Session
Technical Session XII: The Next Generation
Abstract
We present a CubeSat mission for the discovery of exoplanets down to 1 Earth radius around the nearest and brightest Sun-like stars. The spacecraft prototype―termed ExoplanetSat―is a 3U space telescope designed to monitor a single target from low Earth orbit. The optical payload will precisely measure stellar brightness, seeking the characteristic dip in intensity that indicates a transiting exoplanet. Once ExoplanetSat identifies a candidate exoplanet, larger assets can be used to conduct follow-up observations to characterize the atmospheric constituents. The prototype will serve as the basis of an eventual fleet of nanosatellites, each independently monitoring a single bright, nearby star. Given the spacecraft’s low mass and sub-pixel sensitivity variations in the science detector, image jitter and its resultant photometric noise is a primary concern. The attitude determination and control subsystem (ADCS) mitigates this using a two-stage pointing control architecture that combines 3-axis reaction wheels for arcminute-level coarse pointing with a piezoelectric translation stage at the focal plane for fine image stabilization to the arcsecond level. The ExoplanetSat optical design combines star camera and science functions into a single device that fits into the 3U form factor. This paper presents the ExoplanetSat science case, mission overview, concept of operations, and spacecraft configuration.
Presentation Slides
The ExoplanetSat Mission to Detect Transiting Exoplanets with a CubeSat Space Telescope
We present a CubeSat mission for the discovery of exoplanets down to 1 Earth radius around the nearest and brightest Sun-like stars. The spacecraft prototype―termed ExoplanetSat―is a 3U space telescope designed to monitor a single target from low Earth orbit. The optical payload will precisely measure stellar brightness, seeking the characteristic dip in intensity that indicates a transiting exoplanet. Once ExoplanetSat identifies a candidate exoplanet, larger assets can be used to conduct follow-up observations to characterize the atmospheric constituents. The prototype will serve as the basis of an eventual fleet of nanosatellites, each independently monitoring a single bright, nearby star. Given the spacecraft’s low mass and sub-pixel sensitivity variations in the science detector, image jitter and its resultant photometric noise is a primary concern. The attitude determination and control subsystem (ADCS) mitigates this using a two-stage pointing control architecture that combines 3-axis reaction wheels for arcminute-level coarse pointing with a piezoelectric translation stage at the focal plane for fine image stabilization to the arcsecond level. The ExoplanetSat optical design combines star camera and science functions into a single device that fits into the 3U form factor. This paper presents the ExoplanetSat science case, mission overview, concept of operations, and spacecraft configuration.
