AST 103 Telescopes Prof. Ken Nagamine UNLV 1 Telescopes • The best observing sites are atop remote mountains Calm, High, Dark, Dry Mauna Kea, Hawaii 2 A telescopes is a tool used to gather light from objects in the universe There are two different types of telescopes • A refracting telescope: focuses light with glass lenses • A reflecting telescope: focuses light with mirrors 3 A refracting telescope uses a lens to focus incoming light 4 Refraction • Refraction is the bending of light when it passes from one substance into another • Your eye uses refraction to focus light 5 Focusing Light • Refraction can cause parallel light rays to converge to a focus 6 Refracting Telescope • Refracting telescopes need to be very long, with large, heavy lenses 7 Reflecting Telescope • Reflecting telescopes can have much greater diameters • Most modern telescopes are reflectors 8 Reflecting telescopes use mirrors to focus incoming starlight 9 Mirrors in Reflecting Telescopes Twin Keck telescopes on Mauna Kea in Hawaii Segmented 10-meter mirror of a Keck telescope 10 Many big telescopes!! 11 Three main functions of a telescope • gather light – (bigger IS better) – makes objects appear brighter Telescopes with a larger collecting area can gather a greater amount of light in a shorter time. • see fine detail (resolution) Telescopes that are larger are capable of taking images with greater detail. • magnify 12 A larger objective lens provides a brighter (not bigger) image 13 But visible light is just one part of spectrum Astronomers are interested in the entire spectrum of light! 14 Astronomers use different instruments to look at light of different wavelengths - sometimes, we even have to go above Earth’s atmosphere. 15 Quiz Which of the following wavelengths can be observed easily by a telescope located on Earth’s surface? a) gamma ray b) X-ray c) ultraviolet d) radio e) all of the above wavelengths f) none of the above wavelengths 16 IR & UV Telescopes SOFIA (IR) GALEX (UV) Spitzer (IR) • Infrared and ultraviolet-light telescopes operate like visible-light telescopes but need to be above atmosphere to see all IR and UV wavelengths 17 Radio wavelength observations are possible from Earth’s surface Green Bank (west virginia) Arecibo, Puerto Rico 18 The Very Large Array (VLA) in New Mexico Interferometer 19 High above Earth’s atmosphere, the Hubble Space Telescope provides stunning details about the universe 20 Earth’s atmosphere hinders astronomical research Image of stars taken with a telescope on the Earth’s surface Same picture taken with Hubble Space Telescope high above Earth’s blurring atmosphere 21 Lecture-Tutorial (LT): Telescopes (pp. 49-51) • Work with a partner! • Read the instructions and questions carefully. • Discuss the concepts and your answers with • • • one another. Come to a consensus answer you both agree on. If you get stuck or are not sure of your answer, ask another group. If you get really stuck or don’t understand what the LT is asking, ask for help. 22 Quiz Which of the following wavelengths of light emitted by the Sun is most effectively blocked by Earth’s atmosphere? a) visible b) radio c) infrared d) gamma 23 Quiz Imagine that you are the head of a funding agency that can afford to build one telescope. Which of the following proposed telescopes would be best to support? a) a radio telescope in orbit around Earth b) an ultraviolet telescope in orbit around Earth c) an X-ray telescope located in New Mexico 24 Quiz The Hubble Space Telescope obtains higher resolution images than most ground-based telescopes because it is a) larger. b) closer to stars. c) above Earth’s atmosphere. 25