The astronomers of Planet Xiddler are back at it. They have developed a new technology for measuring the radius of a planet by analyzing its cross sections.
And so, they launch a satellite to study a newly discovered, spherical planet. The satellite sends back data about three parallel, equally spaced circular cross sections which have radii A, B and C megameters, with 0<A<B<C. Based on these values, the scientists calculate the radius of the planet is R megameters. To their astonishment, they find that A, B, C and R are all whole numbers!
What is the smallest possible radius of the newly discovered planet?
Let's first discuss the method to the Xiddlerian algorithmic madness. Setting up a reference frame, let's assume that we rotate the newly discovered planet so that the cross sections are parallel to the xy-plane and that the smallest cross section has the largest value of z, at say z=k. Let's additionally assume that the equal distance between each cross section is h for some 0<h<R. Then we have the following system of equations: A2+k2=R2B2+(k−h)2=R2C2+(k−2h)2=R2 where 0<h<k<R are unknown.
By taking the difference between the first two equations we get the hyperbola (k−h)2−k2+B2−A2=h2−2kh+B2−A2=0 or equivalently h=k±√k2−B2+A2. Naturally, since we want h<k, we need to choose the lower branch of the hyperbola, that is h1(k)=k−√k2−B2+A2. Similarly, by taking the difference between the first and last equations, we get the hyperbola (k−2h)2−k2+C2−A2=4h2−4kh+C2−A2=0 or equivalently h=k±√k2−C2+A22. Here, again, we can safely choose the lower branch since otherwise we are not guaranteed to have (k−2h)2<(k−h)2 (which is equivalent to B<C), that is h2(k)=k−√k2−C2+A22.
The intersection of these two curves occurs when k=2√k2−B2+A2−√k2−C2+A2. Squaring both sides gives k2=4(k2−B2+A2)−4√k2−B2+A2√k2−C2+A2+(k2−C2+A2), or equivalently 4√k2−B2+A2√k2−C2+A2=4k2−4(B2−A2)−(C2−A2). Squaring both sides again gives 16(k2−B2+A2)(k2−C2+A2)=(4k2−4(B2−A2)−(C2−A2))2 or equivalently 0=16k4−16((B2−A2)+(C2−A2))k2+(A2−B2)(C2−A2)−16k4+8(4(B2−A2)+(C2−A2))k2+(4(B2−A2)+(C2−A2))2=8(2(B2−A2)−(C2−A2))k2−(4(B2−A2)+(C2−A2))2+16(C2−A2)(B2−A2)=8(2(B2−A2)−(C2−A2))k2−(4(B2−A2)−(C2−A2))2. That is, k2=(4(B2−A2)−(C2−A2))28(2(B2−A2)−(C2−A2))=(4B2−3A2−C2)28(2B2−A2−C2) and hence R2=A2+k2=A2+(4B2−3A2−C2)28(2B2−A2−C2)=8A2(2B2−A2−C2)+(4B2−3A2−C2)28(2B2−A2−C2)=B2+(C2−A2)28(2B2−A2−C2) That is, R=R(A,B,C)=√B2+(C2−A2)28(2B2−A2−C2).
So we can just about start hunting and pecking for suitable triples (A,B,C)∈N3 such that R∈N, but we can narrow the search by including 0<A<B<C<R. Additionally, since k2 must be a positive integer we must additionally have 8∣(C2−A2)2 and 2B2−A2−C2>0. The first conclusion is equivalent to the condition that A≡Cmod2, while the second conclusion ensures that we must have C<√2B2−A2. After a while of hunting an pecking, we see that (2,7,8) yields R(A,B,C)=8. An exhaustive search of triples A<B<C<8 with A≡Cmod2 and C<√2B2−A2 reveals only four valid competitors: (1,4,5)⇒R(1,4,5)=4√7(1,6,7)⇒R(1,6,7)=6√16511(2,5,6)⇒R(2,5,6)=5√224(3,6,7)⇒R(3,6,7)=4√1547 Since each of the competitors does not produce a sufficiently whole numbered R, the smallest radius the newly discovered planet can be is 8=R(2,7,8) megameters.
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