This page no longer updated from 31 October 2001. Latest version can be found at www.astronautix.com

astronautix.com ASTRO E

Astro-E
Astro-E -

29,202 bytes. 413 x 263 pixels.



Class: Astronomy. Type: X-Ray. Nation: Japan.

ASTRO-E was to be fifth in a series of Japanese astronomy satellites devoted to observations of celestial X-ray sources. It was to be a joint Japanese-US mission, with the US contributing significantly to two of the three types of instruments on-board. It was developed at Japan's Institute of Space and Astronautical Science (ISAS) in collaboration with other Japanese institutions, as well as NASA's Goddard Space Flight Center and the Massachusetts Institute of Technology (MIT).

ASTRO-E was designed for broad-band, high-sensitivity, high-resolution spectroscopy. Its instruments were not only sensitive to both low and high energy X-rays, but could distinguish very small differences in the energy of the X-ray photons detected.

ASTRO-E was to cover an energy range of 0.4 to 700 keV using three kinds of instruments with the following energy ranges:

ASTRO-E was planned to answer questions regarding the creation of the chemical elements, the consequences of matter falling onto black holes, and the processes of heating gases to X-ray emitting temperatures.

The 1,650 kg spacecraft was to conduct a five year mission in a 550 km circular orbit 550 km. Since the XRS had to be cooled to nearly absolute zero - 0.06 Kelvin - the instrument would only operate for the first two years of the mission while the on-board supply of solid neon coolant lasted.

ASTRO-E was to complement NASA's Chandra X-ray Observatory and ESA's XMM X-ray Multi-Mirror (XMM) spacecraft.

It was customary for Institute of Space and Astronautical Science satellites to have two names, one given before launch and one after. The pre-launch name was a project name that designated the series the satellite belonged to and a letter that designated what number that satellite was to be in that series. ASTRO-E was to be the fifth satellite in the 'ASTRO' series. The ASTRO series of satellites are often for cosmic X-ray astronomy, although one was a Solar X-ray astronomy satellite and ASTRO-F will be an infrared astronomy mission. Other series included 'MUSES' (engineering led projects), 'SOLAR', and 'PLANET'. The post-launch name was a proper name, chosen shortly after launch. Previous X-ray astronomy satellites have been renamed Hakucho (Swan, or the constellation Cygnus; was to be CORSA-B), Tenma (Heavenly Horse, or the constellation Pegasus; ASTRO-B), Ginga (Galaxy; ASTRO-C), and ASCA (ASTRO-D). The name 'ASCA' was a pun --- it's an acronym for Advanced Satellite for Cosmology and Astrophysics, and at the same time, sounds like the name from Japanese history, Asuka. Asuka was a region near Nara, and the name for a period in Japanese history (in the 7th century) when the Asuka region was her capital, and also the culture of that era.


Specification

Total Mass: 1,650 kg.


ASTRO E Chronology


10 February 2000 ASTRO E Launch Site: Kagoshima . Launch Vehicle: M-V. FAILURE: First stage failure. An anomalous vibration was detected 25 seconds after launch. At 41 seconds ceramic heat shields in the first stage nozzle broke and fell off, and thrust vector control on the nozzle was lost.

X-ray astronomy satellite. Stage 1 lost control, and separated with the rocket off-course at 75 seconds in the flight. Stage 2 burned correctly and separated at 218 seconds, followed by the third stage burn at 621 seconds. Last signals were received at 20 minutes after launch. ASTRO-E was to have separated from the third stage at 23 minutes, but ended in an orbit with a perigee of only 80 km and an apogee of 410 km. It probably reentered on the first orbit at around 0230 - 0300 GMT somewhere between East Africa and western China.



Back to Index
Last update 12 March 2001.
Contact Mark Wade with any corrections or comments.
Conditions for use of drawings, pictures, or other materials from this site..
© Mark Wade, 2001 .