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Choose the best answer to each of the following. Explain your reasoning with one or more complete sentences. The chances for life on Titan's surface are considered slim, mainly because (a) there's little oxygen in the atmosphere; (b) the liquid methane and ethane rain would be lethal; (c) the surface temperature is far below the freezing point of water.

Short Answer

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Option (c): The surface temperature is far below the freezing point of water.

Step by step solution

01

Understand the Context

Read the question carefully to understand the conditions on Titan, Saturn's largest moon, which can affect the possibility of life on its surface.
02

Analyze Option (a)

Consider option (a): 'there's little oxygen in the atmosphere.' While oxygen is important for life on Earth, other life forms may not require it, and some can even be harmed by it. This makes option (a) a less definitive reason for life being unlikely on Titan.
03

Analyze Option (b)

Examine option (b): 'the liquid methane and ethane rain would be lethal.' Although these chemicals can be harmful to Earth-like life forms, certain hypothetical life forms might adapt to these conditions, which means this option is not the strongest reason by itself.
04

Analyze Option (c)

Review option (c): 'the surface temperature is far below the freezing point of water.' Water is a key element for known life, and extreme cold would prevent liquid water from being present, making life as we know it impossible on the surface. This is a more definitive reason for slim chances of life on Titan.
05

Choose the Best Answer

Compare all options and identify which presents the most compelling and scientifically valid reason for slim chances of life on Titan. Option (c) is most convincing since water is essential for life as we know it, and the absence of liquid water due to low temperatures strongly limits the possibility of life.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Titan
Titan is the largest moon of Saturn and presents a fascinating subject for scientists interested in astrobiology. One key feature that makes Titan special is its thick atmosphere, which is primarily composed of nitrogen, much like Earth's atmosphere. However, it also contains a significant proportion of methane.

The dense smog of Titan's atmosphere has led to some comparisons with a young Earth before life took hold. This similarity has inspired research into the potential for past or present habitability. However, conditions are vastly different from Earth. The presence of methane and ethane clouds sets Titan apart as a unique environment in our solar system. Exploration missions by space agencies, such as the Cassini-Huygens mission, have provided crucial data, imaging, and insights about Titan's atmosphere and surface conditions.

Titan's atmosphere is so substantial that it creates a surface pressure 1.5 times that of Earth. But, with a surface temperature around \(-179.2°C\), it is incredibly cold. This frigid world offers a different perspective from what we are used to on Earth, encouraging scientists to think outside the box when considering the potential for life.
Habitability
Habitability refers to the potential of an environment to support life. When scientists talk about the habitability of places like Titan, they consider various factors like temperature, the presence of water, the chemical makeup of the atmosphere, and energy sources available for metabolism.

On Titan, a significant factor in considering habitability is the severe cold. The moon's surface temperature is so low that any water present is frozen solid, which poses significant challenges for life as we understand it. Despite these conditions, habitability studies push the boundaries of what we understand as conducive to life.

Researchers explore how life might adapt to environments that are very different from Earth, including chemical compositions that involve methane and ethane. The study of extreme conditions on Earth, where life thrives against the odds, informs these theories.
  • Presence of liquid water
  • Source of energy
  • Right chemical elements
These remain key markers when assessing habitable conditions, making Titan an intriguing, if challenging, candidate.
Extremophiles
Extremophiles are organisms that thrive in environments considered inhospitable for most known life forms. These hardy life forms have adapted to live in extreme conditions, such as high temperatures, deep-sea vents, and highly acidic environments on Earth.

The concept of extremophiles is crucial when considering the potential for life on Titan. Titan's low temperatures and organic-rich lakes composed of methane and ethane might seem hostile, yet extremophiles prompt scientists to keep an open mind to life's resilience.

Several types of extremophiles provide insights for astrobiologists:
  • Thermophiles thrive in hot environments.
  • Acidophiles live in acidic settings.
  • Halophiles flourish in high salt concentrations.
  • Cryophiles persist in freezing temperatures, much like those on Titan.
By studying extremophiles, scientists gain a clearer picture of how life could potentially survive in the alien environments of other planets and moons, expanding our understanding of what makes an environment habitable.
Saturn's Moon
Titan is one of Saturn's many moons, but it stands out due to its size and unique characteristics. It is the second largest moon in our solar system and is larger than the planet Mercury.

Saturn itself is a gas giant, not directly hospitable to life as we know it. However, its moons, including Titan, offer compelling environments for astrobiological study. Titan's distinct features, such as its thick atmosphere and surface lakes filled with hydrocarbons, make it particularly interesting.

Saturn's Moons, including Titan, are targets for exploration missions aimed at uncovering their secrets. The features of Titan—in addition to the geysers on Enceladus, another of Saturn's moons—suggest complex geological processes and potential interactions with underlying oceans or water reservoirs.

Understanding these moons provides context about our solar system's history and the possibility of life beyond Earth. Studying Saturn's moons, therefore, stands as a vital step toward answering the age-old question of whether we are alone in the universe.

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Most popular questions from this chapter

What is tidal heating? Briefly explain how it can arise and persist as a result of orbital resonances. How does tidal heating affect Io?

On Earth, fish breathe oxygen that is dissolved in the ocean. Do you expect that we will find dissolved oxygen in Europa's ocean? Why or why not? Based on your answer, if we could somehow transport fish to Europa, is it possible that they could survive in the europan ocean? What other types of life from Earth might survive on Europa?

Although Europa is a promising place to look for life, penetrating its thick, icy crust will be difficult. Suggest a possible way of making a spacecraft that could enter the europan ocean. If it is technically feasible, do you think we should do it soon, or wait until we have further evidence of life? Defend your opinion.

Choose the best answer to each of the following. Explain your reasoning with one or more complete sentences. The moons of Saturn may have large amounts of ammonia and methane ice, while those of Jupiter do not because (a) methane and ammonia come only from comets that exist in the Oort cloud; (b) Jupiter's strong magnetic field encourages water ice to form; (c) the greater cold at Saturn's distance from the Sun means that ices of ammonia and methane could condense there but not at Jupiter.

Choose the best answer to each of the following. Explain your reasoning with one or more complete sentences. Why were scientists so surprised to find active geology on Enceladus? (a) because it is so small; (b) because it lacks any possibility of tidal heating; (c) because it is so far from the Sun.

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