the universe and electromagnetic spectrum state objectives 2e. and 4.f

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The Universe and Electromagnetic Spectrum State Objectives 2e. and 4.f.

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  • Slide 1
  • Slide 2
  • The Universe and Electromagnetic Spectrum State Objectives 2e. and 4.f.
  • Slide 3
  • What are Electromagnetic Waves? Form of energy that travels at the speed of light (300,000 km/s) Uses electric and magnetic fields Can travel through a vacuum (empty space) Two Characteristics Wavelength- distance between two points on a wave Frequency- number of waves that pass a point in one second Electromagnetic spectrum is a collection of EM waves of all known frequencies
  • Slide 4
  • Properties of Waves
  • Slide 5
  • Electromagnetic Spectrum
  • Slide 6
  • Gamma Rays Gamma: carry the most energy Shortest wavelength & highest frequency Produced by hottest objects in universe Kills living cells Used to sterilize medical equipment, kill bacteria in food, and treat cancer
  • Slide 7
  • Uses of Gamma Rays
  • Slide 8
  • X-Rays X-rays: high energy through soft tissue & matter, but lower energy in hard tissue & matter Can damage or kill living cells, so precautions must be taken Used in medical imaging and security screening devices
  • Slide 9
  • Uses of X-Rays
  • Slide 10
  • Ultraviolet Rays Ultraviolet (UV) rays: has both positive and negative effects on living organisms Helps produce vitamin D in the skin and causes tanning Prolonged exposure causes sunburns and skin cancer Most UV radiation is blocked by the ozone layer Can be used to disinfect objects and in blacklights
  • Slide 11
  • Effects of Ultraviolet Rays
  • Slide 12
  • Visible Light Visible light: the only part of the spectrum that is detectable by the human eye longer wavelength & lower frequency than UV- rays Allows us to see different colors Objects reflect the color of the spectrum you see and absorb the other colors Order from longest wavelength to shortest red, orange, yellow, green, blue, indigo, violet Roy G Biv
  • Slide 13
  • Infrared Waves Infrared: cannot be seen by humans but is felt as heat. Wavelengths longer than visible and have frequencies which are lower than visible Used in thermal imaging cameras (night vision), and TV remote controls Can be used to observe faint objects in space.
  • Slide 14
  • Uses of Infrared Waves
  • Slide 15
  • Microwaves Pass easily through earths atmosphere so they can be used to transmit signals (TV broadcasts) Also used to cook food, in radar detectors, & cell phones Microwave ovens work by causing water and fat molecules to vibrate. Some scientists believe prolonged exposure to microwaves through cells phones and other devices can lead to brain cancer.
  • Slide 16
  • Radio Waves Radio waves: carries the least amount of energy longest wavelength & lowest frequency Main use is communication Different frequencies
  • Slide 17
  • Draw a line to match the description to the wave type. Radio Microwaves Infrared Visible light Ultraviolet X-rays Gamma rays Prolonged exposure can harm skin Only part of the spectrum the human eye can detect Used to transmit information Humans release this in the form of heat Kills living cells Used in cell phones and to cook food. Might cause brain cancer Damaging to soft tissue, but is used with precaution for medical imaging
  • Slide 18
  • Review http://www.youtube.com/watch?v=5GIvk tBSxvw http://www.youtube.com/watch?v=5GIvk tBSxvw
  • Slide 19
  • Parts of the Universe The universe is all space, matter, and energy that exists The exact size is unknown, but it is believed to still be expanding outward. Stars group together in clusters. Clusters group together in galaxies. Galaxies group together in groups. Galaxy groups group together in super-clusters.
