Abstract
Abstract
Stable Compact Dark Matter Objects (SCDMO) of planet scale mass and much smaller radii are considered in planet systems with a central star on highly eccentric orbits of SCDMO crossing the star. Possible connections of the presence of these SCDMO in a planet system with specific interactions with planets and the star, in particular, with triggering of cycles of activity of the central star are suggested to study in experiments in the solar system.
Subject
General Physics and Astronomy