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AKARI (ASTRO-F) > What's New Back Numbers
What's New Back Numbers
High Resolution Far-Infrared All-Sky Image Data Released (January 2015)
The AKARI Far-Infrared All-Sky image data are completed and released to the researchers across the world. The new AKARI image maps have four to five times better resolution than that of conventional far-infrared all-sky images, as well as data at longer wavelengths. The AKARI image data are expected to contribute to a very wide variety of astronomical studies, for instance in areas of star and planet formation and galaxy evolution.
AKARI made a step to a key to understand the material evolution in the universe (March 2014)
A team of astronomers based at the University of Tokyo has made a significant step in better understanding the material evolution of the universe. Led by Ms Tamami I. Mori, a research fellow for the Japan Society for the Promotion of Science, the study may help to give new insights into complex carbon chemistry in the galaxy.
Soccer Balls in Interstellar Space (March 5, 2013)
An international team of astronomers led by Masaaki Otsuka (Academia Sinica Institute of Astronomy and Astrophysics or ASIAA) has detected the C60 fullerene (molecules of carbon with 60 atoms arranged in patterns resembling a soccer ball) in the dying star M1-11. Multi wavelength observing data including that from AKARI take scientists closer to understanding the prevalence and formation of C60 in space.Soccer Balls in Interstellar Space - Subaru Telescope (External link)
AKARI Finds Carbon Monoxide Molecules Embedded in Ten Million Degree Gas (February 8, 2012)
A scientific team using the Japanese AKARI infrared space observatory finds carbon monoxide (CO) molecules in the ten million degree gas associated with the young supernova remnant Cassiopeia A (Cas A). The team is led by Dr. Jeonghee Rho, who holds a joint appointment at the SETI Institute, and at the SOFIA Science Center at NASA Ames Research Center (both located in Mountain View California). Theoretically it was neither predicted nor expected to find the carbon monoxide molecule associated with a highly energetic supernova remnant. Energetic electrons and heavy-element atoms produced by nuclear processes in supernovae should have destroyed these molecules. This finding could change our current understanding of the cycle of carbon and molecules in the interstellar gas and dust clouds.
AKARI detected the light from the first stars (October 2011)
Japanese infrared astronomy satellite AKARI measured the sky brightness at the wavelength of 1 ~ 4 micrometers and detected large spatial fluctuation that cannot be explained by the known sources. This fluctuation can be attributed to the clustering of the first stars of the universe, which were formed 300 million years after the Big Bang. The result will provide an important clue for the investigation of star formation history in the early universe for which little observational evidence has been found. The paper will be published in the November 1st issue of The Astrophysical Journal.
Gold dust collection in the sky:
AKARI reveals dusty veils enshrouding two Red Giant stars with unprecedented sensitivities and accuracies. The research would help to decipher the riddle of the cosmic reincarnation of matter surrounding the mystery of the origin of the basic chemical building blocks of life such as carbon.
Astronomy & Astrophysics is publishing a special feature devoted to the new results obtained with the infrared satellite AKARI, a JAXA project with the participation of ESA. It includes 17 articles dealing with various subjects. Some papers are based on the AKARI all-sky survey, which has just been released. Others are dedicated to pointed observations of many astronomical targets from solar system bodies to distant galaxies.
The AKARI Point Source Catalogues are in the public domain from March 30th, 2010. Far-Infrared and Mid-Infrared catalogues are available to world-wide researchers.
The latest news from AKARI project are presented. The initial version of the AKARI All-Sky Survey infrared source catalogue is now ready for scientific analysis. Three science highlights showing new insights to the activities between the old star / supernovae and interstellar media are presented from the second issue of the PASJ AKARI special issue.
We report on a pair of the initial scientific results from the Far-Infrared Surveyor (FIS); the observation of the nearby galaxy M101 and the deep far-infrared sky-survey programme. These results will be presented in the Annual Meeting of the Astronomical Society of Japan to be held at Gifu University in September 26th--28th, and also reported in the Publications of Astronomical Society of Japan (AKARI first results special issue). Note that AKARI's FIS instrument successfully completed its mission observations on the evening of this August 26th in Japan.
