Astrogator in STK

Total Page:16

File Type:pdf, Size:1020Kb

Astrogator in STK Astrodynamics (AERO0024) TP1: Introduction Teaching Assistant ⎯ Amandine Denis Contact details Space Structures and Systems Lab (S3L) Structural Dynamics Research Group Aerospace and Mechanical Engineering Department Room: +2/516 (B52 building) [email protected] 04 3669535 2 Today’s program Objectives Presentation of STK Exercise 1: « What does STK do, anyway? » Exercise 2: Do It Yourself! 3 Objectives of this session Discover STK and its possibilities Discover STK interface Discover basic functions and options Illustrate the first lesson 4 Objectives of this session At the end of this session, you should be able to: Create a new scenario Handle graphics windows (2D and 3D, view from/to, …) Use common options of the Properties Browser Insert a satellite in three different ways (database, Orbit Wizard, manually) Insert a facility Calculate a simple access Generate simple reports 5 Presentation of STK Design, analyze, visualize, and optimize land, sea, air, and space systems. 6 Presentation of STK – interface 7 8 9 Presentation of STK 10 11 Presentation of STK – basic elements New scenario - Model the World! Insert object - Populate the World! Properties browser - Decide everything! Animation Reports Tabs 12 Exercise 1 First contact: « What does STK do, anyway? » AGI tutorial Illustration of a Molniya orbit Notion of scenario Rules of thumb Orbit Wizard Insertion of a facility Graphics windows Calculation of a simple access 13 Exercise 1: what does STK do, anyway? Î Are Molniya orbits really a great way to spy on the USA? How many periods of access? When does the first access occur? What is the duration of the first access? Remarks/questions ? 14 Exercise 2 Do It Yourself! : Application to the satellites of the first lesson Insertion of satellites and definition of orbits: • Using Orbit Wizard • Importing from Data Base • Manually Illustration of differents satellites and orbits Options of visualization 15 Exercise 2: application to the 1st lesson >> Represent in STK all the satellites named during the first lesson. To create a satellite: ⇒ Insert >>New… >> Satellite Orbit wizard : cfr ex1 From Database Define properties Visualization: ⇒ Day/night limit ( 2D graphics Properties Browser >> Lighting) 16 Exercise 2: application to the 1st lesson Debriefing: 17 Astrodynamics (AERO0024) TP2: Introduction (2) Today’s program Objectives Exercise 1: A concrete problem Exercise 2: Use in celestial mechanics Exercise 3: Delfi-C3 operation 2 Objectives of this session At the end of this session, you should be able to: Use STK autonomously to solve simple problems Define and use constraints Calculate access Import and visualize planets 3 Exercise 1 A concrete problem: « When could I see the ISS ? » AGI tutorial Outline to build a scenario Constraints 4 Exercise 2 Use in celestial mechanics: The Venus Transit of 2004 AGI tutorial Planets and orbits Insertion of sensors Access calculation (Deck Access) 5 6 7 Exercise 3 Delfi-C3 operations When does the Delfi-C3 team have access to their satellite? When can they operate it? How much does it help if the OUFTI-1 ground station is also used? How long can the two teams communicate through Delfi-C3 transponder ? 8 Astrodynamics (AERO0024) TP3: Orbital elements Today’s program Objectives Exercises 1 & 2: SSO satellites Exercise 3: XMM - RKF7 algorithm 2 Objectives of this session At the end of this session, you should be able to: Calculate orbital elements Check your results with STK Create customized reports Export reports and use data in Matlab 3 Exercise 1 & 2: SSO satellites Ex. 1: Determine the altitude and the inclination of a sun- synchronous satellite for which T=100 min (circular orbit). Use STK to check your results. 