King David's Altar in Jerusalem Dated by the Bright Appearance of Comet
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The Comet's Tale, and Therefore the Object As a Whole Would the Section Director Nick James Highlighted Have a Low Surface Brightness
1 Diebold Schilling, Disaster in connection with two comets sighted in 1456, Lucerne Chronicle, 1513 (Wikimedia Commons) THE COMET’S TALE Comet Section – British Astronomical Association Journal – Number 38 2019 June britastro.org/comet Evolution of the comet C/2016 R2 (PANSTARRS) along a total of ten days on January 2018. Composition of pictures taken with a zoom lens from Teide Observatory in Canary Islands. J.J Chambó Bris 2 Table of Contents Contents Author Page 1 Director’s Welcome Nick James 3 Section Director 2 Melvyn Taylor’s Alex Pratt 6 Observations of Comet C/1995 01 (Hale-Bopp) 3 The Enigma of Neil Norman 9 Comet Encke 4 Setting up the David Swan 14 C*Hyperstar for Imaging Comets 5 Comet Software Owen Brazell 19 6 Pro-Am José Joaquín Chambó Bris 25 Astrophotography of Comets 7 Elizabeth Roemer: A Denis Buczynski 28 Consummate Comet Section Secretary Observer 8 Historical Cometary Amar A Sharma 37 Observations in India: Part 2 – Mughal Empire 16th and 17th Century 9 Dr Reginald Denis Buczynski 42 Waterfield and His Section Secretary Medals 10 Contacts 45 Picture Gallery Please note that copyright 46 of all images belongs with the Observer 3 1 From the Director – Nick James I hope you enjoy reading this issue of the We have had a couple of relatively bright Comet’s Tale. Many thanks to Janice but diffuse comets through the winter and McClean for editing this issue and to Denis there are plenty of images of Buczynski for soliciting contributions. 46P/Wirtanen and C/2018 Y1 (Iwamoto) Thanks also to the section committee for in our archive. -
How We Found About COMETS
How we found about COMETS Isaac Asimov Isaac Asimov is a master storyteller, one of the world’s greatest writers of science fiction. He is also a noted expert on the history of scientific development, with a gift for explaining the wonders of science to non- experts, both young and old. These stories are science-facts, but just as readable as science fiction.Before we found out about comets, the superstitious thought they were signs of bad times ahead. The ancient Greeks called comets “aster kometes” meaning hairy stars. Even to the modern day astronomer, these nomads of the solar system remain a puzzle. Isaac Asimov makes a difficult subject understandable and enjoyable to read. 1. The hairy stars Human beings have been watching the sky at night for many thousands of years because it is so beautiful. For one thing, there are thousands of stars scattered over the sky, some brighter than others. These stars make a pattern that is the same night after night and that slowly turns in a smooth and regular way. There is the Moon, which does not seem a mere dot of light like the stars, but a larger body. Sometimes it is a perfect circle of light but at other times it is a different shape—a half circle or a curved crescent. It moves against the stars from night to night. One midnight, it could be near a particular star, and the next midnight, quite far away from that star. There are also visible 5 star-like objects that are brighter than the stars. -
Small Bodies of the Solar System Don Yeomans
news and views teakre Small bodies of the Solar System Don Yeomans ,-.......-..-.- "_.."..._..".."....".._..I........... ".........._ "_.""".." ".......... " "............_..._.." ....".."-..- ..-.... "....""... Discoveries of comets that behave like asteroids and asteroids that behave like comets are making us reassess our view of Earth's smallest neighbours. cientists have a strong urge to place Mother Nature's objects into neat Sboxes. For most of the past halfcentury, the comets and asteroids of the Solar System did seem to belong in two separate popula- tions -each within their own box. The rules werethatcomets,withawiderangeoforbits, were solid, dirty iceballs originating in the so-called Oort cloud at theedge of the Solar System. Asteroids were definedas bitsofrock anfimed mostly to a region between Mars and Jupiter and travelling roughly in the same plane and inthe same direction as the planets about theSun (Fig. 1).Fromtjme to Lime over the past 50 years, objects were bund that did not really belong in either )OX, but they were onlyconsidered as occa- iional exceptions to the rules. Within the Figure 1 The usual view of corneta and utcroida. The inna Soh System cuntlinr the Sun and the ,ast few years, however,Mother Nature has four terreatrid planar:Mercury, Venu%Euth and Ma.fie lump of mdc that make up thenuin ticked over the boxes entirely, spilling the asteroid bdt between him and Jupiterorbit the Sun in the meplane andthe medirection PJ the :ontents and demanding thatscientists rec- planets. Most tometa have highly dlipticnl orbits, whichmeans they spend most of their timein the )gnizE crossover objects - asteroids that outer reache of the Solar System with only briefpasages dose to the Sun. -
