The Electromagnetic Spectrum and Telescopes Rose Emanuel Journey into Space Journey Museum, July 18-20, 2012.

Slides:



Advertisements
Similar presentations
Telescopes Section 1-4. Telescope l Tele – distant, far l Scope- see l Invented in the 16 th century l First used by Galileo Who found moons around Jupiter.
Advertisements

Astronomy Notes to Accompany the Text
Chapter 5 Telescopes. 5.1 Optical Telescopes The Hubble Space Telescope 5.2 Telescope Size The Hubble Space Telescope 5.3 Images and Detectors Diffraction.
Unit 11, Section 1.  Light can take millions of years to travel to Earth  All electromagnetic radiation travels at the speed of light, which is 300,000.
Chapter 4 – Stars, Galaxies, and the Universe.  The electromagnetic spectrum includes the entire range of radio waves, infrared radiation, visible light,
Chapter 24: Studying the Sun (and other stars)
Telescopes Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Telescopes: The Tools of Astronomy Types of Telescopes –Land Based –Space Based Infrared Visible Ultraviolet X-ray Gamma Hubble Space Telescope.
© 2011 Pearson Education, Inc. Lecture Outlines Astronomy Today 7th Edition Chaisson/McMillan © 2011 Pearson Education, Inc. Chapter 5.
X-Ray UltravioletVisibleInfraredRadio The Electromagnetic Spectrum and the Universe.
A Galaxy Revealed in Multiple Wavelengths 0 Topic: Multiwavelength observations Concepts: Infrared observations, X-ray observations, Optical observations,
1 Earth’s Atmosphere & Telescopes Whether light is absorbed by the atmosphere or not depends greatly on its wavelength. Earth’s atmosphere can absorb certain.
Chapter 3: Telescopes. Goals Describe basic types of optical telescopes Explain why bigger is better for telescopes Describe how the Earth’s atmosphere.
TELESCOPES. WHAT IS A TELESCOPE A telescope is an instrument that gathers electromagnetic radiation from objection in space and concentrates it for better.
Short wavelength High energy Long wavelength Low energy 1. Astronomers Observe Light Radiated Toward Earth By Matter in Space 2. Light is Energy That.
Space Technology Telescopes Chapter 18 Section 2.
Chapter 5.
Chapter 5 Telescopes: “light bucket”. Telescopes have three functions 1.Gather as much light as possible: LGP ∝ Area = πR 2 LGP ∝ Area = πR 2 Why? Why?
 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.
Telescopes & Light: Part 1. A Telescopes is a tool used to gather light from objects in the universe.
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 21 power point Stars,galaxies, and the universe.
Stars, Galaxies, and the Universe.  To understand how telescopes work, its useful to understand the nature of the electromagnetic radiation. Light is.
Light and Telescopes.
The Solar System: A6: Telescopes.
Compare refracting and reflecting telescopes. Have you ever bent or slowed down light? How?
Telescopes. Telescope An instrument that collects electromagnetic radiation from objects in space Concentrates the electromagnetic radiation for better.
1 Stars, Galaxies & Universe Chapter 3. 2 Tools of Astronomy Constellations are groups of stars that form a pattern. The electromagnetic spectrum is made.
Chapter 5 Telescopes Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Astronomy and the Electromagnetic Spectrum
Warm up question  1. How do you think astronomers can see planets, stars, and galaxies that are so far away?
 Named after Edwin Hubble, the astronomer who discovered the expansion of the universe. Launched in 1990 and contains a 2.4 m (95 in) mirror with which.
Tools for Studying Space. © 2011 Pearson Education, Inc. Telescopes.
Survey of the Universe Tom Burbine
© 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley This work is protected by U.S. copyright laws and is provided solely for the use of.
Exploring the Universe Harcourt Science Unit D Chapter 4 Mrs.Strand 6th grade Lockwood Middle School.
Tools of Astronomy.
Key Ideas Describe characteristics of the universe in terms of time, distance, and organization. Identify the visible and nonvisible parts of the electromagnetic.
Tools of Astronomy. Electromagnetic Radiation Light travels as an “Electromagnetic” Wave The light you see is called Visible Light Speed of light: 186,000.
Lecture Outlines Astronomy Today 7th Edition Chaisson/McMillan © 2011 Pearson Education, Inc. Chapter 5.
Astronomy Chapter 26 Studying Space. Astronomy  The scientific study of the universe Benefits  Exciting discoveries Black holesBlack holes pulsarspulsars.
Telescopes.
Telescopes Portals of Discovery. Telescope A telescope is an instrument designed to aid the observation of remote objects by collecting some form of electromagnetic.
6.3 Telescopes and the Atmosphere 6.4 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does Earth’s atmosphere affect ground-based observations?
Chapter 3 Telescopes. Gemini North Telescope, Mauna Kea, Hawaii.
Astronomy Astronomy the scientific study of the universe Scientists who study the universe are called astronomers Early Astronomers includes: Nicolaus.
Viewing the Universe. 8Astronomers gather information about objects throughout the universe by detecting various kinds of energy given off by these objects.
The Lives and Deaths of Stars A presentation of the Universe in the Parks program The University of Wisconsin-Madison Department of Astronomy.
Stellar Evolution. Solar Composition Most stars in space have this composition: 74% hydrogen, 26% helium Fusion is the energy maker of the sun.
1 Assembling the Jigsaw-Puzzle Picture of the Universe Presented to the NASA Night Sky Network January 31, 2006 Dr. Jeffrey D. Rosendhal Carl Sagan Center.
Electromagnetic Spectrum What’s the Wavelength?. E-M Spectrum
Chapter 5 Telescopes Chapter 5 opener. This composite photograph shows two of the premier optical telescopes available to astronomers today. At the top,
Chapter 4: Telescopes. E O Optical telescopes: Reflectors and refractors Refractors use lenses E: eyepiece O: objective.
1 Earth’s Atmosphere & Telescopes Whether light is absorbed by the atmosphere or not depends greatly on its wavelength. Earth’s atmosphere can absorb certain.
Why look at different frequencies of light? Cooler objects are only visible at long wavelengths: radio, microwaves, IR. Hotter objects are only visible.
Chapter 21: Stars, Galaxies, Universe Section 1: telescopes
Chapter 24 Sec. 1 Light Sec. 2: Tools of Astronomy
A black hole: The ultimate space-time warp Ch. 5.4 A black hole is an accumulation of mass so dense that nothing can escape its gravitational force, not.
“Images from Space” Examining the Technology That Lets Us Explore the Universe.
Add to table of contents:  Pictures of telescopesPg. 82  TelescopesPg. 83.
 From the ground the atmosphere distorts images.  Light pollution from streetlights, city lights, car lights, and more hinders the seeing conditions.
Astronomical Imaging: Do You See What I See? Using Filters to View Astronomical Pictures.
Telescope Technology Types of Telescopes Hubble Telescope and NASA’s Great Observatories.
OTHER TELESCOPES.
Stars, Galaxies, and the Universe
6.3 Telescopes and the Atmosphere
Ch.1, Sec.2 - Telescopes Optical Telescopes
Using Telescopes to Observe Electromagnetic Radiation in Space
Telescopes and the Electromagnetic Spectrum Section 3
Telescopes 4/23/15 IN: What is a telescope? How is it used?
Presentation transcript:

