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Mouse: A Mini Observatory for UV Space Exploration of the Galactic Poles and Equator
Ist Teil von
Symposium - International Astronomical Union, 1994, Vol.161, p.52-54
Erscheinungsjahr
1994
Link zum Volltext
Quelle
Alma/SFX Local Collection
Beschreibungen/Notizen
The small orbiting observatory MOUSE is described in its essential features.
Insights in the optical solution (a 2 mirrors 3 reflections telescope using pure
hyperbolical surfaces, no aspherics) are given which fit such type of optical
layout to scientific requirements. An in-flight recentering of the photons
collected by a solar-blind photon counter device will allow for an equivalent
angular resolution of 2–3 arcsec over a field-of-view exceeding one square degree.
The capabilities of the proposed satellite (imaging, low resolution grisms,
polarizers) are described. The choice of the selected sky areas (the two Galactic
Poles, the galactic equator and some Bulge Windows) is justified in terms of
forefront astrophysical scientific objectives requiring imaging in UV over large
fields. The science comprises UV analysis of a complete sample of QSOs, stellar
population in galaxies, White Dwarfs, Globular and Open Clusters and OB
Associations. In addition a plan for the early UV detection of Supernova events is
described.