On which of these planets is the atmospheric greenhouse effect strongest? a. Venus b. Earth c. Mars

Short Answer

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Venus

Step by step solution

01

Understand the Greenhouse Effect

The greenhouse effect is a natural process that warms a planet's surface. When the sun's energy reaches a planet's atmosphere, some of it is reflected back to space and the rest is absorbed and reradiated by greenhouse gases.
02

Analyze Planetary Atmospheres

Compare the atmospheres of Venus, Earth, and Mars. Venus has an extremely thick atmosphere composed mainly of carbon dioxide. This leads to a very strong greenhouse effect. Earth's atmosphere also contains greenhouse gases but to a lesser extent. Mars has a thin atmosphere with much lower concentrations of greenhouse gases.
03

Compare Greenhouse Effects

Evaluate the strength of the greenhouse effect on each planet. Venus has the strongest greenhouse effect due to its dense carbon dioxide-rich atmosphere, which traps heat very efficiently. Earth's greenhouse effect is moderate, while Mars has a very weak greenhouse effect because of its thin atmosphere.
04

Conclusion

Based on the analysis of the atmospheric compositions and the greenhouse effects of each planet, it is clear that Venus has the strongest atmospheric greenhouse effect.

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Key Concepts

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

Venus atmosphere
The atmosphere of Venus is primarily composed of carbon dioxide, making up about 96.5% of its atmospheric content. This thick atmosphere creates a very strong greenhouse effect.

Sulfuric acid clouds and a variety of other gases make up the remaining atmosphere, trapping heat extremely efficiently. Surface temperatures on Venus can soar as high as 467°C (872°F). These extreme conditions are largely due to its heavy atmosphere, which is 90 times denser than Earth’s.

It's also interesting that Venus, despite its distance from the Sun, is considerably hotter than Mercury because its thick atmosphere traps so much solar energy. This extreme greenhouse effect creates a runaway scenario, meaning the planet continues to get hotter over time.
greenhouse gases
Greenhouse gases are atmospheric constituents that absorb and emit radiation within the thermal infrared range. They are crucial for maintaining the warmth of a planet’s surface. These gases include carbon dioxide (CO₂), methane (CH₄), water vapor (H₂O), nitrous oxide (N₂O), and several others.

On Venus, carbon dioxide is the primary contributor to its intense greenhouse effect. On Earth, while CO₂ is also significant, water vapor and methane play critical roles in regulating the temperature. The thin atmosphere of Mars contains only small amounts of greenhouse gases, contributing to a much weaker greenhouse effect.

The greenhouse effect works as follows: when sunlight enters the atmosphere, the surface absorbs it and radiates it back as heat. Greenhouse gases trap some of this heat and radiate it back to the surface, maintaining a much warmer environment than would be possible without them.
planetary atmospheres
Different planets have distinct types of atmospheres, heavily influencing their climates and surface conditions.
  • Venus: Atmosphere dominated by CO₂, with very high surface pressures and temperatures.
  • Earth: Balanced composition of nitrogen (78%), oxygen (21%), and other trace gases, including CO₂ and water vapor, which sustain life and a moderate greenhouse effect.
  • Mars: Thin atmosphere primarily composed of CO₂ (95%), but with significantly lower pressure and temperatures compared to Earth and Venus.
Comparatively, atmospheric density vastly affects the greenhouse effect. Venus' thick CO₂ atmosphere traps heat strongly, Earth's balanced atmosphere supports life, and Mars' thin atmosphere leads to a weaker greenhouse effect.

Each planet’s atmosphere also evolves due to geological and possibly biological processes, which can dramatically change planetary climates over time.

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Most popular questions from this chapter

Go to the National Snow \& Ice Data Center (NSIDC) website (http://nsidc.org). What are the current status and the trend of the Arctic sea ice? How does it compare with previous years and with the median shown? (More data might be reported on NOAA's Arctic theme Web page: wwwarctic.noaa.gov.) Is anything new reported about Antarctic ice? Qualitatively, how might a change in the amount of ice at Earth's poles affect the albedo of Earth, and how does the albedo affect Earth's temperature?

Oxygen molecules \(\left(\mathrm{O}_{2}\right)\) are 16 times as massive as hydrogen molecules \(\left(\mathrm{H}_{2}\right)\). Carbon dioxide molecules \(\left(\mathrm{CO}_{2}\right)\) are 22 times as massive as \(\mathrm{H}_2.\) a. Compare the average speed of \(\mathrm{O}_{2}\) and \(\mathrm{CO}_{2}\), molecules in a volume of air. b. Does this ratio depend on air temperature?

The ability of wind to erode the surface of a planet is related in part to the wind's kinetic energy. a. Compare the kinetic energy of a cubic meter of air at sea level on Earth (mass \(1.23 \mathrm{kg}\) ) moving at a speed of \(10 \mathrm{m} / \mathrm{s}\) with a cubic meter of air at the surface of Venus (mass \(64.8 \mathrm{kg}\) ) moving at \(1 \mathrm{m} / \mathrm{s}\). b. Compare the kinetic-energy value you determined for Earth in part (a) with that of a cubic meter of air at the surface of Mars (mass \(0.015 \mathrm{kg}\) ) moving at a speed of \(50 \mathrm{m} / \mathrm{s}\). c. Why do you think there is not more evidence of wind erosion on Earth?

Convection in the ________________causes weather on Earth. a. stratosphere b. mesosphere c. troposphere d. ionosphere

\(\mathbf{T} / \mathbf{F}:\) Life is responsible for the presence of oxygen in Earth's atmosphere.

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