A Universe Full of Surprises
JUST a century ago, scientists believed that the entire universe was contained within our galaxy, the Milky Way. During the 20th century, however, major advances in astronomy, physics, and technology revealed the breathtaking scale of the cosmos. Some of the discoveries have also been humbling. For example, in recent decades astronomers have come to the realization that they do not know what makes up over 90 percent of the universe. What is more, the discoveries that led to that conclusion have caused scientists to question their understanding of the fundamentals of physics itself. Of course, such questions are nothing new.
For instance, toward the end of the 19th century, physicists observed something odd about the speed of light. They found that relative to an observer, light always traveled at the same speed no matter how fast the observer was moving. But that seemed to defy common sense! The problem was addressed in 1905 in Albert Einstein’s special theory of relativity, which showed that distance (length), time, and mass are not absolutes. Then, in 1907, after a flash of intuition that he termed “the happiest thought of my life,” Einstein began to develop his general theory of relativity, which he published in 1916. In this revolutionary work, Einstein wove gravity, space, and time together and refined the physics of Isaac Newton.
The Expanding Universe
Based on the evidence of the day, Einstein believed that the universe is static
Hubble also cleared up a long-standing mystery about certain fuzzy, luminous patches in the night sky, which were named nebulae because they appeared to be clouds of gas. But were all these nebulae within our galaxy, or were they outside it, as British astronomer Sir William Herschel (1738-1822) suggested over a century earlier?
When Hubble first estimated the distance to one of these entities, the Great Nebula in the constellation Andromeda, he concluded that the nebula was actually a galaxy a million light years away. That put it well beyond the Milky Way, which has a diameter of a “mere” 100,000 light years. As Hubble charted the distances to other nebulae, he began to unveil the enormous scale of the cosmos and triggered a revolution in astronomy and cosmology.*
It was soon thereafter that Hubble observed that the universe is expanding, for he saw that distant galaxies were receding from us. He also noticed that the farther away the galaxy, the faster the recession. Those observations imply that the universe of yesterday was smaller than that of today. When Hubble published his groundbreaking work in 1929, he paved the way for the development of the big bang theory of the origin of the universe, which indicates that the universe originated in a cosmic explosion approximately 13 billion years ago. But the picture is still incomplete.
How Fast Is the Expansion?
Since the time of Hubble, astronomers have been trying to measure as accurately as possible the rate of expansion, referred to as the “Hubble constant.” Why is this measurement so important? If astronomers could calculate how fast the universe is expanding, they could use that calculation to estimate its age. Moreover, the rate of expansion might have serious implications for the future. How so? It is reasoned that if, for instance, the universe is expanding too slowly, gravity might ultimately win out and cause everything to collapse in a final “big crunch”! But if the expansion is too rapid, the universe might expand forever and dissipate entirely.
While more precise measurements have provided answers to some questions, other questions have been raised
Dark Energy and Dark Matter
In 1998, researchers analyzing light from a special kind of supernova, or exploding star, found evidence that the expansion of the universe is actually accelerating!* At first, the scientists were skeptical, but evidence soon mounted. Naturally, they wanted to know what form of energy was causing the accelerating expansion. For one thing, it seemed to be working in opposition to gravity; and for another, it was not predicted by present theories. Appropriately, this mysterious form of energy has been named dark energy, and it may make up nearly 75 percent of the universe!
Dark energy, however, is not the only “dark” oddity discovered in recent times. Another was confirmed in the 1980’s when astronomers examined various galaxies. These galaxies, as well as our own, appeared to be spinning too fast to hold together. Evidently, then, some form of matter must be giving them the necessary gravitational cohesion. But what kind of matter? Because scientists have no idea, they have called the stuff dark matter, since it does not absorb, emit, or reflect detectable amounts of radiation.* How much dark matter is out there? Calculations indicate that it could make up 22 percent or more of the mass of the universe.
Consider this: According to current estimates, normal matter accounts for about 4 percent of the mass of the universe. The two big unknowns
A Never-Ending Quest
Science is in search of answers, but all too often one set of answers leads to another layer of puzzles. This fact calls to mind a profound statement recorded in the Bible at Ecclesiastes 3:11. It reads: “Everything [God] has made pretty in its time. Even time indefinite he has put in their heart, that mankind may never find out the work that the true God has made from the start to the finish.”
Of course, at present we can absorb only limited amounts of knowledge because of our short life span, and much of that knowledge is speculative, subject to change. But that situation is temporary, for God has purposed to grant faithful humans endless life in Paradise on earth, where they can examine his handiwork for an eternity and thus gain true knowledge.
Therefore, we need not fear doomsday speculations about the universe. After all, science has only scratched the surface of reality, whereas the Creator knows all.
Astronomy is the study of extraterrestrial objects and matter. Cosmology, a branch of astronomy, “is the study of the structure and development of the universe and the forces that work on it,” says The World Book Encyclopedia. “Cosmologists try to explain how the universe formed, what has happened to it since, and what might happen to it in the future.”
The exploding stars are called type 1a supernovas, and they may shine as brightly as a billion suns for a short time. Astronomers use these supernovas as a standard for measurement.
Dark matter was postulated in the 1930’s and confirmed in the 1980’s. Today astronomers measure how much dark matter a cluster of galaxies may have by observing how the cluster bends light from more distant objects.
The year 2009 has been designated the “International Year of Astronomy,” and it marks the 400th anniversary of the first use of an astronomical telescope by Galileo Galilei.
[Box on page 17]
LOOK UP AND BE HUMBLE
When an ancient servant of God looked up at the clear, unpolluted night sky, he felt reverential awe, which he put to verse. Psalm 8:3, 4, reads: “When I see your heavens, the works of your fingers, the moon and the stars that you have prepared, what is mortal man that you keep him in mind, and the son of earthling man that you take care of him?” Yet, the psalmist had no telescopes or special cameras. How much more, then, should we feel in awe!
[Diagram on page 18]
(For fully formatted text, see publication)
74% dark energy
22% dark matter
4% normal matter
[Picture Credit Line on page 16]
Background: Based on NASA photo
[Picture Credit Line on page 18]
Background: Based on NASA photo