Abstract
The aim of this paper was to develop a model from experimental data allowing a prediction of the cardiopulmonary responses to steady-state submaximal exercise in varying gravitational environments, with acceleration in the Gz axis (a g) ranging from 0 to 3 g. To this aim, we combined data from three different experiments, carried out at Buffalo, at Stockholm and inside the Mir Station. Oxygen consumption, as expected, increased linearly with a g. In contrast, heart rate increased non-linearly with a g, whereas stroke volume decreased non-linearly: both were described by quadratic functions. Thus, the relationship between cardiac output and a g was described by a fourth power regression equation. Mean arterial pressure increased with a g non linearly, a relation that we interpolated again with a quadratic function. Thus, total peripheral resistance varied linearly with a g. These data led to predict that maximal oxygen consumption would decrease drastically as ag is increased. Maximal oxygen consumption would become equal to resting oxygen consumption when a g is around 4.5 g, thus indicating the practical impossibility for humans to stay and work on the biggest Planets of the Solar System.
| Original language | English |
|---|---|
| Pages (from-to) | 2907-2917 |
| Number of pages | 11 |
| Journal | European Journal of Applied Physiology |
| Volume | 111 |
| Issue number | 12 |
| DOIs | |
| State | Published - Dec 2011 |
Keywords
- Arterial blood pressure
- Cardiac output
- Heart rate
- Hypergravity
- Microgravity
- Oxygen consumption
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