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| *1 Humans evolved to run, hence may be optimized for > 1 gee | .'''(1)''' Humans evolved to run, hence may be optimized for > 1 gee | 
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| *2 The human vestibular system can adapt to high RPMS | .'''(2)''' The human vestibular system can adapt to high RPMS | 
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| *1 Test the Vernikos theory: do healthy humans do '''better''' in > 1 gee environments? *2 Learn about long term vestibular adaption, and the transition from rotation to non-rotation | *'''(1)''' Test the Vernikos theory: do healthy humans do '''better''' in > 1 gee environments? *'''(2)''' Learn about long term vestibular adaption, and the transition from rotation to non-rotation | 
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| *3 Select astronauts for vestibular tolerance for rotating habitats in microgravity *4 Make low BMI people into heros | *'''(3)''' Select astronauts for vestibular tolerance for rotating habitats in microgravity *'''(4)''' Make low BMI people into heros | 
Gee Plus
Adapting to a High RPM Environment
The Experiment
A 9 meter radius, rotating long-duration space habitat simulation on Earth, simulating 1.4 gees at 10 RPM. 1.4 gees is the vector sum of 1 gee horizontal and 1 gee vertical. Experimental subjects with BMI < 20, having a "gravitational BMI" < 28 but the same "metabolic BMI".
Postulates
- (1) Humans evolved to run, hence may be optimized for > 1 gee - see work by Joan Vernikos, NASA Ames (retired)
- zero gee causes rapid "aging"
 
- (2) The human vestibular system can adapt to high RPMS - Experiments with rotating rooms show 6 RPM adaptation in 3 days, 10 RPM in 5 days
- Experiments with rotating tube beds suggest 30 RPM ( ! ) adaptation for head movements
- Athletes undergo much faster head rotations
 
Goals
- (1) Test the Vernikos theory: do healthy humans do better in > 1 gee environments? 
- (2) Learn about long term vestibular adaption, and the transition from rotation to non-rotation - frequent transitions through the hub to 1 gee and 0 RPM
 
- (3) Select astronauts for vestibular tolerance for rotating habitats in microgravity 
- (4) Make low BMI people into heros 
Math
a = 9.81 \times gee ~=~ \omega^2 R ~=~ { \Large \left( { 2 \pi } \over T \right) }^2 R ~=~ 4 \pi^2 { \Large { R \over T^2 } } ~~~ T in seconds
gee \times T^2 \approx 4 R ~~~~~ T ~=~ 60 / RPM
R ~=~ { \Large \left( 30 \over RPM \right)}^2 gee
