Titan Chemistry Science Daily Website Research Proposal

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The temperatures on Saturn, which average in the range of -99 F. To -290 F, or -73 C. To -179 C, mean that ethynyl's highly reactive status is necessary to perform the chemical process that results in the creation of triacetylene and the polyynes that serve as ultraviolet radiation shields and appear as haze from a distance (About that, 2009, Scientific Blogging). Saturn is otherwise too cold to have the heat to propel chemical reactions, in the absence of reactive molecules like ethynyl.

The modeling techniques used by the scientists to reproduce this process involved crossed molecular beam machines to "collide supersonic gaseous beams of ethynyl and diacetylene molecules," and a mass spectrometer measurement of the reaction (About that, 2009, Scientific Blogging).

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Analysis confirmed that the results of the collision yielded triacetylene, plus a single hydrogen atom. Later computations also confirmed the spectrometer's analysis of the distribution of electrons in atoms and thus the overall energy level of the molecules in the products.

These developments are exciting for scientists because they provide clues as to the possible chemical reactions that could have given birth to our own planet, the Earth. Titan's current atmosphere is thought to resemble Earth's early atmosphere, "the researchers' study suggests triacetylene may have been formed in Earth's early atmosphere and offers clues to the evolution of Earth's atmosphere before the development of life some 3.5 billion years ago (Unraveling, 2009, Science Centric).

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"Titan Chemistry Science Daily Website" (2009, October 07) Retrieved May 22, 2025, from
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"Titan Chemistry Science Daily Website" 07 October 2009. Web.22 May. 2025. <
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"Titan Chemistry Science Daily Website", 07 October 2009, Accessed.22 May. 2025,
https://www.aceyourpaper.com/essays/titan-chemistry-science-daily-website-18843
   

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