How did the mechanism for protein synthesis -- the ribosome -- come into being? Answering that question would be useful not just in the study of life on Earth, but also in learning where else in the universe we might expect to find life. Intense work on the subject is ongoing at the University of Houston, where a team led by George E. Fox, a professor of biology and biochemistry, is studying how protein synthesis began and evolved. Protein synthesis happens when RNA copies genetic information from DNA and turns that raw data into proteins that are essential to the functioning of living cells. "Since many of the components of the ribosome are shared by all organisms, we know this machinery is very, very old," Fox said. "If we can discover the earliest aspects, then scientists may be able to devise experiments to see how simple RNAs might have given rise to this machinery. This information would help us to better understand how life evolved on Earth and how ribosomes actually work,...
A Novel Solution to Fermi’s Paradox
Enrico Fermi's famous question "Where are they?" continues to resonate among scientists and laymen alike. After all, shouldn't the universe be teeming with life, and hasn't intelligent life had enough time to spread through our own galaxy? Some estimates put the average age of Earth-like planets in the Milky Way at 6.4 billion years, whereas our own Earth is 4.5 billion years old. Some biospheres, in other words, may have had a two billion year jump on us. Shouldn't we be seeing signs of extraterrestrial life? One intriguing solution to the Fermi paradox appears in Karl Schroeder's novel Permanence (New York: Tor Books, 2002). Using a hypothesis from evolutionary biology called 'adaptationism,' Schroeder's protagonist argues that consciousness is not necessarily required for toolmaking. "In fact, consciousness appears to be a phase. No species we have studied has retained what we could call self-awareness for its entire history. Certainly none has evolved into some state above...
Triple Asteroid Discovered
Asteroid 87 Sylvia, known since 2001 to be part of a double system, has just gotten more interesting. A team of astronomers at the University of California at Berkeley and the Observatoire de Paris have now established that the asteroid is actually part of a triple system, the first ever discovered. Using data from the European Southern Observatory's Very Large Telescope array in Chile, the team found two small moons in nearly circular orbits. Astronomical names are always a challenge, but in this case naming comes easy. 87 Sylvia was named for Rhea Sylvia, the mother of the founders of Rome. Thus it made perfect sense for Berkeley's Franck Marchis to propose Romulus and Remus as the names of the moons. The suggestion has already been approved by the International Astronomical Union. Image: Artist's conception shows twin moonlets, Romulus and Remus, orbiting the large main-belt asteroid 87 Sylvia. Credit: European Southern Observatory. Calling them 'moons' should not obscure the fact...
New Data on Catastrophic Asteroid Impacts
The recent images from Cassini's flyby of Mimas remind us how violent the history of the early Solar System was. Now a study at the Australian National University shows that three huge asteroids -- between 20 and 50 kilometers across and traveling as a cluster -- collided with the Earth some 3.2 billion years ago. The result: volcanic eruptions, the creation of major fault lines, earthquakes and a variety of disruptive effects deep inside Earth's crust. This work grows out of evidence of extraterrestrial impact deposits from this era discovered in South Africa and extends the effects of those impacts to the Pilbara region of Western Australia. According to an ANU news release, the materials studied in the eastern Transvaal had indicated that impact craters several hundreds of kilometers in diameter had been created in oceanic parts of the Earth. In the Australian studies, the impacts coincide with the formation of fault escarpments and fault troughs and a major volcanic episode....
Finding the Sun’s Twin
A star in the constellation Serpens may be a close match for our own Sun. HD 143436 (also known as HIP 78399, from its listing in the Hipparcos survey) is an 8th magnitude star that's 140 light years from Earth and visible with binoculars. According to a recent article on the star by astronomer Ken Croswell, both its spectral type and its absolute magnitude are closely similar to Sol, and the star appears to be equally hot, with a temperature of 5768 Kelvin vs. the Sun's 5777 K. In terms of mass, HD 143436 is the Sun's twin. Finds like this are intriguing because they raise the possibility that similar stars have similar solar systems, within which may lurk a terrestrial world. No one knows whether this star has a planet like Earth around it -- or any planets at all, for that matter -- but we do know that the close stellar match calls for further work. Exactly how old HD 143436 is remains conjectural, with an uncertainty either way of 2.9 billion years. The star may be as old as the...
