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The Hungaria Family (the closest region of the Main Belt to Mars) is animportant source of Planet-Crossing-Asteroids and even impactors of terrestrialplanets. We present the possibility that asteroids coming from the HungariaFamily get captured into co-orbital motion with the terrestrial planets in theinner solar system. Therefore we carried out long term numerical integrations(up to 100 Myr) to analyze the migrations from their original location - theHungaria family region- into the inner solar system. During the integrationtime we observed whether or not the Hungarias get captured into a co-orbitalmotion with the terrestrial planets. Our results show that 5.5% of 200Hungarias, selected as a sample of the whole group, escape from the Hungariaregion and the probability from that to become co-orbital objects (Trojans,satellites or horseshoes) turns out to be about 3.3%: 1.8% for Mars and 1.5%for the Earth. In addition, we distinguished in which classes of co-orbitalmotion the asteroids get captured and for how long they stay there in stablemotion. Most of the escaped Hungarias become Quasi-satellites and the onescaptured as Trojans favor the L_5 lagrangian point. This work highlights thatthe Hungaria region is a source of Mars and also Earth co-orbital objects.

Hungaria region as possible source of Trojans and satellites in the inner solar-system