  Granvik et al. (2016) report an absence of asteroids on orbits with perihelia
near the Sun that they attribute to the 'supercatastrophic disruption' of these
bodies. Here we investigate whether there is evidence for this process among
other bodies with similarly low perihelia: near-Earth asteroids, SOHO comets,
as well as meter-sized and millimeter-sized meteoroids. We determine no known
near-Earth asteroids have past (last 10^4 years) histories residing
significantly inside the Granvik et al. (2016) limit, indirectly supporting the
disruption hypothesis. The exception is asteroid (467372) 2004 LG which spent
2500 years within this limit, and thus presents a challenge to that theory.
Phaethon has a perihelion distance hovering just above the limit and may be
undergoing slow disruption, which may be the source of its dust complex. We
find that the rate at which ungrouped SOHO comets are observed is consistent
with expected rates for the injection of small (25 m) class asteroids into the
near-Sun region and suggest that this fraction of the SOHO-observed comet
population may in fact be asteroidal in origin. We also find that there is an
absence of meter-sized bodies with near-Sun perihelia but an excess of
millimeter-sized meteoroids. This implies that if near-Sun asteroids disrupt,
they do not simply fragment into meter-sized chunks but disintegrate ultimately
into millimeter-sized particles. We propose that the disruption of near-Sun
asteroids as well as the anomalous brightening and destruction processes that
affect SOHO comets occur through meteoroid erosion, that is, the removal of
material through impacts by high-speed near-Sun meteoroids.
