We have not kept a record of where we found any of the texts and images we have used.
|
|
- Hester Fowler
- 6 years ago
- Views:
Transcription
1 Copyright Information We believe that most of the texts and images are in the public domain. We do not own the copyright to the texts and images used in ATM Letters Journal. We have not kept a record of where we found any of the texts and images we have used. If you believe that you own the rights to any of the texts and images we use, please contact us and we will add an acknowledgement. All logos and trademarks in ATM Letters Journal are property of their respective owner.
2 January/February Issue, 2006 A Brief History of Telescope In Focus: Designing and Making Lurie-Houghton Telescope
3 CONTENTS Issue January/February Volume 4 Number 1 Spectrum Robotic Telescopes Advanced telescope techniques. 8 ADVANCED TECHNIQUES Making Lurie-Houghton Newtonian Telescope Building s Report of 5-inch telescope by Aki Lötjönen. 19 PRAXIS 8 Designing Lurie-Houghton Telescope Detailed calculations and design recommendations. 38 BACK TO THEORY LHTCALC Java Script Lurie-Houghton Calculator 48 OPTICAL COMPUTING 19 MODAS 4.2xx New release with valuable changeover under development 49 COMPUTER AND TELESCOPES History A Brief History of Telescopes The telescope is undoubtedly one of the world's most farreaching inventions. For the past four centuries the telescope has stood at the forefront of human discovery. From its humble beginnings in seventeenth-century Holland, when a simple spectacle-maker first presented his invention to his country's military leaders, to today's colossal structures housed in spaceage cathedrals, the telescope has unlocked nature's secrets. The history of the telescope is a rich story of human ingenuity and perseverance involving some of the most colorful figures of the scientific world - Galileo, Johann Kepler, Isaac Newton, William Herschel, George Ellery Hale, and Edwin Hubble BIBLIOGRAPHY Contents ATM Digest OPTICS ABC UPDATE GALLERY ATTACHED NEXT ISSUE ADVERTISMENT ON THE COVER Fortune: This picture was made by the Bulgarian amateur astronomer and telescope maker Pencho Markishki ( markishky@yahoo.com). Hi is also advanced astro photograph, that reached great success with his very simple optics. More innovative photos can be seen on his home page at following url.: Image Credit: Pencho Markishki
4 Hubble 15 Years of Discovery July/August March/April Issue, Bibliography: James Short, Europe s foremost maker of Reflecting Telescopes In Focus: Trigonometric and Coddington Raytrace
5 CONTENTS Issue March/April Volume 4 Number 2 Spectrum Hubble 15 Years of Discovery Advanced telescope techniques. 3 SPACE OPTICS Cleaning Optics If it's not dirty, don't clean it. 23 OPTICS ABC Trigonometric and Coddington Raytrace Aberrations and Raytracing BACK TO THEORY TRIGON.BAS, CODDING.BAS Trigonometric and Coddington raytrace. 33 OPTICAL COMPUTING DiffCalc Simulation of diffraction limited star and CCD images. 37 COMPUTER AND TELESCOPES History James Short: Europe s foremost maker of Reflecting Telescopes James Short was born in Edinburgh in 1710 and received a good education, progressing to Edinburgh University in He attended lectures by Colin Maclaurin, Professor of Mathematics, and became interested in science. He mastered the craft of making mirrors for reflecting telescopes and had a good understanding of optical theory. During his working life of over 35 years, Short made about 1,360 instruments - not only for customers in Britain but also for export: one is still preserved in Leningrad, another at Uppsala and several in America. Short was principal British collator and computer of the Transit of Venus observations made throughout the world on 6th June His instruments traveled on Endeavour with Captain Cook to observe the next Transit of Venus on 3rd June 1769, but Short died before this event took place BIBLIOGRAPHY Contents ATM Digest OPTICS ABC UPDATE ATTACHED GALLERY NEXT ISSUE ADVERTISMENT ON THE COVER VLT and Hubble Collage of the Hubble Space Telescope above the world s largest optical/infrared telescope, the ESO s Very Large Telescope (VLT). Image Credit: ESO/ST-ECF
6 SUBARU Japan s Eye of the Universe July/August May/June Issue, Bibliography: Vasco Ronchi In Focus: Merit Function Optimization
7 CONTENTS Issue May/June Volume 4 Number 3 Spectrum Subaru Japan s Eye of the Universe Earth s greatest telescopes. 3 ADVANCED OPTICS Grinding, Polishing, Materials Glossary. 18 OPTICS ABC 18 Merit Function Optimization Aberrations and Raytracing. 27 BACK TO THEORY AUTOFOCUS.BAS First steps in optimization. 29 OPTICAL COMPUTING 33 FRED Optical design and analysis package. 33 COMPUTER AND TELESCOPES History Vasco Rionchi Vasco Ronchi was an Italian physicist known for his work in optics. He was born on 19th December 1897 in Florence, Italy. Along with Enrico Fermi, he was a student of Luigi Puccianti. He studied from at the Faculty of Physics of the University of Pisa In 1922 he published work describing testing methods for optics using simple equipment. The Ronchi Test is widely used in amateur telescope making. He served numerous terms as the President of the 'Union Internationale d'histoire des Sciences' within the UNESCO. He authored 900 papers and 30 books BIBLIOGRAPHY Contents ATM Digest BOOKS UPDATE ATTACHED GALLERY NEXT ISSUE ADVERTISMENT ON THE COVER Subaru Telescope is located on the summit of Mauna Kea, a dormant volcano on the big island of Hawaii. The summit of Mauna Kea is one of the best astronomical observing sites in the world. With 13 telescopes form 11 countries now operating, Mauna Kea has more telescopes from more countries than any other observing site. In addition to Subaru, there are three other 8-10m class telescopes on Mauna Kea, the Gemini North telescope and the two Keck telescopes. Image credit: Subaru
