VACUUM MONSTER (Interplanetary Dust Collector)

The VACUUM MONSTER was a a highly sensitive volume-sampling micrometeorite collector developed by the University of Washington, in cooperation with Litton Industries, to capture interplanetary dust particles at an altitude of 35 km. The collector, capable of sampling over 106 cubic feet of ambient stratospheric air during a five-hour period, was named after the creature in the Beatles movie Yellow Submarine that sucked up everything.

In the image at left we can see an scheme of the collector and an actual picture of it (click to enlarge). The pump that powered the collector measured four meters long and used an air ejector system driven by the catalytic decomposition of hydrazine, with 150 pounds of hydrazine stored on board. It was a modified version of the one developed by Litton for sampling stratospheric bomb debris from nuclear tests. Air was drawn through a horn-shaped inlet and passed over 22 cylindrical collection rods mounted perpendicular to the airstream. These rods, coated in silicone oil, trapped incoming particles by inertial deposition. The rods were each 0.25 inches in diameter and 2.25 inches long and were highly efficient at capturing particles larger than approximately 2 micrograms. Before and after the collection phase, the rods were sealed from contamination using a slide-gate mechanism, a butterfly valve, and a removable cover, all of which were critically cleaned in a class-100 cleanroom.

To minimize contamination from the balloon or the gondola, the collector was suspended 3000 feet below the balloon using a nylon line. A 30-foot tail boom with 400 cubic feet of deployed sail area gave the collector wind-vane-like aerodynamics, ensuring that the horn inlet always faced the incoming stratospheric wind. This setup created an environment analogous to a laminar-flow cleanroom. The orientation of the collector was continuously monitored with a flux gate magnetometer and a sequence camera. Only the upstream-facing halves of the rods were exposed to incoming particles, while the downstream halves served as controls to identify and rule out any contamination from handling or the instrument itself.

Balloon launched on: 4/21/1970 at  
Launch site: Columbia Scientific Balloon Facility, Palestine, Texas, US  
Balloon launched by: NCAR National Scientific Balloon Flight Station
Balloon manufacturer/size/composition: Zero Pressure Balloon Winzen - 2.900.000 cuft (1.0 mil. Stratofilm)
Flight identification number: 542P
End of flight (L for landing time, W for last contact, otherwise termination time): 4/21/1970
Balloon flight duration (F: time at float only, otherwise total flight time in d:days / h:hours or m:minutes - ): F 3 h
Landing site: In Lake Charles, Louisiana, US
Payload weight: 815 lbs.

The balloon was launched on April 21, 1970 from the NCAR's flight station of Palestine, Texas. During the flight, approximately 171,000 cubic feet of air were sampled, and the scanning process was fully effective only for particles larger than 10 micrograms. Twelve particles were found on the upstream rod surfaces and seven on the downstream, which represented a low signal-to-noise ratio. However, morphological analysis using a scanning electron microscope and chemical analysis using a microprobe identified at least two particles as likely extraterrestrial in origin: a 12-micron opaque spherule composed primarily of Fe and Mg, and a 10-by-30-micron cellular particle composed of Si, Mg, S, and Fe. The spherule's composition was consistent with chondritic material, while the complex porous structure of the cellular particle made it unlikely to be an ablation product, suggesting a more primitive, possibly cometary origin.

The payload was recovered in Lake Charles, Louisiana.

• Cosmic dust - Collection and research Annual review of earth and planetary sciences. Volume 13. Palo Alto, CA, Annual Reviews, Inc., 1985, p. 147-173
• Cosmic Dust webpage University of Washington
• NCAR Scientific Balloon Facility Annual Report, 1970 National Center for Atmospheric Research, February 1971
• The Physical Nature of Interplanetary Dust as Inferred by Particles Collected at 35 KM Evolutionary and Physical Properties of Meteoroids, Proceedings of IAU Colloq. 13, held in Albany, NY, 14-17 June 1971