The Search For ET, What Does The Drake Equation Say?

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Is There Life On Other Planets In The Milky Way? What Does The Drake Equation Say?

Charles Drake is a long time proponent for scientific research into the existence of extraterrestrial life. His inspirational work has certainly helped create the intellectual environment necessary to create the Search For Extraterrestrial Intelligence (SETI).

It was in 1960 when Charles Drake brought forth his famous equation designed to predict how many civilizations might exist in our Milky Way galaxy. It's a long equation, if you haven't seen it, multiplying a long sequence of probabilities in an effort to make a prediction. Included in the long list is

  • The average rate of star formation in our galaxy

  • The fraction of those that have planets

  • The fraction of those planets that can harbor life

  • The fraction of those that do produce life

  • The fraction of those that produce intelligent life

  • The fraction of those that produce technological civilizations that release detectable signals into space

  • The length of time that those civilizations release detectable signals into space


  • That's a lot of probabilities to multiply in order to get a final answer. Certainly in the 1960s the necessary values of many of those probabilities were either poorly known or not known at all. So the predictions of the number of concurrent technical civilizations varied from none to many thousands, depending upon the guesses of factors entered into the equation.

    As astronomical research began to fill in some of these unknowns, a reasonable estimate seemed to be that the number of technical civilizations in the galaxy was about the same as the number of years an averate technical civilization existed. We, as a technical civilization, have been broadcasting radio signals into space for a little over a hundred years. So we might estimate that the number of civilizations in the galaxy is at least a hundred or so.

    Some considerations about the probability of extraterrestrial life create optimism. Carl Sagan noted that primitive life started on our planet very early in earth's formation -- withing a few hundred million years. More recently, earth life forms have been found living in the harshest environments. In fact, a new term has been coined for these hearty life forms -- extremophiles.

    Current theory is that earth-like life seems primarily to need a bit of energy and liquid water in order to get started. The mission has become: follow the water. That's what's driving the renewed interest in Mars exploration efforts. And it appears that in the past, perhaps as recent as a few millions or tens of millions of years ago, Mars had copious amounts of water.

    In addition, Europa, a moon of Jupiter, is likely to be a large ice ball with a vast ocean beneath the ice. Gravitational stresses on Europa from its close proximity to Jupiter could provide much of the energy needed by primitive life forms. Even Ganymede and Callisto are suspected of having subterranean water.

    It's also been confirmed that planet formation around stars is anything but rare. In fact, planet formation seems to be something that commonly happens around stars. So there are planets -- lots of them. And if our solar system is any indication, there's water on a very reasonable percentage of the rocky planets and large moons. So the ingredients for at least primitive live seem to exist throughout the galaxy.

    However, there's a few pessimistic factors that also come into play. One is called the Fermi paradox, named after the great nuclear physicist Enrico Fermi. When discussions of alien life came up, and excitement about the possible numbers entered the conversation, he asked "If they are out there, where are they?" Meaning, why haven't they found us?

    While we may not yet have the capability of detecting technological civilizations, surely some galaxy civilizations are much more advanced than ours, and should be able to detect us. So -- where are they?

    During the cold war there developed a pessimism about the possibility of large numbers of technical civilizations because we, the one technical civilization we know of, seemed about to do ourselves in. It was a growing concern that technical civilizations don't last long because their social and political inertial lags so far behind their technical development. The worry was (and perhaps still is) that they eventually blow themselves up.

    With that concern having waned a bit with the breakdown of the cold war, we now see another self imposed threat. We seem to be headed for a global warming catastrophe. Again there is sign for pessimism.

    So here we are, still without an answer. We know that life seems to be able to exist in places we'd have previously assumed were too hostile, leaving hope that places like Mars, Europa, and perhaps even Titan might harbor primitive life. We know that on earth, even though early conditions were not very conducive to life, it began anyway. We know that planets do indeed seem to be around a large percentage of stars.

    Yet the SETI program has so far found nothing. As Fermi asked: "Where are they?"

    Travel With The Children Of Tau Ceti And Find Out What Extraterrestrial Life Might Be Like 

    We've already sent humans to the moon, and are preparing to send them to Mars. It's only a matter of time before we take the next step -- the next big step -- that of sending humans to the nearest stars to find life on extrasolar planets.