  • Slide 20
  • Galaxies Huge collection of stars, gas, & dust held together by gravity 3 types of galaxies: elliptical, spiral, & irregular http://www.youtube.com/watch?v=Mu 6ODjj7EvI http://www.youtube.com/watch?v=Mu 6ODjj7EvI
  • Slide 21
  • Spiral galaxy
  • Slide 22
  • Elliptical galaxies
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  • Irregular galaxies
  • Slide 24
  • Galaxy Groups The Milky Way (our galaxy) is located in the Local Group. The Local Group contains 36 galaxies. The Local Group is part of the Virgo Supercluster (at least 100 galaxies). Atlas of the Universe
  • Slide 25
  • Our Galaxy - The Milky Way From the side, the Milky Way appears to be a narrow disk with a bulge in the middle. The galaxys spiral structure is visible only from above or below.
  • Slide 26
  • Stars Stars are objects made of gases which produce light and heat from fusion reactions inside the star. Smaller stars fuse hydrogen into helium. Larger stars form heavier elements. Stars form & end their life in nebulae:
  • Slide 27
  • Nebulae Nebulae are large clouds of gas, plasma & dust within a galaxy Typically a few light-years wide. Light-year is the distance light travels in one year (about 9.5 trillion km)
  • Slide 28
  • Nebulae
  • Slide 29
  • Life Cycle of a Star http://www.youtube.com/watch?v=mz E7VZMT1z8 http://www.youtube.com/watch?v=mz E7VZMT1z8
  • Slide 30
  • How far away are stars? Parallax: apparent shift in the position of an object when viewed from two different locations. Can be used to measure the distance of stars from Earth that are relatively close. Proxima Centauri: closest star to earth Proxima Centauri (4.3 light years away 40 trillion km)
  • Slide 31
  • The Expanding Universe All distant galaxies are moving rapidly away from our galaxy and from each other.
  • Slide 32
  • The Expanding Universe Red Shift: occurs when a star or other object is moving away from Earth Blue Shift: occurs when a star or other object is moving toward Earth
  • Slide 33
  • The Expanding Universe
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  • Slide 35
  • Origins of the Universe Big Bang Theory : states that all matter and energy were once packed into a tiny particle smaller than a speck of dust. The particle began to expand and matter and energy moved rapidly outward in all directions. The matter cooled and collected to form stars, galaxies, nebulae, and planets. Most scientists believe the universe is about 13.7 billion years old. http://www.history.com/shows/the- universe/videos/what-put-the-bang-in-the-big- bang#what-put-the-bang-in-the-big-bang http://www.history.com/shows/the- universe/videos/what-put-the-bang-in-the-big- bang#what-put-the-bang-in-the-big-bang
  • Slide 36
  • Origins of the Universe
  • Slide 37
  • Telescopes Telescopes are instruments that collect and focus light or other forms of electromagnetic radiation. Many telescopes use mirrors to collect light from space. Space telescopes in orbit provide clearer pictures because the atmosphere distorts images and absorbs some radiation.
  • Slide 38
  • Four Views of the Crab Nebula Different type of telescopes collect electromagnetic radiation at different wavelengths. Astronomers are able to learn a great deal about the Crab Nebula by examining these different images.
  • Slide 39
  • Hubble Space Telescope Launched in 1990 One of NASAs most successful missions. Orbits 353 miles above Earth Completes one orbit every 97 minutes Hubble Site
  • Slide 40
  • HUBBLE SPACE TELESCOPE
  • Slide 41
  • Chandra X-ray observatory Launched in 1999. Detects x-rays from the hottest regions of the universe Orbits Earth at an altitude of 86,500 miles. Has observed the black hole at the center of the Milky Way and discovered several other black holes.
  • Slide 42
  • Chandra Images
  • Slide 43
  • Spitzer Space Telescope Launched in 2003 Observes infrared radiation Heliocentric (sun-centered) orbit Parts of the telescope must be kept at -450 degrees Fahrenheit so as not to interfere with infrared detection.
  • Slide 44
  • Spitzer space telescope
  • Slide 45
  • James Webb Telescope Currently being built to replace Hubble Scheduled to launch in 2018 Will observe radiation in infrared and visible light Will be able to see galaxies that have shifted beyond visible spectrum
  • Slide 46
  • Webb Telescope Webb-Cam