B. D. Shaw and M. J. Harrison: Influences of support fibers on shapes of heptane/hexadecane droplets in reduced gravity
3
depend on the fiber surface as well as the interactions between
the fiber and the liquid comprising the droplet. Because the
fiber surfaces were not characterized in a detailed fashion in the
present experiments, it is difficult to predict characteristics of
any films that might be present. As a result, we have presented
analyses only for macroscopic droplet shapes and have not con-
sidered theory related to the film or the satellite droplets/bub-
bles.
droplet is f = gρ πD /6, where g is the gravitational accelera-
g
L
tion and ρ is the liquid density. The surface tension force f
L
σ
exerted on the droplet is characterized by f = 2πdσ, where σ is
σ
a characteristic surface tension. The Bond number is the ratio of
3
f to f , i.e., Bo = gρ D /(12dσ). It is estimated that Bo << 1 for
g
σ
L
the microgravity experiments under consideration here such
that gravitational effects should not cause significant asymme-
try of a droplet about a support fiber, i.e., only small deflections
of a droplet from its location of symmetry about a fiber are
required to balance gravitational forces normal to the fiber.
Momentum effects might also influence droplet shapes. For
example, internal flows are typically present within droplets
burning in microgravity, and there is also a momentum change
associated with vaporization at the gas-liquid interface. The
ratio of inertial forces to surface tension forces is the Weber
number (We). Inertial forces related to flows within droplets are
Conclusions
This research has shown that previous theory [7] and the asymp-
totic theory developed in this paper can be used to predict sha-
pes of burning or evaporating heptane/hexadecane droplets sup-
ported on thin fibers in reduced gravity. For the theory to be
accurate, however, it appears that droplets need to maintain
nearly steady positions on support fibers. This implies that sha-
pes of nearly stationary fiber-supported burning droplets are
dominated by surface tension and the contact angle between the
liquid and the fiber, which is in agreement with computational
analyses [12].
The asymptotic analyses provided a simplified expression
that can be used to calculate shapes of droplets supported on
thin fibers in the limit of having fiber diameters much smaller
than droplet diameters (measured perpendicular to the fibers).
The asymptotic analyses illustrate that for cos(θ) = O(1) and ε
<< 1, two spatial zones exist where droplet shapes behave dif-
ferently. Away from a fiber, a droplet is essentially spherical. As
the fiber is approached, however, deviations from spherical
symmetry can be significant.
It is also noted that for cos(θ) << 1 and ε << 1, theory sug-
gests that droplets should be nearly spherical everywhere, even
near the fiber. As a result, it seems worthwhile to seek droplet-
fiber combinations that will promote large contact angles (sub-
ject to Eqs. (24) and (25)). Finding such combinations may
allow gas-phase spherical symmetry to be more closely approa-
ched in microgravity droplet experiments that require support
fibers. Because ε increases as a droplet burns (i.e., as a droplet
reduces in size), Eqs. (24) and (25) should be applied to the
smallest droplet size of interest in an experiment.
This research has also shown that satellite droplets/bubbles
can be formed on support fibers during combustion of hepta-
ne/hexadecane droplets. This is an interesting topic that is not
well understood at present, and it would be of interest to per-
form further studies of this phenomenon. Such studies would
likely require experiments with well-characterized fiber surfa-
ces.
2
2
characterized by ρ U D , where U is a characteristic flow velo-
L
city within a droplet. Surface tension forces are characterized by
the product Dσ. The ratio of these forces yields the Weber num-
2
ber (We ) for liquid flows We = ρ U D/σ. By using data on U
L
L
L
values from microgravity droplet experiments [20] it is estima-
ted that We << 1 for the experiments discussed here indicating
L
that liquid momentum effects should not cause significant
asymmetry of a droplet about a support fiber.
A gas-phase Weber number (We ) may also be defined as the
g
ratio of the pressure change across the liquid-vapor interface
associated with momentum changes at the droplet surface (cha-
2
2
racterized by u ρ /ρ ) to the pressure change across the
s
L
g
liquid-vapor interface associated with surface tension (charact-
erized by σ/D). Here, u is the negative of the time-rate-of-
s
change of the droplet radius and ρ is the gas density at the
g
liquid-gas interface (it is assumed that ρ >> ρ ). The velocity
L
g
u is characterized as u = k/D, where k is the burning-rate con-
s
s
2
stant based on the droplet diameter (i.e. k = -d(D )/dt where t is
time). The ratio of these pressure variations yields
2
2
We =k ρ /(Dσρ ). Interestingly, this expression predicts that
g
L
g
We ∝ 1/D such that momentum changes at the liquid surface
g
may become important for small droplets. The droplets under
consideration here were large enough such that We was much
g
smaller than unity. As a result, vapor momentum effects should
not cause significant asymmetry of a droplet about a support
fiber.
Viscous stresses may also affect droplet shapes. The liquid-
phase capillary number Ca is the ratio of the characteristic
L
viscous stress μ U/D (where μ is the liquid viscosity) to the
L
L
characteristic surface tension stress (σ/D), i.e., Ca = μ U/σ.
L
L
We may also define a gas-phase capillary number Ca as the
g
ratio of gas-phase viscous stresses normal to the droplet surfa-
2
Appendix A
ce, which are characterized as μ u /D = μ ρ k/(ρ D ), to surfa-
g g
g L
g
ce tension stresses, which are characterized as σ/D, i.e., Ca =
g
The Bond number (Bo) is the ratio of gravitational forces to
capillary forces. To estimate Bo, consider a droplet with an ave-
rage diameter D (based on the droplet volume) that is supported
μ ρ k/(ρ Dσ) (μ and u are the gas-phase viscosity and velo-
g L
g
g
g
city on the gas side of the gas-liquid interface, respectively). It
is estimated that Ca << 1 and Ca << 1 for the droplets consi-
L
g
on a fiber of diameter d. The gravitational force f acting on the
dered here such that viscous effects should not cause significant
g
38
Microgravity sci. technol. XIII/4 (2002)