    Research has already discovered over a hundred planets of other stars. If don't want to wait perhaps hundreds of years for science to make the journey to other stars, you can take a journey to a planet orbiting a nearby star now. With my novel, you can travel with The Children Of Tau Ceti to a seemingly benevolent extra-solar planet by the name of Eden, orbiting the star Tau Ceti.

    Tau Ceti is a prime candidate -- a Sun-like star, a bit smaller, a bit younger, but perfect to harbor an earth-like planet. We don't know what's there, but on thing we can count on: Tau Ceti life, if it exists, would be much different than anything we've ever seen.

    But planets that look peaceful and enticing from afar might be quite different up close. That's what Alpha and his young companions find when they become The Children Of Tau Ceti.

    Let former astronomer and computer scientist L. D. Smith take you on a realistic adventure to Tau Ceti. A science fiction mystery I know you'll enjoy. You can purchase either the paperback book or the less expensive PDF file for immediate download.

    Travel along with a group of youngsters incubated to be born 20 years before arriving at the solar system around Tau Ceti. The children are brought up in a biosphere that has decades of development before them in order to give them a survivable environment.

    Totally on their own, with only androids to raise and nurture them, they select names for themselves from the many stars they learn of in their extensive studies. They'll be fully trained and prepared for an incredible adventure when they arrive at an earth-like planet orbiting Tau Ceti.

    Or will they?

    The Children Of Tau Ceti -- An Excerpt 

    Aldebaran Explores the Shore of a Great Sea

    Aldebaran swaggered through the cool sand of the beach, her boots held in her hand. She stood and watched the waves lap at her feet. It's wonderful, she thought. She'd seen such Earth scenes on videos, but there was nothing like this aboard the Destiny. At best all they had were a few small ponds.

    She flinched as a shadow of one of the flying creatures flitted along the sand in front of her. She looked up in time to see the creature dive close to the water, it's long snout scooping a flopping apparition from the waves.

    Several of the creatures were circling nearby. It was apparent that they hunted the shallow coastal waters. Further inland she could see far fewer of them. Apparently the one that had swooped at her was out of it's normal habitat. I must have been a puzzling sight that needed a closer look, she thought.

    She watched as another of the creatures swooped and captured its prey. The action was normal enough, but it still left her with the question: what fed on the land animals, which seemed to grow in abundance but not over-abundance?

    She walked further along the beach watching the feeding ritual, but could never clearly see any of the sea creatures. Then she noticed that some of the large ferns near the beach were broken. They looked out of place among the healthy plants spanning the rest of the beach. She wondered if a whirlwind could have damaged them, or perhaps a large animal. The last thought enticed her to examine them in more detail. Maybe there were some predators on the planet, big enough to fell large plants.

    When she got to the broken ferns and looked down at the tracks in the sand, she stood aghast.

    "This can't be," she said.

    See more details of the novel at The Children Of Tau Ceti.

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    What Is The Drake Equation? 

    The Drake equation (also sometimes called the "Green Bank equation," the "Green Bank Formula," or erroneously labeled the "Sagan equation") is an equation allowing scientists to quantify the uncertainty of the factors that determine the number of such extraterrestrial civilizations. It is used in the fields of exobiology and the search for extraterrestrial intelligence (SETI).

    This equation was devised by Dr. Frank Drake (now Professor Emeritus of Astronomy and Astrophysics at the University of California, Santa Cruz) in 1960, in an attempt to estimate the number of extraterrestrial civilizations in the Milky Way (our galaxy) with which we might come into contact.

    More On The Fermi Paradox 

    Category: File - :Arecibo message.svg|thumb|right|140px|A graphical representation of the Arecibo message - Humanity's first attempt to use radio waves to actively communicate its existence to alien civilizations

    The Fermi paradox is the apparent contradiction between high estimates of the probability of the existence of extraterrestrial civilizations and the lack of evidence for, or contact with, such civilizations.

    The age of the universe and its vast number of stars suggest that if the Earth is typical, extraterrestrial life should be common.Sagan, Carl. Cosmos, Ballantine Books 1985 In an informal discussion in 1950, the physicist Enrico Fermi questioned why, if a multitude of advanced extraterrestrial civilizations exist in the Milky Way galaxy, evidence such as spacecraft or probes are not seen. A more detailed examination of the implications of the topic began with a paper by Michael H. Hart in 1975, and it is sometimes referred to as the Fermi-Hart paradox. Another closely related question is the Great Silence?even if travel is hard, if life is common, why don't we detect their radio transmissions?

