Does global warming make Triton blush?

Bonnie J. Buratti (), Michael D. Hicks and Ray L. Newburn, Jr
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Bonnie J. Buratti: Jet Propulsion Laboratory, California Institute of Technology, Palomar Observatory
Michael D. Hicks: Jet Propulsion Laboratory, California Institute of Technology, Palomar Observatory
Ray L. Newburn, Jr: Jet Propulsion Laboratory, California Institute of Technology, Palomar Observatory

Nature, 1999, vol. 397, issue 6716, 219-219

Abstract: Abstract Neptune's largest moon, Triton, is one of two satellites in the Solar System that are currently geologically active. At least two geyser-like plumes were observed by the Voyager 2 spacecraft in 1989, and dozens of streaky deposits hint at the existence of many more1. Triton also exhibits complex seasonal changes in its 165-year journey about the Sun2. Because Triton's atmosphere transports volatiles (primarily nitrogen and methane) during this seasonal cycle, its atmospheric pressure may fluctuate by up to an order of magnitude over decades3. Photometric measurements of its albedo and colour over half a century show that seasonal volatile transport has occurred4. There have also been indications that more extreme, short-lived changes, perhaps due to geological events, have occurred on Triton. An anomalously red spectrum was reported for Triton in 1977 (56), and global warming has now been observed7.

Date: 1999
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DOI: 10.1038/16615

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