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"Japanese infrared space observatory goes into orbit", "ATRO-F (AKARI) Satellite details 2006-005A NORAD 28939", "JAXA Hopes To Keep Akari Going Despite Power Failure", "The Infrared Astronomical Satellite AKARI and Nikon", "Current Status of the AKARI Mission After one year of observations", "Asteroid Catalog Using AKARI: AKARI/IRC Mid-Infrared Asteroid Survey", http://www.dajf.org.uk/wp-content/uploads/DAP-2013-fact-sheet.doc, http://www.ir.isas.jaxa.jp/ASTRO-F/Observation/PSC/Public/, Star formation over three generations in the, The first infrared detection of a supernova remnant in the, Detection of mass-loss from relatively young red-giant stars in the, Detection of the molecular gas surrounding the, Active star formation viewed from the outside: The peculiar spiral galaxy, Superscripts indicate joint development with. We also carried out an operation called "baking" to prevent gases with impure objects that come out from the onboard equipment and electronic mother boards from negatively impacting the devices. Since its launch on February 22. Photo 2: ASTROF observation equipment under the vibration test in Sagamihara. As part of the renovations and countermeasures, we polished a backup mirror, and that was successfully completed in early March. 4754 Panthoos is a Jupiter trojan from the Trojan camp, approximately 53 kilometers in diameter. AKARI operated with a 68.5 cm-diameter telescope cooled down to 6K and observed in the wavelength range 2-180 µm from a sun-synchronous polar orbit at 700 km altitude. Second (phase-2) all-sky survey started on 10 November 2006.

The paper will be published in the November 1st issue of The Astrophysical Journal. [11], During December 2007, JAXA performed orbit correction manoeuvres to bring Akari back into its ideal orbit. 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. Therefore, the discovery this time was unexpected. It is likely spherical in shape and has a longer-than-average rotation period of 27.68 hours. Following the end of its mission, the 1.1 metric-ton satellite was not deorbited and constitutes a space hazard. The infrared astronomy satellite AKARI started the regular observations in May 2006. The finding became very helpful and contains important data that can help reveal the origin of a planet and life, as there are still lots of mysteries in how dust, one of raw materials to help create a planet, is formulated and destroyed by supernova explosions. The purpose of the test is to ensure the AOCS performs smoothly in its early phase, even if the launch season is changed. AKARI is now in its Post-Helium phase, where imaging and spectroscopic capabilities are available in the 1.8 to 5.5 micron wavelength range. It was discovered on 2 November 1991, by Belgian astronomer Eric Elst at the La Silla site of the European Southern Observatory in Chile. Akari (ASTRO-F) was an infrared astronomy satellite developed by Japan Aerospace Exploration Agency, in cooperation with institutes of Europe and Korea.

Measurements made with the Hipparcos spacecraft show an annual parallax shift of 0.04385″, which is equivalent to a distance of around 74.4 ly (22.8 pc) from the Sun. The AKARI asteroid catalogue is constructed by laborious processes from the enormous quantity of data of the AKARI All-Sky Survey observations, like collecting gold dust. Discover the beauty hidden in the maps. Photo 1: The ASTRO-F after it just completed the test: You can see the wiring for the thermometers andheaters set for the test.

The Large Magellanic Cloud is an important observation target to study the birth of the Galaxy.

This was necessary because the boiled off helium led to an increase in altitude. AKARI ran out of its on-board supply of cryogen, liquid Helium at 08:32:40 (UT) on August 26th, 2007, after successful operation and observations that began on May 8th, 2006, achieving the expected lifetime of 550 days. [13], The Akari All-Sky Survey Point Source Catalogues was released on 30 March 2010.

The in-orbit ASTRO-F was given a nickname of "Akari" (meaning a "light.")

Photo 1: Looking into the telescope (right) and measuring the light axis (by NIKON) Photo 2: The satellite put in the vacuum chamber for baking. Its motto is One JAXA and its corporate slogan is Explore to Realize.

Photo 2: Explanatory session at the European Space Astronomy Center (Spain).

This test was carried out with equipment that included a gyro detached from the satellite and placed on the fixed board (as seen in the front of the photo) so as not to be impacted by vibrations from the outside. It will finish its first coverage of the entire sky in early November following almost 6 months of observations.

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