In its time the Infrared Space Observatory (ISO) was the most sensitive infrared satellite ever launched. ISO made particularly important studies of the dusty regions of the Universe, where visible light telescopes can see nothing. The wealth of data collected by ISO still produce important science results.
In 1983 the US–Dutch–British IRAS satellite inaugurated infrared space astronomy by mapping 250 000 cosmic infrared sources and large areas of extended emission. However, that was only the beginning. ISO's detectors, with an enhanced sensitivity and resolution (by 1000 times in sensitivity and by 100 times in angular resolution at 12 microns), have allowed a much closer look, a much more detailed perception of the 'infrared scenery'. ISO has therefore provided astronomers with a unique facility to see both familiar objects in an unusual way and objects that are invisible at other wavelengths.
Infrared radiation is primarily 'heat', or thermal radiation. Even objects that we think of as being very cold, such as an ice cube, emit infrared radiation.
For this reason, ISO, operating at wavelengths from 2.5 to 240 microns, could observe astronomical objects that remain hidden for optical telescopes, such as cool objects that are unable to emit in visible light. Opaque objects, those surrounded by clouds of dust, are another specialty of ISO because the longer IR wavelengths can penetrate the dust, allowing us to see deeper into such clouds.
On average, ISO performed 45 observations per revolution (a period of almost 24 hours). Throughout all of its lifetime - more than 900 revolutions - ISO successfully completed well some 30 000 scientific observations.
The satellite essentially consisted of a cryostat, the telescope, four scientific instruments, and the service module:
Observing the cool Universe requires cooled instruments which can work at temperatures close to absolute zero, –273°C. Keeping the temperature this low was the task of the large liquid-helium cryostat on board ISO, filled before launch with 2286 litres of superfluid helium. This cryostat made ISO one of the coldest objects in the universe. ISO’s lifetime was limited by its helium supply, so nearly all observations had to stop when this coolant liquid was depleted on 8 April 1998.
A telescope with a 60-centimetre diameter primary mirror feeds infrared light via a pyramidal mirror to the four instruments. The fields of view and the selection of wavelengths were varied, to suit the nature of the object examined.
ISO’s infrared camera (ISOCAM) covered the 2.5 to 17 micron band with two different detectors. It can be compared to a normal photo camera, taking pictures of the 'infrared face' of astronomical objects at a high resolution (so as to distinguish very fine details).
The ISO photo-polarimeter (ISOPHOT) was designed to detect the amount of infrared radiation emitted by an astronomical object. The broad range of wavelengths at which ISOPHOT operated (between 2.5 and 240 microns) allowed it to 'see' objects as cool as the clouds of dust lying among stars and galaxies, whose temperature may be just a few degrees above –273°C.
The Short-Wave Spectrometer (SWS) covered the 2.4 to 45 micron band. It has provided valuable information about the little known chemistry of the Universe, since many molecules emit copiously in the infrared. Moreover, SWS has been able to study the physical conditions of those chemical constituents, such as temperature or density.
The Long-Wave Spectrometer (LWS) operated at the 45 to 196.8 micron band. LWS has focused on cooler objects than SWS. It is especially useful studying the physical condition in very cold dust clouds in the space between stars.
The service module provided electrical power, attitude control, and telecommunications.
ISO's highly elliptical orbit around the Earth took almost 24 hours. For almost 17 hours per day ISO was outside the radiation belts surrounding Earth. During this time, all of ISO's detectors could be operated.
ISO was launched by an Ariane 44P launcher from Europe's spaceport in Kourou, French Guiana, on 17 November 1995. Initially it was supposed to be operational for 18 months, but thanks to meticulous engineering and some good fortune, the satellite's working life was stretched to more than 28 months until May 1998.
Just before ISO was switched off on 16 May 1998, its orbit was changed to force the satellite to burn up in the atmosphere, contributing to preserving the environment in space.
However, ISO continued to give scientific surprises to the very end. ISO's 'last-light' observation - taken with the SWS instrument just before midnight on 10 May - was of emission lines from hydrogen in the hot supergiant star Eta Canis Majoris.
The ISO project was started by ESA in 1983 under its Horizon 2000 science programme. The investment involved covered satellite development, launch, and in-orbit operation. The scientific instruments were provided separately by a group of eleven European countries. The United States and Japan co-operated on ground support operations in return for average daily observing time of half an hour each.
The scientific instruments were developed by multinational teams, with leaders in France, Germany, the Netherlands, and the United Kingdom.
The satellite was developed, manufactured, integrated, and tested by an industrial consortium made up of 32 companies, mostly from Europe, headed by Aérospatiale, France.
Last update: 14 October 2003