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A Cubesat Payload for Exoplanet Detection. | LitMetric

A Cubesat Payload for Exoplanet Detection.

Sensors (Basel)

INAF-Astrophysical Observatory of Capodimonte, Salita Moiariello, 16, 80131 Naples, Italy.

Published: March 2017

The search for undiscovered planets outside the solar system is a scientific topic that is rapidly spreading into the astrophysical and engineering communities. In this framework, the design of an innovative payload to detect exoplanets from a nano-sized space platform, like a 3U cubesat, is presented. The selected detection method is photometric transit, and the payload aims to detect flux decrements down to ~0.01% with a precision of 12 ppm. The payload design is also aimed at false positive recognition. The solution consists of a four-facets pyramid on the top of the payload, to allow for measurement redundancy and low-resolution spectral dispersion of the star images. The innovative concept is the use of a small and cheap platform for a relevant astronomical mission. The faintest observable target star has V-magnitude equal to 3.38. Despite missions aimed at ultra-precise photometry from microsatellites (e.g., MOST, BRITE), the transit of exoplanets orbiting very bright stars has not yet been surveyed photometrically from space, since any observation from a small/medium sized (30 cm optical aperture) telescope would saturate the detector. This cubesat mission can provide these missing measurements. This work is set up as a demonstrative project to verify the feasibility of the payload concept.

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Source
http://www.ncbi.nlm.nih.gov/pmc/articles/PMC5375779PMC
http://dx.doi.org/10.3390/s17030493DOI Listing

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