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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.

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)
Exomars Trace Gas Orbiter
_______________ completes Aerobraking
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 ____________
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.
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.
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.