The asteroid explorer Hayabusa finally departed its target, the asteroid Itokawa, in late April this year and is now heading back home to the Earth. Last month, about three months after Hayabusa's encounter, on the 26th of July, 2007, the infrared astronomical satellite AKARI also succeeded in observing Itokawa with its onboard instrument, the Infrared Camera (IRC). Figure shows the image of Itokawa taken at a wavelength of 7 micrometres by AKARI. It can be clearly seen that Itokawa moves rapidly on the sky during the observation of about 12 minutes.
The first Japanese infrared astronomy satellite AKARI, launched in February 2006, continues observations in good condition. Further initial scientific results will be presented in the annual meeting of the Astronomical Society of Japan on the 28th - 30th of March 2007. Five selected results are explained here. On this occasion, the research concerns observations chiefly using the Near- and Mid-Infrared Camera (IRC), one of the instruments onboard AKARI.
AKARI continues its mission to map the entire sky in infrared light. AKARI commenced the mission's All-Sky Survey observations in May, 2006 and will finish its first coverage of the entire sky in November. During the survey observations, AKARI investigated one of the most important targets for studies of the formation of galaxies, the Large Magellanic Cloud, with more wavelength bands than has ever been made in the past, producing stunning images of our nearest neighbour in the Universe.
The Japan Aerospace Exploration Agency (JAXA) infrared astronomical satellite AKARI (formerly known as ASTRO-F) was launched on February 21st, 2006 (UT) from Uchinoura Space Centre, Japan. AKARI is continuing its' mission of surveying the entire sky, making a complete map of our cosmos in infrared light. Here we report two new exciting images recently made by AKARI, depicting scenes from the birth and death of stars.
The infrared satellite AKARI (formerly ASTRO-F) of the Japan Aerospace Exploration Agency (JAXA), which was launched from the Uchinoura Space Center on the 21st of February (UT), captured light for the first time when the telescope aperture lid was opened on the 13th of April. After the aperture lid was jettisoned the instruments became fully operational and their performance was confirmed. Following this, the telescope focus adjustment and the optimization of the attitude control system, etc., were successfully carried out.
We have moved from the performance verification (PV) phase to Phase 1 (real observations) of the mission. Infrared images of world class resolution and sensitivity has been presented to the general public.
AKARI has opened its' eye!
Because of trouble with the Sun sensors the opening of the aperture lid was postponed for about a month.
The operation was carried in the evening (in Japan) of April 13th. While the satellite was in contact with JAXA's Uchinoura Space Centre, the wire that fastens the lid was cut by the onboard time sequence program. Immediately after this, the signal from the FIS instrument dropped and we confirmed that it was observing the dark sky. After an orbit, the data transmitted to the ground confirmed that the Focal-Plane Star Sensor (FSTS) was seeing many stars and that the first glimpse of the galactic plane had been seen in part of the FIS data.
Now AKARI is in the performance verification phase. Both the FIS and IRC are operating fine. Some preliminary data have been obtained. Please stay tuned until we will present the first data to public in the near future.
The ASTRO-F satellite aboard the M-V Launch Vehicle No. 8 (M-V-8) has been launched at 6:28 a.m. on February 22, 2006 (Japan Standard Time, JST) from the Uchinoura Space Center (USC).
The ASTRO-F was given a nickname of "AKARI" (meaning a "light.")
Preparation of the ASTRO-F launch is progressing on schedule at JAXA's Uchinoura Space Center. The satellite has completed standalone tests and was connected onto the 3rd stage of the M-V-8 rocket. Function tests after the connection was also went successfully. The satellite is covered by the nose fairing and will be mounted on the 1st & 2nd stage of the rocket.
We have completed ASTRO-F integration tests in the ISAS Sagamihara campus, and shipped the spacecraft to the launch site, JAXA's Uchinoura Space Center (USC) in Kagoshima prefecture. The flight operation of ASTRO-F started on December 27th. On the 29th, we made the first functional tests of the satellite using the ground facilities in USC, and confirmed that the satellite is in healthy status.
