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The $\rm\Lambda$CDM cosmological model is remarkable: with just 6 parametersit describes the evolution of the Universe from a very early time when allstructures were quantum fluctuations on subatomic scales to the present, and itis consistent with a wealth of high-precision data, both laboratorymeasurements and astronomical observations. However, the foundation of$\rm\Lambda$CDM involves physics beyond the standard model of particle physics:particle dark matter, dark energy and cosmic inflation. Until this `newphysics' is clarified, $\rm\Lambda$CDM is at best incomplete and at worst aphenomenological construct that accommodates the data. I discuss the pathforward, which involves both discovery and disruption, some grand challengesand finally the limits of scientific cosmology.

$\Lambda$CDM: Much more than we expected, but now less than what we want