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Recent theoretical developments in the description of jet evolution in thequark gluon plasma have allowed to account for the effects of hydrodynamicgradients in the medium modified jet spectra. These constitute a crucial steptowards using jets as tomographic probes of the nuclear matter they traverse.In this work, we complement these studies by providing leading ordercalculations of widely studied jet observables, taking into account matteranisotropies. We show that the energy distribution inside a jet is pushedtowards the direction of the largest matter anisotropy, while the away regionis depleted. As a consequence, the jet mass and girth gain a non-trivialazimuthal dependence, with the average value of the distribution increasingalong the direction of largest gradients. However, we find that, for these jetshapes, matter anisotropic effects can be potentially suppressed by vacuumSudakov factors. We argue that the recently proposed measurements of energycorrelations within jets do not suffer from such effects, with the azimuthaldependence being visible in a large angular window, regardless of the shape ofthe distribution.

Picturing QCD jets in anisotropic matter: from jet shapes to Energy Energy Correlators