We report the discovery of the most distant known active galactic nucleus,
the radio galaxy TN J0924-2201 at z = 5.19. The radio source was selected f
rom a new sample of ultrasteep spectrum sources, has an extreme radio spect
ral index alpha(365 MHz)(1.4 GHz) = -1.63, and is identified at near-IR wav
elengths with a very faint, K = 21.3 +/- 0.3 object. Spectroscopic observat
ions show a single emission line at lambda similar to 7530 Angstrom, which
we identify as Ly alpha. The K-band image, sampling rest-frame U band, show
s a multicomponent, radio-aligned morphology, which is typical of lower-red
shift radio galaxies. TN J0924-2201 extends the near-IR Hubble, or K-z, rel
ation for powerful radio galaxies to z > 5 and is consistent with models of
massive galaxies forming at even higher redshifts.