A Crewed Mars Exploration Architecture Using Fly-by and Return Trajectories
description
Transcript of A Crewed Mars Exploration Architecture Using Fly-by and Return Trajectories
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A CREWED MARS EXPLORATION ARCHITECTURE USING FLYBY AND RETURN TRAJECTORIES
Andrew S.W. Thomas NASA Astronaut, Explora1on Branch, Astronaut Oce, NASA Johnson Space Center
Cesar A. Ocampo
Senior Engineer, Odyssey Space Research LLC., NASA Johnson Space Center
Damon F. Landau Jet Propulsion Laboratory, California Ins1tute of Technology
FISO Telecon 04-08-15
Presentation given by: C. Ocampo and D. Landau
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This presentation is not a stand-alone presentation document. It requires narration.
These are part of the results of an internal NASA-JSC study with NASA-JPL collaboration titled The Mars Lite Study
2015 All rights reserved
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Inspira1on Mars Founda1on
Aims to launch a manned mission to y by Mars in by 2021
Founda1on claims that space explora+on provides a catalyst for growth, na+onal prosperity, knowledge and global leadership.
By taking advantage of this window of opportunity, the Inspira1on Mars Founda1on intends to revitalize interest in science, technology, engineering and mathema+cs (STEM) educa+on.
hPp://www.inspira1onmars.org/
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Figure Only: EME-Inspiration Mars Foundation. (in case next slide video does not work for some)
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Video: EME-Inspiration Mars Foundation. Click center of screen once to start.
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Figure Only: EME-Inspiration Mars Foundation Fly Around. (in case next slide video does not work for some)
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Video: EME-Inspiration Mars Foundation Fly Around. Click center of screen once to start.
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Single Flyby Mission: fast in-and-out
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Ballistic single flyby Pass.
Speed up Catch up
dip in and out v v
v
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Figure Only: Single Flyby Mission: fast in-and-out: (in case next slide video does not work for some)
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Video: Single Flyby Mission: fast in-and-out: Click center of screen once to start.
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Solu1on: Use Low Energy Flyby and Return Trajectories with Two Flyby Events
Inherit natural abort op1on
The two yby events separated by months
Place massive transit habitat(s) on these trajectories
eliminate inser_on and departure of massive assets into and out of Mars Orbit
1st yby event is used to drop o a crew taxi
2nd yby event picks-up and uses a hyperbolic rendezvous for Earth return
Assume Mars Stay Habitat has been Pre-deployed at Mars
Favor launch, en-route maneuvers, Earth arrival speeds over transit >mes. Assume no new major technology development.
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Work summarized and presented as paper AAS 15-372 at the 25th AAS/AIAA Space Flight Mechanics Mee1ng, Williamsburg, VA, January 2015
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Mars Free Returns
Damon Landau
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Broad Search of Mars Free-Returns Search parameters
Launch 20152052
Maximum ight 1me: 1200 days
Maximum Launch V: 7 km/s
Maximum Arrival V: 9 km/s
Minimum Mars yby al1tude: 300 km
Heliocentric revolu1ons between encounters: 0 or 1
Number of gravity assists: 1 or 2
Parameters specic to Star algorithm
Time step for encounter dates: 3 days
Maximum V at yby: 20 m/s
V step for 180 transfers: 20 m/s 13
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Trajectory Search Methodology
1. Grid up Earth, Mars, and Earth encounter 1mes
2. Calculate outbound & inbound legs independently
3. Filter on low V to match in & out V at Mars
Turns a 3-D search into two 2-D searches
720M sequences considered with only 7.3M trajectory computa1ons (Lambert ts)
44,725 trajectories met all constraints
Flight time < 1200 d
Mars Flyby V < 20 m/s Alt > 300 km
Launch Dates
V < 7 km/s
Earth Return
V < 9 km/s 2015
2052
3-day increments
V constraint violated
Time node deleted
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Double-Flyby Free-Returns
Flight time < 1200 d
Launch Dates
V < 7 km/s
Mars or Venus
V < 20 m/s
Mars or Venus
V < 20 m/s
Earth Return
V < 9 km/s 2015
2052
3-day increments
EMME, EMVE, EVME sequences in single run
Transform 4-D search into three 2-D searches
280B sequences assessed with only 27M trajectory ts
1,425 trajectories met all constraints
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Building Mul1ple Flybys Flyby V calcula1on builds trajectory segments with three encounters:
departure body to yby body (incoming leg) and yby body to arrival body (outgoing leg).
