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We present and analyze a new M' detection of the young exoplanet betaPictoris b from 2008 VLT/NaCo data at a separation of ~ 4 AU and a highsignal-to-noise rereduction of L' data taken in December 2009. Based on ourorbital analysis, the planet's orbit is viewed almost perfectly edge-on (i ~ 89degrees) and has a Saturn-like semimajor axis of 9.50 (+3.93, -1.7) AU.Intriguingly, the planet's orbit is aligned with the major axis of the outerdisk (Omega ~ 31 degrees) but probably misaligned with the warp/inclined diskat 80 AU often cited as a signpost for the planet's existence. Our resultsmotivate new studies to clarify how $\beta$ Pic b sculpts debris diskstructures and whether a second planet is required to explain the warp/inclineddisk.

A 5 Micron Image of beta Pictoris b at a Sub-Jupiter Projected Separation: Evidence for a Misalignment Between the Planet and the Inner, Warped Disk