international colloquium and workshop “ganymede lander: scientific goals and experiments”
DESCRIPTION
Golubev Yu.F., Grushevskii A.V., Koryanov V.V., Tuchin A.G. [email protected] A Method of Orbits Designing Using Gravity Assist Maneuvers to the Landing on the Jovian’s Moons. International Colloquium and Workshop “Ganymede Lander: scientific goals and experiments” - PowerPoint PPT PresentationTRANSCRIPT
Golubev Yu.F., Grushevskii A.V.,Koryanov V.V., Tuchin A.G.
A Method of Orbits Designing Using Gravity Assist Maneuvers to the Landing on the
Jovian’s Moons
International Colloquium and Workshop“Ganymede Lander: scientific goals and experiments”
Moscow, Russia, 4-8 March 2013
Keldysh Institute of Applied MathematicsRussian Academy of Sciences
CB-Classic Billiard
Duplex ShuttingCGB-Classic Gravitational Billiard
3D-gravity assist maneuver
Picture from: Barrabéz E., Gómez G., Rodríguez-Canabal J. Notes for the gravitational assistedtrajectories. // Advanced topics in astrodynamics. Summer course. Barcelona, July 2004.
ESA- JUICE MISSION
ESA- JUICE Mission Endgame
Ganymede Flyby-JOI-G&C-Flyby Sequence
Roscosmos part: Ganymede Landing
Flexible JOI Data Flexible G&C-Flyby Sequence GOI Ganymede Circular Orbit Landing
Roscosmos part: Ganymede Landing. Resonance beginning. Typical scenario
ESTK complex of Keldysh IAM RAS Ballistic CenterNavigation and Ancillary Information Facility (NAIF) - NASARefined Flyby Model
Moon Orbital period of SC after the satellite flyby rated to satellite’s orbital period
Number of rounds after a flyby
Ganymede 6 1Ganymede 5 2Ganymede 4 1Ganymede 3 1Ganymede 2.5 2Ganymede 2 1
Joining to Jovian System After Interplanetary Part
Time of Jovian sphere of action2029/06/03 09:25:10 UTC
Flyby hyperbola ( J2000) Semimajor axe, km 5252.572592 Eccentricity 1.163115 Inclination 23.44 grad V-Infinity, km/s 4.91 Pericenter Time 2029/08/29 17:20:35 UTC Pericenter altitude 12.5 RJ
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RADIATION HAZARD PROBLEM (M. Podzolko e.a., SINP MSU Data)
Quasi-Singularity of the Radiation Hazard
Typical radiation hazard analysis on the ENDGAME phase
Dynamics of the radiation accumulation
Typical radiation hazard analysis on the ENDGAME phase
Dynamics of the radiation accumulation- zoom scale
Dynamics of the radiation accumulation- on one orbit. Quasi-singularity
Period after flyby of GANYMEDE 42.9 daysDistance in pericenter rated to Jupiter’s radius 11.5Distance in apocenter rated to Jupiter’s radius 98.0
Tisserand-Poincare graph(by N.Strange, J.Sims, Kevin W.Kloster, James M.Longuski e.a.)
The V∞ Globe (from Russel, Strange et al. (2007))
Representsall possibleV∞vector tips after a fly-by
JUICE Tisserand-Poincare graph type
Pareto front of Tisserand Graph for the Roscosmos Laplace mission
Pareto front trees of Tisserand graphfor Russian Laplace mission
Research basement
Orbit correction algorithm preceding spacecraft’s Jovian moons gravity assists
Gravity assists refined model ESTK KIAM RAS Ballistic centre
complex Navigation and Ancillary Information
Facility (NAIF) - NASA ephemeris — will be refined during JUICE by ESA
Fly-by sequence selection strategy Lambert problem solution; The phase-beams method; Delta V minimizations; Gravity-assist parameters permanent
corrections; Simulations results are presented.
Gravity-assist sequence. Effective Type T1
Low-radiation sequence type T2
Type: Hyper-low-radiation,Expensive Delta V T3
Using PHASE BEAM method of Gravity Assists Sequences Determination
Virtual Trajectories Splitting After Swing-by
Applications for Another Kinds of Flybys
Callisto & Ganymede
Tour design problem lends itself well to optimization schemes
Callisto & Ganymede assists us to minimize fuel requirements