Low Thrust Transfer to Sun-Earth L 1 and L 2 Points with a Constraint on the Thrust Direction LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava,

Slides:



Advertisements
Similar presentations
Nanoparticle Electric Propulsion for Space Exploration Phys 483 Monday, March Team 1: Perry Young, Kiyoshi Masui, Mark Hoidas, Andrew Harris.
Advertisements

The ballistic support of the “SPECTR-RG” spacecraft flight to the L2 point of the Sun-Earth system I.S. Ilin, G.S. Zaslavskiy, S.M. Lavrenov, V.V. Sazonov,
More Satellite Orbits Introduction to Space Systems and Spacecraft Design Space Systems Design.
Solar Imaging Radio Array (SIRA) Trajectory and Formation Analysis Flight Dynamics Analysis Branch Code 595 (572) Dave Folta Bo Naasz Frank.
Comparative Assessment of Human Missions to Mars Damon F. Landau Ph. D. Preliminary Exam September 13, 2005.
Low-thrust trajectory design ASEN5050 Astrodynamics Jon Herman.
Институт прикладной математики им. М.В.Келдыша РАН Keldysh Institute of Applied Mathematics, Russian Academy of Sciences.
 Falcon 9 Heavy › To carry crew capsule and propellant required to rendezvous with transit vehicle Image Credit:
Possible Orbits for the First Russian/Brazilian Space Mission Alexander A. Sukhanov Space Research Institute (IKI) of Russian Academy of Sciences Moscow,
Babakin Space Center, Space Research Insitute, Makeev Rocket Design Bureau COSMOS ONE: THE FIRST SOLAR SAIL a project of The Planetary Society with Cosmos.
07/07/2005 Coupling with PF2012: No existing PF “as is” able to accommodate Karin On going study in France to develop a new generation of PF product line.
1 ESAIL proof of concept mission Juha-Pekka Luntama Pekka Janhunen Petri Toivanen.
NEO Surveyor Thomas M. Randolph Jet Propulsion Laboratory
Principles of Propulsion and its Application in Space Launchers Prof. Dr.-Ing. Uwe Apel Hochschule Bremen REVA Seminar1.
EGR 4347 Analysis and Design of Propulsion Systems
October 1, 2013 John Brophy Jet Propulsion Laboratory California Institute of Technology Pasadena, CA.
AAE450 Spring 2009 Arbitrary Payload Cost Optimization to LLO Tasks: Payload Cost / Mass Optimization (Launch to LLO) Disprove Momentum Transfer Alternative.
The Lander is at a 25 km Lunar altitude and an orbital period of approximately 110 minutes. After separation occurs the Lander is completely self sufficient.
AAE450 Spring 2009 Analysis of Trans-Lunar Spiral Trajectory [Levi Brown] [Mission Ops] February 12,
AAE450 Spring 2009 Final Sizing and Trajectory Design for 100 g/10kg Payloads [Levi Brown] [Mission Ops] March 12,
Project X pedition Spacecraft Senior Design – Spring 2009
Spacecraft Propulsion Dr Andrew Ketsdever Lesson 13 MAE 5595.
Chapter 6: Maneuvering in Space By: Antonio Batiste.
A Comparison of Nuclear Thermal to Nuclear Electric Propulsion for Interplanetary Missions Mike Osenar Mentor: LtCol Lawrence.
28 October st Space Glasgow Research Conference, Glasgow, United Kingdom.
1 Possibilities for Traveling to Mars Charles C. Renn.
Rocket Propulsion Contents: Review Types of Rockets New concept 1 Example 1 Whiteboards 1,2,3Whiteboards123 Concept 2, Example 2Concept 2Example 2 Whiteboards:
Final Version Bob G. Beaman May 13-17, 2002 Micro-Arcsecond Imaging Mission, Pathfinder (MAXIM-PF) Electrical Power System (EPS)
Samara State Aerospace University (SSAU) Samara 2015 SELECTION OF DESIGN PARAMETERS AND OPTIMIZATION TRAJECTORY OF MOTION OF ELECTRIC PROPULSION SPACECRAFT.
Sub-Optimal Solutions for Satellite Orbital Transfers 6th International Workshop and Advanced School 6th International Workshop and Advanced School "Spaceflight.
Optimal Low-Thrust Deorbiting of Passively Stabilized LEO Satellites Sergey Trofimov Keldysh Institute of Applied Mathematics, RAS Moscow Institute of.
Low-Thrust Transfers from GEO to Earth-Moon Lagrange Point Orbits Andrew Abraham Moravian College, 2013.
THE DIURNAL TEMPERATURE REGIME OF THE SURFICIAL REGOLITH OF PHOBOS IN THE LANDING SITE REGION OF THE FOBOS-GRUNT LANDER FOR DIFFERENT SEASONS: THE MODEL.
