Solar System Litho! IS~~SOIII\3 for Earth and Space Science

Total Page:16

File Type:pdf, Size:1020Kb

Solar System Litho! IS~~SOIII\3 for Earth and Space Science Educational Product EaTeachers Grades K-12 NASA-EP-33 8 Solar System Litho! IS~~SOIII\3 for Earth and Space Science This set contains the following materials: Our Star-The Sun Mercury Venus Earth Moon Mars Jupiter Saturn Uranus Neptune Pluto Asteroids: Ida with Moon and Gaspra (Inset) NASA Resources for Educators Electronic Resources for Educators National Aeronautics and Our Star - The Sun @ Space Administration Our Star The Sun 7 National Aeronautics and - Space Administration v The Sun is a huge, bright sphere of mostly ionized gas the Sun. Temperature steadily increases with altitude degrees K. The process that heats the corona is.very about 5billionyears old. The closest star to Earth, it is 16 up to 50,000 K, while density drops to 100,000 times mysterious and poorly understood, since the laws of million km distant (this distance is called an Astronomi- less than in the photosphere. Above thechromosphere thermodynamics state that heat energy flows from a cal Unit). The next closest star is 300,000 times further lies the corora ("crown"), extending outward from the hotter to a cooler place. Mysterious phenomena, such away. There are probably millions of similar stars in the Sun in the form of the "solar wind" to the edge of the as this, are studied by researchers in NASA's Space Milky Way galaxy (and even more galaxies in the Uni- solar system. The corora is extremely hot -millions of Physics Division. vem), but the Sun is the most important to us because it supports life on Earth. It powers photosynthesis in green plants and is ultimately the source of all food and fossil fuel. The Sun's power causes the seasons, the climate, the Fast Facts SignmCant Dates cumnts in the ocean, the circulation of the air, and the weather in the atmosphere. Spectral Type of Star G2 V 585 BC First solar eclipse successfully predicted The Sun is some 333,400 times more massive than 1610 Galileoobservessunspdswithhistelescope 4.5 Billion Years Earth (mass= 1.99 x 1030 kg), and contains99.86% of the Age 1650-1715 Maunder Sunspot Minimum discovered mass of the entire solar system. It is held together by Mean Distance to Earth 150 Million Kilometers 1854 Fust connectionmade between solar activity gravitational attraction, producing immense pressure Rotation Period (at equator) 26.8 days andgeomagneticactivity and temperature at its core (more than a billion times Radius 695poO Kilometers Helium lines first observed in solar spectrum that of the atmosphere on Earth, and a density about First measurenent of of magnetic fields 160 times that of water). Mass 1.99 x 1030 Kilograms taken At the core the temperature is 16 million degrees K, Composition Hydrogen 7196, Helium 26.596, First radio emission from Sun observed which is sufficient to sustain thermonuclear fusion Other 2.5% First observation of solar ultraviolet using a reactions. The released energy prevents the collapse Temperature sounding- of the Sun and keeps it in gaseous form. The total Effective Surface l,OMI,OMIKtemperatureofmrona discovered energy radiated is 383 billion trillion kilowatts/sec- Energy Output (Luminosity) viacodspectralines ond, which is equivalent to that generated by 100 Solar Constant First observation of solar x-rays using a billion tons of TNT exploding each second. Inclination of Solar Equator to Ecliptic 7.2S0 sounding- In addition to the energy-producing solar core, the Galactic dcrays found to change interior has two distinct regions: a radiative and a in intensity with the 11-year sunspot cycle convective zone. From the edge of the core outward, ~argestohewed solar &re occukd - first through the radiative and then through the con- About the Image- First direct observations of solar wind made vective zone, the temperature decreases from 8 million byMariner2 to 7,000 K, and density decreases from 20 gm/cm3to 4 This image of the Sun, taken January24,1992,is ztiezoed First observations of solar gamma rays made x lo-' gm/m3. It takes about 10 million years for from space at x-ray wavelengths. The image, as seen by the by Orbiting Solar Observatory 1(OS01) photons to escape from the dense core and reach the soft X-ray Telescopeon theJapan/US/UKYohkoh Mission First mammmmt of solar neutrino flux surface. (orbiting solar obserpultory), reveals the hot, three-dimen- taken Because the Sun is gaseous, it rotates faster at the sionalgeomettyof the corona across thefill disk of the Sun. Skylab obsened Sun, discovered coronal equator (26.8 days) than at the poles (as long as 35 The large bright areas are regions where the Sun's magnetic holes as days). The Sun's "surface," known the photosphere, field is so strong that it can trap hot gases even though the 1982 First observations of neutrons