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AKARI (ASTRO-F)
Purpose of Mission
Outline of Satellite
Focal Plane Instruments
Operation Plan
Scientific Targets
Results
Outreach - Q & A -
AKARI (ASTRO-F)

AKARI (Previously known as ASTRO-F or IRIS - InfraRed Imaging Surveyor) is the second space mission for infrared astronomy in Japan. AKARI has been developed by members of JAXA/ISAS and collaborators. IRAS (Infrared Astronomical Satellite, launched in 1983 by the United Kingdom, the United States, and the Netherlands) carried out the first all-sky survey at infrared wavelengths and made a huge impact on astronomy. The AKARI mission is an ambitious plan to make an all-sky survey with much better sensitivity, spatial resolution and wider wavelength coverage than IRAS. AKARI has a 68.5cm telescope cooled down to 6K, and will observe in the wavelength range from 1.7 (near-infrared) to 180 (far-infrared) micron. AKARI was successfully launched into space by a M-V rocket. AKARI has been placed in a sun-synchronous polar orbit of about 700 km.

AKARI finishes its cool observations (August 28, 2007)

AKARI Conference 2009

AKARI, a light to illuminate the misty Universe
February 16 - 19, 2009 Fukutake Hall, The University of Tokyo, Tokyo, Japan
http://akari2009.com/

What's New

AKARI: current status and recent science highlights (November 2008)

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.

FIS All-Sky Map

Results Page

Press Release (ISAS/JAXA Topics)

For Astronomers
U.K. Site ESAC/ESA Site Korean Site
JAXA/ISAS Home Page
JAXA Institute of Space and Astronautical Science
LIRA Home Page
Infrared Astrophysics Group