IRAS infrared satellite  updated March 3, 2016  D. Carrigan (subject line must be sensible)

Channeling Adv. Accel. Dyson/IA
SETI Biography Bibliography Infrared

For a comprehensive Dyson Sphere search it is useful to have a whole sky survey. This rules out point and shoot satellite instruments like the Spitzer Space Telescope and NICMOS (the Near Infrared Camera and Multi-object Spectrograph on Hubble). In addition, the search instrument needs to be sensitive to temperatures ranging from roughly 100 to 600 ºK. The wavelengths associated with this interval span 10 to 100 μm. Ground-based infrared telescopes are ruled out for this regime because of the high sky background. This eliminates the sensitive, whole sky, ground-based 2MASS survey as the principle search tool because it only goes out to 2.17 μm. Finally good angular resolution is useful to rule out associations with nearby stars.

The IRAS database is the best existing resource available to address these three requirements [see, for example, C. Beichman, Ann. Rev. Ast 25, 521-63 (1987)]. The IRAS satellite flew in 1983. It identified 250,000 infrared point sources and scanned 98% of the sky. These sources were measured with four filters centered at 12, 25, 60, and 100 μm. This is almost ideal for a Dyson Sphere search. One of the principle motivations of the IRAS program was an investigation of cosmic dust. Partly as a result of that the lens of the telescope had a diameter of only 60 cm so that the angular extent of a “point source” is O(1 minute). The positional reconstruction error is quoted as about 2" to 6" in-scan and about 8" to 16" cross-scan. The sensitivity was O(0.5 Jy) for the 12, 25, and 60 μm bands and 1 Jy for the 100 μm band.

The 2MASS survey with nearly 500 M sources is both much more sensitive and precise in the near infrared. Each of the two 2MASS telescopes had a mirror diameter of 1.3 m. The positional reconstruction error is 0.5". However a blackbody source centered on the 12 μm IRAS band must be at least 10 Jy to register in the 2MASS 2.17 μm band. This is a factor of order ten times higher than the minimum IRAS sensitivity. If the two sources can be correlated one can take advantage of the better 2MASS angular resolution and pointing accuracy.


(The photo of IRAS is from NASA)