To see both poles simultaneously, the satellite must be on Earth's equatorial plane (Elektro-L does oscillates about this plane a little bit).neufer wrote:BDanielMayfield wrote:
The Sun illuminated both poles on the date the APOD was taken, but the view doesn’t extend clear to both poles because the satellite isn’t high enough. Since the Earth’s radius is 6,378 and the satellite (and all others in geostationary orbits) is 42,164 km from the Earth’s center the maximum latitude visible would be ~ 90 - arctan (6378/42164) = 81.4 deg.
- How about 90 - arcsin(6378/42164) = 81.3 deg
The same height the geostationary satellite need to be to see either pole.BDanielMayfield wrote:
Extra point question: How high would the satellite need to be to actually see both poles?
The simple no-atmosphere answer is infinity. The tangent planes at both poles would be parallel assuming a perfect sphere and they would only intersect at infinity. However, with the atmosphere, refraction allows for a finite distance away to see both poles.
Assuming a nominal refraction model, stars that are just visible on the horizon are actually ≈0.7° below. Using 0.7°, then the minimum distance to where both poles just become visible = 6378km/tan(0.7°) = 522,020 km, or ~1.36 x the moons orbital radius.
So it is also the case that during several days about an equinox, the sun is visible from both poles - only about 1/2° above the horizon (on a clear day of course).