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Listen to this story via streaming audio, a downloadable file, or get help. January 10, 2002: If "E.T." is out there, whether
in the form of intelligent beings or much simpler organisms,
we may soon be hot on its trail. For the first time in history,
the dream of searching for signs of life in other solar systems
belongs not only on the philosopher's wish list, but on the list
of doable and planned human endeavors. Scientists crossed a new frontier in "exo-planet" research just last year when, using the Hubble Space Telescope, they detected sodium in the atmosphere of a large alien world orbiting the star HD 209458. The Hubble data not only revealed that exo-planets have atmospheres, but also that we can analyze them from a distance. For the first time, humans are discovering and exploring worlds outside the solar system.
So far, all known extra-solar planets
are gas giants -- unlikely abodes for life as we know it. In
fact, some are so large that they might not be planets at all,
but a kind of failed star called a "brown dwarf." Of greater interest are Earth-size planets,
which are too small for even the
Hubble Space Telescope to detect. Nevertheless, astronomers believe
they exist. Beginning in 2006, Kepler will monitor
about 100,000 nearby stars, searching
for the slight dimming that occurs when an orbiting planet blocks
some of the parent star's light. Because Kepler will be
sensitive enough to detect planets as small as Earth, this celestial
survey will give scientists an idea of how common Earth-like
planets are -- and identify candidates for further study. It is indeed a daunting challenge, but worth the effort. The goal is nothing short of finding worlds that could support life -- and perhaps some that do. Above: By taking advantage of the wave nature of light, interferometry can cancel out some of the light coming from a star, enabling the telescope to image the much dimmer planets in orbit around it. Image courtesy NASA's Terrestrial Planet Finder mission. Seeing E.T.'s "breath" Right: If an alien astronomer on a distant planet were exploring our solar system, they might guess that something special is happening on Earth. The spectra of Venus and Mars show the mark of a carbon dioxide-rich atmosphere, but only Earth's spectrum has strong ozone and water vapor fingerprints as well. Scientists will use clues such as these to search for the chemical signs of life on planets around other stars. Click on the image for a graphic showing the spectral fingerprints of several important chemicals for astrobiology. Image courtesy NASA's Terrestrial Planet Finder mission. If life is widespread on a planet, its
atmosphere should show signs of life's presence. Just as the
air you exhale has more carbon dioxide and less oxygen than the
air you inhale, the combined "breathing" of all the
life on a planet will change the chemistry of its atmosphere.
If life is plentiful on the planet, these changes may be large
enough to notice. Above: Even life on Earth can surprise scientists. The strange deep-sea creatures in this ecosystem, discovered in 1977, thrive on chemical energy rather than sunlight. [more] Fortunately, the chemical constraints within which life must function make it likely that simple molecules such as oxygen and carbon dioxide will play the same roles in an extraterrestrial biology as they do on Earth. "Suppose," says Meyer, "that there is silicon-based life. [It might be] photosynthetic, and you would still end up with oxygen in the atmosphere. You could go there and the life could be completely different, but some of the chemistry could still be the same [as on Earth]." "The small molecules are going
to be more universal," agrees Des Marais. "Large molecules
like DNA and chlorophyll represent later, highly significant
innovations of life on Earth, but also the ones that may have
differed elsewhere." Above: Oxygen gas is a good indicator of life. But, scientists caution, oxygen has been abundant on Earth only since the advent of photosynthesis -- probably a billion years or more after life began! To have the greatest chance of spotting extraterrestrial life, astrobiologists must consider how life looked on the young Earth, too, when the atmosphere was different. Image courtesy David Des Marais and Kevin Zahnle. Oxygen and its tag-along cousin ozone will top the list of target molecules. Without life, oxygen should be rare on rocky worlds. A small amount of it can be created without life by ultraviolet radiation that splits water vapor into hydrogen and oxygen. But that oxygen would be readily consumed by rocks and minerals on the planet's surface in the "oxidizing" reactions that produce, for example, rust. Volcanic gases also react with oxygen and remove it from the atmosphere. Geological processes alone usually work against the accumulation of oxygen. An oxygen-rich atmosphere is, therefore, out of chemical equilibrium, suggesting that some active agent -- namely photosynthetic life -- is constantly replenishing the supply. As Carl Sagan noted in a 1997 Scientific American article, "the great concentration of oxygen (20 percent) in Earth's dense atmosphere is very hard to explain by [any means other than life.]" The same would be true of planets around other stars. Below: This planet, which harbors abundant life, has an oxygen-rich atmosphere (with a dash of methane) and telltale signs of chlorophyll on the