4 Exercise 1 & 2: SSO satellites Ex. 2: Determine the perigee and apogee for the following satellite: -SSO - Constant argument of perigee -T = 3h Use STK to check your results. 5 Exercise 3 : XMM - RKF7 algorithm Reproduce graph from Lecture 4, showing time-step of the RKF7(8) algorithm vs true anomaly for XMM satellite. XMM data: Perigee = 7000 km Apogee = 114000 km i = 40° 6 Astrodynamics (AERO0024) TP4: Astrogator Today’s program Objectives Introduction to Astrogator Exercise 1: OUFTI-1 Exercise 2: Hohmann transfer 2 Today’s objectives After this exercise session, you should be able to: design missions involving orbital, impulsive maneuvers This imply that you will be able to: • Use Astrogator when appropriate • Create a simple mission control sequence (MCS) • Use the following segments: ‘initial state’, ‘propagate’, ‘impulsive maneuver’ • Create summaries 3 Today’s program Introduction to Astrogator ⇒ What is it ? ⇒ Components of Astrogator: • Mission Control Sequence • Segments • Stopping conditions Ex.1: OUFTI-1 Ex.2: Hohmann transfer 4 What’s Astrogator? Astrogator is STK’s mission planning module Used for: ⇒ Trajectory design ⇒ Maneuver planning ⇒ Station keeping ⇒ Launch window analysis ⇒ Fuel use studies Derived from code used by NASA contractors Embedded into STK 5 Astrogator in STK Astrogator is one of 11 satellite propagators Propagator generates ephemeris Astrogator satellite acts like other STK satellites ⇒ Can run STK reports (including Access) ⇒ Can animate in 3D and 2D windows Generates ephemeris by running Mission Control Sequence (MCS) Components used in MCS configured in Astrogator Browser 6 Astrogator MissionMission Control Control Sequence Sequence ConfigurationConfiguration Astrogator EphemerisEphemeris Runs Mission Control Sequence OtherOther Mission Mission DataData The Mission Control Sequence A series of segments that define the problem A graphical programming language Two types of segments ⇒ Segments that produce ephemeris ⇒ Segments that change the run flow of the MCS Segments pass their final state as the initial state to the next segment ⇒ Some segments create their own initial state 8 The Mission Control Sequence State Segment 1 Ephemeris State Segment 2 Ephemeris State 9 10 MCS tree 11 MCS toolbar 12 13 14 15 Parameters of the segment currently selected 16 Segments Two types: That produce ephemeris That change the run flow 17 Segments that produce ephemeris Initial State – specifies initial conditions Launch – simulates launching Propagate – integrate numerically until some event Maneuver – impulsive or finite Follow – follows leader vehicle until some event Update – updates spacecraft parameters 18 Initial state segment Specify spacecraft state at some epoch Choose any coordinate system Enter in Cartesian, Keplerian, etc. Enter spacecraft properties: mass, fuel, etc. 19 Launch segment Specify launch and burnout location Specify time of flight Use any central body Connects launch and burnout points with an ellipse Creates its own initial state 20 Propagate segment Numerically integrates using chosen propagator Propagator can be configured in Astrogator browser Propagation continues until stopping conditions are met 21 Stopping conditions Define events on which to stop a segment Stop when some “calc object” reaches a desired value ⇒ A calc object is any calculated value, such as an orbital element ⇒ Calc objects can be user-defined 22 Stopping conditions Can also specify constraints: ⇒ Only stop if another calc object is =, <, >, some value ⇒ Determines if exact point stopping condition is met, then checks if constraints are satisfied ⇒ Multiple constraints behave as logical “And” Segments can have multiple stopping conditions ⇒ Stops when the first one is met ⇒ Behaves as a logical “Or” 23 Stopping conditions Multiple conditions : «OR» Constraints : « AND » 24 Maneuver segment Maneuver segment owns two distinct segments: ⇒ Finite maneuver ⇒ Impulsive maneuver Combo box controls which one is run Finite maneuver created from impulsive maneuver with “Seed” button 25 Impulsive maneuver Adds delta-V to the current state Can specify magnitude and direction of delta-V Computes estimated burn duration and fuel usage, based on chosen engine Can configure engine model in Astrogator browser 26 Impulsive maneuver State Impulsive Maneuver Add delta-V to state State 27 Finite maneuver Works like propagate segment, thrust added to force model Can specify the direction of the thrust vector ⇒ Can be specified in plug-in Magnitude of thrust comes from engine model 28 Follow segment Choose leader to follow Specify offset from the leader Follow leader between “joining conditions” and “separation conditions” ⇒ Behave just like stopping conditions Creates its own initial state 29 Update segment Used to update spacecraft properties Useful to simulate stage separation, docking, etc Set properties to a new value, or add or subtract from their current value 30 Update segment State Update Update state parameters State 31 Segments that change run flow Auto-Sequences – called by propagate segments Target Sequence – loops over segments, changing values until goals are met Backwards Sequence – changes direction of propagation Return – exits a sequence Stop – stops computation 32 Auto-sequences Automatic sequence browser Instead of stopping a segment, stopping conditions can trigger an auto-sequence An auto-sequence is another sequence of segments ⇒ Behaves like a subroutine After the auto-sequence is finished, control returns to the calling segment Auto-sequences can inherit stopping conditions from the calling segment 33 Auto-sequences example Initial State Propagate Apoapsis Duration = 1 day Periapsis Burn In Plane Burn Out Of Plane Sequence Sequence
Recommended publications
  • Machine Learning Regression for Estimating Characteristics of Low-Thrust Transfers
    MACHINE LEARNING REGRESSION FOR ESTIMATING CHARACTERISTICS OF LOW-THRUST TRANSFERS A Thesis Presented to The Academic Faculty By Gene L. Chen In Partial Fulfillment of the Requirements for the Degree Master of Science in the School of Aerospace Engineering Georgia Institute of Technology May 2019 Copyright c Gene L. Chen 2019 MACHINE LEARNING REGRESSION FOR ESTIMATING CHARACTERISTICS OF LOW-THRUST TRANSFERS Approved by: Dr. Dimitri Mavris, Advisor Guggenheim School of Aerospace Engineering Georgia Institute of Technology Dr. Alicia Sudol Guggenheim School of Aerospace Engineering Georgia Institute of Technology Dr. Michael Steffens Guggenheim School of Aerospace Engineering Georgia Institute of Technology Date Approved: April 15, 2019 To my parents, thanks for the support. ACKNOWLEDGEMENTS Firstly, I would like to thank Dr. Dimitri Mavris for giving me the opportunity to pursue a Master’s degree at the Aerospace Systems Design Laboratory. It has been quite the experience. Also, many thanks to my committee members — Dr. Alicia Sudol and Dr. Michael Steffens — for taking the time to review my work and give suggestions on how to improve - it means a lot to me. Additionally, thanks to Dr. Patel and Dr. Antony for helping me understand their work in trajectory optimization. iv TABLE OF CONTENTS Acknowledgments . iv List of Tables . vii List of Figures . viii Chapter 1: Introduction and Motivation . 1 1.1 Thesis Overview . 4 Chapter 2: Background . 5 Chapter 3: Approach . 17 3.1 Scenario Definition . 17 3.2 Spacecraft Dynamics . 18 3.3 Choice Between Direct and Indirect Method . 19 3.3.1 Chebyshev polynomial method . 20 3.3.2 Sims-Flanagan method .
