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This month's IEEE GlobalSpec Newsletter Challenge:
An amateur astronomer is certain he has calculated the precise atmospheric re-entry time of a defunct satellite with a decaying orbit, predicting the event will occur exactly two months in the future. In reality, the satellite burns up in the atmosphere over two weeks earlier than predicted. What went wrong in the astronomer’s calculations?
And the answer is:
Predicting the exact timing of satellite re-entry is difficult due to many factors. Several parameters must be known to a high level of accuracy and any uncertainty in these values can create errors in the predicted re-entry time. Yet the most important contributing factor to the orbital decay of a satellite – atmospheric drag – is difficult to model and subject to a number of uncertainties.
Atmospheric drag on a satellite depends on numerous variables, including the shape of the satellite, its size and its spatial orientation (which all have an effect on the effective “drag surface” of the satellite). The density of the atmosphere plays a large role in determining atmospheric drag, and depends on, among other factors: the satellite’s altitude (which is different at the perigee and apogee of an elliptical orbit) and the satellite’s position in any one orbital revolution (the atmosphere is denser on the day-time side of Earth).
Perhaps the most significant source of uncertainty is the changing density of the atmosphere due to solar winds. For instance, during a solar flare, the density of the upper atmosphere increases due to the influx of solar particles. Furthermore, there are periodic variations in the speed of the solar wind as a result of the locations of coronal holes on the sun.
These factors make it challenging to predict exact re-entry times, which is why the astronomer’s forecast turned out to be inaccurate.
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