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Practical Calculations for Designing a Newtonian Telescope
Practical Calculations for Designing a Newtonian Telescope Jeff Beish (Rev. 07 February 2019) INTRODUCTION A Newtonian reflecting telescope can be designed to perform more efficiently than any other type of optical system, if one is careful to follow the laws of nature. One must have optics made from precision Pyrex or a similar material and figured to a high quality. The mounting hardware must be well planned out and properly constructed using highest quality materials. The Newtonian can be used for visual or photographic work, for "deep sky" or "planetary" observing, or a combination of all these. They are easy to layout and to construct using simple household tools. The design mathematics is simple and can be easily accomplished by hand calculator. The Newtonian reflector can be easily modified for other types of observing such a photometry, photography, CCD imaging, micrometer work, and more. Since a reflecting telescope does not suffer for chromatic aberration we don't have to worry about focusing each color while observing or photographing with filters as we would in a single or double lens refractor. This is a problem especially associated with photography. Since the introduction of the relatively low cost Apochromatic refractors (APO) in the past few years these problems no longer hamper the astrophotographer as much. However, the cost of large APO's for those requiring large apertures is prohibitive to most of us who require instruments above 12 or so inches. Remember, even with the highest quality optics a Newtonian can be rendered nearly useless by tube currents, misaligned components, mirror stain, and a secondary mirror too large for the application of the instrument. -
Telescopes and Binoculars
Continuing Education Course Approved by the American Board of Opticianry Telescopes and Binoculars National Academy of Opticianry 8401 Corporate Drive #605 Landover, MD 20785 800-229-4828 phone 301-577-3880 fax www.nao.org Copyright© 2015 by the National Academy of Opticianry. All rights reserved. No part of this text may be reproduced without permission in writing from the publisher. 2 National Academy of Opticianry PREFACE: This continuing education course was prepared under the auspices of the National Academy of Opticianry and is designed to be convenient, cost effective and practical for the Optician. The skills and knowledge required to practice the profession of Opticianry will continue to change in the future as advances in technology are applied to the eye care specialty. Higher rates of obsolescence will result in an increased tempo of change as well as knowledge to meet these changes. The National Academy of Opticianry recognizes the need to provide a Continuing Education Program for all Opticians. This course has been developed as a part of the overall program to enable Opticians to develop and improve their technical knowledge and skills in their chosen profession. The National Academy of Opticianry INSTRUCTIONS: Read and study the material. After you feel that you understand the material thoroughly take the test following the instructions given at the beginning of the test. Upon completion of the test, mail the answer sheet to the National Academy of Opticianry, 8401 Corporate Drive, Suite 605, Landover, Maryland 20785 or fax it to 301-577-3880. Be sure you complete the evaluation form on the answer sheet. -
The Theory of Multiple Simultaneous Discoveries
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Electronic archive of Tomsk Polytechnic University В целом видно, что студенты положительно оценивают наличие дисциплины «Творческий проект» в учебном плане и дают высокую оценку качеству ее проведения. Вывод: Кто такой инженер? И что такое творчество? Инженер от лат. «ingenium» означает способность, изобретательность. Инженер имеет дело с разработкой и внедрением инноваций и для этого ему необходим творческий как подход как основа будущей деятельности. Творчество – создание чего-то нового, которое непременно разрешает определенную проблему. Отсюда видно, что эти два понятия тесно связаны. Поэтому авторы считают, что дисциплина «Творческий про- ект» положительно влияет на процесс обучения студентов младших курсов и дает возможность получения глубоких практических знаний технических основ будущей профессии. ЛИТЕРАТУРА: 1. Всемирная инициатива CDIO. Стандарты: информ.