(Sketch.) Let $P$ and $Q$ be two points on a parabola, and let $R$ be the point where the respective tangents to the parabola intersect. Let $X$ the midpoint of $PQ$. Then $RX$ is parallel to the axis of symmetry of the parabola (proved below). Draw lines through $P$ and $Q$ parallel to $RX$, and reflect these lines in the respective tangents; the focus $F$ is the intersection of the reflected lines.
To show that $RX$ is parallel to the axis of symmetry: Drop perpendiculars from $P,Q,R$ to the directrix, meeting it at $P',Q',R'$ respectively. As you alluded to, the tangent at $P$ is the perpendicular bisector of the segment $FP'$, and likewise for $Q$ and $FQ'$. So, in $\triangle FP'Q'$, two of the perpendicular bisectors pass through $R$; therefore the third does as well. Since $RR'$ is a line through $R$ and perpendicular to $P'Q'$, it must be the perpendicular bisector, that is, $R'$ is the midpoint of $P'Q'$. By parallels, (the extension of) $RR'$ bisects $PQ$, that is, $RR'$ passes through $X$. So $RX$ is perpendicular to the directrix, as claimed.
Edit: Just for reference, here's what this looks like analytically: The direction of $RX$ is $(2,1)$; reflecting in $RP$ just means exchanging $x$ and $y$ coordinates, so the direction of $PF$ is $(1,2)$, and the line through $P$ in that direction is $2x-y=1$. Reflecting in $RQ$ means negating the $y$-coordinate, so the direction of $QF$ is $(2,-1)$, and the line through $Q$ in that direction is $x+2y=1$. The intersection of these lines is $(\frac35,\frac15)$.
So, when you look at an body's orbit around the sun, you'll end up with an aphelion and a perihelion. These form the major axis, or the longest axis of the ellipse.
We know that $a^3/T^2 = 7.495\times10^{-6}$ from the Third Law.
$a$ represents the semi-major axis, and is half of the sum of aphelion distance (furthest) and perihelion distance (closest).
Given that $T = 27740\ \text{days}$ from 76 years, we can figure out that...
$a^3=(7.495\times10^{-6})\times(27740^2)$ --> $a \approx 17.933354$.
If aphelion $d_1$ + perihelion $d_2$ = twice the semimajor axis $2a$, and the shortest distance is $.59\ \text{a.u.}$, then we can solve for $a$:
$d_1\ \text{(far)} + d_2\ \text{(near)} = 2a\ \text{(long axis)}$
$d_1 = 2a - d_2 = 35.86 - .59 = 35.27\ \text{a.u.}$
Best Answer
Let $a$ be the minimum distance of the comet from Sun, that is the distance between focus and vertex of the parabola. The equation of the parabola, with vertex at $(0,0)$, is then: $$ x={1\over4a}y^2. $$ Substitute here the coordinates of the known position $C$ of the comet: $C=(a+50,50\sqrt3)$ (in units of $10^6\ $km) and solve for $a$.
EDIT.
A more geometrical solution (see diagram below). Let $KH$ be the directrix of the parabola so that $CH=CS=100$. Triangle $CSH$ is equilateral, hence $KS={1\over2}CH=50$ and $VS={1\over2}KS=25$.