Coordinating Europe’s role in the global asteroid hunt
Near-Earth Objects (NEOs) are asteroids or comets with sizes ranging from one meter to tens of kilometres that orbit the Sun and whose orbital paths come close to that of Earth's. Of the more than 700 000 known asteroids in our Solar System, about 17 000 are known to be NEOs.
Dramatic proof that any of these can strike Earth came on 15 February 2013, when an unknown object travelling at 66 000 km/hr and thought to be 17-20 m in diameter exploded high above Chelyabinsk, Russia, with 20-30 times the energy of the Hiroshima atomic bomb.
The resulting shock wave caused widespread damage and injuries, making it the largest known natural object to have entered Earth's atmosphere since the 1908 Tunguska event, which destroyed a remote forest area of Siberia.
The major concern with NEOs is the potential threat that they pose to life on our planet, which has been affected numerous times in past eons by impacts.
The good news is that the timescale of the most dangerous events – having major, planetary-scale effects – is extremely long, exceeding not only a human lifetime but the rise and fall of entire civilizations. Nevertheless, even the much more frequent impacts of much smaller bodies are potentially hazardous events and these merit adequate monitoring.
Moreover, NEO monitoring is crucial as our scientific knowledge of the NEO population is still incomplete.
To date, more than 90% of objects with diameters larger than 1 km have been discovered, but this figure drops to only 10% when considering 100 m-sized objects, any one of which would be many times more destructive if they hit Earth than the Tunguska or Chelyabinsk events.
NEO Segment
Goals of the NEO Segment span:
Expand knowledge of the current and future position of NEOs relative to Earth
Estimate the likelihood of Earth impacts
Assess the consequences of any possible impact
Develop NEO deflection methods
The NEO Segment observes NEOs, predicts their orbits, produces impact warnings when necessary and is involved in potential mitigation measures.
The NEO Segment is based on syndicating and federating Europe’s current observation capabilities and data sources, while developing new sky-survey technologies such as automated telescopes together with a more efficient data and information handling network.
For more information, access the NEO Segment page via http://www.esa.int/ssa-neo