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    Astronomy 101

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    • Introduction to Astronomy
      • 1.1What is Astronomy?
      • 1.2History of Astronomy
      • 1.3Overview of the Universe
    • The Solar System
      • 2.1Overview of the Solar System
      • 2.2Planets and their Characteristics
      • 2.3Other Celestial Bodies in the Solar System
    • Stars and Galaxies
      • 3.1Introduction to Stars
      • 3.2Life Cycle of Stars
      • 3.3Introduction to Galaxies
      • 3.4Types of Galaxies
    • The Milky Way and Other Galaxies
      • 4.1Overview of the Milky Way
      • 4.2Other Notable Galaxies
      • 4.3Interstellar Medium and Cosmic Dust
    • Telescopes and Observatories
      • 5.1Introduction to Telescopes
      • 5.2Types of Telescopes
      • 5.3Famous Observatories
    • The Sun and the Moon
      • 6.1Overview of the Sun
      • 6.2Solar Phenomena
      • 6.3Overview of the Moon
      • 6.4Lunar Phenomena
    • The Earth and the Sky
      • 7.1Earth's Rotation and Revolution
      • 7.2Seasons and Climate
      • 7.3Sky Phenomena
    • Space Exploration
      • 8.1History of Space Exploration
      • 8.2Notable Space Missions
      • 8.3Future of Space Exploration
    • Astrobiology
      • 9.1Introduction to Astrobiology
      • 9.2Search for Extraterrestrial Life
      • 9.3Extremophiles on Earth
    • Cosmology
      • 10.1Introduction to Cosmology
      • 10.2The Big Bang Theory
      • 10.3Dark Matter and Dark Energy
    • Space-Time and Relativity
      • 11.1Introduction to Space-Time
      • 11.2Special Relativity
      • 11.3General Relativity
    • Black Holes and Neutron Stars
      • 12.1Introduction to Black Holes
      • 12.2Properties of Black Holes
      • 12.3Introduction to Neutron Stars
      • 12.4Properties of Neutron Stars
    • Wrap-up and Future Study
      • 13.1Review of Key Concepts
      • 13.2Current Research in Astronomy
      • 13.3How to Continue Studying Astronomy

    Telescopes and Observatories

    Unit 3: Famous Observatories

    location used for observing terrestrial or celestial events

    Location used for observing terrestrial or celestial events.

    Observatories are specialized structures or locations used for observing celestial events. They are equipped with powerful telescopes and other astronomical instruments to study outer space. In this unit, we will explore some of the most famous observatories, both space-based and ground-based, that have significantly contributed to our understanding of the universe.

    Hubble Space Telescope

    Launched in 1990, the Hubble Space Telescope is one of the most well-known space-based observatories. Named after the astronomer Edwin Hubble, it orbits Earth and captures high-resolution images of distant galaxies, nebulae, and other celestial bodies. Hubble's observations have led to breakthroughs in astrophysics, such as determining the rate of expansion of the universe.

    Chandra X-ray Observatory

    The Chandra X-ray Observatory, launched by NASA in 1999, observes the universe in X-ray wavelengths. X-rays, which are absorbed by Earth's atmosphere, can reveal high-energy regions of the universe, such as supernova remnants, black holes, and neutron stars. Chandra's high-resolution X-ray images have provided invaluable data on these phenomena.

    Kepler Space Telescope

    The Kepler Space Telescope, operational from 2009 to 2018, was designed to discover Earth-like planets orbiting other stars in the habitable zone (the region around a star where conditions might be right for liquid water). Kepler discovered over 2,600 confirmed exoplanets, making a significant contribution to the field of exoplanetology.

    Mauna Kea Observatories

    Located in Hawaii, the Mauna Kea Observatories are a collection of independent astronomical research facilities and large telescope observatories. The location is ideal for ground-based observatories because of its dark skies, high elevation, and dry climate. The observatories house the world's largest optical, infrared, and submillimeter telescopes.

    Very Large Telescope (VLT)

    The Very Large Telescope, located in the Atacama Desert of northern Chile, is a ground-based observatory operated by the European Southern Observatory (ESO). The VLT consists of four 8.2-meter telescopes, which can be used individually or in combination, making it the most advanced optical instrument in the world. It has made numerous significant scientific discoveries, including the first direct image of an exoplanet and observations of the afterglow of the furthest known Gamma Ray Burst.

    These observatories have greatly expanded our knowledge of the universe, providing insights into galaxies, stars, planets, and other celestial phenomena. They continue to be invaluable tools in the ongoing exploration and understanding of our universe.

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