8 Leon Foucault: The Dance of Shadows July/August JulyAugust Issue, Spectrum: Planet Hunters Could Find Life Software: LensForge for Mac OS X In Focus: Calculating Geometrical MTF
9 CONTENTS Issue July/August Volume 4 Number 4 Spectrum Planet Hunters Could Find Life Extrasolar Planets Searching. 3 SPACE OPTICS Glass Types Optical materials glossary. 16 OPTICS ABC 3 Calculating Geometrical MTF Image quality analysis. 18 BACK TO THEORY MTFPLOTTER.BAS Geometrical MTF plotter. 23 OPTICAL COMPUTING LensForge Optical design and analysis package for Max OS X. 29 COMPUTER AND TELESCOPES History Leon Foucault: The Dance of Shadows One of Foucault's many accomplishments was the publication, in 1859, of his development of the older pinhole technique into the Foucault test. Viewing the reflected pinhole across a straight knife edge causes a pattern of shadows that clearly shows the figure of the mirror. This simple improvement granted an enormous increase in the perfection of telescope optics. Foucault went on to analyze the patterns made by mirrors as they are polished from spherical to parabolic form. He also experimented with moving the light towards the mirror and the straight edge away from it, and with the various ellipsoidal mirror forms that can be made in this way. In his fifty year lifetime, Foucault also devised the famous Foucault pendulum, that was the first experimental demonstration of the rotation of the earth. He was also responsible for an accurate determination of the velocity of light, measured the distance to the sun with improved precision, and pioneered the silver on glass telescope mirror BIBLIOGRAPHY Contents ATM Digest OPTICS ABC UPDATE ATTACHED GALLERY NEXT ISSUE ADVERTISMENT ON THE COVER Jean Bernard Leon Foucault was a French physicist who is considered one of the most versatile experimentalists of the nineteenth century. He is well known for his experiments in optics and mechanics and was involved in the development of a method to measure the speed of light with extreme accuracy. Foucault is most often remembered for proving, with the use of a pendulum, that the Earth rotates on its axis. Image credit: OAMP
10 September/October Issue, 2006 Henry Fitz: America s First Commercial Telescope Maker In Focus: An alternative Floation Cell for parabollicaly shaped Mirrors by using an elastic Foundation Theory: Optical Apertures Software: CODE V
11 CONTENTS Issue September/October Volume 4 Number 5 Spectrum It is a Question of Aperture A Baker Street Reminiscence by Dr. John H. Watson 3 SHORT STORY Useful ATM Formulas ATM theoritical glossary. 8 OPTICS ABC An alternative Floation Cell for parabollicaly shaped Mirrors by using an elastic Foundation BACK TO THEORY ATMFORMULAS.XLS Graphical representation of the most commonly used ATM formulas. 27 OPTICAL COMPUTING CODE V Optical design and analysis package review. 29 COMPUTER AND TELESCOPES History Henry Fitz: America s First Commercial Telescope Maker Henry Fitz was preceded by the earliest American telescope makers, notably Amasa Holcomb, and followed by Alvan Clark and John Brashear, the most important makers from the United States. Fitz was the first important American telescope maker because his pioneering techniques of local correction of poor quality glass allowed him to construct the largest American made refractor. American made telescopes were much less expensive, than those from Europe, and local manufacture was an important factor in the proliferation of observatories in Nineteenth Century America BIBLIOGRAPHY Contents ATM Digest ATTACHED UPDATE BOOKS GALLERY NEXT ISSUE ADVERTISMENT ON THE COVER The Dudly s Observatory 13-inch Fitz refractor. Henry Fitz received commissions to build larger and larger telescopes for leading American universities and institutions. Among his larger telescopes were two 13" telescopes, one made for the Allegheny Observatory in 1861 that is still in service, and one for the Dudley Observatory in Albany, New York. The Dudley telescope went into private hands around the turn of the century, and fell into obscurity until 1994 Image credit: S&T
12 November/December July/August Issue, Issue, Alvan Clark & Sons: World s Greatest Telescope Makers In Focus: Field Correctors for a Fast Newtonian with Parabolic Primary Software: Ross Null Calculator
