Top Document: [sci.astro] ET Life (Astronomy Frequently Asked Questions) (6/9) Previous Document: F.08 What is happening with SETI now? Next Document: F.10 Why do we assume that other beings must be based on carbon? Why couldn't organisms be based on other substances? See reader questions & answers on this topic! - Help others by sharing your knowledge Author: Joseph Lazio <jlazio@patriot.net> There are two possibilities for sending information to other technological civilizations over interstellar distances: send matter or send radiation. The focus in SETI has been on detecting electromagnetic radiation, particularly radio, because compared to all other known possibilities, it is cheap, easy to produce, and can travel across the Milky Way Galaxy. Compared to radiation, most matter has a distinct disadvantage: it is slow. Radiation can travel at the speed of light whereas (most) matter is constrained to travel slower. Distances between stars are so large, it makes no sense to use a slow mode of communication when a faster one is available. The speed at which spacecraft travel is the primary justification why there is little effort spent within the SETI community searching for interstellar spacecraft (that and the fact that there is no evidence that there are any such interstellar spacecraft from other civilizations in our vicinity). A secondary justification is that spacecraft are relatively expensive. The launch of a single Earth-orbiting spacecraft can cost US $100 million. It is difficult to imagine building and launching a fleet of interstellar spacecraft for US $500 million, yet this is the estimated cost of a next-generation radio telescope capable of detecting TV signals over interstellar distances. It is possible that future technology will make spacecraft cheaper. It is difficult to imagine a technology that would make spacecraft cheaper without also lowering the cost of a new telescope. Although chunks of matter, i.e., spacecraft, seem a rather inefficient way to communicate across interstellar space, what about a beam of matter. Most often suggested in this context is a beam of neutrinos. Neutrinos are nearly massless so they travel at almost the speed of light. They also interact only weakly with matter, so a beam of neutrinos could cross the Milky Way Galaxy without any significant absorption by interstellar gas and dust clouds. This advantage is also a disadvantage: The weakness of their interaction makes it difficult to detect a beam of neutrinos, far more difficult than detecting a beam of electromagnetic radiation. (A beam of electrons or protons could be accelerated to nearly the speed of light and would be far easier to detect. However, electrons and protons are charged particles. When travelling through interstellar space, the direction of their travel is influenced by the magnetic field of the Milky Way Galaxy. The Milky Way's magnetic field has "small-scale" irregularities in it that would divert and scatter such a beam. The result is that one could not "aim" such a beam in any particular direction [except possibly to the very closest stars] because its actual path would be influenced by the [unknown] direction[s] of the magnetic field it would encounter.) The known forms of radiation are electromagnetic and gravitational. Electromagnetic radiation results from the acceleration of charged particles and is used commonly: Radio and TV broadcasts are radio radiation, microwave ovens produce microwave radiation, X-ray machines produce X-ray radiation, overhead lights produce visible radiation, etc. Gravitational radiation results from the acceleration of massive objects. Gravitational radiation has never been detected directly, and its indirect detection resulted in the 1993 Nobel Prize. Gravity is a much weaker force than electromagnetism. Thus, detectable amounts of gravitational radiation result only from events like the explosion of a massive star or the gravitational interaction between two closely orbiting neutron stars or black holes. Again, it is possible that a future technology might result in gravitational radiation becoming easier to detect. It is still difficult to imagine that it would not also result in electromagnetic radiation. Of the various forms of electromagnetic radiation---radio, microwave, infrared, visible, ultraviolet, X-ray, and gamma-ray---only radio and gamma-ray can cross the Milky Way Galaxy. The other forms suffer varying amounts of absorption by interstellar dust and gas clouds (though they could still be used to communicate over shorter distances). Gamma rays are extremely energetic and are produced by events like the explosion of nuclear bombs. Radio radiation is far less energetic. Thus, to send the same amount of information requires far less energy (i.e., it's cheaper) to send it via radio than gamma ray. The above are merely plausibility arguments to suggest why radio is likely to be a preferred method of communication among technological civilizations. Of course, they may reason that they are only interested in communicating with other civilizations technologically advanced enough to transmit and detect neutrino beams or gravitational radiation (or maybe even some undiscovered method). If so, the existing radio SETI programs are doomed to failure. Nonetheless, it does seem sensible to search first using the most simple technology. User Contributions:Top Document: [sci.astro] ET Life (Astronomy Frequently Asked Questions) (6/9) Previous Document: F.08 What is happening with SETI now? Next Document: F.10 Why do we assume that other beings must be based on carbon? Why couldn't organisms be based on other substances? 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Last Update March 27 2014 @ 02:11 PM
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