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RUNNER Alex Christensen, William Hatch, Keyvan Johnson, Jorden Luke, Benjamin Maxfield, Andrew Mugleston, Cody Palmer, Jackson Pontsler, Jacob Singleton, Nathan Spencer, Erik Stromberg, Bryce Walker, Cameron Weston ECE 5240 Space Systems Design Spring 2014 Center for Space Engineering

ANGELS Power Slice Electronics Simulations Overview · 2014. 5. 28. · Student Object Designation Diameter Date (dV) Est. ΔV. Distance. Alex Christensen (2001 QC34) 166 - 743 6/17/2019

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  • RUNNER

    Alex Christensen, William Hatch, Keyvan Johnson, Jorden Luke, Benjamin Maxfield, Andrew Mugleston, Cody Palmer, Jackson Pontsler,

    Jacob Singleton, Nathan Spencer, Erik Stromberg, Bryce Walker, Cameron Weston

    ECE 5240 Space Systems Design Spring 2014

    Center for Space Engineering

  • 2

    Picture of Team

    Cameron Weston

    Charles Swenson

    William Hatch

    Jackson Pontsler

    Nathan Spencer

    Bryce Walker

    Keyvan Johnson

    Jorden Luke

    Alex Christensen

    Andrew Mugleston

    Benjamin Maxfield

    Cody Palmer

    Jacob Singleton

    Erik Stromberg

  • 3

    RUNNER

    • Research Utility Nanosatellite for Near Earth object Rendezvous

    • Acronym Invokes image of a “fast scout” – A spacecraft that is a “Runner”, scout, or explorer that

    will characterize the selected Near Earth Object and pave a way for future NASA missions. Future missions include advanced manned and robotic exploration and sample return.

    = +

  • 4

    Presentation Overview • Mission Objectives

    • Concepts of Operation

    • Spacecraft Description – Science Payload – Propulsion – Navigation – Attitude Determination and

    Control System – Power – Communications – Onboard Computing Data Handling – Mechanical Systems – System Budgets

    • Summary / Appendix

  • 5

    Mission Objectives 1 & 2

    • Objective 1 Investigate a near-Earth object through proximity operations to characterize its mass, orbital position, rotational dynamics, and appearance in support of future manned and robotic missions.

    • Objective 2 Observe the thermal, mechanical, mineralogy and water content at the surface of a near Earth object in order to better understand the formation process of our solar system and to enable the future use of mineral resources from these objects.

    NEO Properties Objectives Mass and density Orbit and rotational period Dimensions, appearance, and albedo Surface thermal and mechanical properties Surface mineralogy Near surface water content

    http://neo.jpl.nasa.gov/neo/

  • 6

    Mission Objective 3

    • Objective 3 – Demonstrate the technologies required to rendezvous a 6U CubeSat launched

    as a secondary payload from the NASA Space Launch System EM-1 mission to a wide variety of near Earth object orbits.

    6U CubeSat Deployer

  • 7

    Objectives and Payload Instruments

    • Traceability from Objective 1 to Science Instrument Selection – Mass → Camera & Rendezvous Dynamics – Orbit → Camera & Spacecraft Ranging – Rotational period→ Camera – Dimensions → Camera & IR Camera

    • Traceability from Objective 2 to Science Instrument Selection – Chemical constituents → Magnetometer; Ablation

    Laser / TOF Mass Spectrometer; Near Range Camera; IR Camera; Magnetometer

    – Mechanical structure → Impact Boom, Accelerometer; Near Range Camera; IR Camera

  • RUNNER ECE5240 Spring 2014 8

    • Near-Earth Object Human Space Flight Accessible Targets Study (NHATS) – Total ΔV ≤12 km/s – Launch 2015 - 2020 – Visual Magnitude ≥ 22

    • Found 66 Objects – Est. Diameters 69 – 3243 m – Encounter Range from Earth

    • 0.015 – 1.334 AU

    • Focused on 12 objects – JPL's HORIZONS system

    Target NEO’s Considered

    Student Object Designation Diameter Date (dV) Est. ΔV DistanceAlex Christensen (2001 QC34) 166 - 743 6/17/2019 5.028 0.015Erik Stromberg (2001 VC2) 100 - 448 12/7/2018 2.102 0.212Bryce Walker (2003 GA) 105 - 469 9/26/2015 4.792 0.331Jacob Singleton 138404 (2000 HA24) 263 - 1177 4/5/2016 3.099 0.350Cody Palmer (2008 DG5) 200 - 893 4/11/2018 3.901 0.371Cameron Weston 152563 (1992 BF) 191 - 853 8/19/2016 3.526 0.402William Hatch (2003 YX1) 115 - 514 11/18/2017 3.018 0.480Jackson Pontsler (2012 DK61) 110 - 491 2/25/2019 3.028 0.487Andrew Mugleston 251732 (1998 HG49) 76 - 340 3/18/2018 3.028 0.790Keyvan Johnson 101955 Bennu (1999 RQ36) 115 - 514 3/26/2018 2.006 0.870Benjamin Maxfield 3361 Orpheus (1982 HR) 272 - 1216 9/23/2017 2.338 1.298Jorden Luke 216985 (2000 QK130) 132 - 590 9/15/2017 2.549 1.336

