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By using an array of high-sensitivity CCD video devices and spectrographs,the activity of meteor events from the poorly-known $\rho$-Geminid meteoroidstream has been monitored during January 2012 and 2013. As a result of thisresearch, the atmospheric trajectory and radiant position of 10 of these eventshas been obtained, but also the orbital parameters of the progenitor meteoroidsand the tensile strength of these particles. The data reveal that theprogenitor of this stream must be a comet. In addition, the emission spectraproduced by three $\rho$-Geminid meteors were also recorded. These are thefirst $\rho$-Geminid spectra discussed in the scientific literature, and haveprovided clues about the chemical nature of these meteoroids and their parentbody.

The $\rho$-Geminid meteoroid stream: orbits, spectroscopic data and implications for its parent body