Infrared Space Observatory oor Nederlands
Infrared Space Observatory
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The Infrared Space Observatory (ISO) was a space telescope for infrared light designed and operated by the European Space Agency (ESA), in cooperation with ISAS (part of JAXA as of 2003) and NASA.
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The Infrared Astronomical Satellite was the first-ever space-based observatory to perform a survey of the entire sky at infrared wavelengths.
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The European Space Agency launched a space-based mission known as the Herschel Space Observatory (formerly called Far Infrared and Sub-millimetre Telescope or FIRST) in 2009.
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Strong extinction in earth's atmosphere of some wavelength regions (such as X-ray, ultraviolet, and infrared) is overcome by the use of space-based observatories.
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ESA’s Infrared Space Observatory (ISO) satellite showed that there might be as many as two million asteroids larger than one kilometre in the region of space known as the 'asteroid belt'.
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First glimpses of the “leftovers” of this meal were obtained thanks to observations with the ESA Infrared Space Observatory, which revealed a 16 500 light-year-wide structure, very similar to that of a small barred galaxy.
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In 2010, the Herschel Space Observatory, a telescope with a comparatively superior spatial resolution and, unlike Spitzer, able to resolve radiation excesses beyond the wavelength of 70 μm, determined the infrared excess as coming from a two-lobed structure that looked like a debris disk seen edge-on.
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The answer to the long-standing mystery has been given by ESA’s Herschel space observatory, the most sensitive infrared telescope ever launched.
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Hogerheijde uses telescopes and satellites that are sensitive to the sub-millimetre and infrared areas of the electro-magnetic spectrum, such as the Herschel Space Observatory in the recent past and the Atacama Large Millimeter Array (ALMA) at present.
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“It’s exciting to get our first look at ATLASGAL, and we will be increasing the size of the map over the next year to cover all of the galactic plane visible from the APEX site on Chajnantor, as well as combining it with infrared observations to be made by the ESA Herschel Space Observatory.
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[2] The researchers also used data from the Wide Field Camera 3 on board the NASA/ESA Hubble Space Telescope and NIRC2 (the Near-Infrared Camera, second generation) at the W. M. Keck Observatory.
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Data from the OSIRIS camera on ESA’s Rosetta spacecraft [2], ESO’s New Technology Telescope (NTT) at the La Silla Observatory in Chile, and NASA’s Infrared Telescope Facility in Hawaii and Spitzer Space Telescope were combined to create the most complete spectrum of an asteroid ever assembled [3].
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Observations with NASA's Chandra X-ray Observatory (shown here in blue) reveal hot regions created by these winds and shocks, while infrared data from NASA's Spitzer Space Telescope (shown in red) outline where the dust and cooler gas are found.
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Together with observations of the deep cloud structure by the 3-metre NASA Infrared Telescope Facility in Hawaii, the level of thermal detail observed from these giant observatories is for the first time comparable to visible-light images from the NASA/ESA Hubble Space Telescope.
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Astronomers at Paranal Observatory in Chile recently enjoyed this unique opportunity when one of the telescope’s instruments, VIMOS (VIsible Multi-Object Spectrograph), was decommissioned to free up a space at the UT3 telescope for the upcoming CRIRES+ (the CRyogenic InfraRed Echelle Spectrograph Upgrade Project).
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Testing equipment such as the infrared spectrometer on the plane will allow scientists to develop next-generation technologies that could be flown into space to gather data cheaply and quickly for a range of scientific applications, says Scott McIntosh, director of the National Center for Atmospheric Research’s High Altitude Observatory in Boulder, Colorado.
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24 December 2018: Few people have ever viewed the Moon through a telescope as monumental as ESO’s Very Large Telescope (VLT). Astronomers at Paranal Observatory in Chile recently enjoyed this unique opportunity when one of the telescope’s instruments, VIMOS (VIsible Multi-Object Spectrograph), was decommissioned to free up a space at the UT3 telescope for the upcoming CRIRES+ (the CRyogenic InfraRed Echelle Spectrograph Upgrade Project).
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