The Comet's Tale
THE COMET’S TALE Journal of the Comet Section of the British Astronomical Association Number 33, 2014 January Not the Comet of the Century 2013 R1 (Lovejoy) imaged by Damian Peach on 2013 December 24 using 106mm F5. STL-11k. LRGB. L: 7x2mins. RGB: 1x2mins. Today’s images of bright binocular comets rival drawings of Great Comets of the nineteenth century. Rather predictably the expected comet of the century Contents failed to materialise, however several of the other comets mentioned in the last issue, together with the Comet Section contacts 2 additional surprise shown above, put on good From the Director 2 appearances. 2011 L4 (PanSTARRS), 2012 F6 From the Secretary 3 (Lemmon), 2012 S1 (ISON) and 2013 R1 (Lovejoy) all Tales from the past 5 th became brighter than 6 magnitude and 2P/Encke, 2012 RAS meeting report 6 K5 (LINEAR), 2012 L2 (LINEAR), 2012 T5 (Bressi), Comet Section meeting report 9 2012 V2 (LINEAR), 2012 X1 (LINEAR), and 2013 V3 SPA meeting - Rob McNaught 13 (Nevski) were all binocular objects. Whether 2014 will Professional tales 14 bring such riches remains to be seen, but three comets The Legacy of Comet Hunters 16 are predicted to come within binocular range and we Project Alcock update 21 can hope for some new discoveries. We should get Review of observations 23 some spectacular close-up images of 67P/Churyumov- Prospects for 2014 44 Gerasimenko from the Rosetta spacecraft. BAA COMET SECTION NEWSLETTER 2 THE COMET’S TALE Comet Section contacts Director: Jonathan Shanklin, 11 City Road, CAMBRIDGE. CB1 1DP England. Phone: (+44) (0)1223 571250 (H) or (+44) (0)1223 221482 (W) Fax: (+44) (0)1223 221279 (W) E-Mail: [email protected] or [email protected] WWW page : http://www.ast.cam.ac.uk/~jds/ Assistant Director (Observations): Guy Hurst, 16 Westminster Close, Kempshott Rise, BASINGSTOKE, Hampshire. -
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. -
45-68 Verdun
| The Determination of the Solar Parallax from Transits of Venus in the 18th Century | 45 | The Determination of the Solar Parallax from Transits of Venus in the 18 th Century Andreas VERDUN * Manuscript received September 28, 200 4, accepted October 30, 2004 T Abstract The transits of Venus in 1761 and 1769 initiated the first global observation campaigns performed with international cooperation. The goal of these campaigns was the determination of the solar parallax with high precision. Enormous efforts were made to send expeditions to the most distant and then still unknown regions of the Earth to measure the instants of contact of the transits. The determination of the exact value of the solar parallax from these observations was not only of scientific importance, but it was expected to improve the astronomical tables which were used, e.g., for naviga - tion. Hundreds of single measurements were acquired. The astronomers, however, were faced by a new problem: How is such a small quantity like the solar parallax to be derived from observations deteriorated by measuring errors? Is it possible to determine the solar parallax with an accuracy of 0.02" as asserted by Halley? Only a few scientists accepted this chal - lenge, but without adequate processing methods this was a hopeless undertaking. Parameter estimation methods had to be developed at first. The procedures used by Leonhard Euler and Achille-Pierre Dionis Duséjour were similar to modern methods and therefore superior to all other traditional methods. Their results were confirmed by Simon Newcomb at the end of the 1 9th century, thus proving the success of these campaigns. -
Southwest Florida Astronomical Society SWFAS the Eyepiece
Southwest Florida Astronomical Society SWFAS The Eyepiece February 2017 Contents: Message from the President .............................................................................. Page 1 Program this Month ......................................................................................... Page 2 Photos by Chuck and Matthew ........................................................................... Page 2 In the Sky this Month ...................................................................................... Page 3 Future Events ................................................................................................. Page 4 Bright Comet Prospects for 2017 ........................................................................ Page 6 Comet Campaign: Amateurs Wanted? ................................................................ Page 14 Club Officers & Positions .................................................................................. Page 16 A MESSAGE FROM THE PRESIDENT I hope everyone is having a good new year. We are now into our heaviest period for public events. On the 11th we have STEMtastic/Edison Day of Discovery downtown. On the 25th we will be at Rotary Park in Cape Coral for the Burrowing Owl Festival. Both of these events are solar observing and displays/handouts. We can use help with these events. You don’t need to bring a scope or even be familiar with solar observing. There is a lot of public interaction and we need people for that. As a followup to the BOF, we will have a public star -
Gotthold Eisenstein and Philosopher John
Gotthold Eisenstein and Philosopher John Franz Lemmermeyer Abstract Before the recent publication of the correspondence between Gauss and Encke, nothing was known about the role that John Taylor, a cotton merchant from Liverpool, had played in the life of Gotthold Eisenstein. In this article, we will bring together what we have discovered about John Taylor’s life. Eisenstein’s Journey to England Gotthold Eisenstein belonged, together with Dirichlet, Jacobi and Kummer, to the generation after Gauss that shaped the theory of numbers in the mid- 19th century, and like Galois, Abel, Riemann, Roch and Clebsch, Eisenstein died young. Today, Eisenstein’s name can be found in the Eisenstein series, Eisenstein sums, the Eisenstein ideal, Eisenstein’s reciprocity law and in his irreducibility criterion, and he is perhaps best known for his ingenious proofs of the quadratic, cubic and biquadratic reciprocity laws. Eisenstein’s father Jo- hann Konstantin Eisenstein emigrated to England in 1840; Eisenstein and his mother followed in June 1842, although Eisenstein’s few remarks on this episode in his autobiography [3] belie the dramatic events that he experienced in Eng- land. On their journey to England, the Eisensteins passed through Hamburg; during the Great Fire in May 1842 about a third of the houses in the Altstadt had burned down. What we learn from Eisenstein’s account is that he was impressed by the sight of railroad lines running right under the foundations of houses (in London?) and by the Menai suspension bridge in Wales: Eisenstein mentions that he undertook six sea voyages, and that on one of them they sailed arXiv:2101.03344v1 [math.HO] 9 Jan 2021 under the tremendous suspension bridge in Anglesey, which was so high that the Berlin Palace would easily have fitted under its main arch. -
Some Graphical Solutions of the Kepler Problem
Some Graphical Solutions of the Kepler Problem Marc Frantz 1. INTRODUCTION. When a particle P moves in an inverse square acceleration field, its orbit is a conic section. If the acceleration is repulsive?that is, of the form /x||FP ||~3Fr for a positive constant ?jland a fixed point F?then the orbit is a branch of a hyperbola with F at the focus on the convex side of the branch. If the acceleration is attractive (?/x||TP\\~3FP), then the orbit is a circle with F at the center, an ellipse or parabola with F at a focus, or a branch of a hyperbola with F at the focus on the concave side of the branch. We refer to such orbits as Keplerian orbits after Johannes Kepler, who proposed them as models of planetary motion. It takes rather special conditions to set up circular or parabolic orbits, so it is proba bly safe to say that inNature most closed orbits are ellipses, and most nonclosed orbits are hyperbolas. Ironically, these are precisely the cases in which it is impossible to formulate the position of P as an elementary function of time t?the very thing we most want to know! Nevertheless, for any given time t it is possible to locate P using graphs of elemen tary functions, thereby achieving a partial victory. This endeavor has an interesting history in the case of elliptical orbits, where locating P is called the "Kepler problem." It involves a famous equation known as "Kepler's equation," which we discuss later. In his book Solving Kepler's Equation over Three Centuries Peter Colwell says [5, p. -
(Preprint) AAS 16-112 ENCKE-BETA PREDICTOR for ORION BURN
