Thursday, July 30, 2009
Koh-i-noor, a Mountain of Light
Wednesday, July 29, 2009
Tesla's Tower of Power
Tesla's Tower of Power
Thursday, July 23, 2009
Are we not the only Earth out there?
In the relatively new science of planet hunting, no find is more prized than finding a planet like ours, one that could support life. As of late August 2007, almost 250 exoplanets -- planets orbiting besides our sun -- had been found [source: BBC News]. The announcement of new planets has become almost routine; some don't even make it into the news. But we do periodically hear about exoplanets that seem similar to Earth or that scientists speculate may hold liquid water, one of the key ingredients for carbon-based life. How many of these Earth-like planets are out there, and are they really like Earth, or do we just hope they are? In this article, we'll take a look at some potential Earths and what they may tell us about the future of planet hunting.
Space Tourism and Space Exploration Image Gallery
Image courtesy NASA This artist's depiction shows a possible Earth-like planet |
In August 2007, scientists announced the discovery of a star which might have once had an Earth-like planet orbiting it. The star was a white dwarf called GD 362, and it's 150 light years from Earth, still within our galaxy. While no Earth-like planets appear to orbit the star now, the presence of asteroid debris can tell us something about a planet that likely once orbited the star.
The debris, which came from an asteroid that was once 125 miles long, showed little carbon and high levels of calcium and iron. That means the rocky material is much like the moon and the rock that makes up the Earth. The presence of this familiar material, scientists say, implies that an Earth-like planet may have orbited the star millions of years ago, before it became a white dwarf. The star also has rings similar to Saturn's, and some of the ring material may be from planets and other objects that were torn apart by the white dwarf's gravity.
GD 362's diameter is about half of the Earth's, but its mass is about that of the sun, making GD 362 far more dense than our planet. However, GD 362 started out as a star like the sun in our solar system. But when the star used up its fuel, it swelled up into a red giant and then ejected its outer shell. The center of that star then transformed into a white dwarf, at once very hot (more than 100,000 Kelvin) and very small. A white dwarf retains about half of its mass but becomes incredibly dense because of its small size. Our sun should become a white dwarf in about five billion years. The process will destroy Mercury, Venus and possibly Earth.
So how many other Earth-like planets are out there (or were out there)? No one knows, but many scientists believe that it's inevitable that other Earths will be found. One NASA scientist told BBC News that some scientists believe that nearly every star has Earth-like planets orbiting it [source: BBC News]. Of course, excitement around finding these other Earths is based on the idea that they may contain alien life or even, centuries from now, allow for far-flung human space colonies -- before our star explodes and destroys the Earth.
Other Possible Earths
Image courtesy NASA In surveying potential candidates for "new Earths," astronomers |
Few planets have been found in the Goldilocks Zone, but in April 2007, European astronomers announced the discovery of one. It was also, at that point, the most Earth-like planet ever found. The planet, called Gilese 581c, is 12,000 miles in diameter, or not much larger than Earth (8,000-mile diameter). It orbits a massive red star called Gilese 581, located in the Libra constellation, 20.5 light years from Earth. Gilese 581c orbits its star very closely, completing an orbit in just 13 Earth-days. This short orbit would make a planet too hot for life, except that Gilese 581's surface temperature is 1/50th that of our sun.
Because it lies in the Goldilocks Zone, Gilese 581c's surface temperature ranges from an estimated 32 degrees Fahrenheit to 102 degrees Fahrenheit. The research team that discovered it believes it has a developed atmosphere. The planet might not only have water -- it might be entirely covered by oceans.
Gilese 581c does have some things working against it. Its gravity is about twice as strong as Earth's, and it receives significant doses of radiation from its star. Both could inhibit life from developing. Even so, Gilese 581c is exciting not only for its Earth-like conditions, but also because of its relative proximity to Earth and its location in the elusive Goldilocks Zone.