The Electromagnetic Spectrum and Telescopes Rose Emanuel Journey into Space Journey Museum, July 18-20, 2012

Major Space Observatories Why put them in space?

Atmospheric Blurring – Twinkling of stars in sky, called scintillation, is caused by moving atmospheric irregularities refracting star light into a blend of paths to the eye – Distorted seeing can be improved by adaptive optics, which employs a powerful laser and correcting mirrors to offset scintillation

Light Pollution

Space vs.Ground-Based Observatories Space-Based Advantages – Freedom from atmospheric blurring – Freedom of atmospheric absorption Ground-Based Advantages – Larger collecting power – Equipment easily fixed Ground-Based Considerations – Weather, humidity, and haze – Light pollution

The Hubble Space Telescope (HST) is able to observe in the ultraviolet, something that ground-based research telescopes cannot do.

X-ray Telescope: Chandra High energy x-rays must skip off the shiny mirror surface at shallow angles to be observed, much different than how optical light telescopes work. Collecting x-rays is like skipping stones on a pond!

Gamma Ray Detectors Gamma rays have too high an energy to be focused with even the shallow angle reflecting technique, so gamma ray telescopes simply point in a desired direction and count the number of photons coming from that direction. The Compton Gamma Ray Observatory

“Invisible” Light in Astronomy Each part of the spectrum provides a piece of the puzzle in understanding our universe. Star birth & star death Warm dust Stars & dust Young stars Black holes & neutron stars

Ultraviolet Images of a Galaxy Clearly Show the Young, Hot Stars

Infrared measurements in Andromeda clearly reveal the hot dust

The Crab Nebula: The Aftermath of a Supernova The Crab Nebula is all that remains of a once-bright star. The white box on the left shows the area covered by the image on the right.

A visible light image of Centaurus A, an interesting galaxy observed with a wide lane of dust across its center. Visible Light View of an Interesting Galaxy, but X-rays Reveal the Real Action! A high-energy jet blasts outward from the galaxy’s center, evidence for a powerful black hole with the mass of one billion Suns!

The infrared reveals the clouds of gas and dust associated with starbirth

X-ray observations of the center of our own galaxy clearly reveal the hot gas swirling into a massive black hole