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- 1. Orbital Space Settlements and a Solar System Wide Web Sourabh kaushal Humanity could be life's ticket to the stars (The dinosaurs weren’t space-faring) www.engineerkaushal.webnode.com
- 6. People Live Everywhere Every continent, including Antarctica Hottest, driest deserts Coldest, iciest regions Wettest rain forests On water For short periods, in orbit 6,000,000,000 people on Earth www.engineerkaushal.webnode.com
- 7. Life is Everywhere On nearly all land areas In nearly all waters In the rocks under the Earth In near-boiling water In ice On desert rocks On a spacecraft on the Moon www.engineerkaushal.webnode.com
- 9. Orbital Space Settlement Who? Ordinary people. What? Artificial ecosystems inside gigantic rotating, pressurized spacecraft. Where? In orbit; near Earth at first. How? With great difficulty. Why? To grow. When? Decades. How much will it cost?If you have to ask, you can't afford it. www.engineerkaushal.webnode.com
- 10. Who Today: highly trained astronauts. $20-40 million tourist trip to Mir Survivor in Space Tomorrow: everyone who wants to go. 100 - 10,000,000 people per colony Ultimately, thousands or even millions of colonies Sounds unrealistic? A hundred years ago nobody had ever flown in an airplane. Today ~ 500 million person/flights per year. www.engineerkaushal.webnode.com
- 11. What A space settlement is a home in orbit, not just a place to work. Live on the inside of air-tight, kilometer scale, rotating spacecraft. www.engineerkaushal.webnode.com
- 12. Where In orbit, not on a planet or moon. Moon (1/6g) and Mars (3/8g) gravity too low. Children will not have the bones and muscles needed to visit Earth. Orbital colonies rotate for 1g. Continuous solar energy. Large-scale construction easier. Much closer: hours not days or months. www.engineerkaushal.webnode.com
- 13. How Materials Moon Oxygen, silicon, metals, some hydrogen for water. Near-Earth Asteroids Wide variety of materials including water, carbon, metals, and silicon. Radiation protection Life support: Biosphere II scientific failure, engineering success! Transportation critical and difficult. www.engineerkaushal.webnode.com
- 14. Why Growth = survival. Largest asteroid converted to space settlements can produce living area ~500 times the surface area of the Earth. 3D object to 2D shells Uncrowded homes for trillions of people. Newland. Nice place to live. www.engineerkaushal.webnode.com
- 15. Real Estate Features Great views Low/0-g recreation Human powered flight Cylindrical swimming pools Dance, gymnastics Sports: soccer Environmental independence Custom living Weather art www.engineerkaushal.webnode.com
- 16. When A few decades should be sufficient to build the first one. No serious effort now. Technology requirements: Safer, cheaper launch Extraterrestrial materials Large scale orbital construction Closed ecological life support systems And much more www.engineerkaushal.webnode.com
- 17. How much will it cost? If you have to ask, you can’t afford it. How much did Silicon Valley cost? Orbital space settlements will be far more expensive: all materials imported transportation difficult build all life support hostile environment new techniques must be developed www.engineerkaushal.webnode.com
- 18. Key Problem: Launch www.engineerkaushal.webnode.com
- 19. Launch Data Systems Major opportunities for information technology. SIAT: wiring trend data were very difficult to develop. Some launch failures caused by software Sea Launch second flight Ariane V The comma “,” www.engineerkaushal.webnode.com
- 20. Information Power Grid IPG: integrated nationwide network of computers, databases, and instruments. The Network is the Computer IPG value help reduce launch costs and failure rates support for automation necessary to exploit solar system exploration by thousands of spacecraft Problems: low bandwidths long latencies intermittent communications www.engineerkaushal.webnode.com
- 24. Mass storage
- 25. Visualization
- 28. Condor pools
- 29. Mass storage
- 30. Instruments
- 32. Terrestrial Grid
- 33. Satellites
- 38. Relevant IPG Research Reservations insure CPUs available for close encounter Co-scheduling insure DSN and CPU resources available Network scheduling Proxies for firewalls Extend to represent remote spacecraft to hide: low bandwidth long latency intermittent communication www.engineerkaushal.webnode.com
- 40. Software agent architecture for continuous examination of the database
- 44. Multi-user virtual reality optimized for launch decision support
- 45. Automated computationally-intensive software testingwww.engineerkaushal.webnode.com
