Small Satellite Aerocapture for Increased Mass Delivered to Venus and Beyond

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Small Satellite Aerocapture for Increased Mass Delivered to Venus and Beyond

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Small Satellite Aerocapture for Increased Mass Delivered to Venus and Beyond Adam Nelessen / Alex Austin / Joshua Ravich / Bill Strauss NASA Jet Propulsion Laboratory Ethiraj Venkatapathy / Robin Beck / Paul Wercinski / Mike Wilder / Gary Allen / Michael Aftomis NASA Ames Research Center Robert Braun / Michael Werner / Evan Roelke University of Colorado Boulder June 14, 2018 2018. All rights reserved.

Overview A multi-organizational team is developing an aerocapture system for Small Satellites Currently in year 1 of a 2-year effort Utilize drag modulation flight control to mitigate atmospheric & navigation uncertainties Initially studied by Putnam and Braun in Drag Modulation Flight Control System Options for Planetary Aerocapture Simplest form is the single event jettison Ballistic coefficient ratio ( β2 β1) provides control authority Study addresses key tall tent pole challenges 1. 2. Orbit targeting accuracy Thermal protection system feasibility 3. Stability before, during, and after jettison event Altitude (km)! 2 Deceleration (g)! 1 Technology development has so far been mission-agnostic Pursue a notional flight system design and target orbit to demonstrate existence proof Design and tools can be custom-tailored for a range of possible science missions Heat Rate (W/cm 2 ) Planet-Relative Velocity (km/s) 2

Mission Applicability Potential Destinations: Venus Earth Mars Titan Ice Giants Vehicle Options: HIAD Mechanical deployable drag skirt Rigid drag skirt Delivery Schemes: Dedicated launch & cruise Delivery by host spacecraft Mechanical deployable drag skirt Rigid drag skirt 3

Mission Applicability Potential Destinations: Venus Earth Mars Titan Ice Giants Vehicle Options: HIAD Mechanical deployable drag skirt Rigid drag skirt Delivery Schemes: Dedicated launch & cruise Delivery by host spacecraft Mechanical deployable drag skirt Rigid drag skirt Initial Focus: Chose Venus to bound the technology s capability. Can scale to easier destinations. Chose rigid drag skirt and host spacecraft delivery to minimize system complexity. 4

ConOps: Exo-Atmospheric Poten8al Hosts: Dedicated carrier spacecraa Discovery or New FronEers missions that target or fly by Venus! " Coast to Atmospheric Entry Atmospheric Entry Entry Velocity = 11 km/s Flight Path Angle! = -5.40 deg Deploy from host S/C

ConOps: Atmospheric Atmospheric Flight Drag Skirt Separation Ballistic Coefficient Ratio: 9 Nominal Time: Entry + 93 sec Nominal Velocity: 8.9 km/s Nominal Peak Heat Rate: 383 W/cm 2 Nominal Peak Deceleration: 9 G! Atmospheric Entry Entry Velocity = 11 km/s Flight Path Angle! = -5.40 deg Atmospheric Exit Nominal Time: Entry + 270 sec Nominal Velocity: 7.75 km/s

ConOps: Post-Aerocapture Initial Orbit Periapsis: 100 km Apoapsis: 2000 km Period: 1.83 hr Drop Heat Shield + Periapsis Raise Maneuver Nominal Time: Atm. Exit + ½ Period Trigger: Timer

ConOps: Post-Aerocapture Initial Orbit Periapsis: 100 km Apoapsis: 2000 km Period: 1.83 hr Final Orbit Periapsis: 200 km Apoapsis: 2000 km Period: 1.85 hr Drop Heat Shield + Periapsis Raise Maneuver Nominal Time: Atm. Exit + ½ Period Trigger: Timer

Representative Flight System Pre-Je&son Configura0on Delivered Flight System Rn= 10 cm 40 cm 150 cm Science Payload ~1.5U available volume Telecom (~2.5 kbps to 70m DSN) IRIS X-Band Radio X-Band Patch Antenna X-Band Circular Patch Array HGA ACS (~10 arcsec pointing accuracy) BCT Star Tracker, Sun Sensors (x4), and Control Electronics BCT Reaction Wheels (x3) Sensonor IMU C&DH JPL Sphinx Board Pyro Control Board! Ra#o = 9 Total Margined Mass = 69kg Thermal Kapton Film Heaters MLI Power (~25 W with body mounted solar cells) Solar Arrays Clyde Space EPS 18650 Li-ion batteries (x11) (~180 Wh) Propulsion (~70 m/s delta-v) 0.5 N Monoprop Thrusters (x4) Mechanical Structure, TPS, Rails, Rollers, Separation Hardware 9

Orbit Delivery Accuracy 3DOF Monte Carlo runs in trajectory tool used to assess orbit targeting accuracy VenusGRAM atmospheric model with 3-sigma variability in density and wind speeds Options for improving orbit targeting accuracy are under investigation Reduce EFPA error Increase ballistic coefficient ratio Improve G&C algorithm for drag skirt separation timing 10

Mass Efficiency Comparison Mass Efficiency Comparison 80 Delivered Mass Orbit Insertion Mass 70 60 Mass [kg] 50 40 42 55 53 51 48 46 40 35 30 20 10 26 14 15 17 20 22 28 33 0 Aerocapture System, 2000km Propulsive, 2000km Propulsive, 3000km Propulsive, 5000km Propulsive, 7500km Target Orbit Apoapsis Altitude [km] Propulsive, 10000km Propulsive, 20000km Propulsive, 35000km The aerocapture-based orbit insertion system delivers 85% more useful mass to a 2000km apoapsis orbit than an all-propulsive system 11

Other Activities NASA Ames Aerothermal analysis TPS sizing CFD simulations Ballistic range test development See Robin Beck s presentation Studies in support of Venus aerocapture utilizing drag modulation for more information Stagnation Point Heating vs Time CU Boulder G&C algorithm development CFD simulations Shot 2800: P = 50 Torr (0.067 atm), r = 0.079 kg/m 3 See Michael Werner s presentation Dynamic propagation of discreteevent drag modulation for Venus aerocapture for more information 12

Conclusions and Future Work This initiative addresses the following key challenges for drag modulation aerocapture at Venus: 1. Orbit targeting accuracy 3DOF Monte Carlo simulations of the maneuver G&C algorithm improvements (Work to Go) 2. Thermal protection systems Preliminary aerothermal assessment and TPS design CFD detailed aerothermal assessment (In Progress) 3. Stability before, during, and after jettison event Preliminary 6 degree-of-freedom simulations CFD analysis of dynamics of drag skirt separation (In Progress) CFD aerodynamic database generation (Work to Go) Ballistic range testing (Work to Go) To improve mission accommodation options, investigating an ADEPT-based mechanical deployable drag skirt option 6DOF Trajectory Simulation CFD Separa=on Analysis Ballistic Range Model Design 13

Thank you! 14

Internal Flight System Configuration Payload Volume (10 cm 3 shown) Pyro Control IMU Star Tracker EPS Board Patch Antenna Reaction Wheel (x3) Avionics Stack (Computer, Radio, ACS Electronics) Separation Rollers (x3) Backshell Circular Patch Antenna Array Thrusters (x4) Batteries (x11) Propulsion Tank Ballast Mass TPS 6/22/18 15 Heatshield Structure