from a solar is just the visible 500 km-thick layer from which most ~bySolarMaxim~~(~ temperature ofthe regions arecnrer 1 million degrees K. The of the Sun's radiation and light finally escapes, and is 1-5 UlyssesfJiesoverpolarq@onsofSun dark amare ammnl holes, which are the origin ofstrermrs the place where sunspots are found. Above the photo- Rduemca sphere lies the chromosphere ("sphere of color") that of particb, called the high speed solar wind, that flozo past 1.1&!km,"BduationrlBrisltEB-l06,NASA~W~DC may be seen briefly during total solar eclipees as a Eflrtha#dthroughthesolsr~atabout700~ reddish rim, caused by hot hydrogen atoms, around ptr=f"'d* A National Aeronautics and J Space Administration Mercury 9 - National Aeronautics and Space Administration Mercury 9 Mercury is the planet closest to the Sun. Of all the planets, the planet. Mercury also has experienced a unique Caloris basin was formed by collision of a gigantic asteroid it has the most elliptical orbit, except for Pluto. Because of geological history which has resulted in a global system of with Mercury. The strong shock wave produced by the its elliptical orbit, Mercury's closest distance to the Sun is fractures caused by shrinkage of the planet. impact traveled through the planet to instantaneously form the only 46 million km while its greatest distance is 70 million hilly, lineated terrain on the opposite side of the planet. krn. Another unique aspect of Mercury is its rotational and Soon after the planet formed it nearly melted from decay of Afterward, eruption of lava within and surrounding the orbital period. Mercury rotates on its axis once every 58.9 radioactive elements and the inward migration of iron that Caloris, and other large basins formed the smooth plains. days and circles the Sun once every 87.9 days. As a result formed its enormous core. This led to the expansion of the Over the next half billion years the core and mantle began to Mercury rotates exactly three times around its axis for planet and extensive fracturing of the surface which cool, Mercury's radius decreased by about 2 to 4 km, and the every two orbits around the Sun. If you wanted to stay up provided an exit for lava to reach the surface and form the crust was subjected to compressive stresses that resulted in a for a solar day on Mercury (sunrise to sunrise), you would smooth plains within and between the craters. At about the unique global system of fractures. As this occurred, volcan- be awake for two Mercurian years (a total of 176 Earth same time and like the other planets, Mercury was subjected ism ceased when compressive stresses in the lithosphere days.) Because Mercury is so close to the Sun, its surface to heavy bombarded by asteroidal and cometary debris left became strong enough to close off magma sources. Since that temperature has the greatest temperature range of any over from accretion of the solar system. During this early time, only occasional impacts of comets and asteroids have planet or satellite in the solar system. The surface tempera- ~eriodof heavv bombardment. the 1300 krn diameter occurred. ture reaches a maximum of 427" Celsius on the side closest to the Sun, and - 183°C on the night side. Mercury's Significant Dates Fast Facts atmosphere is tenuous and like a vacuum. The atmosphere is composed of sodium and potassium, which is probably 1610 - Italian astronomer Galileo Galilei made first Namesake Messenger of the Roman Gods derived from the surface. While Mercury does have an telescopic obersewation of Mercury. Diameter 4878 km atmosphere, it does not have satellites. 1631 - French astronomer Pierre Gassendi made first Mean Distance from Sun 57.8 million km telescopic obervations of the transit of Mercury Mass 61100 the mass of Earth Physically, Mercury is smaller than any other planet except across the face of the Sun. Density 5.44 glcc Pluto, measuring about one-third the size of Earth. 1639 - Italian astronomer Giovanni Zupus discovered Surface Temperature However, Mercury's density (5.4 g/cm3) is about the same Mercury has phases, which is evidence that the Maximum Day Side 740" Kelvin (467" C) as Earth's; therefore, scientists assume that the planet has planet circle the Sun. Maximum Night Side 90" Kelvin (-1 83" C) an enormous iron core that composes some 75 percent of 1841 - German astronomer, Johann Franz Encke made the Rotational Period 58.6 days Mercury's diameter (42 percent of the volume). The core is first mass determination using gravity effect on the Eccentricity of Orbit 0.206 surrounded by a rocky mantle and crust only about 600 km comet Encke. Rotational Period thick. Aside from Earth, Mercury is the only terrestial 1889 - Italian astronomer, Giovanni Schiaparelli produced (1 Mercury Day) 58.6 Earth days planet with a magnetic field. Although the magnetic field the first map of Mercury's surface features.
