In 2004, Hubble created the Hubble Ultra Deep Field哈勃超深场 (HUDF), the deepest visible-light image of the Universe, and now, with its brand-new camera, Hubble is seeing even farther. This image was taken in the same region as the visible HUDF, but is taken at longer wavelengths¹. Hubble's newly installed Wide Field Camera 3 (WFC3) collects light from near-infrared² wavelengths红外波长 and therefore looks even farther back towards the Big Bang宇宙大爆炸, because the light from hot young stars in these very distant galaxies³ is stretched out of the ultraviolet and visible regions of the spectrum⁴光谱，范围 into near-infrared wavelengths by the expansion of the Universe. This new deep view also provides insights into how galaxies grew in their formative years early in the Universe's history. A boon⁵恩惠，福利 to astronomers⁶ worldwide, the new WFC3 data — taken by the HUDF09 team — have set a multitude of teams to work, furiously狂怒地，有力地 searching for the most distant galaxies yet discovered. In just three months, twelve scientific papers on these new data have been submitted.

This image was taken by the HUDF09 team [1], which has made it available for research by astronomers worldwide. The photo was taken with the new WFC3/infrared camera on Hubble in late August 2009, during a total of four days of pointing for 173 000 seconds of total exposure time. Infrared light is invisible to the human eye and therefore does not have colours that can be perceived觉察，理解. The representation is "natural" in that shorter infrared wavelengths are represented as blue and the longer wavelengths as red. The faintest objects are about one billion times fainter than the dimmest暗淡的，模糊的 visible objects seen with the naked eye肉眼.

These Hubble observations are blazing a trail开拓道路 for Hubble's successor, the NASA/ESA James Webb Space Telescope (JWST), which will look even farther into the Universe than Hubble, at infrared wavelengths. The launch of JWST is planned for 2014.