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Posted: 29 Jan 2015 11:29 PM PST
Excerpt from sciencedaily.com
Two phenomena known to inhibit the potential habitability of planets -- tidal forces and vigorous stellar activity -- might instead help chances for life on certain planets orbiting low-mass stars, astronomers have found.
Two phenomena known to inhibit the potential habitability of planets -- tidal forces and vigorous stellar activity -- might instead help chances for life on certain planets orbiting low-mass stars, University of Washington astronomers have found.
In a paper published this month in the journal Astrobiology, UW doctoral student Rodrigo Luger and co-author Rory Barnes, research assistant professor, say the two forces could combine to transform uninhabitable "mini-Neptunes" -- big planets in outer orbits with solid cores and thick hydrogen atmospheres -- into closer-in, gas-free, potentially habitable worlds.
Most of the stars in our galaxy are low-mass stars, also called M dwarfs. Smaller and dimmer than the sun, with close-in habitable zones, they make good targets for finding and studying potentially habitable planets. Astronomers expect to find many Earthlike and "super-Earth" planets in the habitable zones of these stars in coming years, so it's important to know if they might indeed support life.
Super-Earths are planets greater in mass than our own yet smaller than gas giants such as Neptune and Uranus. The habitable zone is that swath of space around a star that might allow liquid water on an orbiting rocky planet's surface, perhaps giving life a chance.
"There are many processes that are negligible on Earth but can affect the habitability of M dwarf planets," Luger said. "Two important ones are strong tidal effects and vigorous stellar activity."
A tidal force is a star's gravitational tug on an orbiting planet, and is stronger on the near side of the planet, facing the host star, than on the far side, since gravity weakens with distance. This pulling can stretch a world into an ellipsoidal or egglike shape as well as possibly causing it to migrate closer to its star.
"This is the reason we have ocean tides on Earth, as tidal forces from both the moon and the sun can tug on the oceans, creating a bulge that we experience as a high tide," Luger said. "Luckily, on Earth it's really only the water in the oceans that gets distorted, and only by a few feet. But close-in planets, like those in the habitable zones of M dwarfs, experience much stronger tidal forces."
This stretching causes friction in a planet's interior that gives off huge amounts of energy. This can drive surface volcanism and in some cases even heat the planet into a runaway greenhouse state, boiling away its oceans, and all chance of habitability.
Vigorous stellar activity also can destroy any chance for life on planets orbiting low-mass stars. M dwarfs are very bright when young and emit lots of high-energy X-rays and ultraviolet radiation that can heat a planet's upper atmosphere, spawning strong winds that can erode the atmosphere away entirely. In a recent paper, Luger and Barnes showed that a planet's entire surface water can be lost due to such stellar activity during the first few hundred million years following its formation.
"But things aren't necessarily as grim as they may sound," Luger said. Using computer models, the co-authors found that tidal forces and atmospheric escape can sometimes shape planets that start out as mini-Neptunes into gas-free, potentially habitable worlds.
How does this transformation happen?
Mini-Neptunes typically form far from their host star, with ice molecules joining with hydrogen and helium gases in great quantity to form icy/rocky cores surrounded by massive gaseous atmospheres.
"They are initially freezing cold, inhospitable worlds," Luger said. "But planets need not always remain in place. Alongside other processes, tidal forces can induce inward planet migration." This process can bring mini-Neptunes into their host star's habitable zone, where they are exposed to much higher levels of X-ray and ultraviolet radiation.
This can in turn lead to rapid loss of the atmospheric gases to space, sometimes leaving behind a hydrogen-free, rocky world smack dab in the habitable zone. The co-authors call such planets "habitable evaporated cores."
"Such a planet is likely to have abundant surface water, since its core is rich in water ice," Luger said. "Once in the habitable zone, this ice can melt and form oceans," perhaps leading to life.
Barnes and Luger note that many other conditions would have to be met for such planets to be habitable. One is the development of an atmosphere right for creating and recycling nutrients globally.
Another is simple timing. If hydrogen and helium loss is too slow while a planet is forming, a gaseous envelope would prevail and a rocky, terrestrial world may not form. If the world loses hydrogen too quickly, a runaway greenhouse state could result, with all water lost to space.
"The bottom line is that this process -- the transformation of a mini-Neptune into an Earthlike world -- could be a pathway to the formation of habitable worlds around M dwarf stars," Luger said.
Will they truly be habitable? That remains for future research to learn, Luger said.
"Either way, these evaporated cores are probably lurking out there in the habitable zones of these stars, and many may be discovered in the coming years."
Posted: 29 Jan 2015 11:20 PM PST
Excerpt from cnn.com
Paleontologists have discovered a 50-ft "dragon" dinosaur species in China that may have roamed the earth 160 million years ago in the Late Jurassic period.
The long skeleton was found in 2006 by some local farmers digging for a fishpond in Qijiang city in China's southwestern Chongqing province.
Lida Xing, a member of the research team from the University of Alberta who made the discovery, told CNN it was named Qijianglong, the "dragon of Qijiang" because farmers thought the bones resembled the shape of Chinese mythical dragons.
The reconstructed skeleton of Qijianglong in Qijiang Museum in China
"We found the dinosaur's huge vertebrae with the skull and the tail, but couldn't find any bones from the hands or the legs. So the locals began to say the long body looked just like a dragon from ancient Chinese stories," he said Xing.
The findings, published earlier this week in the Journal of Vertebrate Paleontology, show that the new species belongs to a group of dinosaurs called mamenchisaurids, known for their extremely long necks, which would measure up to half their body length.
Most sauropods, or long-necked dinosaurs, such as those depicted in the popular animated series, "The Land Before Time," have necks that only span one third of their body length.
The skeleton is now housed in a local museum in Qijiang, but will be moved to a new dinosaur museum in the city that is currently being built.
Dinosaurs were NOT wiped out by a global firestorm: Asteroid impact was not hot enough to ignite nearby plants, study claims
Posted: 29 Jan 2015 11:32 PM PST
Excerpt from dailymail.co.uk
By Jonathan O'Callaghan
The theory that a global firestorm accompanied the asteroid that killed off the dinosaurs may not be correct, according to a new study.
A team of researchers has found that heat near the impact site would not have been sufficient to ignite plants.
It suggests our understanding of the mass extinction event that wiped out the dinosaurs may not be as complete as thought.
UK researchers studied the asteroid impact 66 million years ago (illustration shown). They found the heat near the impact site in Mexico was not intense enough to ignite plant material. A heat pulse lasted less than a minute, too short to set plants alight
The team of researchers from the University of Exeter, University of Edinburgh and Imperial College London recreated the immense energy that would have been released from the asteroid impact 66 million years ago.
They found that the intense but short-lived heat near the impact site could not have ignited live plants, challenging the idea that the impact led to global firestorms.
These firestorms have previously been considered a major contender in the puzzle to find out what caused the mass extinction of life on Earth 66 million years ago.
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