Chemical Composition of Stars

Slides:



Advertisements
Similar presentations
David - Doppler He is known for the principle he proposed he first proposed in concerning the colored light of double stars in He hypothesized that.
Advertisements

Origin of the Universe. Origin and Age of the Universe Humans have observed celestial objects for thousands of years contemplating their place in the.
Spectroscopy Study Guide
Fingerprints in Sunlight Understanding Spectroscopy
1 Hydrogen in the Milky Way Hydrogen is the most abundant element in our galaxy. The 21-cm Line.
The Doppler Effect.
Spectroscopy: and finding out the elements of deep space objects.
Spectral analysis of starlight can tell us about: composition (by matching spectra). temperature (compare to blackbody curve). (line-of-sight) velocity.
Red Shift, Blue Shift Radial velocity – the movement of an object toward or away from us An Observer Velocity away Velocity toward.
A photon checks into a hotel. The desk clerk asks, “Do you need help with your luggage?” The photon replies, “I don’t have any. I’m travelling light.”
< BackNext >PreviewMain Section 1 Stars Chapter 15 Bellringer List ways that stars differ from one another. How is the sun like other stars? How is it.
Before the bell rings, in your notes, write out the important aspects of a correctly designed experiment. Make sure to include a description of your variable.
Spectral Emission.
Stars and Galaxies 28.1 A Closer Look at Light Chapter 28.
UNIVERSE PART II: Spectral Analysis. POWERPOINT “Spectral Analysis” QUIZ #2 – Due Tuesday, September 15 1) What is a spectroscope? 2) What is the difference.
Science 9: Unit E: Space Exploration Topic 3: Spectroscopy and the Doppler Shift.
Rainbows from Space. Astronomer’s Tools Telescopes Telescopes –On Earth or in Earth orbit Cameras Cameras Prisms (spectroscope) Prisms (spectroscope)
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.
Spectra  Chemistry and Doppler Effect Lecture 10.
Chapter 5 Light: The Cosmic Messenger. 5.2 Learning from Light Our goals for learning What types of light spectra can we observe? How does light tell.
How are stars classified? What is an H-R diagram and how do astronomers use it?
A105 Stars and Galaxies  Homework 4 due Sept. 21  Telescopes  Read units 26, 27  News Quiz Tuesday Today’s APODAPOD ROOFTOP TONIGHT 8:30.
Copyright © by Holt, Rinehart and Winston. All rights reserved. CHAPTER 2 STARS, GALAXIES AND THE UNIVERSE.
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 Doppler Effect.
IP Light and the doppler effect © Oxford University Press 2011 Light and the doppler effect.
Chapter 27 Stars and Galaxies Section Characteristics of Stars A star is a body of gases that gives off a tremendous amount of radiant energy.
Astronomy Big Idea: The sun is one of billions of stars in one of billions of galaxies in the universe.
Origin of the Universe. Origin and Age of the Universe Humans have observed celestial objects for thousands of years contemplating their place in the.
Chapter 30.1: Characteristics of Stars. At the center of the most violent starburst region in the local universe lies a cluster of brilliant, massive.
Prepare your scantron: Fill in your name and fill the bubbles under your name. LAST NAME FIRST, First name second Put your 4-digit code instead of “ IDENTIFICATION.
Spectral Analysis Gleaming Information From The Stars.
Aim: How does light provide evidence of the universe’s composition? I. Light – a form of electromagnetic radiation. A. electromagnetic radiation – energy.
How do we really know what's out there? Space is a pretty big place and, after all, we've never been farther from earth than our moon. How do we know what.
Waves. The time it takes for one wavelength to pass is called the period. The number of wavelengths passing at a given time is called frequency.
The Electromagnetic Spectrum in our Universe. Background info. ★ Everything astronomers know about the universe comes from studying light from distant.
Electromagnetic Spectrum. Element Spectrum Each element has a spectral “fingerprint” — a pattern of bright or dark lines that is UNIQUE to that element.
An Expanding Universe Redshift, Blueshift and the Doppler Effect.
Red Shift – Expanding Universe 5 a day. 1. If a star or galaxy is moving away from us, its wavelength will shift which way? 2. If a star or galaxy is.
EARTH & SPACE SCIENCE Chapter 30 Stars, Galaxies, and the Universe
What do we know about the universe?
The Doppler Effect The sound of a police car siren changes as it moves past you. The pitch of the siren seems to change. Ahead of the car, the sound waves.
EVIDENCE SUPPORTING THE EXPANDING UNIVERSE The Electromagnetic Spectrum and The Doppler Effect.
Starlight What is it? What does it tell us? Write down all notes in RED.
WHEN YOU WISH UPON A STAR. Spectral lines of elements are unique to each element No other element has these exact spectral lines.
8.8A TO DESCRIBE COMPONENTS OF THE UNIVERSE, INCLUDING STARS, NEBULAE, AND GALAXIES, AND USE MODELS SUCH AS THE HERZTSPRUNG-RUSSELL DIAGRAM FOR CLASSIFICATION.
Chapter 19 Stars, galaxies and the Universe. Section 1 Stars.
Space Explorations Science 9. THE SPECTROSCOPE: NEW MEANINGS IN LIGHT Topic 3.
COLOR By: Me. Color When you put sunlight into a triangular-shaped glass, you can break up the light into a spread of colors of the spectrum. White color.
The Spectroscope.
Using Technology to Interpret Space
Spectroscopy Lecture.
Most of what is known about stars comes from spectral studies.
Prepare your scantron: Setup:
Add to table of contents:
Stars and spectral analysis:
How do scientists know what stars and planets are made of?
Which color of visible light has the shortest wavelength?
The Study of Light Picture taken
Redshift Ms. Griswold 5/14/2014.
Characteristics of Stars
Electromagnetic Radiation
Optical Telescopes, Radio Telescopes and Other Technologies Advance Our Understanding of Space Unit E: Topic Three.
Star Light The spectrum of light a star emits can tell us what type of atom is present both inside the core and in its atmosphere. The pattern of dark.
WHEN YOU WISH UPON A STAR
Chapter 19 Bellringer What are stars made of?
Spectral analysis of starlight can tell us about:
Chapter 3 Review Worksheet
Characteristics of Stars
Unit E – Space Exploration
Presentation transcript:

Chemical Composition of Stars

What is the purpose of fingerprints? How are fingerprints useful? Where do you see fingerprints being used?

Activity Students are to press their thumb gently onto the ink pad and then press their thumb onto the notes Students should wipe the ink off their thumb with the wipe provided Students should compare/contrast their fingerprint with their neighbor.

Types of Fingerprints

Review-Electromagnetic Spectrum

Spectrometer Students will put on the glasses provided and take note of the spectral lines that appear on the right (3:00 position) Students should write notes as to what colors are being observed and in which order the colors appear Students will reproduce what they observed using colored pencils on the spectrometer worksheet provided for two gases

Class Discussion How did the fingerprint activity relate to the spectrograph activity? Each person has a unique set of fingerprints and each element of a star has a unique line spectrum By comparing a star’s spectrum with the spectrum of known elements, astronomers can infer how much of each element is found in the star

Examples of Line Spectrums of Elements

Chemical Composition Of Stars In Clusters Can Tell History Of Our Galaxy and Others Doppler effect If the spectral lines are shifted toward the blue end of the spectrum for the star, then the star is moving towards us. If the dark lines are shifted toward the red end of the spectrum for the star, it is moving away from us.

Animation http://www.classzone.com/books/earth_science/terc/content/visualizations/es2802/es2802page01.cfm