To Orbit (Continued) and Spacecraft Systems Engineering Scott Schoneman 13 November 03.
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Transcript of To Orbit (Continued) and Spacecraft Systems Engineering Scott Schoneman 13 November 03.
To Orbit (Continued) To Orbit (Continued) and Spacecraft Systems and Spacecraft Systems
EngineeringEngineering
Scott SchonemanScott Schoneman
13 November 0313 November 03
AgendaAgenda Some brief history - a clockwork universe?Some brief history - a clockwork universe? The BasicsThe Basics
What is really going on in orbit - the popular myth of zero-GWhat is really going on in orbit - the popular myth of zero-G Motion around a single bodyMotion around a single body Orbital elementsOrbital elements Ground tracksGround tracks
PerturbationsPerturbations J2 and gravity modelsJ2 and gravity models DragDrag ““Third bodies”Third bodies”
Orbit PropagationOrbit Propagation
Basic Orbit EquationsBasic Orbit Equations
Circular Orbit Velocity:Circular Orbit Velocity:
Circular Orbit Period:Circular Orbit Period:
Escape Velocity:Escape Velocity:
rvc
rvc
rve
2
3rt
Perturbations: Reality is More Complicated Perturbations: Reality is More Complicated Than Two Body MotionThan Two Body Motion
Orbit PerturbationsOrbit Perturbations
Non-spherical Earth gravity effects (i.e Non-spherical Earth gravity effects (i.e “J-2 Effects”)“J-2 Effects”)Earth is an “Oblate Spheriod” Not a SphereEarth is an “Oblate Spheriod” Not a Sphere
Atmospheric Drag: Even in Space!Atmospheric Drag: Even in Space!““Third” bodiesThird” bodiesOther effectsOther effects
Solar Radiation pressureSolar Radiation pressureRelativistic EffectsRelativistic Effects
J2 Effects - PlotsJ2 Effects - Plots J2-orbit rotation rates are a function of:J2-orbit rotation rates are a function of:
semi-major axissemi-major axis inclinationinclinationeccentricityeccentricity
(Regresses West)(Regresses East)
Applications of J2 EffectsApplications of J2 Effects
Sun-synchronous OrbitsSun-synchronous OrbitsThe regression of nodes matches the Sun’s longitude The regression of nodes matches the Sun’s longitude
motion (360 deg/365 days = 0.9863 deg/day)motion (360 deg/365 days = 0.9863 deg/day)Keep passing over locations at same time of day, same Keep passing over locations at same time of day, same
lighting conditionslighting conditionsUseful for Earth observationUseful for Earth observation
““Frozen Orbits”Frozen Orbits”At the right inclination, the Rotation of Apsides is zeroAt the right inclination, the Rotation of Apsides is zeroUsed for Molniya high-eccentricity communications Used for Molniya high-eccentricity communications
satellitessatellites
Third-Body EffectsThird-Body EffectsGravity from additional objects complicates matters greatlyGravity from additional objects complicates matters greatly
No explicit solution exists like the ellipse does for the 2-body problemNo explicit solution exists like the ellipse does for the 2-body problemThird body effects for Earth-orbiters are primarily due to the Sun and MoonThird body effects for Earth-orbiters are primarily due to the Sun and Moon
Affects GEOs more than LEOsAffects GEOs more than LEOsPoints where the gravity and orbital motion “cancel” each other are called the Points where the gravity and orbital motion “cancel” each other are called the
Lagrange pointsLagrange pointsSun-Earth L1 has been the destination for several Sun-science missions Sun-Earth L1 has been the destination for several Sun-science missions
(ISEE-3 (1980s), SOHO, Genesis, others planned)(ISEE-3 (1980s), SOHO, Genesis, others planned)
Lagrange Points ApplicationLagrange Points ApplicationGenesis Mission:Genesis Mission:
NASA/JPL Mission to collect solar wind samples from outside NASA/JPL Mission to collect solar wind samples from outside Earth’s magnetosphere (Earth’s magnetosphere (http://http://genesismission.jpl.nasa.govgenesismission.jpl.nasa.gov//))
Launched: 8 August 2001Launched: 8 August 2001Returning: Sept 2004Returning: Sept 2004
Third-Body Effects: SlingshotThird-Body Effects: SlingshotA way of taking orbital energy from one body ( a planet ) and giving it to A way of taking orbital energy from one body ( a planet ) and giving it to
