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Gravitational stress and exercise.

This paper deals with the influence of G forces on certain circulatory and metabolic adjustments to dynamic exercise. Leg exercise in the sitting position increases systemic mean pressure both at normal and at increased G, thus improving G tolerance. When the force of gravity is increased to three times its normal value, leg exercise produces a much more marked increment in stroke volume than in heart rate, which contrasts with the case at normal gravity. Beta-adrenergic blockade, which strongly inhibits the heart rate response to gravitational stress, but leaves the systemic mean pressure and G tolerance unaffected, exaggerates the dominance of the stroke volume increase in exercise at increased G. With leg exercise at increasing work loads at 3G, the O2 uptake tends to level off and the arterial lactates to rise at a lower load than at normal gravity, indicating that the upper limit for the O2 uptake is lowered by the G force. A progressive increase of the venous admixture in the lungs suggests that the primary limitation of the O2 transport occurs in the pulmonary gas exchange.

Adrenergic beta-Antagonists↗

Thermoregulatory responses of unanesthetized rats exposed to gravitational fields of 1 to 4g.

Rats exposed to 2g environments (achieved by centrifugation) exhibit a decreased ability to maintain colonic temperature (Tco) when challenged with a 1 hr drop in ambient temperature (Ta). As an extension of this work the present study considers whether the altered ability to maintain Tco is proportional to the magnitude of the acceleration field in the range from 1g-4g, and whether the magnitude of the decreased thermoregulatory ability is related to the onset time of the temperature drop relative to that of the acceleration. Male, Sprague-Dawley rats were instrumented on the experimental day with thermistors for measuring Tco. The unanesthetized rat was then placed in a plexiglas chamber, positioned on a centrifuge 1.37 m in radius, and exposed to 1.5, 2, 2.5, 3, 3.5, or 4g for 5-7 hrs. The exposure to reduced temperature (Ta = approximately 7 degrees C) for 1 hr began 3 hrs after initiation of centrifugation. These experiments indicated that the magnitude of the cold-induced drop in Tco was linearly related to the acceleration field. The effect of a specific stressor (cold) on the thermoregulatory system is therefore a direct function of the gravitational field.

Acceleration↗

Endothelial stress by gravitational unloading: effects on cell growth and cytoskeletal organization.

All organisms on Earth have evolved to survive within the pull of gravity. Orbital space flights have clearly demonstrated that the absence or the reduction of gravity profoundly affects eukaryotic organisms, including man. Because (i). endothelial cells are crucial in the maintenance of the functional integrity of the vascular wall, and (ii). cardiovascular deconditioning has been described in astronauts, we evaluated whether microgravity affected endothelial functions. We show that microgravity reversibly stimulated endothelial cell growth. This effect correlated with an overexpression of heat shock protein 70 (hsp70) and a down-regulation of interleukin 1 alpha (IL-1alpha), a potent inhibitor of endothelial cell growth, also implicated in promoting senescence. In addition, gravitationally unloaded endothelial cells rapidly remodelled their cytoskeleton and, after a few days, markedly down-regulated actin through a transcriptional mechanism. We hypothesize that the reduction in the amounts of actin in response to microgravity represents an adaptative mechanism to avoid the accumulation of redundant actin fibers.

Actins↗

Observation and modelling of clamshell droplets on vertical fibres subjected to gravitational and drag forces.

Extensive experimental investigation of the wetting processes of fibre-liquid systems during air filtration (when drag and gravitational forces are acting) has shown many important features, including droplet extension, oscillatory motion, and detachment of drops from fibres as airflow velocity increases, and also movement or flow of droplets along fibres. A detailed experimental study of the processes was conducted using stainless steel filter fibres and H2O aerosol, which coalesce on the fibre to form clamshell droplets. The droplets were predominantly observed in the Reynolds transition flow region, since this is the region where most of the above features occur. The droplet oscillation is believed to be induced by the onset of the transition from laminar to turbulent flow as the increasing droplet size increases Reynolds number for the flow around the droplet. Two-dimensional flow in this region is usually modelled using the classical Karman vortex street, however there exist no 3D equivalents. Therefore to model such oscillation it was necessary to create a new conceptual model to account for the forces both inducing and preventing such oscillation. The agreement between the model and experimental results is very good for both the radial and transverse oscillations.

