BRITE-Constellation: Nanosatellites for Precision Photometry of Bright Stars

W. W. Weiß, S. M. Ruciński, A. F. J. Moffat, A. Schwarzenberg‐Czerny, Otto Koudelka, C. Cordell Grant, Robert Zee, R. Kuschnig, S. M. Mochnacki, J. M. Matthews,

Publications of the Astronomical Society of the Pacific · 2014 · 228 citations · 19 references

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Abstract

BRITE-Constellation (where BRITE stands for BRIght Target Explorer) is an inter-national nanosatellite mission to monitor photometrically, in two colours, the brightness and temperature variations of stars generally brighter than mag(V) ≈ 4, with precision and time coverage not possible from the ground. The current mission design consists of six nanosats (hence Constellation): two from Austria, two from Canada, and two from Poland. Each 7 kg nanosat carries an optical telescope of aperture 3 cm feeding an uncooled CCD. One instrument in each pair is equipped with a blue filter; the other with a red filter. Each BRITE instrument has a wide field of view ( ≈ 24 degrees), so up to about 15 bright stars can be observed simul-taneously, sampled in 32 pixel×32 pixel sub-rasters. Photometry of additional fainter targets, with reduced precision but thorough time sampling, will be possible through onboard data processing.

References

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