Hubble's law:

Discovery and Explanation of the Red Shift

Edwin Hubble first proposed this law in 1929 based on a study of the light received from the distant galaxies. He observed that the characteristic colors, or spectral lines (see spectrum), emitted by the stars in the galaxies do not have exactly the same wavelengths observed in the laboratory; rather they are systematically shifted to longer wavelengths, toward the red end of the spectrum.

Such red shifts could occur because other galaxies are moving away from our own galaxy, the Milky Way. The change in the wavelength of light that results from the relative motion of the source and the receiver of the light is an example of the Doppler effect. The precise definition of the red shift is the increase in the wavelength divided by the original wavelength; for a given relative velocity, this quantity is the same for all wavelengths or colors. For example, a red shift of 0.05 means that all wavelengths are increased by 5% because of the recessional velocity. Thus the velocity of any given galaxy is measured by its red shift.

Subsequent work has confirmed the general features of Hubble's law, but one specific part—Hubble's constant—has been drastically corrected. This value suggests the relative rate at which the scale of the universe changes with time. The value is currently estimated at about 45 to 46 mi (72 to 74 km) per second per megaparsec, based on studies of type 1a supernovas, which have a known brightness, using Cepheid variable stars to determine the supernovas distances. There is still some uncertainty in the value of this constant—a more recent estimate based on data from the Planck space observatory was about 42 mi (67 km) per second per megaparsec, and a third, more recent method that was based on type 1a supernovas but used red giants to determine distances resulted in an estimate of about 43 mi (70 km) per second per megaparsec—although the difference much less what it was in 1990. Hubble's original value for the expansion rate was between five and ten times too large because he underestimated the distances to the galaxies. The Hubble constant has received much attention because its reciprocal can be thought of as a time that represents the age of the universe. A low Hubble's constant implies that the universe is expanding slowly and therefore must be very old to have reached its current size. Conversely, a high estimate implies a rapid expansion and a relatively young universe. Current estimates place the age of the universe at around 13.799 billion years.

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