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ARTEM1S�Architecture for Radiation Testing at Earth-Moon L1 Station

Presenter: Danielle Waters

December 11, 2018

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Context

  • NASA has been charged by the current administration to return to the Moon with a Mars forward focus
  • Our goal: boots on the Moon by 2022, the 50th anniversary of the Apollo 17

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Problem

  • Current program: Lunar Gateway
    • Originally planned to support asteroid mining mission
    • 1st module launching in 2022 (too late)
    • Near-Rectilinear Halo Orbit around the Moon
      • Not Mars forward

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Goals: Rapid Lunar Station

  • Study effects of Deep Space radiation in free space in proximal location
  • Flexible & constant access to Earth & Moon
  • Test new technologies in-situ
  • Facilitate future Mars missions
  • Economically Self-Sustaining

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Rationale for L1 Location

  • Orbital flight characteristics, different from Interplanetary flight
    • Thermal, shadow, pointing, attitude, etc.
  • Simulates deep space due to 4π sr exposure to Galactic Cosmic Rays (GCRs) and Solar Energetic Particles (SEPs)
  • Easily accessible to Earth & ALL latitudes of the Moon
  • Well-positioned for further Earth Neighborhood exploration
    • Avoids Earth and Moon gravity wells on way out of Earth’s Sphere of Influence

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SEP

SEP

SEP

SEP

GCR

GCR

GCR

GCR

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Concept: Station

  • Simple
    • 2 Combined Bigelow B330 Expandable Habitats
      • 330 m3 volume ea. (30% of current ISS volume)
      • Houses up to 6 astronauts
      • Ready to launch to LEO by 2021 and orbit Moon by 2022 according to a Feb 2018 statement by founder, Robert Bigelow

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Concept: Station

  • Self-Sustaining
    • Bigelow B330 Expandable Habitats
      • Independent station – propulsion, avionics, life support
      • Micro-meteroid and orbital debris shield, MLI, BETA cloth
    • Kilopower fission reactor
      • Moon has 14 Earth days of shadow per month
      • Solar power drops off ~1/r2 from the Sun, applies to Mars
        • Fission power essential for Moon and Mars missions
      • 3-4 units would power Power and Propulsion Element planned for Lunar Gateway station (30-40kW)
      • Certified in May 2019

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Concept: Architecture

  • Phase 1a
    • Tele-operated from Earth/ ISS
    • Primarily plants and sensors collecting data
      • No telerobotic way to care for animals ethically, yet
  • Phase 1b
    • Develop telerobotic system to care for test animals
    • Short-duration crew visits to tend animals and gather data
      • 1-2 weeks

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Concept: Architecture

  • Phase 2:
    • Long-duration crew missions
      • 3 months initially
      • Eventually simulate 8-month transit to Mars
      • Crew documents effectiveness of countermeasures to extended exposure to GCR and SEP radiation
      • Solar Storm Shelter
    • Telerobotic support to Lunar rover missions

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Concept: Funding

  • Lunar Tourism
    • Cheaper ticket for station than Lunar surface
  • Lunar Toys
    • Send up plush “alien” toys regularly, take pic of them up there with Earth or Moon in background and market them as “space pals”

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Merits & Limitations

  • Merits:
    • Opportunity to test out new technologies
      • Radiation shielding for deep space
      • Nuclear fission reactor
      • Expandable module
    • Provides constant presence in space beyond LEO
      • Constant communication to support lunar missions
      • Constant access to Moon and Earth
    • Central location for space port to other planets
    • Simulates Interplanetary flight better than orbital
  • Limitations:
    • Waypoints add some delta-V over direct transfers
    • Longer transit time to lunar surface than NRHO

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Summary

  • L1 is prime location to study the effects of radiation on living beings
  • Utilizing existing technologies in a test-bed environment allows for rapid development and build
  • Excellent jumping-off point to Moon & continue further into the solar system

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L1 Halo Orbit

Mars Transfer Orbit

LEO

L1 Transfer Orbit

Moon Transfer Orbit into LLO

  • Assemble station in LEO
  • “Layovers” at ISS to acclimate to Space
  • L1 Bigelow Station
  • Radiation Shielding Testbed
  • Nuclear Testbed
  • Lunar Tourism
  • “Alien” Toys
  • Remote Ops on Moon Surface
  • Lunar Transfer Point
  • Mars Transfer Start
  • Resources transferred to and waste removed from moon

Cislunar Infrastructure 2022-2030

Not to scale

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Future Studies

  • Investigate more options for radiation shielding in deep-space
    • Water & fuel outer Shield (Passive)
    • Plasma shield using electrostatic & electromagnetic fields (Active)
  • Investigate way to implement telerobotics in live animal radiation testing in space
  • Investigate Bi-modal Nuclear Thermal Rocket(BNTR) and VASIMR

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Thank you!

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References

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Backup Slides

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Architecture: Station

  • Water shielding from radiation
    • Already have to taker water, this makes it useful
    • Self-sustaining through waste-recycling program
    • Water is highly efficient at shielding from radiation

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  • Bimodal NTR
    • Alternate power source to Kilopower
    • Long-term propulsion and power source for Mars missions

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Merits of L1

  • Easily Accessible from Earth & to Moon
    • L1 has similar total transit time to NHRO, lower overall ΔV, & greater launch/transfer flexibility

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L1 Halo Orbit

NRHO

L2 Halo Orbit

Distance to Earth (km)

326,400

384,400

448,900

Distance to Lunar Surface (km)

58,000

2,000-75,000

64,500

ΔV LEO to Lunar Station

3.77 km/s

3.95 km/s

3.43 km/s

Transit Time LEO to Lunar Station

4 days

5 days

8 days

ΔV Lunar Station to Moon Pole

0.75 km/s

0.73 km/s

.8 km/s

Transit Time Lunar Station to Moon Pole

2 days

0.5 days

3 days

ΔV Lunar Station to Moon Equator

0.7 km/s

.898 km/s

.75 km/s

Transit Time Lunar Station to Moon Equator

2 days

0.5 days

3 days

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StemRad Shielding

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