-метод. изд. / пер. с англ. и ред. А. И. Чучалина, Т. С. Петровской, Е. С. Ку- люкиной; Том. политехн. ун-т. – Томск, 2011. 2. Рабочие программы по дисциплине «Творческий проект» [Элек- тронный ресурс] – URL: http://portal.tpu.ru/fond2 (дата обраще- ния: 13.09.15). Научный руководитель: В.С. Иванова, к.т.н., доцент, каф. ТП ИНК. THE THEORY OF MULTIPLE SIMULTANEOUS DISCOVERIES D.V. Isaeva National research Tomsk polytechnic university, Institute of non- destructive testing, Precise instrument making department, group 1B3V Since the beginning of time, people have been making different dis- coveries and inventions. They make great discoveries, which are based not only on the experience of previous generations, but on experiments and scientific analysis. However, what is the nature of discoveries? Theories of invention has been an ongoing discussion for more than a century. -
Celestron Kids 50Mm Newtonian Telescope Manual
A B 50mm Newtonian Telescope #22014 Solar Warning C • Always use your telescope with adult supervision. F • Never look directly at the Sun with the naked eye or with a telescope unless you have the proper solar filter. D Permanent and irreversible eye damage may result. • Never use your telescope to project an image of the E Sun onto any surface. Internal heat build-up can damage the telescope and any accessories attached to it. • Never use an eyepiece solar filter or a Herschel wedge. Internal heat build-up inside the telescope can cause these devices to crack or break, allowing unfiltered sunlight to pass through to the eye. • Do not leave the telescope unsupervised, especially Assembly when children are present or when adults unfamiliar Step 1: Remove all the parts form the box. with the correct operating procedures of your telescope are present. Thanks for buying the Celestron Kids STEM 50mm Newtonian Telescope—a real, functional reflector telescope with a removable panel that reveals its inner workings! Before using your telescope, take a few minutes to make sure all the components are in the box and assemble the scope. Parts A. Eyepiece B. Telescope Tube C. Tripod Adjustment Collar D. Tripod Hub Step 2: Attach the 3 tripod legs to the tripod hub by E. Tripod Legs (3) screwing them into the threaded holes. F. Dust Cap Use Your Telescope Step 1: When you are ready to view through your telescope, remove the plastic cover on the eyepiece. Step 2: Remove the dust cap. Step 3: Attach the main telescope tube to the tripod hub. -
Some Comments on Multiple Discovery in Mathematics
Journal of Humanistic Mathematics Volume 7 | Issue 1 January 2017 Some Comments on Multiple Discovery in Mathematics Robin W. Whitty Queen Mary University of London Follow this and additional works at: https://scholarship.claremont.edu/jhm Part of the History of Science, Technology, and Medicine Commons, and the Other Mathematics Commons Recommended Citation Whitty, R. W. "Some Comments on Multiple Discovery in Mathematics," Journal of Humanistic Mathematics, Volume 7 Issue 1 (January 2017), pages 172-188. DOI: 10.5642/jhummath.201701.14 . Available at: https://scholarship.claremont.edu/jhm/vol7/iss1/14 ©2017 by the authors. This work is licensed under a Creative Commons License. JHM is an open access bi-annual journal sponsored by the Claremont Center for the Mathematical Sciences and published by the Claremont Colleges Library | ISSN 2159-8118 | http://scholarship.claremont.edu/jhm/ The editorial staff of JHM works hard to make sure the scholarship disseminated in JHM is accurate and upholds professional ethical guidelines. However the views and opinions expressed in each published manuscript belong exclusively to the individual contributor(s). The publisher and the editors do not endorse or accept responsibility for them. See https://scholarship.claremont.edu/jhm/policies.html for more information. Some Comments on Multiple Discovery in Mathematics1 Robin M. Whitty Queen Mary University of London [email protected] Synopsis Among perhaps many things common to Kuratowski's Theorem in graph theory, Reidemeister's Theorem in topology, and Cook's Theorem in theoretical com- puter science is this: all belong to the phenomenon of simultaneous discovery in mathematics. We are interested to know whether this phenomenon, and its close cousin repeated discovery, give rise to meaningful questions regarding causes, trends, categories, etc. -