    JPL Small-Body Database

    http://neo.jpl.nasa.gov/cgi-bin/nhatshttp://ssd.jpl.nasa.gov/?horizons

  • RUNNER ECE5240 Spring 2014 9

    • Launch – Secondary payload on SLS EM-1

    and/or latter missions – Launch opportunities between 2015-

    2020 – Size limited to 6U, 12 Kg CubeSat – Compliance with containerized

    specifications of PSC Launcher – No pressurized vessels and no

    pyrotechnic devices

    • Target – Object within 5 km/s ΔV for

    rendezvous after EM-1 ejection

    • Communications – Use of the NASA Deep Space Network.

    Mission Constraints and Assumptions

  • RUNNER ECE5240 Spring 2014 10

    Transfer to NEO rendezvous point

    Rendezvous

    Space Launch System

    Loiter near Moon, await NEO phasing

    Secondary payload

    Proximity operations

    Data downlink

    DSN

    RUNNER Mission Concept

  • 11

    Perpendicular to Ecliptic Plane

    http://lcogt.net/spacebook/equatorial-coordinate-system

    Solar Arrays Track Sun

    Solar array axis normal to ecliptic

    Communication Antenna

  • 12

    Goal: Eclipse avoidance Dawn-Dusk Orbit / Noon Vector

    NEA Rendezvous Science Phase 1

    Characterize appearance and size Photograph and map Determine size and other characteristics / features

  • 13

    NEA Rendezvous Science Phase 1

    Characterize appearance and size Photograph and map Determine size and other characteristics / features

  • 14

    NEA Rendezvous Science Phase 2

    Do science: Ablation laser Magnetometer Accelerometer Spectrometers and cameras Probe / Joust

  • 15

    NEA Rendezvous Science Phase 2

    Do science: Ablation laser Magnetometer Accelerometer Spectrometers and cameras Impact Probe Accelerate

    towards NEO

    Impact Probe

  • 16

    NEA Rendezvous Science Phase 2

    Do science: Ablation laser Magnetometer Accelerometer Spectrometers and cameras Impact Probe Move to Noon-Midnight vector

  • 17

    RUNNER Spacecraft Break Down

  • 18

    Science Payload Breakdown

    Payload

    Dimensions and Appearance

    Thermal Properties Mineralogy

    Mechanical Properties

    Long-range Camera

    Short-range Camera

    Rangefinder

    IR Camera (2x) Ablation Laser

    Mass Spectrometer

    Magnetometer

    Impact Probe

    High Gain Accelerometer

    Low Gain Accelerometer

    Laser Pulse

    Atoms, Ions, Particles

    Mass Spectrometer

  • 19

    Instrument Mass

    • Estimated total mass approximately 1 kg

    Instrument Quantity Unit (kg) Total (kg) Total (cm3)Visible Imager 2 0.200 0.400 14.00

    Microbolometer 2 0.028 0.056 29.04Ablation Laser 1 0.195 0.195 106.50

    Mass Spectrometer 1 0.300 0.300 300.00Magnetometer 1 0.005 0.005 0.75

    Rangefinder 1 0.022 0.022 40.96Low Gain Accel 1 0.001 0.001 0.03High Gain Accel 1 0.002 0.002 0.04

    Science Board 1 0.150 0.150 150.00Total 0.981 (kg) 641.3 (cm3)

    Items in red are low TRL and estimated masses

  • 20

    Instrument Telemetry

    • Total Science Telemetry is 2.4 Gb – Total bits are based off the rate of the instrument and the time instrument is on

    according to the concept of operations (~20 days)

    Instrument Rate Sample Size (bits) Total Bits over Mission (Mbits)Visible Imager Once per Day 72000000 2160Microbolometer Once per Day 15728640 157.3Mass Spectrometer 10 Hz for 2 min 256 3.072Magnetometer 1 Hz 48 86.4Rangefinder Once per Day 16 4.8E-04Low Gain Accel 10 Hz for 5 min 32 0.960High Gain Accel 10 Hz for 5 min 32 0.960

    Total 2409

  • 21

    BFRIT-3 Busek 3-cm Ion Thruster

    • Thruster, cathode, PPU – 1U, 1kg • Iodine Propellant (TRL-4)

    Image courtesy of Busek.com

  • 22

    Maximum Capabilities (6 Panels, 1 AU)

    Nominal Operations Nominal Operations

    ISP (s) ISP (s)

  • RUNNER ECE5240 Spring 2014 23

    Rendezvous STK Astrogator

    1992_Bf leaving orbit on 5 Aug, 2017 resulted in an orbit very similar to the 1992_BF asteroid, but off phase.

