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First published online August 22, 2008
Journal of Experimental Biology 211, 2767-2772 (2008)
Published by The Company of Biologists 2008
doi: 10.1242/jeb.020073
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The effects of gravity on human walking: a new test of the dynamic similarity hypothesis using a predictive model
Department of Anthropology, University of Arizona, 1009 E. South Campus Drive, Tucson, AZ 85721, USA
e-mail: raichlen{at}email.arizona.edu
Accepted 26 June 2008
| Summary |
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Key words: stride length, Froude number, force-driven harmonic oscillator, inertial properties
| INTRODUCTION |
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Alexander noted that dynamic similarity is only possible, and therefore
only testable, when two animals have equal ratios of the inertial and
gravitational forces governing locomotion
(Alexander, 1976
; see also
Alexander and Jayes, 1983
). For
terrestrial locomotion, the inertial force is generally assumed to be the
centripetal force that acts on an animal as it vaults over its stance leg,
which acts as an inverted pendulum (see
Donelan and Kram, 1997
).
Therefore, the ratios of inertial to gravitational forces in two animals are
equal when they walk at the same Froude number [velocity2/(gravity
x hip height)]. Although many researchers rely on the DSH in studies of
comparative biomechanics, recent work has questioned its validity (see
Donelan and Kram, 1997
;
Donelan and Kram, 2000
). The
purpose of the present study is to test the DSH using a predictive kinematic
model to assess its utility in understanding human locomotion.
Most tests of dynamic similarity examine the impacts of changes in inertial
forces on dynamic similarity (e.g. through differences in limb length in
comparative studies) (see Alexander and
Jayes, 1983
; Alexander and
Maloiy, 1984
; Gatesy and
Biewener, 1991
; Bullimore and
Burn, 2006
). The DSH has been broadly supported by studies showing
that animals that differ in size generally use equal relative stride lengths
(stride length divided by hip height) when walking at the same Froude numbers
and they transition from a walk to a run at equal Froude numbers
(Alexander and Jayes, 1983
).
Donelan and Kram, noting the importance of gravity in the DSH, suggested that
dynamic similarity should account for locomotor differences not only due to
size but also due to changes in gravitational environments
(Donelan and Kram, 1997
). Thus,
as gravitational forces change, individuals walking at the same Froude numbers
should continue using equal relative stride lengths and should transition from
a walk to a run at the same Froude numbers.
In an innovative test of the effects of gravity on the DSH in humans,
Donelan and Kram used a treadmill that alters the effects of gravity on
locomotion by introducing an adjustable upward force on the body through a
harness system attached to the torso
(Donelan and Kram, 1997
;
Donelan and Kram 2000
; see also
Kram et al., 1997
). Results
from these earlier studies showed that humans deviated from dynamic similarity
as gravity was reduced. As gravity decreased, humans walked with relatively
shorter strides (Donelan and Kram,
1997
), and the walk–run transition occured at higher Froude
numbers in very low gravitational fields
(Kram et al., 1997
). Thus, the
DSH may not be a governing principle of animal locomotion and should be used
with caution (Donelan and Kram,
2000
).
Gravity and swing phase
One critique of these studies, fully acknowledged by the authors, is that
their novel experimental design did not alter the gravitational environment
for the limbs during swing phase (Donelan
and Kram, 1997
; Donelan and
Kram, 2000
). Gravity should have an important effect on swing
phase, and possibly on overall stride kinematics, because limbs act somewhat
like suspended pendula (see Hildebrand,
1985
). Therefore, the duration of swing phase is related to limb
mass distribution and gravity, and the natural period of the limb (T)
is:
![]() | (1) |
![]() | (2) |
In Eqn 2, I is the limb's mass moment of inertia about the hip joint (kg m–2), m is the limb's mass (kg) and L is the distance of the limb's center of mass from the hip joint (m). If all else is equal, a relatively long swing period (due to either a relatively large d or to reduced g) will lead to a relatively long stride period (the sum of swing and stance durations) and a relatively low stride frequency (the reciprocal of stride duration). Since velocity (v) is equal to the product of stride length and stride frequency, low stride frequencies lead to long strides at a given speed.
Both comparative and experimental studies support these connections between
pendular limb swing and stride lengths and stride frequencies
(Inman et al., 1981
;
Martin, 1985
;
Holt et al., 1990
;
Skinner and Barrack, 1990
;
Steudel, 1990
;
Mattes et al., 2000
;
Raichlen, 2004
;
Raichlen, 2005
;
Raichlen, 2006
). For example,
when weights were affixed to the ankles of dogs and humans, leading to a large
d and, therefore, a longer natural swing period, stride lengths
increased and stride frequencies decreased
(Inman et al., 1981
;
Martin, 1985
;
Holt et al., 1990
;
Skinner and Barrack, 1990
;
Steudel, 1990
;
Mattes et al., 2000
).
