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Big Bang Theory

Future Work



Although the big bang model has done a good job of explaining what is seen in the Universe, there are still many unanswered questions. There is still disagreement about the exact value of the Hubble constant by approximately a factor of two. The Hubble Space Telescope is making observations similar to those made by Edwin Hubble in order to try to measure this quantity more accurately. Preliminary results have been announced, but it will be some time before a value can be accurately determined. These measurements are very difficult to make, since they are at the limits of the telescope's ability to observe.



Another open question is how galaxies actually formed from what was very close to a uniform, homogeneous medium in the early universe. From the uniformity of the microwave background radiation, it is known that this uniformity was better than one part in a thousand. Just by looking at the sky, however, a great deal of structure in the Universe is seen up to very large-size scales of clusters of galaxies and beyond. There must have been some type of clumping which occurred to start the process (with gravity helping the process along), but what started it? Physicists are seeking the answer in quantum mechanics, the science of very small events. The answer resides there because at the moment of the big bang, the Universe was subatomic in size.

Resources

Books

Hawking, Stephen W. A Brief History of Time. Toronto: Bantam Books, 1988.

Silk, Joseph. A Short History of the Universe. New York: Scientific American Library, 1994.

Weinberg, Steven. The First Three Minutes: A Modern View of the Origin of the Universe. New York: Basic Books, 1977.

Periodicals

Glanz, James, "Photo Gives Weight to Einstein's Thesis of Negative Gravity." New York Times. April 3, 2001.

Overbye, Dennis, "Radio Telescope Proves a Big Bang Prediction." New York Times. September 20, 2002.

Peebles, P. James, David N. Schramm, Edwin L. Turner, and Richard G. Kron. "The Evolution of the Universe." Scientific American (October 1994): 53–57.


Larry Gilman

KEY TERMS

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Cepheid variable star

—A class of young stars that cyclically brighten and dim. From the period of its brightness variation, the absolute brightness of a Cepheid variable can be determined. Cepheid variables in distant galaxies give a measure of the absolute distance to those galaxies.

Hubble constant

—The constant of proportionality in Hubble's Law which relates the recessional velocity and distance of remote objects in the universe whose motion is determined by the general expansion of the universe.

Light-year

—The distance that light travels in one year, equal to 5.87 million miles 9.46 million km.

Parsec

—3.26 light-years.

Additional topics

Science EncyclopediaScience & Philosophy: Ballistic galvanometer to Big–bang theoryBig Bang Theory - Studying The Universe, Measurement Techniques, Historical Background, The Spiral Nebulae, Implications Of Hubble's Law