A zero point calibration of the Red Giant Branch Tip (TRGB) in the $I$-band is determined from OGLE photometry of the Magellanic Clouds (MCs). It is shown that TRGB measurements made in star-forming regions, with concomitantly high quantities of gas and dust, are less precise and biased to fainter magnitudes, as compared to the same measurements made in quiescent regions. Once these low accuracy fields are excluded from consideration, the TRGB can be used for the first time to constrain the three-dimensional plane geometry of the LMC. Composite CMDs are constructed for the SMC and LMC from only those fields with well-defined TRGB features, and the highest accuracy TRGB zero point calibration to date is presented. The $I$-band TRGB magnitude is measured to be flat over the color range $ 1.45 < (V-I)_0 < 1.95$ mag, with a modest slope introduced when including metal-rich (up to $(V-I)_0 = 2.2$ mag) Tip stars into the fit. Both the flat, blue zero point and the shallow slope calibration are consistent with the canonical value of $-4.05$ mag for the old, metal-poor TRGB, and would appear to resolve a recent debate in the literature over the methods absolute calibration.
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