Meeting contribution: Bright lights on giant planets

Details Meeting contribution: Bright lights on giant planets Meeting contribution: Bright lights on giant planets

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jbaa..117...98m&link_type=abstract

Journal of the British Astronomical Association, vol.117, no.2, p.98-100

Astronomy and Astrophysics

Astronomy

Scientific paper

Prof Miller explained that his scientific background was in chemistry rather than astronomy, but that he had become involved with planetary science, and especially aurorae, through an interest in the chemical composition of planetary atmospheres. The various colours seen in aurorae were powerful probes of the chemical constituents of atmospheres, and the speaker illustrated this with an image of the aurora borealis of our own planet. The deep red emission seen at the highest celestial altitudes could be attributed to atomic oxygen, and likewise the brighter green emission below it. Towards the lower edge of the aurora, closest to the horizon, reddish-pink emission stemmed from molecular nitrogen.

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