ASK HN: Can any of you solve this?
zombal.com
zombal.com
The surface area of the entire spherical sky is: 4\piR^2
This can be represented by a spherical integral that I'm not sure I can write cleanly here.
We just need to change the bounds of that integral to find the area of the observable part of that shell. The Intersecting Chord Theorem along with some trigonometry can be used to find these bounds.
The answer I get is:
(1 - cos(x)) / 2 where x = Arctan(sqrt(r(R-r)) / r)
This seems to have the correct asymptotic behavior (as r approaches 0, cos(x) approaches cos(pi/2) = 0, and the answer approaches 50%
EDIT: My previous answer assumed the shapes were cones instead of spheres. Sorry about the confusion.
sin theta = r_earth / (r_earth + altitude)
theta = arcsin( r_earth/(r_earth + altitude))
p_visible = (2pi - 2*theta)/(2pi)
p_visible = 1 - arcsin ( r_earth / (r_earth + altitude))/pi
.
.
Sanity checks:
r_earth = 6378.1 X 1000 m
altitude = 1m
p_visible = .50006
.
altitude = 10^7 m
p_visible = .66766
This fits intuitively: the further away you are from the Earth's surface, the more of the sky you can see without the horizon interfering.
You're not just referring to the percentage of the surface area of a sphere (which earth isn't), atmospheric distribution isn't uniform even if we go by volume (or should we be going by density?), then there's the curvature of light in the atmosphere to take into consideration, and the arbitrary descisions as to what height above sea level our observer is standing at, the variable nature of the tropopause ...
an interesting problem, but likely more interesting as a mental exercise than in actual execution.
Define "The Sky" as an enclosing sphere. When it has the same size as the Earth, the percentage of it you can see is 0. As it gets larger, so the percentage you can see goes to 50%.
What portion of the night sky (constellations) can we see? About 50%
50%, duh.
Draw a circle. Within that circle, with the same center as the first circle, draw a smaller circle. Choose a point on that circle, and draw a tangent line from that point. Now, consider the fact that the portion of the exterior circle between the two intersections the tangent line has to it is not half of the circle.
The same principle applies when expanding to three dimensions: a plain can only divide a sphere in half if it passes through the center of the sphere. When that plain must be tangent to a smaller sphere with the same center, it is only possible to divide the larger sphere in half when the radius of the smaller sphere is zero.
As such, the portion of sky visible from any point on a sphere is less than 50%.