Rainbows from Space. Astronomer’s Tools Telescopes Telescopes –On Earth or in Earth orbit Cameras Cameras Prisms (spectroscope) Prisms (spectroscope)

Slides:



Advertisements
Similar presentations
Excited Elements.
Advertisements

Spectroscopy Study Guide
Fingerprints in Sunlight Understanding Spectroscopy
1 Fingerprints in Sunlight Understanding Spectroscopy Stanford University Solar Center.
Stars, starlight AND The Big Bang. OUTCOME QUESTION(S): S1-4-06: How do astronomers measure the great distances in the universe? S1-4-07: What is the.
Spectroscopy: and finding out the elements of deep space objects.
ASTR100 (Spring 2008) Introduction to Astronomy Properties of Light and Matter Prof. D.C. Richardson Sections
Spectral analysis of starlight can tell us about: composition (by matching spectra). temperature (compare to blackbody curve). (line-of-sight) velocity.
Test #1, Wednesday, Feb 10 I will post a review for Test 1 in the A101 homepage under the link to “Lectures” this week. I will tell you the topics to review.
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.
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.”
CHAPTER 28 STARS AND GALAXIES
Chapter 2 Decoding the Hidden Messages in Starlight
< 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.
The Electromagnetic Spectrum
Earth Science 24.1 The Sun: Study of Light
Key Ideas How are stars formed?
Learning from Light Our goals for learning What are the three basic types of spectra? How does light tell us what things are made of? How does light tell.
Astrophysics and Cosmology How do we know what we know about the universe around us?
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.
Blackbody Radiation And Spectra. Light is a form of _______. Why is this important? With very few exceptions, the only way we have to study objects in.
FYNvpI. Topic 3: The Spectrocope: New Meanings in Light Science 9 - Space.
Stars and Galaxies 28.1 A Closer Look at Light Chapter 28.
WHAT ARE STARS? Huge, hot balls of gas that are trillions of kilometers away from the Earth.
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.
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.
The UniverseSection 1 Section 1: The Life and Death of Stars Preview Key Ideas Bellringer What Are Stars? Studying Stars The Life Cycle of Stars.
READING Unit 22, Unit 23, Unit 24, Unit 25. Homework 4 Unit 19, problem 5, problem 7 Unit 20, problem 6, problem 9 Unit 21, problem 9 Unit 22, problem.
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.
Astronomy Big Idea: The sun is one of billions of stars in one of billions of galaxies in the universe.
The UniverseSection 1 Key Ideas 〉 How are stars formed? 〉 How can we learn about stars if they are so far away? 〉 What natural cycles do stars go through?
Spectral Analysis Gleaming Information From The Stars.
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.
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.
The Electromagnetic Spectrum in our Universe. Background info. ★ Everything astronomers know about the universe comes from studying light from distant.
Tools of Modern Astronomy
We see light as color and brightness It’s actually electromagnetic radiation: Partly electric, partly magnetic Flows in straight line (radiates)
Spectroscopy and Atoms
Deep Space and Solar System New Test/New Quiz. Universe Biggest Oldest Galaxy Milky Way Solar System Star Sun PlanetMoon Smallest Youngest.
Starlight What is it? What does it tell us? Write down all notes in RED.
Electromagnetic Radiation. The transfer of energy by electromagnetic waves. The speed of an electromagnetic wave is a product of its wavelength and frequency.
Space Explorations Science 9. THE SPECTROSCOPE: NEW MEANINGS IN LIGHT Topic 3.
4. Complex Knowledge: demonstrations of learning that go aboveand above and beyond what was explicitly taught. 3. Knowledge: meeting the learning goals.
Starter 1.Where are most asteroids located? 2.Describe the structure of a comet. 3.Where do short period comets come from? What about long period comets?
The Spectroscope.
Using Technology to Interpret Space
Atoms and Spectra.
Spectroscopy Lecture.
Prepare your scantron: Setup:
The Spectroscope: New Meanings in Light
 Spectroscopy continued 
Stars, starlight AND Light Information. Stars, starlight AND Light Information.
Stars and spectral analysis:
ELECTROMAGNETIC SPECTRUM
Stars and HR Diagrams.
Unit III Part 1: Weathering and Erosion
 Spectroscopy continued 
Optical Telescopes, Radio Telescopes and Other Technologies Advance Our Understanding of Space Unit E: Topic Three.
1. People have studied the stars for centuries
5.4 Learning from Light Our goals for learning
The Spectroscope: New Meanings in Light
5.4 Learning from Light Our goals for learning
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.
The Sun.
Unit E – Space Exploration
A Closer Look at Visible Light
Topic 3 – Part III The Doppler Effect
Light: Electromagnetic spectrum & Doppler Shift
Presentation transcript:

Rainbows from Space

Astronomer’s Tools Telescopes Telescopes –On Earth or in Earth orbit Cameras Cameras Prisms (spectroscope) Prisms (spectroscope) Photometer (measures brightness) Photometer (measures brightness) Computer Computer

Orion Nebula

Eagle Nebula

Crab Nebula

Light from space Because most objects in space are too far away to visit, examining their light is the only tool we have to explore them. Because most objects in space are too far away to visit, examining their light is the only tool we have to explore them. Distance, temperature, composition, and motion details are a few of the things we can deduce from their light. Distance, temperature, composition, and motion details are a few of the things we can deduce from their light.

