The BRITE Constellation nanosatellite mission: Testing, commissioning and operations
arXiv:1608.00282 · doi:10.1088/1538-3873/128/970/125001
Abstract
BRITE (BRIght Target Explorer) Constellation, the first nanosatellite mission applied to astrophysical research, is a collaboration among Austria, Canada and Poland. The fleet of satellites (6 launched, 5 functioning) performs precise optical photometry of the brightest stars in the night sky. A pioneering mission like BRITE - with optics and instruments restricted to small volume, mass and power in several nanosatellites, whose measurements must be coordinated in orbit - poses many unique challenges. We discuss the technical issues, including problems encountered during on-orbit commissioning (especially higher-than expected sensitivity of the CCDs to particle radiation). We describe in detail how the BRITE team has mitigated these problems, and provide a complete overview of mission operations. This paper serves as a template for how to effectively plan, build and operate future low-cost niche-driven space astronomy missions.
54 pages, 12 figures, accepted by PASP
Cited by in corpus (21)
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- Machine learning search for variable stars
- The Most Massive Heartbeat: An In-depth Analysis of ι Orionis
- BRITE-Constellation: Data processing and photometry
- Revisiting the pulsational characteristics of the exoplanet host star Pictoris
- X-ray Spectroscopy of the gamma-ray Brightest Nova V906 Car (ASASSN-18fv)
- Seismic modelling of early B-type pulsators observed by BRITE: I. Ophiuchi
- Lupi: measuring the heartbeat of a doubly-magnetic massive binary with BRITE-Constellation
- The variability of the BRITE-est Wolf-Rayet binary, Velorum I. Photometric and spectroscopic evidence for colliding winds
- The chaotic wind of WR 40 as probed by BRITE
- The Pictoris b Hill sphere transit campaign. Paper I: Photometric limits to dust and rings
- BRITE-Constellation reveals evidence for pulsations in the enigmatic binary Carinae
- BRITE-Constellation photometry of $\bpi^5$ Orionis, an ellipsoidal SPB variable
- Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE - Constellation
- Constraining the near-core rotation of the gamma Doradus star 43 Cygni using BRITE-Constellation data
- Space Photometry with BRITE-Constellation
- BRITE observations of Centauri and Lupi, the first non-eclipsing members of the new class of nascent binaries
- Evolving pulsation of the slowly rotating magnetic Cep star CMa
- New BRITE-Constellation observations of the roAp star Alpha Circini
- Spectrum of the secondary component and new orbital elements of the massive triple star Delta Ori A
- Optimization of exposure time division for wide field observations