13 CONTENTS Issue November/December Volume 4 Number 6 Spectrum SuperWASP Planetary transit telescope project 4 ADVANCED TELESCOPE TECHNIQUES Objective Types A glossary 11 OPTICS ABC Field Correctors for a Fast Newtonian with Parabolic Primary 16 BACK TO THEORY VIGNETTING.XLS Vignetting in a Newtonian telescope OPTICAL COMPUTING RossNullXP Ross Null Lens calculator COMPUTER AND TELESCOPES History Alvan Clark & Sons: World s Greatest Telescope Makers A renowned American maker of some of the world s largest and best lenses for refracting telescopes. Together with his sons, George Bassett Clark ( ) and Alvan Graham Clark ( ), he founded Alvan Clark & Sons at Cambridgeport, Massachusetts, in 1846, and proceeded five times to make the objectives for the largest refracting telescopes in the world. These included the 26-inch lens at the US Naval Observatory (the first fine achromatic lens produced in the United States), the 32-inch lens at Pulkovo Observatory, the 36- inch lens at Lick Observatory, and the 40-inch lens at Yerkes Observatory, the largest ever built. The optical work of Clark & Sons was recognized as unsurpassed anywhere and represented the first significant American contribution to astronomical instrument-making; prior to this, American telescopes had never compared with those of European manufacture. Alvan Graham Clark is also remembered particularly for his discovery of the (white dwarf) companion of Sirius in BIBLIOGRAPHY ATM Digest ON THE COVER Contents OPTICS ABC ATTACHED UPDATE GALLERY NEXT ISSUE ADVERTISMENT The trial mounting for the great Russian telescope in Pulkovo, Russia constructed by Alvan Clark & Sons The refractor was destroyed in the Siege of Leningrad (today St. Petersburg) and only the lens survives. The 32-inch objective can be seen in the Pulkovo s Museum. 80 Image credit: SA
14 MODAS RLD (Reloaded) Beta version now available Advertisement
We have not kept a record of where we found any of the texts and images we have used.
Copyright Information We believe that most of the texts and images are in the public domain. We do not own the copyright to the texts and images used in ATM Letters Journal. We have not kept a record of
More informationTelescopes. Some of these are made into satellites and put into the atmosphere
Telescopes Telescopes Telescopes collect more light than the eye can which is why they allow us to see much fainter objects than is possible with the naked eye In the past astronomers look through them,
More informationTELESCOPE NOTES. Figure 1
TELESCOPE NOTES Figure 1 In its simplest form a lens is a clear disk of glass with curved surfaces. When parallel light rays from a distant object pass through the lens they are bent (refracted) and come
More informationTWO SMALL PIECES OF GLASS A Space Science Program for Grades 5-12
Teacher Idea Kit TWO SMALL PIECES OF GLASS A Space Science Program for Grades 5-12 Presented by Funded in part by: Two Small Pieces of Glass Suggested for Grades 5-12 Objectives After visiting the planetarium
More informationEarth s Atmosphere & Telescopes. Atmospheric Effects
Earth s Atmosphere & Telescopes Whether light is absorbed by the atmosphere or not depends greatly on its wavelength. Earth s atmosphere can absorb certain wavelengths of light so much that astronomers
More informationAstronomy. Optics and Telescopes
Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Optics and Telescopes - Refraction, lenses and refracting telescopes - Mirrors and reflecting telescopes - Diffraction limit,
More informationTelescopes. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. A Warm Up Exercise. Key Ideas:
Telescopes A Warm Up Exercise If we measure the wavelengths of emission lines and absorption lines from the same gas, we find that (ignoring any Doppler shifts) a) Some emission lines shift to the red
More informationAlvan Clark & Sons Business and Family Papers, (bulk ) Finding Aid. Adler Planetarium & Astronomy Museum
Alvan Clark & Sons Business and Family Papers, 1850-1934 (bulk 1850 1918) Finding Aid Adler Planetarium & Astronomy Museum Webster Institute for the History of Astronomy Chicago, Illinois 2013 Contact
More informationTelescope Terminology
Suffolk County Community College AST 103 Student name: Telescope Terminology T he history of mankind's understanding of the universe may be broken into two separate and distinct periods: B.T. (which stands
More informationGround- and Space-Based Telescopes. Dr. Vithal Tilvi
Ground- and Space-Based Telescopes Dr. Vithal Tilvi Telescopes and Instruments Astronomers use telescopes to gather light from distant objects and instruments to record the data Telescopes gather light
More informationTelescopes: Portals of Discovery
Telescopes: Portals of Discovery How do light and matter interact? Emission Absorption Transmission Transparent objects transmit light Opaque objects block (absorb) light Reflection or Scattering Reflection
More informationPhysics 112 Star Systems
Physics 112 Star Systems Lecture 8 Telescopes and Spectrometers Kevin H Knuth University at Albany Fall 2013 Equipped with his five senses, man explores the universe around him and calls the adventure
More informationA Question. Simple Magnifier. Magnification by a Lens 11/29/2011. The last lecture
The last lecture Exam: Final: Consult the website, especially room assignments. Makeup: Register with me today. Tea and Cookies: Tuesdays 5PM, NPB 2175 A Question Unpolarized light of intensity I goes
More informationWhy Use a Telescope?
