Cosmic Expansion - Spectroscopy Experiment

In summary, Astronomers have long believed that light travels the same distance at the same speed between a source and observer, but recent studies have shown that light can be affected by gravity and thus, its trajectory may vary. This effect can be observed by comparing the red and violet wavelengths of light using a spectrograph at different distances.
  • #1
Farahday
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Astronomers tend to presume that between any given source and observer, all light travels the same distance at the same speed. But light bends in the presence of gravity. Observe a simple prism and you will note the red wavelength bends less than violet. Forget stars and planets, how many mass-laden particles are there in 15 billion light years of space?

Light at lower wavelengths has a more distant trajectory from source to observer when it is repeatedly exposed to micro gravity and would take longer to traverse the distance. Is it possible that 'wavelength lag' alters the elemental absorption markers toward the red end of the scale?

Any suggestions how to set up an experiment?
 
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  • #2
One way to test this hypothesis would be to use a spectrograph and observe the same star or other source of light at different distances. By comparing the intensity of different wavelengths of light at different distances, it should be possible to detect any discrepancies between the red and violet ends of the spectrum. This could then be used to calculate how much the light has been affected by gravity over the course of its journey.
 

Related to Cosmic Expansion - Spectroscopy Experiment

1. What is cosmic expansion?

Cosmic expansion refers to the phenomena in which the universe is constantly expanding, with galaxies moving away from each other. This is supported by evidence from the redshift of galaxies, which indicates that they are moving away from us.

2. How does spectroscopy help in studying cosmic expansion?

Spectroscopy is a technique used to study the properties of light emitted by celestial objects. By analyzing the spectrum of light from distant galaxies, we can measure their redshift, which provides valuable information about their distance and rate of expansion.

3. What is the significance of the cosmic expansion - spectroscopy experiment?

This experiment helps us understand the behavior of the universe and its expansion. It also provides evidence for the Big Bang theory, which states that the universe began with a rapid expansion from a single point.

4. How is the cosmic expansion rate measured using spectroscopy?

The cosmic expansion rate, also known as the Hubble constant, is measured by determining the redshift of galaxies and their distance from Earth. By plotting a graph of the redshift vs. distance, we can calculate the slope of the line, which gives us the expansion rate.

5. What are the potential implications of the cosmic expansion - spectroscopy experiment?

The results of this experiment can have significant implications for our understanding of the universe and its evolution. It can also help us predict the future fate of the universe and potentially reveal new insights about dark energy and dark matter.

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