header graphic
Dust and Aerosol Measurement Feasibility Test (DAFT)


      P-Trak and components  
    The P-Trak® and its components (clockwise from the left: alcohol wick, wick container, container cap, P-Trak®, and battery pack).  
    A cross section of the modified P-Trak condenser chamber  
    A cross section of the modified P-Trak® condenser chamber shows the microgrooves that NASA engineers cut on the inside diameter to improve the flow of alcohol back to the wick in microgravity.  
    DustTrak and P-Trak  
    An engineer holding the DustTrak® (top) and the P-Trak® in their approximate locations in the Expedite the Process of Experiments to Space Station (EXPRESS) Rack (the blue velcro board has been superceded by straps).  
    The DustTrak®—shown here with its battery pack—is insensitive to gravitational forces. It is used to determine the accuracy of the modified P-Trak®.  
acrobat icon
DAFT Overview Chart
acrobat icon
DAFT Short Overview Presentation

The Dust and Aerosol Measurement Feasibility Test (DAFT) was designed to ensure that a modified P-Trak®—a key component of the forthcoming NASA Smoke Aerosol Measurement Experiment (SAME)—will perform properly in the unique environment of microgravity. If the P-Trak® performs as expected, the device will be used in SAME to provide data that will help scientists design better fire detectors for future, longduration, manned missions.

The Challenge

The P-Trak® is a commercial device that counts ultrafine particles (it can recognize particles as small as 0.02 micrometers in diameter). It works by passing particulate-laden air through a heated chamber of vaporous isopropyl alcohol. The individual particles serve as seeds around which the alcohol condenses when cooled, forming droplets large enough to be detected and counted as they scatter light from a laser beam (see the schematic on the other side). The P-Trak® must be tested in microgravity prior to its use in SAME because its alcohol condenser was redesigned to work properly in microgravity. (The original smooth-walled P-Trak® condenser—meant for Earth based use—depends on gravity.) NASA scientists modified the unit’s condenser by forming microgrooves in its wall to increase the alcohol flow back to the wick (see photo on right). This modification was based on the knowledge gained from previous microgravity fluids physics experiments conducted by researchers at NASA Glenn Research Center

The Plan

The main components of the DAFT experiment, the P-Trak® and the DustTrak® aerosol monitoring devices, were delivered to the International Space Station (ISS) in February 2005. (The DustTrak® uses a sensor to determine the intensity of light being scattered by particles and translates that number into an aerosol mass measurement. It is being used to test the accuracy of the P-Trak® because it is insensitive to gravitational forces.) The rest set of tests were conducted in February and March 2005 and the results were encouraging. Importantly, the muddied condenser performed as expected. The second set of tests will be conducted after the balance of DAFT parts (including a calibrated aerosol source and an unmodified P-Trak®) are delivered to the ISS.

Research Procedure

During the ISS tests conducted in 2005, astronauts performed several steps: 1. Turned on the P-Trak® and the DustTrak® 2. Attached high-efficiency particulate air (HEPA) filters to the inlets to “zero” the particle counters (since the HEPA filter removes all airborne particles, if the particle counters do not read “zero” something is amiss) 3. Connected the devices to a common sampling hose 4. Recorded the ISS environment for several minutes 5. Reconnected the HEPA filters to “zero” the particle counters 6. Turned off the P-Trak® and the DustTrak® The tests were conducted in the U.S. Laboratory Module Destiny in front of EXPRESS Rack 4; in the modules’s aft end and port side and in Node 1. (The EXPRESS Rack is a standardized payload rack system that transports, stores, and supports experiments aboard the ISS. Node 1 is a hub to which various modules are attached.) Three of the tests sampled undisturbed cabin air; the other test validated the instruments at high particulate levels by having an astronaut create airborne debris at the P-Trak® and DustTrak® inlets by separating pieces of Velcro®.

Results So Far

The three tests that sampled the undisturbed environment in the ISS showed very low levels of airborne particulates, averaging fewer than 0.005 mg/m3 from the DustTrak® and fewer than 15 particles/cm3 from the P-Trak® (these are typical readings at the baseline). These numbers are dramatically lower than the values recorded in the space shuttle in an earlier experiment (~0.050 mg/m3). Lower levels are to be expected because the ISS has HEPA filtration for the cabin air as compared to merely a fine screen on the shuttle air handler. Furthermore, the typical shuttle crew of seven astronauts generates more airborne particulate than an ISS crew of two astronauts.

Future DAFT Tests

The next series of tests will take place once the remaining DAFT equipment is delivered to the ISS. These will be performed with Arizona Road Dust (ARD)—a standard aerosol test material of known particle size and distribution—and nitrogen aerosol inside a 15-liter Mylar® bag. Testing a known particulate will allow scientists to establish definitively how well the P-Trak® works in microgravity.

Project Management:

Contacts at NASA Glenn Research Center

Project Manager: William Sheredy

Project Scientist: Dr. Gary Ruff

Principal Investigator: Dr. David Urban. NASA GRC


Dust and Aerosol Measurement Feasibility Test News





View Archives