The Infrared Space Observatory (ISO)

Autor: Paul Barr, Martin F. Kessler
Rok vydání: 1994
Předmět:
Zdroj: Infrared Physics & Technology. 35:211-220
ISSN: 1350-4495
DOI: 10.1016/1350-4495(94)90082-5
Popis: The Infrared Space Observatory (ISO), a fully approved and funded project of the European Space Agency (ESA), will operate at wavelengths from 2.5 to 200 μm. ISO will provide astronomers with a unique facility of unprecedented sensitivity for a detailed exploration of the universe ranging from objects in the solar system right out to the most distant extragalactic sources. The satellite essentially consists of a large liquid-helium cryostat, a telescope with a 60-cm diameter primary mirror and four scientific instruments. The instrument complement is: an imaging photo-polarimeter (2.5–200 μm), a camera (2.5–17 μm), a short wavelength spectrometer (2.5–45 μm) and a long wavelength spectrometer (45–180 μm). These instruments are being built by international consortia of scientific institutes and will be delivered to ESA for in-orbit operations. ISO is scheduled to be launched in 1995 and will be operational for at least 18 months. In keeping with ISO's role as an observatory, two-thirds of its observing time will be made available to the general astronomical community.
Databáze: OpenAIRE