10 January 2017
Spotting a previously unknown asteroid for the first time always raises the big question: is there a risk it will impact Earth?
Yet, upon discovery, analysts often have very little to go on. The
initial image from the observatory, survey team or individual backyard
astronomer who spotted the rock typically gives only basic information –
its location in the sky and its brightness – and sometimes these aren’t
known terribly accurately.
The most crucial information needed to determine with any degree of
confidence whether it is a ‘near-Earth object’ (NEO) – and that it will
miss Earth (or not) – is the new object’s path. And determining that
requires a series images acquired over a period of days or even months.
“We need multiple follow-on images to compute the trajectory and make a
risk estimate, but even then the uncertainty can be very large. It
really takes many months of observations to get a good, reliable impact
risk estimate, and in the meantime, there can be reason to worry,” says
Ettore Perozzi of the NEO Coordination Centre at ESA’s facility in
Italy.
Spotted from Arizona:
This is precisely what happened on 19 October, when asteroid 2016 WJ1 was discovered by the Catalina Sky Survey.
Additional images were taken by observers worldwide over the next few
weeks, including by a team working at ESA’s own observatory on Tenerife
in the Canary Islands, but uncertainty of the path meant that a possible
close approach in June 2065 – with a worrying impact probability of
about 1 in 8000 – could not be excluded.
“The additional images allowed us to refine our knowledge of the
trajectory sufficiently to begin searching astronomical archives, to see
if anyone had previously imaged this asteroid without having recognised
it as such,” says Marco Micheli, observer at the NEO centre.
If any were found, the team would score what astronomers call a ‘precovery’ – short for pre-discovery.
Precovering:
While these were inconclusive, the team assumed they were, in fact,
accurate and then used these to call up additional, highly accurate
images from a Canadian astronomical image search system.
Bingo: two sets of images from 4 and 5 July 2003 with the Canada–France–Hawaii Telescope were found.
“After careful inspection we were able to pinpoint the object, and the
team were able to perform some very accurate determinations,” says
Detlef Koschny, responsible for the NEO portion of ESA’s Space
Situational Awareness programme.
“The result was that we could preclude any risk of Earth impact from asteroid 2016 WJ1 anytime soon or well into the future.”
ESA is now developing a new set of automated, wide-field-of-view ‘Fly-Eye’ telescopes that will conduct nightly sky surveys, creating a large future archive of images that will make critical precovery confirmations more efficient in future.
ESA is now developing a new set of automated, wide-field-of-view ‘Fly-Eye’ telescopes that will conduct nightly sky surveys, creating a large future archive of images that will make critical precovery confirmations more efficient in future.
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