Astronomy Instrumentation Astronomy Summer School for West Africa Daniel Okoh.

Slides:



Advertisements
Similar presentations
Astronomy Notes to Accompany the Text
Advertisements

For centuries, astronomers learned about the sky by studying the light coming from astronomical objects, first by simply looking at the objects, and later.
Journal 9/9/14 Imagine you’re standing at the base of a tall flagpole. Explain how you might measure the height of this flagpole without getting closer.
Astronomy and the Electromagnetic Spectrum
Distances to Astronomical Objects
Astronomical distances The SI unit for length, the meter, is a very small unit to measure astronomical distances. There units usually used is astronomy:
Lesson 7-2 Sectors of Circles.
Telescopes. Tomorrow night Viewing session # 1 7:00 – 8:00 p.m. DRESS WARMLY! Bring paper and writing utensil for taking notes.
Observational Astronomy. Astronomy from space Hubble Space Telescope.
Lecture 1 PHYS Lecture 1: Angles, Parallax and Astronomical Distance Units Objectives: Understand basic astronomical terminology to describe.
The Science of Astronomy
Apparent/Actual Motions Summary
Angles Angle  is the ratio of two lengths:
Powers of Ten, Angles, Units, Mechanics Chapters 1, 4
Prof. D.C. Richardson Sections
Chapter 3: Telescopes. Goals Describe basic types of optical telescopes Explain why bigger is better for telescopes Describe how the Earth’s atmosphere.
Chapter 0 Charting the Heavens
5 Telescopes How big is yours?. 5 Goals Telescopes Angular Sizes “Seeing” Magnitudes.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 10 Measuring the Stars.
Prologue Welcome to PH109 Exploring the Universe Dr. Michael L. Cobb Fall, 2003.
Telescopes Amateur and Professional. Galileo 1609.
Telescopes and Astronomical Instruments The 2 main points of telescopes are 1)To make images with as much angular information as possible 2)To gather as.
Properties of Stars. Distance Luminosity (intrinsic brightness) Temperature (at the surface) Radius Mass.
Summary January The wobble technique assumes that a star will physically be perturbed by the orbit of a planet around it and the resulting motion.
Question 1 Constellations appear to move across the sky at night because 1) the Earth orbits the Sun. 2) the Moon orbits the Earth. 3) stars are in constant.
Introduction to the Solar System The solar system is made up of the sun, orbiting planets, their moons, and other objects traveling around the sun. The.
Studying Space Chapter 26 Notes Standards 2b Students know galaxies are made of billions of stars and comprise most of the visible mass in the universe.
Grab your text book Chapter 1 Astronomy Today 7th Edition
Patterns in the Sky (cont)
Unit 1 Physics Detailed Study 3.1 Chapter 10: Astronomy.
Distances in Space. How Far Away are Stars & Other Celestial Bodies? Use Stellarium to observe the sky and discuss what observations you might be able.
Distances of the Stars. Key Ideas Distance is the most important & most difficult quantity to measure in Astronomy Method of Trigonometric Parallaxes.
1) Celestial objects are things seen in Earth’s sky that is outside our atmosphere.
Introduction to Astronomy.  Observations lead to theories and laws  Laws are concise statements that summaries a large number of observations.  Theories.
ASTR 111 – 003 Fall 2007 Lecture 01 Aug. 27, 2007 Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I: Solar System Ch1: Astronomy and.
Chapter 18 – Studying Space Astronomy – The study of space, stars the visible universe. Year – The amount of time required for the Earth to orbit the sun.
Studying for the Exam Relevant chapters: E, 1, 2 & 3 To prepare for the exam it is helpful to … –review readings –review lecture notes online (esp. concept.
Bellringer Name as many Modern constellations in the night sky as you are able.
Chapter 19 The Stars Distances to stars are measured using parallax.
Chapter 0 Lecture Charting the Heavens.
3 Copyright – Anglo Australian Observatory Light and Telescopes Astronomy: The Science of Seeing.
Tools and Technology Space Objects By: Brittany D. Alexander.
Astronomy By: Shannon Allen. Vocabulary Calendar - a system for organizing time Year – the time required for the earth to orbit the sun once Month – roughly.
Astronomical distances The SI unit for length, the metre, is a very small unit to measure astronomical distances. There units usually used is astronomy:
Light hits Matter: Refraction Light travels at different speeds in vacuum, air, and other substances When light hits the material at an angle, part of.
ASTR 111 – 003 Fall 2006 Lecture 01 Aug. 28, 2006 Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy II Ch1: Astronomy and the Universe.
Astronomical Tools. Guiding Questions 1.What methods do scientists use to expand our understanding of the universe? 2.What makes up our solar system?
Astronomy Big Idea: The sun is one of billions of stars in one of billions of galaxies in the universe.
Exploring the Universe
1 Lines in the Sky In order to use the sky to measure time you need to measure the location of objects in the sky. We will look at two methods of measuring.
Some Basic Facts 12 Constellations of the Zodiac: groups of stars
Science 9: Unit E: Space Exploration Topic 5: What Channel is That?
Astronomy Unit 2 Telescopes Celestial Spheres/Constellations Apparent Motion of the Stars Motion of the Planets.
Trigonometry Tutorial * Right Triangles * Tangents * Small Angle Approximation * Triangulation * Parallax.
Lecture 13 Light: the Cosmic Messenger Telescopes and Observational Astronomy.
Chapter 0: Charting the Heavens. Units of Chapter 0 The “Obvious” View Earth’s Orbital Motion The Motion of the Moon The Measurement of Distance Science.
Radio Telescopes. Angular resolution Distant objects are separated by an angle. –Degrees, arc-minutes, arc-seconds Angular resolution refers to the ability.
Observational Astronomy Mapping the Heavens Coordinate Systems We have two different ways to locate objects in the sky: Celestial equatorial system -Right.
Day 5 notes Parallax measurements Small angular measurements Units of large distances.
Stars Distances to stars: Although the sky seems full of stars, most of the universe is empty space (about 75%) This contradiction exist because most stars.
Astronomy Chapter 1 Charting the Universe. Obj.#1 What is Astronomy? Astronomy is the study of the Universe The universe is the total of all space, time,
Homework #4 What is the maximum resolution of your eyes (assume the wavelength range that your eyes are sensitive to is 300 – 700 nm and that your iris.
Navigating the Night Sky
Seeing the Sky Naked-Eye Astronomy.
Astronomical distances.
Astronomy Visual SOL Review
An experiment to determine the distance to the
12/29/2018 The Sky.
Astronomical Tools.
Angular Resolution 1. 1.
Presentation transcript:

