Radio Waves Where do they come from?. Radio waves belong to a family The electromagnetic spectrum (EM) is a continuum of waves, sometimes called electromagnetic.

Slides:



Advertisements
Similar presentations
AST 101 Lecture 9 The Light of your Life
Advertisements

Radiation and Spectra Chapter 5
Week 1 C Chapter 5 Electromagnetic Radiation A photon is the smallest element of electromagnetic energy. Photons are energy disturbances moving through.
Atomic structure refresher…..
Wavelength Visible light wavelength Ultraviolet radiation Amplitude Node Chapter 6: Electromagnetic Radiation.
Electromagnetic Radiation (How we get most of our information about the cosmos) Examples of electromagnetic radiation: Light Infrared Ultraviolet Microwaves.
ASTRONOMY 161 Introduction to Solar System Astronomy Class 9.
Electromagnetic Radiation Electromagnetic radiation - all E-M waves travel at c = 3 x 10 8 m/s. (Slower in water, glass, etc) Speed of light is independent.
Light. Photons The photon is the gauge boson of the electromagnetic force. –Massless –Stable –Interacts with charged particles. Photon velocity depends.
PHYS 206 Matter and Light At least 95% of the celestial information we receive is in the form of light. Therefore we need to know what light is and where.
Spectrophotometry Chapter 17, Harris
Chapter 11: Electromagnetic Waves
Unit 4 Atomic Physics and Spectra. The Electromagnetic Spectrum.
Light acts like a Wave Light can be though of as a propagating electromagnetic wave. The wave travels at the maximum allowed speed (c=3x10 8 m/s) through.
Spectral analysis of starlight can tell us about: composition (by matching spectra). temperature (compare to blackbody curve). (line-of-sight) velocity.
Light. What is Light? The third form of energy The only thing astronomers study Electromagnetic radiation The thing that our eyes detect How radio works.
ISP Astronomy Gary D. Westfall1Lecture 6 The Nature of Light Light and other forms of radiation carry information to us from distance astronomical.
The Nature of Light In Astronomy. Herschel’s Infrared experiment Invisible (to our eyes) light immediately beyond the color red is call infrared light.
A) gamma rays b) infrared c) sound d) visible light e) radio Which of these is NOT a form of electromagnetic radiation? Question 1.
ELECTROMAGNETIC RADIATION
ElectroMagnetic Radiation Spectrum The basics about light and waves.
Quiz 1 Each quiz sheet has a different 5-digit symmetric number which must be filled in (as shown on the transparency, but NOT the same one!!!!!) Please.
Light. Light Terminology Which is not a measure we use to identify a type of light? A. Wavelength B. Speed C. Frequency D. Energy.
Index Unit 03 Electron Configuration Module 01: Light as a Wave Based on the PowerPoints By Mr. Kevin Boudreaux, Angelo State Univerisity U03Mod01 Light.
ELECTROMAGNETIC WAVES SECONDARY 3 PHYSICS. WHAT ARE EM WAVES? Electromagnetic waves (EM waves for short) are waves that can travel in a vacuum. These.
Electromagnetic Radiation
© 2010 Pearson Education, Inc. Light and Matter: Reading Messages from the Cosmos.
Chapter 7 Light.
Chapter 3 Light and Matter
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.
Electromagnetic Radiation. Is light a wave or a particle? Yes It’s both, and neither At atomic scales, we have no exact analogs for phenomena For some.
12.6 Light and Atomic Spectra
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.
Properties of Light.
Waves, Sound, and EM Waves. Sound Example of compressional wave Can travel through any type of matter Speed of sound depends on the substance the medium.
Chapter 5: Light.
Physics and the Quantum Mechanical Model
Chapter 13 Section 3 -Quantum mechanical model grew out of the study of light -light consists of electromagnetic radiation -includes radio and UV waves,
Mechanisms of Radio Wave Emission How different mechanisms create Radio Waves that are detectable by Radio Telescopesdifferent mechanisms.
Light 1)Exam Review 2)Introduction 3)Light Waves 4)Atoms 5)Light Sources October 14, 2002.
© 2007 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
Exam #1 Approaching 1 st Exam will be in four days (Friday, Sept. 18) – Chapters closed book/notes exam 40 questions, multiple choice, no calculators.
1 CHAPTER 13: Electrons in the Atom. 2 Quantum Mechanical Model of the Atom and Ernest Schrodinger The model of the atom was developed based on the study.
Electromagnetic Radiation (How we get information about the cosmos) Examples of electromagnetic radiation? Light Infrared Ultraviolet Microwaves AM radio.
Introduction to Spectroscopy Yongsik Lee.
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.
What is light? Light can act either like a wave or like a particle Particles of light are called photons.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 2 Light and Matter.
Electrons and Light. Light’s relationship to matter Atoms can absorb energy, but they must eventually release it When atoms emit energy, it is released.
Radiation (Ch 12 YAC) Thermal energy is emitted by matter as a result of vibrational and rotational motion of molecules, atoms and electrons. The energy.
1.1 What’s electromagnetic radiation
Chemistry Physics and the Quantum Mechanical Model.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 3.
The Study of Light.
Light Monday, October 6 Next Planetarium Shows: Tues 7 pm, Wed 7 pm.
Unit 3.  Much of the information we get in astronomy is carried by “light”.
Light and The Electromagnetic Spectrum Why do we have to study “light”?... Because almost everything in astronomy is known because of light (or some.
Radiation in Astronomy Electromagnetic Radiation I. Electromagnetic Radiation (EM) (EM) Energy travels through space as EM. $ Electromagnetic electric.
© 2017 Pearson Education, Inc.
The Solar System Lesson2 Q & A
Radiation in Astronomy
Stars and Galaxies Lesson2 Q & A
Electromagnetic Radiation
Chapter 17, Section 1 and 2: Nature of Electromagnetic Waves
Light and The Electromagnetic Spectrum
Radiation, Spectroscopy, and Telescopes
Introduction and Basic Concepts
Light and Matter Chapter 2.
Light and The Electromagnetic Spectrum
Friday, Resonance gone bad!
Presentation transcript:

