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    • A telescope is a simple optical instrument designed to observe distant objects by collecting and magnifying light. It consists of a few essential components: an objective lens or mirror and an eyepiece. The objective lens or mirror gathers light from the target, while the eyepiece magnifies the image for observation.

      Telescope

      Telescope

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    • The Large Array Radio Telescope, often referred to as the Very Large Array (VLA), is a remarkable astronomical observatory located in New Mexico, USA. Operated by the National Radio Astronomy Observatory (NRAO), the VLA is one of the world's premier radio telescope facilities.

      NRAO Large Array Radio Telescope

      NRAO Large Array Radio Telescope

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    • The Neil Gehrels Swift Observatory, previously known as the Swift Gamma-Ray Burst Explorer, is a space observatory dedicated to the study of gamma-ray bursts (GRBs), one of the universe's most energetic and enigmatic phenomena. Launched in 2004, this mission is named in honor of Dr. Neil Gehrels, a prominent astrophysicist.

      Neil Gehrels Swift Observatory

      Neil Gehrels Swift Observatory

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    • The Hubble Space Telescope (HST) is one of the most influential space observatories ever built. Launched on April 24, 1990, by NASA and the European Space Agency (ESA), it has provided humanity with breathtaking images and invaluable scientific data, evolving our understanding of the cosmos.

      NASA/ESA HST—Hubble Space Telescope

      NASA/ESA HST—Hubble Space Telescope

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    • Nancy Grace Roman Space Telescope (or Roman Space Telescope), formerly NASA's Wide-Field Infrared Survey Telescope (WFIRST) is a groundbreaking space observatory mission designed to expand our understanding of the universe by conducting large-scale astronomical surveys in the infrared spectrum. WFIRST represents a crucial addition to NASA's arsenal of space telescopes, complementing the capabilities of the Hubble Space Telescope and addressing a wide range of astrophysical questions.

      NASA WFIRST—Wide-Field Infrared Survey Telescope/Nancy Grace Roman Space Telescope

      NASA WFIRST—Wide-Field Infrared Survey Telescope/Nancy Grace Roman Space Telescope

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    • NASA's Transiting Exoplanet Survey Satellite (TESS), is a space mission designed to discover and study exoplanets orbiting stars outside our solar system. Launched on April 18, 2018, TESS is revolutionizing our understanding of exoplanets by searching for these distant worlds in a systematic and comprehensive manner.

      NASA TESS—Transiting Exoplanet Survey Satellite

      NASA TESS—Transiting Exoplanet Survey Satellite

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    • The Submillimeter Wave Astronomy Satellite (SWAS), a NASA space mission, was dedicated to exploring the universe in the submillimeter wavelength range, a relatively uncharted territory in astronomical observations. Launched in 1998, SWAS was designed to observe molecular clouds and star-forming regions to better understand the processes of star birth.

      NASA SWAS—Submillimeter Wave Astronomy Satellite

      NASA SWAS—Submillimeter Wave Astronomy Satellite

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    • The NASA Spitzer Space Telescope, also known as the Spitzer, was a remarkable space observatory mission designed to explore the universe in the infrared portion of the electromagnetic spectrum. Launched in 2003, Spitzer was part of NASA's Great Observatories program.

      NASA Spitzer Space Telescope

      NASA Spitzer Space Telescope

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    • The NASA Laser Interferometer Space Antenna (LISA) is a groundbreaking mission designed to detect and study gravitational waves, ripples in spacetime caused by massive celestial events like the collision of black holes and neutron stars. LISA represents an international collaboration, with contributions from both NASA and the European Space Agency (ESA).

      NASA LISA—Laser Interferometer Space Antenna

      NASA LISA—Laser Interferometer Space Antenna

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    • The NASA James Webb Space Telescope (JWST), often referred to as Webb, stands as a monumental advancement in space exploration and astronomy. Launched in December 2021, the JWST boasts an array of cutting-edge scientific instruments, including the Near Infrared Spectrograph (NIRSpec), Mid-Infrared Instrument (MIRI), and Near Infrared Camera (NIRCam). This advanced technology will enable Webb to observe the universe in unprecedented detail.

      NASA James Webb Space Telescope

      NASA James Webb Space Telescope

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    • NASA's Imaging X-ray Polarimetry Explorer (IXPE) is a groundbreaking space mission designed to advance our understanding of celestial objects emitting X-rays. Launched in 2021, IXPE is equipped with cutting-edge technology to measure the polarization of X-rays, providing valuable insights into the high-energy universe.

      NASA IXPE—Imaging X-ray Polarimetry Explorer

      NASA IXPE—Imaging X-ray Polarimetry Explorer

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    • The NASA Fermi Gamma-ray Space Telescope, previously known as the Gamma-ray Large Area Space Telescope (GLAST), is a space observatory launched in 2008, dedicated to exploring the gamma-ray universe. Fermi is designed to detect and study high-energy gamma-ray emissions from a wide range of celestial sources, contributing to our understanding of the universe's most energetic phenomena.

      NASA GLAST/Fermi—Gamma-ray Large Area Space Telescope

      NASA GLAST/Fermi—Gamma-ray Large Area Space Telescope

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    • The NASA Far Ultraviolet Spectroscopic Explorer (FUSE), was a space mission launched in 1999 with the primary goal of studying the universe in the far-ultraviolet (FUV) region of the electromagnetic spectrum. FUSE was part of NASA's Great Observatories program and was instrumental in advancing our understanding of celestial objects.

      NASA FUSE—Far Ultraviolet Spectroscopic Explorer

      NASA FUSE—Far Ultraviolet Spectroscopic Explorer

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    • The Constellation-X, (Con-X), was a proposed NASA X-ray space observatory mission aimed at advancing our understanding of the high-energy universe. While the mission was in development, it represented a significant step forward in X-ray astronomy.

      NASA CxP—Constellation-X Space Observatory

      NASA CxP—Constellation-X Space Observatory

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    • Suzaku, previously known as Astro-E2, is a Japanese space mission launched by the Japan Aerospace Exploration Agency (JAXA) in collaboration with NASA. This X-ray observatory was designed to study high-energy X-rays from celestial sources, providing critical insights into the universe's most extreme and energetic phenomena.

      JAXA/NASA Suzaku (Astro-E2) Satellite

      JAXA/NASA Suzaku (Astro-E2) Satellite

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    • The Cosmic Origins Spectrograph (COS) is a cutting-edge scientific instrument that has significantly advanced our understanding of the universe's origins and evolution. Installed on the Hubble Space Telescope (HST) during the fifth and final HST servicing mission in 2009, COS is designed to dissect the light from distant celestial objects into its constituent wavelengths, providing scientists with invaluable data on the composition, temperature, and motion of various cosmic phenomena.

      COS—Cosmic Origins Spectrograph

      COS—Cosmic Origins Spectrograph

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