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  2. Infrared telescope - Wikipedia

    en.wikipedia.org/wiki/Infrared_telescope

    An infrared telescope is a telescope that uses infrared light to detect celestial bodies. Infrared light is one of several types of radiation present in the electromagnetic spectrum . All celestial objects with a temperature above absolute zero emit some form of electromagnetic radiation . [ 1 ]

  3. James Webb Space Telescope - Wikipedia

    en.wikipedia.org/wiki/James_Webb_Space_Telescope

    The James Webb Space Telescope (JWST) is a space telescope designed to conduct infrared astronomy.As the largest telescope in space, it is equipped with high-resolution and high-sensitivity instruments, allowing it to view objects too old, distant, or faint for the Hubble Space Telescope. [9]

  4. Fine Guidance Sensor and Near Infrared Imager and Slitless ...

    en.wikipedia.org/wiki/Fine_Guidance_Sensor_and...

    The FGS will help the telescope aim and stay pointed at whatever it is commanded to look at. [7] FGS helps provide data to the JWST Attitude Control System (ACS) and to do this it has a big sky coverage and sensitivity, to give a high probability it can find a guide star. [8] NIRISS is designed for performing: [9] [10] Near-infrared imaging

  5. Photometric system - Wikipedia

    en.wikipedia.org/wiki/Photometric_system

    The sensitivity usually depends on the optical system, detectors and filters used. For each photometric system a set of primary standard stars is provided. A commonly adopted standardized photometric system is the Johnson-Morgan or UBV photometric system (1953).

  6. Infrared - Wikipedia

    en.wikipedia.org/wiki/Infrared

    The sensitivity of Earth-based infrared telescopes is significantly limited by water vapor in the atmosphere, which absorbs a portion of the infrared radiation arriving from space outside of selected atmospheric windows. This limitation can be partially alleviated by placing the telescope observatory at a high altitude, or by carrying the ...

  7. Infrared astronomy - Wikipedia

    en.wikipedia.org/wiki/Infrared_astronomy

    Infrared astronomy is a sub-discipline of astronomy which specializes in the observation and analysis of astronomical objects using infrared (IR) radiation. The wavelength of infrared light ranges from 0.75 to 300 micrometers, and falls in between visible radiation, which ranges from 380 to 750 nanometers, and submillimeter waves.

  8. A New Space Telescope Will Unravel a Great Cosmic Mystery - AOL

    www.aol.com/news/space-telescope-unravel-great...

    The telescope will be able to look at a patch of sky 100 times larger than both the Hubble Space Telescope and the James Webb Space Telescope can. It will be able to peer up to 13.2 billion light ...

  9. Observational astronomy - Wikipedia

    en.wikipedia.org/wiki/Observational_astronomy

    See also Radio telescopes. Infrared astronomy deals with the detection and analysis of infrared radiation (this typically refers to wavelengths longer than the detection limit of silicon solid-state detectors, about 1 μm wavelength). The most common tool is the reflecting telescope, but with a detector sensitive to infrared wavelengths. Space ...