Deflecting NEOs in Route of Collision with the Earth
โ Scribed by Andrea Carusi; Giovanni B. Valsecchi; Germano D'Abramo; Andrea Boattini
- Publisher
- Elsevier Science
- Year
- 2002
- Tongue
- English
- Weight
- 107 KB
- Volume
- 159
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
โฆ Synopsis
We consider a small sample of known near Earth objects (NEOs), both asteroids and comets, with low minimum orbital intersection distance (MOID). Through a simple numerical procedure we generate slightly different orbits from this sample in such a way that these bodies will collide with the Earth at a specific epoch. Then we study the required change in orbital velocity (along track v) in order to deflect these NEOs at different epochs before the impact event. The orbital evolution of these NEOs is performed through a full N-body numerical integrator. A comparison with analytical estimates is also performed in selected cases. Interesting features in the v/time before impact plots are found; as a prominent result, we find that close approaches to the Earth before the epoch of the impact can make the overall deflection easier.
๐ SIMILAR VOLUMES
We obtain the size and orbital distributions of near-Earth asteroids (NEAs) that are expected to be in the 1 : 1 mean motion resonance with the Earth in a steady state scenario. We predict that the number of such objects with absolute magnitudes H < 18 and H < 22 is 0.65 ยฑ 0.12 and 16.3 ยฑ 3.0, respe
Chemilnminescence of MgI, CaI, and Sri was observed in a beam-gas arrangement when atomic beams of Mg, Ca, and Sr were excited to the 'P, states. Total collision and chemiluminescence cross sections were measured. For MgI, in the region of the A 211-X 2I;+ transition reported from absorption experim