    [Show full text]
  • Astrodynamics
    Politecnico di Torino SEEDS SpacE Exploration and Development Systems Astrodynamics II Edition 2006 - 07 - Ver. 2.0.1 Author: Guido Colasurdo Dipartimento di Energetica Teacher: Giulio Avanzini Dipartimento di Ingegneria Aeronautica e Spaziale e-mail: [email protected] Contents 1 Two–Body Orbital Mechanics 1 1.1 BirthofAstrodynamics: Kepler’sLaws. ......... 1 1.2 Newton’sLawsofMotion ............................ ... 2 1.3 Newton’s Law of Universal Gravitation . ......... 3 1.4 The n–BodyProblem ................................. 4 1.5 Equation of Motion in the Two-Body Problem . ....... 5 1.6 PotentialEnergy ................................. ... 6 1.7 ConstantsoftheMotion . .. .. .. .. .. .. .. .. .... 7 1.8 TrajectoryEquation .............................. .... 8 1.9 ConicSections ................................... 8 1.10 Relating Energy and Semi-major Axis . ........ 9 2 Two-Dimensional Analysis of Motion 11 2.1 ReferenceFrames................................. 11 2.2 Velocity and acceleration components . ......... 12 2.3 First-Order Scalar Equations of Motion . ......... 12 2.4 PerifocalReferenceFrame . ...... 13 2.5 FlightPathAngle ................................. 14 2.6 EllipticalOrbits................................ ..... 15 2.6.1 Geometry of an Elliptical Orbit . ..... 15 2.6.2 Period of an Elliptical Orbit . ..... 16 2.7 Time–of–Flight on the Elliptical Orbit . .......... 16 2.8 Extensiontohyperbolaandparabola. ........ 18 2.9 Circular and Escape Velocity, Hyperbolic Excess Speed . .............. 18 2.10 CosmicVelocities
    [Show full text]
  • Orbital Fueling Architectures Leveraging Commercial Launch Vehicles for More Affordable Human Exploration
    ORBITAL FUELING ARCHITECTURES LEVERAGING COMMERCIAL LAUNCH VEHICLES FOR MORE AFFORDABLE HUMAN EXPLORATION by DANIEL J TIFFIN Submitted in partial fulfillment of the requirements for the degree of: Master of Science Department of Mechanical and Aerospace Engineering CASE WESTERN RESERVE UNIVERSITY January, 2020 CASE WESTERN RESERVE UNIVERSITY SCHOOL OF GRADUATE STUDIES We hereby approve the thesis of DANIEL JOSEPH TIFFIN Candidate for the degree of Master of Science*. Committee Chair Paul Barnhart, PhD Committee Member Sunniva Collins, PhD Committee Member Yasuhiro Kamotani, PhD Date of Defense 21 November, 2019 *We also certify that written approval has been obtained for any proprietary material contained therein. 2 Table of Contents List of Tables................................................................................................................... 5 List of Figures ................................................................................................................. 6 List of Abbreviations ....................................................................................................... 8 1. Introduction and Background.................................................................................. 14 1.1 Human Exploration Campaigns ....................................................................... 21 1.1.1. Previous Mars Architectures ..................................................................... 21 1.1.2. Latest Mars Architecture .........................................................................
    [Show full text]
  • Method for Rapid Interplanetary Trajectory Analysis Using Δv Maps with Flyby Options
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by DSpace@MIT METHOD FOR RAPID INTERPLANETARY TRAJECTORY ANALYSIS USING ΔV MAPS WITH FLYBY OPTIONS TAKUTO ISHIMATSU*, JEFFREY HOFFMAN†, AND OLIVIER DE WECK‡ Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA. Email: [email protected]*, [email protected]†, [email protected]‡ This paper develops a convenient tool which is capable of calculating ballistic interplanetary trajectories with planetary flyby options to create exhaustive ΔV contour plots for both direct trajectories without flybys and flyby trajectories in a single chart. The contours of ΔV for a range of departure dates (x-axis) and times of flight (y-axis) serve as a “visual calendar” of launch windows, which are useful for the creation of a long-term transportation schedule for mission planning purposes. For planetary flybys, a simple powered flyby maneuver with a reasonably small velocity impulse at periapsis is allowed to expand the flyby mission windows. The procedure of creating a ΔV contour plot for direct trajectories is a straightforward full-factorial computation with two input variables of departure and arrival dates solving Lambert’s problem for each combination. For flyby trajectories, a “pseudo full-factorial” computation is conducted by decomposing the problem into two separate full-factorial computations. Mars missions including Venus flyby opportunities are used to illustrate the application of this model for the 2020-2040 time frame. The “competitiveness” of launch windows is defined and determined for each launch opportunity. Keywords: Interplanetary trajectory, C3, delta-V, pork-chop plot, launch window, Mars, Venus flyby 1.
