Space Station Viewing Times
The International Space Station can sometimes be seen fom Lincoln. It
appears as a bright star, moving across the sky from West to East, travelling
faster than high flying aircraft and usually brighter than most stars.
A typical flyby looks like this: A dim speck of light -- the ISS --
appears near the horizon. It brightens quickly, then glides leisurely
across the sky, crossing it in 3 to 5 minutes. At its best, the station
can outshine every star and planet except the Sun, the Moon and possibly
Venus. More often it looks like an ordinary star, eye-catching because
it moves (the ISS orbits Earth every 90 minutes at an altitude of 375
km).
There are no bright lights on the outside of the station. It glows by
reflecting sunlight, as much as 90% of the light that hits it. Much of
the ship is covered by a light-colored insulating blanket; other surfaces
are painted white or made of anodized aluminium. Even the awesome solar
arrays, which must absorb sunlight to power the station, aren't completely
black. Their reflectivity is near 35%.

Because the station shines by reflection, we can see it only during
the hours around local sunset or dawn. Those are the times when the sky
above can be dark and, simultaneously, the ISS can be brightly lit by
the rising or setting Sun.
The times are for latitude 53.2°N, 0.5°W and are accurate
to around one minute for the first observation or five minutes for those
near the bottom of the table.
The table is organised as follows:
> Date
> Magnitude: A measure of the brightness of the Space
Station. The lower the figure, the brighter the star.
> Visibility Starts: Time and direction when the Station
becomes visible (or leaves the Earths shadow - morning apparition).
At altitudes below 10 degrees the station is difficult to observe.
Times are UK local time. (BST or GMT depending on the season)
> Max. Altitude: The maximum elevation from the horizon
during visibility
> Visibility Ends: The time and direction when the Station
enters the Earths shadow (evening apparition). It is possible to continue
to observe below 10 degrees but usually only with binoculars.
We are seeking permission from the copyright holder to automatically
import the table directly into this page but in the meantime please
click here for the table on the 'Heavens Above' Website.
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