TOEFL Reading Practice Test #30
TOEFL Reading Practice Test #30 - Conditions on Early Earth and the Beginnings of Life
Approximately 3.8 billion years ago marks a significant estimate for the beginning of life on Earth. However, the question of how life began is not resolved, with numerous conflicting theories offering different approaches. This uncertainty contrasts sharply with the optimism of 1953, when Stanley Miller and Harold Urey conducted a groundbreaking experiment at the University of Chicago. The researchers simulated early Earth’s conditions by creating a laboratory “atmosphere” composed of methane, ammonia, and hydrogen circulating over boiling water. When they introduced electric sparks to mimic lightning, a reddish substance rich in amino acids—the building blocks of proteins—appeared. At the time, this discovery suggested a relatively straightforward path from the synthesis of amino acids to the emergence of life presumably.
Since then, this initial optimism has faded for two main reasons. First, creating life involves much more than synthesizing amino acids or other molecular “bricks” like sugars, DNA components, or cell membrane lipids. The real challenge lies in assembling these parts into functional structures capable of life. Second, the fundamental assumptions of Miller and Urey’s experiment have been called into question. Today, most scientists agree that Earth’s early atmosphere was not predominantly composed of methane and ammonia, as these hydrogen-rich molecules would have likely been destroyed by the ultraviolet sunlight penetrating an atmosphere lacking an ozone layer. Instead, evidence points to an atmosphere dominated by carbon dioxide, released during Earth’s violent formation through asteroid impacts.
If the early atmosphere consisted mainly of nitrogen and carbon dioxide, as researchers now believe, the conditions for forming life’s molecular building blocks were far less favorable. Essential compounds like formaldehyde and hydrogen cyanide, which react with water to form amino acids, would have been challenging to produce. Hydrogen cyanide, in particular, would have been scarce in a carbon-dioxide-rich environment. Interestingly, these compounds are abundant in comets, such as Halley, Hyakutake, and Hale-Bopp, leading scientists to propose that comets might have delivered these organic precursors to Earth.
This hypothesis offers a compelling resolution to the apparent conflict between earlier ideas about life’s origins and current understandings of Earth’s formation. Comets, which likely played a crucial role in forming Earth’s oceans, may have simultaneously deposited large amounts of organic material. Scientists estimate that throughout Earth’s history, comets delivered organic matter nearly a million times the mass of all life currently on the planet. Most of this organic matter likely arrived during the period of heavy bombardment that ended about 3.8 billion years ago, coinciding with the appearance of life on Earth.
TOEFL Reading Practice Test #30 - Conditions on Early Earth and the Beginnings of Life
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