As more powerful and precise telescopes go into space, future efforts will involve examining exoplanets' atmospheres for traces of oxygen and methane and looking for rocky planets that lie in the Goldilocks Zone. Scientists are also increasing their use of automated telescopes that are programmed to look for minuscule variations in a star's brightness caused by an orbiting planet passing in front of it. With a rapidly increasing pace of discovery of exoplanets and a practically infinite number of stars in the universe, many other exciting discoveries are ahead of us.
The ideal discovery would be a planet similar in composition to Earth that lies within the Goldilocks Zone and orbits a stable star. But it's important to keep in mind that popular depictions of extraterrestrial life are likely wrong. Some life forms may be no more advanced than bacteria. Others may be highly advanced but unrecognizable, a thought that has caused some scientists to advocate the search for so-called weird life.
Tuesday, July 14, 2009
Does space have a shape?
Centuries ago, human beings looked up at the night sky and imagined that a black globe enveloped the Earth. They believed the stars were simply pinpoints of light. The sun, moon and other planets circled the Earth in a regular, perfect pattern. In their minds, the universe was small, centered on Earth and organized into perfect spheres.
Scien tists like Copernicus and Galileo discovered flaws in this philosophy. It took more than a century after Galileo's discoveries for the world to accept that the Earth wasn't the center of the universe. As time passed, we began to learn more about the universe. Today, we study the cosmos through advanced telescopes, satellites and probes.
Now we have images of galaxies<>
But what about the big picture? What do we know about the universe as a whole? Is it expanding? Is it infinite? If it isn't infinite, what lies beyond the boundary of space? And what exactly does space look like?
These questions fall under the category of cosmology, the study of the universe. People have tried many different approaches to study the universe. Some concentrated on mathematics. Others preferred using physics. And quite a few took a philosophical approach.
There's no consensus among cosmologists about what space looks like, but there are plenty of theories. Part of the challenge of describing space is that it's very difficult to visualize. We're used to thinking about locations in two dimensions. For example, you can determine your location on a map using longitude and latitude. But space has four dimensions. Not only do you have to add depth to the dimensions of length and width, you also must addtime. In fact, many cosmologists refer to this collection of dimensions as space-time.
Space is Big
The Big Bang, Gravity and
General Relativity
Three theories that are instrumental in understanding the shape of the universe are the big bang, thetheory of gravity and Einstein’s theory of general relativity. Cosmologists consider all of these theories when forming hypotheses about the shape of space. But what exactly do these theories try to explain?
The big bang theory is an attempt to describe the beginning of the universe. Through observation and analysis, astronomers determined that the universe is expanding. They have also detected and studied light that originated billions of years ago back when the universe was very young. They theorized that at one time, all the matter and energy in the universe was contained in an incredibly tiny point. Then, the universe expanded suddenly. Matter and energy exploded outward at millions of light years every fraction of a second. These became the building blocks for the universe as we know it.
F = GMm/r2.
F is the force of gravitational attraction. The M and m represent the masses of the two objects in question. The r2 is the distance between the two objects squared. So what’s the G? It’s the gravitational constant. It represents the constant proportionality between any two objects, no matter what their masses. The gravitational constant is 6.672 x 10-11 N m2 kg-2 That’s a very small number, and it explains why objects don’t just stick to each other all the time. It takes objects of great mass to have anything more than a negligible gravitational effect on other objects.
If the big bang theory is true, then when the universe began there must have been a huge burst of energy to push matter so far so fast. It had to overcome the gravitational attraction among all the matter in the universe. What cosmologists are trying to determine now is how much matter is actually in the universe. With enough matter, the gravitational attraction will gradually slow and then reverse the universe’s expansion. Eventually, the universe could shrink into another singularity. This is called the big crunch. But if there’s not enough matter, the gravitational attraction won’t be strong enough to stop the universe’s expansion, and it will grow indefinitely.
What about the theory of relativity? Besides explaining the relationship between energy and matter, it also leads to the conclusion that space is curved. Objects in space move in elliptical orbits not because of gravity, but because space itself is curved and therefore a straight line is actually a loop. In geometry, a straight line on a curved surface is a geodesic.
