SpaceElevatorEnvironment: Difference between revisions
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*[[TBD| The Space Elevator by Edwards, Westling]] | *[[TBD| The Space Elevator by Edwards, Westling]] | ||
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|Detailed model of ribbon / magnetic field interactions || some charging and forces are expected || Some initial work in The | |Detailed model of ribbon / magnetic field interactions || some charging and forces are expected || Some initial work in The Space Elevator by Edwards & Westling | ||
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|Detailed model of damage extent and flux due to meteors || Include the expected increase in orbital debrisover the next couple decades. || | |Detailed model of damage extent and flux due to meteors || Include the expected increase in orbital debrisover the next couple decades. || | ||
*[[Image:The_Leonids_and_the_SE.odt ]] by Edwards | *[[Image:The_Leonids_and_the_SE.odt ]] by Edwards | ||
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|Thermal modeling of the ribbon during transition between sun and shadow || || | |Thermal modeling of the ribbon during transition between sun and shadow || Initial calculations and possibly an FEA are needed || None at this time | ||
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[[SpaceElevatorWikiOverview| Return to Overview]] | [[SpaceElevatorWikiOverview| Return to Overview]] |
Revision as of 18:55, 16 July 2008
The Environment
The elevator stretches from the Earth to high orbit - passing through Earth weather, the ionosphere, radiation belts and out beyond the Earth's magnetosphere. In each of these environments there are concerns and hazards for the space elevator and a complete understanding is required to be able to produce a viable design.
Hazard | Impact | Details / Solutions |
Lightning | Severed ribbon | Solution: Anchor location in lightning-free zone |
Wind | dynamic destruction of the ribbon | Solution: Anchor location where limited wind, ribbon design |
Radiation 1 | ribbon degradation | Solution: Select CNTs and other materials for ribbon that are radiation resistant |
Radiation 2 | hazard to electronics and cargo | Solution: May be able to ascend at a higher speed and use shielding (passive and active) to get radiation to acceptable levels |
Debris | ribbon destruction | Solution: Ribbon design with a width larger than a meter insures only a small part of the ribbon will be damaged by any impact. The ribbon design also isolates damage along the length of the ribbon. Active avoidance limits impacts larger than 1 cm. |
Meteors | ribbon destruction | Same as for debris though lower flux and active avoidance can not be used. |
Earth's magnetic field | Current generation in ribbon | Ribbon is geosynchronous so only flucuations in the magnet field will create any current and this is small |
Interplanetary magnet field | Current generation | The ribbon travels quickly through the interplanetary magnetic field but the field is too weak to generate and substantial current. |
Solar wind/particles | ribbon degradation | same as radiation above |
Gravitational influence | ribbon oscillation | The Moon and sun will both exert a gravitational pull on the ribbon at a roughly 24 hour period. The natural frequency of the ribbon is about 7.2 hours and there will be little coupling |
Thermal cycling | ribbon wear and oscillation | Each day the lower end of the ribbon will go in and out of the Earth's shadow. This will change the temperature and length of the ribbon |
Atomic oxygen | ribbon destruction | Solution: Coating the affected section of the ribbon with an oxygen resistant material |
Major Work Items Required
- Experimental tests of ribbon in atomic oxygen
- Radiation protection for humans in transit
- Detailed modeling of ribbon degradation lifetime
Additional Work Needed
Item | Notes | Completed and Ongoing Efforts |
Full characterization of environmental effects | Start from "The Space Elevator" book and studies done by others | |
Detailed model of ribbon / magnetic field interactions | some charging and forces are expected | Some initial work in The Space Elevator by Edwards & Westling |
Detailed model of damage extent and flux due to meteors | Include the expected increase in orbital debrisover the next couple decades. |
|
Thermal modeling of the ribbon during transition between sun and shadow | Initial calculations and possibly an FEA are needed | None at this time |