    [Show full text]
  • Imp-C Orbit and Launch Time Analysis
    IMP-C ORBIT AND LAUNCH TIME ANALYSIS BY STEPHEN J. PADDACK / I BARBARA E. SHUTE Nb 5 72614 I I GPO PRICE $ - IACCESSION NUMBER) (THRUI OTS PRICE(S) $ HA / ~PAoIih .(CODE1 7mx 3-TZ-P -'-so Hard copy (HC) % (NASA CR OR TMX OWAD NUMBER) (CATEOORY) 3#8 I j .. Microfiche (MF) JANUARY 1965 1 -GODDARD SPACE FLIGHT CENTER - GREENBELT, MARYLAND \ X-643 -6 5-40 IMP-c ORBIT AND LAUNCH TIME ANALYSIS Stephen J. Paddack and Barbara E. Shute Special Projects Branch Theoretical Division January 1965 Goddard Space Flight Center Greenbelt, Maryland TABLE OF CONTENTS -Page Abstract.. ........................................ vii NOMENCLATURE ................................... viii INTRODUCTION .................................... 1 I. ASSUMPTIONS .................................. 2 A. Nominal Initial Orbits ........................... 2 B. Dispersions on Initial Conditions .................... 4 C. Restraints on Launch Time ....................... 4 It. COMPUTING TECHNIQUES AND PROGRAMS ............. 7 A. ITEM ...................................... 7 B. Launch Window Program ......................... 7 C. Analog Stability Program ......................... 8 D. Program Comparison ........................... 8 E. Selection of Mean Elements ....................... 8 III. LAUNCH WINDOW MAPS.. ......................... 9 A. Yearsurvey ................................. 9 1. Lifetime Boundary ........................... 10 2. Spacecraft Restraints Boundary .................. 10 B. DetailedMap ................................. 11 IV. SPACECRAFT DATA.............................
    [Show full text]
  • Spacecraft Conjunction Assessment and Collision Avoidance Best Practices Handbook
    National Aeronautics and Space Administration National Aeronautics and Space Administration NASA Spacecraft Conjunction Assessment and Collision Avoidance Best Practices Handbook December 2020 NASA/SP-20205011318 The cover photo is an image from the Hubble Space Telescope showing galaxies NGC 4038 and NGC 4039, also known as the Antennae Galaxies, locked in a deadly embrace. Once normal spiral galaxies, the pair have spent the past few hundred million years sparring with one another. Image can be found at: https://images.nasa.gov/details-GSFC_20171208_Archive_e001327 ii NASA Spacecraft Conjunction Assessment and Collision Avoidance Best Practices Handbook DOCUMENT HISTORY LOG Status Document Effective Description (Baseline/Revision/ Version Date Canceled) Baseline V0 iii NASA Spacecraft Conjunction Assessment and Collision Avoidance Best Practices Handbook THIS PAGE INTENTIONALLY LEFT BLANK iv NASA Spacecraft Conjunction Assessment and Collision Avoidance Best Practices Handbook Table of Contents Preface ................................................................................................................ 1 1. Introduction ................................................................................................... 3 2. Roles and Responsibilities ............................................................................ 5 3. History ........................................................................................................... 7 USSPACECOM CA Process .............................................................
    [Show full text]
  • Launch Conjunction Assessment Handbook Version 1.0  December 2018
    JFSCC, 18th Space Control Squadron Combined Space Operations Center (CSpOC) Vandenberg Air Force Base, California, USA Tel +1-805-605-3533 www.space-track.org LAUNCH CONJUNCTION ASSESSMENT HANDBOOK VERSION 1.0 DECEMBER 2018 18 SPCS Process for Launch Conjunction Assessment TABLE OF CONTENTS Contents Revision History _________________________________________________________________________________________ 1 Important Definitions ___________________________________________________________________________________ 2 18th Space Control Squadron ____________________________________________________________________________________2 Launch Conjunction Assessment _________________________________________________________________________________2 Launch Collision Avoidance ______________________________________________________________________________________2 General Pertubations _____________________________________________________________________________________________2 Special Pertubations ______________________________________________________________________________________________2 Launch Conjunction Assessment Authorities __________________________________________________________ 3 Air Force Instruction 91-217 Space Safety And Mishap Prevention Program ________________________________3 Title 14 Code of Federal Regulations (14 CFR)__________________________________________________________________3 USSTRATCOM SSA Sharing Program _____________________________________________________________________________3 Space-Track.org____________________________________________________________________________________________________4
