Astronomy 1 – Winter 2011 Lecture 6; January 14 2011.

Slides:



Advertisements
Similar presentations
Astronomy Notes to Accompany the Text Astronomy Today, Chaisson, McMillan Jim Mims.
Advertisements

Physics and the Quantum Mechanical Model
Introduction to Astrophysics Lecture 3: Light. Properties of light Light propagates as a wave, and corresponds to oscillations of electric and magnetic.
My Chapter 22 Lecture.
The Nature of Light Chapter Five.
Light. Properties Light is key to understanding the universe by analyzing light; we learn what planets & stars are made of and their temperature. Light.
Light and Atoms Chapter 3.
4-1 Radiant Energy. Waves  Light travels in Waves similar to ocean waves  Light waves are electromagnetic and consist of an electric and magnetic fields.
ASTRONOMY 161 Introduction to Solar System Astronomy Class 9.
The Nature of Light Chapter Five. Determining the Speed of Light Galileo tried unsuccessfully to determine the speed of light using an assistant with.
Astronomy 101 Section 020 Lecture 5 The Nature of Light John T. McGraw, Professor Laurel Ladwig, Planetarium Manager.
6 Light and Temperature Astronomy: The Science of Seeing.
Characteristics of Light
Astronomy 1 – Winter 2011 Lecture 7; January
4 Light and Temperature Astronomy: The Science of Seeing.
A) gamma rays b) infrared c) sound d) visible light e) radio Which of these is NOT a form of electromagnetic radiation? Question 1.
5 Light and Temperature Astronomy: The Science of Seeing.
© 2004 Pearson Education Inc., publishing as Addison-Wesley Orbital Energy and Escape Velocity orbital energy = kinetic energy + gravitational potential.
Chapter 2 Decoding the Hidden Messages in Starlight
Chapter 5: Light.
Chapter 7 Light.
Chapter 3 Light and Matter
Blackbody Radiation & Atomic Spectra. “Light” – From gamma-rays to radio waves The vast majority of information we have about astronomical objects comes.
Lecture 11 Electromagnetic Waves Chapter 21.8  Outline Discovery and Studies of Electromagnetic Waves Properties of Electromagnetic Waves The Spectrum.
Chapter 3 Radiation. Units of Chapter Information from the Skies 3.2 Waves in What? The Wave Nature of Radiation 3.3 The Electromagnetic Spectrum.
Lecture Outlines Astronomy Today 7th Edition Chaisson/McMillan © 2011 Pearson Education, Inc. Chapter 3.
Stellar Parallax & Electromagnetic Radiation. Stellar Parallax Given p in arcseconds (”), use d=1/p to calculate the distance which will be in units “parsecs”
Guiding Questions 1. How fast does light travel? How can this speed be measured? 2. Why do we think light is a wave? What kind of wave is it? 3. How is.
Light as Messenger.
Energy Energy is a property that enables something to do work
Chapter 4 Light and Atoms Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Electromagnetic Radiation. Electromagnetic Spectrum.
Light and Optics Chapter 22, 23. Light as an Electromagnetic wave  Light exhibits behaviors which are characteristic of both waves and particles Interference,
Donna Kubik PHYS162 Fall, Because of its electric and magnetic properties, light is called electromagnetic radiation. It consists of perpendicular,
Lecture 12 ASTR 111 – Section 002.
Chapter 5: Light.
Electromagnetic Radiation. Electromagnetic Spectrum.
Energy. Radiant Energy Radiant: think light…. How does light carry energy through space???
5-1 How we measure the speed of light 5-2 How we know that light is an electromagnetic wave 5-3 How an object’s temperature is related to the radiation.
The Nature of Light Waves vs. Particles. Particle (Corpuscular) Theory Advocated by Newton ( ) Said energy is carried by tiny particles from source.
The planets move in ellipses with the Sun at one focus. Conic section orbits are a natural outcome of the 1/d 2 nature of the gravitational force, in fact.
Astronomy Astronomy the scientific study of the universe Scientists who study the universe are called astronomers Early Astronomers includes: Nicolaus.
Light.
The Nature of Light Chapter Five. Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I Ch1: Astronomy and the Universe Ch2: Knowing the.
Chapter 3 Radiation. Units of Chapter Information from the Skies 3.2 Waves in What? The Wave Nature of Radiation 3.3 The Electromagnetic Spectrum.
Light. I. What is Light? A. Isaac Newton White light is composed of _____________.
Waves and Properties of Light
Electromagnetic waves are formed when an electric field couples with a magnetic field. The magnetic and electric fields of an electromagnetic wave are.
© 2004 Jones and Bartlett Publishers Chapter thru 4-4 Light and the Electromagnetic Spectrum Courtesy of Astrophysics Data Facility at the NASA Goddard.
Electromagnetic Radiation. Electromagnetic Spectrum.
Astronomy 1010 Planetary Astronomy Fall_2015 Day-17.
 Explain important properties of the electromagnetic spectrum  Describe the important characteristics of light  Discuss and calculate the speed of.
Electromagnetic Radiation, Atomic Structure & Spectra.
Investigating Astronomy Timothy F. Slater, Roger A. Freeman Chapter 2 Decoding the Hidden Messages in Starlight.
Lecture Outline Light ELECTROMAGNETIC SPECTRUM. What Is Light? Take out a piece of paper Answer the question.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 3.
Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I Ch1: Astronomy and the Universe Ch2: Knowing the Heavens Ch3: Eclipses and the Motion.
Diffraction Grating bends white light coming from an object
How do we obtain detailed information about the Universe?
Energy Energy – the ability or the capacity to do work
Light and the Atomic Spectra
MYP Physics Color and Light Practice Quiz
Chemistry 141 Friday, October 27, 2017 Lecture 22 Light and Matter
Light Physics Mrs. Coyle.
DO NOW In your notes… answer the following question using bullet points: What do you know about light? Causes sunburn Allows plants to make food Allows.
WAVE INTERACTIONS.
The Nature of Light Chapter Five.
Chapter 3-1 Notes: The Electromagnetic Spectrum
Light is a WAVE EM Spectrum & EM Waves.
Light and Quantized Energy
Presentation transcript:

Astronomy 1 – Winter 2011 Lecture 6; January

Previously on Astro-1 Newton’s Laws of Motion: 1.Inertia 2.Relation between force and acceleration 3.Action/Reaction Inertial and gravitational mass Newton’s Law of gravity The orbits of planets Tides

Homework – Due 01/19/11 On your own: answer all the review questions in chapters 4 thru 5 To TAs: answer questions 4.41, 4.47, 5.30, 5.33, 5.40, 5.41

Today on Astro-1 The nature of light 1.Speed of light 2.Light is a wave 3.Light is electromagnetic fields Beyond visible light Blackbodies and the temperature of light

Is the speed of light finite? Galileo tried, but couldn’t measure it. In 1676 Ole Rømer noticed that the measurements of the eclipses of Jupiter’s moons were systematically off, depending on how distant Earth was from Jupiter. From this he deduced the speed of light (in terms of AU).

Newton’s used this experiment to prove that prisms do not add color to light but merely bend different colors through different angles. It also proved that white light, such as sunlight, is actually a combination of all the colors that appear in its spectrum.

Question 6.1 (iclickers!) White light passes through a prism and separates into a spectrum of colors. All of these colors are recombined into a single beam by means of a lens. What color is this beam? A) White B) Black (no light left) C) It will be in the ultraviolet region of the spectrum D) It will be in the infrared region of the spectrum

What about “invisible light?” Around 1800 British astronomer William Herschel passed sunlight through a prism and held a thermometer just past the red end of the visible spectrum. The thermometer registered a temperature increase, indicating there was “infrared” light that we could not see.

But what “wiggles” to make the wave? In 1860 James Clerk Maxwell showed that all forms of light consist of oscillating electric and magnetic fields that move through space at a speed of 3.00 × 10 5 km/s or 3.00 × 10 8 m/s. This figure shows a “snapshot” of these fields at one instant. All light is electromagnetic radiation. Maxwell wrote 4 equations that describe all the basic properties of electricity and magnetism.

Frequency and wavelength of an electromagnetic wave ν = frequency of an electromagnetic wave (in Hz – a Hertz is one cycle per second) c = speed of light, 3×10 8 m/s λ = wavelength of the wave (in meters) Example: What is the frequency of visible light at 540 nm?

Question 6.2 (iclickers!) Radio waves travel through space at what speed? A) Much faster than the speed of light B) Faster than the speed of light, since their wavelength is longer C) Slower than the speed of light D) At the speed of light 3x10 8 m/s

An opaque object emits electromagnetic radiation according to its temperature. Temperature is a measure of the average speed of the atoms in an object. Most things in everyday life (people, furniture, etc.) are too cool to emit light, so you can’t see them in the dark.

Astronomers use the Kelvin temperature scale. The “degrees” are the same as the Celsius system, only with 273 added, and they aren’t called degrees (just K). The are no negative numbers – “absolute” zero is the coldest possible temperature.

Summary What is light? Light is electromagnetic radiation

The End See you on Wednesday! (Monday is a holiday)