Light. Review Question What is light? Review Question How can I create light with a magnet?

Slides:



Advertisements
Similar presentations
24.1 The Study of Light Visible light from sun is only a small part of what’s emitted Electromagnetic waves Radio waves, IR, light, UV,
Advertisements

Big Questions If astronomers measure an object’s apparent brightness (flux), what do they need to know to figure out how far away that object is? Why are.
24.1 The Study of Light.
Radiation:.
Light and Spectroscopy
Light and Atoms Chapter 3.
Exam 1 Next Tuesday Covers chapters 1, 2, S1, 4, 5 and 6 2 essay questions/25 multiple choice Allowed one standard sized sheet of notes, writing on one.
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.
Frequency and Wavelength How are frequency, wavelength, and speed related for electromagnetic radiation in empty space? –speed = frequency x wavelength,
NATS From the Cosmos to Earth The Doppler Effect.
Astro 201: Sept. 14, 2010 Read: Hester, Chapter 4 Chaos and Fractal information on class web page On-Line quiz #3: available after class, due next Tuesday.
Spectrum from a Prism. Example of a Spectrum Kirchoff’s Laws.
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.
© 2004 Pearson Education Inc., publishing as Addison-Wesley Orbital Energy and Escape Velocity orbital energy = kinetic energy + gravitational potential.
CHAPTER 28 STARS AND GALAXIES
Chapter 28.1 Electromagnetic Spectrum. Scientists learn about the Universe by collecting Wave- Energy from the Electromagnetic Spectrum.
Chapter 5 Light: The Cosmic Messenger. 5.1 Basic Properties of Light and Matter Our goals for learning: What is light? What is matter? How do light and.
Chapter 2 Decoding the Hidden Messages in Starlight
ISNS Phenomena of Nature The Eye The eye consists of pupil that allows light into the eye - it controls the amount of light allowed in through the.
How do Astronomers know what they know? Almost everything we know about Astronomy was learned by gathering and studying light from distant sources Properties.
Chapter 3 Light and Matter
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.
Prentice Hall EARTH SCIENCE
Chapter 5 Light: The Cosmic Messenger Light in Everyday Life Power – describes the rate of energy use. 1 Watt = 1 Joule/sec. Spectrum – The component.
Chapter 5 Light: The Cosmic Messenger
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.
Stars and Galaxies 28.1 A Closer Look at Light Chapter 28.
Scientists learn about the Universe by collecting Wave- Energy from the Electromagnetic Spectrum.
Astronomy Chapter 4 Review Game
Properties of Light.
Feb. 3, 2011 Ch 5b. 5.1Basic Properties of Light and Matter Light: electromagnetic waves 1. Velocity (c = speed of light), wavelength and frequency (colors),
The SUN.
Light. Review Question What is light? Review Question How can I create light with a cow magnet?
Electromagnetic Spectrum. The electromagnetic spectrum covers a wide range of wavelengths and photon energies.
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.
Why is Light so useful in Astronomy? It can tell us many properties of planets and stars: –How warm / hot they are (Surface temperature) –What they’re.
Sept 14 and 16, 2010 Ch 5b and c. 5.2Learning from Light: Origin of Starlight 1. How photons are produced 2. Relation temperature  motion of atoms 3.
© 2004 Pearson Education Inc., publishing as Addison-Wesley 6. Light: The Cosmic Messenger.
1 Nature of Light Wave Properties Light is a self- propagating electro- magnetic wave –A time-varying electric field makes a magnetic field –A time-varying.
Chapter 24 Studying the Sun. Electromagnetic radiation includes gamma rays, X- rays, ultraviolet light, visible light, infrared radiation, microwaves,
The Doppler Effect.
Light 1)Exam Review 2)Introduction 3)Light Waves 4)Atoms 5)Light Sources October 14, 2002.
Practice Questions Electromagnetic Spectrum. The electromagnetic spectrum Figure 3.5 Identify the following portions of the Electromagnetic spectrum:
Units to cover 25, Types of Spectra Kirchoff ’ s Laws: –If the source emits light that is continuous, and all colors are present, we say that this.
Astronomy Big Idea: The sun is one of billions of stars in one of billions of galaxies in the universe.
Atoms & Starlight (Chapter 6).
ATOMS - he nucleus is surrounded by orbiting electrons.
2.4 Studying the Sun. Electromagnetic Radiation  The visible light we see is only a fraction of energy coming from various objects  Most of what we.
Chapter 24 Sec. 1 Light Sec. 2: Tools of Astronomy
Lecture 13 Light: the Cosmic Messenger Telescopes and Observational Astronomy.
Investigating Astronomy Timothy F. Slater, Roger A. Freeman Chapter 2 Decoding the Hidden Messages in Starlight.
Starlight What is it? What does it tell us? Write down all notes in RED.
Chapter 24 Video Field Trip: Fireball Write down five facts from the video!
The Electromagnetic Spectrum. When a beam of white light passes through a glass prism, the light is separated or refracted into a rainbow-colored band.
Telescopes.
Light.
Atoms and Spectra.
Planetary Discovery in the era of Spacecraft Exploration Xi Zhang
Spectroscopy Lecture.
© 2017 Pearson Education, Inc.
Electromagnetic Radiation (Light)
Tools of Astronomy.
The Study of Light Picture taken
Spectral analysis of starlight can tell us about:
Light and Matter Chapter 2.
Electromagnetic Spectrum
Q due Thursday, March 3, 6:00 pm.
Unit 3 Practice Test Answer KEY
5.4 Thermal Radiation 5.5 The Doppler Effect
Presentation transcript:

