The Threat to Earth from Asteroids & Comets |
Since it formed over 4.5 billion years ago, Earth has been hit many times by
asteroids and comets whose orbits bring them into the inner solar system. These
objects, collectively known as Near Earth Objects or NEOs, still pose a danger
to Earth today. Depending on the size of the impacting object, such a collision
can cause massive damage on local to global scales. There is no doubt that
sometime in the future Earth wil suffer another cosmic impact; the only question
is "when?". There is strong scientific evidence that cosmic collisions have
played a major role in the mass extinctions documented in Earth's fossil record.
That such cosmic collisions can still occur today was demonstrated graphically
in 1994 when Comet Shoemaker-Levy 9 broke apart and 21 fragments, some as large
as 2 km in diameter, crashed into the atmosphere of Jupiter. If these fragments
had hit Earth instead, we would have suffered global catastrophes of the kind
that inspire science fiction movies: The dangers posed by these intruders in the inner solar system are now the subject of serious scientific investigation. Excellent introductions to the NEOs and the threat they pose to our planet can be found at the following websites:
Following the 2003 NASA report from the Near-Earth Object Science Definition Team, Congress went even further and in 2005 assigned NASA the task of detecting 90% of near-Earth objects with a size greater than 140 meters in diameter by the year 2020. In response to these mandates from Congress, several programs have been undertaken to map the orbits of large NEOs that might pose a danger to Earth. These include the following projects:
What can be done if one of these surveys finds an asteroid on a collision course with the Earth? Scientists and engineers at the B612 foundation are looking at ways of using a spacecraft to gently change the orbit of an asteroid. One promising approach is the "gravity tractor" invented by NASA astronauts Ed Lu and Stan Love. Next: Pan-STARRS and NEOs |
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