Skip to main content

Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

  • News & Views
  • Published:

Astrochemistry

Insights into ultrafast H3+ formation provide a glimpse into primordial chemistry

When atoms first appeared in the Universe, molecules were needed to help coalesce them into stars. The trihydrogen cation H3+ is among the prime candidates for that process, and now two independent studies provide detailed insight into the ultrafast dynamics of the formation of this important ion from two hydrogen molecules.

This is a preview of subscription content, access via your institution

Access options

Buy this article

Prices may be subject to local taxes which are calculated during checkout

Fig. 1: Sketch of the experimental set-up.

References

  1. Mi, Y. et al. Nat. Chem. https://doi.org/10.1038/s41557-023-01231-z (2023).

    Article  PubMed  Google Scholar 

  2. Zhou, L. et al. Nat. Chem. https://doi.org/10.1038/s41557-023-01230-0 (2023).

    Article  PubMed  PubMed Central  Google Scholar 

  3. Hogness, T. R. & Lunn, E. G. Proc. Natl Acad. Sci. USA 10, 398–405 (1924).

    Article  CAS  PubMed  PubMed Central  Google Scholar 

  4. Thomson, J. J. Phil. Mag. 21, 225–249 (1911).

    Article  CAS  Google Scholar 

  5. Herbst, E. & Klemperer, W. Astrophys. J. 185, 505–534 (1973).

    Article  CAS  Google Scholar 

  6. Hamilton, D. C. et al. Geophys. Res. Lett. 7, 813–816 (1980).

    Article  CAS  Google Scholar 

  7. Drossart, P. et al. Nature 340, 539–541 (1989).

    Article  CAS  Google Scholar 

  8. Oka, T. & Jagod, M.-F. J. Chem. Soc. Faraday Trans. 89, 2147–2154 (1993).

    Article  CAS  Google Scholar 

  9. Geballe, T. & Oka, T. Nature 384, 334–335 (1996).

    Article  CAS  PubMed  Google Scholar 

  10. McCall, B. J. et al. Astrophys. J. 567, 391 (2002).

    Article  CAS  Google Scholar 

  11. Koskinen, T. T., Aylward, A. D. & Miller, S. Nature 450, 845–848 (2007).

    Article  CAS  PubMed  Google Scholar 

  12. Eland, J. H. D. Rapid Commun. Mass Spectrom. 10, 1560–1562 (1996).

    Article  CAS  Google Scholar 

  13. Hoshina, K., Furukawa, Y., Okino, T. & Yamanouchi, K. J. Chem. Phys. 129, 104302 (2008).

    Article  PubMed  Google Scholar 

  14. Ekanayake, N. et al. Sci. Rep. 7, 4703 (2017).

    Article  PubMed  PubMed Central  Google Scholar 

  15. Scherer, N. F., Khundkar, L. R., Bernstein, R. B. & Zewail, A. H. J. Chem. Phys. 87, 1451–1453 (1987).

    Article  CAS  Google Scholar 

  16. Calvert, C. R., Bryan, W. A., Newell, W. R. & Williams, I. D. Phys. Rep. 491, 1–28 (2010).

    Article  CAS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Marcos Dantus.

Ethics declarations

Competing interests

The author declares no competing interests.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Dantus, M. Insights into ultrafast H3+ formation provide a glimpse into primordial chemistry. Nat. Chem. 15, 1202–1203 (2023). https://doi.org/10.1038/s41557-023-01298-8

Download citation

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1038/s41557-023-01298-8

Search

Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing