Srama, R.; Ahrens, T. J.; Altobelli, N.; Auer, S.; Bradley, J. G.; Burton, M.; Dikarev, V. V.; Economou, T.; Fechtig, H.; Görlich, M.et al.; Grande, M.; Graps, A. L.; Grün, E.; Havnes, O.; Helfert, S.; Horányi, M.; Igenbergs, E.; Jeßberger, E. K.; Johnson, T. V.; Kempf, S.; Krivov, A. V.; Krüger, H.; Moragas-Klostermeyer, G.; Lamy, P.; Landgraf, M.; Linkert, D.; Linkert, G.; Lura, F.; Mocker-Ahlreep, A.; McDonnell, J. A. M.; Möhlmann, D.; Morfill, G. E.; Müller, M.; Roy, M.; Schäfer, G.; Schlotzhauer, G. H.; Schwehm, G. H.; Spahn, F.; Stübig, M.; Svestka, J.; Tschernjawski, V.; Tuzzolino, A. J.; Wäsch, R.; Zook, H. A.: The Cassini Cosmic Dust Analyzer. Space Science Reviews 114, pp. 455 - 471 (2004)
A star’s chemical composition strongly influences the ultraviolet radiation it emits into space and thus the conditions for the emergence of life in its neighbourhood.
A single star has provided information about the collision of the Milky Way with the dwarf galaxy Gaia-Enceladus. The event likely took place approximately 11.5 billion years ago.