Abstract
The images of comet Halley's nucleus returned during three spacecraft encounters in March 19861,2 are challenging the theory of the release of particles from a comet's nucleus. Instead of a spherically symmetric outflow, each spacecraft observed strong jets flowing from the sunward side of the nucleus. Here we present ground based 2–23 μm photometry and 10.3 μm imaging of Halley taken within hours of the Giotto spacecraft encounter. The photometry shows a colour temperature of 360 K and silicate emission features at 10 and 20 μm, and the image shows jet activity similar to that observed by Giotto, but on a scale of thousands of km. The expected 10 μm surface brightness, based on the particle mass distribution measured by Giotto and assuming solid, spherical grains, is a factor of six lower than the observed value. We suggest that fluffy particles could remove this discrepancy.
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Hayward, T., Gehrz, R. & Grasdalen, G. Ground-based infrared observations of comet Halley. Nature 326, 55–57 (1987). https://doi.org/10.1038/326055a0
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DOI: https://doi.org/10.1038/326055a0
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