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Fast spin of the young extrasolar planet β Pictoris b

Author

Listed:
  • Ignas A. G. Snellen

    (Leiden Observatory, Leiden University, Postbus 9513, 2300 RA Leiden, The Netherlands)

  • Bernhard R. Brandl

    (Leiden Observatory, Leiden University, Postbus 9513, 2300 RA Leiden, The Netherlands)

  • Remco J. de Kok

    (Leiden Observatory, Leiden University, Postbus 9513, 2300 RA Leiden, The Netherlands
    Netherlands Institute for Space Research (SRON), Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands)

  • Matteo Brogi

    (Leiden Observatory, Leiden University, Postbus 9513, 2300 RA Leiden, The Netherlands)

  • Jayne Birkby

    (Leiden Observatory, Leiden University, Postbus 9513, 2300 RA Leiden, The Netherlands)

  • Henriette Schwarz

    (Leiden Observatory, Leiden University, Postbus 9513, 2300 RA Leiden, The Netherlands)

Abstract

Near-infrared spectroscopic observations of the young extrasolar planet β Pictoris b indicate that it spins significantly faster than any planet in the Solar System, in line with the extrapolation of the known trend in spin velocity with planet mass.

Suggested Citation

  • Ignas A. G. Snellen & Bernhard R. Brandl & Remco J. de Kok & Matteo Brogi & Jayne Birkby & Henriette Schwarz, 2014. "Fast spin of the young extrasolar planet β Pictoris b," Nature, Nature, vol. 509(7498), pages 63-65, May.
    • Handle: RePEc:nat:nature:v:509:y:2014:i:7498:d:10.1038_nature13253
    DOI: 10.1038/nature13253
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    Cited by:

    1. Ken Rice, 2014. "The Detection and Characterization of Extrasolar Planets," Challenges, MDPI, vol. 5(2), pages 1-28, September.

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