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The bright NLS1 galaxy MCG-6-30-15 harbors one of the most studied AGN inhigh-energy astrophysics boasting one of the strongest broad Fe K lines everseen as well as the first time-variable warm absorber. We will obtain a 100ksobservation of MCG6 during XRISMs PV phase which will characterize its spectralsignatures with unprecedented resolution. Our primary goals are to establish thekinematics of the multi-phase outflow across all ionization states in the X-raybandpass to verify the spin of the supermassive black hole and to identify anymisalignment of the accretion flow between the inner and outer disk/torus.Werequest simultaneous observations with XMM-Newton and NuSTAR to realize the fullscience return of the XRISM data. [truncated! Please see actual data for full text]