Why did Isaac Newton conclude that the universe was static? Was he correct?

Short Answer

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Isaac Newton concluded that the universe was static, assuming a balance between gravitational forces and stellar momentum. Although this made sense with the science available in his time, we now know this conclusion to be incorrect, following Einstein's theory of relativity and 20th-century observations, confirming that the universe is expanding and not static.

Step by step solution

01

Understanding Newton's Perspective

Isaac Newton concluded that the universe was static because, according to his law of gravity, an infinite and eternal universe would cause matter to come together due to gravitational attraction, leading to a 'gravitational collapse'. Newton suggested that for the universe to be static, there must be a perfect balance between the forces of attraction of the stars and their momentum due to their movement.
02

Evaluating the Correctness of Newton's Conclusion

While Newton's logic was sound on the basis of his own understanding and the science available during his time, it eventually turned out to be incorrect. This occured due to Einstein's introduction of the theory of relativity which showed that space and time were intertwined into a four-dimensional spacetime. Moreover, with observations of an expanding universe made in the 20th century, the model of the universe had to be adjusted, leading to the conclusion that the universe is not static but expanding.

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Key Concepts

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

Gravitational Collapse
The concept of 'gravitational collapse' is a phenomenon that occurs when an astronomical body, such as a star or gas cloud, falls in on itself due to the force of gravity overpowering any other internal pressures that might be resisting the collapse. This is an important process in the universe as it's responsible for the formation of various structures, including stars, black holes, and galaxies.

Isaac Newton, renowned for formulating the law of universal gravitation, theorized that a static universe would eventually succumb to this gravitational collapse, as all matter would be drawn together purely by gravity. He envisioned the universe like a crowded dance floor, where dancers (stars) would eventually huddle up (collapse) without some sort of outward motion or repulsion keeping them apart. Newton proposed that for the universe to remain static, there had to be a precise balance between the pull of gravity and the motion of the stars.

However, this idea of a precise balance is more a thought experiment than a reality. In the vast cosmos, such a delicate balance is not observed. Modern astrophysics tells us that gravitational collapse is common and is the driving force behind the birth of new stars, when regions within giant molecular clouds succumb to gravitational pull, resulting in protostars that eventually heat up and sustain nuclear fusion.
Theory of Relativity
Albert Einstein's theory of relativity revolutionized the way we understand gravity and the fabric of the cosmos. In essence, it transcends the idea of gravity as a force and instead describes it as the curvature of spacetime. This theory comprises two parts: the special theory of relavity, which provided a new framework for all of physics by proposing new concepts of space and time, and the general theory of relativity, which introduced the modern understanding of gravity.

Einstein's general relativity posits that massive objects cause a distortion in the spacetime continuum, much like a heavy ball placed on a trampoline distorts the surface. Smaller objects roll towards the heavier object not because they are pulled by a mysterious force but because the fabric of space itself is curved by the mass. This concept helped to explain why Newton's notion of a static universe was flawed. As it turns out, rather than being unchanging, the universe's spacetime fabric is dynamic and constantly evolving, leading to phenomena such as the expansion of the universe and black holes, which were not predicted by Newtonian physics.

Moreover, general relativity predicts that the universe could not be static: either it is expanding or contracting, but it cannot just hang in balance everlasting, as Newton had thought.
Expanding Universe
The discovery of an 'expanding universe' is one of the most remarkable achievements of 20th-century astronomy. Employing the Doppler Effect, astronomers like Edwin Hubble observed that galaxies appear to be moving away from us, with their light being redshifted—a shift towards the longer wavelengths—which indicates that they are moving farther away.

These observations directly conflict with Newton's image of a static universe. If all galaxies are moving away from each other, then the universe must have been denser and smaller in the past. This revelation is one of the foundational pillars of the Big Bang theory, the leading explanation of the universe's origins and development.

The observation of an expanding universe implies that not only is there no gravitational collapse pulling everything together, but also that the cosmos is getting more spacious over time. With this perspective, the focus shifted from an eternal, unchanging realm to a dynamic, evolving entity that began at a certain point in time and has been expanding and evolving over billions of years. The understanding of an expanding universe lays the groundwork for cosmology, the study of the universe's birth, structure, and eventual fate.

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Most popular questions from this chapter

If a photon from the cosmic microwave background had wavelength \(\lambda_{0}\) when it was emitted at redshift \(z\), its wavelength today is \(\lambda=\lambda_{0} /(1+z)\). (a) Let \(T\) be the symbol for the temperature of the cosmic microwave background today. Explain why the radiation temperature was \(T_{0}=T(1+z)\) at redshift \(z\). (b) What was the radiation temperature at \(z=1\) ? (c) At what redshift was the radiation temperature equal to \(293 \mathrm{~K}\) (a typical room temperature)?

(a) Was there ever an era when the universe was radiationdominated and matter and radiation were at the same temperature? If so, approximately when was this, and were there atoms during that era? If not, explain why not. (b) Was there ever an era when the universe was radiation-dominated and matter and radiation were not at the same temperature? If so, approximately when was this, and were there atoms during that era? If not, explain why not.

How does modern cosmology preclude the possibility of either a center or an edge to the universe?

Use the Starry Night Enthusiast TM program to determine how the solar system moves through the cosmic microwave background. This motion appears to be taking us towards the constellation Leo. First, select Favourites \(>\) Guides \(>\) Atlas to display the entire celestial sphere from the center of a transparent Earth. Open the Find pane and click on the magnifying glass symbol to display the Find categories and click on Constellation. Double-click on Leo to center on this constellation and click again on the Find pane tab to close this pane and display the full screen. Select View \(>\) Constellations \(>\) Astronomical and View \(>\) Constellations \(>\) Labels to display and label the constellations. (a) Draw a sketch showing the Sun, the plane in which the Earth orbits the Sun, and the direction in which the solar system moves through the cosmic microwave background. (b) Use the date controls in the toolbar to step through the months of the year. In which month is the Sun placed most nearly in front of the Earth as the solar system travels through the cosmic background radiation?

. Describe two different ways in which the cosmic microwave background is not isotropic.

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