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tokens: ACKNOWLEDGEMENTS I acknowledge the support from the European Research Council (ERC) Consolidator Grant funding scheme ( project STARKEY , grant agreement number 615604) and from the Centre National d’Études Spatiales (CNES). I thank all the members of the STARKEY group and Professor Alessandro Bressan for the fruitful discussions. I thank the anonymous referee for carefully reading the manuscript and for the useful suggestions that improved this work. This work has made use of data from the European Space Agency (ESA) mission Gaia ( https://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.