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.
arXiv comment54 pages, 12 figures, accepted by PASP
References in corpus (4)
- Kepler Mission Design, Realized Photometric Performance, and Early Science
- The CoRoT satellite in flight : description and performance
- BRITE-Constellation: nanosatellites for precision photometry of bright stars
- Massive pulsating stars observed by BRITE-Constellation. I. The triple system Beta Centauri (Agena)
Cited by in corpus (48)
- Probing the interior physics of stars through asteroseismology
- Advances in Space Quantum Communications
- Gaia Data Release 2: Variable stars in the colour-absolute magnitude diagram
- On the sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars
- Forward asteroseismic modeling of stars with a convective core from gravity-mode oscillations: parameter estimation and stellar model selection
- BRITE-Constellation high-precision time-dependent photometry of the early-O-type supergiant Puppis unveils the photospheric drivers of its small- and large-scale wind structures
- Machine learning search for variable stars
- Triple system HD 201433 with a SPB star component seen by BRITE-Constellation: Pulsation, differential rotation, and angular momentum transfer
- The Most Massive Heartbeat: An In-depth Analysis of ι Orionis
- BRITE-Constellation: Data processing and photometry
- Short-term variability and mass loss in Be stars III. BRITE and SMEI satellite photometry of 28 Cygni
- 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
- Short-term variability and mass loss in Be stars IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of Puppis (B7-8 IIIe)
- The variability of the BRITE-est Wolf-Rayet binary, Velorum I. Photometric and spectroscopic evidence for colliding winds
- Lupi: measuring the heartbeat of a doubly-magnetic massive binary with BRITE-Constellation
- beta Cas: the first delta Scuti star with a dynamo magnetic field
- Short-term variability and mass loss in Be stars V. Space photometry and ground-based spectroscopy of Cas
- Studying the photometric and spectroscopic variability of the magnetic hot supergiant Orionis Aa
- A BRITE view on the massive O-type supergiant V973 Scorpii: Hints towards internal gravity waves or subsurface convection zones
- The K2 Bright Star Survey I: Methodology and Data Release
- The chaotic wind of WR 40 as probed by BRITE
- Let there be more variability in two gamma Cas stars
- The Pictoris b Hill sphere transit campaign. Paper I: Photometric limits to dust and rings
- Point Spread Function Estimation for Wide Field Small Aperture Telescopes with Deep Neural Networks and Calibration Data
- 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
- Fermi-LAT Observations of V549 Vel 2017: a Sub-Luminous Gamma-Ray Nova?
- 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
- BRITE photometry and STELLA spectroscopy of bright stars in Auriga: Rotation, pulsation, orbits, and eclipses
- BRITE photometry of the massive post-RLOF system HD149404
- Magnetic characterization and variability study of the magnetic SPB star o Lup
- Evolving pulsation of the slowly rotating magnetic Cep star CMa
- Radial oscillations and gravitational wave echoes of strange stars with nonvanishing lambda
- On the nature of the single eclipse per 80d orbit of the H-rich luminous WN star WR22
- A search for transiting planets in the Pictoris system
- Five years of BRITE-Constellation photometry of the luminous blue variable P Cygni: properties of the stochastic low-frequency variability
- 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
- Photometry of Beta Lyrae in 2018 by the BRITE satellites
- Light-curve instabilities of Beta Lyrae observed by the BRITE satellites
- Onboard Dynamic Image Exposure Control for the Star-Planet Activity Research CubeSat (SPARCS)
- Halo Photometry and Asteroseismology for 98 of the Brightest Stars Observed by TESS
- Optimization of exposure time division for wide field observations