Journal Article↗

Observation and modelling of barrel droplets on vertical fibres subjected to gravitational and drag forces.

Extensive experimental investigation of the wetting processes of fibre/liquid systems during air filtration (when drag and gravitational forces are acting) has shown many important features, including droplet extension, oscillatory motion, and detachment or flow of drops from fibres as airflow velocity increases. A detailed experimental study of the aforementioned processes was conducted using glass filter fibres and H(2)O aerosol, which coalesce on the fibre to form barrel droplets with small contact angles. The droplets were predominantly observed in the Reynolds transition (or unsteady laminar) flow region. The droplet oscillation appears to be induced by the onset of vortexes in the flow field around the droplet as the increasing droplet size increases the Reynolds number. Flow in this region is usually modelled using the classical two-dimensional Karman vortex street, and there exist no 3D equivalents. Therefore to model such oscillation it was necessary to create a new conceptual model to account for the forces both inducing and inhibiting such oscillation. The agreement between the model and experimental results is acceptable for both the radial and transverse oscillations.

Journal Article↗

Continuous split-flow thin cell and gravitational field-flow fractionation of wheat starch particles.

The combined employment of the SPLITT (split-flow thin) cell--a relatively new system for fast, continuous binary separation--and of gravitational field-flow fractionation (GrFFF)--a fractionation technique suitable for micron particle size distribution determination--was investigated for starch separation and characterization. Emphasis is placed on the main advantages of both techniques: operating under gentle earth gravity field, low cost and ease of maintenance. The reproducibility of GrFFF is demonstrated. Both the SPLITT separation and GrFFF fractionation results were checked by optical microscopy. Application examples of typical starch fractionation experiments are reported and discussed.

Chemical Fractionation↗

Adaptation of the macular vestibuloocular reflex to altered gravitational conditions in a fish (Oreochromis mossambicus).

Young fish (Oreochromis mossambicus) were exposed to microgravity (micro g) for 9 to 10 days, or to hypergravity (hg) for 9 days. For several weeks after termination of micro g and hg, the roll-induced static vestibuloocular reflex (rVOR) was recorded. In stage 11/12-fish, the rVOR amplitude (angle between the maximal up and down movement of an eye during a complete 360 degree lateral roll) of micro g-animals increased significantly by 25% compared to 1 g-controls during the first post-flight week but decreased to the control level during the second post-flight week. Microgravity had no effect in stage 14/16 fish on the rVOR amplitude. After 3 g-exposure, the rVOR amplitude was significantly reduced for both groups compared to their 1 g-controls. Readaptation to 1 g-condition was completed during the second post-3 g week. We postulate a critical period during which the development of the macular vestibuloocular reflex depends on gravitational input, and which is limited by the first appearance of the rVOR. At this period of early development, exposure to microgravity sensitizes the vestibular system while hypergravity desensitizes it.

Adaptation, Physiological↗

Gravitational unloading effects on muscle fiber size, phenotype and myonuclear number.

The effects of gravitational unloading with or without intact neural activity and/or tension development on myosin heavy chain (MHC) composition, cross-sectional area (CSA), number of myonuclei, and myonuclear domain (cytoplasmic volume per myonucleus ratio) in single fibers of both slow and fast muscles of rat hindlimbs are reviewed briefly. The atrophic response to unloading is generally graded as follows: slow extensors > fast extensors > fast flexors. Reduction of CSA is usually greater in the most predominant fiber type of that muscle. The percentage of fibers expressing fast MHC isoforms increases in unloaded slow but not fast muscles. Myonuclear number per mm of fiber length and myonuclear domain is decreased in the fibers of the unloaded predominantly slow soleus muscle, but not in the predominantly fast plantaris. Decreases in myonuclear number and domain, however, are observed in plantaris fibers when tenotomy, denervation, or both are combined with hindlimb unloading. All of these results are consistent with the view that a major factor for fiber atrophy is an inhibition or reduction of loading of the hindlimbs. These data also indicate that predominantly slow muscles are more responsive to unloading than predominantly fast muscles.

