  Our understanding of planetary systems different to our own has grown
dramatically in the past 30 years. However, our efforts to ascertain the degree
to which the Solar system is abnormal or unique have been hindered by the
observational biases inherent to the methods that have yielded the greatest
exoplanet hauls. On the basis of such surveys, one might consider our planetary
system highly unusual - but the reality is that we are only now beginning to
uncover the true picture. In this work, we use the full eighteen-year archive
of data from the Anglo-Australian Planet Search to examine the abundance of
'Cool Jupiters' - analogs to the Solar system's giant planets, Jupiter and
Saturn. We find that such planets are intrinsically far more common through the
cosmos than their siblings, the hot Jupiters. We find that the occurrence rate
of such 'Cool Jupiters' is $6.73^{+2.09}_{-1.13}$\%, almost an order of
magnitude higher than the occurrence of hot Jupiters (at
$0.84^{+0.70}_{-0.20}$\%). We also find that the occurrence rate of giant
planets is essentially constant beyond orbital distances of $\sim$1\,au. Our
results reinforce the importance of legacy radial velocity surveys for the
understanding of the Solar system's place in the cosmos.
