Do have nanosatellites a role in detecting exoplanets?
Werner W. Weiss, Vera Maria Passegger, Jason Rowe

TL;DR
This paper evaluates the potential of nanosatellites, specifically the BRITE-Constellation, to detect exoplanets through high-precision photometry, estimating that about six planets could be detected in a 180-day observation period.
Contribution
It introduces a simulation assessing BRITE-Constellation's capability to detect exoplanets, considering technical constraints and stellar data, which is a novel application for nanosatellites.
Findings
Approximately six exoplanets could be detected in 180 days.
Most detectable planets are expected to be Jupiter-sized.
The detection capability depends on observation duration and duty cycle.
Abstract
In December 2012, Austria will launch its first two satellites: UniBRITE and BRITE-Austria. This is the first pair of three, forming a network called BRITE-Constellation. The other pairs being contributed by Canada and Poland. The primary goal of BRITE-Constellation is the exploration of short term intensity variations of bright stars (V>6 mag) for a few years. For each satellite pair, one will employ a blue filter and the other a red filter. With the discovery of the first exoplanet in 1992, more than 800 have been detected since. The high-precision photometry from the BRITE instrument will enable a transit search for exoplanets around bright stars. To estimate the capability of BRITE to detect planets, we include in our calculations technical constraints, such as photometric noise levels for stars accessible by BRITE, the duty cycle and duration of observations. The most important…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Spacecraft Design and Technology · Astronomy and Astrophysical Research
