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An engineering approach to miogravity syndrome
Abstract
The human species is rapidly expanding. Barring global catastrophe and unnatural constraints, it will, in a brief time on the scale of natural history, fill the uttermost reaches of the solar system. The beachhead established by President Kennedy's lunar program will lead to lunar, Martian and free space settlements in the next century. In a single generation of those who call them home, the constant 9.81 m.s-2 pull of Earth's gravity, which has influenced the evolution and development of terrestrial life forms for billions of years, will fade from common experience. Miogravity syndrome, a prognosticated complex arising in reduced gravity environments such as the surfaces of the Moon and Mars and principally encompassing muscle atrophy, cardiovascular deconditioning and bone demineralization, stands to replace physics and rocketry as the fundamental challenge of interplanetary astronautics. Mirroring our past few million years of changing climate and resources, the mobility of humans between diverse gravitational environments on the high frontier will critically depend on our ability to adapt. Tomorrow, as ever, a mushrooming penchant for toolmaking will spearhead the human career.
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The human exploration of space occasions travel, work and residence in environments having different coefficients of gravity. Increasing attention has been given over its history to the adverse physiological effects of prolonged exposure to reduced or zero gravity. Muscle atrophy and bone demineralisation are the foremost cumulative symptoms, the latter of which is believed to be irreversible under present medical technology. Rotating space stations and spacecraft can simulate gravity in orbit or during inertial transit but this provision for reduced gravity environments such as exist on Luna, Mars and the outer moons has not been adequately addressed. This paper describes a class of centrifugal habitats for reduced gravity environments which promise to provide incremental levels of simulated gravity in accommodations which are comfortable, spacious and readily accessible to outposts and colonies on planetary surfaces. The members of this class share a common geometric basis but exhibit infinite variety both in scale and in the details of their implementation.
Hindlimb suspension (HS) is a ground-based simulation model for spaceflight commonly used to study the effects of unloading on skeletal muscle. The purpose of the present study was to determine the effects of a daily short-duration, high-load exercise training program in ameliorating the atrophic response and associated adaptations in the mechanical properties of the soleus (SOL) and medial gastrocnemius (MG) muscles to HS. Male Sprague-Dawley rats (mean body weight, approximately 250 g) were assigned randomly to one of three groups: control (CON, n = 7), HS, (n = 7), and HS plus exercise (HS-EX, n = 8). The exercise consisted of rats climbing up a 1-m grid inclined at approximately 85 degrees for eight repetitions with a load equal to 75% body weight attached to their tails repeated four times daily during their active period. Following 7 days, soleus wet weights in the HS and HS-EX rats were 42 and 23% lower than those in the CON rats. The SOL muscle weight to body weight ratio in the HS group was 32% smaller than that in the CON group, whereas it was similar to that of CON in the HS-EX. Maximum tetanic tensions in the HS and HS-EX groups were 44 and 27% less than that in CON, with that in HS-EX being significantly greater than that in HS.(ABSTRACT TRUNCATED AT 250 WORDS)
The manned exploration of the solar system and the surfaces of some of the smaller planets and larger satellites requires that we are able to keep the adverse human physiological response to long term exposure to near zero and greatly reduced gravity environments within acceptable limits consistent with metabolic function. This paper examines the physiological changes associated with microgravity conditions with particular reference to the weightless demineralizatoin of bone (WDB). It is suggested that many of these changes are the result of physical/mechanical processes and are not primarily a medical problem. There are thus two immediately obvious and workable, if relatively costly, solutions to the problem of weightlessness. The provision of a near 1 g field during prolonged space flights, and/or the development of rapid transit spacecraft capable of significant acceleration and short flight times. Although these developments could remove or greatly ameliorate the effects of weightlessness during long-distance space flights there remains a problem relating to the long term colonization of the surfaces of Mars, the Moon, and other small solar system bodies. It is not yet known whether or not there is a critical threshold value of 'g' below which viable human physiological function cannot be sustained. If such a threshold exists permanent colonization may only be possible if the threshold value of 'g' is less than that at the surface of the planet on which we wish to settle.
It is generally agreed that the single factor that most limits human survivability in non-Earth environments is the phenomenon of bone demineralization and the medical problems induced by the subsequent imbalance in the calcium metabolism. Alterations of skeletal properties occur as a result of disturbances in the normal mechanical loading environment of bone. These alterations or "adaptations" obey physical laws, but the precise mathematical relationships remain to be determined. Principles governing unloading and overloading of bone are gaining more attention as a consequence of the planning of manned space stations, moon and Mars bases and spaceflights of long duration. This paper reviews the subject of bone remodeling and presents a mathematical framework which allows for the prediction of skeletal adaptation on Earth and in non-Earth gravity environments by power law relationships.
With the prospect of long duration space missions in Earth orbit or to Mars, there is a need for adequate information on the physiological adaptations that will occur. One consequence of prolonged exposure to microgravity is muscle atrophy (loss of muscle mass). After a long duration space flight, muscle atrophy along with skeletal calcium loss would affect the capacity of astronauts to re-adapt to gravity on return to Earth. Of importance are any countermeasures which can attenuate the adaptive responses to microgravity. Experimentation is difficult in space with small subject numbers and mission constraints. Prolonged bed rest using healthy volunteers is used as an Earth-based model to simulate the muscle atrophy which occurs in the microgravity environment.