AIMing a light across millions of kilometres

aimingalight
ESA’s Asteroid Impact Mission concept, currently under study, would be humanity’s first mission to a binary asteroid: the 800 m-diameter Didymos is accompanied by a 170 m-diameter secondary body. AIM would send science results back to Earth via a high-bandwidth laser link. Credit: ESA – ScienceOffice.org Enlarge

Imagine beaming a light across millions of kilometres of empty space, all the way back to Earth. ESA’s proposed Asteroid Impact Mission is intended to do just that: demonstrate laser communications across an unprecedented void.

The Asteroid Impact Mission, or AIM, undergoing detailed design ahead of a final go/no-go decision by ESA’s Ministerial Council in December 2016, is a deep-space technology-demonstration mission that would also be humanity’s first probe to a double asteroid.

Among its innovative technologies, would return results to scientists several times faster than standard radio signals.

“Optical communications in general is not yet a well-established technology for space and ESA’s European Data Relay System (EDRS) will be the first commercial application,” explains ESA optics engineer Zoran Sodnik.

“In principle it works something like Morse code, with encoded rapid flashes on and off. ERDS with satellites in high orbits will use laser links to return environmental data from Europe’s low-orbiting Sentinel satellites on a realtime basis, a technique previously demonstrated using ESA’s Alphasat and Artemis telecom missions.

“In 2013 ESA’s Optical Ground Station in Tenerife participated in a two-way contact with NASA’s LADEE lunar orbiter, across 400 000 km.

“But AIM will need to operate much further: we are benchmarking a maximum span of 75 million kilometres, or half the distance between Earth and the Sun. That might sound like a lot, but operating around Mars one day will involve much further distances still.”

A laser beam shone back from AIM’s 13.5 cm-diameter laser telescope at such a distance would have a ground footprint of about 1100 km – further than from London to Berlin. Also a lot but the equivalent radio beam radiating out across space would end up wider than our whole planet.

“The much higher frequency of laser light is what gives us higher directivity and as a result increased bandwidth,” adds ESA laser engineer Clemens Heese.

“At the same time, many photons will get lost on the way, so we need to use sophisticated photon counting methods to detect the signal reliably using our receiver telescope of around 1 m diameter.

“While radio communications is a very mature technology and close to optimum efficiency, there’s still lots of room for development with . So this is the way we need to go to really boost the quantity and speed of data we can deliver to scientists.”

 

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