Mimas: A Tortured History, and a Warning
Can any other surface in the Solar System be this battered? The twin views below show Saturn's moon Mimas as imaged by Cassini on August 2. Note how the false-color brings out the variation across this tortured surface -- at left is an enhanced clear-filter image, at right a color composite of ultraviolet, infrared and clear-filter images. The most prominent feature in both is the 140-kilometer wide Herschel Crater, an ancient strike that is today filled with landslide material. Close study reveals numerous other craters and long grooves similar to those found on asteroids. Are these grooves related to the enormous impact that created the Herschel crater? No one knows, but study of this moon's turbulent history may help scientists understand how many impactors have moved through the Saturn system, a reminder of how dangerous a place the Solar System can be when you're in the crosshairs of an approaching piece of space debris. Mimas is a tiny place, measuring just 397 kilometers...
A Theory of Interstellar Migration
A continuing preoccupation at Centauri Dreams is long-term thinking. What can we as a species do to extend our time-frame beyond the infuriating short-term outlook of today, so that we can start thinking realistically about shaping a future beyond our own lifetimes? This kind of thinking will be necessary when we build our first interstellar probes, traveling journeys that will surely take decades and may involve centuries. What will drive us to think and plan within the millennial time frames that would allow humans to expand into and throughout the galaxy? Novelist Stephen Baxter addresses this question in a recent paper in the Journal of the British Interplanetary Society. Baxter points out the enormity of the time challenge: Voyager 1, the fastest human object ever built, travels at some 17.3 kilometers per second. It would reach Alpha Centauri (if headed in that direction) in 73,000 years. But starships that can reach 0.1c are not beyond possibility. If we can develop them, it's...
The Search for Missing Quasars
Quasars remain a mystery in several key areas. These massive black holes that live at the center of distant galaxies are voracious, and we know that they can consume the equivalent mass of a thousand stars every year. Surrounded by rings of dust and gas, they light up as they pull in this material to become the fantastically bright objects we observe not just in visible light, but in infrared and x-ray light as well. And that's the problem. To get a count on how many quasars are out there, astronomers have measured the cosmic x-ray background, where quasars outshine everything in the universe. It should be possible to predict how many quasars there are using this method, but it doesn't seem to work. In fact, the estimated number derived from the x-ray background doesn't match the figures derived from x-ray and optical observations of known quasars. In other words, something is hiding many of the universe's quasars from our view. Now the Spitzer Space Telescope has used its infrared...
Life’s Potential in the Early Universe
Complex carbon-based molecules are considered the building blocks of life. Now the Spitzer Space Telescope has detected evidence for molecules made up of hydrogen and carbon in galaxies some 10 billion light years from Earth. The organic compounds -- polycyclic aromatic hydrocarbons, known as 'PAHs' -- are common on Earth and in galaxies like the Milky Way, but no instrument has found them as far back in time as Spitzer. PAHs are called 'organic' because of their carbon atoms. That doesn't translate to 'life-bearing,' for any molecule containing carbon is considered 'organic,' whether or not biology is involved. But find organic compounds and you find at least the potential for life. "This is 10 billion years further back in time than we've seen them before," said Dr. Lin Yan of the Spitzer Science Center at the California Institute of Technology in Pasadena, Calif. Yan and team will publish their findings in the August 10 issue of the Astrophysical Journal. What makes the Spitzer...
Thinking About Cosmos 2
Regular readers of Centauri Dreams will know James Benford as the scientist who showed that microwaves could move a sail in a vacuum. That experiment, performed at the Jet Propulsion Laboratory, involved a 10-kilowatt microwave beam and a 10 sq cm sail in a vacuum chamber. The material used was a carbon fiber material commonly called carbon-carbon, in which carbon molecules are fused together in a structure called a 'microtruss.' Developed by San Diego's Energy Science Research Laboratories, carbon-carbon is terrifically interesting as a possible material for early solar and beamed sail work. The president of Microwave Sciences in Lafayette CA, Benford wrote in a recent e-mail about the failed Cosmos 1 solar sail launch. He had hoped to oversee a microwave experiment using the Deep Space Network's Goldstone facilities to test the effects of a microwave beam on a sail in operational conditions, but that was not to be. At least, not this time. Benford's message is worth quoting, and is...
