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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.
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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/
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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
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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
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NEA Rendezvous Science Phase 1
Characterize appearance and size Photograph and map Determine size and other characteristics / features
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NEA Rendezvous Science Phase 2
Do science: Ablation laser Magnetometer Accelerometer Spectrometers and cameras Probe / Joust
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NEA Rendezvous Science Phase 2
Do science: Ablation laser Magnetometer Accelerometer Spectrometers and cameras Impact Probe Accelerate
towards NEO
Impact Probe
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NEA Rendezvous Science Phase 2
Do science: Ablation laser Magnetometer Accelerometer Spectrometers and cameras Impact Probe Move to Noon-Midnight vector
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RUNNER Spacecraft Break Down
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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
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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
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BFRIT-3 Busek 3-cm Ion Thruster
• Thruster, cathode, PPU – 1U, 1kg • Iodine Propellant (TRL-4)
Image courtesy of Busek.com
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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.
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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
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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
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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
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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