A History of Astronomy, Astrophysics and Cosmology - Malcolm Longair
ASTRONOMY AND ASTROPHYSICS - A History of Astronomy, Astrophysics and Cosmology - Malcolm Longair A HISTORY OF ASTRONOMY, ASTROPHYSICS AND COSMOLOGY Malcolm Longair Cavendish Laboratory, University of Cambridge, JJ Thomson Avenue, Cambridge CB3 0HE Keywords: History, Astronomy, Astrophysics, Cosmology, Telescopes, Astronomical Technology, Electromagnetic Spectrum, Ancient Astronomy, Copernican Revolution, Stars and Stellar Evolution, Interstellar Medium, Galaxies, Clusters of Galaxies, Large- scale Structure of the Universe, Active Galaxies, General Relativity, Black Holes, Classical Cosmology, Cosmological Models, Cosmological Evolution, Origin of Galaxies, Very Early Universe Contents 1. Introduction 2. Prehistoric, Ancient and Mediaeval Astronomy up to the Time of Copernicus 3. The Copernican, Galilean and Newtonian Revolutions 4. From Astronomy to Astrophysics – the Development of Astronomical Techniques in the 19th Century 5. The Classification of the Stars – the Harvard Spectral Sequence 6. Stellar Structure and Evolution to 1939 7. The Galaxy and the Nature of the Spiral Nebulae 8. The Origins of Astrophysical Cosmology – Einstein, Friedman, Hubble, Lemaître, Eddington 9. The Opening Up of the Electromagnetic Spectrum and the New Astronomies 10. Stellar Evolution after 1945 11. The Interstellar Medium 12. Galaxies, Clusters Of Galaxies and the Large Scale Structure of the Universe 13. Active Galaxies, General Relativity and Black Holes 14. Classical Cosmology since 1945 15. The Evolution of Galaxies and Active Galaxies with Cosmic Epoch 16. The Origin of Galaxies and the Large-Scale Structure of The Universe 17. The VeryUNESCO Early Universe – EOLSS Acknowledgements Glossary Bibliography Biographical SketchSAMPLE CHAPTERS Summary This chapter describes the history of the development of astronomy, astrophysics and cosmology from the earliest times to the first decade of the 21st century. -
A Complete Bibliography of Publications in Journal for the History of Astronomy
A Complete Bibliography of Publications in Journal for the History of Astronomy Nelson H. F. Beebe University of Utah Department of Mathematics, 110 LCB 155 S 1400 E RM 233 Salt Lake City, UT 84112-0090 USA Tel: +1 801 581 5254 FAX: +1 801 581 4148 E-mail: [email protected], [email protected], [email protected] (Internet) WWW URL: http://www.math.utah.edu/~beebe/ 10 May 2021 Version 1.28 Title word cross-reference $8.95 [Had84]. $87 [CWW17]. $89.95 [Gan15]. 8 = 1;2;3 [Cov15]. $90 [Ano15f]. $95 [Swe17c]. c [Kin87, NRKN16, Rag05]. mul [Kur19]. muld [Kur19]. [Kur19]. · $100 [Apt14]. $120 [Hen15b]. $127 [Llo15]. 3 [Ano15f, Ash82, Mal10, Ste12a]. ∆ [MS04]. $135.00 [Smi96]. $14 [Sch15]. $140 [GG14]. $15 [Jar90]. $17.95 [Had84]. $19.95 -1000 [Hub83]. -4000 [Gin91b]. -601 [Mul83, Nau98]. 20 [Ost07]. 2000 [Eva09b]. [Hub83]. -86 [Mar75]. -Ft [Edd71b, Mau13]. $24.95 [Lep14, Bro90]. $27 [W lo15]. $29 -inch [Ost07]. -year [GB95]. -Year-Old [Sha14]. $29.25 [Hea15]. $29.95 [Eva09b]. [Ger17, Mes15]. 30 [Mau13]. $31.00 [Bra15]. $34 [Sul14]. $35 Zaga´_ n [CM10]. [Ano15f, Dev14b, Lau14, Mir17, Rap15a]. $38 [Dan19b, Vet19]. $39.95 [Mol14b]. /Catalogue [Kun91]. /Charles [Tur07]. $39.99 [Bec15]. $40 [Dun20, LF15, Rob86]. /Collected [Gin93]. /Heretic [Tes10]. 40 [Edd71b]. $42 [Nau98]. $45 [Kes15]. /the [War08]. $49.95 [Ree20]. $49.99 [Bec15]. $50 [Kru17, Rem15]. $55 [Bon19b]. $60 [Mal15]. 0 [Ave18, Hei14a, Oes15, Swe17c, Wlo15, 600 [GB95]. $72 [Ave18]. $79 [Wil15]. 1 2 Ash82]. [Dic97a]. 1970 [Kru08]. 1971 [Wil75]. 1973 [Doe19]. 1975 [Ost80]. 1976 [Gin02d]. 1979 1 [Ano15f, BH73a, Ber14, Bru78b, Eva87b, [Ano78d]. -
OPEN SCIENCE' an Essay on Patronage, Reputation and Common Agency Contracting in the Scientific Revolution