EXTROVERTSpace Propulsion 12 Electric Propulsion Continued.
© Lavochkin Association, 2013 Ganymede Lander mission overview.
Radiation environment estimates for Europa lander mission M. V. Podzolko 1, I. V. Getselev 1, Yu. I. Gubar 1, I. S. Veselovsky 1,2, A. A. Sukhanov 2 1.
rd Global Trajectory Optimisation Competition Workshop Aula Magna del Lingotto, Turin (Italy), June 27, 2008 © 2008 DEIMOS Space, S.L. –
PLANETARY PROBE LASER PROPULSION CONCEPT 7 TH INTERNATIONAL PLANETARY PROBE WORKSHOP JUNE 2009, BARCELONA LE, T. (1), MOBILIA, S. (2), PAPADOPOULOS,
Spacecraft Trajectories You Can Get There from Here! John F Santarius Lecture 9 Resources from Space NEEP 533/ Geology 533 / Astronomy 533 / EMA 601 University.
VASIMR: The Future of Space Travel (?) Kevin Blondino 8 October 2012.
AAE450 Spring 2009 Support structure for Orbital Transfer Vehicle (OTV) Tim Rebold STRC [Tim Rebold] [STRC] [1]
Space Station Will it be accessible for You and Me?
AAE450 Spring 2009 Preliminary Trans-Lunar Analysis [Levi Brown] [Mission Ops] January 29,
FAST LOW THRUST TRAJECTORIES FOR THE EXPLORATION OF THE SOLAR SYSTEM
What happened to the Mars Climate Explorer in September 1999? By Leslie Palomino.
PARKINSON-SAT EA 469 Spacecraft Design Joe Campbell Thomas Dendinger Greg Lewis Paul Lwin.
Computational Modeling of Hall Thrusters Justin W. Koo Department of Aerospace Engineering University of Michigan Ann Arbor, Michigan
Rocket Propulsion Contents: Review Types of Rockets New concept 1 Example 1 Whiteboards 1,2,3Whiteboards123 Concept 2, Example 2Concept 2Example 2 Whiteboards:
AAE450 Spring 2009 Brian Erson Attitude Control Systems Trans Lunar Phase Alternative Design Comparison [Brian Erson] [Attitude] 1.
FEDERAL SPACE AGENCY OF RUSSIAN FEDERATION LAVOCHKIN ASSOCIATION "PHOBOS-GRUNT" PROJECT MISSION CONCEPT & CURRENT STATUS OF DEVELOPMENT IKI, 13 October.
Ion Energetics of the Modes of the CubeSat Ambipolar Thruster Timothy A. Collard 1, J. P. Sheehan 1, and Alec D. Gallimore 1 1 Aerospace Engineering, University.
TRACKING OF PHOBOS-GRUNT MISSION IN LOW EARTH ORBIT Alexander S. Samotokhin, Andrey G. Tuchin M.V. Keldysh Institute of Applied Mathematics of Russian.
© 2014 Orbital Sciences Corporation. All Rights Reserved. SPRSA Excess Capacity Panel Carol P. Welsch Orbital Sciences Corporation June 10, Welsch.
20c - 1 NASA’s Goddard Space Flight Center Propulsion Chuck Zakrwski NASA/GSFC Code 597 August 16-17, 2005.
Presented by: Jamie Quinnell Jean Moiso Gus Mashensic.
Final Version Gary Davis Robert Estes Scott Glubke Propulsion May 13-17, 2002 Micro Arcsecond X-ray Imaging Mission, Pathfinder (MAXIM-PF)
INFORMATION SUPPORT SYSTEM OF THE SOLAR SAIL MISSION: PRACTICAL ASPECTS. Nazarov, V. 1 ; Gotlib V. 1 ; Lipatov A. 1 ; Bashe, I. 2 ; Korotkov, F. 1 ; Markov,
An Earth – Moon Transportation System Patrick Zeitouni Space Technology.
Newton’s thought experiment: orbital velocity. Surface escape velocities Planet V escape, ft/sec Mercury13,600 Venus33,600 Earth36,700 Moon7,800 Mars16,700.
Cost Comparison of Higher Parking Orbit Scale up for Arbitrary Payload
Deployment Optimization for Various Gravitational Wave Missions
Rocket Propulsion Contents: Review Types of Rockets New concept 1
Technical Resource Allocations
A Parametric Study of Interplanetary Mission Using Solar Sail
Future In-Space Operations (FISO) Telecon Colloquium
Unit D – Space Exploration
Week 6 Presentation Thursday, Feb 19, 2009
Week 4 Presentation Thursday, Feb 5, 2009
Main information on the «WORLD SPACE OBSERVATORY» project
Presentation transcript:

Low Thrust Transfer to Sun-Earth L 1 and L 2 Points with a Constraint on the Thrust Direction LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June, 2002 Alexander A. Sukhanov Natan A. Eismont Space Research Institute (IKI) of Russian Academy of Sciences Moscow, Russia Space Research Institute (IKI) of Russian Academy of Sciences Moscow, Russia