Sharpening Our View of the 10th Planet
Over the weekend, more news came in about 2003 UB313, the soon to be renamed new planet discovered at Palomar Observatory. As discussed in astronomer Mike Brown's page on the discovery, 2003 UB313 is the largest object found orbiting the Sun since Neptune and its moon Triton in 1846. There seems to be no doubt that it is larger than Pluto and, like that planet, a member of the Kuiper Belt, a vast band of icy objects beyond Neptune. Remarkably, the 2003 UB313 team has found 80 bright Kuiper Belt objects since beginning its survey of the outer Solar System in 2001, but none so newsworthy as this one. Artist2003 UB313 takes twice as long to orbit the Sun as Pluto, and it is currently more than three times more distant, although it moves in an elliptical orbit that can bring it within Pluto's orbit and close to that of Neptune. Size limits can now be set ranging from 2210 to 3550 kilometers, depending on the nature of the surface and how it reflects light. Hubble measurements, already...
The Real Planet X
A day after the news about 2003 EL61, a Kuiper Belt object originally thought to be larger than Pluto, we now have another world that appears significantly larger still. 2003 UB313 was discovered with the Samuel Oschin Telescope at the Palomar Observatory by astronomers Mike Brown (Caltech), Chad Trujillo (Gemini Observatory), and David Rabinowitz (Yale University). Evidently the lower limit of its size is Pluto, and it may be (and probably is) larger. Image: Three views of the new planet. Credit: Mike Brown, California Institute of Technology. Now some 97 AU from the Sun, the planet is the farthest-known object in the Solar System. A news release from Caltech quotes Brown on 2003 UB313 and its credentials as a planet: "It's definitely bigger than Pluto," says Brown, who is professor of planetary astronomy. Scientists can infer the size of a solar-system object by its brightness, just as one can infer the size of a faraway light bulb if one knows its wattage. The reflectance of the...
A New Planet Larger Than Pluto?
A bright, slowly moving object in the outer Solar System may be a world larger than Pluto. A team of astronomers led by Jose-Luis Ortiz at the Sierra Nevada Observatory in Baja, California found the object, called 2003 EL61, using observations made in 2003. It is some 51 AU from the Sun (one AU, or Astronomical Unit, is the distance from Earth to the Sun), and evidently comes as close as 35 AU, inside Pluto's average distance of 39 AU. An analysis of older observations shows the object in images dating back to 1995. [Note: the Sierra Nevada Observatory was mistakenly identified as being in Spain in an earlier version of this post]. Is 2003 EL61 a new planet? And for that matter, how do we define what a planet is? That debate is sure to be reignited as we weigh the possibilities here, for a world larger than Pluto surely has to be considered a planet. But size measurements this far out from the Sun are tricky, and rely on an object's albedo, a measure of how much light the object...
Tantalizing Evidence for Cosmic Strings
An object called CSL-1 may have a lot to say about the nature of the universe. The odd thing about this double source -- evidently a pair of galaxies -- is that both galaxies appear identical. They share a common redshift, a similar shape, and their luminosity profiles match that of two giant elliptical galaxies. Moreover, the spectra of the two components seem to be identical. Is this a double image of the same galaxy? If so, then something tantalizing is going on. String theory, the latest and still evolving explanation for how the universe works, says that there should be gigantic counterparts to the strings that make up the fundamental particles of matter. A single-dimensional string millions of light years in length -- think of it as a thread of energy -- is one prediction made by string theory, and CSL-1 may indicate the presence of just such a cosmic string. For a cosmic string would be so energetic that it would warp spacetime around it, with the effect that a string lying...
Enceladus Flyby Reveals Bizarre Geology
No body in the solar system is as reflective as Saturn's moon Enceladus. Its terrain also appears relatively young, with the early Cassini flybys revealing regions that are only lightly cratered. It seems that Enceladus has undergone a number of episodes of geologic convulsion, with the southernmost latitudes seeing the most recent activity, producing a tortured surface marked by crisscrossing faults, folds and ridges. All this comes from findings revealed by the July 14 Enceladus flyby and discussed recently in a news release from the Cassini Imaging Central Laboratory for Operations. The latest flyby brought Cassini within 175 kilometers (109 miles) of the moon, showing that the landscape near its south pole is studded with ice boulders the size of houses, while impact craters in the region are almost entirely absent. Some of the ice blocks are up to 100 meters (328 feet) across, and they appear in an area that lacks the fine-grained frost found elsewhere on Enceladus. All that...
