It can't be shadow of ISS (assuming that ISS is the satelite from where this picture is made) or anything casted on ground/clouds, hundred of
kilometers below. It should transform at some total solar eclipse at the ground/clouds zone.
It is simple: when you are near an object, it is big. When you go further and further, it becames smaller and smaller. We define here as angular size
relative to the point of view.
Whilst the object's angular size eclipsing the sun is bigger than the sun's angular size, we have a total eclipse (no solar light). But when angular
size of the object is smaller than the sun, we have a penumbra situation.
Now, when we are at the ground (or at the clouds, 10 kilometers up or down means nothing relative to the ISS altitude), we see ISS very small, less
than 60 arcseconds, only instruments are able to resolve details. On the other hand, the sun's angular size is about half of degree. MUCH BIGGER than
the ISS. (there are many ISS transits onto the sun/moon, and anybody can google them and see the difference in angular size)
one example:
antwrp.gsfc.nasa.gov...
So, something very small..how much sunlight can block to make some kind of shadow? Virtually zero.
So it is a simple geometrical equation to make an ideea how long the ISS shadow will cast in space.
Assume the ISS is a perfect round object 100 meters in size. Assume you are at the maximum distance when ISS it makes a full eclipse of the sun, so,
it have 0.5 degrees in angular size.
Therefore, the distance is:
100/tan(0.5) = 11500 meters.
We can double this distance, because even when ISS angular size is smaller but comparable to the sun (let's say half), it can produce some kind of
detectable penumbra.
This is theoretically. Practically, the distance is much shorter, simple because ISS is NOT a 100 meters disc, but a much thinner structure. More,
it's shadow will became fuzzy and fuzzy. I feel that the detectable shadow can be casted only maximum a couple of kilometers or so.
NO WAY casting shadow down to the ground/clouds hundred of kilometers away.
Now second solution, another sattellite captured briefly, and maybe by one of the pair of cameras...
Not sure what to say...but there in orbit, satelites have high velocities..about 8 km/sec... So, chances to see another sattelite are smaller because
very brieffly going one "near" the other when having different orbits (near enough to appear with some details in the image), and again to the
smaller exposure time of the image...
When trying to understand this, it became important to know what is the angle of the image captured (or the angular resolution of the camera), to
estimate the distance to the alleged sattelite and to judge if there can be or not some motion blur. If there is some motion blur, in what direction?
i don't think the fuzziness is due to motion blur.
About something really small, debris, it could be real, and it may have share the ISS orbit (being a product of it) enough to appear on that short
exposure time when picture is taken, and posibly appearing a bit unfocused (as fuzziness suggest). More, this debris particle appear dark, maybe
because is in the ISS shadow itself.
[edit on 9/8/09 by depthoffield]
[edit on 9/8/09 by depthoffield]
[edit on 9/8/09 by depthoffield]
[edit on 9/8/09 by depthoffield]