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INTERSTELLAR PROPULSION Mason Hoene HONR 289V Section 0101 WHERE - PowerPoint PPT Presentation

INTERSTELLAR PROPULSION Mason Hoene HONR 289V Section 0101 WHERE TO GO? How to Look: Create new satellites Search for exoplanets Identify planets in the habitable zone Destinations: Alpha Centauri system


  1. INTERSTELLAR PROPULSION Mason Hoene HONR 289V – Section 0101

  2. WHERE TO GO? How to Look: • Create new satellites • Search for exoplanets • Identify planets in the habitable zone Destinations: • Alpha Centauri system • Proxima b

  3. HOW TO GET THERE? Methods of Propulsion: ▪ Fusion Rockets ▪ Laser Sails ▪ Antimatter Rockets

  4. FUSION ROCKETS VARIABLES ▪ Produce energy from deuterium/helium-3 ▪ Controlled variables: These are the things that are kept the same throughout your experiments. reaction ▪ Independent variable: The one variable that you purposely change and test. ▪ 12% speed of light ▪ Dependent variable: The measure of change observed because of the independent variable. It is important to decide how you are going to measure the change. ▪ Travel to nearest star in 36 years PLANET MASS PERIOD OF ROTATION DISTANCE FROM THE SUN Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune

  5. FUSION ROCKETS VARIABLES Benefits: ▪ Drawbacks: Controlled variables: These are the things that are kept the same throughout your experiments. ▪ Independent variable: The one variable that you purposely change and test. ▪ ▪ Human transport Limited energy ▪ Dependent variable: The measure of change observed because of the independent variable. It is important to decide how you are going to measure the change. ▪ Technology is already production in current being developed for technology PLANET MASS PERIOD OF ROTATION DISTANCE FROM THE SUN ▪ other purposes Extremely expensive Mercury spacecraft and fuel Venus ▪ Earth Scarcity of helium-3 fuel Mars source Jupiter Saturn Uranus Neptune

  6. ANTIMATTER ROCKETS ▪ Produce energy from reaction between antimatter and matter ▪ 50% speed of light ▪ Travel to nearest star in 8 years

  7. ANTIMATTER ROCKETS Benefits: Drawbacks: ▪ ▪ Allows for human Extremely expensive to transport create antimatter ▪ ▪ Antimatter has already Very little antimatter been created has been created so far ▪ ▪ Fastest propulsion Gamma radiation from reaction

  8. LASER SAILS ▪ Propulsion generated from mirrors reflecting laser beams ▪ Laser beams generated on Earth ▪ 20% speed of light ▪ Travel to nearest star in 20 years

  9. LASER SAILS Benefits: Drawbacks: ▪ ▪ Concept developed Very low mass through solar sails allowance ▪ ▪ No onboard fuel needed Can only send ▪ Most reasonable for the unmanned probes ▪ near future Limited viewing time of destination

  10. FUTURE OF INTERSTELLAR TRAVEL ▪ Unmanned Exploration  Use of laser sails to send small probes  Better data to find best destination ▪ Propulsion Development  Advances in fusion and antimatter technology  New propulsion methods  Eventual human missions

  11. REFERENCES ▪ Bonsor, K. (2018, June 28). How Antimatter Spacecraft Will Work. Retrieved May 12, 2019, from https://science.howstuffworks.com/antimatter2.htm ▪ Duffy, A. (2016, April 13). Space lasers and light sails: The tech behind Breakthrough Starshot. Retrieved May 12, 2019, from https://cosmosmagazine.com/space/space-lasers-and-light-sails-tech-behind- breakthrough-starshot ▪ Glaser, L. B. (2019, March 26). The hunt is on for closest Earth-like planets. Retrieved May 12, 2019, from https://phys.org/news/2019-03-closest-earth-like- planets.html ▪ Howell, E. (2018, March 30). Exoplanets: Worlds Beyond Our Solar System. Retrieved May 12, 2019, from https://www.space.com/17738-exoplanets.html ▪ Masetti, M., & Mukai, K. (2016, February 4). The Cosmic Distance Scale. Retrieved May 12, 2019, from https://imagine.gsfc.nasa.gov/features/cosmic/nearest_star_info.html ▪ Williams, M. (2019, April 29). How Long Would It Take To Travel To The Nearest Star? Retrieved May 12, 2019, from https://www.universetoday.com/15403/how- long-would-it-take-to-travel-to-the-nearest-star/

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