Comparative studies of natural variation in limb mass distribution also
support the links between limb swing and overall stride kinematics
(Preuschoft and Gunther, 1994
;
Raichlen, 2004
;
Raichlen, 2005
;
Raichlen, 2006
). Animals with
large values of d due to heavy muscles in the hands and feet (such as
primates with grasping extremities) use relatively longer strides and lower
stride frequencies than animals with more proximally concentrated limb mass
(Raichlen, 2004
;
Raichlen, 2005
;
Raichlen, 2006
).
It is important to note that gravity can still play a role in determining
limb swing even if the limbs do not swing as completely passive pendula. Holt
and colleagues introduced a model that predicts kinematics at preferred
walking speeds by assuming that the limb acts like a force-driven harmonic
oscillator (FDHO) during swing phase, accounting for not only gravitational
forces but also for some muscle action during swing
(Holt et al., 1990
). This
model considers the limb to be a mostly passive pendulum but does include a
constant to account for the damping effects of muscles and tendons and
provides a driving force. The FDHO successfully predicts stride frequencies
and stride lengths at preferred walking speeds under a variety of conditions
including forwards and backwards walking
(Holt et al., 1990
;
Schot and Decker, 1998
) and
walking with ankle weights (Holt et al.,
1990
). Thus, experimental studies, comparative biomechanics and
biomechanical models support the hypothesis that the limbs swing as suspended
pendula assisted by some degree of muscular action and under the influence of
gravity.
The present study examines the effects of gravity on dynamic similarity
using a very simple kinematic model that links limb mass distribution and
swing kinematics to overall locomotor kinematics as a function of speed and
gravitational forces. The model presented here expands on the FDHO to predict
stride lengths over a range of speeds and explicitly predicts the
walk–run transition speed. The model will therefore examine the
parameters that deviated from dynamic similarity in previous reduced gravity
experiments (Donelan and Kram,
1997
; Kram et al.,
1997
). I use the model presented here to test the hypothesis that
humans do in fact walk with dynamic similarity in reduced gravity once the
effects of altered gravity on limb swing are considered. Additionally, since
previous studies have altered gravitational forces for the upper body but not
the limbs (Donelan and Kram,
1997
; Kram et al.,
1997
; Donelan and Kram,
2000
), the model is used to examine the kinematic effects of
altering gravitational acceleration on the body alone in order to compare
model predictions against previous treadmill studies.
| MATERIALS AND METHODS |
|---|
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Model development
Based on the assumption that the limbs swing as FDHOs, the period of the
limb is calculated following Turvey et al.
(Turvey et al., 1988
; see also
Holt et al., 1990
) as:
![]() | (3) |
![]() | (4) |
![]() | (5) |
Stance duration (tst) is calculated by first assuming
that step length (Lst; distance traveled during stance
phase) does not change with speed and is equal to:
![]() | (6) |
![]() | (7) |
![]() | (8) |
![]() | (9) |
![]() | (10) |
![]() | (11) |
![]() | (12) |
Altering gravitational fields
If the dynamic similarity hypothesis is correct, when gravitational
acceleration is altered in the model, predicted relative stride lengths should
be equal at the same Froude numbers. In order to predict the effects of
altered gravity on kinematics and test for dynamic similarity, model
parameters are first converted into dimensionless numbers. Thus, a given
velocity is converted into a Froude number (Fr) (dimensionless
velocity):
![]() | (13) |
![]() | (14) |
From Eqn 15, it is clear that gravity plays a major role in determining dSLs at a given speed in two ways (denoted by the curved braces above): (a) by changing the calculation of swing duration, and (b) by changing calculation of velocity from Froude numbers. To predict the effects of reduced gravitational forces on locomotion, the gravitational acceleration constant, g, is changed to some fraction of earth's gravitational acceleration; if gravitational forces influence both the limbs and the body, g is changed in both places in the equation (i.e. a and b in Eqn 15). Altering gravitational forces in the velocity calculations alone (b in Eqn 15) will model the limbs swinging in earth's gravity, while the rest of the body experiences a different gravitational field.
|
Testing the model: sample
To test the model, stride lengths were predicted for a sample of humans and
were measured during treadmill walking. A sample of 11 individuals (five
males, six females; see Table
1) volunteered to participate in this project. All subjects gave
informed consent and all procedures were approved by the University of Arizona
Human Subjects Committee. Each subject performed a series of treadmill walking
trials at three speeds (1.0, 1.5 and 2.0 m s–1).
Pressure-sensitive footswitches were attached to the underside of their feet
at the heel and hallux (Delsys, Inc., Boston, MA, USA) to determine the time
of touch-down and toe-off. Stride duration was calculated as the time elapsed
between two successive touch-downs of the same foot. Using treadmill velocity,
stride lengths were calculated as the product of velocity and stride duration.
