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astronautix.com Haruka


Other Designations: HALCA. Manufacturer's Designation: Muses-B. Code Name: VSOP. Class: Astronomy. Type: Radio. Nation: Japan. Agency: Institute of Space and Astronautical Sciences, Tok. Manufacturer: Nippon Electric Corp, Tokyo.

The Muses B satellite was renamed 'Haruka', meaning 'Far-away', after launch. It formed the space segment of the VLBI Space Observatory Program. Its 8 metre diameter radiotelescope antenna allowed very long baseline radio astronomy when used together with ground based radio telescopes of the VLBI Space Observatory Program. This resulted in very high resolution observations of deep-space radio objects. Its detectors operated at 1.6, 5 and 22 GHz.

HALCA (MUSES-B), the first astronomical satellite dedicated to Very-Long Baseline Interferometry (VLBI), was launched on its maiden flight by ISAS's M-V launch vehicle from Kagoshima Space Center on February 12, 1997.

As suggested by its development name MUSES-B, the satellite is the second in the series of ISAS's Mu Space Engineering Satellites. Since the satellite's successful deployment, in particular the main reflector mesh, and the testing of new engineering technologies incorporated within it, such as the two-way communications link between the satellite and tracking stations, HALCA has been used for space VLBI observations.

HALCA's telescope has a main reflector with an effective diameter of 8 m, consisting of a mesh of gold-coated molybdenum wire, suspended between six extendible masts and shaped by a tension-truss arrangement. It uses Cassegrain optics, with a hexagonal sub-reflector inscribed in a 1.1 m diameter circle.

The sub-reflector was deployed on February 24, 1997, and placed 3.4 m above the surface of the main reflector. Deployment of the main antenna masts took place over February 26-27, 1997. Radio waves were focused by the reflectors into a 2.5 m long feed horn.HALCA's telescope had a main reflector with an effective diameter of 8 m, consisting of a mesh of gold-coated molybdenum wire, suspended between six extendible masts and shaped by a tension-truss arrangement.

It used Cassegrain optics, with a hexagonal sub-reflector inscribed in a 1.1 m diameter circle. The sub-reflector was deployed on February 24, 1997, and placed 3.4 m above the surface of the main reflector. Deployment of the main antenna masts took place over February 26-27, 1997. Radio waves are focused by the reflectors into a 2.5 m long feed horn.

After launch, the satellite, known during its development as MUSES-B, was renamed HALCA - an acronym for the Highly Advanced Laboratory for Communications and Astronomy. HALCA was also a transliteration of the Japanese word "haruka", meaning far away, as HALCA's elliptical orbit took it out to an apogee 21,400 km above the Earth's surface, and, at the same time, it explored the mysteries of the distant universe.

The VSOP (VLBI Space Observatory Program) mission was led by the Institute of Space and Astronautical Science, in collaboration with the National Astronomical Observatory of Japan. The name VSOP reminded us of some kind of brandy, that is, "Very Superior Old Pale." The program was named by two professors who enjoyed a drink.


Specification


Haruka Chronology


12 February 1997 Haruka Program: Muses. Launch Site: Kagoshima . Launch Vehicle: M-V. Perigee: 569 km. Apogee: 21,415 km. Inclination: 31.4 deg.

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Last update 3 May 2001.
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