Long-wavelength spectrometer from the Infrared Space Observatory (identical spare model)

Long-wavelength spectrometer from the Infrared Space Observatory (identical spare model) Long-wavelength spectrometer from the Infrared Space Observatory (identical spare model) Long-wavelength spectrometer from the Infrared Space Observatory (identical spare model)

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Creative Commons LicenseThis image is released under a CC BY-NC-SA 4.0 Licence

Buy this image as a print 

Buy

License this image for commercial use at Science and Society Picture Library

License

Creative Commons LicenseThis image is released under a CC BY-NC-SA 4.0 Licence

Buy this image as a print 

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License this image for commercial use at Science and Society Picture Library

License

Science Museum Group
© The Board of Trustees of the Science Museum

Science Museum Group Collection
© The Board of Trustees of the Science Museum

Science Museum Group Collection
© The Board of Trustees of the Science Museum

Twin spare of the long-wavelength spectrometer from ISO (Infra-red Space Observatory). Assembled and tested at Rutherford Appleton Laboratory, c.1993.

Cosmic dust between the stars blocks out visible light, but it can be penetrated by infrared. Scientists study the infrared radiation emitted by gas molecules to find out more about cooler areas of space where stars have yet to form, or have died.

This instrument is identical to one flown on the Infrared Space Observatory, launched in 1995. This satellite revealed the presence of water in many parts of our galaxy.

Details

Category:
Temporary Exhibitions
Object Number:
L2009-4033
Materials:
plastic (unidentified), metal (unknown), steel (metal), aluminium (metal), rubber (unidentified) and electronical component
Measurements:
overall: 255 mm x 385 mm x 260 mm, 7.048 kg
type:
spectrometer - infra-red
credit:
On loan from Rutherford Appleton Laboratory

Parts

Long-wavelength spectrometer from the Infrared Space Observatory (identical spare model)

Long-wavelength spectrometer from the Infrared Space Observatory (identical spare model)

Twin spare of the long-wavelength spectrometer from ISO (Infra-red Space Observatory). Assembled and tested at Rutherford Appleton Laboratory, c.1993.

More

Cosmic dust between the stars blocks out visible light, but it can be penetrated by infrared. Scientists study the infrared radiation emitted by gas molecules to find out more about cooler areas of space where stars have yet to form, or have died.

This instrument is identical to one flown on the Infrared Space Observatory, launched in 1995. This satellite revealed the presence of water in many parts of our galaxy.

Measurements:
overall: 255 mm x 385 mm x 260 mm, 7.048 kg
Materials:
plastic (unidentified) , metal (unknown) , steel (metal) , aluminium (metal) , rubber (unidentified) and electronical component
Object Number:
L2009-4033/1
type:
spectrometer - infra-red
Carry case for long-wavelength spectrometer from the Infrared Space Observatory (identical spare model)

Carry case for long-wavelength spectrometer from the Infrared Space Observatory (identical spare model)

Carry case for twin spare of the long-wavelength spectrometer from ISO (Infra-red Space Observatory). Assembled and tested at Rutherford Appleton Laboratory, c.1993.

Measurements:
overall: 255 mm x 385 mm x 260 mm, 7.048 kg
Materials:
plastic (unidentified) , metal (unknown) , aluminium (metal) and rubber (unidentified)
Object Number:
L2009-4033/2
type:
carry case