SOLAR ECLIPSE NEWSLETTER SOLAR ECLIPSE October 2003 NEWSLETTER
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White Peak Trails and Cycle Routes
Things to See and Do The High Peak Trail by funded part Project The Countryside The Cromford and High Peak Railway was one of the first The White Peak is a spectacular landscape of open views railways in the world. It was built between 1825 and s www.derbyshire.gov.uk/buse characterised by the network of fields enclosed by dry stone Several Peak District 1830 to link the Peak Forest Canal at Whaley or 2608 608 0870 walls. North and south of Hartington the trails go down into villages have annual Bridge (north of Buxton) to the Traveline from timetables and services other updates, Check the deep valley of the Upper Dove and the steeper gorge at well dressings (a Cromford Canal – a distance of Hire. Cycle Waterhouses and tableau of flower- Beresford Dale. On the lower land are the towns and villages 33 miles. The railway itself was Hire Cycle Ashbourne to Leek and Derby links 108 Travel TM built from local stone in traditional style. based pictures designed like a canal. On the around the village flat sections the wagons were Hire. Cycle Hay Interesting Places wells). Ask at visitor pulled by horses. Large Manifold Track below Thor’s Cave Parsley and Hire Cycle Ashbourne to Buxton links 542 Bowers centres for dates. The Trails and White Peak cycle network have a rich industrial steam powered Centre. Hire Cycle Ashbourne and Hire Cycle Water heritage and railway history. beam engines in The Manifold Track Carsington to Wirksworth and Matlock links 411 Travel TM Look out for the sculpted benches along the Trails and the From Track to Trail And Further Afield ‘engine houses’ This was the Leek and Manifold Valley Light Railway. -
NFU Derbyshire Calendar 2017
NFU Derbyshire Calendar 2017 Event Topic(s)/Speaker(s) Date Venue Time January 2017 NVZ Update Meetings Sarah Belton, Senior 24 January Bluebell Inn, Tissington, nr Ashbourne, Derbyshire DE6 1NH 11am Hydrogeologist from Hafren Water NVZ Update Meetings Sarah Belton, Senior 24 January Twin Oaks Hotel, Palterton, Chesterfield S44 6UZ 2:30pm Hydrogeologist from Hafren Water NSA Central Region ‘Early Gathering’ NFU Livestock advisers on 26 January Agricultural Business Centre, Bakewell, Derbyshire DE45 1AH 10am – hand to answer questions 5pm What next? - AHDB / NFU meeting 26 January Staffordshire County Showground, Weston Rd, Stafford ST18 7:30pm 0BD Green Futures Farming Advice Service, 30 January Bluebell Inn, Tissington, Buxton Road, Tissington DE6 1NH 7:30pm Natural England and Environment Agency February 2017 What next? - AHDB / NFU meetings Barclays Bank, AHDB & NFU 1 February Bluebell Inn, Buxton Rd, Tissington DE6 1NH 7:30pm Crops board 2 February NFU, Agriculture House, North Gate, Uppingham, Oakham LE15 12:30pm 9NX Sugar forum 7 February Carre Arms, 1 Mareham Lane, Sleaford NG34 7JP 7pm Melbourne Branch Meeting 7 February The John Thompson Inn, Ingleby, Melbourne, Derbyshire DE73 7:30pm 7HW Derby Branch Meeting 13 February The Black Cow, Dalbury Lees, Ashbourne, Derby DE6 5BE 7:30pm Derbyshire and Staffordshire – BVDFree To book contact 15 February The Bentley Brook Inn, Ashbourne DE6 1LF 7:30pm [email protected] / 07773 234673 NEW ADDITIONS ARE HIGHLIGHTED IN RED The voice of British farming NFU East Midlands, Agriculture -
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. -
THE STUDY of SATURN's RINGS 1 Thesis Presented for the Degree Of
1 THE STUDY OF SATURN'S RINGS 1610-1675, Thesis presented for the Degree of Doctor of Philosophy in the Field of History of Science by Albert Van Haden Department of History of Science and Technology Imperial College of Science and Teohnology University of London May, 1970 2 ABSTRACT Shortly after the publication of his Starry Messenger, Galileo observed the planet Saturn for the first time through a telescope. To his surprise he discovered that the planet does.not exhibit a single disc, as all other planets do, but rather a central disc flanked by two smaller ones. In the following years, Galileo found that Sa- turn sometimes also appears without these lateral discs, and at other times with handle-like appendages istead of round discs. These ap- pearances posed a great problem to scientists, and this problem was not solved until 1656, while the solution was not fully accepted until about 1670. This thesis traces the problem of Saturn, from its initial form- ulation, through the period of gathering information, to the final stage in which theories were proposed, ending with the acceptance of one of these theories: the ring-theory of Christiaan Huygens. Although the improvement of the telescope had great bearing on the problem of Saturn, and is dealt with to some extent, many other factors were in- volved in the solution of the problem. It was as much a perceptual problem as a technical problem of telescopes, and the mental processes that led Huygens to its solution were symptomatic of the state of science in the 1650's and would have been out of place and perhaps impossible before Descartes. -
Directory of Churches
