|
| You are here: Categories » Education and reference » The Universe
|
The 1920s were important years in the development of modern astronomy.
In 1922, the Russian physicist Alexandra Friedman produced
computations showing that the structure of the universe was not static
and that even a tiny impulse might be sufficient to cause the whole structure
to expand or contract according to Einstein's Theory of Relativity.
George Lemaitre was the first to recognize what Friedman's work meant.
Based on these computations, the Belgian astronomer Lemaitre declared
that the universe had a beginning
and that it was expanding as a result
of something that had triggered
it. He also stated that the
rate of radiation could be used as
a measure of the aftermath of that
"something".
The theoretical musings of these two scientists did not attract much
attention and probably would have been ignored except for new observational
evidence that rocked the scientific world in 1929. That year the
American astronomer Edwin Hubble, working at the California Mount
Wilson observatory, made one of the most important discoveries in the
history of astronomy. Observing a number of stars through his huge telescope,
he discovered that their light was shifted towards the red end of
the spectrum and, crucially, that this shift was directly related to the distance
of the stars from Earth. This discovery shook the very basis of the
universe model held until then.
According to the recognized rules of physics, the spectra of light
beams travelling towards the point of observation tend towards violet
while the spectra of light beams moving away from the point of observation
tend towards red. (Just like the fading of a train's whistle as it moves
away from the observer) Hubble's observation showed that according to
this law, the heavenly bodies were moving away from us. Before long,
Hubble made another important discovery; The stars weren't just racing
away from Earth; they were racing away from each other as well. The only
conclusion that could be derived from a universe where everything
moves away from everything else is that the universe constantly "expands".
Hubble had found observational evidence for something that George
Lemaitre had "prophesized" a short while ago and one of the greatest
minds of our age had recognized almost fifteen years earlier. In 1915,
Albert Einstein had concluded that the universe could not be static because
of calculations based on his recently-discovered theory of relativity
(thus anticipating the conclusions of Friedman and Lemaitre). Shocked by
his findings, Einstein added a "cosmological constant" to his equations in
order to "make the answer come out right" because astronomers assured
him that the universe was static and there was no other way to make his
equations match such a model. Years later, Einstein was to admit that his
cosmological constant was the biggest mistake of his career.
Hubble's discovery that the universe was expanding led to the emergence
of another model that needed no fiddling around with to make the
equations work right. If the universe was getting bigger as time advanced,
going back in time meant that it was getting smaller; and if one
went back far enough, everything would shrink and converge at a single
point. The conclusion to be derived from this model was that at some
time, all the matter in the universe was compacted in a single point-mass
that had "zero volume" because of its immense gravitational force. Our
universe came into being as the result of the explosion of this point-mass
that had zero volume. This explosion has come to be called the "the Big
Bang" and its existence has repeatedly been confirmed by observational
evidence.
There was another truth that the Big Bang pointed to. To say that
something has zero volume is tantamount to saying that it is "nothing".
The whole universe was created from this "nothing". And furthermore
this universe had a beginning, contrary to the view of materialism, which
holds that "the universe has existed for eternity".
|
|
Leave a comment or ask a question
|
|
Total comments: 0
Disclaimer
- The e-articles directory is not responsible for any and all copyright infringements by writers and authors. If you suspect the information contained by this page for any copyright infringements, please contact us to investigate the issue
|
|
|
GLOBAL WARMING AND ASTROLOGY - Today we are facing a serious problem of global warming. Global warming is a very serious question against mankind. It should give higher priority to solve. The scientist of world now tries to (more...)
The Temperature of the Earth - Temperature and atmosphere are the first essential factors for life on
Earth. The Blue Planet has both a temperature that is livable and an atmosphere
that is breathable for living things, (more...)
The solar system - We live near the outer edge of a spiral galaxy, a giant Catherine wheel, glowing with the light of 100
billion stars and stretching 100,00 light years through space. Our galaxy is called The (more...)
The Sun - The architecture of the Sun consists of a series of nested shells, one inside the other, similar to the layers
of an onion.
At the very centre and stretching a quarter of the way (more...)
Neptune - Neptune is the outermost planet of the gas giants. It has an equatorial diameter of 49,500 kilometres
(30,760 miles). If Neptune were hollow, it could contain nearly 60 Earths. Neptune orbits th (more...)
Pluto - Pluto was discovered on February 18, 1930, making it the last planet found in our Solar System. Pluto is
usually farther from the Sun than any of the nine planets; however, due to the eccentrici (more...)
Uranus - Uranus is the seventh planet from the Sun and is the third largest in the solar system. It was discovered by
William Herschel in 1781. It has an equatorial diameter of 51,800 kilometres (32,190 (more...)
The Earth - From the perspective we get on Earth, our planet appears to be big and sturdy with an endless ocean of
air. From space, astronauts often get the impression that the Earth is small with a thin, f (more...)
Saturn - Saturn is the sixth planet from the Sun and is the second largest in the solar system with an equatorial
diameter of 119,300 kilometres (74,130 miles). Much of what is known about the planet is (more...)
|
|
|