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BethanyKismet |
Astronomy News & Rumor Thread |
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I used to post these all seperately, but let's try keeping it neat this time around. Post news on the final frontier here!
Last Edited By: General Ceel 12/09/09 6:00.
Edited 3 times.
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BethanyKismet |
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I'm sure that some of you have already read this but....
'Significant Amount' of Water Found on MoonBy Andrea Thompson, Senior Writer posted: 13 November 2009 12:16 p.m. ET
It's official: There's water ice on the moon, and lots of it. When melted, the water could potentially be used to drink or to extract hydrogen for rocket fuel. NASA's LCROSS probe discovered beds of water ice at the lunar south pole when it impacted the moon last month, mission scientists announced today. The findings confirm suspicions announced previously, and in a big way. "Indeed, yes, we found water. And we didn't find just a little bit, we found a significant amount," Anthony Colaprete, LCROSS project scientist and principal investigator from NASA's Ames Research Center at Moffett Field, Calif. The LCROSS probe impacted the lunar south pole at a crater called Cabeus on Oct. 9. The $79 million spacecraft, preceded by its Centaur rocket stage, hit the lunar surface in an effort to create a debris plume that could be analyzed by scientists for signs of water ice. Those signs were visible in the data from spectrographic measurements (which measure light absorbed at different wavelengths, revealing different compounds) of the Centaur stage crater and the two-part debris plume the impact created. The signature of water was seen in both infrared and ultraviolet spectroscopic measurements. "We see evidence for the water in two instruments," Colaprete said. "And that's what makes us really confident in our findings right now." How much? Based on the measurements, the team estimated about 100 kilograms of water in the view of their instruments - the equivalent of about a dozen 2-gallon buckets - in the area of the impact crater (about 80 feet, or 20 meters across) and the ejecta blanket (about 60 to 80 meters across), Colaprete said. "I'm pretty impressed by the amount of water we saw in our little 20-meter crater," Colaprete said. "What's really exciting is we've only hit one spot. It's kind of like when you're drilling for oil. Once you find it one place, there's a greater chance you'll find more nearby," said Peter Schultz, professor of geological sciences at Brown University and a co-investigator on the LCROSS mission. This water finding doesn't mean that the moon is wet by Earth's standards, but is likely wetter than some of the driest deserts on Earth, Colaprete said. And even this small amount is valuable to possible future missions, said Michael Wargo, chief lunar scientist for Exploration Systems at NASA Headquarters. Scientists have suspected that permanently shadowed craters at the south pole of the moon could be cold enough to keep water frozen at the surface based on detections of hydrogen by previous moon missions. Water has already been detected on the moon by a NASA-built instrument on board India's now defunct Chandrayaan-1 probe and other spacecraft, though it was in very small amounts and bound to the dirt and dust of the lunar surface. Water wasn't the only compound seen in the debris plumes of the LCROSS impact. "There's a lot of stuff in there," Colaprete said. What exactly those other compounds are hasn't yet been determined, but could include organic materials that would hint at comet impacts in the past. More questions The findings show that "the lunar poles are sort of record keepers" of lunar history and solar system history because these permanently-shadowed regions are very cold "and that means that they tend to trap and keep things that encounter them," said Greg Delory, a senior fellow at the Space Sciences Laboratory and Center for Integrative Planetary Sciences at the University of California, Berkeley. "So they have a story to tell about the history of the moon and the solar system climate." "This is ice that's potentially been there for billions of years," said Doug Cooke, associate administrator at Exploration Systems Mission Directorate at NASA Headquarters in Washington, D.C. The confirmation that water exists on the moon isn't the end of the story though. One key question to answer is where the water came from. Several theories have been put forward to explain the origin of the water, including debris from comet impacts, interaction of the lunar surface with the solar wind, and even giant molecular clouds passing through the solar system, Delory said. Scientists also want to examine the data further to figure out what state the water is in. Colaprete said that based on initial observations, it is likely water ice is interspersed between dirt particles on the lunar surface. Some other questions scientists want to answer are what kinds of processes move, destroy and create the water on the surface and how long the water has been there, Delory said. Link to Chandrayaan? Scientists also are looking to see if there is any link between the water observed by LCROSS and that discovered by Chandrayaan-1. "Their observation is entirely unique and complementary to what we did," Colaprete said. Scientists still need to work out whether the water observed by Chandrayaan-1 might be slowly migrating to the poles, or if it is unrelated. Bottom line, the discovery completely changes scientists' view of the moon, Wargo said. The discovery gives "a much bigger, potentially complicated picture for water on the moon" than what was thought even just a few months ago, he said. "This is not your father's moon; this is not a dead planetary body." Let's go? NASA plans to return astronauts to the moon by 2020 for extended missions on the lunar surface. Finding usable amounts of ice on the moon would be a boon for that effort since it could be a vital local resource to support a lunar base. "Water really is one of the constituents of one of the most powerful rocket fuels, oxygen and hydrogen," Wargo said. The water LCROSS detected "would be water you could drink, water like any other water," Colaprete said. "If you could clean it, it would be drinkable water." The impact was observed by LCROSS's sister spacecraft, the Lunar Reconnaissance Orbiter, as well as other space and ground-based telescopes. The debris plume from the impacts was not seen right away and was only revealed a week after the impact, when mission scientists had had time to comb through the probe's data. NASA launched LCROSS - short for Lunar Crater Observation and Sensing Satellite - and LRO in June. |
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Surge Korso |
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Yeah I read about this, exciting stuff no? From waterless to significant amount of water, can really change things.
