infrared astronomy oor Nederlands
infrared astronomy
en
(astronomy) the astronomical observation and study of objects, cooler than most stars, using the infrared part of the electromagnetic spectrum
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Infraroodastronomie
en
observational astronomy of emissions over the wavelength band 0.75 to 300 micrometers
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Infrared astronomy is the branch of astronomy and astrophysics that studies astronomical objects visible in infrared (IR) radiation.
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Recent advances in infrared astronomy revealed a space only six light-years across, packed with a thick population of stars.
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Infrared astronomy has also been used to assess the composition of solid materials in the interstellar medium, including silicates, kerogen-like carbon-rich solids, and ices.
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This is why imaging with aperture synthesis has been used successfully in radio astronomy since the 1950s and in optical/infrared astronomy only since the turn of the millennium.
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Astronomical interferometers are commonly used for high-resolution optical, infrared, submillimetre and radio astronomy observations.
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But ifyou go into the infrared... or use radio astronomy or X-ray astronomy... you can see what's going on there.
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- The availability of independent means of launch which has made it possible to carry out several wholly European large-scale space missions, giving Europe a pioneering position in particular fields (e.g. astrometry, infrared or X-ray astronomy);
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Modern infrared astronomy
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Astronomical interferometers are widely used in optical astronomy, infrared astronomy, submillimetre astronomy and radio astronomy.
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SOFIA is NASA’s stratospheric observatory for infrared astronomy, which makes its observations from a modified Boeing 747.
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For many Harm Habing is "the face" for the Dutch infrared astronomy, and particularly the space research involving the cool universe.
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To elaborate on SRON’s contributions to infrared astronomy, Peter Roelfsema gave a talk on this subject for an interested audience of about fifty people.
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The decisive factors for these findings were data from the Stratospheric Observatory for Infrared Astronomy, SOFIA, which observed Comet Wirtanen as it passed Earth in December 2018.
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This is why imaging with aperture synthesis has been used successfully in radio astronomy since the 1950s and in optical/infrared astronomy only since the 2000 decade.
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Far-infrared astronomy is the branch of astronomy and astrophysics that deals with objects visible in far-infrared radiation (extending from 30 μm towards submillimeter wavelengths around 450 μm).
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Researchers from various institutions, including SRON and Delft University of Technology, have demonstrated that it is possible to make a highly sensitive space camera for far-infrared astronomy by using a special type of superconducting detector.
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Xander Tielens is closely involved in the development and use of large apparatus and satellites, including the SOFIA telescope for infrared astronomy and the European Herschel satellite which is used to study the formation of galaxies and stars.
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Researchers from various institutions, including SRON and the Microelectronics Department from Delft University of Technology, have demonstrated that it is possible to make a highly sensitive space camera for far-infrared astronomy by using a special type of superconducting detector.
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To our eyes, most of these stars would be hidden behind the dust, but ESO’s Visible and Infrared Survey Telescope for Astronomy (VISTA) sees near-infrared light, which passes right through dust.
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This will soon drastically increase by a factor of 10 or so as the Visible and Infrared Survey Telescope for Astronomy (VISTA) with its near infrared camera will alone produce about 150 TB of data each year.
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05 Gusht 2019: The telescope in this eye-catching picture is appropriately named VISTA, short for the Visible and Infrared Survey Telescope for Astronomy.
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5 August 2019: The telescope in this eye-catching picture is appropriately named VISTA, short for the Visible and Infrared Survey Telescope for Astronomy.
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5. elokuuta 2019: The telescope in this eye-catching picture is appropriately named VISTA, short for the Visible and Infrared Survey Telescope for Astronomy.
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ESOcast 74 looks at ESO’s pair of survey telescopes at Paranal: the Visible and Infrared Survey Telescope for Astronomy (VISTA) and the VLT Survey Telescope (VST).
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One of them, the 4.1-metre Visible and Infrared Survey Telescope for Astronomy (VISTA), is located on a neighbouring peak not far from the Paranal summit.
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