Recommended publications
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Planetary Data Workshop
    NASA Conference Publication 2343 NASA-CP-2343-PT-I 19840026295 Part 1 Planetary Data Workshop Proceedings of a workshop held at Goddard Space Flight Center Greenbelt,. Maryland November 29-December 1, 1983 NI_A NASA Conference Publication 2343 Part 1 Planetary Data Workshop Hugh H. Kieffer, Chairman NASA Office of Space Science and Applications Washington, D.C. Proceedings of a workshop held at Goddard Space Hight Center Greenbelt, Maryland November 29-December l, 1983 N/_A National Aeronautics and Space Administration ScientificandTechnical Information Branch 1984 Contributing Authors Hugh Kieffer U.S. Geological Survey Raymond E. Arvidson Washington University William A° Baum Lowell Observatory Larry Bolef Washington University Larry H. Brace Goddard Space Flight Center Roger N. Clark University of Colorado Randal Davis University of Colorado Richard Elphic University of California - Los Angeles John Pearl Goddard Space Flight Center Chris Russell University of California - Los Angeles Stephen R. Saunders Jet Propulsion Laboratory Richard A. Simpson Stanford University William Smythe Jet Propulsion Laboratory Laurence A. Soderblom California Institute of Technology I. A. Stewart University of Colorado R. J. Walker University of California - Los Angeles Charles Acton Jet Propulsion Laboratory Isadore Adler University of Maryland Joseph K. Alexander Goddard Space Flight Center Donald E. Anderson Naval Research Laboratory Donald L. Anderson Arizona State University John Anderson Jet Propulsion Laboratory Daniel Baker Los Alamos National Laboratory Edwin S. Barker McDonald Observatory Reta F. Beebe New Mexico State University Jay T. Bergstralh Jet Propulsion Laboratory Michael L. Bielefield Space Telescope Science Institute A. Lyle Broadfoot University of Arizona James Brown Donald B. Campbell Arecibo Observatory G.
    [Show full text]
  • Your Guide to the Transit of Mercury of 9Th May 2016
    !1 ! Your guide to the Transit of Mercury of 9th May 2016 a publication of the Public Outreach & Education Committee of the Astronomical Society of India Your guide to the Transit of Mercury 2016 !2 ! This work is licensed under a Creative Commons (Attribution - Non Commercial - ShareAlike) License. Please share/print/ photocopy/distribute this work widely, with attribution to the Public Outreach and Education Committee (POEC) of the Astronomical Society of India (ASI) under this same license. This license is granted for non-commercial use only. Contact details of the Public Outreach and Education Committee of the ASI : URL : http://astron-soc.in/outreach Email : [email protected] Facebook : asi poec Twitter : www.twitter.com/asipoec Download from : The pdf of this documents is available for free download from : http://astron-soc.in/outreach/activities/sky-event-related/transit- of-mercury-2016/ (also http://bit.ly/tom-india) Acknowledgement : We thank all those who made images available online either under the Creative Commons License or by a copyleft through image credits. Compiled by Niruj Ramanujam with contributions from Samir Dhurde, B.S. Shylaja and N. Rathnasree, for the POEC of the ASI April 2016 Your guide to the Transit of Mercury 2016 !3 1. Transit of Mercury ! Transit of Mercury, 8 Nov 2006, Transit of Venus, 6 Jun 2012, photographed by Eric Kounce, from Hungary Texas, USA DID YOU KNOW? The planets, with their moons, steadily revolve around the The next transit Sun, with Mercury taking 88 days and Neptune taking as of Mercury will much as 165 years to make one revolution! We barely occur on 9 May notice any of this, unless something spectacular happens to 2016 but it will not be visible remind us how fast this motion actually is.
