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We present a measurement of the trigonometric parallax for a nearby very low mass star recently discovered by Delfosse et al. (2001). Using schmidt plates measured on the SuperCOSMOS plate scanning machine we nd a parallax of = 19237 mas, giving a distance of d =5 :2 +1:2 0:8 pc. Using this distance we nd the absolute magnitude and kinematics for the object to be consistent with an intermediate{age disk object of mass 0:08 M. This star is clearly nearby and is on these measurements between the 30th and 86th closest known stellar system to the Sun; it could be the closest M 9 dwarf to the Sun.

Research NoteThe trigonometric parallax of DENIS-P J104814.7-395606.1