    [Show full text]
  • Technical Constraints Impact on Mission Design to the Collinear Sun-Earth Libration Points
    1 Technical Constraints Impact on Mission Design to the Collinear Sun-Earth Libration Points N. Eismont, A. Sukhanov, V. Khrapchenkov Space Research Institute, Russian Academy of Sciences ABSTRACT For the practical realization of the mission to the collinear Sun-Earth libration points technical constraints play a significant role. In the paper the influence of the constraints generated by the use of piggi-back mode of the delivering spacecraft to the vicinity of libration points are studied. High elliptical parking orbit of Molniya is taken as initial orbit for start to the L1, L2 libration points. The parameters of this orbit are supposed to be fixed and determined by the main payload demands. The duration of the passenger payload keeping on the mentioned 12 hours period orbit is limited for the case when launcher upper stage is used for the velocity impulse applying to put spacecraft onto transfer orbit to the libration point. The possibility to use one axis attitude control of the spacecraft for the executing correction maneuvers are investigated, supposing that spacecraft is spin stabilized with the spin axis directed to the Sun and maneuver impulse goes along this axis. The cost of constraints is presented in terms of characteristic velocity and time of transfer to the libration point vicinity. The goal of the paper is to understand the possibility of using regular launches of Molniya communication satellite by Soyuz-Fregat launch vehicle for sending low cost scientific spacecraft to Sun-Earth libration points. INTRODUCTION The mission to the vicinity of Sun-Earth collinear libration points are fulfilled and planned for the scientific experiments gaining big advantages from use of this region of space for optimal measurement conditions.
    [Show full text]
  • Determination of Close Approaches for Earth-Fixed Launch Trajectories
    AAS-98-134 DETERMINATION OF CLOSE APPROACHES FOR EARTH-FIXED LAUNCH TRAJECTORIES James Woodburn= The deployment of large constellations of satellites in Low Earth Orbit increases the probability of close approaches with newly launched satellites. A new algorithm for determining launch window blackout intervals based on the avoidance of close approaches for launch trajectories which are fixed relative to the Earth Fixed coordinate system is presented. This algorithm is more robust than the technique of performing close approach analyses by sampling the launch window and significantly more efficient. The example case presented shows an improvement in efficiency by a factor of 200 while detecting blackout intervals as small as 0.3 seconds in duration. INTRODUCTION As the number of objects in orbit about the Earth increases, the determination of close approaches between objects is becoming an increasingly important aspect of satellite operations. A recent study by Jenkins and Schumacher 1 indicates the growing importance of close approach prediction for the Shuttle and the Mir space station. The basic problem is to determine when two objects will have a conjunction where the risk of collision is unacceptably large. There are many ways of defining what constitutes risk. These definitions range in complexity from the specification of a minimum allowable separation distance between the two objects to using complex probability density functions to determine the statistical probability of collision during a conjunction. Prior studies of the close approach problem have focused on the case where all objects are assumed to be in orbit about the Earth and the nominal ephemeris of the objects is known.
    [Show full text]
  • Overview of the Esa Jovian Technology Reference Studies