Radio Waves Where do they come from?

Radio waves belong to a family The electromagnetic spectrum (EM) is a continuum of waves, sometimes called electromagnetic radiation. These waves may be created in a number of ways, but all share the following characteristics:

Family Trait 1: No Medium EM waves do not require a medium to move from source to observer. Mechanical waves (such as sound) must travel through a medium –“In space, no one can hear you scream” Tagline from the movie Aliens. This is one (rare) example of Hollywood getting the science right!

Family Trait 2: Same Speed They all travel at the same speed, c, the speed of light in a vacuum –an unfortunate choice, since most people don’t associate light and radio as being part of the same EM spectrum –c ≈ 3 x 10 8 m/s When traveling through a medium, the wave speed, v, is found by the formulav = c/n –where n is the index of refraction of the medium through which the wave is moving

Family Trait 3: Fixed relationship Frequency (f) and wavelength (λ) are related as f = c/λ This is an inverse relationship: the larger (higher) the frequency gets, the smaller the wavelength becomes Note to teachers: Throughout our presentations, we will be using f for frequency. The Greek letter nu ( ν ) is traditionally used for frequency, unfortunately it looks too much like a vee (v) in most fonts. The inconsistency in notation is a constant source of confusion for introductory physics students!

Family Trait 4: Wave behavior Physical Properties –Wavelength –Frequency –Amplitude –Phase Behaviors –Reflection –Refraction –Diffraction –Interference –Doppler Shift

Family Trait 5: Particle Behavior The frequency of an EM wave is related to its energy by the formula f = E/h (more commonly written as E = h·f) h is Planck’s constant = x J/Hz This behavior is attributed to a particle called a photon. That EM radiation appears to be both a wave and a particle is called “wave-particle duality” (to be discussed in another section) The wave behavior dominates the lower frequency spectrum (Radio waves), while the particle nature shows itself more readily in the higher frequencies

EM Spectral Bands For convenience, scientists have divided the spectrum into bands. Those bands are, in order of increasing wavelength (decreasing frequency): Gamma Rays, X-Rays, Ultraviolet, Visible, Infrared, Microwave, and Radio –Microwaves are often considered part of the Radio band Images/animations courtesy NRAO / AUI / NSF Shorter Wavelengths Longer Wavelengths

Anatomy of EM waves EM waves consists of a traveling electric field (E) and a traveling magnetic field (B). The E and B fields are in-phase and orthogonal (at right angles) to one another. Image/animation courtesy NRAO / AUI / NSF

Human detections of EM waves Humans have built-in detectors of EM waves, called eyes. We see EM waves in the Visible part of the Spectrum. Sound is NOT part of the EM spectrum!!! –Sound is a mechanical wave, which requires a medium. Humans have a different set of detectors for mechanical waves, called ears.

