Deflecting asteroids

Earth would need to be ready for an imminent asteroid threat. Luckily, scientists are working hard to give the planet the best range of defensive strategies. – Agencies

OUR solar system is full of rogue rocks.

Millions of them orbit around the Sun or around other objects, the shattered remains of planets, moons or comets.

If they are within one-third the distance from Earth to the Sun, they are classified as near-Earth objects (NEOs), and are of special interest because of their potential to destroy our planet.

The first NEO was spotted in 1989. In 1994, US Congress asked space agency Nasa to identify 90% of NEOs with planet-destroying potential – those 1km in diameter or larger – by 2005.

That task complete, Nasa was given a new target of 90% of NEOs 140m or larger. That goal has remained more elusive – it is estimated only 40% of all NEOs in that category have been discovered.

Even with millions of dollars in funding and the best technology Nasa can muster, asteroids still catch us unawares.

Nasa completely missed one that smacked into the Norwegian Sea in March this year. A Hungarian astronomer, Krisztián Sárneczky, spotted it with only hours to spare. Scientists believe it’s a matter of when, not if, a big one will chart a collision course with Earth.

If spotted far enough out, humanity has time to prepare. Time to send out warnings, time to evacuate cities, time to nudge its trajectory, time to hit it with nukes. The key to planetary defence is early detection.

The world’s early warning systems are surprisingly informal. Collections of observatories volunteering time and resources make up our principal defence. But NEOs are a relatively new global concern.

In time, our collective need for a comprehensive asteroid alert system may pave the way for international collaboration on projects of undeniable importance. – 360info

Reality check

• Of the 1.2 million objects floating in our solar system, 29,264 are near-Earth objects.

• Every day, 80 to 100 tonnes of dust and small meteorites fall from space onto planet Earth. Almost all of them burn up in our atmosphere.

• An asteroid’s potential danger is a function of its size, its speed relative to Earth’s, its mass and the angle of the collision. Big, fast, heavy rocks coming in at a steep angle are the most dangerous.

• The first “asteroid” discovered was in fact a dwarf planet, Ceres. It was spotted by Giuseppe Piazzi, a Catholic priest and astronomer, in 1801. Dispute about whether Ceres is a planet or an asteroid was responsible for the 2006 demotion of Pluto to dwarf planet status.