1 Why Use a Telescope? All astronomical objects are distant so a telescope is needed to Gather light -- telescopes sometimes referred to as light buckets Resolve detail Magnify an image (least important
More informationThe Birth of ATM in the USA
The Birth of ATM in the USA (as told by a Brit!) Keith Venables FRAS The origins of ATM Galileo Newton Herschel Rosse Herschel Commercially available late 19 th C telescopes Clark Cooke Calver Browning
More informationYou will have a lab this week on telescopes, in which you will build a refracting telescope. In the first lecture, back in the first week of classes,
You will have a lab this week on telescopes, in which you will build a refracting telescope. In the first lecture, back in the first week of classes, we already talked about telescopes and adaptive optics.
More informationMeasuring Light waves
Measuring Light waves We normally measure wavelengths (λ) using nanometers (nm) 1 nm = 10-9 m 400-700 nm Increasing wavelengths (λ)! Visible light has wavelengths between 400-700 nm! To detect other types
More informationAstronomical Instruments
Astronomical Instruments 1 Human Eye iris Until 17 th century all astronomical studies limited to naked eye observations. Equipment used were mainly to measure positions of celestial objects in the sky.
More informationGrade 5. Practice Test. Telescopes: An Introduction Powerful Telescopes
Name Date Grade 5 Telescopes: An Introduction Powerful Telescopes Today you will read two passages. Read these sources carefully to gather information to answer questions and write an essay. Excerpt from
More informationHow do they work? Chapter 5
Telescopes How do they work? Chapter 5 1. History 2. Lenses & Hardware 3. Reflecting Telescopes 4. Refracting Telescopes History Hans Lippershey Middleburg, Holland invented the refractor telescope in
More informationTelescopes. Telescopes Key Concepts. glass
Telescopes Telescopes Key Concepts 1) A refracting telescope uses a lens to gather light; a reflecting telescope uses a mirror. ) The main purposes of a telescope are to gather light and resolve fine detail.
More informationD = telescope aperture h = wavelength of light being observed D and h must be in the same units.
the diameter or aperture. Because stars are extremely far away, they appear as point sources of light even with a telescope. Their brightness in the telescope depends only on the size of the aperture.
More informationTopographic Features of Mars Observed by G.H. Hamilton (1924) and C.F. Capen (1969) Authored by Gene Cross & Rodger W. Gordon
Topographic Features of Mars Observed by G.H. Hamilton (1924) and C.F. Capen (1969) Authored by Gene Cross & Rodger W. Gordon (Presented by Gene Cross, July 20, 2006) 1 Abstract Topographic features on
More informationHow Light Beams Behave. Light and Telescopes Guiding Questions. Telescopes A refracting telescope uses a lens to concentrate incoming light at a focus
Light and Telescopes Guiding Questions 1. Why is it important that telescopes be large? 2. Why do most modern telescopes use a large mirror rather than a large lens? 3. Why are observatories in such remote
More informationTelescopes. Astronomy 320 Wednesday, February 14, 2018
Telescopes Astronomy 320 Wednesday, February 14, 2018 Telescopes gather light and resolve detail A telescope is sometimes called a light bucket. Number of photons collected per second is proportional to
More informationTMT-J Project Office, National Institute of Natural Sciences/ National Astronomical Observatory of Japan TELESCOPE (TMT) ( NAOJ)
SPECIAL REPORT TMT~Thirty Meter Telescope Tomonori Usuda (TMT-J Project Director) and Miki Ishii (Public Relations) TMT-J Project Office, National Institute of Natural Sciences/ National Astronomical Observatory
More informationLight and motion. = v c
Light and motion This means that if you know what wavelength some radiation was emitted at (as you would for, say, a hydrogen Balmer line), then the observed wavelength tells you the velocity of the object
More informationThe tools of an astronomer
NASA The tools of an astronomer Szydagis 01.31.2018 1/13 http://optical-technologies.info/wavefrontsensors-the-ultimate-optical-diagnostic-tool/ Copyright 2015 Tangient LLC 2012 Tracey Technologies. All
More informationIt will cover material up to, but not including, Will consist of a few short-answers, 1-2 short essay, and a few problems + extra credit.
