  The Einstein-Cartan equations in first-order action of torsion are
considered. From Belinfante-Rosenfeld equation special consistence conditions
are derived for the torsion parameters relating them to the metric. Inside
matter the torsion is given by the spin which leads to an extended
Oppenhaimer-Volkov equation. Outside matter a second solution is found besides
the torsion-free Schwarzschild one with the torsion completely determined by
the metric and vice-versa. This solution is shown to be of non-spherical origin
and its uniqueness with respect to the consistence is demonstrated. Unusual
properties are discussed in different coordinate systems where the cosmological
constant assumes the role of the Friedman parameter in
Friedman-Lama\^itre-Robertson-Walker cosmoses. Parameters are specified where
wormholes are possible. Transformations are presented to explore and map
regions of expanding and contracting universes to the form of static metrics.
The autoparallel equations are solved exactly and compared with geodesic
motion. The Weyl tensor reveals that the here found solution is of Petrov-D
type.