The outgoing legs for one trajectory segment match with the incoming legs to another trajectory segment.
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Launch Dates
Mars or Venus
Mars or Venus
Earth Return
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Launch Dates
Mars or Venus
Mars or Venus
Earth Return
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Flight Times
Trajectories in black also satisfy Trans-Mars Injection V < 4.5 km/s and Earth entry < 12.5 km/s
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Launch Opportuni1es
Trajectories in black also satisfy Trans-Mars Injection V < 4.5 km/s and Earth entry < 12.5 km/s
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3:2 Resonance Free Returns
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2:1 Resonance Free Returns
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Short Flight Time
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Double Mars Flyby
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Venus Flybys
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con1nue Using Free Returns for extended Human Mars Explora1on missions
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Determine how to use 2 yby events
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Solu1on 1: Dual Habitat Concept
OTH = Outbound Transit Habitat RTH = Return Transit Habitat 26
Sketch credited to Ryan Whitley (JSC)
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Solu1on 2: Loiter Habitat Concept
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Sketch credited to Ryan Whitley (JSC)
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Copernicus: A Generalized
Trajectory Design and Op_miza_on System
Developed jointly between the University of Texas and the NASA Johnson Space Center (2001-present)
Hosted at NASA-JSC
Current Development at JSC
Current Lead Developer:
Jacob Williams, ERC-NASA-JSC, Houston, Texas
28 http://www.nasa.gov/centers/johnson/copernicus/
Used
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Impulsive Gravity Assist to Real Flyby Conversion
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Impulsive Gravity Assist to Real Flyby Conversion
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Figure Only: Initial Guess for An Earth-Venus-Mars-Earth Free Return. Animation on next slide.
Earth Depart
Earth Arrive
Venus Flyby
Mars Flyby
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Video: EVME Trajectory Construction Iteration Sequence. Click center of screen once to start.
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Dual Habitat Model
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Uses an Earth-Mars conjunc1on class trajectory for the Outbound Habitat and an Earth-Mars-Earth Flyby and Return Trajectory for the Return Habitat
Crew Taxi Drop-o and Transfer to a 1-Sol Orbit
1-Sol Orbit Departure and Hyperbolic
Rendezvous with Return Habitat
Low energy conjunc1on class Earth-Mars
3:2 Resonant Earth-Mars-Earth Free Return Trajectory (Habitat orbits Sun twice while the Earth orbits Sun 3 1mes
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OTHEarth Departure10/13/2039
RTHMars Flyby10/21/2041
OTHMars Arrival06/21/2040
RTHEarth Departure06/04/2039
RTH Earth Arrival05/13/2042
RTH E-M-E Trajectory
(3:2 Resonant w/Earth)
2039 2040 2041 2042 2043
RTH
OTH
EarthDep.
EarthDep.
MarsFly by
MarsFly by
Crew at Mars
EarthArr.
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Figure Only: Dual Habitat Model Animation on next slide
OTH Mars Arrive
RTH Mars Flyby Pickup, Hyperbolic Rendezvous
RTH Earth Arrive
RTH Earth Depart
OTH Earth Depart
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Video: Dual Habitat Model Animation. Click center of screen once to start.
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Dual Habitat Model 37
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Loiter Habitat Model Uses an Earth-Mars-Mars-Earth Flyby and Return Trajectory
Mars Flyby 1 to Mars Flyby 2
Loiter Leg
Crew Taxi Drop-o and Transfer to a 1-Sol Orbit
1-Sol Orbit Departure and Hyperbolic
Rendezvous with Loiter Habitat
In live discussion point out the key features/pros/cons
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Video: Loiter Hab Mars Centered Iteration Sequence. Click center of screen once to start.
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41 Figure only: Converged Solution of previous slide video.
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Figure: Mars Arrival Flyby-Loiter-Mars Departure Flyby
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Figure only: Loiter Hab Mode;. (in case next slide video does not work for some)
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Video: Loiter Hab Model Animation. Click center of screen once to start.
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Figure Only: Loiter Hab Model Fly Around. (in case next slide video does not work for some)
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Video: Loiter Hab Model Fly Around. Click center of screen once to start.
