Star Anomaly is one of the most intriguing and unsolved discrepanciesbetween theoretical calculations and experimental data observed in the domain of few-nucleon systems at low energies. Previous and upcoming measurements of the breakup reaction with the use of the BINA detector enablesystematic studies of the Star configurations at intermediate energies. Adedicated simulation was developed to study feasibility of registering suchevents with the required accuracy and to support the future data analysis.An additional rotation angle β has been introduced to parametrise the Starconfigurations. First results concerning the acceptance of certain segmentsof BINA for registering the Star configurations are presented.
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