1. Khufu’s Starship Jennifer Nill Chelsea Donaldson Graham Risch Henry Shennan Jonathan Lumpkin Jennifer Nill Chelsea Donaldson Graham Risch Henry Shennan Jonathan Lumpkin Conceptual Design Review Fall 2010 Rev A September 16, 2010

2. Mission Overview Objectives: -Collect 3 different types of data including: -Magnetic field strength and orientation -Ultra-Violet radiation strength -Solar cell efficiency -Capture multiple photo images of the surroundings of the BalloonSat during flight Objectives: -Collect 3 different types of data including: -Magnetic field strength and orientation -Ultra-Violet radiation strength -Solar cell efficiency -Capture multiple photo images of the surroundings of the BalloonSat during flight

3. Mission Overview Expectations: Our team would like to prove/discover…  That the Earth’s magnetic field is in the process of polar reversal and is subsequently at a weaker strength than would be expected if the poles were not in transition of “flipping”.  That there is greater UV radiation at higher elevations proving that the Earth’s atmosphere blocks out a portion of the ultraviolet wavelengths of the electromagnetic spectrum.  The efficiency of encapsulated solar cells under different atmospheric conditions.  What the “edge of space” looks like from our homemade satellite at high elevations. Expectations: Our team would like to prove/discover…  That the Earth’s magnetic field is in the process of polar reversal and is subsequently at a weaker strength than would be expected if the poles were not in transition of “flipping”.  That there is greater UV radiation at higher elevations proving that the Earth’s atmosphere blocks out a portion of the ultraviolet wavelengths of the electromagnetic spectrum.  The efficiency of encapsulated solar cells under different atmospheric conditions.  What the “edge of space” looks like from our homemade satellite at high elevations.

4. Mission Overview Purpose: To use the onboard instruments to characterize temperature, humidity, magnetic flux, and incident radiation and how these are affected by the atmosphere, temperatures, and elevation as the satellite travels vertically through the atmosphere as well as gather photographic evidence of the flight to the “edge of space”. Purpose: To use the onboard instruments to characterize temperature, humidity, magnetic flux, and incident radiation and how these are affected by the atmosphere, temperatures, and elevation as the satellite travels vertically through the atmosphere as well as gather photographic evidence of the flight to the “edge of space”.

5. Design Drawings:

6. Design Drawings:

7. Design Parts: Foam core structure Hot glue Aluminum tape Velcro Insulation Batteries HOBO data logger Parts: Foam core structure Hot glue Aluminum tape Velcro Insulation Batteries HOBO data logger Switches Digital camera, 2GB memory card Heater kit Solar cells Photodiodes Computer chip Magnetometer

8. Design Functional Block Diagram:

9. Management Organizational Chart: NamesDuties ChelseaTeam Leader/Magnetometer Experiment Design JenUV Sensor Experiment Design JohnStructural Design HenryIT/Programming GrahamSolar Panel Experiment Design/Budget manager

10. Management Schedule: Design complete 9/16/2010 Acquire all hardware 9/28/2010 Magnetometer sensor test complete 9/30/2010 Prototyping design complete 10/4/2010 DD Rev A/B and CDR presentation 10/5/2010 Cold test complete 10/12/2010 Drop test complete 10/12/2010 Whip test complete 10/12/2010 Testing of final design complete 10/26/2010 Mission simulation 10/28/2010 LLR presentation and DD Rev C 11/2/2010 Weigh In 11/5/2010 Final presentations due 11/30/2010 Design document Rev D due 12/4/2010 Design Expo 12/4/2010 Hardware Turn in 12/7/2010

11. Budget ItemCostWeight Adruino Nano$18.9510 g HOBO H08-004-02-30 g Canon A570IS digital camera-220 g Heating Circuit-100 g 9V Batteries and 5V regulator$20<35 g Foam Core and Foam Insulation-150 g External Switches-15 g PVC pipe with rubber bushings$3.5515 g Encapsulated Solar Cells$15.8080 g MicroMag 3-axis Magnetometer$59.9510 g Dry Ice$10.00- UV Photodiodes$80.0020 g Totals$208.25685 g

12. Worries… Our team’s biggest worries about the mission and/or design are the possibilities of whether: The magnetometer will be isolated enough in our design to not have the other instruments onboard cause interference Our structural design will be strong enough to survive the impact of the fall after its flight We can maintain an internal temperature of greater than -10˚C with our structural design Our team’s biggest worries about the mission and/or design are the possibilities of whether: The magnetometer will be isolated enough in our design to not have the other instruments onboard cause interference Our structural design will be strong enough to survive the impact of the fall after its flight We can maintain an internal temperature of greater than -10˚C with our structural design