Hi Berner,<br /><br />That is a good question indeed. I am not sure there is an evidenced answer to your question, especially in terms of quantified budget.<br /><br />The Sun's gravity well extends over several tens of thousands of AU. Very light particles coming from the rest of the galaxy are stopped by solar wind quite close, with a bow shock (between 50 and several hundreds of AU depending on interstellar medium intensity). The bow shock is well inside the Sun's grav well. Once stopped or slowed down they can be captured. Heaviest elements, including dusts, rocks and exoplanetesimals can penetrate the bow shock and be deviated or captured, e.g. on orbits with large semi-major axis. <br />The H2O for instance, vaporized beneath the frost line, is flushed by the solar wind towards the outer system but not with enough energy to leave the grav well. Many molecules should be re-accreted.<br /><br />You mention the solar wind as a way to lose matter. But there is another way. Planetesimals or asteroids might be expelled by orbit instability / close encounters. Half of them are predicted to be expelled along their life. Some are injectd on higher orbits. Others may be expelled.<br /><br />Btw this means too that the Solar System should capture such objects all along Sun's wandering around the Milky Way. <br /><br />Best regards.