An experimental low-thrust mission to the Sun-Earth L1 and L2 points is considered (Module-M mission) MISSION GOALS Solar wind exploration Magnetic storm prediction Testing new technologies MISSION STEPS Delivery of the spacecraft component to the International Space Station (ISS) by Progress cargo spaceship Assembling the spacecraft at ISS Launch from ISS and transfer to L 1 using Solar Electric Propulsion Transfer to the L 1 point and insertion into a halo orbit Launch from the halo orbit, transfer to L 2 point, and insertion into a halo orbit LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

SPACECRAFT CONCEPT Spacecraft is spin-stabilized with spin axis orthogonal to the Sun Solar arrays form a cylindrical surface coaxial to the spin axis Thrusters are directed along the spin axis in both directions LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

THRUSTER PARAMETERS NameD-38 TypeTAL Power750 W Specific impulse2200 s Efficiency (including loss in PPU)0.5 Thrust force0.035 N Mass flow rate1.6  kg/s Resource3000 hours Propellantxenon LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

SPACECRAFT PARAMETERS Wet initial mass290 kg Xenon mass85 kg Characteristic velocity7.5 km/s Solar panel area110 m 2 Effective solar array area30 m 2 Electric power3 kW Number of thrusters8 Number of simultaneously running thrusters2 Maximum time of the low thrust run7340 hr LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

SPIRAL TRANSFER LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

ORBIT SHADOWING Launch in June-July or December-January minimizes the orbit shadowing down to 7.5 percent of the spiral transfer time These optimal launch dates lead to a high (> 50°) inclination to the ecliptic plane Launch in May or November was selected for the further analysis: the shadowing is 8.5 percent, inclination to the ecliptic plane is 35° LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

PARAMETERS OF THE SPIRAL TRANSFER Time of flight280 days Number of orbits1330 Consumed characteristic velocity6850 m/s Propellant consumption78.9 kg Spacecraft mass211.1 kg LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

TRANSFER TO L 1 AND INSERTION INTO A HALO ORBIT Time of flight (after the spiral)140 days Characteristic velocity of the insertion into halo290 m/s Propellant consumption2.8 kg Spacecraft mass in halo208.3 kg Amplitude A y of the halo orbit62,000 km LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

L 1 TO L 2 TRANSFER WITH ZERO COMPLETE ORBITS 10 LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June, 2002

L 1 TO L 2 TRANSFER WITH ZERO COMPLETE ORBITS Consumed characteristic velocity306 m/s  v 1 50 m/s  v m/s  v 3 60 m/s Time between  v 1 and  v 2 70 days The transfer duration181 days Propellant consumption2.9 kg Final spacecraft mass205.4 kg A y amplitude of the L 2 halo800,000 km LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

L 1 TO L 2 TRANSFER WITH ONE COMPLETE ORBIT 12 LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June, 2002

LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June, L 1 TO L 2 TRANSFER WITH ONE COMPLETE ORBIT Consumed characteristic velocity224 m/s  v 1 65 m/s  v 2 18 m/s  v m/s Time between  v 1 and  v 2 82 days The transfer duration259 days Propellant consumption2.2 kg Final spacecraft mass206.1 kg A y amplitude of the L 2 halo300,000 km

14 L 1 TO L 2 TRANSFER WITH TWO COMPLETE ORBITS LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June, 2002

L 1 TO L 2 TRANSFER WITH TWO COMPLETE ORBITS Consumed characteristic velocity70 m/s  v 1 35 m/s  v 2 2 m/s  v 3 33 m/s Time between  v 1 and  v 2 70 days The transfer duration319 days Propellant consumption0.7 kg Final spacecraft mass207.6 kg A y amplitude of the L 2 halo150,000 km LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

SYMMETRIC TWO-IMPULSE L 1 TO L 2 TRANSFER LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

SYMMETRIC TWO-IMPULSE L 1 TO L 2 TRANSFER Consumed characteristic velocity86 m/s  v 1 43 m/s  v 2 43 m/s The transfer duration307 days Propellant consumption0.8 kg Final spacecraft mass207.5 kg A y amplitude of the L 2 halo62,000 km LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

SUMMARY OF THE TRANSFERS LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,

CONCLUSIONS The low thrust orthogonal to the Sun allows performing: – transfer to L 1 or L 2 Sun-Earth point; – insertion into a halo orbit; – halo-to-halo transfer. This makes it possible to simplify the spacecraft design and control Duration of both the Earth-to-halo and halo-to-halo transfers can be shortened by means of a higher propellant consumption Propellant consumption can be reduced by means of the duration increase for both the Earth-to-halo and halo-to-halo transfers LIBRATION POINT ORBITS AND APPLICATIONS Parador d'Aiguablava, Girona, Spain 10 – 14 June,