Episodic formation of cometary material in the outburst of a young Sun-like star

Abstract

The Solar System originated in a cloud of interstellar gas and dust. The dust is in the form of amorphous silicate particles1,2 and carbonaceous dust. The composition of cometary material, however, shows that a significant fraction of the amorphous silicate dust was transformed into crystalline form during the early evolution of the protosolar nebula3. How and when this transformation happened has been a question of debate, with the main options being heating by the young Sun4,5 and shock heating6. Here we report mid-infrared features in the outburst spectrum of the young Sun-like star EX Lupi that were not present in quiescence. We attribute them to crystalline forsterite. We conclude that the crystals were produced through thermal annealing in the surface layer of the inner disk by heat from the outburst, a process that has hitherto not been considered. The observed lack of cold crystals excludes shock heating at larger radii.

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Figure 1: Silicate emission in the 8–12-μm range.

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Acknowledgements

We are grateful to A. F. Jones for providing us with timely visual observations of EX Lupi during the preparation of our infrared measurements. The presented work was partly supported by the Hungarian Research Fund. The research of Á.K. is supported by the Netherlands Organization for Scientific Research.

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Correspondence to P. Ábrahám.

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Ábrahám, P., Juhász, A., Dullemond, C. et al. Episodic formation of cometary material in the outburst of a young Sun-like star. Nature 459, 224–226 (2009). https://doi.org/10.1038/nature08004

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