Does General Relativity Explain Mercury's Perihelion Precession and the CMBR?

In summary, perihelion orbital precession is an observed phenomenon that is explained using General Relativity. It is the result of the influence of a body (in this case, Mercury) on another body (Jupiter).
  • #1
neelakash
511
1
Can anyone help me to know that if General relativity explains the perihelion of mercury or the CMBR...

If so,how?
 
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  • #2
Suggest a good textbook

Hi, neelakash,

neelakash said:
Can anyone help me to know that if General relativity explains the perihelion of mercury or the CMBR

GR explains the "extra-Newtonian term" in the precession of the perihelia of Mercury (and Venus, various asteroids, and various binary pulsars); in the case of Mercury, most of the observed precession is due to the perturbing influence of Jupiter, but after subtracting away everything they could explain, nineteenth century astronmers were left with an unexplained remainder which agreed perfectly with Einstein's rough computation using GR in 1915.

The CMBR is not primarily a gravitational phenomenon, so much of the explanation involves physics other than GR, but certainly GR is involved in the explanation of some of the characteristics of this radiation.

Try D'Inverno, Understanding Einstein's Relativity, Oxford University Press, 1992, for a good discussion (at the advanced undergraduate level) of these phenomena.
 
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  • #3
[Can anyone help me to know that if General relativity explains the perihelion of mercury or the CMBR...

If so,how?]

Newton's theory of gravitation significantly erred when it was applied to calculate the precession of Mercury's orbit. No one knew why. Then Einstein invented General Relativity to explain relativity of accelerated observers in a similar fashion as his Special Relativity had done with inertial observers. To adequately treat acceleration Einstein had to invent stronger equations with more terms that when simplified reduced to Newton's equation for gravitation. Lo and behold the extra terms invented to explain earthly phenomena also explained heavenly phenomena like Merc's weird precession.

It was the same thing with the CMBR. These guys P & W stuck out a horn looking for stray cat calls and bumped into heavenly hissing. The hissing had a microwave frequency. The CMBR. What did it mean? It came from every direction in the sky so it couldn't be explained by a single source. If you do a calculation something like radiocarbon dating, you get that the temperature of the CMBR implies this radiation has been around as long as the universe, a universe that many believe has evolved from a titanic explosion, a "big bang". Put together these two clues and you have something that apparently comes from everywhere in the universe and is as old as the universe, so it must have come from the beginning of the universe. Voila, it came from the Big Bang.

So who cooked up the Big Bang? Friedmann, Lemaitre, Hubble, et al, but it was Einstein's GR that explained it, and Einstein missed it when his equations called for it. He couldn't believe it. Something wrong with the simple formulation. Have to add a compensating factor to keep the universe Newtonian! So Einstein invented the Cosmological Constant to keep the universe from flying apart. Along comes Hubble who discovers it IS flying apart. Man, was Einstein pissed. Biggest blunder he ever made. However, solutions to Einstein's equation with or without the cosmological constant indicate the Big Bang and thereby, the source of the CMBR. There are other explanations for the CMBR, other than the Big Bang model, but they're not as good.

I hope you get the point here. These guys accidentally discovered these things about the universe. They were trying to solve certain problems and then they made a connection to solve seemingly unrelated problems. One can't calculate these "connections". They just come when you spend a lot of time sweating over boring equations that seem to be going nowhere. So that answers your question "how".

Here's a question for you: What does it mean when someone says a planet's orbit precesses? More formally stated, what is perihelion or aphelion orbital precession?
 

1. What is general relativity?

General relativity is a theory of gravity that was developed by Albert Einstein in the early 20th century. It describes how objects with mass affect the fabric of space and time, and how this curvature of spacetime causes objects to move in a certain way.

2. How does general relativity differ from Newton's theory of gravity?

While Newton's theory of gravity describes gravity as a force between objects with mass, general relativity explains gravity as the curvature of spacetime caused by these objects. General relativity also predicts more accurate results in extreme situations, such as near black holes or during the expansion of the universe.

3. What evidence supports the concept of general relativity?

There is a significant amount of evidence that supports general relativity, including the bending of light near massive objects, the precession of Mercury's orbit, and the gravitational redshift of light. Additionally, the predictions made by general relativity have been consistently confirmed by experiments and observations.

4. How does general relativity explain the concept of time dilation?

According to general relativity, time is not absolute but is instead relative to the observer's frame of reference. Time dilation occurs when an object is moving at a high speed or in a strong gravitational field, causing time to pass slower for that object compared to a stationary observer. This has been confirmed through experiments, such as the famous Hafele-Keating experiment.

5. Can general relativity be unified with quantum mechanics?

Currently, there is no complete theory that unifies general relativity and quantum mechanics. However, many physicists are working towards a theory of quantum gravity that would combine these two theories and provide a more complete understanding of the universe. Some promising approaches include string theory and loop quantum gravity.

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