another ( a spacecraft )another ( a spacecraft )Used extensively for outer planet missions (Pioneer 10/11, Voyager, Used extensively for outer planet missions (Pioneer 10/11, Voyager,
Galileo, Cassini)Galileo, Cassini)Analogous to Hitting a Baseball: Same Speed, Different DirectionAnalogous to Hitting a Baseball: Same Speed, Different Direction
planet’s orbit velocity
spacecraft incomingto planet
hyperbolic flyby(relative to planet)
spacecraft departing planet
departing sun-centric velocity
incoming sun-centric velocity
Hohmann TransferHohmann Transfer
Hohmann transfer is the most efficient Hohmann transfer is the most efficient transfer (requires the least transfer (requires the least V) between V) between 2 orbit assuming:2 orbit assuming: Only 2 burns allowedOnly 2 burns allowed Circular initial and final orbitsCircular initial and final orbits
Perform first burn to transferPerform first burn to transfer
to an elliptical orbit which just touchesto an elliptical orbit which just touches
both circular orbitsboth circular orbits
Perform second burn to transferPerform second burn to transfer
to final circular GEO orbitto final circular GEO orbit
GEO orbit
GTO orbit
Initial CircularParking
Orbit
Earth-Mars TransferEarth-Mars Transfer
Mars at Spacecraft Arrival
Mars at Spacecraft Departure
• A (nearly) Hohmann transfer to Mars
Atmospheric DragAtmospheric Drag
Along with J2, dominant perturbation for LEO satellitesAlong with J2, dominant perturbation for LEO satellitesCan usually be completely neglected for anything higher Can usually be completely neglected for anything higher
than LEOthan LEOPrimary effects:Primary effects:
Lowering semi-major axisLowering semi-major axisDecreasing eccentricity, if orbit is ellipticalDecreasing eccentricity, if orbit is elliptical
In other words, apogee is decreased much more than In other words, apogee is decreased much more than perigee, though both are affected to some extentperigee, though both are affected to some extent
For circular orbits, it’s an evenly-distributed spiralFor circular orbits, it’s an evenly-distributed spiral
Atmospheric DragAtmospheric Drag Effects are calculated using the same equation used for aircraft:Effects are calculated using the same equation used for aircraft:
To find acceleration, divide by mTo find acceleration, divide by m m / Cm / CDDA : “Ballistic Coefficient”A : “Ballistic Coefficient”
For circular orbits, rate of decay can be expressed simply as:For circular orbits, rate of decay can be expressed simply as:
As with aircraft, determining CAs with aircraft, determining CDD to high accuracy can be tricky to high accuracy can be tricky Unlike aircraft, determining Unlike aircraft, determining is even trickier is even trickier
ACVF D2
2
1
m
ACaa DREV
22
Dragging Down the ISSDragging Down the ISS
Applications of DragApplications of DragAerobraking / aerocaptureAerobraking / aerocapture
Instead of using a rocket, dip into the Instead of using a rocket, dip into the atmosphereatmosphereLower existing orbit: aerobrakingLower existing orbit: aerobrakingBrake into orbit: aerocaptureBrake into orbit: aerocapture
Aerobraking to control orbit first Aerobraking to control orbit first demonstrated with Magellan mission to demonstrated with Magellan mission to VenusVenus
Used extensively by Mars Global Used extensively by Mars Global SurveyorSurveyor
Of course, all landing missions to bodies Of course, all landing missions to bodies with an atmosphere use drag to slow down with an atmosphere use drag to slow down from orbital speed (Shuttle, Apollo return to from orbital speed (Shuttle, Apollo return to Earth, Mars/Venus landers)Earth, Mars/Venus landers)
Reentry Dynamics: Reentry Dynamics: Coming Back to EarthComing Back to Earth
Ballistic ReentryBallistic Reentry SuborbitalSuborbital
Reentry VehiclesReentry Vehicles
OrbitalOrbital Mercury and GeminiMercury and Gemini
Skip EntrySkip Entry ApolloApollo
Gliding EntryGliding Entry ShuttleShuttle
““Systems” EngineeringSystems” Engineering Looking at the “Big” PictureLooking at the “Big” Picture Requirements: What Does the Satellite Need to Do? Requirements: What Does the Satellite Need to Do?