The Hunt for ‘Hot Earths’
By now we all know what a 'hot Jupiter' is -- a gas giant orbiting breathtakingly close to its parent star. The radial velocity searches for extrasolar planets that have found so many new worlds are particularly sensitive to high-mass planets in close orbits, so it makes sense that the early list of discoveries would be populated mostly with hot Jupiters. It's intriguing (and typical of the entire field of extrasolar planet detection) that this is a category of planet few scientists expected to find, especially in such numbers. But look what has happened to the planet hunt. In 2000, Geoff Marcy and Paul Butler detected the first planet with a mass below that of Saturn. It orbits the star HD 46375, some 109 light years away in the constellation Monoceros. The duo also discovered a planet 70 percent of Saturn's mass orbiting the star 79 Ceti, 117 light years away in the constellation Cetus. In 2004, a team led by Portuguese researcher Nuno Santos discovered a planet 14 times the size...
Lighting Up the Solar Wind
Tracking down the history of a star is no easy matter, but a supernova called SN 1979C is providing unexpected assistance. Just as researchers can study ancient climates by examining the concentric rings inside a tree, astronomers using the European Space Agency's XMM-Newton space observatory have found a way to study the rings around a star. SN 1979C, it turns out, produced huge stellar winds late in its life that flung particles into space over a period of millions of years. The result: a series of concentric rings lit up by x-rays when the star exploded. "We can use the X-ray light from SN 1979C as a 'time machine' to study the life of a dead star long before it exploded," says Dr Stefan Immler, leader of the team, from NASA's Goddard Space Flight Center, USA. "All the important information that usually fades away in a couple of months is still there." Image (click to enlarge): XMM-Newton image of X-ray light from the galaxy M100. Credit: European Space Agency. Immler and...
To the Stars via Radioactive Decay
If you wanted to reach Alpha Centauri in 40 years, one way to do it would be to boost a spacecraft up to 10 percent of lightspeed as quickly as possible and then let it coast to destination. Or you could do something entirely different: push your payload at constant acceleration halfway to Centauri, turn it around at the halfway point, and perform a uniform deceleration that gets you to into Centauri space with zero speed. To achieve the latter -- no small feat, needless to say -- requires a constant acceleration of 0.0105g. That number comes from the work of Italian physicist and mathematician Claudio Maccone, whose new paper "Radioactive Decay to Propel Relativistic Interstellar Probes Along a Rectilinear Hyperbolic Motion (Rindler Spacetime)" discusses a novel way to design an interstellar probe. Maccone's study of constant acceleration (using what special relativity calls 'hyperbolic motion') shows that it could provide an ideal mission profile if we can find a way to propel a...
Terrestrial Worlds in the Making?
So many of the planets discovered in the last ten years have been gas giants, circling their parent stars in extremely tight orbits. We assume there are rocky, terrestrial worlds out there in abundance, but until more advanced detection techniques are in place, how can we be sure? An important answer may be offered by BD +20 307, a Sun-like star some 300 light years from our Solar System. It's surrounded by a warm disk of silicate dust particles that shows all the signs of being formed from the collision of rocky bodies up to planet size. Located in the constellation Aries, the star has one more ace up its sleeve. Its dust -- found in greater profusion than has ever been observed around a Sun-like star this long after its formation -- exists at distances comparable to that of the Earth from the Sun. Finding such an infrared dust signature at Earth-like distances (i.e., 1 AU) has long been a goal of researchers. As revealed in the July 21 issue of the British science journal Nature,...
Rare Occultation Promises New Look at Charon
With excitement building over what everyone hopes will be a January launch of the New Horizons mission to Pluto and Charon, astronomers have found yet another tool for studying the distant worlds. They're taking advantage of a rare alignment in which Charon, Pluto's moon, passes in front of a star. Such an event has been observed only once, some 25 years ago, and with less capable instrumentation. We'll know a lot more about the results of the July 10-11 occultation in September, when they're presented at the 2005 meeting of the American Astronomical Society's Division of Planetary Sciences meeting, to be held in Cambridge, England. There, scientists from MIT and Williams College will report on observations taken with four telescopes located at various sites in Chile. Remarkably, the team was able to muster more than 100 square meters of telescope surface facing Charon, a number that represents a '...noticeable fraction of the world's total telescope area,' according to an MIT news...