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![Page 1: 1 Granular Fluidization in Reduced Gravity University of Tulsa Supported by Research Corp. Justin Mitchell, Aaron Coyner, Rebecca Ragar, Matt Olson, Ian.](https://reader034.fdocuments.us/reader034/viewer/2022051619/56649e725503460f94b7202b/html5/thumbnails/1.jpg)
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Granular Fluidization in Reduced Gravity
University of TulsaSupported by Research Corp.
Justin Mitchell, Aaron Coyner, Rebecca Ragar, Matt Olson, Ian Zedalis, Adrienne McVey, Whitney Marshall
Michael Wilson*, Shawn Jackson
*Currently at National Research Council
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Project Description Goals
Look for definitive inelastic collapse of a 3-d granular system in zero gravity.
Determine parameters necessary for a granular gas, the precursor to collapse.
Methods Preliminary
testing on NASA KC-135A low gravity aircraft
Future flight on Space Shuttle
Testing on sounding rocket*
* É. Falcon et al. , Phys. Rev. Lett. 80. 440 (1999).
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Why Investigate Granular Gases?
Large granular systems, such as planets, are not well understood.
Asteroids, planetary rings, etc. are not fully explained by gravity because sizes are too small for gravity to act alone.
Inelastic collapse models provide plausible method for formation of these smaller objects.
Small scale granular gas studies allow for lab testing of the models on reasonable time scales.
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Experimental Description Box set: 8 sapphire
walled cubes, 1 in3 each.
Box set mechanically shaken sinusoidally along body diagonal.
Each cube has one free wall attached to a piezoelectric sensor.
Video cameras view 3 orthogonal box set faces.
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Box Set as Flown on KC-135A
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System Acceleration
Shaking direction is perpendicular to mean effective gravity.
In “microgravity” the residual acceleration is ~0.03 gearth *.
Residual acceleration is usually pointed up.
shaking
gearth
Residual acceleration
* From Charles Thomas, Boston University
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Granular Phases
SolidGrains pack in one corner
FluidGrains slosh around box walls
Gas~uniform distribution of kinetic grains
gresidual
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Phase Diagram
=A2/gresidual
is the ratio of wall acceleration to gresidual
diverges as gresidual goes to zero.
o Wall acceleration, density and gresidual define the phase.
0 10 20 30 40 50
gas
fluid
solid
c
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Experiment Geometries
• Shaking parallel to g
c2.0 *• A2 = 19.6 m/s2
g
shaking
gresidual
shaking
Normal Geometry Our Geometry
• Shaking normal to gresidual
c17
• A2 = 5.00 m/s2
*Y. Lan, A. D. Rosato, Phys. Fluids 7, 1818 (1995).
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Conclusions
There is a c that defines the phase transition to a
granular gas.
Geometry and density affect the value of c.
=A2/gresidual is a convenient way to compare
shaken granular experiments.
o Our geometry requires a higher wall accelerations
(in proportion to gresidual) to show a phase
transition.
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Future Work Ball tracking to give speed distribution.
Analyze impact data to obtain pressure information for gas phases.
First flight was preparation for later experiments.
Second KC-135A flight
Make free floating
Space Shuttle
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Ball diameter 0.50 mm Ball diameter 1.0 mmCell # #balls mfp (mm) L/mfp %Oc.Vl. Cell # #balls mfp (mm) L/mfp %Oc.Vl.
1 1000 17.1 1.4 0.5 4 250 17.1 1.4 1.02 3100 5.5 4.3 1.5 5 775 5.5 4.3 3.03 10000 1.7 13.9 4.9 6 2500 1.7 13.9 9.87 3100 0.50 mm balls
775 1.00 mm balls 4.5 Cell volume 13400 mm3Mean edge length 23.7 mm
Experiment Parameters
0.50 mm and/or 1.00 mm grade 200 brass
Mean free path (mfp) ~Vol./(Nd2)
%Oc.Vl. = % of volume occupied by balls
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25
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0 0.1 0.2 0.3 0.4 0.5
time (sec)
Hei
gh
t (m
m)
Residual Acceleration Balls above dense clusters follow parabolic
path. gResidual 0.023 gEarth
Within 25% of BU Data