This work is distributed as a Discussion Paper by the STANFORD INSTITUTE FOR ECONOMIC POLICY RESEARCH SIEPR Discussion Paper No. 06-38 THE HISTORICAL ORIGINS OF 'OPEN SCIENCE' An Essay on Patronage, Reputation and Common Agency Contracting in the Scientific Revolution By Paul A. David Stanford University & the University of Oxford December 2007 Stanford Institute for Economic Policy Research Stanford University Stanford, CA 94305 (650) 725-1874 The Stanford Institute for Economic Policy Research at Stanford University supports research bearing on economic and public policy issues. The SIEPR Discussion Paper Series reports on research and policy analysis conducted by researchers affiliated with the Institute. Working papers in this series reflect the views of the authors and not necessarily those of the Stanford Institute for Economic Policy Research or Stanford University. THE HISTORICAL ORIGINS OF ‘OPEN SCIENCE’ An Essay on Patronage, Reputation and Common Agency Contracting in the Scientific Revolution By Paul A. David Stanford University & the University of Oxford [email protected] or [email protected] First version: March 2000 Second version: August 2004 This version: December 2007 SUMMARY This essay examines the economics of patronage in the production of knowledge and its influence upon the historical formation of key elements in the ethos and organizational structure of publicly funded open science. The emergence during the late sixteenth and early seventeenth centuries of the idea and practice of “open science" was a distinctive and vital organizational aspect of the Scientific Revolution. It represented a break from the previously dominant ethos of secrecy in the pursuit of Nature’s Secrets, to a new set of norms, incentives, and organizational structures that reinforced scientific researchers' commitments to rapid disclosure of new knowledge. -
The Myth of the Sole Inventor
Michigan Law Review Volume 110 Issue 5 2012 The Myth of the Sole Inventor Mark A. Lemley Stanford Law School Follow this and additional works at: https://repository.law.umich.edu/mlr Part of the Intellectual Property Law Commons Recommended Citation Mark A. Lemley, The Myth of the Sole Inventor, 110 MICH. L. REV. 709 (2012). Available at: https://repository.law.umich.edu/mlr/vol110/iss5/1 This Article is brought to you for free and open access by the Michigan Law Review at University of Michigan Law School Scholarship Repository. It has been accepted for inclusion in Michigan Law Review by an authorized editor of University of Michigan Law School Scholarship Repository. For more information, please contact [email protected]. THE MYTH OF THE SOLE INVENTORt Mark A. Lemley* The theory of patent law is based on the idea that a lone genius can solve problems that stump the experts, and that the lone genius will do so only if properly incented. But the canonical story of the lone genius inventor is largely a myth. Surveys of hundreds of significant new technologies show that almost all of them are invented simultaneously or nearly simultaneous- ly by two or more teams working independently of each other. Invention appears in significant part to be a social, not an individual, phenomenon. The result is a real problem for classic theories of patent law. Our domi- nant theory of patent law doesn't seem to explain the way we actually implement that law. Maybe the problem is not with our current patent law, but with our current patent theory. -
Newtonian Telescope Collimation with the Astrosystems Lightpipe/Sighttube and Autocollimator
Newtonian Telescope Collimation with the Astrosystems LightPipe/SightTube and Autocollimator Contents Introduction i Preparation 1 - 2 Mechanical Alignment with the Crosshair SightTube 2 - 3 Optical Collimation with the LightPipe collimator 4 - 5 Fine Optical Collimation with the Autocollimator 5 - 6 Checking Optical Collimation - Star Test 7 Secondary Offset 8-9 References / Further Reading 9 i Introduction The first two steps, preparation and mechanical alignment, need only be performed the first time the telescope is assembled. Thereafter, only the optical alignment and star testing are needed to collimate your telescope. Don't underestimate the importance of mechanical alignment. Most troublesome collimating jobs can be traced back to mistakes or assumptions regarding the