Astronomy 210 Section 1 MWF 1500-1550 134 Astronomy Building This Class (Lecture 13): Thermal Radiation Next Class: Exam #1 on Friday! Thursday Review Session Hour Exam #1 Music: The Space Race is Over
More informationUniverse. Chapter 6. Optics and Telescopes 8/12/2015. By reading this chapter, you will learn. Tenth Edition
Roger Freedman Robert Geller William Kaufmann III Universe Tenth Edition Chapter 6 Optics and Telescopes By reading this chapter, you will learn 6 1 How a refracting telescope uses a lens to form an image
More informationFrom the Subaru Telescope to TMT
From the Subaru Telescope to TMT KASHIKAWA Nobunari, Associate Professor, National Astronomical Observatory of Japan I t has been fifteen years since the Subaru Telescope began operation. It stands as
More informationFig. 2 The image will be in focus everywhere. It's size changes based on the position of the focal plane.
Instruments 1. Basic Optics 1. Rays of Light 2. Waves of light 3. Basic Imaging Systems 4. A Basic Telescope 5. Aberrations 6. Mirrors 2. Some Real Instruments 1. Galileo's Telescope 2. Keplerian Optics
More informationTelescopes... Light Buckets
Telescopes... Light Buckets Now that we have an understanding of what light is and why it s important to astronomy, what tools are required to study light from distant objects? The telescope is the tool
More informationContents: -Information/Research Packet. - Jumbled Image packet. - Comic book cover page. -Comic book pages. -Example finished comic
Contents: -Information/Research Packet - Jumbled Image packet - Comic book cover page -Comic book pages -Example finished comic Nicolaus Copernicus Nicholas Copernicus was a Polish astronomer who lived
More informationOptical Instruments. Chapter 25. Simple Magnifier. Clicker 1. The Size of a Magnified Image. Angular Magnification 4/12/2011
Optical Instruments Chapter 25 Optical Instruments Analysis generally involves the laws of reflection and refraction Analysis uses the procedures of geometric optics To explain certain phenomena, the wave
More informationNOTES: Arvind Borde The Bending of Light and Telescopes. Light travels in straight lines... except when it bends (refraction).
Arvind Borde The Bending of Light and Telescopes Light travels in straight lines...... except when it bends (refraction). 1 The bending of light causes lensing. 2 And lensing is what our eyes, cameras,
More informationCoursework Booklet 2
Level 3 Applied Science UNIT 16: Astronomy and Space Science PHYSICS SECTION Coursework Booklet 2 1 P a g e Astronomy and space science Learning aim B Undertake measurement and observation of astronomical
More informationCollecting Light. In a dark-adapted eye, the iris is fully open and the pupil has a diameter of about 7 mm. pupil
Telescopes Collecting Light The simplest means of observing the Universe is the eye. The human eye is sensitive to light with a wavelength of about 400 and 700 nanometers. In a dark-adapted eye, the iris
More informationUniverse. Chapter 6. Optics and Telescopes 11/16/2014. By reading this chapter, you will learn. Tenth Edition
Roger Freedman Robert Geller William Kaufmann III Universe Tenth Edition Chapter 6 Optics and Telescopes By reading this chapter, you will learn 6 1 How a refracting telescope uses a lens to form an image
More informationOptics and Telescopes
Optics and Telescopes Guiding Questions 1. Why is it important that telescopes be large? 2. Why do most modern telescopes use a large mirror rather than a large lens? 3. Why are observatories in such remote
More information11.3 The Telescope. object. Figure 1 A Galilean telescope eye. reflecting telescope: telescope that uses a parabolic mirror to focus light
(b) Most s are now made of two or more lenses. What kind of lenses are involved in Huygenian, Ramsden, Periplan, and Kellner designs? Which of those s is the best one to use? Why? (c) The Dutch naturalist
More informationOptics and Telescope. Chapter Six
Optics and Telescope Chapter Six ASTR 111 003 Fall 2007 Lecture 06 Oct. 09, 2007 Introduction To Modern Astronomy I: Solar System Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-15) Chap.
More informationChapter 5. Telescopes. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 5 Telescopes Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Why do we need Telescopes? Large collection area for photons than the eye long integration
More informationChapter 5. Telescopes. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 5 Telescopes Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Tools of the Trade: Telescopes The Powers of a Telescope Collecting Power Bigger telescope,
More informationTopics for Today. Clicker Q: Radio Waves. Radios. Discussion of how do ROTATING STARS yield Doppler-broadened spectral emission lines
ASTR 1040 Accel Astro: Stars & Galaxies Topics for Today Basic principles of eyes, camera, telescopes Twinkle and absorption by our atmosphere What light gets through, what does not Next lecture: Telescopes
More informationConditions Governing Access: This collection is stored offsite. It is available for research by special arrangement
OVERVIEW OF THE COLLECTION Title: Albert G. Ingalls Papers Collection Dates: C. 1920-1956 Extent and Forms of Material: 8.7 cubic feet (26 boxes) Repository: Archives Center, National Museum of American
More informationLight and Telescopes
Light and Telescopes The key thing to note is that light and matter interact. This can happen in four principal ways: 1) emission a hot object such as the filament in a light bulb emits visible light 2)
More informationChapter 6 Lecture. The Cosmic Perspective. Telescopes Portals of Discovery Pearson Education, Inc.
