02 June 2006

Photographing the International Space Station

Forrest M. Mims III, Editor


The International Space Station (ISS) is so large that the sunlight it reflects toward the Earth is highly visible for an hour or so before sunrise and after sunset.

The Space Station is so bright that it is easily photographed with a camera mounted on a tripod, which is how the images in Figs 1-3 were made.

Figure 1 is a 10-second time exposure that shows the track of the ISS from northwest to southeast over Geronimo Creek Observatory in South-Central Texas, the field from where I have made many thousands of sun and sky measurements since May 1988. The image has been processed to remove noise caused in part by bright moon light.

The stars in the original, unprocessed image are very slightly oblong. This occurred because the camera was fixed and the rotation of the Earth caused a slight apparent motion of the stars even during the brief 10-second time exposure.

Figure 2 is a second 10-second time exposure that shows the ISS as it enters the Earth's shadow and disappears from view. The dimming of the ISS begins as the rays of sunlight that illuminate it begin to graze the top of the atmosphere. The dimming rapidly increases as the rays of sunlight pass through increasingly thicker layers of atmosphere. Figure 3, a cropped version of Fig. 2, shows the dimming effect.

A careful analysis of the intensity of the ISS light trail as it passes into the shadow of the Earth would permit layers of aerosols to be identified. This would make an interesting study should there be another major volcanic eruption that contaminates the stratosphere with particulate matter.

Many kinds of film and digital cameras can be used to photograph the ISS, but a camera with a time exposure capability will provide the best results.

Both Figs. 1 and 2 were acquired using a tiny Casio EX-Z850 8.1 megapixel camera set to its shutter priority mode. The flash was disabled, the ISO was set to 200, and a 10-second time exposure was selected. It was impossible to see the ISS through the camera's tiny viewfinder or on its very bright LCD display. Therefore, the camera, which was mounted on a tripod, was pointed in the general direction of the satellite, and the shutter was released. Six separate exposures were made, and all captured a full ten-second trace.

For information on when the ISS will be visible over your location, see NASA's Human Space Flight web site.


 
Figure 1. The International Space Station passes over Geronimo Creek Observatory at 20:27:04 CST on 11 May 2006 (Casio EX-Z850, ISO 200 for 10 seconds at f2.8). The image has been cropped and background noise has been artificially removed during post processing. Photograph by Forrest M. Mims III.
 
Figure 2. The ISS enters the shadow of the Earth and disappears from view in this cropped image (Casio EX-Z850, ISO 200 for 10 seconds at f2.8). The bright glow at lower left is from the nearly full moon. Some of the background noise caused by moon light has been artificially removed during post processing. Photograph by Forrest M. Mims III.
 
Figure 3. This cropped version of Fig. 2 clearly shows the dimming of the ISS as it enters Earth's shadow and disappears from view. Photograph by Forrest M. Mims III.
   
Copyright 2005 by Society for Amateur Scientists