With the decision by the Russian authorities to de-orbit the 15 year old Mir
space station, there has been much interest in when and where it will come down.
To provide those interested with as much information as possible, we show
above a new graph plotting the orbital height of Mir against time. Clearly visible
are the re-boosts which have ocurred over the last year, and the gradual decay
in between. The height is averaged over one orbit, and the gradual decrease
is caused by atmospheric drag. As can
be seen from the plot, the rate of descent is not constant and this variation is caused by
changes in the density of the tenuous outer atmosphere due mainly to solar activity.
This graph is updated continuously as new orbital data is published by NASA,
and re-entry will occur when the lowest point of the orbit descends to
approximately 100 km. Close to the end, the drag will be much higher because
of the increase in air density at lower altitudes and so Mir will descend
very rapidly in the last few days.
It is notoriously difficult to predict exactly when and where a satellite will
re-enter the atmosphere, especially when the expected re-entry is still several
weeks away. Heavens-Above does not currently attempt to make such predictions,
but Alan Pickup's excellent
Decay Watch page
is a good source. Please note that Alan's predictions assume an uncontrolled
satellite, but the Russians intend to bring down Mir in a controlled
manner in the South Pacific Ocean, so as to minimise risk of pieces landing
on populated areas. Launch of a Progress vehicle to act as a "tug" is expected in
the near future.