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The Parameters of Galaxies |
"Let's see the very thing and nothing else." - Wallace Stevens, "Credences of Summer" It is a more serious question than most people realize, I think, to ask: How can we travel the length and breadth of our galaxy? I don't want to say there are no solutions. Science fiction has conceived warp drive, subspace communications, the tesseract, suspended animation, and starship colonies journeying for generations from one star to another, and surely the human imagination has the potential to act, somehow, on whatever it conceives. But presently our most advanced space technologists are still grappling with the problems of sending human beings to Mars, which at closest approach is only a few light minutes from Earth. Given the size of just the Milky Way galaxy alone, trekking from star to star seems like a far-fetched notion. It seems doubtful, at the moment, that human beings will ever actually, physically visit and explore other planetary systems. You can't get there from here, apparently. |
a mile or 25,000 miles, we generally speak of how long it takes to travel those distances. A person walking relatively briskly can cover a mile in about fifteen minutes. It is well within the range of human beings to walk across North America, some 3,000 miles, over a period of several months. It would take years to walk (and sail) around the 25,000 mile circumference of the Earth, but there is time enough for any healthy human being to do it. Still, when we think of walking, 25,000 miles seems like a long way. Of course these things have been said before. But that fact does not mitigate the strangeness of time and space: light, whose constant speed is about 186,000 miles per second, travels more than seven Earth-circumferences in one second. This alone is essentially unimaginable; it's one of those things we can talk about rationally enough, but which we cannot possibly comprehend. Yet it's possible to say meaningful things with it, such as the time it takes light to travel from the Sun to the Earth (about 8 minutes), or the time it took Voyager 2's radio signals to reach Earth from Neptune (about 4 hours). As far as anyone knows, the speed of light is a physical constant of the universe which has obtained since the moment of creation, whatever that means, and which will obtain until the end of the universe, whatever that means. After Neptune there is Pluto, and after Pluto there is the Oort cloud of comets, and then interstellar space. The nearest star to our solar system is Alpha Centauri, a triple star system in which the nearest of the three (Proxima Centauri) is approximately 4.24 light-years away. The idea of physical "distance" begins to become unraveled in one's mind even at this relatively nearby location. A photon of light that covers more than seven Earth-circumferences in 1 second, covers the distance between Proxima Centauri and Earth in a little over 4 years. It's possible to make a scale model in your mind, to make this distance more or less recognizable. If the distance from the Earth to the Sun was six inches (six inches equals 93 million miles), then the distance to Proxima Centauri would be about 26 miles. Altair, the bright star in the constellation Auriga, is about 16.5 light-years distant; on the six-inch scale it would be about 100 miles away. These stars are said to be "nearby." Of the brightest stars in the sky, many are not nearby in comparison to Proxima Centauri and Altair. Betelgeuse, the topmost star in the familiar figure of Orion, is some 520 light-years away; on the six-inch scale, Betelgeuse would be over 3,000 miles distant. Rigel, at Orion's foot, is some 900 light-years from Earth, more than 5,000 miles away on the six-inch scale. And six inches, just to be clear, is equivalent to about 93,000,000 miles. The whole Milky Way galaxy, containing the Sun and its neighbors, and perhaps as many as 300 billion other stars of various sizes and temperatures, is thought to be about 100,000 light-years in diameter. The six-inch scale will not help, at this point, because even on this scale the galaxy itself is well over half a million miles |
Wind from LL Orionis collides with the Orion nebula. NASA photo |
The problem, of course, is that the distances between objects in the galaxy prohibit the journeys. Even the nearest stars, like Alpha Centauri, Barnard's star, or Sirius, are so far away their distances are incomprehensible, simple as they seem. The main parameters restricting travel among the stars are first, the physical distances themselves, which in a Newtonian sense are pretty much constant, at least as we now perceive interstellar space, and second our understanding of those immense distances, which is to say, the properties of galaxies themselves. The problem of deep-space travel, that is, is a problem of understanding and overcoming immense distances. The sense of this immensity does not lend itself to a single context or remark or group of remarks. To gain even a hazy understanding of the distances between visible objects in a galaxy, and even beyond galaxies, let me come down, again, to some basic facts, by way of numbers, and then discover what the numbers imply. For example, to understand small distances like |
by Dana Wilde |