Answer
We can see the graph of the four orbits below:
We can see that the Earth's distance from the sun is much smaller than the others' distances from the sun.
Work Step by Step
$r = \frac{a~(1-e^2)}{1+e~cos~\theta}$
Earth:
$a = 1.00$
$e = 0.017$
$\theta = 0^{\circ}~~~~~~~r = 0.98$
$\theta = 90^{\circ}~~~~~~r = 1.00$
$\theta = 180^{\circ}~~~~~r = 1.02$
$\theta = 270^{\circ}~~~~~r = 1.00$
Jupiter:
$a = 5.20$
$e = 0.048$
$\theta = 0^{\circ}~~~~~~~r = 4.95$
$\theta = 90^{\circ}~~~~~~r = 5.19$
$\theta = 180^{\circ}~~~~~r = 5.45$
$\theta = 270^{\circ}~~~~~r = 5.19$
Uranus:
$a = 19.20$
$e = 0.047$
$\theta = 0^{\circ}~~~~~~~r = 18.30$
$\theta = 90^{\circ}~~~~~~r = 19.16$
$\theta = 180^{\circ}~~~~~r = 20.10$
$\theta = 270^{\circ}~~~~~r = 19.16$
Pluto:
$a = 39.40$
$e = 0.249$
$\theta = 0^{\circ}~~~~~~~r = 29.59$
$\theta = 90^{\circ}~~~~~~r = 36.96$
$\theta = 180^{\circ}~~~~~r = 49.21$
$\theta = 270^{\circ}~~~~~r = 36.96$
We can see the graph of the four orbits below:
We can see that the Earth's distance from the sun is much smaller than the others' distances from the sun.