Biology - Life on Earth

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Biology – Module 3 – Life on Earth 1) Analysis of the oldest sedimentary rocks provides evidence for the origin of life. • Identify the relationship between the conditions on early Earth and the origin of organic molecules. The approximate age of the Earth is 4.5 Billion years. During the Hadean Eon was the formation of the earth as it was transformed from a gaseous cloud into a solid body. The heavier molten iron sank down and became the core, whereas the lighter rock rose to the surface – forming the crust. As a result of the high temperatures at the centre of the Earth and due to volcanic activity, there as an emission of gases, or out-gassing, of volatile molecules, such as water (H2O), methane (CH4), ammonia (NH3), hydrogen (H2), nitrogen (N2), and carbon dioxide (CO2). The environment was also anoxic as there was no free oxygen. This meant that there was no ozone layer, thus the Earth was exposed to huge amounts of solar radiation (i.e UV). Early Earth, with an atmosphere of water vapour, hydrogen, methane and ammonia, provided an environment in which the production of organic carbon-containing molecules would be fairly easy. The energy for driving these reactions could have come from a number of sources, in particular the sun. Ultraviolet light would easily have reached the Earth’s surface because no ozone layer existed. Other possible energy sources could have been lightning, hot springs and volcanoes, radioactivity in the crust, and impact from meteorites. At this stage, organic molecules would have most likely formed in the lower atmosphere or the Earth’s surface. Stages of the Earth’s Development: - Dense clouds of water formed in the atmosphere, which reflects the sun’s heat - Earth cooled sufficiently to allow for the formation of a rocky crust. - Volcanic gas eruptions increased the air pressure, forming clouds which
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