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Hubble space telescope

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N. P. CHOUDHARY THE JAT BOY

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Hubble space telescope

  1. 1. A PRESENTATION ON THE HUBBLE SPACE TELESCOPE Guided By: Dr. CHANDRA SHEKHAR RAJORIA Assistant Professor Presented By: NARENDRA PAL SARAN B.Tech. VIII Sem (ME-I) GOVT. ENGINEERING COLLEGE BIKANER
  2. 2. INTRODUCTION  What is a space telescope? A space telescope is a special equipment developed for the purpose of observing distant planets, galaxies, and other outer space objects, from outer space. The Hubble which is orbiting the Earth outside the atmosphere is subject neither to electromagnetic radiation or light pollution from artificial light sources on the Earth.
  3. 3. •Named for Edwin Hubble (a great astronomer) •Launched 24-04-1990 •Changed our view and understanding of the Universe. Getting to know The Hubble
  4. 4. Hubble Facts Hubble orbits 400 mi above the Earth Orbits the Earth every 95.6 minute Launch mass 11.11 tons Size 13.2 m × 4.2 m Velocity 7160 m/s Launched by Space Shuttle Discovery
  5. 5. DESIGN & WORKING PRINCIPLE
  6. 6. 1. PRIMARY MIRROR Hubble’s 2.4 meter-diameter primary mirror is made of a special glass coated with aluminum and a compound that reflects ultraviolet light. It collects light from the telescope’s targets and reflects it to the secondary mirror. 2. SECONDARY MIRROR Like the primary mirror, Hubble’s secondary mirror is made of special glass coated with aluminum and a compound to reflect ultraviolet light. It is 0.33 meters in diameter and reflects the light back through a hole in the primary mirror and into the instruments.
  7. 7. 3. APERTURE DOOR Hubble’s aperture door can close, if necessary, to prevent light from the Sun from entering the telescope. 4. COMMUNICATION ANTENNAS Data stored in Hubble’s solid-state recorder is converted to radio waves and then beamed through one of the spacecraft’s high-gain antennas to a NASA communications satellite, which relays it to the ground.
  8. 8. 5. SOLAR PANELS To operate in space, the HST needs a power supply, communications equipment, computers, and a control system. Power is supplied by two 25-foot-long solar panels, each containing 48,760 individual photo cells. Together, the two panels are capable of generating 2,800 W. The power generated by the panels is also used to charge six nickel-hydrogen batteries that provide power to the spacecraft for about twenty-five minutes per orbit while Hubble flies through the earth's shadow.
  9. 9. 6. SUPPORT SYSTEMS Essential support systems such as computers, batteries, gyroscopes, reaction wheels, and electronics are contained in these areas. 7. Wide Field Camera 3 (WFC3) WFC3 sees three different kinds of light: near- ultraviolet, visible and near-infrared, though not simultaneously. Its resolution and field of view are much greater than that of Hubble's other instruments. It will be used to study dark energy and dark matter, the formation of individual stars and the discovery of extremely remote galaxies previously beyond Hubble's vision.
  10. 10. 8. ACS The Advanced Camera for Surveys is designed primarily for wide-field imagery in the visible wavelengths, though it also sees in ultraviolet and near infrared. 9. NICMOS The Near Infrared Camera and Multi-Object Spectrometer is an instrument for near-infrared imaging and spectroscopic observations of many types of astronomical targets.
  11. 11. 10. Cosmic Origins Spectrograph (COS) Astronauts installed the Cosmic Origins Spectrograph during SM4 in place of the Corrective Optics Space Telescope Axial Replacement (COSTAR). The most powerful ultraviolet spectrograph ever flown, COS measures the structure and composition of the ordinary matter concentrated in the “cosmic web.” It also studies how galaxies, stars, and planets formed and evolved, and is helping determine how elements needed for life first formed.
  12. 12. Its main function is spectroscopy—the separation of light into its component colors (or wavelengths) to reveal information about an object’s chemical content, temperature, density, and motion. STIS also performs imaging, covering most of the ultraviolet bands, the entire optical wavelength band, and some wavelengths extending into the near-infrared. 11. Space Telescope Imaging Spectrograph(STIS)
  13. 13. 12. FGS Hubble has three Fine Guidance Sensors. Two are needed to point and lock the telescope on the target and the third can be used for stellar position measurements, known as astrometry. During SM4, spacewalking astronauts exchanged one of these optical sensors with a refurbished unit that has enhanced, on-orbit alignment capability.
  14. 14. Hubble data is transmitted to Earth through a NASA relay satellite which downlinks it to a ground station in White Sands, NM. From there, it is forwarded to Goddard Space Flight Center for initial processing and quality checking. Within minutes it is sent to the Space Telescope Science Institute, where it is further processed, archived, and made available to the Principal Investigator who successfully proposed the observation. WORKING PRINCIPLE
  15. 15. How Does Hubble Create the Images?
  16. 16. How Does Hubble Create the Images? Images come from Hubble in black & white (real colors). Colors are assigned based on chemical elements present, called representative colors. Blue = Oxygen Red = Sulfur Green= Hydrogen
  17. 17. Hubble’s Accomplishments  NASA now knows that the universe is 13.7 billion years old, thank to Hubble  Hubble showed NASA how plants born  HST suggests the universe started increasing it’s speed recently  Hubble sensed the first organic molecule on a planet outside our solar system
  18. 18. Conclusion In conclusion the Hubble space telescope has been a major help in the discovery of the secrets of the universe. It is unfortunate that it will out of commission by 2014 but we will have it’s legacy. The James Webb Space Telescope (JWST), is scheduled for launch in 2018.
  19. 19. THANKS FOR YOUR ATTENTION

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