Minisat-1 (LEGRI)


Minisat-1


* Mission Overview

The Minisat-1 mission was a Spanish-led mission with a primary instrument being the Low Energy Gamma-ray Imager (LEGRI), a coded masked prototype instrument. The satellite was launched on April 21, 1997 from a Pegasus XL rocket (a “winged” rocket dropped from an aircraft) and the LEGRI instrument onboard was activated on May 19, 1997. The instrument was a collaboration between the University of Valencia, University of Alicante, Centro de Investigaciones Energeticas, Medioambientales y Technologicas (CIEMAT), Instituto Nacional de Technica Aerospacial (INTA), University of Southampton, University of Birmingham, and the Rutherford Appleton Laboratory.

Minisat-1 was the first operational mission in the Minisat series. It was planned with a two year mission span, but ultimately operated sucessfully for five years before re-entry into the Earth’s atmosphere. LEGRI was not the only instrument on MiniSat-1, but is the primary one of interest to high-energy astrophysics.

* Instrumentation

LEGRI was a coded mask array gamma ray detector. The detector plane was a mosaic of 10 x 10 of 80 HgI2 and 20 CdZnTe crystals 0.5 cm thick with an active area of 1 cm2: the mixed detectors were intended to test differing technologies under identical conditions. The detector was passively shielded on the back and sides by the mechanical assembly and by a tantalum collimator and aluminium window in the pointing direction. The coded mask was mounted 540 mm in front of the instrument and was made of tungsten elements attached to a honeycomb plate and support structure. A start sensor allowed precise tracking of attitude of the spacecraft to permit ground-based analysis without blurring from spacecraft motion. The instrument has a spatial resolution of 20 arcminutes, and could perform moderate spectroscopy (with 4 keV resolution at 30 eV).

* Science

LEGRI was primarily a proof-of-concept mission for coded-mask gamma-ray imaging. Having shown the concept worked, LEGRI detected and characterized gamma-ray burst sources in particular.


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Page authors: Lorella Angelini Jesse Allen
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