro, 2006 height 16.2 Dosage (3-2-10-1-0); DI: 1.67; CD: 0.44 See gray pages—Nasrullah RACE AND (BLACK TYPE) RECORD Runaway Groom, 1979 Blushing Groom, by Red God Age Starts 1st 2nd 3rd Earned 18s, BTW, $347,537 Cherokee Run, 1990 1,122 f, 72 BTW, 1.53 AEI Yonnie Girl, by Call the Witness 2 3 1 0 1 $29,280 28s, BTW, $1,531,818 3 2 2(2) 0 0 $180,000 807 f, 49 BTW, 1.48 AEI Cherokee Dame, 1980 Silver Saber, by Drone Totals 5 3(2) 0 1 $209,280 Kafwain, dkb/br, 2000 Unraced 11s, BTW, $715,848 7 f, 6 r, 6 w, 1 BTW Dame Francesca, by Francis S. Won At 2 563 f, 19 BTW, 1.06 AEI Moment of Hope, 1983 Timeless Moment, by Damascus A maiden special weight race at Hol ($49,700, 8.5f, 6.47 AWD 23s, BTW, $406,222 AW in 1:41.43, by 23/4, dftg. Mayor Marv, Fiery Swazi's Moment, 1990 266 f, 6 BTW, 0.91 AEI Careless Moment, by Baffle Rebel, Mr. Holmes, Life Goes On, Lifeline, Mr. Hot 11s, BTW, $176,255 Stuff, Personality Kid, Mickey Rocks). 10 f, 7 r, 5 w, 1 BTW Swazi Girl, 1980 Hatchet Man, by The Axe II 28s, BTW, $118,660 Won At 3 6 f, 6 r, 4 w, 1 BTW Our Duckling, by Quack Sham S (G3A, $200,000, 9f in 1:47.86, by 6, dftg. Take the Points, Mr. -
Perturbation of the Oort Cloud by Close Stellar Encounter with Gliese 710
Bachelor Thesis University of Groningen Kapteyn Astronomical Institute Perturbation of the Oort Cloud by Close Stellar Encounter with Gliese 710 August 5, 2019 Author: Rens Juris Tesink Supervisors: Kateryna Frantseva and Nickolas Oberg Abstract Context: Our Sun is thought to have an Oort cloud, a spherically symmetric shell of roughly 1011 comets orbiting with semi major axes between ∼ 5 × 103 AU and 1 × 105 AU. It is thought to be possible that other stars also possess comet clouds. Gliese 710 is a star expected to have a close encounter with the Sun in 1.35 Myrs. Aims: To simulate the comet clouds around the Sun and Gliese 710 and investigate the effect of the close encounter. Method: Two REBOUND N-body simulations were used with the help of Gaia DR2 data. Simulation 1 had a total integration time of 4 Myr, a time-step of 1 yr, and 10,000 comets in each comet cloud. And Simulation 2 had a total integration time of 80,000 yr, a time-step of 0.01 yr, and 100,000 comets in each comet cloud. Results: Simulation 2 revealed a 1.7% increase in the semi-major axis at time of closest approach and a population loss of 0.019% - 0.117% for the Oort cloud. There was no statistically significant net change of the inclination of the comets during this encounter and a 0.14% increase in the eccentricity at the time of closest approach. Contents 1 Introduction 3 1.1 Comets . .3 1.2 New comets and the Oort cloud . .5 1.3 Structure of the Oort cloud . -
Week 5: January 26-February 1, 2020
5# Ice & Stone 2020 Week 5: January 26-February 1, 2020 Presented by The Earthrise Institute About Ice And Stone 2020 It is my pleasure to welcome all educators, students, topics include: main-belt asteroids, near-Earth asteroids, and anybody else who might be interested, to Ice and “Great Comets,” spacecraft visits (both past and Stone 2020. This is an educational package I have put future), meteorites, and “small bodies” in popular together to cover the so-called “small bodies” of the literature and music. solar system, which in general means asteroids and comets, although this also includes the small moons of Throughout 2020 there will be various comets that are the various planets as well as meteors, meteorites, and visible in our skies and various asteroids passing by Earth interplanetary dust. Although these objects may be -- some of which are already known, some of which “small” compared to the planets of our solar system, will be discovered “in the act” -- and there will also be they are nevertheless of high interest and importance various asteroids of the main asteroid belt that are visible for several reasons, including: as well as “occultations” of stars by various asteroids visible from certain locations on Earth’s surface. Ice a) they are believed to be the “leftovers” from the and Stone 2020 will make note of these occasions and formation of the solar system, so studying them provides appearances as they take place. The “Comet Resource valuable insights into our origins, including Earth and of Center” at the Earthrise web site contains information life on Earth, including ourselves; about the brighter comets that are visible in the sky at any given time and, for those who are interested, I will b) we have learned that this process isn’t over yet, and also occasionally share information about the goings-on that there are still objects out there that can impact in my life as I observe these comets. -
