Slides:



Advertisements
Similar presentations
Chapter 6: Telescopes – Portals of Discovery. Visible light is only one type of electromagnetic radiation emitted by stars Each type of EM radiation travels.
Advertisements

Optics and Telescopes Chapter Six. Telescopes The fundamental purpose of any telescope is to gather more light than the naked eye can In many cases telescopes.
Chapter 5 Telescopes. 5.1 Optical Telescopes The Hubble Space Telescope 5.2 Telescope Size The Hubble Space Telescope 5.3 Images and Detectors Diffraction.
Unit 11, Section 1.  Light can take millions of years to travel to Earth  All electromagnetic radiation travels at the speed of light, which is 300,000.
Optical Astronomy Imaging Chain: Telescopes & CCDs.
Telescopes Analyzing electromagnetic spectra to search for understanding of celestial objects.
Chapter 6 Optics and Telescopes
Discovering the Universe Eighth Edition Discovering the Universe Eighth Edition Neil F. Comins William J. Kaufmann III CHAPTER 3 Light and Telescopes CHAPTER.
Optics and Telescopes Chapter Six.
Telescopes and Spacecraft Astronomy 311 Professor Lee Carkner Lecture 7.
Telescopes and Spacecraft Astronomy 311 Professor Lee Carkner Lecture 7.
Honors Ch Pg Almost everything we know about the universe (space) comes by studying light from distant sources. Light from what?
Learning Objectives Explain the significance of light and astronomy
Chapter 3: Telescopes. Goals Describe basic types of optical telescopes Explain why bigger is better for telescopes Describe how the Earth’s atmosphere.
Astronomy 101 Section 020 Lecture 6 Optics and Telescopes John T. McGraw, Professor Laurel Ladwig, Planetarium Manager.
Telescopes and Spacecraft Astronomy 311 Professor Lee Carkner Lecture 7.
Telescopes and Spacecraft Astronomy 311 Professor Lee Carkner Lecture 7.
Telescopes and Spacecraft Astronomy 311 Professor Lee Carkner Lecture 7.
Telescopes and Spacecraft Astronomy 311 Professor Lee Carkner Lecture 7.
WAVES MEDIUM VIBRATES PERPENDICULARLY TO THE WAVE DIRECTION IF f IS THE WAVE FREQUENCE AND λ IS THE WAVELEGTH THEN c, THE WAVE VELOCITY, IS GIVEN BY: c.
Telescopes & Light. The Powers of a Telescope Light Gathering Power Light Gathering Power : Astronomers prefer *large* telescopes. A large telescope can.
Light and Telescopes What do you think? What is the main purpose of a telescope? Why do stars twinkle?
Optical Telescopes.
Telescopes Section 15.1.
Land Based Telescopes. Telescopes: "light buckets" Primary functions: 1. ___________ from a given region of sky. 2. ______ light. Secondary functions:
Reflective Refractive Spectro scopy Space Large telescopes How Optical works $ 200 $ 200$200 $ 200 $ 200 $400 $ 400$400 $ 400$400 $600 $ 600$600 $
Chapter 5 Telescopes: “light bucket”. Telescopes have three functions 1.Gather as much light as possible: LGP ∝ Area = πR 2 LGP ∝ Area = πR 2 Why? Why?
ISNS Phenomena of Nature The Eye The eye consists of pupil that allows light into the eye - it controls the amount of light allowed in through the.
Chapter 3 Light and Telescopes. What do you think? What is the main purpose of a telescope? Why do stars twinkle?
Optics and Telescopes Lecture 11. Why do we use telescopes? Human eyes are lenses! Human eyes are lenses! Using larger lenses… Using larger lenses… 
Basic Telescope Design Refractors: Utilizes a lens (or lenses) to produce the refraction of light to focus light from an object. The main lens is called.
Telescopes.
Optics and Telescopes. Optics and Telescopes: Guiding Questions 1.How do reflecting and refracting telescopes work? 2.Why is it important that professional.
Review for Test #1  Responsible for: - Chapters 35 and 36 and section Notes from class - Problems worked in class - Homework assignments  Test.
Astronomical Tools. Essential Questions 1.What is Light? 2.How do telescopes work, and how are they limited? 3.What kind of instruments do astronomers.
