ESA's new X-ray optics for observing the hot Universe

May 18, 2014
Artist's impression of a galaxy that is releasing material via two strong jets (shown in red/orange) as well as via wide-angle outflows (shown in gray/blue). Both jets and outflows are being driven by the black hole located at the galaxy's centre. Black holes, which lurk unseen at the centres of almost all galaxies, are regarded as one of the keys to understanding galaxy formation and evolution. Credit: ESA/AOES Medialab

A new idea to use super-polished silicon wafers as the heart of a telescope is set to reveal more of the hot, high-energy Universe, peering back into its turbulent history.

Invisible X-rays tell us about the very hot matter in the Universe – black holes, supernovas and superheated gas clouds. Today's X-ray observatories, ESA's XMM-Newton and NASA's Chandra, were launched in the last century, and are still delivering world-class science. But they are starting to age.

To replace them, ESA is planning a much more capable X-ray observatory for launch in 2028, which would probe 10 to 100 times deeper into the Universe than the current generation of X-ray telescopes.

"This demands a whole new type of X-ray ," explains Marcos Bavdaz, leading the technology push for ESA's future science missions. "To reach the kind of size needed, this new mission's mirrors will have to be 10 times lighter than XMM's, while delivering even sharper images."

The problem is that energetic X-rays do not behave like typical light waves – try to reflect them with a standard mirror and they are absorbed inside. Instead, X-rays can only be reflected at shallow angles, like stones skimming along water.

That means multiple mirrors must be stacked together to build a large-enough telescope. XMM has 174 gold-plated nickel mirrors, nested inside one another like Russian dolls.

But to reach the performance required for ESA's next X-ray mission, tens of thousands of densely packed mirror plates will be needed. How can this be done?

A new approach is required. 'Silicon pore optics', developed by ESA, draws on high-tech equipment and materials from the semiconductor industry.

ESA’s new X-ray optics for observing the hot Universe
Curved mirrors stacked within one of three optical modules of ESA's XMM-Newton telescope. Each one contains 58 mirrors with a total telescope optical surface of more than 120 m2 – bigger than a tennis court. Credit: ESA

"We make use of industrial silicon wafers, normally used to manufacture microprocessors," adds Eric Wille, optical system engineer for the X-ray optics development.

"We take advantage of their stiffness and super-polished surface, stacking a few dozen at a time together to form a single 'mirror module'."

Many hundreds of these modules will be fitted together to form the optics of the X-ray mission.

Grooves are cut into the wafers, leaving stiffening ribs and paper-thin mirrors, which are then covered with reflective metal. For maximum accuracy, semiconductor manufacturing techniques are applied for the stacking process.

"Stacking is done by a specially designed robot, aiming for micron-scale precision," Eric describes. "We've seen big jumps in quality as the robotics improve."

"All the stacking takes place in a cleanroom, since tiny dust particles risk large deformations in the mirror stack.

"The semiconductor industry is improving the quality of , which will further improve the mirror quality in future."

The company cosine Research, leading the silicon pore optics consortium, has succeeded in the routine production of complete mirror modules.

A silicon pore optics mirror stack consisting of 35 mirror plates. The plates are made of silicon wafers. Hundreds of pores allow the X-rays to propagate through the mirror stack and be reflected on the coated stripes. Credit: cosine Research

Hundreds of mirror plates are regularly made by Micronit Microfluidics, a company specialised in micromachining large quantities of glass and silicon products.

Another consortium member, Kayser-Threde, has vibration-tested a mirror module and its mounting system, showing the design is capable of enduring a launch to space.

ESA's mission to the hot, high-energy universe

In November 2013 the science theme 'the hot and energetic Universe' was selected for the second Large-class mission, or L2, in ESA's Cosmic Vision science programme – to be pursued with an advanced X-ray observatory.

With a launch date foreseen for 2028, the mission will address two key questions. How and why does ordinary matter assemble into the galaxies and galactic clusters that we see today, and how do black holes – lurking at the centre of almost all galaxies – grow and influence their surroundings?

Still many years from launch, the underlying optical technology required is being prepared as a joint effort between ESA's Technology Research Programme – turning innovative ideas into working prototypes – and its Science Core Technology Programme – developing enabling technologies for future science missions.

Explore further: ESA's new vision to study the invisible Universe

add to favorites email to friend print save as pdf

Related Stories

Image: X-raying the cosmos

Apr 22, 2014

When we gaze up at the night sky, we are only seeing part of the story. Unfortunately, some of the most powerful and energetic events in the Universe are invisible to our eyes – and to even the best optical ...

Faster, cheaper chips from space technology

Mar 26, 2010

(PhysOrg.com) -- Our world is full of integrated semiconductor circuits, commonly known as microchips. Today you find them in computers, cars, mobile phones and in almost every electrical device. Technology ...

A new view of the energetic universe

Dec 03, 2013

The Nuclear Spectroscopic Telescope Array, or NuSTAR, sees the high-energy X-rays emitted by the densest, hottest regions of the universe. The brainchild of Fiona Harrison, Caltech's Benjamin M. Rosen Professor ...

Recommended for you

SpaceX's next cargo launch set for Sept 20

Sep 12, 2014

SpaceX's next unmanned cargo trip to restock supplies at the International Space Station is scheduled for September 20, the US space agency said Friday.

Not just cool – it's a gas

Sep 12, 2014

In space, a new way of producing gas is being tested for steering satellites. On Earth, it is now fighting fires without harming the environment – and business insiders say it could be revolutionary.

Solar storm heads Earth's way after double sun blasts

Sep 11, 2014

Two big explosions on the surface of the sun will cause a moderate to strong geomagnetic storm on Earth in the coming days, possibly disrupting radio and satellite communications, scientists said Thursday.

User comments : 0