Collecting Expensive Wines It Has Been Said That Life Is Too Short to Be Drinking Bad Wine
AMBROSIA COLLECTING EXPENSIVE WINES It has been said that life is too short to be drinking bad wine. Suneeta Sodhi Kanga agrees and gives you a taste of the world’s best wines HE mystery of wines never ceases to amaze and fascinate people. amount of fruit make better wines because there is a greater concentration Since the beginning of time, man has been attracted to things of flavour in the grapes. Sometimes these come from small parcels of land that are hard to find. Rare wines are as coveted as any other that are in high demand like Burgundy for example. It is the smallest wine treasure. Collecting expensive wines can yield great pleasures region in the world but commands very high prices. Twhether you long to hold in your hands a piece of wine history, make a The History of the Chateau: Chateaux that have a reputation of few thousand dollars by auctioning a great buy, or simply enjoy one of the consistently producing wines of top notch standard even in weaker world’s most beloved elixirs with like-minded connoisseurs. vintages command higher prices. Popularity of the wine maker and family Just as no one factor makes up the taste of wine, it is a highly personal reputation also matter. For example, Rothschild in Bordeaux and Famille combination of internal and external forces that determines price also. In Perrin in the Rhone Valley. a way, it is those very factors that make the wine market as dynamic and Wine making techniques: Wine making techniques like ageing of the exciting as it is today. -
Extremely Low Linear Polarization of Comet C/2018 V1 (Machholz–Fujikawa–Iwamoto)
Extremely low linear polarization of comet C/2018 V1 (Machholz–Fujikawa–Iwamoto) Evgenij Zubko a,*, Ekaterina Chornaya b,c, Maxim Zheltobryukhov c, Alexey Matkin c, d,e,f g Oleksandra V. Ivanova , Dennis Bodewits , Anton Kochergin b,c, Gennady Kornienko c, Igor Luk’yanyk d, Dean C. Hines h, Gorden Videen i,j a Humanitas College, Kyung Hee University, 1732, Deogyeong-daero, Giheung-gu, Yongin-si, Gyeonggi-do 17104, South Korea b Far Eastern Federal University, 8 Sukhanova St., Vladivostok 690950, Russia c Institute of Applied Astronomy of RAS, 10 Kutuzova Emb., Saint-Petersburg 191187, Russia d Astronomical Observatory, Taras Shevchenko National University of Kyiv, 3 Observatorna St., Kyiv, 04053, Ukraine e Astronomical Institute of the Slovak Academy of Sciences, SK-05960 Tatranska� Lomnica, Slovak Republic f Main Astronomical Observatory of National Academy of Sciences, 27 Akademika Zabolotnoho St., Kyiv, 03143, Ukraine g Auburn University, Physics Department, Auburn, AL 36849-5319, USA h Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA i Space Science Institute, 4750 Walnut Street, Boulder Suite 205, CO 80301, USA j Department of Astronomy and Space Science, Kyung Hee University, 1732, Deogyeong-daero, Giheung-gu, Yongin-si, Gyeonggi-do 17104, South Korea We measured the degree of linear polarization P of comet C/2018 V1 (Machholz-Fujikawa-Iwamoto) with the broadband Johnson V filter in mid-November of 2018. � � Within a radius of ρ � 17,000 km of the inner coma, we detected an extremely low linear polarization at phase angles α � 83 –91.2 and constrained the polarization maximum to Pmax � (6.8 � 1.8)%. -
A Search for the Origin of the Interstellar Comet 2I/Borisov
A&A 634, A14 (2020) Astronomy https://doi.org/10.1051/0004-6361/201937231 & © C. A. L. Bailer-Jones et al. 2020 Astrophysics A search for the origin of the interstellar comet 2I/Borisov Coryn A. L. Bailer-Jones1, Davide Farnocchia2, Quanzhi Ye ( )3, Karen J. Meech4, and Marco Micheli5,6 1 Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany e-mail: [email protected] 2 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA 3 Department of Astronomy, University of Maryland, College Park, MD 20742, USA 4 Institute for Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA 5 ESA NEO Coordination Centre, Largo Galileo Galilei 1, 00044 Frascati (RM), Italy 6 INAF – Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monte