De molekyler som skal til for at liv kan dannes på en planet kan observeres i støvskyer ude i rummet. Nogen forskere mener at fremkomsten af de livgivende stoffer ligefrem er en naturlig del af den proces der fører til stjernedannelsen.

Videnskabsjournalist fra Science Stories Jens Degett taler med Professor Liv Hornekær fra  Institut for Fysik og Astronomi på Århus Universitet om de mekanismer, som ligger bag dannelsen af liv.

Stjerner, støv og liv i rummet

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Science Stories fortæller historier om videnskab baseret på nysgerrighed og fascination af viden og indsigt, men vi kan også være kritiske og stille spørgsmål ved veletablerede dogmer. Vi stræber efter at forstå grundlaget for viden og sætte den i perspektiv. Redaktionen er uafhængig og ikke underlagt udefrakommende politiske eller kommercielle interesser.