Space distribution of near Earth asteroids and lines of search for them

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Scientific paper

We investigate the space distribution of the orbits of 600 near-Earth asteroids and the visible distribution of NEAs over the celestial sphere for different ecliptical longitudes λE. The previous conclusion (which was based on a quite small number of NEAs) that the space concentration of NEAs at λE = 350...300 (September-October) is greater by 30-50 per cent as compared to other periods is confirmed. Well-founded recommendations as to the seasons and zones on the celestial sphere most suitable to the search for new NEAs are given.

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