    There have been attempts to resolve the Fermi Paradox by locating evidence of extraterrestrial civilizations, along with proposals that such life could exist without human knowledge. Counterarguments suggest that intelligent extraterrestrial life does not exist or occurs so rarely that humans will never make contact with it.

    Starting with Hart, a great deal of effort has gone into developing scientific theories about, and possible models of, extraterrestrial life, and the Fermi paradox has become a theoretical reference point in much of this work. The problem has spawned numerous scholarly works addressing it directly, while various questions that relate to it have been addressed in fields as diverse as astronomy, biology, ecology, and philosophy. The emerging field of astrobiology has brought an interdisciplinary approach to the Fermi paradox and the question of extraterrestrial life.

    What Exactly Is SETI? 

    Search for Extra-Terrestrial Intelligence (SETI) is the collective name for a number of activities people undertake to search for extraterrestrial life. SETI projects use scientific methods to search for electromagnetic transmissions from civilizations on distant planets. The United States government contributed to earlier SETI projects, but recent work has been primarily funded by private sources.

    There are great challenges in searching across the sky for a first transmission that could be characterized as intelligent, since its direction, spectrum and method of communication are all unknown beforehand. SETI projects necessarily make assumptions to narrow the search, and thus no exhaustive search has been conducted so far.

    In Search Of Earth-Like Planets 

    Have you heard of the new planet hunter satellite named Kepler? It's the latest effort to find planets beyond our own solar system.

    Well over 100 extra-solar planets have already been found in that last several years. These were located by watching for wobbling motions of stars the planets are orbiting.

    Planets don't exactly orbit stars, rather planets and stars orbit one another. It's an easier concept to grasp if you imagine a star with a single planet. There is a point about which both the star and the planet revolve. Since the star has the greater mass, the point is much closer to the star than the planet. The planet appears to be traveling in a rather large circle (or ellipse), and the star a much smaller circle (or ellipse). In face, the rotational center point might even be closer the the center of the star than it's own perimeter.

    Scientists can't actually see the small proper motion that an orbiting planet might impose upon a star, but what they can do is precisely monitor the spectrum from the star. As the star moves to and fro in it's orbit around the center of mass point, its spectrum will alternately shift blue then red by a small amount. The Doppler shift is caused whenever the distant star is moving either toward (blue shift) or away (red shift) the earth.

    Only very massive planets can cause a significant enough effect on a star for scientists to detect the motion, so only very large planets have been discovered. These are Jupiter-sized planets, and even larger. While this has proven that planets around stars is likely a common thing, it has done little to demonstrate that life might exists on other planets. Jupiter sized planets are not really what's most interesting. What would be most exciting is to find some earth-sized planets in zones around stars where the temperature would allow liquid water to exist.

    That's the quest of the Kepler satellite. Kepler is to examine some 100,000 stars that are similar to our sun, and see if earth-sized planets exist in orbits around any of them. But Kepler will use a different technique than the old Doppler method.

    To get the increased sensitivity needed to detect earth-sized planets, Kepler will be monitoring the brightness of the stars, looking for very small fluctuations in that brightness. The brightness fluctuations scientists are looking for are the type caused by a planet moving across the face of a star, eclipsing the star's light. When a planet does this, it blocks off enough light from the star for Kepler to detect it.

    When such a miniscule drop in brightness is detected, Kepler can also monitor the spectrum from the star, and compare it to the spectrum when the brightness returns to normal. Differences in the spectrum will indicate some information about any atmosphere that might exist on the eclipsing planet.

    You'll be right if you're thinking that not all planets orbiting the observed stars will ever eclipse the star as seen from our location. In fact, most won't. But -- some probably will, giving Kepler the opportunity to detect some likely candidates for life on planets of other stars.

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    by BetchaLikeIt

    L. D. Smith is an author, graphic artist, astronomer, and computer scientist.

    You can see his latest novels at Novels, his artwork at Betchalikeit,... (more)

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