When? Where? How?When? Where? How? Juggling All The PiecesJuggling All The Pieces
Mission Design: Orbits, etc.Mission Design: Orbits, etc. Instruments and PayloadsInstruments and Payloads Electronics and PowerElectronics and Power CommunicationsCommunications MassMass Attitude ControlAttitude Control PropulsionPropulsion Cost and ScheduleCost and Schedule
Mission DesignMission Design Low Earth Orbit (LEO)Low Earth Orbit (LEO)
Earth or Space ObservationEarth or Space Observation International Space Station SupportInternational Space Station Support Rendezvous and ServicingRendezvous and Servicing
Geosynchronous Orbit (GEO)Geosynchronous Orbit (GEO) Communication SatellitesCommunication Satellites Weather SatellitesWeather Satellites Earth and Space ObservationEarth and Space Observation
Lunar and Deep SpaceLunar and Deep Space LunarLunar Inner and Outer PlanetaryInner and Outer Planetary Sun ObservingSun Observing
Spacecraft Design ConsiderationsSpacecraft Design Considerations
Instruments and PayloadsInstruments and Payloads Optical InstrumentsOptical Instruments RF Transponders (Comm. Sats)RF Transponders (Comm. Sats) ExperimentsExperiments
Electronics and PowerElectronics and Power Solar Panels and BatteriesSolar Panels and Batteries Nuclear PowerNuclear Power
CommunicationsCommunications Uplink/DownlinkUplink/Downlink Ground Station LocationsGround Station Locations Frequencies and Transmitter PowerFrequencies and Transmitter Power
Spacecraft Design ConsiderationsSpacecraft Design Considerations(Cont’d)(Cont’d)
Mass PropertiesMass Properties Total MassTotal Mass Distribution of Mass (Moments of Inertia)Distribution of Mass (Moments of Inertia)
Attitude ControlAttitude Control Thrusters: Cold Gas and/or Chemical PropulsionThrusters: Cold Gas and/or Chemical Propulsion Gravity Gradient (Non-Spherical Earth Effect)Gravity Gradient (Non-Spherical Earth Effect) Spin StablizedSpin Stablized Magnetic TorquersMagnetic Torquers
PropulsionPropulsion Orbit Maneuvering and/or Station KeepingOrbit Maneuvering and/or Station Keeping Chemical or ‘Exotic’Chemical or ‘Exotic’ Propellant SupplyPropellant Supply
Spacecraft Design ConsiderationsSpacecraft Design Considerations(Cont’d)(Cont’d)
Cost and ScheduleCost and ScheduleDevelopmentDevelopmentLaunchLaunchMission LifetimeMission Lifetime
1 Month, 1 Year, 1 Decade?1 Month, 1 Year, 1 Decade?
Spacecraft Integration and TestSpacecraft Integration and Test
GPS SatellitesGPS Satellites
Constellation of 24 satellites in Constellation of 24 satellites in 12,000 nm orbits 12,000 nm orbits First GPS satellite launched in 1978First GPS satellite launched in 1978 Full constellation achieved in 1994. Full constellation achieved in 1994.
10 Year Liftetime 10 Year Liftetime Replacements are constantly being Replacements are constantly being
built and launched into orbit. built and launched into orbit.
Weight: ~2,000 pounds Weight: ~2,000 pounds Size: ~17 feet across with the Size: ~17 feet across with the
solar panels extended. solar panels extended. Transmitter power is only 50 Transmitter power is only 50
watts or less. watts or less.