Throughout the new year's days we carried out maintenance works of the mechanical cooler system and the thrusters. The flight operation of whole satellite system will start from January 10th.
ASTRO-F cleared the last hurdle of integration tests when the thermal vacuum test was successfully and safely completed. The Test began on the 1st of October and continued 24 hours a day until the 16th.
In the thermal vacuum test, the function of each component of the satellite was verified to operate correctly whilst maintaining the temperature corresponding to the severe environment of the vacuum of outer space. The assembled satellite was inserted into an enormous vacuum chamber, and the walls of the chamber were cooled with liquid Nitrogen after evacuation. A heater was placed beside the satellite to reproduce the same environment that the satellite components will endure in space.
It was confirmed that the temperature of the spacecraft body was controlled as expected and the equipment operated normally in this environment. This was also the last test to check the scientific instruments. Several problems that were pointed out during this test will be reflected in the final adjustments before the launch.
With the completion of this test, ASTRO-F moves one step closer to launch.
A portion of the ASTRO-F pointed observation opportunities has been made available to the wider astronomical community outside the ASTRO-F project team for open time proposals.
Observation opportunities with ASTRO-F have been announced to scientists in Japan/Korea and ESA member state countries. This announcement for open time was made on September 20th and will close on November 18th 6:00 (UT).
This observation time opportunity in the so called Phase 2 of the mission. Twenty per cent of pointed observations have been reserved for Japanese and Korean open time as well as ten per cent for European astronomers.
All the information for the open time opportunities can be found on the observers web page.
We held Open Time Proposal Preparation Workshops in four countries, namely in the U.K., Spain (ESAC/ESA), Korea, and Japan. There were 20-50 participants at every meeting and the general atmosphere was enthusiastic.
ASTRO-F satellite is under the final integration test since March, and things are going well so far.
In May we had carried out a full configuration vibration test and confirmed that all system functions perfectly. Special attention was paid to the telescope system which had trouble two years ago. We opened the aperture lid of the cryostat (a capsule to keep the telescope and scientific instruments in vacuum and low-temperature) and checked the optical axis of the telescope. The same measurement was made in last October immediately after the installation of the telescope. Comparison of two measurements assured that there is no effective change of the axis; i.e. the telescope is tough enough against the vibration at the launch.
The aperture was closed again (this was the last chance for us to see the instruments on ground), and prepared for the cryogenic tests.
In parallel, the satellite bus module experienced "baking" process. It was installed in the space chamber, then warmed up to about 50 C in vacuum. This process removes unnecessary "out gas" from the parts of the satellite which might contaminate the instruments in orbit. After about one week baking the bus module was safely back in the clean room. Note that the cryostat and scientific instruments have been baked already and did not participate this time.
The cryogenic test of the ASTRO-F scientific instruments, cryogenic system, telescope and the insturments was carried out from November 30th - December 8th at the Sumitomo Heavy Industries plant in Niihama. This is the first test since they were assembled in the flight configuration in last August. The cryogenic system performed correctly and the instruments inside cooled to the expected temperature. Every instrument functioned correctly and a lot of data was taken. This data will be analyzed and subsequently used to estimate the final pre-launch performances.
Then, the instruments were brought back to ISAS and a cryogenic vibration test was carried out. There was no change in the system before or after the test, and it was confirmed that the instruments will be able to withstand the launch conditions.
With the success of the present tests, the instrument development has conquered a significant mountain in the development of the ASTRO-F project.
The first photograph shows a rare and interesting view of the telescope looking down into the aperture of the cryostat (which is usually sealed up until the satellite is in orbit). This picture was taken during the alignment test of the telescope carried out at the Sumitomo Heavy Industries Niihama factory in the first week of October, 2004. As the telescope improvement was successively completed, we need to check whether the telescope will still in good condition after the vibration tests of the cryostat. This will be done by measuring the telescope light axis. To confirm the test procedures and also to obtain the reference data, we carried out this first test. The test was successful. We were able to measure the light axis to an accuracy of 1/200 degree.