Animals↗

Response of renal sympathetic nerve activity to parabolic flight-induced gravitational change in conscious rats.

The renal sympathetic nerve activity (RNA) response to gravitational changes induced by parabolic flight was examined in chronically instrumented conscious rats. Two types of RNA responses were found. In six out of 12 rats, the RNA did not respond during the 2 G period, but immediately fell to background levels on entry into microgravity (microG), then recovered to the 1 G control level during continued microG (shutdown obvious group). In the other six rats, the RNA increased to 158+/-13% at the end of the 2 G period, increased further to 195+/-22% on entry into microG, then gradually recovered to that seen at 1 G (shutdown obscure group). The mean arterial pressure in the shutdown obvious group was significantly higher and the heart rate tended to be higher than in the shutdown obscure group, suggesting that the baseline sympathetic tone in the shutdown obvious group was higher than in the shutdown obscure group. These results suggest that the RNA response to parabolic flight might be affected by the baseline sympathetic tone.

Animals↗

Micropreparation of hemopoietic stem cells from the mouse bone marrow suspension by gravitational field-flow fractionation.

Gravitational field-flow fractionation is a relatively simple experimental technique. This method was used for the characterization of stem cells from mouse bone marrow. Because these cells are bigger than the other cells in bone marrow, it is possible to separate them from the mixture. The fractions collected after passing through the separation channel were characterized using a Coulter Counter and used for transplantation into irradiated mice.

Animals↗

Orthostatic intolerance: different abnormalities in the neural sympathetic response to a gravitational stimulus.

In this paper we shall focus on the different abnormalities in the neural sympathetic response to a gravitational stimulus, characterising syndromes with symptoms of orthostatic intolerance. In Vaso vagal Syncope, an increase or a reduction of cardiac and vascular sympathetic modulation have been described in occasional and habitual fainters, respectively. Pure Autonomic Failure (PAF) is characterized by a global cardiovascular denervation. Accordingly, the spectral markers of cardiac and vascular sympathetic modulation are absent or reduced. However, a concomitant vagal diminished activity is present. In Chronic Orthostatic Intolerance (COI), the most common form of dysautonomia in young female, an abnormal regional distribution of sympathetic discharge has been hypothesized during standing. Indeed, an overall increased sympathetic activity is present in recumbent position; during tilt a blunted vascular sympathetic discharge, with a concomitant exaggerated cardiac sympathetic modulation, is evident. Baroreflex Failure is a syndrome that may result from neck surgery or irradiation due to different forms of regional cancer. It is characterized by a volatility of blood pressure and heart rate, without habitual orthostatic hypotension. In the present paper, we describe a case of Baroreflex Failure with marked orthostatic hypotension in spite of a huge muscle sympathetic nerve activity (MSNA) and high levels of plasma cathecolamines. The most relevant finding was the absence of any coordinate rythmicity in blood pressure, heart rate and MSNA, both at rest and during tilt, particularly in the frequency band likely to be related with sympathetic modulation, i.e. at 0.1 Hz. We hypothesize that the absence of 0.1 Hz spontaneous fluctuations might play a role in sustaining orthostatic hypotension.

Gravity Sensing↗

0957 + 561 A, B: twin quasistellar objects or gravitational lens?

0957 + 561 A, B are two QSOs of mag 17 with 5.7 arc s separation at redshift 1.405. Their spectra leave little doubt that they are associated. Difficulties arise in describing them as two distinct objects and the possibility that they are two images of the same object formed by a gravitational lens is discussed.

Journal Article↗

An effective gravitational temperature for sedimentation.

