First pictures from the map of the universe mission

The AKARI (formerly ASTRO-F) infrared space telescope is making its All-Sky Survey at infrared wavelengths with sharper images and a much higher sensitivity than the first infrared astronomical sky survey satellite launched in 1983.
AKARI will leave a tremendous legacy for the future of astronomy. Most of the light ever emitted in the Universe was emitted in the infra-red part of the spectrum, so the range of objects that can be studied by this survey is huge.

"These first images are extremely promising," said Dr. Stephen Serjeant, Senior Lecturer in Astrophysics at the Open University, said. "The beautiful filigree structure in the nebula was impossible to see with the previous satellite IRAS. After having worked on this for so many years, it is wonderful to see our labours rewarded so clearly. AKARI can do many things that no other telescope on the Earth or in space can."

Glenn White, Professor of Astronomy at The Open University and The CCLRC Rutherford Appleton Laboratory, adds: "The AKARI mission will redefine our view of the Universe at infrared wavelengths, achieving considerably sharper images through its improved higher spatial resolution and sensitivity over the whole sky than previously available. It offers a major new observatory facility to probe the cradles of star formation, that are normally obscured from the view of other telescopes, the formation and evolution of planetary systems, and to observe the embryonic galaxies assembling toward the edge of the observable universe. History tells us that any similar step forward in performance over what has gone before, is likely to reveal unexpected new phenomena or classes of objects that can help to redefine our understanding of the Universe"

Image Credit: JAXA

These two images of the reflection nebula IC4954 were taken by the two instruments on board Akari - the Far-Infrared Surveyor (FIS) – on the left - and the near- and mid-Infrared Camera (IRC) – on the right. The observed wavelengths are 90 and 9 microns, respectively. The IC4954 region is situated at a distance of about 6000 light years from us and extends more than 10 light years across.

In these first infrared images of this area it is possible to see individual stars that have recently been born. They are embedded in gas and dust and could not be seen in visible light. Is it also possible to see the gas clouds from which these stars are made.




Image Credit: JAXA/IRAS

Images of the reflection nebula IC4954, taken by Akari’s near-mid-infrared camera (IRC) (left) and IRAS, the only previous infrared sky surveyor (right).

This image comparison shows the enormous improvement in resolution and sensitivity brought by Akari, which is already able to provide us with much more precise information about this star forming region than previous observations.

Launched in 1983, the IRAS Infra-Red Astronomical Satellite was the first mission to make a complete infrared survey of the entire sky. The mission resulted from the joint venture between the USA, United Kingdom, and the Netherlands. IRAS produced infrared maps of the Universe which have been used until the present day.




Image Credit: JAXA

These infrared images of the galaxy M81 were taken by the near- and mid-Infrared Camera (IRC) on board Akari. The observed wavelengths are 3, 4, 7, 11, 15, and 24 microns, respectively. M81 is a spiral galaxy located at a distance of about 12 million light years from us.

The images at 3 and 4 microns show the distribution of stars in the inner part of the galaxy without any obscuration from intervening dust clouds. At 7 and 11 microns it is possible to see the radiation from organic materials in the interstellar gas of the galaxy. The distribution of the dust heated by young hot stars is exhibited in the images at 15 and 24 micron, showing that the star forming regions sit along the spiral arms of the galaxy.

Dr Richard Savage, postdoctoral research fellow at the University of Sussex, said "It's wonderful to see the first images coming from the AKARI space telescope, after so much hard work by everyone on the project. It's particularly gratifying to see how well AKARI is functioning; this bodes extremely well for the science we will be able to produce from the mission." Michael Rowan-Robinson, Head of Astrophysics at Imperial College London, said: "The great power of the AKARI mission is that it is an all-sky survey in the far infrared with improved sensitivity and greatly improved resolution compared to the IRAS mission of the 1980s. It will be a major step forward at these wavelengths."

Dr. Seb Oliver (Reader in Astronomy at the University of Sussex) says "Dr. Richard Savage and I have just returned from Japan where we spent an exhausting time looking at the first data from Akari. We are delighted that everything appears to be performing just as we hoped and look forward to many exciting results to come."

Dr Chris Pearson, European Space Agency support astronomer to the Japanese at JAXA's Institute of Space and Aeronautical Science (ISAS), said "It is an enormous milestone for all those involved in the AKARI mission to finally see the fruits of their years of hard labour manifested in these breathtaking images of our infrared Universe. The team is now looking forward to producing an atlas of the entire infrared sky in addition to many more such beautiful images"

Particle Physics & Astronomy Research Council News Release