    DOCUMENT OVERVIEW OF THE ESA JOVIAN TECHNOLOGY REFERENCE STUDIES prepared by/préparé par Alessandro Atzei, Arno Wielders, Anamarija Stankov, Peter Falkner reference/réference SCI-AP/2004/TN-085/AA issue/édition 3 revision/révision 0 date of issue/date d’édition 30/03/07 status/état Final Document type/type de document Technical Note SCI-AP a ESTEC Jovian Studies Overview Keplerlaan 1 - 2201 AZ Noordwijk - The Netherlands April_2_04_07 .doc Tel. (31) 71 5656565 - Fax (31) 71 5656040 Overview of the ESA Jovian Technology Reference Studies issue 3 revision 0 - 30/03/07 page 2 of 148 APPROVAL Title Overview of the ESA Jovian Technology Reference Studies issue 3 revision 0 titre issue revision author Alessandro Atzei, Arno Wielders, Anamarija Stankov, Peter date 30/03/07 auteur Falkner date approved by date approuvé by date Overview of the ESA Jovian Technology Reference Studies issue 3 revision 0 - 30/03/07 page 3 of 148 T ABLE O F C ONTENTS INTRODUCTION .....................................................................................................................................................7 Technology reference Studies....................................................................................................................7 Purpose of this document...........................................................................................................................7 STUDYING THE JOVIAN SYSTEM ..........................................................................................................................9
    [Show full text]
  • Analysis of Launch Windows for Representative Mars
    TECHNICAL NASA TM X-1651 MEMORANDUM N Qc3 (ACCESSION NUMBER! < ANALYSIS OF LAUNCH WINDOWS CnnnKI'l\wlrl PTRCTTTbAl.LUU YA AR=A- ORBITS FOR REPRESENTATIVE MARS MISSIONS NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WASHINGTON, D. C. SEPTEMBER 1968 NASA TM X-1651 b ANALYSIS OF LAUNCH WINDOWS FROM CIRCULAR ORBITS FOR REPRESENTATIVE MARS MISSIONS By Larry A. Manning, Byron L. Swenson, and Jerry M. Deerwester NASA Headquarters Mission Analysis Division Moffett Field, Calif. NATIONAL AERONAUTICS AND SPACE ADMINISTRATION ~ ~~ For sale by the Clearinghouse for Federal Scientific and Technical lnformotion Springfield, Virginia 22151 - CFSTI price $3.00 TABLE OF CONTENTS Page swm ................................ 1 INTRODUCTION ............................. 2 M!ITHOD OF ANALYSIS .......................... 3 Orbit Geometry ........................... 3 # Impulsive Analysis ......................... 4 Plane-Change Modes ......................... 5 MISSION SELECTION CRITERLA ...................... a WRICALANALYSIS ........................... 10 EarthLaunchWindow ......................... 10 MarsLaunchWindov ......................... 11 Mission Profile Reselection ..................... 13 Sensitivity of Velocity Requirements ................ 14 CONCLUSIONS .............................. 15 APPENDIX A - THREE-IMPULSE ANALYSIS .................. 17 APPENDIX B - EXRTH DEPARTURE REQUI-S ............... 20 APPENDIX C - MARS DEPARTLTRF: R?3QUIMTS . * - . - . - * 21 APPENDIXD-NOTATION. ........................ 22 REFERENCES .............................. 24
    [Show full text]
  • SSO−A Space Station STA 05/23/18 1
    Approved by OMB 3060−0678 Date & Time Filed: May 23 2018 2:04:15:700PM File Number: SAT−STA−20180523−00042 Callsign: FEDERAL COMMUNICATIONS COMMISSION APPLICATION FOR SPACE STATION SPECIAL TEMPORARY AUTHORITY FOR OFFICIAL USE ONLY APPLICANT INFORMATION Enter a description of this application to identify it on the main menu: SSO−A space station STA 05/23/18 1. Applicant Name: Spaceflight, Inc. Phone Number: (425) 478−2848 DBA Name: Fax Number: Street: 1505 Westlake Ave. North, Ste 600E−Mail: KristinaH@SpaceflightIndustries. com City: Seattle State: WA Country: USA Zipcode: 98109 − Attention:Kristina Hloptsidis 1 2. Contact Name: Jonathan L. Wiener Phone Number: 703−216−9224 Company:Goldberg Godles Wiener & Wright Fax Number: LLP Street: 1025 Connecticut Ave, NW E−Mail: [email protected] Ste 1000 City: Washington State: DC Country: USA Zipcode: 20036−2413 Attention: Relationship: Legal Counsel (If your application is related to an application filed with the Commission, enter either the file number or the IB Submission ID of the related application. Please enter only one.) 3. Reference File Number or Submission ID 4a. Is a fee submitted with this application? If Yes, complete and attach FCC Form 159.If No, indicate reason for fee exemption (see 47 C.F.R.Section 1.1114). Governmental Entity Noncommercial educational licensee Other(please explain): 4b. Fee ClassificationCXW − Space Station (Non−Geostationary) 5. Type Request Change Station Location Extend Expiration Date Other 6. Temporary Orbit Location 7. Requested Extended Expiration Date 2 8. Description(If the complete description does not appear in this box, please go to the end of the form to view it in its entirety.) Spaceflight Inc.
    [Show full text]