NEW YORK — All the stars, planets and galaxies that can be seen today make up just 4 percent of the universe. The other 96 percent is made of stuff astronomers can't see, detect or even comprehend.
These mysterious substances are called dark energy and dark matter. Astronomers infer their existence based on their gravitational influence on what little bits of the universe can be seen, but dark matter and energy themselves continue to elude all detection.
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"The overwhelming majority of the universe is: who knows?" explains science writer Richard Panek, who spoke about these oddities of our universe on Monday (May 9) at the Graduate Center of the City University of New York (CUNY) here in Manhattan. "It's unknown for now, and possibly forever."
In Panek's new book, "The 4 Percent Universe" (Houghton Mifflin Harcourt, 2011), Panek recounts the story of how dark matter and dark energy were discovered. It's a history filled with mind-boggling scientific surprises and fierce competition between the researchers racing to find answers. [Strangest Things in Space
Some of the first inklings astronomers had that there might be more mass in the universe than just the stuff we can see came in the 1960s and 1970s. Vera Rubin, a young astronomer at the Department of Terrestrial Magnetism at the Carnegie Institution of Washington, observed the speeds of stars at various locations in galaxies.
Simple Newtonian physics predicted that stars on the outskirts of a galaxy would orbit more slowly than stars at the center. Yet Rubin's observations found no drop-off at all in the stars' velocities further out in a galaxy. Instead, she found that all stars in a galaxy seem to circle the center at roughly the same speed.
"It means that galaxies should be flying apart, should be completely unstable," Panek said. "Something's missing here."
But research by other astronomers confirmed the odd finding. Ultimately, based on observations and computer models, scientists concluded that there must be much more matter in galaxies than what's obvious to us. If the stars and gas that we can see inside galaxies are only a small portion of their total mass, then the velocities make sense.
Astronomers nicknamed this unseen mass dark matter.
Where is it?
Yet, in the nearly 40 years that followed, researchers still haven't been able to figure out what dark matter is made of.
A popular hypothesis is that dark matter is formed by exotic particles that don't interact with regular matter, or even light, and so are invisible. Yet their mass exerts a gravitational pull, just like normal matter, which is why they affect the velocities of stars and other phenomena in the universe.
However, try as hard as they might, scientists have yet to detect any of these particles, even with tests designed specifically to target their predicted properties.
"I think on the dark matter side there is some discouragement among the people who are kind of mid-career," Panek said. "They went into this field thinking, 'OK, we're going to solve this problem and then we'll build from there.' But 15, 20 years later, they're saying, 'I've invested my career in this and I don’t know if I'm going to find anything in my lifetime.'"
Still, many hold out hope that we're getting close and that experiments such as the newly built Large Hadron Collider particle accelerator in Geneva may finally solve the puzzle.
Dark energy is possibly even more baffling than dark matter. It's a relatively more recent discovery, and it's one that scientists have even less of a chance of understanding anytime soon.
It all started in the mid-1990s, when two teams of researchers were trying to figure out how fast the universe was expanding, in order to predict whether it would keep spreading out forever, or if it would eventually crumple back in on itself in a "Big Crunch."
To do this, scientists used special tricks to determine the distances of many exploded s
These mysterious substances are called dark energy and dark matter. Astronomers infer their existence based on their gravitational influence on what little bits of the universe can be seen, but dark matter and energy themselves continue to elude all detection.
"The overwhelming majority of the universe is: who knows?" explains science writer Richard Panek, who spoke about these oddities of our universe on Monday (May 9) at the Graduate Center of the City University of New York (CUNY) here in Manhattan. "It's unknown for now, and possibly forever."
In Panek's new book, "The 4 Percent Universe" (Houghton Mifflin Harcourt, 2011), Panek recounts the story of how dark matter and dark energy were discovered. It's a history filled with mind-boggling scientific surprises and fierce competition between the researchers racing to find answers. [Strangest Things in Space
Some of the first inklings astronomers had that there might be more mass in the universe than just the stuff we can see came in the 1960s and 1970s. Vera Rubin, a young astronomer at the Department of Terrestrial Magnetism at the Carnegie Institution of Washington, observed the speeds of stars at various locations in galaxies.
Simple Newtonian physics predicted that stars on the outskirts of a galaxy would orbit more slowly than stars at the center. Yet Rubin's observations found no drop-off at all in the stars' velocities further out in a galaxy. Instead, she found that all stars in a galaxy seem to circle the center at roughly the same speed.
"It means that galaxies should be flying apart, should be completely unstable," Panek said. "Something's missing here."
But research by other astronomers confirmed the odd finding. Ultimately, based on observations and computer models, scientists concluded that there must be much more matter in galaxies than what's obvious to us. If the stars and gas that we can see inside galaxies are only a small portion of their total mass, then the velocities make sense.
Astronomers nicknamed this unseen mass dark matter.
Where is it?
Yet, in the nearly 40 years that followed, researchers still haven't been able to figure out what dark matter is made of.
A popular hypothesis is that dark matter is formed by exotic particles that don't interact with regular matter, or even light, and so are invisible. Yet their mass exerts a gravitational pull, just like normal matter, which is why they affect the velocities of stars and other phenomena in the universe.
However, try as hard as they might, scientists have yet to detect any of these particles, even with tests designed specifically to target their predicted properties.
"I think on the dark matter side there is some discouragement among the people who are kind of mid-career," Panek said. "They went into this field thinking, 'OK, we're going to solve this problem and then we'll build from there.' But 15, 20 years later, they're saying, 'I've invested my career in this and I don’t know if I'm going to find anything in my lifetime.'"
Still, many hold out hope that we're getting close and that experiments such as the newly built Large Hadron Collider particle accelerator in Geneva may finally solve the puzzle.
Dark energy is possibly even more baffling than dark matter. It's a relatively more recent discovery, and it's one that scientists have even less of a chance of understanding anytime soon.
It all started in the mid-1990s, when two teams of researchers were trying to figure out how fast the universe was expanding, in order to predict whether it would keep spreading out forever, or if it would eventually crumple back in on itself in a "Big Crunch."
To do this, scientists used special tricks to determine the distances of many exploded s
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