December 21, 2009
Extended X-Ray Vision Of High-Energy Cosmos
As elements of the integrated circuits running our computers, phones and electronics, silicon wafers are everywhere. An ESA-led effort is establishing an out-of-this-world use for these commonplace items: when stacked together precisely by the thousand they promise to deliver astronomy's clearest X-ray view yet of the most violent regions of space.
"ESA has been working with specialist European firms to develop this new optical technique and build up a supporting industry," said Marcos Bavdaz, Head of ESA's Advanced Technology Section. "This "Ësilicon pore optics' effort is part of the Agency's preparation for the International X-ray Observatory (IXO), a candidate mission with NASA and Japan's space agency for around 2020."
The Dutch company cosine Research is leading an international consortium of industrial partners and research institutes from ESA member states. This month, their latest results were presented: optics in flight configuration underwent testing in X-ray facilities, revealing excellent optical performance.
Hot secrets of the X-ray sky
Observing the sky in X-rays reveals a violent Universe of exploding stars, black holes and incandescent gas clouds. With temperatures of millions of degrees, such high-energy objects shine at X-ray wavelengths but not in visible light. Astronomers could only study this violent, high-energy Universe once the space age gave them a way of placing telescopes above the X-ray-absorbing atmosphere.
Actually forming a focused image from X-rays, however, is no easy task. Medical X-rays are well-known, but they are not focused images "“ just shadows cast through body parts using techniques pioneered by X-ray discoverer Wilhelm Roentgen in 1895.
Standard optical designs do not work because energetic X-rays are reflected only at extremely shallow angles. While visible light reflects off a mirror like a ball bouncing off a wall, X-ray reflection works more like a stone skimming along a pond. Telescope mirrors must face sideways instead of straight on, and many mirrors are needed to gather sufficient X-rays. So an X-ray telescope is more like a set of Russian dolls, with mirrors stacked around each other.
New technology for broader, sharper X-ray views
ESA's XMM-Newton X-ray space observatory uses more than 250 gold-coated nickel mirrors, while NASA's Chandra relies on fewer mirrors made of heavier glass. For IXO, the aim is to boost XMM's collecting area 20-fold, while delivering three times the resolution. Achieving this demands new technology: while NASA is investigating an alternative called "Ëslumped glass', ESA is focusing on silicon pore optics, based around commercial silicon wafers.
ESA's Eric Wille, overseeing the project together with Kotska Wallace, explained: "Manufacturers already polish these wafers to optical quality to better "Ëprint' the tiny structures needed for the latest microprocessors. So the wafers need no further polishing, while also being both light and stiff."
Semiconductor industry technologies are being harnessed to prepare silicon wafers and shape them into the complex structures required. They are cut into paper-thick square plates with "Ëribs' diced into them to facilitate stacking. They are then tapered into a wedge shape to direct X-rays along the desired optical path, after which metal coatings are added. An industrial robot performs their precision stacking and mounting.
The technique is called "Ësilicon pore optics' because the massed stacks of ribbed silicon are porous, X-rays being able to reflect through each pore in the assembled silicon stack "Ëpetals'. IXO would need more than 200 000 silicon plates overall. The next step is to streamline the assembly process for mass production and further improve quality, opening the door to unprecedented discoveries in the X-ray sky.
Image 1: This artist's impression shows a supermassive black hole surrounded by an accretion disc and dust torus. Material within the accretion disc is accelerated to extremely high velocities by the inexorable gravitational pull of the black hole. The ESA-NASA-JAXA International X-ray Observatory (IXO) mission candidate, being considered for launch around 2020, will enable more detailed study of the composition and behavior of such highly energetic material, which radiates at X-ray wavelengths. Credits: ESA / V. Beckmann (NASA-GSFC)
Image 2: Proposed design for the International X-ray Observatory (IXO), a joint ESA-NASA-JAXA candidate mission being considered for launch around 2020. The partner space agencies have agreed that the new mission will have a 20-fold increase in collecting area compared to the current XMM-Newton while also having a threefold increase in resolution. To achieve this within the mission's stringent mass restrictions requires new techniques to achieve stiff but lightweight mirrors. The two technologies under investigation are NASA's "Ëslumped glass' technique and ESA's "Ësilicon pore optics'. Credits: ESA CDF
Image 3: Test mirror module produced for the ESA's silicon pore optics research project. Mirror plates are stacked up then two sets of stacks are co-aligned together to form a module in flight configuration. Hundreds of such modules would then be put together in order to form a "Ëpetal'. A total of eight carefully-shaped petals would serve to form the X-ray optics of the IXO candidate mission. An international consortium coordinated by cosine Research has so far demonstrated every step in the chain up to module assembly, with completed modules being put to the test in X-ray facilities. Credits: ESA/cosine/SPO consortium
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