  Recently, Brown et al. (2004) reported the exciting discovery of an ~800 km
radius object, (90377) Sedna, on a distant, eccentric orbit centered at ~490 AU
from the Sun. Here we undertake a first look exploring the feasibility of
accreting this object and its possible cohorts between 75 AU (Sedna's
perihelion distance) and 500 AU (Sedna's semi-major axis distance) from the
Sun. We find such accretion possible in a small fraction of the age of the
solar system, if such objects were initially on nearly circular orbits in this
region, and if the solar nebula extended outward to distances far beyond the
Kuiper Belt. If Sedna did form in situ, it is likely to be accompanied by a
cohort of other large bodies in this region of the solar system.
