|
Blame it all on
Henrietta Leavitt. If it hadn't been for her, Edwin Hubble might never
have discovered that the universe is flying apart due to an event that
would later be known as the "Big Bang." Ms. Leavitt, while
studying Cepheid variable stars in the Small Magellanic Cloud in 1912,
discovered that the luminosity or brightness of these variable stars
is directly related to the time required for the star to go from
maximum to minimum brightness or luminosity. It's unfortunate that
this brilliant woman astronomer hasn't received more credit for her
work.
Cepheid Variable
Stars.
Cepheid variable
stars are one of the so called "standard candles" that
astronomers use to determine the distance to other galaxies. The
property that allows determining distance using these variables is the
constant relationship between their actual or absolute brightness and
their period of variability. The problem is that we don't know their
absolute brightness, only their relative brightness. The relative
brightness is how bright a light source appears from whatever distance
we happen to view it. The absolute brightness is how bright stars
appear if all are viewed from the same distance. For instance, our sun
appears much brighter than Sirius (the Dog Star) because it is much
closer to us, but if Sirius were viewed at the same distance as our
sun, Sirius would appear much brighter because its absolute brightness
is greater. So, we have a conundrum we need to solve. We want to use
Cepheid variables to determine distance, but first we need to know the
distance to a few of them so we can calibrate the absolute brightness
versus distance knowing the period of variability. This problem can be
solved using another of the standard candles known as parallax.
If you hold one
finger up at arm's length and view it first with your left eye closed
and the right one open, then with your right eye closed and your left
one open, you will note that the finger appears to move from side to
side. This is due to the fact that your eyes are spaced apart (to give
us stereo vision and depth perception,) and the finger is viewed at
different angles by your two eyes. Astronomers can use this apparent
motion of stars as viewed from widely spaced observatories to
determine the distance to nearby stars. Fortunately, there are several
Cepheid variable stars close enough to measure the distance to them
using parallax. After calibrating our Cepheid variable standard
candles, we can use them to measure the distance to other galaxies
that contain this type of variable stars.
It is worth noting
that the authors of The Urantia Book endorse the use of variable stars
to measure distances in the universe. On page 459B, the authors inform
us, "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."
Using Ms. Leavitt's
relationship between brightness and the period of variability of
Cepheid variables, Hubble was able to determine the distance to M31,
known as the Andromeda galaxy. Hubble found that the distance to M31,
our closest neighbor galaxy, is about 1 million light years. And in
fact this is the figure that The Urantia Book indicates on p 170.
Unfortunately, this figure is in error. Today, it is known that the
distance is actually about 2.2 million light years from Urantia, our
planet, to M31. In 1952, Walter Baade discovered that there are two
types of Cepheid variables with different period-luminosity
relationships.1 Hubble had used the wrong population, and
thus came up with the wrong distance to M31. Because of Walter Baade's
discovery, the size of the astronomers' universe doubled overnight!
The popular press had a field day poking fun at the astronomers for
this sudden inflation of the universe.
Mr. Hubble's
Variable Constant.
As Edwin Hubble
observed galaxies at greater and greater distance, he noted that the
farther a galaxy is from us, the faster it seems to be receding from
us. He could tell this from the so-called "red shift" of the
light reaching us from the distant galaxy. When a star or galaxy moves
away from us, its various colors of visible light are shifted toward
the red end of the spectrum. This red shift is mentioned on p 134 of
The Urantia Book.
The conclusion
Hubble reached from his observations was that the universe is
expanding. Initially, Hubble had trouble accepting this
conclusion. At first, he supported the so-called "tired
light" theory, which supposes that something happens to the light
as it passes through space to lower it's frequency and hence move its
color toward the red end of the spectrum; this could account for the
red shift. But later he decided that the red shift was indeed a sign
of an expanding universe. This idea was another of the major
cosmological shocks to which science had introduced the world in the
past few centuries. An earlier one was the concept that the earth is
not the center of the universe. Everyone had considered the
universe as stable and unchanging; to go from a stolid, steady, and
dependable universe to an expanding one was too much of a change for
some people. Even the brilliant Albert Einstein rejected the expanding
universe notion. It wasn't until he visited Mt. Palomar and saw for
himself the evidence on the photographic plates that he accepted the
idea of an expanding universe.
Hubble used the
information he had gathered to determine a relationship between the
distance to a distant galaxy and its speed of recession from us. This
relationship is known as Ho, the Hubble constant. Mathematically, the
Hubble constant is: Ho = V/d, where V is the velocity of the body away
from us, and d is its distance from us. The Hubble constant has the
interesting dimensions of kilometers per Megaparsec per second. A
megaparsec is about 3.26 million light years, and a light year is the
distance light travels in a year at the speed of 186,000 miles per
second, or about 19 trillion miles. Hubble determined a value for Ho
of between 500 and 550 km/Mps/sec.2 This means that
for every megaparsec a galaxy is further from us, it's speed away from
us increases by about 525 km/sec.
The authors of The
Urantia Book inform us that, "Many influences interpose to make
it appear that the recessional velocity of the external universes
increases at the rate of more than one hundred miles a second for
every million light-years increase in distance." (134) When
converted to the same terms as the Hubble constant, the value given in
The Urantia Book is 525 km/sec/Mpc. Thus, the authors cite Hubble's
value, but reject this speed of recession. They go on to state,
"But this apparent speed of recession is not real; it results
from numerous factors embracing angles of observation and other
time-space distortions."
|