    [Show full text]
  • King David's Altar in Jerusalem Dated by the Bright Appearance of Comet
    Annals of Archaeology Volume 1, Issue 1, 2018, PP 30-37 King David’s Altar in Jerusalem Dated by the Bright Appearance of Comet Encke in 964 BC Göran Henriksson Department of Physics and Astronomy, Uppsala University, Box 516, SE 751 20 Uppsala, Sweden *Corresponding Author: Göran Henriksson, Department of Physics and Astronomy, Uppsala University, Box 516, SE 751 20 Uppsala, [email protected] ABSTRACT At the time corresponding to our end of May and beginning of June in 964 BC a bright comet with a very long tail dominated the night sky of the northern hemisphere. It was Comet Encke that was very bright during the Bronze Age, but today it is scarcely visible to the naked eye. It first appeared as a small comet close to the zenith, but for every night it became greater and brighter and moved slowly to the north with its tail pointing southwards. In the first week of June the tail was stretched out across the whole sky and at midnight it was visible close to the meridian. In this paper the author wishes to test the hypothesis that this appearance of Comet Encke corresponds to the motion in the sky above Jerusalem of “the sword of the Angel of the Lord”, mentioned in 1 Chronicles, in the Old Testament. Encke was first circumpolar and finally set at the northern horizon on 8 June in 964 BC at 22. This happened according to the historical chronology between 965 and 960 BC. The calculations of the orbit of Comet Encke have been performed by a computer program developed by the author.
    [Show full text]
  • Spectrum May June 2016.Pub
    Inside this issue: The Spectrum The Calendar 2 The Newsletter for the Buffalo Astronomical Obs report 3 Association Wilson Star Search 7 Randy B. Article 9 Astro Events 11 Eyes on the Earth 12 Star Chart 13 14 Mars Viewing 15 May/June Volume 18, Issue 3 Map 17 ….In This Issue: Did you miss Astro Day? Phil Newman didn’t! Here are some of his slides. hps://db./U8GFuAgM (more pic next issue). Dark Maer And The Demise Of The Dinosaurs. Randy Boswell does it again with another fascinang arcle. Usual charts, calendars. And obs report Don’t forget the 2016 BAA elecons are almost here. You will be deciding on who will serve on the board and guide the associaon into the next few years. There will be more informaon in upcoming meengs and posts, so stay tuned. 1 BAA Schedule of Astronomy Fun for 2016 Public Nights and Events Public Nights ‐ First Saturday of the Month March through October. 2016 Tentave Schedule of Events: May 7 Public Night at BMO May 9 Mercury Transit visible from Buffalo ‐ trip to clear skies anyone?? May 13 BAA meeng May 14 Wilson Star Search June 4 Public Night BMO June 10 BAA meeng‐ Elecons/party June 11 Wilson Star Search July 2 Public Night BMO July 9 Wilson Star Search July 30 BAA annual star party at BMO Aug 6 Public Night BMO Aug 13 Wilson Star Search‐ think meteors! Sep 2/3/4 Black Forest (Rain Fest) Star Party Cherry Springs Pa. Sep 3 Public Night BMO Sep 9 BAA Meeng Sept 10 Wilson Star Search Oct 1 Public Night BMO Oct 8 Wilson Star Search Oct 14 BAA meeng Nov 11 BAA meeng Dec 9 BAA Holiday party 2 Observatory Report The refrigerator is full again (thanks to Dennis B), so I will connue to hold "Tues at the Observatory" The Snow season is over, and the rainy season has started (never stopped), I will be holding Tues night on the clearest night Mon/Tue/or Wed.
