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Section 22-1 Study Guide Radiation from Space Ms. Grady Light from the Past When you look at a star, the light that you see left the star many years ago. Light travels fast and distances between objects in space are so great that it take millions of years for the light to reach Earth. Light and other energy leaving a star are forms of radiation. Radiation is energy that is transmitted (sent out/put out) from one place to another by electromagnetic waves. See picture below.↓ Because of the electric and magnetic properties (belongings) of this radiation, it is called electromagnetic radiation. Example: Electromagnetic waves carry energy (force/power) through empty space and through matter (anything that has mass and takes up space). When you turn on the radio. When you look down a microscope. When you have an X ray taken. Electromagnetic radiation is everywhere around you. The arrangement of electromagnetic radiation is called the Electromagnetic spectrum. The Electromagnetic spectrum is arranged by wavelengths + frequency. The shorter the wavelength = the higher the frequency. . 1 Forms of electromagnetic radiation differ (change) in their frequencies (occurrence/rate). Frequency is the number of wave crests that pass a given point per unit of time. Electromagnetic Radiation Sound waves are a type of mechanical wave. We hear the voices of astronauts while they are in space because astronauts speak into a microphone. The radio waves travel through space and through the Earth’s atmosphere. Two types of electromagnetic radiation are: Radio waves Visible light from the sun. They cannot travel through empty space. These sound waves are converted (changed) into electromagnetic waves called radio waves. They are then changed (converted) back to sound waves by electronic equipment and audio speakers ↓. Other examples of electromagnetic radiation are: Gamma rays X rays↓ Ultra violet waves Infrared waves Microwaves↓ 2 Radio waves microwaves Communication Is an oven to on – radio heat food. waves, TV, radar signals Communication on remote control Infrared waves = heat Thermal images communication Visible lights Can be seen by human eyes colors Not affected by atmosphere Ultraviolet rays Sterilize (kill bacteria) but also kill good living cells. Example, Sunburn →skin cancer X-rays Few penetrate (get through) Earth’s thick atmosphere Gamma Rays Radiation treatment to kill cancer cells (gamma treatment) Speed of Light Speed of light (speed of all electromagnetic waves) = travel at 300,000 km/s in a vacuum (km/s= kilometers/second). Visible light and other forms of electromagnetic radiation travel at this very fast speed. The universe is so large that it takes millions of years for the light from some stars to reach earth. When electromagnetic light reaches earth, scientists use it to learn about the star it came from. For example, one tool for studying electromagnetic radiation is the telescope. 3 Optical Telescopes →Uses light to produce (show) magnified (overblown) images of faraway objects. Telescopes use radiation spectrum to explore the space. Light is collected by an objective lens or mirror. It then forms an image (picture) at the focal point of the telescope. A focal point is the point where the light is bent by the lens or reflected by the mirror comes together to form an image (picture). The eyepiece increases the image for the eyes. Refracting telescope – uses convex lens that gathers light (+) plus one (1) concave lens (eyepiece) that brings image to the eye. Refracting – lights bend when they pass through lenses. Reflecting – (lights) hit (mirror) and come back Reflecting telescope - uses a curved (concave) mirror, and a flat mirror, and a convex lens. 4 Concave Convex Concave surface – curves inward Convex surface bulges outward Concave lens causes light rays to spread apart or diverse Concave mirror causes light rays to meet or converge Convex lens causes light rays to meet or converge Convex mirror causes light rays to spread apart or diverge. Observatories = buildings that have dome-shaped roofs for viewing the sky. Not all telescopes are located in observatories. The Hubble Space Telescope is an example of one. The Hubble Space Telescope High quality images When the largest mirror of this reflecting telescope was shaped, a mistake was made. Launched in 1990 by the space shuttle Discovery. Repaired (fixed) in 1993 for because the mirror did not work properly In 1997 and 1999, two more missions to fix Hubble were carried out (took place). After it was fixed, Hubble could view a large cluster of galaxies known as Abell 2218. Large Reflecting Telescopes Early 1600sLippershey Gailileo – was the first person who used a telescope to observe. He invented the telescope. 5 The Keck telescope mirrors (located in Hawaii, USA) Are built out of many small mirrors that are pieced together. Have segmented mirrors (mirrors put together in parts) 10 m wide. Fun fact – In 2000, the European Southern Observatory’s telescope (located in Chile, South America) consisted of four 8.2 – m reflectors. This is the largest optical telescope. Active and Adaptive Optics Active optics – computer corrects images (pictures) that are distorted (unclear) by temperature changes → mirror errors Adaptive optics –laser probes atmosphere and transmits (sends out) information to a computer about air turbulence (commotion/disturbances). The computer then fixes (corrects) the telescope’s mirror thousands of times per second. Telescope images (pictures) are clearer (easier to see) when corrections for air turbulence, temperature changes, and mirrorshape changes are made. Radio Telescopes - can be used without light and in bad weather. Radio waves are an example of long – wavelength energy in the electromagnetic spectrum. They pass freely though the Earth’s atmosphere Picture of Radio telescopes Radio telescopes study radio waves traveling through space. They are useful 24 hours a day under most conditions. The metal dish gathers radio waves onto an antenna. A computer produces (makes) images. Infrared Telescopes Example: IRAS – was the first infrared telescope. Only stars in space give off visible light – all objects give off heat (infrared waves) Infrared telescopes carried into space. 6