Chapter 6 Lecture The Cosmic Perspective Telescopes Portals of Discovery 2014 Pearson Education, Inc. Telescopes Portals of Discovery CofC Observatory 6.1 Eyes and Cameras: Everyday Light Sensors Our goals
More informationTELESCOPES An overview of the main tools used by astronomers to study the universe.
Lesson 203: TELESCOPES An overview of the main tools used by astronomers to study the universe. Fundamental Questions Attempting to give thorough and reasonable answers to the following questions will
More informationIII. ASTRONOMY TOOLS:
III. ASTRONOMY TOOLS: A. Since light is so important to astronomers, they want to collect as much of it as possible from a given object, and quantitatively study it in great detail. 1. Astronomers use
More informationAST 101 Intro to Astronomy: Stars & Galaxies
AST 101 Intro to Astronomy: Stars & Galaxies Telescopes Mauna Kea Observatories, Big Island, HI Imaging with our Eyes pupil allows light to enter the eye lens focuses light to create an image retina detects
More informationAstronomical Techniques
Astronomical Techniques Lecture 2 Yogesh Wadadekar ISYA 2016, Tehran ISYA 2016, Tehran 1 / 51 How sun moves? How do stars move in the sky? ISYA 2016, Tehran 2 / 51 Celestial sphere ISYA 2016, Tehran 3
More informationEarth based radio telescopes
I am telescope. My purpose is to collect as much light as possible from some distant source and deliver it to a detector/observer for detailed study. Different Telescopes opaque opaque Space based telescopes
More informationEdwin Hubble Changed Our Ideas About the Universe
Edwin Hubble Changed Our Ideas About the Universe Astronomers continue to use the Hubble Space Telescope named after him. Transcript of radio broadcast: 28 April 2009 ANNOUNCER: EXPLORATIONS -- a program
More informationThe Main Point. Familiar Optics. Some Basics. Lecture #8: Astronomical Instruments. Astronomical Instruments:
Lecture #8: Astronomical Instruments Astronomical Instruments: Optics: Lenses and Mirrors. Detectors. Ground Based Telescopes: Optical, Infrared, and Radio. Space Based Telescopes. Spacecraft Missions.
More informationAstronomy is remote sensing
Astronomy is remote sensing We cannot repeat (or change) the Universe in a controlled environment. We cannot make planets, stars, or galaxies. We cannot make the vacuum of space, nor the shape of spacetime
More informationConcave mirrors. Which of the following ray tracings is correct? A: only 1 B: only 2 C: only 3 D: all E: 2& 3
Concave mirrors Which of the following ray tracings is correct? A: only 1 B: only 2 C: only 3 D: all E: 2& 3 1 2 3 c F Point C: geometrical center of the mirror, F: focal point 2 Concave mirrors Which
More informationObservational Astronomy - Lecture 3 Telescopes and the Electromagnetic Spectrum
Observational Astronomy - Lecture 3 Telescopes and the Electromagnetic Spectrum Craig Lage New York University - Department of Physics craig.lage@nyu.edu April 1, 2014 1 / 1 The Electromagnetic Spectrum
More informationAstronomy- The Original Science
Astronomy- The Original Science Imagine that it is 5,000 years ago. Clocks and modern calendars have not been invented. How would you tell time or know what day it is? One way to tell the time is to study
More informationChapter 18: Studying Space Astronomy: The Original Science
Chapter 18: Studying Space 18.1 Astronomy: The Original Science What is Astronomy? Astronomy is the study of the universe People in ancient cultures used the seasonal cycles of the stars, planets, and
More informationChapter 6 Lecture. The Cosmic Perspective Seventh Edition. Telescopes Portals of Discovery Pearson Education, Inc.
Chapter 6 Lecture The Cosmic Perspective Seventh Edition Telescopes Portals of Discovery Telescopes Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning: How do eyes
More informationAstronomy 1 Fall 2016
Astronomy 1 Fall 2016 One person s perspective: Three great events stand at the threshold of the modern age and determine its character: 1) the discovery of America; 2) the Reformation; 3) the invention
More informationTelescopes Refractors Reflectors Catadioptrics
Optical Aberrations As indicated by the history of telescopes, limits of design were encountered as the instrument was developed. Here are diagrams to better explain each aberration: Telescopes Refractors
More informationChapter 3 Telescopes The tools of Astronomy
Chapter 3 Telescopes The tools of Astronomy Very Large Array (VLA), National Radio Astronomy Observatory (NRAO), Socorro, New Mexico (Radio telescope: 27 antennas, Y configuration, 25 meters diameter each)
More informationWhat are the most important properties of a telescope? Chapter 6 Telescopes: Portals of Discovery. What are the two basic designs of telescopes?
