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Astronomers use
various types of standard candles or cosmic yardsticks to measure
distances to stars and galaxies. One of these yardsticks is the
class of stars known as the Cepheid variable stars. One of the
apparent errors in The Urantia Book comes from using the distance to
the Andromeda galaxy that astronomers held in the 1930's. This
distance was determined using Cepheid variable stars in M31, also
called the Andromeda galaxy.
Henrietta
Leavitt, a Harvard astronomer, determined in 1917 that there is a
direct relationship between the luminosity (brightness) of Cepheid
variable stars and the length of their period. The longer between
periods of peak brightness, the greater the absolute luminosity of
these stars. Using this relationship, astronomers can determine the
distance to other galaxies by noting the period and apparent
luminosity of the Cepheid variable stars in these other galaxies.
In 1924, the well
known astronomer Edwin Hubble presented a paper to the American
Astronomical Society showing that M31, the great spiral galaxy in
Andromeda, is about 750,000 light years from earth. This distance is
now known to be about 2.2 million light years from earth.
Hubble got the wrong distance to M31 because he was using Shapley's
calibration of a period luminosity (P-L) relationship for Cepheid
variable stars--which was in error because Shapley was unaware that
there were actually two types of Cepheid variable stars (now known
as Type 1 and Type 2 populations) having differing P-L
relationships...
The authors of
The Urantia Book tell us that it takes light from M31 a million
years to reach the earth, which would make that galaxy one million
light years distant from us. It is interesting that they extol the
use of the Cepheid variable stars by astronomers to make this
measurement: "In one group of variable stars the period of
light fluctuation is directly dependent on luminosity, and knowledge
of this fact enables astronomers to utilize such suns as universe
lighthouses or accurate measuring points for the further exploration
of distant star clusters. By this technique it is possible to
measure stellar distances most precisely up to more than one million
light-years." (456)
When astronomers
first started using the Cepheid variables as standard candles, two
million light years was about the limit of distances they could
measure using this technique due to atmospheric distortion. Now,
with improved terrestrial telescopes and the now repaired
space-based Hubble telescope, that range has been pushed out to 60
million light years or more. Recently, this improvement in seeing
has enabled astronomers to measure the distance to a galaxy in the
Virgo cluster. The distance measured using Cepheid variable stars in
the M100 galaxy was 56 million light years1. Being able
to measure galaxies at this distance also allows the astronomers to
determine a value for Hubble's constant, which is important in
determining the age of the universe. Unfortunately for the current
cosmology, the value of Hubble's constant they obtained indicated
that the universe may be only 10 billion years old. This is rather
embarrassing, because there are stars in globular clusters
calculated to be as much as 16 billion years old. Will the
cosmologists be able to apply another patch to keep the Big Bang
theory limping along, or are their backs up against the wall?
Stay tuned for the next exciting episode of "Cosmologists Meet
Reality."
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