The slow sedimentation of suspensions of solid particles in a fluid results in complex phenomena that are poorly understood. For a low volume fraction (phi) of particles, long-range hydrodynamic interactions result in surprising spatial correlations in the velocity fluctuations; these are reminiscent of turbulence, even though the Reynolds number is very low. At higher values of phi, the behaviour of sedimentation remains unclear; the upward back-flow of fluid becomes increasingly important, while collisions and crowding further complicate inter-particle interactions. Concepts from equilibrium statistical mechanics could in principle be used to describe the fluctuations and thereby provide a unified picture of sedimentation, but one essential ingredient--an effective temperature that provides a mechanism for thermalization--is missing. Here we show that the gravitational energy of fluctuations in particle number can act as an effective temperature. Moreover, we demonstrate that the high-phi behaviour is in fact identical to that at low phi, provided that the suspension viscosity and sedimentation velocity are scaled appropriately, and that the effects of particle packing are included.

Journal Article↗

Gravitational microlensing by low-mass objects in the globular cluster M22.

Gravitational microlensing offers a means of determining directly the masses of objects ranging from planets to stars, provided that the distances and motions of the lenses and sources can be determined. A globular cluster observed against the dense stellar field of the Galactic bulge presents ideal conditions for such observations because the probability of lensing is high and the distances and kinematics of the lenses and sources are well constrained. The abundance of low-mass objects in a globular cluster is of particular interest, because it may be representative of the very early stages of star formation in the Universe, and therefore indicative of the amount of dark baryonic matter in such clusters. Here we report a microlensing event associated with the globular cluster M22. We determine the mass of the lens to be 0.13(+0.03)(-0.02) solar masses. We have also detected six events that are unresolved in time. If these are also microlensing events, they imply that a non-negligible fraction of the cluster mass resides in the form of free-floating planetary-mass objects.

Journal Article↗

Magnification of light from many distant quasars by gravitational lenses.

Exceptionally bright quasars with redshifts up to z = 6.28 have recently been discovered. Quasars are thought to be powered by the accretion of gas onto supermassive black holes at the centres of galaxies. Their maximum (Eddington) luminosity depends on the mass of the black hole, and the brighter quasars are inferred to have black holes with masses of more than a few billion solar masses. The existence of such massive black holes poses a challenge to models for the formation of structures in the early Universe, as it requires their formation within one billion years of the Big Bang. Here we show that up to one-third of known quasars with z approximately equal to 6 will have had their observed flux magnified by a factor of ten or more, as a consequence of gravitational lensing by galaxies along the line of sight. The inferred abundance of quasar host galaxies, as well as the luminosity density provided by the quasars, has therefore been substantially overestimated.

Journal Article↗

The central image of a gravitationally lensed quasar.

A galaxy can act as a gravitational lens, producing multiple images of a background object. Theory predicts that there should be an odd number of images produced by the lens, but hitherto almost all lensed objects have two or four images. The missing 'central' images, which should be faint and appear near the centre of the lensing galaxy, have long been sought as probes of galactic cores too distant to resolve with ordinary observations. There are five candidates for central images, but in one case the third image is not necessarily the central one, and in the others the putative central images might be foreground sources. Here we report a secure identification of a central image, based on radio observations of one of the candidates. Lens models using the central image reveal that the massive black hole at the centre of the lensing galaxy has a mass of <2 x 10(8) solar masses (M(o)), and the galaxy's surface density at the location of the central image is > 20,000M(o) pc(-2), which is in agreement with expections based on observations of galaxies that are much closer to the Earth.

Journal Article↗

Neptune's capture of its moon Triton in a binary-planet gravitational encounter.

Triton is Neptune's principal satellite and is by far the largest retrograde satellite in the Solar System (its mass is approximately 40 per cent greater than that of Pluto). Its inclined and circular orbit lies between a group of small inner prograde satellites and a number of exterior irregular satellites with both prograde and retrograde orbits. This unusual configuration has led to the belief that Triton originally orbited the Sun before being captured in orbit around Neptune. Existing models for its capture, however, all have significant bottlenecks that make their effectiveness doubtful. Here we report that a three-body gravitational encounter between a binary system (of approximately 10(3)-kilometre-sized bodies) and Neptune is a far more likely explanation for Triton's capture. Our model predicts that Triton was once a member of a binary with a range of plausible characteristics, including ones similar to the Pluto-Charon pair.

Journal Article↗