Chapter 6 Telescopes: Portals of Discovery What are the most important properties of a telescope? 1. Light-collecting area: Telescopes with a larger collecting area can gather a greater amount of light
More informationOn the Shoulders of Giants: Isaac Newton and Modern Science
22 May 2012 MP3 at voaspecialenglish.com On the Shoulders of Giants: Isaac Newton and Modern Science SHIRLEY GRIFFITH: This is Shirley Griffith. STEVE EMBER: And this is Steve Ember with the VOA Special
More informationASTR-1010: Astronomy I Course Notes Section VI
ASTR-1010: Astronomy I Course Notes Section VI Dr. Donald G. Luttermoser Department of Physics and Astronomy East Tennessee State University Edition 2.0 Abstract These class notes are designed for use
More informationAssignments. For Mon. 1 st Midterm is Friday, Oct. 12. Read Ch. 6 Optionally do MT1-sample-problems
Assignments For Mon. Read Ch. 6 Optionally do MT1-sample-problems 1 st Midterm is Friday, Oct. 12 Chapter 5 Light: The Cosmic Messenger Thermal Radiation 1. Hotter objects emit photons with a higher average
More informationTelescopes, Observatories, Data Collection
Telescopes, Observatories, Data Collection Telescopes 1 Astronomy : observational science only input is the light received different telescopes, different wavelengths of light lab experiments with spectroscopy,
More informationModels of the Solar System. The Development of Understanding from Ancient Greece to Isaac Newton
Models of the Solar System The Development of Understanding from Ancient Greece to Isaac Newton Aristotle (384 BC 322 BC) Third in line of Greek thinkers: Socrates was the teacher of Plato, Plato was the
More informationTelescopes and estimating the distances to astronomical objects
Telescopes and estimating the distances to astronomical objects Why do we use telescopes? 1. Light-collecting area: A telescope is a light bucket Q: How much more light can a telescope with a diameter
More informationStudying the universe
Studying the universe What is astronomy? A branch of science that deals with study of stars, planets, the universe as a whole The idea is that we live in a clockwork universe and is governed by laws that
More informationChapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 2 The Rise of Astronomy Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Periods of Western Astronomy Western astronomy divides into 4 periods Prehistoric
More information2 OBSERVING THE SKY: THE BIRTH OF ASTRONOMY
2 OBSERVING THE SKY: THE BIRTH OF ASTRONOMY 1 2.1 The Sky Above Did you ever lie flat on your back in an open field and look up? If so, what did the sky look like? Most people think it appears to look
More informationTELESCOPES POWERFUL. Beyond the Book. FOCUS Book
FOCUS Book POWERFUL TELESCOPES Why do we need telescopes in order to observe stars that are very far away? Why do stars look bright in the sky while most galaxies, which have billions of stars, are too
More informationKepler correctly determined the motion of the planets giving his 3 Laws which still hold today for the planets and other orbital motion: moons around
Kepler correctly determined the motion of the planets giving his 3 Laws which still hold today for the planets and other orbital motion: moons around planets, exoplanets around other stars, stars in the
More informationTools of Astronomy: Telescopes
Tools of Astronomy: Telescopes Lecture 9 1 Refracting Telescopes Large lens to gather and focus light. Incoming Light Objective Lens Focus Eyepiece 2 Problems w/ Refracting Tel s Must make a large piece
More informationPicturing the Universe. How Photography Revolutionized Astronomy
a c t i v i t y Picturing the Universe 15 How Photography Revolutionized Astronomy The invention of practical photography by Louis Daguerre was announced in Paris in 1839. News of the daguerreotype process
More informationFinal Announcements. Lecture25 Telescopes. The Bending of Light. Parts of the Human Eye. Reading: Chapter 7. Turn in the homework#6 NOW.
Final Announcements Turn in the homework#6 NOW. Homework#5 and Quiz#6 will be returned today. Today is the last lecture. Lecture25 Telescopes Reading: Chapter 7 Final exam on Thursday Be sure to clear
More informationCredit: NASA. History and Astronomy Glenn Holliday Rappahannock Astronomy Club Night in Washington's Day at Kenmore November
Credit: NASA History and Astronomy Glenn Holliday Rappahannock Astronomy Club Night in Washington's Day at Kenmore November 13 2015 People = Astronomy Credit: Science Museum of Brussels 37,000 years old
More informationFocus Question: How do astronomers study light?