(Preprint) AAS 16-112 ENCKE-BETA PREDICTOR FOR ORION BURN TARGETING AND GUIDANCE Shane Robinson,∗ Sara Scarritt,∗ and John L. Goodmany The state vector prediction algorithm selected for Orion on-board targeting and guidance is known as the Encke-Beta method. Encke-Beta uses a universal anomaly (beta) as the independent variable, valid for circular, elliptical, parabolic, and hy- perbolic orbits. The variable, related to the change in eccentric anomaly, results in integration steps that cover smaller arcs of the trajectory at or near perigee, when velocity is higher. Some burns in the EM-1 and EM-2 mission plans are much longer than burns executed with the Apollo and Space Shuttle vehicles. Burn length, as well as hyperbolic trajectories, has driven the use of the Encke-Beta nu- merical predictor by the predictor/corrector guidance algorithm in place of legacy analytic thrust and gravity integrals. INTRODUCTION On-board software tasks for on-orbit burn targeting, guidance, and navigation require the use of trajectory integrators to predict state vectors forward or backward in time. Burn targeting meth- ods and active guidance routines make extensive use of trajectory prediction algorithms. These predictions may be over time intervals ranging from tens of seconds to hours or even days. Such predictions require higher fidelity numerical integration schemes and higher order acceleration mod- els than very short time interval propagations cyclically executed at high rates, such as those found in the propagation phase of an on-board Kalman filter. A high fidelity state vector predictor may also be used to predict a state vector uplinked by Mission Control forward or backward in time to the current on-board time, so that the high rate short time interval propagator can be reinitialized. -
02. Solar System (2001) 9/4/01 12:28 PM Page 2
01. Solar System Cover 9/4/01 12:18 PM Page 1 National Aeronautics and Educational Product Space Administration Educators Grades K–12 LS-2001-08-002-HQ Solar System Lithograph Set for Space Science This set contains the following lithographs: • Our Solar System • Moon • Saturn • Our Star—The Sun • Mars • Uranus • Mercury • Asteroids • Neptune • Venus • Jupiter • Pluto and Charon • Earth • Moons of Jupiter • Comets 01. Solar System Cover 9/4/01 12:18 PM Page 2 NASA’s Central Operation of Resources for Educators Regional Educator Resource Centers offer more educators access (CORE) was established for the national and international distribution of to NASA educational materials. NASA has formed partnerships with universities, NASA-produced educational materials in audiovisual format. Educators can museums, and other educational institutions to serve as regional ERCs in many obtain a catalog and an order form by one of the following methods: States. A complete list of regional ERCs is available through CORE, or electroni- cally via NASA Spacelink at http://spacelink.nasa.gov/ercn NASA CORE Lorain County Joint Vocational School NASA’s Education Home Page serves as a cyber-gateway to informa- 15181 Route 58 South tion regarding educational programs and services offered by NASA for the Oberlin, OH 44074-9799 American education community. This high-level directory of information provides Toll-free Ordering Line: 1-866-776-CORE specific details and points of contact for all of NASA’s educational efforts, Field Toll-free FAX Line: 1-866-775-1460 Center offices, and points of presence within each State. Visit this resource at the E-mail: [email protected] following address: http://education.nasa.gov Home Page: http://core.nasa.gov NASA Spacelink is one of NASA’s electronic resources specifically devel- Educator Resource Center Network (ERCN) oped for the educational community. -
Encke's Minima and Encke's Division in Saturn's A-Ring
ENCKE’S MINIMA AND ENCKE’S DIVISION IN SATURN’S A-RING Pedro Ré http://astrosurf.com/re When viewed with the aid of a good quality telescope Saturn is undoubtedly one of the most spectacular objects in the sky. Many amateur astronomers (including the author) say that their first observation of Saturn turned them on to astronomy. Saturn’s rings are easily visible with a good 60 mm refractor at 50x. The 3D appearance of this planet is what makes it so interesting. Details in the rings can be seen during moments of good seeing. The Cassini division (between ring A and B) is easily visible with moderate apertures. The Encke minima and Encke division are more difficult to observe and require large apertures and telescopes of excellent optical quality. These two features can be observed in Saturn’s A-Ring. The Encke minima consists of a broad, low contrast feature located about halfway out in the middle of the A-Ring. The Encke division is a narrow, high contrast feature located near the outer edge of the A-Ring. Unlike the Encke minima, the Encke division is an actual division of the ring (Figure 1). Figure 1- Saturn near Opposition on June 11, 2017. D. Peach, E. Kraaikamp, F. Colas, M. Delcroix, R. Hueso, G. Thérin, C. Sprianu, S2P, IMCCE, OMP. The Encke division is visible around the entire outer A ring. Astronomy Picture of the Day (20170617) https://apod.nasa.gov/apod/ap170617.html 1 Galileo Galilei observed the disk Saturn for the first time using one of his largest refractor.