RS-15's solar elevation from 2007 to 2010

These charts show how RS-15's solar elevation will change over the next few years. Solar elevation is a cheap and cheerful way of estimating the illumination of satellites in near-circular orbits. The dotted red lines show the maximum and minimum angular radius of Earth as seen from the satellite. Above the dotted lines means the satellite is in continuous sunlight; below them every orbit will at some time take the satellite into eclipse, the lower the elevation the longer the eclipses. Between the dotted lines the satellite may be eclipsed depending on the orientation of its perigee relative to the sun.

AO-7 is in a relatively stable orbit, but this model looks so far into the future that it is sure to be affected by decay and other perturbations.

RS-15's solar elevation in 2007.

RS-15's solar elevation in 2007

RS-15's solar elevation in 2008.

RS-15's solar elevation in 2008

RS-15's solar elevation in 2009.

RS-15's solar elevation in 2009

RS-15's solar elevation in 2010.

RS-15's solar elevation in 2010

Document history

2007-11-25: first version.