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

Cool Jupiters greatly outnumber their toasty siblings: Occurrence rates from the Anglo-Australian Planet Search