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Deficiency of molecular hydrogen in the disk of β Pictoris

Nature volume 412, pages 706–708 (2001)Cite this article

Abstract

Molecular hydrogen (H2) is by far the most abundant material from which stars, protoplanetary disks and giant planets form, but it is difficult to detect directly. Infrared emission lines from H2 have recently been reported1 towards β Pictoris, a star harbouring a young planetary system2. This star is surrounded by a dusty ‘debris disk’ that is continuously replenished either by collisions between asteroidal objects3 or by evaporation of ices on Chiron-like objects4. A gaseous disk has also been inferred from absorption lines in the stellar spectrum5,6,7,8. Here we present the far-ultraviolet spectrum of β Pictoris, in which H2 absorption lines are not seen. This allows us to set a very low upper limit on the column density of H2: N(H2) ≤ 1018 cm-2. This non-detection is puzzling when compared to the quantity of H2 inferred from the infrared observations, but it does show that H2 is not in the disk on the direct line of sight. Carbon monoxide (CO) has been seen in absorption against the star8,9,10, yielding a ratio of CO/H2 > 6 × 10-4. As CO would be destroyed under ambient conditions in about 200 years (refs 9, 11), our result demonstrates that the CO in the disk arises from evaporation of planetesimals.

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Figure 1: Far ultraviolet spectrum of β Pic from 905 to 1,188 Å, as obtained by the FUSE satellite.
Figure 2: Plot of the observed O vi emission doublet and H2 absorption lines.

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Acknowledgements

We thank Gopal-Krishna, G. Pineau des Forêts and S. Cabrit for discussions, and R. Kurucz for providing a model of the β Pic stellar atmosphere. The work at Johns Hopkins University was supported by NASA; the work at the Institut d’Astrophysique de Paris and at LAM was supported by CNES. The work reported here is based on data obtained by the NASA-CNES-CSA FUSE mission, operated by the Johns Hopkins University.

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Authors and Affiliations

  1. Institut d’Astrophysique de Paris, CNRS, 98 bis bld Arago, Paris, F-75014, France

    A. Lecavelier des Etangs, A. Vidal-Madjar, J.-M. Désert, R. Ferlet, G. Hébrard & M. Lemoine

  2. Department of Physics and Astronomy, Johns Hopkins University, Baltimore, 21218, Maryland, USA

    A. Roberge, P. D. Feldman, M. André, W. P. Blair, S. Friedman & H. W. Moos

  3. Laboratoire d'Astrophysique de Marseille, BP 8, Marseille, F-13376 Cedex 12, France

    M. Deleuil & J.-C. Bouret

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  1. A. Lecavelier des Etangs
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Correspondence to A. Lecavelier des Etangs.

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Lecavelier des Etangs, A., Vidal-Madjar, A., Roberge, A. et al. Deficiency of molecular hydrogen in the disk of β Pictoris. Nature 412, 706–708 (2001). https://doi.org/10.1038/35089006

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