Consider the idea that Mercury has a solid iron-bearing mantle that is permanently magnetized like a giant bar magnet. Using the fact that iron demagnetizes at temperatures above \(770^{\circ} \mathrm{C}\), present an argument against this explanation of Mercury's magnetic field.

Short Answer

Expert verified
Mercury's mantle cannot be permanently magnetized like a giant bar magnet, because the internal temperature of Mercury exceeds the Curie temperature of iron (\(770^{\circ}C\)), at which point iron loses its permanent magnetism.

Step by step solution

01

Understand Iron's Magnetic Properties

Iron is a substance that can hold permanent magnetism, and it is known to demagnetize or lose its magnetism when heated above its Curie temperature, which is \(770^{\circ}C\) for iron.
02

Consider the Thermal Condition of Mercury

Mercury, the smallest planet in our solar system, has extreme temperatures. The side facing the sun can reach temperatures up to \(427^{\circ}C\), and the dark side can drop down to \(-173^{\circ}C\). However, the internal temperature of a terrestrial planet like Mercury is considerably higher due to the heat produced by decaying radioactive isotopes and residual heat from planetary formation. The core temperature of Mercury is estimated to be around \(2000^{\circ}C\) to \(3500^{\circ}C\).
03

Connect the Facts

Given that iron loses its permanent magnetization when heated above its Curie temperature of \(770^{\circ}C\), and the core temperature of Mercury is well above this temperature. Therefore, it can be inferred that the solid iron in Mercury's mantle cannot hold permanent magnetism as a giant bar magnet due to its core temperature being well above the Curie temperature of iron.

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Key Concepts

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

Iron's Magnetic Properties
Iron is one of the most common materials known for having magnetic properties. It’s an element that can be magnetized, creating a magnetic field around it. In everyday objects, iron's magnetic properties are harnessed in the form of small magnets, such as those found on refrigerator doors, or at a much more industrial scale, like in the motors of electric machines. What's intriguing about iron is how its magnetic properties are affected by temperature. When iron is in its ferromagnetic state, the atoms align in a common direction, which gives iron its magnetic capabilities. However, when heated to high temperatures, the alignment is disturbed, leading to a loss of magnetization. This property is pivotal when exploring magnetic fields in planetary bodies, like Mercury's magnetosphere.
Curie Temperature
The Curie temperature, named after the French physicist Pierre Curie, is a critical point for magnetic materials such as iron. It is the temperature at which certain materials lose their permanent magnetic properties to become only paramagnetic. This is a state where the material magnetizes only in the presence of an external magnetic field and does not retain magnetization after the external field is removed. In the case of iron, its Curie temperature is approximately --- --- --- at --- --- --- --- --- --- --- --- --- --- --- --- --- --- --- --- --- --- --- --- --- --- --- [...] the Curie temperature is closely related to the microscopic order of atoms and their magnetic moments within the material. Beyond this temperature, the thermal agitation overcomes the magnetic forces aligning the moments, causing a random distribution and thus demagnetization. Understanding the Curie temperature is crucial when analyzing the likelihood of naturally occurring magnetic fields in the environment or in the technological application of magnetic materials.
Planetary Core Temperature
The temperature of a planet's core is a fundamental aspect of its geological and magnetic properties. For terrestrial planets like Earth and Mercury, the core is primarily made up of metals such as iron and nickel. These metals, in their molten state, can create a dynamo effect, generating a planet's magnetic field. However, the temperature of the core also plays a significant role in whether the metals therein can sustain a magnetic field. If a planet's core temperature is above the Curie temperature of the materials it’s made of – in this instance, iron – it means that the ferromagnetic or permanent magnetism is not sustainable in the core. Instead, what may contribute to the planetary magnetic field has to be dynamic in nature, such as the movement of molten metal, rather than the permanent magnetization of the solid iron-bearing layer. Hence, knowing the core temperature helps scientists infer not only the state of the planetary interior but also gives insights into the mechanics behind magnetic field generation in planets.

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Most popular questions from this chapter

Why is it impossible for liquid water to exist on Mars today? If liquid water existed on Mars in the past, what must have been different then?

Figures 11-6b and \(11-6 c\) show a planet in synchronous rotation and Mercury with a 3 -to- 2 spin-orbit coupling, respectively. Stand up and demonstrate how planets move in each of these rotations by "orbiting" around a stationary classmate who represents our Sun. How would Mercury's motion be different if it had a 4-to-2 spin-orbit coupling instead?

Use the Starry Night Enthusiast \({ }^{\mathrm{TM}}\) program to examine Mercury. Select Favourites \(>\) Solar System \(>\) Mercury from the menu. Select View > Feet from the menu to remove the image of the astronaut's spacesuit from the view. Select Options \(>\) Solar System > Planets-Moons. .. from the menu to allow you to examine the complete surface of the planet. In the PlanetsMoons Options dialog box, slide the control next to the label Show dark side all the way to the right (Brighter) end of the scale. Click OK to close the dialog box. Use the Zoom controls in the toolbar to zoom in and out on the view. Rotate the image of Mercury by placing the mouse cursor over the image of the planet, holding down the mouse button, and moving the mouse. (On a two- button mouse, hold down the left mouse button.) As you explore the surface of the planet Mercury, estimate the diameter of the largest craters by measuring their size on the screen with a ruler and comparing to the diameter of Mercury (see Table 11-1). (Note that the rosette patterns surrounding both planetary poles are an artifact of the technique used to produce these images).

Why is it reasonable to assume that the primordial atmospheres of the Earth, Venus, and Mars were roughly the same?

Suppose that Venus had no atmosphere at all. How would the albedo of Venus then compare with that of Mercury or the Moon? Explain your answer.

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