Main Topic 10: Atmospheric Interaction and Orbital End States

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Last updated 3:22 PM on 4/30/26
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7 Terms

1
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Aerobraking

  • aerodynamic drag

  • orbital energy

____________ is an orbital maneuver in which a spacecraft uses ________ from a planet’s atmosphere to reduce its _______, rather than relying entirely on onboard propulsion.

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<ul><li><p>drag force</p></li><li><p> velocity vector</p></li><li><p>negative work</p></li></ul><p>______________</p><ul><li><p>maneuver</p></li></ul><p></p>
  • drag force

  • velocity vector

  • negative work

______________

  • maneuver

Aerobreaking Considerations

  • This ________ opposes the spacecraft’s ________ and performs

________work.

  • The _________ must be carefully controlled to prevent overheating or

    excessive structural loads. The heat load during an aerobraking pass

    can build up rapidly because: (photo)

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  • Exomars Trace Gas Orbiter

_______________ completes Aerobraking

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  • Orbital decay

    • lower altitude

    • re-entry,

    • Low Earth Orbit (LEO).

___________ is the gradual reduction of a satellite's orbit, leading to ___________ and eventual ________ primarily caused by atmospheric drag in ____________

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  • shape of the satellite

  • 150 km

Aerodynamic drag force

  • The reference area, Aref, and the drag coefficient, CD , in will depend on the exact____________.

  • It is often assumed that in the absence of specific information, then CD = 1 in the very outer regions of the atmosphere in the low-density or rarefied flow, increasing to CD = 2 when approaching an orbital altitude of ____ km.

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  • 10-4 km/s

  • 7.5 km/s

    • ISS

Consequences of orbital decay

  • Typically, satellites in LEO exceeding a radial decay rate of approximately _____ km/s are considered to bein a critical state of orbital decay.

  • For a satellite with Vs approximately___ km/s (similar to the ____ in LEO), a radial decay rate exceeding that threshold could see a significant orbital decay over a relatively short period.

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  • Mach 12

    • aerodynamic friction

  • heat shield

  • blunt body

    • kinetic heating

  • kinetic energy

Atmospheric re -entry

  • High re-entry velocities, which canexceed Mach ____, generate substantial ___________ on the spacecraft, producing heat.

  • So much heat is generated during re-entry that the spacecraft must be equipped with a thermal protection system (TPS), such as a _______, to prevent it from burning up or vaporizing.

  • A ________ is preferred for a re- entry shape, which causses the shock wave to stand off from the spacecraft, reducing _______ and creating high drag.

  • Managing the thermal environment during re-entry is critical, as the spacecraft’s ________ must be dissipated safely.