We derive analytically the angular velocity of a spheroid, of an arbitrary aspect ratio
$\kappa$
, sedimenting in a linearly stratified fluid. The analysis demarcates regions in parameter space corresponding to broadside-on and edgewise settling in the limit
$Re, Ri_v \ll 1$
, where
$Re = \rho _0UL/\mu$
and
$Ri_v =\gamma L^3\,g/\mu U$
, the Reynolds and viscous Richardson numbers, respectively, are dimensionless measures of the importance of inertial and buoyancy forces relative to viscous ones. Here,
$L$
is the spheroid semi-major axis,
$U$
an appropriate settling velocity scale,
$\mu$
the fluid viscosity and
$\gamma \ (>0)$
the (constant) density gradient characterizing the stably stratified ambient, with the fluid density
$\rho_0$
taken to be a constant within the Boussinesq framework. A reciprocal theorem formulation identifies three contributions to the angular velocity: (1) an
$O(Re)$
inertial contribution that already exists in a homogeneous ambient, and orients the spheroid broadside-on; (2) an
$O(Ri_v)$
hydrostatic contribution due to the ambient stratification that also orients the spheroid broadside-on; and (3) a hydrodynamic contribution arising from the perturbation of the ambient stratification whose nature depends on
$Pe$
;
$Pe = UL/D$
being the Péclet number with
$D$
the diffusivity of the stratifying agent. For
$Pe \ll 1$
, this contribution is
$O(Ri_v)$
and orients prolate spheroids edgewise for all
$\kappa \ (>1)$
. For oblate spheroids, it changes sign across a critical aspect ratio
$\kappa _c \approx 0.41$
, orienting oblate spheroids with
$\kappa _c < \kappa < 1$
edgewise and those with
$\kappa < \kappa _c$
broadside-on. For
$Pe \ll 1$
, the hydrodynamic component is always smaller in magnitude than the hydrostatic one, so a sedimenting spheroid in this limit always orients broadside-on. For
$Pe \gg 1$
, the hydrodynamic contribution is dominant, being
$O(Ri_v^{{2}/{3}}$
) in the Stokes stratification regime characterized by
$Re \ll Ri_v^{{1}/{3}}$
, and orients the spheroid edgewise regardless of
$\kappa$
. Consideration of the inertial and large-
$Pe$
stratification-induced angular velocities leads to two critical curves which separate the broadside-on and edgewise settling regimes in the
$Ri_v/Re^{{3}/{2}}$
–
$\kappa$
plane, with the region between the curves corresponding to stable intermediate equilibrium orientations. The predictions for large
$Pe$
are broadly consistent with observations.