Optics and Telescope Chapter Six. ASTR 111 – 003 Fall 2007 Lecture 06 Oct. 09, 2007 Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy.
Tools of Astronomy.
Optics and Telescopes Kathy Cooksey Acknowledgements Tyler Nordgren & Julie Rathbun University of Redlands Johnny B. Holmes Christian Brothers University.
Telescopes. Images can be formed through reflection (mirror) or refraction (lens). Reflecting mirror Optical Telescopes.
Astronomy 1020-H Stellar Astronomy Spring_2015 Day-19.
is transparent ERAU Astronomical Observatory Meade inch Schmidt Cassegrain Reflecting Telescope.
Reflecting Telescopes. Mirrors A flat mirror reflects light in straight lines. A curved mirror can focus light to a point. A perfect parabolic mirror.
Optics and Telescopes Chapter Six. Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I Ch1: Astronomy and the Universe Ch2: Knowing the.
Units to cover 25, Types of Spectra Kirchoff ’ s Laws: –If the source emits light that is continuous, and all colors are present, we say that this.
Telescopes The instruments we use to study the universe.
Telescopes. Light Hitting a Telescope Mirror huge mirror near a star * * * small mirror far from 2 stars In the second case (reality), light rays from.
Light & Telescopes (Chapter 5) All of what we know and understand about the stars is the result of observation and analysis of light.
A Basic Refractor Telescope The size of the telescope is the diameter of the light-collecting lens.
Chapter 4: Telescopes. E O Optical telescopes: Reflectors and refractors Refractors use lenses E: eyepiece O: objective.
Chapter 21: Stars, Galaxies, Universe Section 1: telescopes
Telescopes Mr. Hibbetts Special thanks to Dr. Dan Bruton, Astronomy and Physics SFA.
Tools of Astronomy Chapter 28.1 Pages The Best Tool The Light that comes to earth from distant objects is the best tool that astronomers can.
Electromagnetic Spectrum. -is the range of all possible frequencies of electromagnetic radiation. The "electromagnetic spectrum" of an object is the characteristic.
The Very Large Array (VLA) in New Mexico. Observations at wavelengths other than visible light are revealing previously invisible sights Visible light.
Universe Tenth Edition Chapter 6 Optics and Telescopes Roger Freedman Robert Geller William Kaufmann III.
Light and Telescopes Chapter 5. In the early chapters of this book, you looked at the sky the way ancient astronomers did, with the unaided eye. In this.
Optics and Telescopes Chapter Six. Some Guiding Questions 1.Why is it important that telescopes be large? 2.Why do most modern telescopes use a large.
Light and Telescopes
Astronomy 04 The Solar System
Telescopes & Light.
Tools of Astronomy.
Tools of Astronomy.
Telescopes and the Electromagnetic Spectrum Section 3
Windows to the Universe
Section 1.2 Telescopes allow us to study space from earth
Optics and Telescopes Chapter Six.
Unit 3 Practice Test Answer KEY
Chapter 5 Telescopes: Refracting , Reflecting, Cassegrain.
Sci. 1-3 Telescopes- then and Now Pages 18-23
Telescopes.
Presentation transcript:

active optics adaptive optics angular resolution (resolution) blocked light blueshift Cassegrain focus charge-coupled device (CCD) coude focus Doppler shift electromagnetic radiation electromagnetic spectrum eyepiece lens focal length focal plane focal point gamma ray infrared radiation interferometry light-gathering power magnification Newtonian reflector Key Terms objective lens photon pixel primary mirror prime focus radio telescope radio wave redshift reflecting telescope reflection refracting telescope refraction Schmidt corrector plate secondary mirror seeing disk spectrum spherical aberration twinkling ultraviolet (UV) radiation very-long-baseline interferometry (VLBI) wavelength X ray