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Loiter Habitat Model Departure Earth
Mars Transit
Mars Mars Transit
Mars Earth Transit
Total MissionDuration
EarthDeparture
V
Mars Fly-by1V
Mars Fly-by2V
Earth ArrivalV
TotalEn-route
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date day day day day km/s km/s km/s km/s km/s
6 Aug 2020 399 325 303 1028 3.794 2.550 3.018 4.714 1.676
8 Sep 2022 380 311 320 1010 3.673 2.573 2.887 3.787 0.621
05 Oct 2024 348 305 325 976 3.335 2.555 2.721 3.018 0.000
27 Nov 2026 280 303 358 941 4.000 2.942 2.989 3.546 0.126
29 Dec 2028 252 305 366 923 4.000 3.746 3.505 4.609 0.205
13 Feb 2031 223 321 379 924 4.000 3.804 3.251 4.317 0.515
31 Mar 2033 218 358 346 922 4.000 3.703 3.108 4.410 1.100
22 Jul 2035 364 346 213 923 4.000 3.100 3.737 3.884 0.856
10 Sep 2037 370 317 234 921 4.000 3.178 3.669 4.118 0.195
3 Oct 2039 367 305 267 939 3.530 2.852 3.041 4.045 0.000
21 Oct 2041 341 302 338 981 3.159 2.635 2.647 3.268 0.000
15 Oct 2043 331 303 381 1016 4.000 2.782 2.666 3.630 0.495
22 Jan 2046 244 315 375 934 4.000 3.762 3.289 4.227 0.477
13 Mar 2048 219 343 360 923 4.000 3.877 3.214 4.453 0.775
7 Jul 2050 347 361 209 917 4.000 3.046 3.606 3.721 1.068
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Drop-O from and Rendezvous with Transi_ng (Loiter) Habitat
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Drop-O from and Rendezvous with Transi_ng (Loiter) Habitat
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1st maneuver: capture, coast to apoapsis
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2nd maneuver: plane change, coast to periapsis
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3rd maneuver: capture into op1mal 1-Sol Orbit Mars Stay
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4th, 5th maneuver: depart and do Hyperbolic Rendezvous
Total In-and-Out DV cost = 2.308 km/s (Oct 2039) (this ranges from 2.1 to 3.1 for all 15 Loiter Habitat Solu_ons) 53
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Figure Only: Mars centered transfers, iteration sequence. (in case next slide video does not work for some)
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Video: Mars centered transfers, iteration sequence. Click center of screen once to start.
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All Dual-Habitat, Loiter-Habitat Solu1ons require same type of Mars Centered Maneuvering
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Figure only: Capture-Departure Geometry Fly Around. (in case next slide video does not work for some)
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Video: Capture-Departure Geometry Fly Around. Click center of screen once to start.
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Figure only: Departure, Hyperbolic Rendezvous. (in case next slide video does not work for some)
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Video: Departure, Hyperbolic Rendezvous. Click center of screen once to start.
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One chance to catch the train ride home.
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(image credit: The Darjeeling Limited, Fox Searchlight Pictures)
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Solu_on 3: Hybrid Dual Loitering Habitat Model Four Flyby Events
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Six E-M-M-E Mission Possibili_es for the Hybrid Dual-Loitering Habitat Strategy
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Dual Loitering Habitat Model: Maneuver Data and Performance
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Concluding Remarks... ! Stair-step approach: Flyby-only, orbital, surface access,
access to Phobos, Deimos
! Launch vehicle (Space Launch System) requirements (ongoing work, paper TBP August 2015, Whitley et al.)
- Dual Habitat Model: Requires 3 SLS Block 2B Launches
- Loiter Habitat Model: Requires 2 SLS Block 2B Launches
! Inser1on-Departure to and from op1mal 1-Sol Orbit is feasible
! Pre-deployment of Mars Stay Assets yet to be addressed (ongoing)
! Sensi1vity studies of Hyperbolic Rendezvous wrt to delays, o-engine performance (ongoing work, paper TBP August 2015, Jedrey et al.) 67
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Thank you
Thanks also to the other members of the NASA JSC-JPL Mars Lite Study Team
John Aitchison Lora Bailey Joe Caram Bret Drake Ricky Jedrey Kent Joosten Stan Love
Fay Mckinney Nathan Strange/JPL
Brenda Ward Ryan Whitley
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