Porzio Catone (RM), Italy Received 2 December 2019 / Accepted 30 December 2019 ABSTRACT The discovery of the second interstellar object 2I/Borisov on 2019 August 30 raises the question of whether it was ejected recently from a nearby stellar system. Here we compute the asymptotic incoming trajectory of 2I/Borisov, based on both recent and pre-discovery data extending back to December 2018, using a range of force models that account for cometary outgassing. From Gaia DR2 astrometry and radial velocities, we trace back in time the Galactic orbits of 7.4 million stars to look for close encounters with 2I/Borisov. The closest encounter we find took place 910 kyr ago with the M0V star Ross 573, at a separation of 0.068 pc (90% confidence interval 1 of 0.053–0.091 pc) with a relative velocity of 23 km s− . -
Nucleus, Neutral and Ionized Coma of Comets 67P/Churyumov-Gerasimenko and 46P/Wirtanen Preparations for the ROSETTA Radio Science Investigations
Global modeling of comets: Nucleus, neutral and ionized coma of comets 67P/Churyumov-Gerasimenko and 46P/Wirtanen Preparations for the ROSETTA Radio Science Investigations I NAUGURAL –D ISSERTATION ZUR ERLANGUNG DES DOKTORGRADES DER MATHEMATISCH–NATURWISSENSCHAFTLICHEN FAKULTAT¨ DER UNIVERSITAT¨ ZU KOLN¨ VORGELEGT VON JORG¨ VON OERTZEN AUS BOBLINGEN¨ KOLN¨ 2003 Berichterstatter: Prof. Dr. F. M. Neubauer Hochsch.-Doz. Dr. M. Patzold¨ Tag der mundlichen¨ Prufung:¨ 4.Dezember2003 Contents 1 Introduction 1 1.1 Kurzzusammenfassung . 1 1.2 Abstract..................................... 3 1.3 Motivation.................................... 4 1.4 Cometarymissions ............................... 5 2 The ROSETTA mission 7 2.1 TheROSETTA Spacecraft............................ 7 2.2 RadioScienceInvestigations . .... 8 2.2.1 ScientificObjectives . .. .. .. .. .. .. .. 8 2.2.2 RadioSubsystem............................ 8 2.3 OtherExperiments ............................... 9 3 Possible Target Comets 11 3.1 46P/Wirtanen .................................. 11 3.2 67P/Churyumov-Gerasimenko . .. 11 3.3 OrbitalElements ................................ 12 3.4 TimelineandGeometricConsiderations . ...... 12 4 Thermal model of a cometary nucleus 15 II CONTENTS 4.1 Introduction................................... 15 4.2 TheCometaryNucleus ............................. 16 4.2.1 ObservationsofCometaryNuclei . 16 4.2.2 Structure ................................ 16 4.2.3 Composition .............................. 17 4.2.4 Albedo ................................. 19 4.2.5 -
November 2020
DOOT Quarterly Magazine of the Indian Institute of Astrophysics Issue 2 November 2020 IIA Publication No.: IIA/Pub/DOOT/2020/Nov/002 Editors’ Panel Sandeep Kataria (Chief Editor) Content Team Fazlu Rahman, Partha Pratim Goswami, Raveena Khan, Soumya Sengupta, Suman Saha, S.V. Manoj Varma, Vishnu Madhu Design Team Anand M N, Arumugam Pitchai, Manika Singla, Prasanna Deshmukh, Rishabh Singh Teja Advisers Dr. Maheswar Gopinathan Dr. Piyali Chatterjee FAIR USE DISCLAIMER The primary intent of this magazine is for Non-profit, Education and Outreach purpose. The material used in this Magazine may be Copyright protected. Wherever possible permissions are obtained from the respective content owners. Appropriate credits are provided to the Owner & Original Source. DOOT Indian Institute of Astrophysics QUARTERLYDOOT MAGAZINE OF THE INDIAN INSTITUTE OF ASTROPHYSICS Invitation For The Next Issue For the next issue of DOOT, we are inviting your contributions under the following categories: Review Articles: Scientific and technical publications (recent publications in academic journals from the IIA family, IIA technical reports, breakthroughs in Astronomy, book review, Journal club discussions, milestones of IIA projects; to be published in simple language) are invited. Project interns and summer school project students can submit an overview of their work. (Word limit: 2000 words) Individual Experiences And Substation Stories: In this section, we invite stories of your personal experience, maybe with a scientific project, an experiment, attending a conference/workshop, a collaborative visit, visit to an observatory, or even a coffee break with a prominent scientist. We also invite interesting stories from our substations at Hanle, Kodaikanal, Kavalur, and Gauribidanur about the ongoing activities and valuable memories.