Natural Radio Sources Lightning, sparks Solar System – our sun, planets Milky way – star forming regions, old stars, supernova remnants, Galactic center Extragalactic – quasars, radio jets Molecules

What causes Radio waves? Vibrating atoms and molecules –Thermal vibrations due to temperature –Rotational energy for asymmetric molecules Excited atoms and molecules –Absorption/emission of energy (a photon) Accelerating charged particles –Movement in electric or magnetic fields

Two categories of radio sources Broadband –Spectral content of source is spread out across many of the EM bands (radio, visible, x-ray) –Observations made in the radio band should correlate with other parts of the EM spectrum (see Sun) Narrowband –Attributes of the source favor one part of the spectrum (or single frequencies) over others –For example: you can’t see the Ozone in the Mesosphere in the visible spectrum, but we can detect their radio waves

Broadband Radiation Broadband radio signals usually have a thermal origin. –Blackbody radiation (Planck’s Law) All objects radiate EM waves in proportion to their internal temperature –Thermal Bremsstrahlung Acceleration of a charged particle (electron) by another charged particle (nucleus) Includes cyclotron and synchrotron radiation

Blackbody Radiation Any object above absolute zero will emit a broad spectrum of radiation The peak of the curve shifts to shorter wavelengths as temperature increases Image courtesy NRAO / AUI / NSF

Thermal Bremsstrahlung Also called free-free radiation Electrons whizzing by ions Image/animation courtesy NRAO / AUI / NSF

Non-Thermal Radiation Most common: Synchrotron radiation Usually electrons accelerating in a magnetic field Image/animation courtesy NRAO / AUI / NSF

Another Non-Thermal Source MASERs (Microwave Amplification by Stimulated Emission of Radiation) – like a LASER, only at radio frequencies, not visible to the eye Usually associated with molecules in stellar gas clouds Image/animation courtesy NRAO / AUI / NSF

The Sun in different “light” Ultraviolet Radio X-Ray Images courtesy of: NRAO/AUI/NSF/G. Dulk, D. Gary (radio), NSO/AURA/NSF (visible) SOHO/NASA (ultraviolet) and Yohkoh/ISIS/NASA (X-Ray) Visible

Narrowband Radiation Electron energy transitions tend to emit visible or UV radiation Vibrational transitions tend to emit IR radiation (mm waves) Rotational transitions tend to emit microwave radiation (Radio waves) –The molecule must have an electric dipole moment

Example: 21 cm Hydrogen Line Image/animation courtesy NRAO / AUI / NSF

Molecules found in space Simple Hydrides, Oxides, Sulfides, Haloids H 2 CONH 3 CSNaCl HCl SiO SiH 4 SiS AlCl H 2 O SO 2 C 2 H 2 S KCl OCSCH 4 PN AlF Nitriles, Acetylenes and Derivatives C 3 HCNCH 3 CN HNC C 2 H 4 C 5 HC 3 NCH 3 C 3 N HNCO C 2 H 2 C 3 O HC 5 NCH 3 C 5 N HNCS C 5 O HC 7 NCH 3 C 4 H HNCCC C 3 S HC 9 NCH 3 C 4 H CH 3 NC C 4 Si HC 11 N C 2 H 5 CN HCCNC Aldehydes, Alcohols, Aethers, Ketones and Amides H 2 CO CH 3 OH HCOOH CH 2 NH CH 2 C 2 H 2 CS C 2 H 5 OH CH 3 COOH CH 3 NH 2 CH 2 C 3 CH 3 CHO CH 3 SH (CH 3 ) 2 O NH 2 CN NH 2 CHO (CH 3 ) 2 CO H 2 CCO Cyclic Molecules C 3 H 2 SiC 2 C-C 3 H Molecular Ions CH HCO + HCNH + H 3 O + HN 2 - HCS + HOCO + SO + HOC + H 2 D - Radicals OH C 3 H CN C 2 O C 2 S CH C 4 H C 3 N NO NS C 2 H C 5 H HCCN SO SiC CH 2 C 6 H CH 2 CN HCO SiN NH MgNC CP

GHz Ozone Line The Mesospheric Ozone line we detect with the MOSAIC system is a change in rotation of the asymmetric ozone molecule This is a quantum mechanical effect, due to the existence of discrete energy levels of rotational angular momentum

Atmospheric opacity As the illustration below shows, there are many EM frequencies which do not pass through our atmosphere, due to absorption by atoms and molecules present. Images courtesy of NASA