Telescopes Focus Question: How do astronomers study light? Telescopes Tools for collecting and analyzing electromagnetic radiation (light) in ways beyond what we can do with our eyes alone Properties of
More information3/7/2018. Light and Telescope. PHYS 1411 Introduction to Astronomy. Topics for Today s class. What is a Telescopes?
PHYS 1411 Introduction to Astronomy Light and Telescope Chapter 6 Topics for Today s class Optical Telescopes Big Telescopes Advances in Telescope Designs Telescopes Mountings Problems with Mirrors and
More informationTools of Modern Astronomy
Tools of Modern Astronomy Are Those Stars Really a Group? 1. Cut ten pieces of thread to different lengths between 5 cm and 25 cm. Tape a 1- cm plastic foam ball to the end of each piece of thread. 2.
More informationChapter 3 Telescopes The tools of Astronomy
Chapter 3 Telescopes The tools of Astronomy Very Large Array (VLA), National Radio Astronomy Observatory (NRAO), Socorro, New Mexico (Radio telescope: 27 antennas, Y configuration, 25 meters diameter each)
More informationThe tools of an astronomer
NASA The tools of an astronomer Szydagis 01.27.2016 1/14 2/14 Activity: Seeing further! If you had to build a device to see something far away how would you do it? What items and materials would you need
More informationObserving the Universe. Optical Instruments
Observing the Universe Optical Instruments Our Eye The fovea has a high concentration of cones sensitive to colour. Other parts of the retina have more rods these are not sensitive to colour, but have
More informationObservational Astrophysics I
Observational Astrophysics I Nikolai Piskunov Oleg Kochukhov Kjell Lundgren 26 January 2018 1 Requirements to pass: n Attend lectures (9 lectures) n Do home work and report it in the class n Do telescope
More informationTelescopes: Portals of Discovery Pearson Education, Inc.
Telescopes: Portals of Discovery 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning: How do eyes and cameras work? The Eye Refraction Incoming light ray Air Glass Refraction is the bending
More informationScientific Revolution
Age of Revolutions Scientific Revolution Scientific Revolution Period of time in which a new way of thinking came about. The beliefs held by many for so long were now being questioned. Use logic and reason
More informationAstronomical Tools. Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes
Astronomical Tools Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes Laws of Refraction and Reflection Law of Refraction n 1 sin θ 1
More informationOptical Instruments. Optical Instruments 1. Physics 123, Fall 2012
Optical Instruments 1 Physics 123, Fall 2012 Name Optical Instruments I. Magnifier The lens in the human eye adjusts its shape to change the focal length, so that objects at a variety of distances can
More informationMagnifying Glass. Angular magnification (m): 25 cm/f < m < 25cm/f + 1. image at 25 cm (= normal near point) relaxed eye, image at (normal) far point
Magnifying Glass Angular magnification (m): 25 cm/f < m < 25cm/f + 1 relaxed eye, image at (normal) far point image at 25 cm (= normal near point) For more magnification, first use a lens to form an enlarged
More informationOuter space: A matter of gravity
1997 2009, Millennium Mathematics Project, University of Cambridge. Permission is granted to print and copy this page on paper for non commercial use. For other uses, including electronic redistribution,
More informationIsaac Newton Benjamin Franklin Michael Faraday
Isaac Newton (4 January 1643 31 March 1727) was born and raised in England. He was a greater thinker and made many discoveries in physics, mathematics, and astronomy. Newton was the first to describe the
More informationPlanetary Orbits: Kepler s Laws 1/18/07
Planetary Orbits: Kepler s Laws Announcements The correct link for the course webpage http://www.lpl.arizona.edu/undergrad/classes/spring2007/giacalone_206-2 The first homework due Jan 25 (available for
More informationTHE SCIENTIFIC REVOLUTION
THE SCIENTIFIC REVOLUTION REVOLUTION: a sudden, extreme, or complete change in the way people live, work, etc. (Merriam-Webster) THE SCIENTIFIC REVOLUTION Time of advancements in math and science during
More informationLecture 11 Optical Instruments Overview
Lecture 11 Optical Instruments Overview Lenses were discovered about 700 years ago. They were mostly used as magnifying glasses for visual aids. It took humanity roughly another 300 years to figure out
More informationLight and Telescopes
Light and Telescopes Astronomy 1 Elementary Astronomy LA Mission College Spring F2015 Quotes & Cartoon of the Day We find them smaller and fainter, in constantly increasing numbers, and we know that we
More information7. Telescopes: Portals of Discovery Pearson Education Inc., publishing as Addison Wesley
7. Telescopes: Portals of Discovery Parts of the Human Eye pupil allows light to enter the eye lens focuses light to create an image retina detects the light and generates signals which are sent to the
More informationWhat do we do with the image?
Astro 150 Spring 2018: Lecture 7 page 1 Reading: Chapter 6, Sect. 6.4; Chapter 14 + assignment posted on Astro 150 website Homework: questions on special reading - answers due in lecture Thursday Exam
More information