12/6/2018 Course Overview.

Slides:



Advertisements
Similar presentations
30.1 notes Characteristics of Stars
Advertisements

X-Ray UltravioletVisibleInfraredRadio The Electromagnetic Spectrum and the Universe.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 10 Measuring the Stars.
Types of Galaxies Elliptical: Spiral: Irregular:.
Physics 133: Extragalactic Astronomy and Cosmology Lecture 14; March
CHARACTERISTICS OF STARS. A star is a ball of gas that gives off a tremendous amount of electromagnetic radiation. The energy comes from a process called.
Electromagnetic Spectrum
COSMOLOGY AND THE ORIGIN OF LIFE ASTRONOMY 123. Cosmology  Cosmology is the empirical study of the organization, structure and evolution of the Universe.
Chapter 30 Section 4 Handout
WHAT ASTRONOMERS LEARN ABOUT THE ELECTROMAGNETIC SPECTRUM.
Objective: I will relate the electromagnetic spectrum to wavelengths of light energy. 9/30/14.
GCSE Science A Physics 1 Space Learning Outcomes Appreciate the range of distance scales appropriate when discussing the universe. Know that atoms of a.
Curriculum Where is HOU used? Not many astronomy courses in high school.  Physics  Math  Earth Science  Integrated Science.
Big Bang Theory Created by Evan Chernenko Click to Start.
Electromagnetic Spectrum  EM Spectrum – a continuous range of wavelengths  Longer wavelengths = low energy  Ex. – radio waves, microwaves  Shorter.
Astrophysics and Cosmology How do we know what we know about the universe around us?
Stars and Galaxies 28.1 A Closer Look at Light Chapter 28.
Chapters 17,18: Cosmology and Life in the Universe.
What Can Spectroscopy Tell Us?. Atom or Molecular Fingerprints Every atom or molecule exists in its own unique energy state. This energy state is dependent.
Astronomy Chapter 26 Studying Space. Astronomy  The scientific study of the universe Benefits  Exciting discoveries Black holesBlack holes pulsarspulsars.
So You Wanna’ Be A STAR Characteristics of Stars Stellar Evolution.
Stars, Galaxies, and the Universe Section 1 Section 1: Characteristics of Stars Preview Key Ideas Analyzing Starlight Stellar Motion Distances to Stars.
© Sierra College Astronomy Department 1 Astronomy 10 Elementary Astronomy COURSE GOALS & OBJECTIVES.
Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.
Electromagnetic Radiation (Light – the Supreme Informant!)
5.1 Electromagnetic Radiation. Wave motion The transfer of energy without matter is called wave motion Two Types.
Atoms & Starlight (Chapter 6).
What is Astronomy? An overview..
EARTH & SPACE SCIENCE Chapter 30 Stars, Galaxies, and the Universe
Big Bang Related Websites: 4- Cosmology; Black Holes and Big Bang Particle Make-up of the Atom.
Astronomy 101 Cumulative Presentation Aleks Alunans.
Stars, Galaxies, and the Universe Section 1 Section 1: Characteristics of Stars Preview Key Ideas Analyzing Starlight Stellar Motion Distances to Stars.
What do we know about the universe?
Bell Quiz 1. What does NASA stand for? 2. How long does it take for light from the sun to get to the Earth? 3. What does this symbol mean? ∞ 4. Who was.
NAME DATE The Unit Organizer BIGGER PICTURE LAST UNIT /Experience NEXT UNIT /Experience UNIT SELF-TEST QUESTIONS is about... UNIT RELATIONSHIPS UNIT SCHEDULE.
Study Notes for Chapter 30: Stars, Galaxies, and the Universe.
Stars Goal: Compare star color to star temperature.
Cosmic address The astronomical unit and the light year Dark matter and dark energy Atoms Matter Forces.
Chapter 30.1: Characteristics of Stars. Characteristics of Stars A star is a _________________________ _______________________________ ____. Size varies.
Stars, Galaxies, and the Universe Section 4 Section 4: The Big Bang Theory Preview Key Ideas Hubble’s Observations A Theory Emerges Big Bang Theory Universal.
COSMOLOGY The study of the origin, structure, and future of the universe.
SCI 151 Academic Success /snaptutorial.com For more course Tutorials
1 Why Learn about Atomic Structure? Knowing the structure of atoms tells us about their –chemical properties –light-emitting properties –light-absorbing.
© 2017 Pearson Education, Inc.
Studying the Sun Notes H- Study of Light Chapter 24
Chapter 30 Section 4 Big Bang Theory.
The Big Bang Theory.
Outline of Space Unit Earth’s Moon (ch. 25)
The Universe.
BIG BANG THEORY.
Origin of the Universe.
Energy Nuclear Fission Nuclear Fusion
Astronomy – A Study of “Our Space”
What is Astronomy? An overview..
Electromagnetic Radiation
Our Place in the Universe
What is Astronomy? An overview..
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
Solar Spectra: A look into temperatures and elements present on the sun.
Section 1: Characteristics of Stars
The Electromagnetic Radiation
Understand the electromagnetic spectrum and how it is organized.
Characteristics of Stars
BIG BANG THEORY.
Cosmology = Big Questions
How Do Astronomers Gather Information About Space?
Section 1: Characteristics of Stars
Chapter 1 The Scale of the Cosmos
What is Astronomy? An overview..
Presentation transcript:

12/6/2018 Course Overview

Scale of the Cosmos Measuring Distances

The Early Astronomers

Motion

Astronomical Tools Measurements Telescopes Spectrographs

Atom and Starlight The Atom The electromagnetic spectrum Stellar Spectra

The Sun Physical Properties Energy Mechanism

12/6/2018 Stars

12/6/2018 Stars Evolution

12/6/2018 Galaxies

12/6/2018 Cosmology

12/6/2018 Dark Matter and Energy

Origins of Life Evolution of Life of Earth 12/6/2018 Origins of Life Evolution of Life of Earth Search For Intelligent Life Forms

Feedback: Privacy Policy Feedback
Do Not Sell My Personal Information
About project: SlidePlayer Terms of Service

© 2024 SlidePlayer.com Inc. All rights reserved.