ReferencesReferences Orbit simulation tools: http://www.colorado.edu/physics/2000/applets/satellites.htmlOrbit simulation tools: http://www.colorado.edu/physics/2000/applets/satellites.html
http://home.wanadoo.nl/dms/video/orbit.htmlhttp://home.wanadoo.nl/dms/video/orbit.html
Current satellites in their orbits: Current satellites in their orbits:
NASA “JTRACK”: NASA “JTRACK”: http://liftoff.msfc.nasa.gov/RealTime/Jtrack/3d/JTrack3D.htmlhttp://liftoff.msfc.nasa.gov/RealTime/Jtrack/3d/JTrack3D.html
““Heavens Above” web page: http://www.heavens-above.com/Heavens Above” web page: http://www.heavens-above.com/ Satellite Tool Kit Astronautics Primer: Satellite Tool Kit Astronautics Primer:
http://www.stk.com/resources/help/help/stk43/primer/primer.htmhttp://www.stk.com/resources/help/help/stk43/primer/primer.htm Other orbital mechanics primers: Other orbital mechanics primers:
http://aerospacescholars.jsc.nasa.gov/HAS/Cirr/SS/L2/orb1.htmhttp://aerospacescholars.jsc.nasa.gov/HAS/Cirr/SS/L2/orb1.htm http://www.heavens-above.com/http://www.heavens-above.com/ History of Orbital Mechanics:History of Orbital Mechanics:
http://es.rice.edu/ES/humsoc/Galileo/Things/ptolemaic_system.htmlhttp://es.rice.edu/ES/humsoc/Galileo/Things/ptolemaic_system.html http://es.rice.edu/ES/humsoc/Galileo/Things/copernican_system.htmlhttp://es.rice.edu/ES/humsoc/Galileo/Things/copernican_system.html http://www-gap.dcs.st-and.ac.uk/~history/Mathematicians/Kepler.htmlhttp://www-gap.dcs.st-and.ac.uk/~history/Mathematicians/Kepler.html http://www-gap.dcs.st-and.ac.uk/~history/Mathematicians/Brahe.htmlhttp://www-gap.dcs.st-and.ac.uk/~history/Mathematicians/Brahe.html http://www-gap.dcs.st-and.ac.uk/~history/Mathematicians/Halley.htmlhttp://www-gap.dcs.st-and.ac.uk/~history/Mathematicians/Halley.html http://www-gap.dcs.st-and.ac.uk/~history/Mathematicians/Newton.htmlhttp://www-gap.dcs.st-and.ac.uk/~history/Mathematicians/Newton.html
ReferencesReferences Third-Body EffectsThird-Body Effects
Interplanetary Superhighway Description: Interplanetary Superhighway Description: http://www.cds.caltech.edu/~shane/superhighway/description.htmlhttp://www.cds.caltech.edu/~shane/superhighway/description.html
http://www.wired.com/wired/archive/7.12/farquhar_pr.html "The Art of Falling" - http://www.wired.com/wired/archive/7.12/farquhar_pr.html "The Art of Falling" - about Robert Farquhar, the ISEE-3/ICE trajectory, the NEAR trajectoryabout Robert Farquhar, the ISEE-3/ICE trajectory, the NEAR trajectory
Genesis mission trajectory: Genesis mission trajectory: http://cfa-www.harvard.edu/~hrs/ay45/2001/2and3BodyOrbits.htmlhttp://cfa-www.harvard.edu/~hrs/ay45/2001/2and3BodyOrbits.html
TextsTexts Spacecraft Mission Design, Brown, Charles, (AIAA): a good, compact Spacecraft Mission Design, Brown, Charles, (AIAA): a good, compact
introduction, with lots of handy formula pagesintroduction, with lots of handy formula pages Space Mission Analysis & Design, Larson & Wertz : a good techincal Space Mission Analysis & Design, Larson & Wertz : a good techincal
introduction with lots of practical formulas, charts, and tables introduction with lots of practical formulas, charts, and tables Space Vehicle Design, Griffin and French, (AIAA): Good overview of all facets of Space Vehicle Design, Griffin and French, (AIAA): Good overview of all facets of
space vehiclesspace vehicles Spaceflight Dynamics, Wiesel, W., (McGraw-Hill): Good, readable coverage of Spaceflight Dynamics, Wiesel, W., (McGraw-Hill): Good, readable coverage of
spacecraft designspacecraft design Chobotov, Vladimir: Orbital Mechanics (2nd edition) (AIAA series): Classic, but Chobotov, Vladimir: Orbital Mechanics (2nd edition) (AIAA series): Classic, but
dry and detailed text on many orbital mechanics topicsdry and detailed text on many orbital mechanics topics