- 46. 2020 Tourism Hotel Doctors Maids Cooks Recreational directors Reservation clerks etc. These may be the first colonists. www.engineerkaushal.webnode.com
- 47. Low/0-g Handicapped/Elderly Colony No wheelchairs needed. No bed sores. Easy to move body even when weak. Never fall and break hip. Grandchildren will love to visit. Need good medical facilities. Telemedicine Probably can’t return to Earth. www.engineerkaushal.webnode.com
- 49. AsterAnts: A Concept for Large-Scale Meteoroid Return Deliver extraterrestrial materials to LEO Support solar system colonization Al Globus, MRJ, Inc. Bryan Biegel, MRJ Inc. Steve Traugott, Sterling Software, Inc. NASA Ames Research Center www.engineerkaushal.webnode.com
- 50. Near Earth Object Materials Mining of large NEOs very difficult to automate Mining involves large forces Materials properties are unknown and variable Capture of small NEO may not require human life support 10 million - 1 billion 10m diameter NEOs Far more 1m diameter NEOs www.engineerkaushal.webnode.com
- 51. Solar Sail in Earth Orbit World Space Foundation www.engineerkaushal.webnode.com
- 53. deployed from Progress resupply vehiclewww.engineerkaushal.webnode.com
- 54. Solar Sailing 1 Net force Photons Sail Sun www.engineerkaushal.webnode.com
- 55. Solar Sailing 2 Orbital velocity Outward spiral Propulsive force Sail Orbital velocity Sun Inward spiral Sail Propulsive force www.engineerkaushal.webnode.com
- 56. NEO Characterization Project www.engineerkaushal.webnode.com
- 57. Solar System Exploration High launch cost of launch = small number exploration satellites one-of-a-kind personnel-intensive ground stations. Model based autonomy = autonomous spacecraft Requirement drivers Autonomous spacecraft use of IPG resources low bandwidths long latencies intermittent communications www.engineerkaushal.webnode.com
- 58. Each Spacecraft Represented by an on-board software object. Communicates with terrestrial proxies to hide communication problems know schedule for co-scheduling and reservations Data stored in Web-accessible archives virtual solar system Controlled access using IPG security for computational editing www.engineerkaushal.webnode.com
- 59. Spacecraft Use of IPG Autonomous vehicles require occasional large-scale processing trajectory analysis rendezvous plan generation Proxy negotiates for CPU resources, saves results for next communication window Proxy reserves co-scheduled resources for data analysis during encounters www.engineerkaushal.webnode.com
- 60. Conclusion The colonization of the solar system could be the next great adventure for humanity. There is nothing but rock and radiation in space, no living things, no people. The solar system is waiting to be brought to life by humanity's touch. And computer science can help. www.engineerkaushal.webnode.com
- 61. NEO Composition Widely varied, includes large amounts of: Water Carbon Metals, particularly iron Silicon Spectral studies don’t agree very well with meteorite analysis www.engineerkaushal.webnode.com
- 62. Detection of 1-meter diameter meteoroids Current Earth-based optical asteroid telescopes Smallest found < 10m diameter Maximum 1m detection distance ~ 106 km 2,000 to 200,000 within range at any given time 5-7 hit the Earth each day Radar required for accurate trajectory and rotation rate www.engineerkaushal.webnode.com
- 63. Solar sail experience Solar sailing used by Mariner 10 mission to Mercury for attitude control Enabled multiple returns to Mercury by reducing control gas consumption Ground deployment test by World Space Foundation Zero-g deployment test by U3P in aircraft Russian Znamia mirror February, 1993 www.engineerkaushal.webnode.com
- 64. Solar sail meteoroid return Characteristic acceleration of 1 mm/s2 produces 1.3 km/s delta-v per month 170-182 meters square sail for 500 kg NEO return at 0.25 mm/s2 characteristic acceleration Once design is refined, mass production of AsterAnts spacecraft ?NASA build first one open source, then pay for meteoroid materials by the ton? www.engineerkaushal.webnode.com
- 65. Summary Capture ~1 m diameter NEOs (Near Earth Objects) Return to LEO (Low Earth Orbit) Solar sails for propulsion Start with one small spacecraft, scale up with copies Early returns have scientific value, later materials for construction and resupply www.engineerkaushal.webnode.com
- 66. Conclusion consumables Challenges Benefits small down payment (one small spacecraft) scales by mass production missions can probably be automated no 1m NEO detection difficult solar sails have little flight experience geosynchronous applications require space manufactured sails www.engineerkaushal.webnode.com