Binary Colloidal Alloy Test - 6: Seeded Growth (BCAT-6-Seeded Growth) - 11.22.16
The Binary Colloid Alloy Test-6: Seeded Growth (BCAT-6-Seeded Growth) builds on previous research looking at how dense groups of particles may be coaxed to form crystal structures when much larger “seed” particles are added. Some materials may consist of large individual crystals, or groups of many smaller crystals organized in a larger structure. Knowing when and how either type of crystal will form gives insight into how to control crystal growth which is important in many industrial processes.
Science Results for Everyone
Information Pending Experiment Details
Paul M. Chaikin, Ph.D., New York University, New York, NY, United States
Andrew D. Hollingsworth, Ph.D., New York University, New York, NY, United States
ZIN Technologies Incorporated, Cleveland, OH, United States
Sponsoring Space Agency
National Aeronautics and Space Administration (NASA)
Human Exploration and Operations Mission Directorate (HEOMD)
ISS Expedition Duration
September 2010 - September 2013
The BCAT predecessors, BCAT-3 operated on ISS, and BCAT, operated on Mir in 1997 and 1998. BCAT-4 launched March 11, 2008 on 1J/A, and BCAT-5 launched June 13, 2009 on 2J/A.
- The crystallization of matter is a well studied field but to this time scientists are still learning the rules by which nature allows matter to form crystals.
- BCAT-6 studies the crystallization of specialized particles in microgravity. It is through these studies that scientists aim to understand how materials crystallize and what makes them crystallize in the way they do. Through this understanding, scientists aim to control and predict crystallization processes.
- Controlling the organization of matter in crystals, atom-by-atom, will allow for the development of a vast improvement in existing technologies in a wide range of fields such as medicine, high-speed computers, high-density memory storage, and electronic displays.
Previous work has shown that the rate of crystal growth initiation is accelerated when spherical seed particles of a certain size ratio are introduced into the colloidal suspension at or above a particular particle number density. Consequently, the number of small microscopic crystals (crystallites) should exceed the number of seeds resulting in smaller crystallites and a greatly increased nucleation rate. These experiments are therefore relevant to many industrial processes where the control of crystal size and crystallization rate are important.
Binary Colloidal Alloy Test-6, Seeded Growth, samples 6 and 7 (BCAT-6, Seeded Growth) builds upon the breakthrough NASA PHaSE experiment which showed that glasses in concentrated systems (as seen on Earth) tend to order into crystals when gravitational effects are absent. Particles which are of a single size have been created for this sample. The size of the particles is selected to be the size of a wavelength of visible light. It is necessary to have the particles this size so that they can be large enough to be observed with visible light but small enough for their movements to be a result of a temperature dependent but seemingly random motion known as Brownian motion. White light from a flashlight and the camera flash are used to detect the colorful reflections produced by colloidal crystals formed following the sample mixing. The idea of applying spherical seed particles to the wall of the sample cell is new and significant. According to theory and simulations, this allows for the formation of an array of crystallites rather than one large crystal as would be produced in a homogeneous solution. In this experiment, half of the surface seen by the camera is covered by seeds, while the other half of the container is not. Two volume fractions are prepared, one at the minimum theoretical volume fraction causing complete crystallization (volume fraction = 0.53) and one in the glassy regime (volume fraction = 0.60).
The ‘crystallization catalysts’ allow for the completion of several experiments at once in order to see the effects of placing seed particles on the cell walls, and to determine how the particle volume fraction can affect the rate of crystal nucleation. If this strategy is successful, this will guide the choice of the optimal particle volume fractions to be used in the seeded growth experiments studied over a wide range in greater detail in the Advanced Colloids Experiment (ACE). While predicted in theory, this experiment has not been possible on earth because of particle sedimentation. Microgravity allows for both index matching (for clarity) and density matching (to avoid sedimentation in 1g). Performing these experiments on the International Space Station (ISS) allows excellent index of refraction matching without the requirement of simultaneous density matching.
Space-based production of crystals could provide larger crystals with better properties to serve as models for studies and improvement to their Earth analogs.
Understanding the mechanisms that affect crystal growth, such as particle size and density, could lead to new methods for controlling this growth and enhancing the properties of materials in many industrial manufacturing processes ranging from plastics, household goods, and medicine just to name a few.
Operational Requirements and Protocols
The current plan for this experiment is to conduct it over a 7-day session, each of which can be run incrementally and will each require about 7 hours of crew-time; a third session to mix and photograph all 10 samples (about 4.6 hours of crew time) and then a fourth session at six months to photograph all ten samples which is slotted to take about four hours of crew time.
Session 1: Set up hardware, take baseline photos of all ten samples; homogenize samples 6-10 then samples 9 and 10, then automatically photograph sample 1 (using EarthKAM software on laptop) every hour for 7 days. Perform sample 1 daily status check each day. After seven-day run, perform crystal search/photography on 6-10. Homogenize sample 2, automatically photograph sample 2 (using EarthKAM software on laptop) every hour for 7 days. Perform sample 1 daily status check each day. After seven-day run, perform crystal search/photography on 6-10. If necessary, tear down after operations are complete but keeping setup intact is preferred to save crew time.
Session 2: Set up hardware, homogenize samples 3, 4 and 5 one at a time then automatically photograph each sample (using EarthKAM software on laptop) every hour for 14 days each. Perform Crystal Check and Photography procedures on 6-10 if crystals not found/photographed in Session 1. If necessary, tear down after operations are complete but keeping setup intact is preferred to save crew time. .
Session 3: Homogenize and photograph samples 1-10 (using EarthKAM software on laptop) and stow sample module for six months. The experiment is torn down after operations are complete. .
Session 4: At six months after homogenization, manually photograph Ssamples 1 through 10. Re-stow sample module and tear down after operations are complete.
Decadal Survey Recommendations
Applied Physical Science in Space AP5
Fundamental Physical Sciences in Space FP1
Information Pending^ back to top
ISS Research Project-BCAT-Seeded Growth
NIH BioMed-ISS Meeting Video Presentation, 2009—BCAT-6-Polystyrene
NIH BioMed-ISS Meeting, 2009—BCAT-6-Polystyrene
Scanning Electron Microscope (SEM) images of a mixture of 3.8 micron diameter ‘seed’ particles together with the bulk colloid (0.33 micron diameter Poly(methyl methacrylate) (PMMA) spheres). Crystal nucleation on the spherical surfaces could produce small nuclei that grow radially outward. Due to curvature that makes it difficult to maintain an unstrained structure, they should detach from the surface, allowing the seed to produce new crystal nuclei. Image courtesy of Glenn Research Center.
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