Astronomy Instrumentation Astronomy Summer School for West Africa Daniel Okoh

Astronomy Instrumentation Outline: Telescopes

Astronomy Instrumentation Telescopes: What are they? They are instruments that enable us ‘see’ distant objects by gathering ‘light’ from them

Astronomy Instrumentation Telescopes: What are they? Optical Telescopes Radio Telescopes

Astronomy Instrumentation Optical Telescopes They come in various sizes and form

Astronomy Instrumentation Optical Telescopes: Basic Operation Objective Eye piece

Astronomy Instrumentation Optical Telescopes: Basic Operation

Astronomy Instrumentation Radio Telescopes They need to be big! Really really big!!

Astronomy Instrumentation Why? The Quest for more! Oliver Twist θ = λ D

Astronomy Instrumentation Telescopes in Space Windows and Walls

Astronomy Instrumentation Telescopes in Space Hubble Space Telescope

Astronomy Instrumentation Angular sizes in astronomy θ

Astronomy Instrumentation If the same object is farther away, the angular size is smaller θ1θ1 θ2θ2

Astronomy Instrumentation Objects of different linear sizes can have the same angular sizes θ

Astronomy Instrumentation Activity 1: Estimate the angular size of your full fist at arm’s length

Astronomy Instrumentation Activity 1: Estimate the angular size of your full fist at arm’s length

Astronomy Instrumentation Activity 1: Estimate the angular size of your full fist at arm’s length θ θ y x x tan θ = x/y 2θ = 2 tan -1 (x/y)

Astronomy Instrumentation Activity 1: Estimate the angular size of your full fist at arm’s length

Astronomy Instrumentation Small angle approximation A d D A = D/d * 57.3 degrees

Astronomy Instrumentation Activity 2: Angular size of the Sun A 1.4*10 6 km A = ?? 1.5*10 8 km

Astronomy Instrumentation Activity 2: Angular size of the Moon A 3,475 km A = ?? 384,400 km

Astronomy Instrumentation 0.5 degrees! for both Sun and Moon Sun and Moon same size? Eclipse Implication? Fist or finger to block out the Moon?

Astronomy Instrumentation Telescope Resolutions 2 degrees!?

Astronomy Instrumentation Why Radio Telescopes should be larger than optical telescopes θ = λ D

Astronomy Instrumentation Activity 3: What Radio = Optical telescope ? A 25 cm Optical Telescope will have same resolution as a …… cm Radio Telescope Assume Optical Telescope λ = 500 nm And Radio Telescope λ = 6 cm 30 km ??

Astronomy Instrumentation VLBI (Very Long Baseline Interferometry)

Astronomy Instrumentation Radio Antenna Surfaces

Astronomy Instrumentation Radio Antenna Surfaces

Astronomy Instrumentation Steering in Azimuth And Elevation Where we have to look to see stars and other objects A.0 B. 10 C. 45 D. 90

Astronomy Instrumentation Steering in Azimuth And Elevation A.0 B. 10 C. 45 D. 90

Astronomy Instrumentation Radio Telescope Receivers Similar in many ways to other receivers we use for TV and other radio collections Major difference: Astronomy signals are really very weak compared to other terrestrial signals What constitutes noise is therefore high Signal to noise ratios can be reduced by reducing receiver temperatures There is need to cool the receivers to really low temperatures God Dependent Cryogenic

Astronomy Instrumentation The Address of stars: Right Ascension Declination Room 105 Department of Physics & Astronomy University of Nigeria Nsukka Enugu State Nigeria

Celestial Equator

Astronomy Instrumentation Activity 4: Telescope Pointing Determine the direction (azimuth and elevation) a telescope should point this evening at 6:34 PM to be able to observe α – Centauri from here in Abuja. Assume 2 telescopes at Nsukka and Abuja are to be used for VLBI observations of Sirius at 8:22 AM tomorrow morning. At what directions should each of the telescopes point? Will it be possible to join a telescope at Nanshan, China to this VLBI observation? What about a telescope at Cape Town, South Africa?