The three theories described above form the basis of the various theories about what the shape of space actually is. But there’s no actual consensus on which shape is the right one.
The Shapes of Space
The three main models of the universe are based on curvature: zero curvature, positive curvatureand negative curvature.
A zero curvature would mean that the universe is a flat or Euclidean universe (Euclidean geometry deals with non-curved surfaces). Imagine space as a two dimensional structure -- a Euclidian universe would look like a flat plane. Parallel lines are only possible on a flat plane. In a flat universe, there is just enough matter so that the universe expands indefinitely without reversing into a collapse, though the rate of expansion decreases over time.
Negative curvature is a little trickier to visualize. The most common description is a saddle. In a negative curvature model, two lines that would be parallel on a flat plane will extend away from each other. Cosmologists call negative curvature models of the universe open universes. In these universes, there’s not enough matter to reverse or slow expansion, and so the universe continues to expand indefinitely.
Does this mean space is shaped like a flat plane, a sphere or a saddle? Not necessarily. Remember that space-time is measured in four dimensions, which reduces the usefulness of two-dimensional examples. And there are many competing theories about what the ultimate shape of the universe actually is.
Another shape is the PoincarĂ© dodecahedral spherical shape. A dodecahedron is a 12-sided object. The PoincarĂ© variation has surfaces that curve outward slightly. What’s puzzling is that the projected size of this universe is smaller than the area we can actually observe. In other words, our visibility exceeds the boundaries of the universe. No problem, say the cosmologists. When you look at a distant galaxy that would seem to lie beyond the boundaries of space, you’re actually experiencing the wrap around effect described above. The galaxy in question would really be behind you, but you’re looking through one face of the dodecahedron as if it were a window. If you could see far enough, you’d be looking at the back of your own head.
How to Measure Space
Optical telescopes let us examine objects within the visible light spectrum but are relatively weak tools. That’s because the light from distant galaxies can intercept clouds of particles and other bodies before reaching Earth. Other devices can measure wavelengths that fall well outside the visible spectrum. Many of the recent studies in cosmology focus on the cosmic microwave background (CMB). The CMB is radiation that the universe generated when it was only 380,000 years old By studying this radiation, cosmologists can draw conclusions about what the universe was like shortly after it began.
Using the Wilkinson Microwave Anisotropy Probe (WMAP), scientists made an interesting discovery about the CMB. They found that the variation in radiation wavelengths of the CMB stops at a certain point. In an infinite, unbounded universe, there would be no limit to the size of wavelengths. We would expect to see variation and frequencies at all sizes. It’s only in a finite universe or a very specialized infinite one that we’d expect to see a definitive cap on wavelengths.
As for expansion, cosmologists call the ratio of the amount of matter in the universe and the amount needed to stop expansion the density parameter. A density parameter greater than 1 would mean a closed universe -- there is more mass in the universe that would be needed to reverse expansion. A density parameter of 1 would mean a flat universe in which expansion slows but never truly stops. And a density parameter between 0 and 1 would mean an open universe that would continue expanding forever.
But we don’t know how much matter really is in the universe. The amount we can detect is relatively small -- 5 percent of the matter needed to reverse expansion. But there appears to be matter that we can’t see at all. Cosmologists have noticed that stars move in an odd way -- they behave as if there is more matter exerting a gravitational influence on them than we can detect. Some cosmologists theorize that this means there is a kind of matter we can’t see at all, called dark matter.
Dark Matter |
But is there enough dark matter to cause a big crunch? That is, is there enough matter in the universe to make up the balance and push the ratio to a 1 or higher? While cosmologists believe there is far more dark matter in the universe than observable matter, they estimate the combination of both visible and dark matter still only comes to about 30 percent of the amount needed to reverse expansion
While we don’t know what the definitive shape of space is right now, research continues to bring us new information every day. And if space has boundaries, what lies beyond them? We don’t know, and we may not be capable of knowing.