/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 18 The atmosphere of Mars is often ... [FREE SOLUTION] | 91Ó°ÊÓ

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The atmosphere of Mars is often pink-orange because a. it is dominated by carbon dioxide. b. the Sun is at a low angle in the sky. c. Mars has no oceans to reflect blue light to the sky. d. winds lift dust into the atmosphere.

Short Answer

Expert verified
d. winds lift dust into the atmosphere.

Step by step solution

01

Identify Relevant Information

Evaluate the given options: Mars' atmosphere composition, Sun's angle, absence of oceans, and winds lifting dust.
02

Analyze Atmospheric Composition

Mars' atmosphere is dominated by carbon dioxide. However, this gas itself doesn’t cause the pink-orange color.
03

Examine The Sun's Angle Effect

The Sun's angle can affect the sky's appearance, but Mars' pink-orange color is observed broadly, not just at sunrise or sunset.
04

Consider Ocean Absence

While it is true Mars lacks oceans, which can impact sky color, this absence does not directly explain the pink-orange tint.
05

Assess Dust Lifting

Strong Martian winds lift dust into the atmosphere. This dust scatters sunlight, giving Mars its characteristic pink-orange hue.
06

Conclusion

The consistent factor explaining Mars' pink-orange sky is the dust lifted into the atmosphere by winds.

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Key Concepts

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

Martian Dust Storms
Martian dust storms are a significant feature of Mars' climate. Unlike Earth, which experiences weather changes primarily due to water vapor, Mars has dry, dusty storms. These storms can be vast, sometimes covering the entire planet. They play a crucial role in shaping the Martian landscape and can last for weeks. The dust particles, composed mainly of iron oxide (rust), give Mars its characteristic reddish hue. When these storms occur, they lift enormous amounts of dust into the atmosphere, causing it to absorb and scatter sunlight differently than it would otherwise. This process is essential for understanding the pink-orange color of the Martian sky.
Atmospheric Composition
The atmosphere of Mars is quite different from that of Earth. It is thin and composed primarily of carbon dioxide (COâ‚‚), making up about 95% of the atmosphere. Other gases present in small amounts include nitrogen and argon. Despite its dominance, carbon dioxide does not cause the pink-orange color of Mars' sky. Instead, it is the iron-rich dust particles lifted by powerful winds that scatter sunlight, resulting in the unique coloration. It's also worth noting that Mars' atmosphere lacks oxygen and water vapor, both of which are abundant on Earth and play critical roles in Earth's weather and sky color. Understanding the composition and behavior of Mars' atmosphere helps scientists predict weather patterns and plan missions effectively.
Light Scattering
Light scattering is a fundamental concept to grasp when exploring why the Martian sky appears pink-orange. On Earth, the sky is blue due to Rayleigh scattering, where shorter blue wavelengths of sunlight are scattered in all directions by gases and particles in the atmosphere. Mars, however, experiences a different type of scattering. The fine dust particles in its atmosphere cause Mie scattering, which affects longer wavelengths, such as red and yellow, more effectively than shorter ones. This type of scattering makes the sunlight appear pink-orange when it permeates the Martian atmosphere. Additionally, the ubiquitous dust in the Martian air helps maintain this color consistently, unlike the variable blue sky of Earth that changes hues with weather and time of day.

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Most popular questions from this chapter

Over the last 800,000 years, Earth's temperature has closely tracked a. solar luminosity. b. oxygen levels in the atmosphere. c. the size of the ozone hole. d. carbon dioxide levels in the atmosphere.

Using the average density of air at sea level (1.225 kilograms per cubic meter, or \(\mathrm{kg} / \mathrm{m}^{3}\) ) and the average mass of Earth's atmosphere above sea level per square meter \(\left(1.033 \times 10^{4} \mathrm{kg} /\right.\) \(\mathrm{m}^{2}\), calculate the total depth of Earth's atmosphere (in kilometers) if its density were the same at all altitudes. (This value is called a scale height, a useful quantity for comparing Earth's atmosphere with the atmospheres of other planets.)

Auroras are the result of a. the interaction of particles from the Sun and Earth's atmosphere b. upper-atmosphere lightning strikes. c. the destruction of stratospheric ozone, which leaves a hole. d. the interaction of Earth's magnetic field with Earth's atmosphere.

In what ways does plant life affect the composition of Earth's atmosphere?

Climate change: a. Go to the timeline on the "Discovery of Global Warming" Web page of the American Institute of Physics (http://aip org/history/climate/timeline.htm). When did scientists first suspect that \(\mathrm{CO}_{2}\) produced by humans might affect Earth's temperature? When were other anthropogenic greenhouse gases identified? When did scientific opinion about global warming start to converge? Click on "Venus \(\&\) Mars"; how did observations of these planets add to an understanding of global climate change? Click on "Aerosols"; how do these contribute to "global dimming"? b. Go to the website for NASA's Goddard Institute for Space Studies (www.giss.nasa.gov), click on "Datasets \(\&\) Images," and select "GISS Surface Air Temperature Analysis." The graphs are updated every year. Note that the temperature is compared to a baseline of the average temperature in \(1951-80 .\) What has happened with the temperature in the last few years? If the annual mean decreased, does that change the trend? What does the 5-year running mean show? How much warmer is it on average now than in \(1880 ?\) c. Go to NOAA's "Trend in Atmospheric Carbon Dioxide" Web page on carbon dioxide levels at the observatory on Mauna Loa (http://esrl.noaa.gov/gmd/ccgg/trends/ mlo.html). What is the current level of \(\mathrm{CO}_{2}\) ? How does this compare with the level from 1 year ago? Scroll down the page and click on "A description of how we make measurements at Mauna Loa." Why is this a good site for measuring \(\mathrm{CO}_{2}\) ? What exactly is measured? Are the numbers cross-checked with other measurements?

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