  • 24

    ADCS Break Down Diagram

  • 25

    Solar Panel Study

    30 cm

    60 c

    m

    20 cm

    Total Number of Subpanels

    Solar cell placement study 2 panels with 3 subpanels (0.18 m2)

    Requirement

  • 26

    Communication Concept of Operations

  • RUNNER ECE5240 Spring 2014 27

    Design Element Symbol Units S-Band X-band Optical Link Frequency f GHz 2.4 8.5 5.66E+05 Transmitter Power Ptx Watts 10.66 2.00 0.10

    Transmitter Power Ptx dBW 10.28 3.01 -10.00 Transmitter

    Antenna Diameter D m 34.000 0.300 0.010 Antenna Gain Gtx dB 55.63 20.07 92.45 Antenna Transmitter Losses Ltx dB -0.5 -0.5 -3 Antenna Beam width θtx Deg 0.26 15.44 0.00 Antenna Misalignment αtx Deg 0.2 1 0.002 Alignment Loss Lθtx dB -7.25 -0.05 -3.48

    Data Rate and Margin Calculations

    Rates

    Data Rate R Bps 1000 1000 1000

    Eb/No Available Eb/No dB 8.60 9.21 16.37

    Required Eb/No - Modulation Format Eb/No dB 9.6 9.6 13.3

    Coding gain dB 7 7 7

    Required Eb/No Eb/No dB 2.60 2.60 6.30

    Required Margin dB 3 3 3

    Margin dB 3.00 3.61 7.07

    Receiver Antenna Diameter D m 0.2 34.0 1.00 Antenna Gain Gr dB 20.00 67.44 133.59 Antenna Receiver Loss Lr dB -0.5 -0.5 -3 Antenna Beam width θr Deg 48.61 0.08 0.00

    Antenna Misalignment αr Deg 0.01 0.01 0

    Alignment Loss Lθr dB 0.00 -0.21 0.00 Total Receiver G dB 19.50 66.73 130.59

    • Trade Study – S-band, X-band, Optical

    • Pros vs cons of each

    • X-Band Selected for RUNNER

    • DSN 34 Meter Dish Antenna

    Band Pro Con S-band Lots available

    hardware Low data rates

    X-band Better data rates Not much hardware available

    Optical Best data rates To complex

  • RUNNER ECE5240 Spring 2014 28

    • TX (8.2GHZ) Length = 9.8414 mm Width = 12.2634 mm Input Impedance = 200.25 Ω USE 18 total patches

    • RX (7.2GHZ) –Length = 10.25 mm –Width = 13.97 mm –Input Impedance = 200.25 –Use 18 total patches

    Antenna Patch Calculations

  • RUNNER ECE5240 Spring 2014 29

    Data Rate VS Distance

    0

    5000

    10000

    15000

    20000

    25000

    30000

    35000

    0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4

    Dat

    a R

    ate

    (Bits

    /sec

    )

    Distance (AU)

    34 Meter Dish

    2W TX4W TX8W TX

    1.1kbits/s

  • 30

    RUNNER Spacecraft

    6U Spacecraft

    Rx & Tx Antennas

    Transmit Antenna

    Solar Panels

    Solar Panels

    Rx & Tx Antennas

  • Propellant Tank

    Thruster and pointing Gimbal

    PPU Electronics

    L-3 Radio Tx / Rx

    ADCS System & wheels Power

    Management

    On-Board Computer

    Battery System

    Imager (near) Imager (far)

    Microbolometers Laser

    Range Finder

    TOF Mass Spectrometer

    Ablation Laser

    Star Tracker

    Impact Boom

    μPPT Attitude Thrusters

  • 32

    Small Satellite Cost Model

    Total Spacecraft Cost ($K) = $14,226

    Total Instrument & Science Cost ($K) = $6,000

  • 33

    Navigation Conclusions

    • Fly by missions are relatively easy to accomplish. Matching an asteroids orbit will take significantly more planning.

    • Based on our simulations, it is possible to reach Near Earth Asteroids using cube sat technology.

    • RUNNER’s distance from earth will be a key consideration in planning missions.

    • The NEA ‘2000 HA24’ has an especially promising orbit in 2018

    �RUNNERPicture of TeamRUNNERPresentation OverviewMission Objectives 1 & 2Mission Objective 3Objectives and Payload InstrumentsTarget NEO’s ConsideredMission Constraints and� AssumptionsRUNNER Mission ConceptPerpendicular to Ecliptic PlaneNEA Rendezvous Science Phase 1NEA Rendezvous Science Phase 1NEA Rendezvous Science Phase 2NEA Rendezvous Science Phase 2NEA Rendezvous Science Phase 2RUNNER Spacecraft Break DownScience Payload BreakdownInstrument MassInstrument TelemetryBFRIT-3 Busek 3-cm Ion ThrusterMaximum Capabilities (6 Panels, 1 AU)Rendezvous STK AstrogatorADCS Break Down DiagramSolar Panel StudyCommunication Concept of OperationsData Rate and Margin CalculationsAntenna Patch CalculationsData Rate VS DistanceRUNNER SpacecraftSlide Number 31Small Satellite Cost Model Navigation Conclusions