Result of the initial testing of the Japanese ACA 12-m antenna to be delivered to ALMA

Result of the initial testing of the Japanese ACA 12-m antenna to be delivered to ALMA

18 March, 2008 / Read time: 3 minutes

In the Llano de Chajantor plateau (Figure 1) of the Atacama Desert, northern Chile, an international astronomical facility of Atacama Large Millimeter/submillimeter Array (ALMA) is currently being constructed in collaboration among Japan, North America, and Europe as an ultimate radio telescope at the millimeter/submillimeter wavelengths (Figure 2).

Japan constructs sixteen parabolic antennas for the Atacama Compact Array (ACA) as part of the ALMA, and three of them were assembled in Chile in the latter half of last year (Figure 3).

One of these three antennas (12 m in diameter) was equipped with a Japanese receiver and was used to obtain the first radio image of the moon at a wavelength of 2 mm (140 GHz). The obtained image shows clearly the temperature distribution of the moon and weak radio emission from the right half of the moon, which is dark in the optical image (Figure 4). This is the first radio image of this celestial object taken with a Japanese ALMA antenna in Chile.

Japan achieved this milestone with the ACA antenna as planned in its fourth year of the Japanese 8-year ALMA construction schedule, which will be completed in 2012.

After completion, ALMA will become a paramount radio telescope with a spatial resolution of 10 times higher than the Subaru Telescope or the Hubble Space Telescope. After it becomes fully operational in 2012, ALMA is expected to produce valuable information on the formation of the galaxy in the early universe and formation of the planetary system as well as the evolution of the universe, by taking the advantage of the millimeter/submillimeter wavelengths, which are very suitable to explore the mysteries of the universe.

This first radio image is one of the important milestones, which checked the fundamental antenna performances.


Figure 1: Assembled antennas are being tested in the mid-level facility

(altitude 2,900 m) near San Pedro de Atacama. They will be eventually
installed in the Chajantorplateau (altitude 5,000 m).

Figure 2: Conceptual drawing of ALMA. National Astronomical Observatory of
Japan constructs the Atacama Compact Array (ACA) System, which consists
of four 12-m antennas, twelve 7-m antennas, and a correlator for these Japanese
antennas, and millimeter/submillimeter receivers, etc. The red oval illustrates
high-precision parabolic antennas for the ACA, which will greatly enhance the
radio image quality from ALMA.
  Figure 3: First three Japanese ACA antennas assembled in Chile
  Figure 4: First Radio Image of the Moon Taken with an ACA Antenna
(Left: Optical image taken with a digital camera; Right: Radio image
taken with an ACA antenna).The radio image clearly shows the temperature
distribution of the moon, demonstrating the fundamental performances of the
antenna. The optical image shows the sun light reflected by the moon surface,
whereas the radio image shows the physical temperature distribution
of the moon. The radio image provides us with fruitful information which
cannot be obtained in the optical image.