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Cosmic Radiation Satellite

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A space telescope (also known as space observatory ) is a telescope in outer space used to observe astronomical objects. Suggested by Lyman Spitzer in 1946, the first operational telescopes were the American Orbiting Astronomical Observatory , OAO-2 launched in 1968, and the Soviet Orion 1 ultraviolet telescope aboard space station Salyut 1 in 1971. Space telescopes avoid several problems caused by the atmosphere, including the absorption or scattering of certain wavelengths of light, obstruction by clouds, and distortions due to atmospheric refraction such as twinkling . Space telescopes can also observe dim objects during the daytime, and they avoid light pollution which ground-based observatories encounter. They are divided into two types: Satellites which map the entire sky ( astronomical survey ), and satellites which focus on selected astronomical objects or parts of the sky and beyond. Space telescopes are distinct from Earth imaging satellites , which point toward Earth for satellite imaging , applied for weather analysis , espionage , and other types of information gathering .

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13-528: The Cosmic Radiation Satellite ( CORSA , also CORSA-A ) was a Japanese space telescope . It was supposed to be Japan's first X-ray astronomy satellite but was lost due to failure of its Mu-3 launch vehicle on 4 Feb 1976. A replacement satellite Hakucho (CORSA-b) was later launched. This article about one or more spacecraft of Japan is a stub . You can help Misplaced Pages by expanding it . Space telescope In 1946, American theoretical astrophysicist Lyman Spitzer , "father of Hubble" proposed to put

26-561: A telescope in space. Spitzer's proposal called for a large telescope that would not be hindered by Earth's atmosphere. After lobbying in the 1960s and 70s for such a system to be built, Spitzer's vision ultimately materialized into the Hubble Space Telescope , which was launched on April 24, 1990, by the Space Shuttle Discovery (STS-31). This was launched due to many efforts by Nancy Grace Roman, "mother of Hubble", who

39-533: Is limited by the filtering and distortion of electromagnetic radiation ( scintillation or twinkling) due to the atmosphere . A telescope orbiting Earth outside the atmosphere is subject neither to twinkling nor to light pollution from artificial light sources on Earth. As a result, the angular resolution of space telescopes is often much higher than a ground-based telescope with a similar aperture . Many larger terrestrial telescopes, however, reduce atmospheric effects with adaptive optics . Space-based astronomy

52-493: Is more important for frequency ranges that are outside the optical window and the radio window , the only two wavelength ranges of the electromagnetic spectrum that are not severely attenuated by the atmosphere. For example, X-ray astronomy is nearly impossible when done from Earth, and has reached its current importance in astronomy only due to orbiting X-ray telescopes such as the Chandra X-ray Observatory and

65-765: The Soviet space program (later succeeded by Roscosmos of Russia). As of 2022, many space observatories have already completed their missions, while others continue operating on extended time. However, the future availability of space telescopes and observatories depends on timely and sufficient funding. While future space observatories are planned by NASA, JAXA and the CNSA , scientists fear that there would be gaps in coverage that would not be covered immediately by future projects and this would affect research in fundamental science. On 16 January 2023, NASA announced preliminary considerations of several future space telescope programs, including

78-564: The XMM-Newton observatory . Infrared and ultraviolet are also largely blocked. Space telescopes are much more expensive to build than ground-based telescopes. Due to their location, space telescopes are also extremely difficult to maintain. The Hubble Space Telescope was serviced by the Space Shuttle , but most space telescopes cannot be serviced at all. Satellites have been launched and operated by NASA , ISRO , ESA , CNSA , JAXA and

91-832: The habitable zones of their stars, where liquid water can exist, by using a coronagraph to block out the light of their stars, as well as provide broad astrophysics observations. HWO builds upon studies conducted for two earlier mission concepts called the Large Ultraviolet Optical Infrared Surveyor (LUVOIR) and Habitable Exoplanets Observatory (HabEx). HWO’s main objective would be to identify and directly image at least 25 potentially habitable worlds. It would then use spectroscopy to search for chemical biosignatures in these planets’ atmospheres, including gases such as oxygen and methane, which could serve as critical evidence for life. HWO would also use its high sensitivity and resolution capabilities to trace

104-593: The Great Observatory Technology Maturation Program, Habitable Worlds Observatory , and New Great Observatories. Habitable Worlds Observatory The Habitable Worlds Observatory (HWO) is a large infrared , optical , and ultraviolet space telescope recommended by the National Academies ’ Decadal Survey on Astronomy and Astrophysics 2020. It will be optimized to search for and image Earth-size habitable exoplanets in

117-564: The HWO concept and decrease budget and schedule risks for the future mission. Two groups will guide the GOMAP activities for HWO: a Science, Technology, Architecture Review Team (START) and a Technical Assessment Group (TAG). The START will quantify HWO’s science objectives based on the Decadal Survey’s guidance and outline the observatory and instrument capabilities needed to accomplish them. Meanwhile,

130-472: The HWO's mission. The HWO is planned have a 6–8 meter mirror for now, but its design should be flexible to leverage launchers with potentially double the mass and volume by the time the HWO launches in the 2040s. Lee Feinberg, NASA HWO lead architect and James Webb Space Telescope manager, stays in communication with the three launchers' representatives. In 2024, he visited SpaceX to track Starship's progress. Former NASA JPL architect Casey Handmer believes

143-528: The TAG will study architecture options for HWO, identify and assess the mission architectures and technologies needed to enable those options, and evaluate the risks associated with those options. The HWO is designed to be launched on a super heavy-lift launch vehicle . The HWO's team hope for the success of big launchers such as SpaceX 's Starship , Blue Origin 's New Glenn or the SLS due to their critical importance to

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156-464: The evolution of galaxies and other cosmic structures. The main science themes for HWO are: In 2023, the National Aeronautics and Space Administration (NASA) established a Great Observatory Maturation Program (GOMAP) to unite government, industry, and academia to develop the technologies needed for HWO. GOMAP aims to draw on lessons from previous NASA missions to streamline development of

169-608: Was the first Chief of Astronomy and first female executive at NASA. She was a program scientist that worked to convince NASA, Congress, and others that Hubble was "very well worth doing". The first operational space telescopes were the American Orbiting Astronomical Observatory , OAO-2 launched in 1968, and the Soviet Orion 1 ultraviolet telescope aboard space station Salyut 1 in 1971. Performing astronomy from ground-based observatories on Earth

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