按键盘上方向键 ← 或 → 可快速上下翻页，按键盘上的 Enter 键可回到本书目录页，按键盘上方向键 ↑ 可回到本页顶部！
————未阅读完？加入书签已便下次继续阅读！
ach 〃station；〃 we tune to has an exceptionally narrow frequency range。 There are no known processes out among the stars and galaxies that can generate such sharp radio 〃lines。〃 If we pick up anything falling into so narrow a channel； it must； we think； be a token of intelligence and technology。
What's more； the Earth turns—which means that any distant radio source will have a sizable apparent motion； like the rising and setting of the stars。 Just as the steady tone of a car's horn dips as it drives by； so any authentic extraterrestrial radio source will exhibit a steady drift in frequency due to the Earth's rotation。 In contrast； any source of radio interference at the Earth's surface will be rotating at the same speed as the META receiver。 META's listening frequencies are continuously changed to pensate for the Earth's rotation； so that any narrow…band Signals from the sky will always appear in a single channel。 But any radio interference down here on Earth will give itself away by racing through adjacent channels。
The META radio telescope at Harvard； Massachusetts； is 26 meters （84 feet） in diameter。 Each day； as the Earth rotates the telescope beneath the sky； a swath of stars narrower than the full moon is swept out and examined。 Next day； it's an adjacent swath。 Over a year； all of the northern sky and part of the southern is observed。 An identical system； also sponsored by The Planetary Society； is in operation just outside Buenos Aires； Argentina； to examine the southern sky。 So together the two META systems have been exploring the entire sky。
The radio telescope； gravitationally glued to the spinning Earth； looks at any given star for about two minutes。 Then it's on to the next。 8。4 million channels sounds like a lot； but remember； each channel is very narrow。 All of them together constitute only a few parts in 100；000 of the available radio spectrum。 So we have to park our 8。4 million channels somewhere in the radio spectrum for each year of observation； near some frequency that an alien civilization； knowing nothing about us； might nevertheless conclude we're listening to。
Hydrogen is by far the most abundant kind of atom in the Universe。 It's distributed in clouds and as diffuse gas throughout interstellar space。 When it acquires energy； it releases some of it by giving off radio waves at a precise frequency of 1420。405751768 megahertz。 （One hertz means the crest and trough of a wave arriving at your detection instrument each second。 So 1420 megahertz means 1。420 billion waves entering your detector every second。 Since the wavelength of light is just the speed of light divided by the frequency of the wave； 1420 megahertz corresponds to a wavelength of 21 centimeters。） Radio astronomers anywhere in the Galaxy will be studying the Universe at 1420 megahertz and can anticipate that other radio astronomers； no matter how different they may look； will do the same。
It's as if someone told you that there's only one station on your home radio set's frequency band； but that no one knows its frequency。 Oh yes； one other thing： Your set's frequency dial； kith its thin marker you adjust by turning a knob； happens to reach from the Earth to the Moon。 To search systematically through this vast radio spectrum； patiently turning the knob； is going to be very time…consuming。 Your problem is to set the dial correctly from the beginning； to choose the right frequency。 If you can correctly guess what frequencies that extraterrestrials are broadcasting to us on—the 〃magic〃 frequencies—then you can save yourself much time and trouble。 These are the sorts of reasons that we first listened； as Drake did； at frequencies near 1420 megahertz； the hydrogen 〃magic〃 frequency。
Horowitz and I have published detailed results from five years of full…time searching with Project META and two years of follow…up。 We can't report that we found a signal from alien beings。 But we did find something puzzling； something that for me in quiet moments； every now and then； raises goose bumps：
Of course； there's a background level of radio noise from Earth—radio and television stations； aircraft； portable telephones； nearby and more distant spacecraft。 Also； as with all radio receivers； the longer you wait； the more likely it is that there'll be some random fluctuation in the electronics so strong that it generates a spurious signal。 So we ignore anything that isn't much louder than the background。
Any strong narrow…band signal that remains in a single channel we take very seriously。 As it logs in the data； META automatically tells the human operators to pay attention to certain signals。 Over five years we made some 60 trillion observations at various frequencies； while examining the entire accessible sky。 A few dozen signals survive the culling。 These are subjected to further scrutiny； and almost all of them are rejected…for example； because an error has been found by fault…detection microprocessors that examine the signal…detection microprocessors。
What's left—the strongest candidate signals after three surveys of the sky—are 11 〃events。〃 They satisfy all but one of our criteria for a genuine alien signal。 But the one failed criterion is supremely important： Verifiability。 We've never been able to find any of them again。 We look back at that part of the sky three minutes later and there's nothing there。 We look again the following day： nothing。 Examine it a year later； or seven years later； and still there's nothing。
It seems unlikely that every signal we get from alien civilizations would turn itself off a couple of minutes after we begin listening； and never repeat。 （How would they know we're paying attention？） But； just possibly； this is the effect of twinkling。 Stars twinkle because parcels of turbulent air are moving across the line of sight between the star and us。 Sometimes these air parcels act as a lens and cause the light rays from a given star to converge a little； making it momentarily brighter。 Similarly； astronomical radio sources may also twinkle—owing to clouds of electrically charged （or 〃ionized〃） gas in the great near…vacuum between the stars。 We observe this routinely with pulsars。
Imagine a radio signal that's a little below the strength that we could otherwise detect on Earth。 Occasionally the signal will by chance be temporarily focused； amplified； and brought within the detectability range of our radio telescopes。 The interesting thing is that the lifetimes of such brightening； predicted from the physics of the interstellar gas； are a few minutes—and the chance of reacquiring the signal is small。 We should really be pointing steadily at these coordinates in the sky； watching them for months。
Despite the fact that none of these signals repeats； there's an additional fact about them that； every time I think about it； sends a chill down my spine： 8 of the 11 best candidate signals lie in or near the plane of the Milky Way Galaxy。 The five strongest are in the constellations Cassiopeia； Monoceros； Hydra； and two in Sagittarius—in the approximate direction of the center of the Galaxy。 The Milky Way is a flat； wheel…like collection of gas and dust and stars。 Its flatness is why we see it as a band of d