Spectroscopy A close up look at the color of light White light is a mixture of all the colors. White light is a mixture of all the colors. Isaac Newton showed that a prism can show the colors that make up white light. Isaac Newton showed that a prism can show the colors that make up white light. Isaac Newton born: December 25, 1642 Woolsthorpe, England died: March 20, 1727

White light is composed of many colors Newton passed sunlight through a piece of glass called a PRISM, and produced colors. Newton passed sunlight through a piece of glass called a PRISM, and produced colors. He called these colors the spectrum, from the word spectre, meaning ghost. He called these colors the spectrum, from the word spectre, meaning ghost.

Rainbow A Rainbow is formed when sunlight passes through raindrops, which act like little prisms. A Rainbow is formed when sunlight passes through raindrops, which act like little prisms.

Spectroscope Today astronomers use very accurate prisms, called spectroscopes, to find out about objects in space. Today astronomers use very accurate prisms, called spectroscopes, to find out about objects in space.

Personal Spectroscope Astronomers’ spectroscopes are quite elaborate, but simple spectroscopes are cheap and easy to use. Astronomers’ spectroscopes are quite elaborate, but simple spectroscopes are cheap and easy to use. Many spectroscopes use a grating, a piece of plastic or glass with thousands of lines scratched in it. Many spectroscopes use a grating, a piece of plastic or glass with thousands of lines scratched in it.

Observing Spectra Look at a white light bulb with the diffraction grating and see the colors – like a rainbow. Look at a white light bulb with the diffraction grating and see the colors – like a rainbow.

Glowing Gases View the gas tubes. View the gas tubes. Every glowing gas has a unique pattern of colors, like a fingerprint is unique to a person. Every glowing gas has a unique pattern of colors, like a fingerprint is unique to a person. Record the colors you see for each gas Record the colors you see for each gas

Gas Tube Spectra Hydrogen Hydrogen Helium Helium Neon Neon Oxygen Oxygen Mercury Mercury

Mystery Gas View the mystery gas and record its pattern of colors. View the mystery gas and record its pattern of colors. Now refer to your drawings of the other gasses and see if you can recognize any of the line patterns. Now refer to your drawings of the other gasses and see if you can recognize any of the line patterns. Can YOU tell what the gas in the mystery tube is? Can YOU tell what the gas in the mystery tube is?

Pleiades

Horsehead Nebula

Bright and Dark Spectra Clouds of glowing gas show bright lines Clouds of glowing gas show bright lines High pressure glowing gas shows continuous colors High pressure glowing gas shows continuous colors Light from high pressure gas passing through cooler gas gives dark lines Light from high pressure gas passing through cooler gas gives dark lines

The Sun’s Spectrum By passing sunlight through a spectroscope we can determine all of the chemical elements that make up the Sun. By passing sunlight through a spectroscope we can determine all of the chemical elements that make up the Sun.

What’s the Sun made of? By matching the dark lines in the Sun’s spectrum with lines observed of elements in a laboratory you can determine what elements are present. By matching the dark lines in the Sun’s spectrum with lines observed of elements in a laboratory you can determine what elements are present.

Solar Spectrum

Doppler Effect Christian Doppler first showed that when a source of light or sound is coming towards you or going away, the color or pitch of the light or sound is raised or lowered. Christian Doppler first showed that when a source of light or sound is coming towards you or going away, the color or pitch of the light or sound is raised or lowered. Christian Doppler born: 29 November 1803 Salzburg, Austria died: March 17, 1853

Sound When a source of sound is coming toward the observer, the pitch of the sound is raised. When a source of sound is coming toward the observer, the pitch of the sound is raised. When a source of sound is going away from the observer the pitch is lowered. When a source of sound is going away from the observer the pitch is lowered.

Sound is a vibration Sound vibrations travel through air like waves in the ocean Sound vibrations travel through air like waves in the ocean

Doppler Effect Demo Sounder first comes toward you, then moves away. Sounder first comes toward you, then moves away. The pitch will be higher when coming toward you, and lower going away. The pitch will be higher when coming toward you, and lower going away. Sounder coming toward you – higher pitch Sounder moving away from you – lower pitch

Why? Sound vibrations travel through air outward from the source. Sound vibrations travel through air outward from the source. When the sound source is moving the waves bunch up, or stretch out. When the sound source is moving the waves bunch up, or stretch out. Low pitched SoundHigh pitched Sound Observer here hears higher pitch Observer here hears lower pitch

Light When a source of light is coming toward the observer, the color of the sound is made bluer. When a source of light is coming toward the observer, the color of the sound is made bluer. When a source of light is going away from the observer the color is reddened. When a source of light is going away from the observer the color is reddened.

Doppler Effect on Light If the line pattern is shifted to the blue end the source is coming towards us. If the line pattern is shifted to the blue end the source is coming towards us. If shifted to the red end, it is moving away. If shifted to the red end, it is moving away.

Using the Doppler Effect to Detect an Unseen Planet If a star has a planet orbiting it, the planet will tug on the star due to its gravity. If a star has a planet orbiting it, the planet will tug on the star due to its gravity. As the planet orbits the star it will tug first on one side of the star, then on the other. As the planet orbits the star it will tug first on one side of the star, then on the other. gravity

Detecting a planet So the star first moves toward us, then away. So the star first moves toward us, then away. When moving towards us the spectrum will be a tiny bit bluer, and redder when moving away. When moving towards us the spectrum will be a tiny bit bluer, and redder when moving away. Unseen planet’s orbit

Lots of Planets Found The number of Extra-Solar planets discovered is now over 150 and growing every month. The number of Extra-Solar planets discovered is now over 150 and growing every month.

Artist’s Conception of 6-8 Earth Mass Planet Orbiting Star Gliese 876