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タイトルCollecting Comet Samples by ER-2 Aircraft: Cosmic Dust Collection During the Draconid Meteor Shower in October 2012
本文(外部サイト)http://hdl.handle.net/2060/20150003807
著者(英)Brown, P.; Moes, T.; Burkett, P. J.; Campbell-Brown, M.; Williams, T.; Frank, D.; Kapitzke, M.; Gonzalez, C.; Robinson, G.-A.; Rodriquez, M.; Bastien, Ron; Broce, S.; Steel, D.; Zolensky, M.; Gearheart, D.
著者所属(英)NASA Johnson Space Center
発行日2014-01-01
言語eng
内容記述Many tons of dust grains, including samples of asteroids and comets, fall from space into the Earth's atmosphere each day. NASA periodically collects some of these particles from the Earth's stratosphere using sticky collectors mounted on NASA's high-flying aircraft. Sometimes, especially when the Earth experiences a known meteor shower, a special opportunity is presented to associate cosmic dust particles with a known source. NASA JSC's Cosmic Dust Collection Program has made special attempts to collect dust from particular meteor showers and asteroid families when flights can be planned well in advance. However, it has rarely been possible to make collections on very short notice. In 2012, the Draconid meteor shower presented that opportunity. The Draconid meteor shower, originating from Comet 21P/Giacobini-Zinner, has produced both outbursts and storms several times during the last century, but the 2012 event was not predicted to be much of a show. Because of these predictions, the Cosmic Dust team had not targeted a stratospheric collection effort for the Draconids, despite the fact that they have one of the slowest atmospheric entry velocities (23 km/s) of any comet shower, and thus offer significant possibilities of successful dust capture. However, radar measurements obtained by the Canadian Meteor Orbit Radar during the 2012 Draconids shower indicated a meteor storm did occur October 8 with a peak at 16:38 (+/-5 min) UTC for a total duration of approximately 2 hours.
NASA分類Lunar and Planetary Science and Exploration
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