Limb inertial properties were calculated from limb length and body mass after
Winter (Winter, 1990
).
|
Hypothesis testing
The effects of reduced gravity on walking were predicted by changing the
gravitational acceleration constant in the model. Two cases were modeled: (1)
changing the gravitational acceleration constant for both the limbs and the
body (i.e. a and b in Eqn 15)
and (2) changing the gravitational acceleration constant for the body only
(i.e. b in Eqn 15). The effects
of gravity were modeled in subjects over a range of Froude numbers
(Fr=0.1, 0.2, 0.3, 0.4) at four different gravitational accelerations
(% of earth's g=100, 75, 50, 25). Model predictions were
compared to previous studies in which gravity was altered for the entire body
including the legs (Newman,
1996
) and for the upper body only
(Donelan and Kram, 1997
;
Kram et al., 1997
).
| RESULTS |
|---|
|
|
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|
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|
Finally, the model predicts that the human walk–run transition should
occur at the same Froude number (Fr=0.58) regardless of gravitational
environment (Fig. 4). These
predicted values are slightly higher than the mean walk–run transition
Froude number found in most experimental studies (Fr
0.50) but
are within the range of variation in these studies [range=0.37–0.66
(Gatesy and Biewener, 1991
;
Hreljac, 1995
; Diedrich and
Warren, 1995; Kram et al.,
1997
; Rubenson et al.,
2004
)]. In treadmill experiments (where gravity was reduced for
the upper body only), Kram and colleagues
(Kram et al., 1997
) showed
that, as gravity was reduced to very low levels, the walk–run transition
occurred at higher Froude numbers (see Fig.
4). When gravitational acceleration is altered in the model for
the upper body only, a similar pattern emerges. In this case, the model
predicts that humans will transition to a run at higher Froude numbers as the
gravitational acceleration constant is reduced.
|
| DISCUSSION |
|---|
|
|
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Model
Simplifying assumptions were made to allow for a clear examination of the
effects of reduced gravity on human stride lengths. For example, step length
is assumed to be constant over all walking speeds, although experimental data
show that human step lengths do change slightly with walking speed (e.g.
Kuo, 2001
). Additionally,
while the FDHO model takes individual variation in limb mass distribution into
account, it does not account for possible variation in muscle and tendon
stiffness. For example, Obusek et al. suggested that there is some individual
variation in the stiffness of the muscle–tendon units that will alter
the duration of swing period (Obusek et
al., 1995
). Despite these assumptions, comparisons of the model
with experimental data support its use in investigations of the effects of
gravity on locomotion. The model predicts stride lengths very well in a sample
of humans walking in normal gravity and predicted that changes in stride
lengths match those from experimental studies when the effects of
gravitational forces are altered for the body only.
It is possible that changes in step length with velocity could impact predicted step lengths in reduced gravity. However, the model results agree with stride length data from parabolic flight experiments of locomotion in reduced gravity. These experiments must be considered the `gold standard' since alterations in gravity are real and felt by all body parts. The model matches data from these experiments better than treadmill studies. Thus, the close correspondence between model predictions and experimental results from parabolic flights further supports use of this model to examine the effects of gravity on locomotion.
Gravity and the DSH
This model supports the prediction that humans will walk with dynamic
similarity in different gravitational environments. As gravity is altered,
dimensionless stride lengths are identical at equal Froude numbers. Dynamic
similarity should occur only when the ratio of inertial to gravitational
forces governing locomotion are equal. When gravity is reduced, equivalent
Froude numbers are only possible at lower absolute velocities. If gravity
influences stance phase only, then we should expect reduced stride lengths in
lower gravitational fields because absolute velocity will be slower at the
same Froude number. However, reduced gravity also increases the period of limb
swing, which leads to longer stride durations and longer stride lengths. The
model suggests that, as gravity is reduced, the increase in swing duration
offsets the reduction in velocity at a given Froude number such that stride
lengths remain constant.
The model predictions also support previous analyses of locomotion on other
planets. The model predicts that the walk–run transition will occur at
equal Froude numbers as gravity is altered. Thus, as predicted by Minetti, the
walk–run transition velocity will decrease as gravity is reduced
(Minetti, 2001
). This finding
explains why Apollo astronauts reported difficulty walking on the lunar
surface and instead preferred running and jumping
(Minetti, 2001
). Confirmation
of these results can improve our understanding of how locomotion will be
constrained in future manned missions to the moon or Mars. For example, it may
be possible to walk more easily on Mars than on the moon since larger
gravitational forces on Mars would allow humans to transition to a run at a
higher velocity.
Conclusions
A simple model, based on few assumptions, was able to predict stride
lengths in earth's gravity for a sample of individuals and successfully
predicted the effects of reduced gravity on human locomotion. The DSH is well
supported by the model, and its use remains a valid way to account for the
effects of gravity on locomotion. Movement in reduced gravity will clearly
affect both swing and stance phase, and analyses of swing-phase or
whole-stride kinematics may require either true-reduced gravity experiments
(e.g. parabolic flights) or the use of predictive locomotor models. These
types of kinematic data may be essential for planning the next generation of
space exploration. Models, properly validated by parabolic flight experiments,
may be the best way to gather necessary data for how locomotion will change
when walking on other planets.
LIST OF SYMBOLS AND ABBREVIATIONS
| Acknowledgments |
|---|
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