  We use Sloan Digital Sky Survey Data Release 5 photometry and spectroscopy to
study a tidal stream that extends over 50 degrees in the North Galactic Cap.
  From the analysis of the path of the stream and the colors and magnitudes of
its stars, the stream is about 20 kpc away at its nearest detection (the
celestial equator). We detect a distance gradient -- the stream is farther away
from us at higher declination. The contents of the stream are made up from a
predominantly old and metal-poor population that is similar to the globular
clusters M13 and M92. The integrated absolute magnitude of the stream stars is
estimated to be M_r = -7.5. There istentative evidence for a velocity
signature, with the stream moving at -40 km/s at low declinations and +100 km/s
at high declinations. The stream lies on the same great circle as Complex A, a
roughly linear association of HI high velocity clouds stretching over 30
degrees on the sky, and as Ursa Major II, a recently discovered dwarf
spheroidal galaxy. Lying close to the same great circle are a number of
anomalous, young and metal-poor globular clusters, including Palomar 1 and
Ruprecht 106.
