ASTR 567: Observational Techniques in Astronomy. ASTR 567: Grading Scheme Start of lecture quizzes………………….. 10% Homeworks……………………………………..25% Highest of.

Slides:



Advertisements
Similar presentations
Early Quantum Theory and Models of the Atom
Advertisements

Universe: from Beginning to End
AST 101 Lecture 9 The Light of your Life
Atomic structure refresher…..
Review. The Wave Nature of Light Important: When a light wave travels from one medium to another, its frequency does not change, but its wavelength does.
Fall 2014Astron 1Instructor: Babar Ali Visible spectrum of the sun.
Light. Photons The photon is the gauge boson of the electromagnetic force. –Massless –Stable –Interacts with charged particles. Photon velocity depends.
The dual nature of light l wave theory of light explains most phenomena involving light: propagation in straight line reflection refraction superposition,
Chapter 18 The Electromagnetic Spectrum and Waves
Light as a Wave One way to think about light is as a traveling wave A wave is just a disturbance or vibration in some medium – (water, air, space) A wave.
The Electromagnetic Spectrum
Structure of Atoms Rutherford's model of the atom was a great advance, however, it does not give an satisfactory treatment of the electrons. To improve.
Waves Light Up the Universe! Dr. Laura A. Whitlock NASA’s Swift Mission Kara C. Granger Maria Carrillo HS.
Neutron Stars and Black Holes PHYS390: Astrophysics Professor Lee Carkner Lecture 18.
ISP Astronomy Gary D. Westfall1Lecture 6 The Nature of Light Light and other forms of radiation carry information to us from distance astronomical.
The Big Bang: Light, Matter and Darkness SOAR Fall 2004.
The Interaction of Light and Matter Commonly drawn symbol for photon A more physically meaningful symbol for the photon as an energy wavepacket confined.
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.
Classical ConceptsEquations Newton’s Law Kinetic Energy Momentum Momentum and Energy Speed of light Velocity of a wave Angular Frequency Einstein’s Mass-Energy.
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.
Review for Exam 3.
Astronomy Unit Review. Topics Solar system(planets, asteroid belt, meteor, meteoroid, meteorite, comet etc) Measurement (AU and Light Years) Sun (structure;
 Celestial Sphere  Imagine a sphere that surrounds our planet in which all the stars are attached. This sphere is allowed to rotate freely around the.
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.
CHAPTER 3 (p ) Light. Only a very small range of wavelengths, 400nm to 700nm, are visible to humans. Wavelengths are very small so astronomers use.
The Evolution of the Universe Nicola Loaring. The Big Bang According to scientists the Universe began ~15 billion years ago in a hot Big Bang. At creation.
1 Lectures on Medical Biophysics Department of Biophysics, Medical Faculty, Masaryk University in Brno.
P+ n e- By 1932, the basic building blocks of matter were known: MODERN PHYSICS.
Cosmology I & II Fall 2012 Cosmology Cosmology I & II  Cosmology I:  Cosmology II: 
Waves, Photons & the EM Spectrum  Astronomers obtain information about the universe mainly via analysis of electromagnetic (em) radiation: visible light.
Modern Physics Modern Physics Global Mechanics Global Mechanics Astrophysics Astrophysics Cosmology and The Little Bang Cosmology and The Little Bang.
Measuring Light Quantitatively Spectroscopy: measuring wavelengths ( ) and frequencies (  ) emitted or absorbed by matter; composition of stars Photometry:
Intro to Cosmology! OR What is our Universe?. The Latest High Resolution Image of the Cosmic Microwave Background Radiation Low Energy RegionHigh Energy.
Solar system: 9 light hours diameter. Spiral galaxy: 80,000 light years diameter.
The Energy in our Universe Dr. Darrel Smith Department of Physics.
The Dark Side of the Universe
Measuring the Universe. Electromagnetic Radiation.
Cosmology, Cosmology I & II Fall Cosmology, Cosmology I & II  Cosmology I:  Cosmology II: 
Radio Waves Interaction With Interstellar Matter
© Sierra College Astronomy Department 1 Astronomy 10 Elementary Astronomy COURSE GOALS & OBJECTIVES.
Physics 2170 – Spring Investigating electromagnetic radiation First midterm is 7:30pm on 2/17/09 Problem.
Atmospheric CO2 reaches 400 PPM
Final Review December 4, 2002 Final Exam will be held in Ruby Diamond Auditorium NOTE THIS!!! not UPL Dec. 11, am-noon Bring your ID, calculator.
Atom and Light ASTR 14: Exploring the Universe. 2 Outline Nature of Light Basic Properties of Light Atomic Structure Periodic Table of the Elements Three.
Chapter 7 Atomic Structure. Light  Made up of electromagnetic radiation  Waves of electric and magnetic fields at right angles to each other.
I know what you are thinking. Why neutrinos are the coolest thing you will never see. 1.They are massless. 2.They can travel through anything, unlike.
Gravitational Waves.
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.
Electromagnetic Spectrum. What kind of wave is electromagnetic radiation? A sound wave is a oscillation of air. A water wave is an oscillation of the.
Solids and Light – Introduction to Light
Midterm Exam Material Covered –Chapter 1 to 6 Format of Exam –Multiple-Choice Questions: 40 to 50 questions –Facts –Concepts –Reasoning –Quantitative --
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh) Nuclear and Radiation Physics Before we start, let us tackle.
Announcements Final exam is Monday, May 9, at 7:30 am. –Students with last names A-K go to 225 CB. –Students with last names L-Z go to 300 CB. –All students.
Planet solar system galaxy local cluster supercluster Intro to Cosmos scale Powers of 10 our place in the cosmos.
High energy Astrophysics Mat Page Mullard Space Science Lab, UCL 1. Overview.
Tubular Nuclear Spectacular Spectra Reaction Action The “App”le of My Eye The Light Fantastic.
Astronomy 1020-H Stellar Astronomy Spring_2016 Day-12.
MEDICAL IMAGING Dr. Hugh Blanton ENTC Lecture 1 EM Introduction.
High Energy Observational Astrophysics. 1 Processes that emit X-rays and Gamma rays.
 Draw a diagram of the relative positions of the sun, moon, and Earth during a  Full moon  New moon.
Modern Physics Wave-Particle Duality Model of the atom Radioactivity / Four Forces of nature.
 Matter is any thing that occupies space & has mass  Present in three states: solid, liquid, & gas  It could be divided into elements & compounds 
Wave Particle Duality.
Atomic Structure & Periodicity
Very Basic Electromagnetism
THEORIES OF LIGHT Is light a wave or a stream of particles?
Chapter 22 The Nature of Light
Stars Notes Ch. 28.
Bell Work: Spring Break
Electromagnetic Spectrum
Presentation transcript:

ASTR 567: Observational Techniques in Astronomy

ASTR 567: Grading Scheme Start of lecture quizzes………………….. 10% Homeworks……………………………………..25% Highest of two midterm grades……….25% Telescope Proposal………………………….15% Final Exam……………………………………….25%

ASTR 370: Cosmology Offered this semester: Prof. Peterson Early history of the Universe, big bang, inflation, structure formation, dark matter and dark energy

ASTR 561: Galaxies and Large Scale Structure Offered this semester: Prof. Giannios Galactic structure and stellar dynamics, ISM, galaxy formation, galaxy clusters, dark matter.

ASTR 562: High Energy Astrophysics Offered in spring semester: Prof. Lyutikov Physics of exotic objects: neutron stars, white dwarfs, supernovae, black holes, magnetars

ASTR 563: Astroparticle Physics Typically offered in spring semesters Covers neutrinos, cosmic rays, dark matter, gravitational waves

Reading for next time: Lawrence section 1.1.1

Gathering Data in Astronomy What are some ways we gather information about the cosmos?

In Situ Solar system probes Apollo lunar landings Particles with Mass Cosmic rays Neutrinos Meteorites Solar wind Massless Particles Gravitons Photons Gathering Data in Astronomy

Astronomical Techniques – Photometry – Spectroscopy – Polarimetry – Astrometry – Imaging All of these exploit the wave and/or particle properties of E/M radiation All photon-based astronomical measurements can be classified as one or more of:

Electromagnetic Radiation Light exhibits wave-particle duality: – Massless light quanta: photons, carry a specific energy: E = hν = hc/λ h = Planck’s constant = × m 2 kg / s c = speed of light = m / s Light can also reflect, refract, diffract, polarize, and interfere with itself.

Production of E/M Waves Electromagnetic waves are created by accelerating a charged particle E/M radiation emitted from a vertically oscillating magnetic dipole

Production of E/M Waves In the quantum view, a photon is created when an electron jumps to a lower energy state or a free electron binds to an atom.

Production of E/M Waves Other types of quantum transitions that produce photons: Electron spin flip in hydrogen Vibration & Rotation Modes

Production of E/M Waves Nuclear processes can also produce photons: – electron+positron annihilation – nuclear fission and fusion – radioactive decay

E/M Wave Structure E/M wave requires no medium (‘ether’) E and B fields oscillate  to each other, sustaining the wave In a vacuum, wave travels in a straight line (geodesic) at constant speed c = λν

E/M Bands Divisions between bands are approximate: none are officially standardized. Sub-divisions are common e.g., near-IR, far-UV, soft X-ray – near, soft : longer λ – far, hard : shorter λ