A

Why every observatory needs a disco ball

Physics Education, vol. 59, pp. 025012

Abstract

Abstract Commercial disco balls provide a safe, effective and instructive way of observing the Sun. We explore the optics of solar projections with disco balls, and find that while sunspot observations are challenging, the solar disk and its changes during eclipses are easy and fun to observe. We explore the disco ball’s potential for observing the moon and other bright astronomical phenomena.

Authors 8

  1. Robert Cumming corresponding

    Chalmers University of Technology

    Affiliation as printed

    Onsala Space Observatory, Department of Space, Earth and Environment, Chalmers University of Technology, Onsala, SE-439 92, Sweden

  2. Leibniz Institute for Astrophysics Potsdam

    Affiliation as printed

    Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany

  3. Livia Pietrow Aachen

    Leiden University

    Affiliation as printed

    Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands

  4. Stockholm University

    Affiliation as printed

    Department of Astronomy, Stockholm University, 106 91 Stockholm, Sweden

  5. University of Geneva

    Affiliation as printed

    Observatoire de l’Université de Genève, Chemin Pegasi 51, 1290 Versoix, Switzerland

  6. Leiden University

    Affiliation as printed

    Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands

  7. Centre National de la Recherche Scientifique · Université Toulouse III - Paul Sabatier · Institut de Recherche en Astrophysique et Planétologie

    Affiliation as printed

    Institut de Recherche en Astrophysique et Planétologie (IRAP), Université Toulouse III—Paul Sabatier, CNRS, CNES, 9 Av. du colonel Roche, 31028 Toulouse Cedex 04, France

  8. Stockholm University

    Affiliation as printed

    Institute for Solar Physics, Department of Astronomy, Stockholm University, Roslagstullsbacken 21, Stockholm, Sweden

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References 22