Drift and accretion of interplanetary dust and the transformation of its orbits

Astronomy and Astrophysics – Astronomy

Scientific paper

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Deposition, Drift Rate, Gravitational Effects, Interplanetary Dust, Planetary Orbits, Statistical Distributions, Mars (Planet), Mercury (Planet), Moon, Orbital Velocity, Particle Size Distribution, Poynting-Robertson Effect

Scientific paper

In statistical distributions of orbits of relatively small dust particles one can easily separate a heavy class of the so-called 'minor' orbits (with a semi-axis a less than 2.5 AU) with retrograde motion (the inclination of the orbit's plane being i greater than 90 deg). Among orbits of larger bodies such orbits are not observed. Motion of all the large bodies is direct (i less than 40 deg); the values of semi-axis a less than 2-3 AU are common. The acquisition of dust particles (far within the orbits of Jupiter and Mars) with retrograde motion can be explained, at first, by disintegration of long-periodic and nearly parabolic comets, and, at second, by a long-term (acting during millions of years) Poynting-Robertson effect. The drift of particles of all possible dimensions is accompanied by gravitational accretion. In the latter the most essential is the influence of Jupiter and Saturn; relatively larger particles with a particle size p less than 1 cm across are accreted to a greater extent. The disintegration of comets, Poynting-Robertson effect and accretion result in simultaneous existence of the above orbits' classes. As Stanyukovitch and Fedynsky have shown, the fall of meteor particles onto the surface of atmosphere-free celestial bodies (Mercury, Moon and possibly, Mars) with the velocity of 20-80 km/sec is followed by the ejection of secondary particles. Their velocity exceeds escape velocity for a corresponding celestial body. Thus, around the orbits of Mercury, Earth and Mars there will be originated an additional source of slowly moving dust. It is due to the Poynting-Robertson effect that the dust soon proves to be inside the region occupied by the zodiacal light.

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