Using Technology to See Beyond the Visible

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Presentation transcript:

Using Technology to See Beyond the Visible Section 3.2 Using Technology to See Beyond the Visible

Beyond the visible Besides the visible light that optical telescopes can give us, other forms of electromagnetic energy can also give us information about objects in space. Read 1st paragraph of page 440. WRITE NOTES on electromagnetic energy: travels at speed of light (300 000km/s) BUT has different wavelengths and frequencies. DRAW wave model of light!

Electromagnetic Energy This energy travels at the speed of light, but has different wavelengths and frequencies from those of visible light. Energy with a short wavelength has a high frequency. Gamma rays are the most dangerous (and have the shortest wavelength) and radio waves are the safest. Draw this

Radio Telescopes Radio waves are received from stars, galaxies, nebulae, the Sun and even some planets. With the development of radio telescopes, astronomers gain an advantage over optical telescopes, because they are not affected by weather, clouds, atmosphere or pollution and can be detected day or night.

Radio Telescopes Much information has been gained about the composition and distribution of matter in space, namely neutral hydrogen, which makes up a large proportion of matter in our Milky Way galaxy. Radio telescopes are made of metal mesh and resemble a satellite dish, but are much larger, curved inward and have a receiver in the center.

Radio Interferometry By combining several small radio telescopes ( just like they do with optical telescopes ) greater resolving power can be achieved. This is referred to as radio interferometry. It improves the accuracy and performance of the image in making radio maps. The greater the distance between the radio telescopes the more accurately they can measure position. Arrays, like the Very Large Array in Sorocco, New Mexico, which uses 27 telescopes arranged in a Y, can improve accuracy even more.

Viewing More Than What The Eye Can See Ultraviolet radiation is absorbed by the atmosphere and therefore cannot be studied very well from Earth. A distant planet orbiting a distant star cannot be seen because of the bright light from its star. However, when viewed in the infrared spectrum through a radio telescope, the stars brightness dims and the planets brightness peaks. The Keck Observatory in Hawaii is actively searching for planets, with its radio telescope. Other discoveries include fluctuations in microwave energy left over from the formation of the universe; X-rays emitted from black holes and pulsating stars; and huge bursts of gamma rays appearing without warning and then fading just as quickly.

Space Probes Space probes are unmanned satellites or remote-controlled ‘landers’ that put equipment on or close to planets where no human has gone before. Probes have done remote sensing on Mercury and Jupiter, taken soil samples on Mars, landed on Venus, and studied Saturn’s rings up close.

Space Probes The most recent probes to explore Mars are still there. They are Spirit and Opportunity. They are looking for evidence of water to determine if Mars at one time could have sustained life.

HOMEWORK: Check & Reflect Page 445: 3, 5, 7, 9 RESEARCH: What is more effective: One large radio telescope (such as the one in Arecibo, Puerto Rico [p.442]) or a large array using radio interferometry (such as that in Socorro, New Mexico [p. 443])? What have we learned from these devices specific devices?