Directory of Churches www.derby.anglican.org Please email any amendments to [email protected] December 2016 Contents Contact Details Diocese of Derby 1 Diocesan Support Office, Church House 2 Area Deans 4 Board of Education 5 Alphabetical List of Churches 6 List of Churches - Archdeaconry, Deanery, Benefice, Parish & Church Order 13 Church Details Chesterfield Archdeaconry Carsington Deanery ................................................................................................................... 22 Hardwick Deanery ..................................................................................................................... 28 North East Derbyshire Deanery .................................................................................................. 32 Peak Deanery ............................................................................................................................. 37 Derby Archdeaconry City Deanery ............................................................................................................................... 45 Duffield & Longford Deanery ...................................................................................................... 51 Mercia Deanery .......................................................................................................................... 56 South East Derbyshire Deanery ................................................................................................. 60 Chesterfield Archdeaconry Carsington Deanery .................................................................................................................. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
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. -
Lick Observatory Records: Photographs UA.036.Ser.07
http://oac.cdlib.org/findaid/ark:/13030/c81z4932 Online items available Lick Observatory Records: Photographs UA.036.Ser.07 Kate Dundon, Alix Norton, Maureen Carey, Christine Turk, Alex Moore University of California, Santa Cruz 2016 1156 High Street Santa Cruz 95064 [email protected] URL: http://guides.library.ucsc.edu/speccoll Lick Observatory Records: UA.036.Ser.07 1 Photographs UA.036.Ser.07 Contributing Institution: University of California, Santa Cruz Title: Lick Observatory Records: Photographs Creator: Lick Observatory Identifier/Call Number: UA.036.Ser.07 Physical Description: 101.62 Linear Feet127 boxes Date (inclusive): circa 1870-2002 Language of Material: English . https://n2t.net/ark:/38305/f19c6wg4 Conditions Governing Access Collection is open for research. Conditions Governing Use Property rights for this collection reside with the University of California. Literary rights, including copyright, are retained by the creators and their heirs. The publication or use of any work protected by copyright beyond that allowed by fair use for research or educational purposes requires written permission from the copyright owner. Responsibility for obtaining permissions, and for any use rests exclusively with the user. Preferred Citation Lick Observatory Records: Photographs. UA36 Ser.7. Special Collections and Archives, University Library, University of California, Santa Cruz. Alternative Format Available Images from this collection are available through UCSC Library Digital Collections. Historical note These photographs were produced or collected by Lick observatory staff and faculty, as well as UCSC Library personnel. Many of the early photographs of the major instruments and Observatory buildings were taken by Henry E. Matthews, who served as secretary to the Lick Trust during the planning and construction of the Observatory. -
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. -
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). -
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. -
TRACE Observations of the 15 November 1999 Transit of Mercury and the Black Drop Effect: Considerations for the 2004 Transit of Venus
Icarus 168 (2004) 249–256 www.elsevier.com/locate/icarus TRACE observations of the 15 November 1999 transit of Mercury and the Black Drop effect: considerations for the 2004 transit of Venus Glenn Schneider,a,∗ Jay M. Pasachoff,b and Leon Golub c a Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA b Williams College—Hopkins Observatory, Williamstown, MA 01267, USA c Smithsonian Astrophysical Observatory, Mail Stop 58, 60 Garden Street, Cambridge, MA 02138, USA Received 15 May 2003; revised 14 October 2003 Abstract Historically, the visual manifestation of the “Black Drop effect,” the appearance of a band linking the solar limb to the disk of a transiting planet near the point of internal tangency, had limited the accuracy of the determination of the Astronomical Unit and the scale of the Solar System in the 18th and 19th centuries. This problem was misunderstood in the case of Venus during its rare transits due to the presence of its atmosphere. We report on observations of the 15 November 1999 transit of Mercury obtained, without the degrading effects of the Earth’s atmosphere, with the Transition Region and Coronal Explorer spacecraft. In spite of the telescope’s location beyond the Earth’s atmosphere, and the absence of a significant mercurian atmosphere, a faint Black Drop effect was detected. After calibration and removal of, or compensation for, both internal and external systematic effects, the only radially directed brightness anisotropies found resulted from the convolution of the instrumental point-spread function with the solar limb-darkened, back-lit, illumination function.