[M42 in H alpha light, Bill Keel] [PNG]

The innermost part of the Orion Nebula M42 taken in a filter emphasizing H-alpha emission. This shows the intricate structure of the nebula as revealed by gas. The four bright stars constitute the Trapezium; most of the ionizing radiation for this part of the nebula comes from the hottest of these stars.

[M42 in continuum light, Bill Keel] [PNG]

The same region of the Orion Nebula, now in a filter that passes essentially pure continuum radiation. Fainter members of the associated star cluster can be seen now free of the strong emission seen at H-alpha; much of the nebular structure seen in this filter is from starlight scattered by dust grains. Both Orion images were taken with a Loral CCD at the Lowell Observatory 1.1m telescope.

Credit: Bill Keel, University of Alabama; taken from his image collection.

  • More images from Bill Keel's collection

    Hartmut Frommert (spider@seds.org)
    Christine Kronberg (smil@lrz.uni-muenchen.de)

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    Last Modification: 7 Jul 1999, 0:25 MET