Light

Review Question What is light?

Review Question How can I create light with a magnet?

Review Question How can I create light with some electrons?

Synchrotron emission Jupiter

Review Question Why do all objects emit radiation?

Review Question What are the three laws of blackbody or thermal radiation?

Blackbody emission

Blackbody/Thermal Spectra

Sunspots are cooler regions of the Sun’s photosphere

Line emission

Discussion The Sun emits radiation like a blackbody. However it has an atmosphere of cooler gas surrounding it. What type of spectrum would you expect the Sun to have?

Solar Spectrum

Iron Absorption lines in the Solar Spectrum

Discussion Explain the difference between how thermal or blackbody radiation is created and how line emission spectrum is created.

Molecular emission and absorption Photons can interact with molecules as well as electrons, causing them to vibrate and/or rotate. Most of these molecular emission/absorption bands are lower energy and are thus in the infrared or radio part of the spectrum.

Discussion How does a microwave heat you food?

Review Question What causes the colors of objects in this room?

Colors of objects All objects both absorb and reflect some of the light that hits them. If an object absorbs red and reflects blue it will appear blue, the color of the object being the color that is least absorbed and best reflected.

Spectrum from Mars

Difference between a Mirror and Scattered Reflection

Discussion A mirror consists of a glass substrate onto which a thin layer of metal is deposited. Why do you think metals are good reflectors of light?

Atmospheric scattering Nitrogen molecules in Earth’s atmosphere scatter blue light more effectively than red, so the sky appears blue.

Discussion Why does the sun appear reddish at sunrise or sunset?

Pleiades reflection nebula

Trifid nebula (M20) in Sagittarius

Doppler Effect The frequency of electromagnet radiation depends on the relative motion of the observer and the source.

Water Waves

Discussion If the leaf is moving toward the source of the water waves, will the frequency be greater or less than when the leaf was still?

Doppler Shift with Light If you are moving toward the source, light is shifted to higher frequencies, or toward the blue end of the spectrum. Astronomers call is a blueshift. Likewise if you are moving away from a source, the light is shifted toward the red end of the spectrum and is called a redshift.

Doppler shifted spectra

Radar measurement of Mercury’s rotation

Important points 1.The light need not appear red or blue. You can have a red spectral line which is blueshifted, or a blue line which is redshifted. 2.The Doppler effect depends on your relative velocity toward or away from an object, not on your distance from it.

Important points 3. The Doppler effect can only measure the radial velocity, the velocity toward or away from a source. It does not depend on the velocity of the object across the plane of the sky.

Telescopes Serve 3 Functions 1.To collect light 2.To resolve fine detail 3.To magnify the image

Resolution The ability to separate two closely spaced objects, such as a double star.

Resolution

Resolution and the atmosphere In general, atmospheric turbulence limits the resolution of even the largest telescopes on Earth to that of a 6 inch telescope.

“Seeing” The apparent size of the stars as viewed through the telescope. Good seeing is typically 1 arcsec.

Bad seeing Good seeing

Discussion What can astronomers do to try and improve resolution of their observations?

Hubble Space Telescope

Keck primary mirror

Adaptive optics Actuators deform the primary mirror hundreds of times a second to try and remove atmospheric distortion.

Adaptive optics turned off

Adaptive optics turned on

Discussion Adaptive optic telescopes work best in the infrared region of the spectrum and not in the visible. Why do you think that is?

Atmospheric absorption