The second photo is also a rare view; the focal plane as seen through the telescope. We can see the IRC detectors just below the center, the FIS entrance aperture is on the left. The focal-plane star sensors are seen in the bottom-left and top of the image.
The final check of the telescope axis after the vibration test will be made next spring.
In the final climax of the reparation of the ASTRO-F Telescope, the vibration test under cryogenic temperature was carried out at ISAS between 28th June and the 1st July. Some inspections and measurements were made after the test, and the telescope passed them without difficulty.
Then followed the test to evaluate the performance of the ASTRO-F telescope at the lowest temperatures. In the test, we obtained detailed data on the focus position, etc.
The final performance evaluation test (FPI integration test) of the two Focal Plane Instruments (FIS, IRC) was carried out from the beginning of June to the 31st of July over three cooling cycles.
From now, the satellite will undergo the final assembly phase and the instruments together with the telescope will be sent to the Sumitomo Heavy Industries (SHI) factory in Niihama where they will be installed into the cryostat. The instruments will not be turned on again until November.
In continuing the refurbishment of the ASTRO-F telescope, the polishing of the back-up primary mirror was begun. The grinding was successfully completed at the beginning of March. The new mirror will be used as the new flight model mirror. Correspondingly, the diameter of the mirror has been increased by 2 cm to 69 cm, becoming closer to the original design specification of 70 cm.
Following this, the new mirror will be adhered to the new pads and the telescope will be assembled. Then the telescope will be cooled and the performance under flight conditions measured. This time, drawing on previous experience and by paying attention to minute detail, we will minimize the effects of the thermal distortion.top:surface, bottom:backside
The second AOCS (Attitude and Orbit Control System) test that was being carried out since the middle of January, finally finished on the 19th March. The main objective of this test was to confirm that the satellite would operate as expected in the case of a Summer launch. Furthermore, the detailed AOCS performance was also evaluated. It was confirmed that even if the launch date changed that the AOCS could work correctly both in the launch operation and regular operation. The data will be analyzed in detail and reviewed around May.
Since April 2003 we have been carrying out the final integration test of the ASTRO-F satellite. The satellite was built up into the flight configuration, then intensive tests of the individual components, as well as the whole satellite system were performed. In late October we carried out a simulation of the launch and observation operations. However, because of the telescope trouble (found after we started the test) and the subsequent delay of the launch, the test had to be paused after we completed the bus module tests. The first period was finished with the review meeting on the November 7th. The satellite will be preserved in ISAS's clean room. The integration test will be restarted in December 2004, together with the telescope and focal-plane instruments. We will try our best to improve the performance of the instruments as much as possible in this one-year period.
The 4th FPI evaluation test in cryostat (FEC#4) was carried out at Sumitomo Heavy Industries, Ltd.(SHI) in Niihama city. The principal purpose of the test was to evaluate the performance of the focal plane instruments (FPIs).
The main observation plans of ASTRO-F are arranged as mission programs (MPs) before the launch by concerned scientists around the world. The fourth symposium to discuss the MPs was held at ISAS (Institute of Space and Astronautical Science) in June 2003.
The final integration test of ASTRO-F has begun. Photo shows the satellite bus module of ASTRO-F which was assembled in a clean room at ISAS. The solar battery paddle around the module will be extended in space.
The mechanical interface between the ASTRO-F satellite and the M-V-6 rocket was confirmed at Tomioka Factory of IHI Aerospace.
A meeting of the ASTRO-F data reduction team was held at University of Sussex in the UK. Scientists from Japan, Korea, UK, and the Netherlands discussed many topics on data reduction.
Drs. Salama, Gry, and Garcia-Lario of ESA/ISO data centre have visited ISAS. ESA has been involved in the ASTRO-F collaborator. We discussed user support for European astronomers and the pointing reconstruction during the survey observation.
The Focal Plane Instruments (FPIs) which was installed into the satellite came back to ISAS after the 1st integration test. Improvement and tune-up of the instruments will continue until next year.
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