ground. Next on the list of target molecules is methane. Scientists suspect that for roughly the first billion years of its history, life on Earth had not yet evolved oxygen-producing photosynthesis. Instead, the microorganisms that then dominated the planet tapped the energy in gases leaking out of the Earth's interior, with some microbes creating methane as a byproduct. On a planet with a similar geology to Earth, methane levels greater than about 100 parts per million would suggest the presence of life. But methane would be a more ambiguous discovery than oxygen, because planets of a different geological make-up might produce abundant methane without life. Other details about these planets -- such as their size, their distance from the parent star, their carbon dioxide and water vapor levels, and their reflectivity -- will help scientists accurately interpret a methane or oxygen discovery. These other details can also be measured (or at least estimated) using TPF and other telescopes. Some of these ideas have already been tested on a planet known to support life -- Earth. In 1990, the Galileo spacecraft made a flyby of our planet on its circuitous journey to Jupiter. As it passed, Galileo's sensors detected high levels of oxygen and methane in Earth's atmosphere and signs of chlorophyll on the ground. Chlorophyll, which absorbs light at the far-red end of the visible spectrum, is a "red flag" for life. The TPF won't be sensitive to chlorophyll on a planet's surface because atmospheric water vapor, which is opaque in the mid-infrared frequency range that TPF will observe, will hide the surface below. Even without chlorophyll, signs of oxygen and methane -- which TPF can detect -- would make a persuasive case for life. If the TPF finds a habitable planet with lots of oxygen and some methane in its atmosphere, it would be a momentous discovery. But would such data really prove life is there? "Proof" is always a tall order in science, especially when discussing extraterrestrial life. Nevertheless, say astrobiologists, such evidence would be "very compelling." Above: This proposed design for NASA's Terrestrial Planet Finder mission will combine the light from four powerful telescopes to make Earth-size planets orbiting other stars visible. [more] One day it might happen ... and after catching its first whiff of E.T.'s breath, humanity won't likely give up the chase. The next step would be an even larger space telescope that could see the planet as more than one pixel, allowing scientists to see surface features such as continents and to observe the changing of the planet's seasons. And perhaps by the end of the next decade it would be possible to send a probe across interstellar space to take a close-up look, which could finally provide incontrovertible evidence. Proof will be for the patient: Even using advanced propulsion technologies, a probe might take decades to reach a neighboring star. But to answer a profound question that's been asked by humanity for centuries, perhaps that isn't too long to wait. |
Credits & Contacts Author: Patrick L. Barry Responsible NASA official: John M. Horack |
Production Editor:
Dr.
Tony Phillips
Curator: Bryan Walls Media Relations: Steve Roy |
The Science and Technology Directorate at NASA's Marshall Space Flight Center sponsors the Science@NASA web sites. The mission of Science@NASA is to help the public understand how exciting NASA research is and to help NASA scientists fulfill their outreach responsibilities. |
Web Links |
PlanetQuest -- Learn more about planet-searching from JPL. Another great site is ExoPlanets.org. The Search for Extraterrestrial Life -- in this Scientific American article, Carl Sagan discusses the chemical signs of life on another planet and a fortuitous "control" experiment -- the 1990 flyby of the Earth by the Galileo space probe Alien Atmospheres -- Science@NASA article: NASA's Hubble Space Telescope has detected the atmosphere of a planet circling a distant Sun-like star Can Silicon-based Life Exist? -- one scientist's answer, from Scientific American Telescope Technology May Yield Images of Extra-Solar Planets -- Washington Post article: Ground-based telescopes equipped with flexible mirrors are on the verge of being able to photograph large planets orbiting nearby stars. The Shape of Extraterrestrial Life --Science@NASA article: NASA scientists pioneer artificial intelligence algorithms to search for extraterrestrial organisms Astrobiology's Most Wanted --Science@NASA article: A failure to recant resulted in the strange case of Giordano Bruno When did photosynthesis emerge on Earth? -- a paper by Davis Des Marais Timeline of the Universe -- a tutorial on the phases of cosmic evolution, from the Big Bang to the emergence of life on Earth. From NASA's Origins program. Astrobiology roadmap -- a series of objectives in the search for life beyond Earth, from the NASA Ames Research Center Interferometry -- more about the technique, from the Space Interferometry Mission website The search for life in the Universe -- from NASA's Origins program NASA's
Astrobiology Institute -- home page The Terrestrial Planet Finder mission -- home page for the space telescope that will look for signs of life on distant worlds The Space Interferometry Mission -- a precursor to the Terrestrial Planet Finder which will pioneer space-based interferometry Kepler space telescope -- home page |
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