    [Show full text]
  • Lunar Distances Final
    A (NOT SO) BRIEF HISTORY OF LUNAR DISTANCES: LUNAR LONGITUDE DETERMINATION AT SEA BEFORE THE CHRONOMETER Richard de Grijs Department of Physics and Astronomy, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia Email: [email protected] Abstract: Longitude determination at sea gained increasing commercial importance in the late Middle Ages, spawned by a commensurate increase in long-distance merchant shipping activity. Prior to the successful development of an accurate marine timepiece in the late-eighteenth century, marine navigators relied predominantly on the Moon for their time and longitude determinations. Lunar eclipses had been used for relative position determinations since Antiquity, but their rare occurrences precludes their routine use as reliable way markers. Measuring lunar distances, using the projected positions on the sky of the Moon and bright reference objects—the Sun or one or more bright stars—became the method of choice. It gained in profile and importance through the British Board of Longitude’s endorsement in 1765 of the establishment of a Nautical Almanac. Numerous ‘projectors’ jumped onto the bandwagon, leading to a proliferation of lunar ephemeris tables. Chronometers became both more affordable and more commonplace by the mid-nineteenth century, signaling the beginning of the end for the lunar distance method as a means to determine one’s longitude at sea. Keywords: lunar eclipses, lunar distance method, longitude determination, almanacs, ephemeris tables 1 THE MOON AS A RELIABLE GUIDE FOR NAVIGATION As European nations increasingly ventured beyond their home waters from the late Middle Ages onwards, developing the means to determine one’s position at sea, out of view of familiar shorelines, became an increasingly pressing problem.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Observer's Handbook 1986
    OBSERVER’S HANDBOOK 1986 EDITOR: ROY L. BISHOP THE ROYAL ASTRONOMICAL SOCIETY OF CANADA CONTRIBUTORS AND ADVISORS A l a n H. B a t t e n , Dominion Astrophysical Observatory, 5071 W. Saanich Road, Victoria, BC, Canada V8X 4M6 (The Nearest Stars). L a r r y D. B o g a n , Department of Physics, Acadia University, Wolfville, NS, Canada B0P 1X0 (Configurations of Saturn’s Satellites). Terence Dickinson, R.R. 3, Odessa, ON, Canada K0H 2H0 (The Planets). David W. Dunham, International Occultation Timing Association, P.O. Box 7488, Silver Spring, MD 20907, U.S.A. (Lunar and Planetary Occultations). Alan Dyer, Queen Elizabeth Planetarium, 10004-104 Ave., Edmonton, AB, Canada T5J 0K1 (Messier Catalogue, Deep-Sky Objects). Fred Espenak, Planetary Systems Branch, NASA-Goddard Space Flight Centre, Greenbelt, MD, U.S.A. 20771 (Eclipses and Transits). M arie Fidler, The Royal Astronomical Society of Canada, 136 Dupont St., Toronto, ON, Canada M5R 1V2 (Observatories and Planetaria). Victor Gaizauskas, Herzberg Institute of Astrophysics, National Research Council, Ottawa, ON, Canada K1A 0R6 (Solar Activity). R o b e r t F. G a r r is o n , David Dunlap Observatory, University of Toronto, Box 360, Richmond Hill, ON, Canada L4C 4Y6 (The Brightest Stars). Ian H alliday, Herzberg Institute of Astrophysics, National Research Council, Ottawa, ON, Canada K1A 0R6 (Miscellaneous Astronomical Data). W illiam Herbst, Van Vleck Observatory, Wesleyan University, Middletown, CT, U.S.A. 06457 (Galactic Nebulae). H e l e n S. H o g g , David Dunlap Observatory, University of Toronto, Box 360, Richmond Hill, ON, Canada L4C 4Y6 (Foreword).
    [Show full text]
  • 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.
    [Show full text]
  • SOLAR ECLIPSE NEWSLETTER SOLAR ECLIPSE October 2003 NEWSLETTER
    Volume 8, Issue 10 SOLAR ECLIPSE NEWSLETTER SOLAR ECLIPSE October 2003 NEWSLETTER The sole Newsletter dedicated to Solar Eclipses INDEX · 2 SECalendar for October Dear All, · 8 Correctie op SE-calender for september Autumn started in the meanwhile. Summer is past. We are getting closer · 8 2nd october secalendar to the end of the year. But of course first the total solar eclipse of 23 No- · 9 Index SENL September · 9 Astronomy Books vember on the South Pole. Quite a few organised tours are having or a · 10 Delta T plane or a boat to the path. Hopefully they all will see the event success- · 10 Subject line from ful. Please send in your accounts and pictures. The SENL will publish. SearchDatabase.com As for Jo and myself, we will not go this time. Financial it is a bit too · 10 Analog or video capture much. Derryl Barr, our good friend wrote: “Only one thing is missing for Laptop from this eclipse: Patrick Poitevin. Is it really an "eclipse" if Patrick isn't · 10 Babcock somewhere within the shadow's path? Perhaps we should call it an Eclise · 10 Delta T September · 11 Electronic imaging eye- (obviously the "P" is missing).” piece · 13 Beating the Black Drop Fred Espenak and Pat Totten visited our new home in Tissington · 14 Photographs of Eclipses (Derbyshire, UK). Although it was a rather short visit, we enjoyed the on Mars time together. We made some plans for the partial eclipse of 14 October · 15 TSE-remote camera con- next year. Sunset eclipse in Hawaii … trol · 17 Thanks · 18 Travelling Birds Movie In the meanwhile the registrations for the International Solar Eclipse Con- · 18 The Moon ference SEC2004 started.
    [Show full text]