placement of components. Quick Tour: If you are familiar with your telescope’s collimation and only want an abbreviated guide to using the AstroSystems collimating tools, just read through the lines in bold type at the beginning of each paragraph. Preparation 1 Position the telescope Place the telescope on a horizontal surface or move it to the horizontal. Position the focuser so it is easily accessible. You will be moving back and forth from the rear to the front of the tube assembly to check progress and it helps to have things positioned for convenience. Assemble the proper tools Gather the necessary tools required to adjust the primary mirror holder, secondary mirror holder, and spider and focuser base. Center spot the primary mirror It is necessary to "spot" the center of the primary and secondary mirrors. To facilitate collimation at night, a white mark on the primary is most visible. -
Scientific Discovery Reloaded
Topoi https://doi.org/10.1007/s11245-017-9531-3 1 Scientifc Discovery Reloaded 2 Emiliano Ippoliti1 3 4 © Springer Science+Business Media B.V., part of Springer Nature 2017 5 Abstract 6 The way scientifc discovery has been conceptualized has changed drastically in the last few decades: its relation to logic, 7 inference, methods, and evolution has been deeply reloaded. The ‘philosophical matrix’ moulded by logical empiricism and 8 analytical tradition has been challenged by the ‘friends of discovery’, who opened up the way to a rational investigation of 9 discovery. This has produced not only new theories of discovery (like the deductive, cognitive, and evolutionary), but also 10 new ways of practicing it in a rational and more systematic way. Ampliative rules, methods, heuristic procedures and even a 11 logic of discovery have been investigated, extracted, reconstructed and refned. The outcome is a ‘scientifc discovery revo- 12 lution’: not only a new way of looking at discovery, but also a construction of tools that can guide us to discover something 13 new. This is a very important contribution of philosophy of science to science, as it puts the former in a position not only to 14 interpret what scientists do, but also to provide and improve tools that they can employ in their activity. 15 Keywords Logic · Discovery · Heuristics · Reasoning · Psychology · Algorithm 16 1 Scientifc Discovery: The Matrix 2006, xii), and they are essential for discovery. Genius (see e.g. Murray 1989), illumination, ‘faculties’ such as intui- 17 38 A long-standing and infuential tradition has shaped the way tion, insight, or ‘divergent thinking’, are common notions 18 39 scientifc discovery has been accounted for. -
Telescope & Instrument Fundamentals
Telescope & Instrument Fundamentals Luc Simard Astronomy 511 Spring 2018 Outline • Apertures, surfaces, stops and pupils • Aberrations and telescope designs • Imaging • Spectroscopy • Observing Strategies and Calibrations • Data Reduction What makes a good telescope site? • Number of clear and photometric nights (> 300) • Larger isoplanatic angle • Longer coherence time • Low water vapor content • Small pressure broadening (mid-IR) Hawaii and Chile are considered to be the best sites on Earth thanks to a combination of geographical factors. Do you know what they are? (Hint: Proximity to a beach is not one of them.) Collecting Area of the Large Telescopes (GTC) All 4-meter class primary mirrors are monolithic 8-10-meter class primary mirrors are either monolithic or segmented - dividing line is between 8 and 10 meters. Primary Aperture - Monolithic Gemini Magellan 1+2/LBT1+2/GMT Thin meniscus (thickness = 20 cm) Honeycomb (thickness = 80-110 cm) D = 8.1m D = 8.4m 120 actuators 1750 alumina silica cores (D = 20 cm) Lower mass = lower thermal inertia Total mass = 15% mass of a solid blank Primary Aperture - Segmented Keck TMT 36 hexagonal segments 492 hexagonal segments Diameter = 1.8 m (82 distinct segments) Thickness = 75 mm Diameter = 1.44 m Weight = 400 kg Thickness = 45 mm Gap = 3 mm Primary Aperture - “Diluteness” PSF PSF Large Binocular Telescope Giant Magellan Telescope PSF Monolithic, unobscured, PSF circular aperture VLT Interferometer Secondary Aperture - Conventional Optical Reflector Gemini Secondary D = 1.023m Central Hole D