If you're looking for life similar to Earth's -- based, that is, on carbon chemistry and water -- you have to determine what kind of stars might have produced such planets. Certain factors weigh heavily in this analysis. The star must be a long-lived, solar-type star with constraints on its luminosity; it must offer an environment within which a planet with liquid water at its surface can exist. This Continuously Habitable Zone (CHZ) is defined this way in a new paper called "Astrobiologically Interesting Stars within 10 parsecs of the Sun," now available on the arXiv site: The inner edge of habitability is the region where water is lost through photolysis and hydrogen escape; the oceans simply evaporate; The outer edge of habitability is the region where C02 clouds form, cooling the planet by lowering its albedo. Also critical is planetary mass. A reasonable upper limit on mass seems to be a few Earth masses; planets larger than this are likely to be entirely covered with oceans,...
FTL Technologies and Inflation Theory
What could inflation theory have to do with the Fermi paradox? Quite a lot, if at least one recent paper is to be believed. The question 'where are they' about extraterrestrial visitation becomes even more pointed when faster-than-light technologies move out of the realm of the impossible to something that may be seriously investigated by physicists. Inflation theory, which holds that the early universe underwent a vast expansion as spacetime itself stretched far beyond the velocity of light, opens the door to technologies that might use this effect to create spacefaring civilizations spanning entire galaxies. Just how fast did inflation occur? In a space of time lasting about 10-35 seconds, the universe could have expanded by a factor of 1030 to 10100. As Brian Greene puts it in The Fabric of the Cosmos: An expansion factor of 1030 -- a conservative estimate -- would be like scaling up a molecule of DNA to roughly the size of the Milky Way galaxy, and in a time interval that's much...
A Fusion Runway to Nearby Stars
When physicist Geoffrey Landis reviewed interstellar concepts at the American Association for the Advancement of Science's 2002 meeting, his wide-ranging presentation considered where we stand on nuclear propulsion, solar and lightsail technologies, and particle-pushed sails. He also addressed the question of the Bussard ramjet, which would use an electromagnetic scoop to collect atoms from the interstellar medium to fuel a fusion reactor. Finding serious problems here (he cites, among other things, the fact that the scoop technology acts more like a brake than an accelerator), Landis went on to consider an alternative: "These problems can be alleviated if, instead of using the ambient interstellar medium, fuel is deliberately emplaced in the path of the spacecraft before flight. In this way, the fuel (probably in the form of small 'pellets') can be chosen to be the optimum composition... The 'runway' of fuel pellets could be emplaced, for example, by a dedicated craft which drops...
The Distance to Alpha Centauri
We can measure interstellar distances, but can we really grasp them? The distance to the nearest stars is so immense that even the scientists who study such things have resorted to homely comparisons. The most charming to my mind is that of the English astronomer Sir John Herschel (1792-1871), the son of the famous William Herschel who discovered Uranus. A wizard at mathematics, Herschel became a leading expert on double stars and the measurement of stellar distances through parallax (the apparent change in position of a nearby star against background stars due to the Earth's changing orbit around the Sun). When it came to the distance to the Alpha Centauri stars, Herschel saw things in terms of ocean voyaging, thinking himself standing on shipboard dropping peas into the water. As he once wrote, ". . . to drop a pea at the end of every mile of a voyage on a limitless ocean to the nearest fixed star, would require a fleet of 10,000 ships of 600 tons burthen, each starting with a full...
The Light of Ancient Stars
The Spitzer Space Telescope once again dazzles us with its capabilities at infrared wavelengths. Now it's the detection of what may be some of the earliest objects in the universe, the hypothetical Population III stars that would have formed a mere 200 million years after the Big Bang itself. These short-lived objects were probably over a hundred times more massive than our Sun. If the scientists investigating the recent Spitzer data are right, they are looking at the redshifted ultraviolet light of these ancient stars, stretched to lower energy levels by the expansion of the universe and now detected as a diffuse glow of infrared light. Image: The top panel is an image from NASA's Spitzer Space Telescope of stars and galaxies in the constellation Draco, covering about 50 by 100 million light-years (6 to 12 arcminutes). This is an infrared image showing wavelengths of 3.6 microns, below what the human eye can detect. The bottom panel is the resulting image after all the stars,...
‘Alien’ Life on Earth?
"We may never find other life away from Earth, but we have already made aliens on this planet and we will continue to do so at an increasing pace," says Peter Ward, author of Life As We Do Not Know It: The NASA Search for (and Synthesis of) Alien Life (Viking, 2005). "In the last five years we've come to realize that we can make microbial life in a lot more ways than Mother Earth did." Aliens on this planet? Ward is talking about laboratory work here on Earth that has modified life as we commonly understand it. That includes creating microbes with at least one amino acid beyond the 20 found in the DNA of native Earth life. Genetic modification also constitutes, in Ward's view, the creation of an alien lifeform, as does modifying a lifeform to reduce its complexity. Ward, a paleontologist who studies these matters within the University of Washington's astrobiology program, is perhaps best known to Centauri Dreams readers as the co-author (with Donald Brownlee) of Rare Earth: Why...
New Moons for Pluto
The Hubble Space Telescope, in operations designed to support the upcoming New Horizons mission to Pluto, has discovered two new Plutonian moons. It's too early to speak with confidence about their size because we don't yet know to what extent light reflects from their surfaces, but the early estimates are for diameters of 32 kilometers (20 miles) and 70 kilometers (45 miles). Charon, at 1200 kilometers, dwarfs these tiny objects, provisionally designated S/2005 P1 and S/2005 P2. Their faintness makes it clear why they weren't spotted before: the new moons are roughly 5000 times fainter than Pluto itself. For more, see this Southwest Research Institute news release. "Our result also suggests that other bodies in the Kuiper Belt may have more than one satellite. We planetary scientists will have to take these new moons into account when modeling the formation of the Pluto system," says co-leader Dr. Alan Stern, executive director of the SwRI Space Science and Engineering Division. And...