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We report the discovery of a radio quiet type 2 quasar (SDSSJ165315.06+234943.0 nicknamed the "Beetle" at z=0.103) with unambiguousevidence for active galactic nucleus (AGN) radio induced feedback acting acrossa total extension of ~46 kpc and up to ~26 kpc from the AGN. To the best of ourknowledge, this is the first radio quiet system where radio induced feedbackhas been securely identified at >>several kpc from the AGN. Turbulent gas isalso found far from the radio axis, ~25 kpc in the perpendicular direction. Wepropose a scenario in which the radio structures have perforated theinterstellar medium of the galaxy and escaped into the circumgalactic medium.While advancing, they have interacted with in-situ gas modifying itsproperties. Our results show that jets of modest power can be the dominantfeedback mechanism acting across huge volumes in radio quiet systems, includinghighly accreting luminous AGN, where radiative mode feedback may be expected.

Galaxy wide radio induced feedback in a radio quiet quasar