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Mak Manto |
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The only thing that could be useful is to have a base on the moon, either to serve as an ear to the universe, searching for life and other events in the
cosmos, or it serves as a launching point for manned trips to Mars.
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BethanyKismet |
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They are doing some studies of long term effects of radiation like you find in space in plans of manned missions to mars.... lemme see if I can find that
article....
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BethanyKismet |
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NASA to Subject Monkeys to RadiationBy Clara Moskowitz, Staff Writer posted: 12 November 2009 09:54 am ET
NASA plans to subject a group of monkeys to radiation to study what might happen to humans on long-term space missions, such as trips to the moon and Mars. The research is the first time in decades that NASA has performed tests on primates, though the agency famously relied on the close human relatives to make some of the first forays into space in the 1950s. "The overall objective of the planned studies with the nonhuman primates is to help NASA predict neurobehavioral effects of space radiation, which are among the most poorly understood health risks for astronauts," NASA spokesman Bill Jeffs told SPACE.com. The agency plans to aim high-energy gamma-ray radiation at 27 squirrel monkeys, then observe how they perform tasks to see how they're affected, Florida Today reported. The experiment is meant to simulate the type of radiation humans are exposed to in space. As NASA plans trips to farther destinations, people will be spending longer amounts of time outside the Earth's protective atmosphere, so more knowledge of the health effects is vital, NASA said. "NASA-funded research has shown that simulated space radiation can affect nerve cells in culture and also the behavior of mice and rats, but these studies are limited in the extent they can be extrapolated to human behavior and performance," Jeffs said. "Studies in nonhuman primates are essential to be able to best predict neurobehavioral effects of radiation on humans." But some animal welfare advocates object to the use of monkeys in research that could harm them. A group of about 100,000 doctors, nurses and laypersons recently petitioned the space agency to put off the $1.75 million project, Florida Today reported, calling the experiment "one giant leap backward for NASA." The doctor planning to carry out the study for NASA, Jack Bergman of Harvard Medical School's McLean Hospital in Boston, declined to comment for this story. Other scientists who have worked with non-human primates defended the need for this type of research. "Due to their phylogenetic proximity to human beings, non-human primates provide a research subject as close to humans as possible," said Christian R. Abee of the University of Texas M. D. Anderson Cancer Center, who is not involved in the current project, but consulted with NASA for earlier primate studies. "Therefore, they are the ultimate translational science subject for many studies." The upcoming study intends to expose the test monkeys to a blast of radiation roughly equivalent to what astronauts would be exposed to on a three-year space voyage - the length of time it would take people to travel to Mars. Though the exposure will likely cause some cellular damage, it will not kill the monkeys, NASA told Florida Today. NASA maintained that the experiments would provide important knowledge for designing future missions. "Currently, there is no information regarding the effects of space radiation on neurobehavioral function in nonhuman primates," Jeffs said. |
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Jaxon Janenham |
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As well as serving as a defense platform to prevent those damned communists from ever getting onto the moon. You can't forget about
that!
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AvadreiaLacroix |
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Mak Manto wrote:What can the moon hear that we can't hear? |
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Khayman |
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I was thinking more along the lines of a prefect site to launch rockets from. But isnt there some *%*$ with the atmosphere which kinda causes interference and
stuff? Also, Moon would make a killer observatory.
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General Ceel |
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bump
Join, visit, or advertise your board at the oldest, largest, and most respected Star Wars community on Yuku/Ezboard: The Gungan Council since 1999. What is 1138? |
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BethanyKismet |
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Vampire Star Is a Ticking Time BombBy SPACE.com staff posted: 17 November 2009 10:12 am ET
A "vampire" star that underwent an outburst in 2000 after gulping down part of a companion star looks to be a ticking time bomb: It is poised to become the long-sought fuse to a certain type of supernova. The gas-sucking star is part of a double star system known as V445 in the constellation of Puppis ("the Stern"). In November 2000, this system underwent a nova outburst, becoming 250 times brighter than before and ejecting a large quantity of matter into space. To study the system further, a team of astronomers used the NACO adaptive optics instrument on the European Southern Observatory's Very Large Telescope (VLT) in Chile to obtain very sharp images of V445 Puppis over a time span of two years. Helium, not hydrogen The images show a bipolar shell, initially with a very narrow waist, with lobes on each side. Two knots are also seen at both the extreme ends of the shell, which appear to move at about 19 million mph (30 million kph). The shell - unlike any previously observed for a nova - is itself moving at about 15 million mph (24 million kph). A thick disk of dust, which must have been produced during the last outburst, obscures the two central stars. The VLT data also suggest that V445 Puppis could one day explode as a Type 1a supernova. Type 1a supernovas are a particular family of these life-ending stellar explosions, one prominent feature of which is a lack of a hydrogen signature in their spectrum, despite the fact that hydrogen is the most common element in the universe. V445 Puppis is the first, and so far only, nova showing no evidence at all for hydrogen. It provides the first evidence for an outburst on the surface of a white dwarf dominated by helium. "This is critical, as we know that Type Ia supernovae lack hydrogen," said team member Danny Steeghs of the University of Warwick in the United Kingdom, "and the companion star in V445 Pup fits this nicely by also lacking hydrogen, instead dumping mainly helium gas onto the white dwarf." A crucial question Type 1a supernovas are thought to arise in stellar systems composed of two stars, one of them being the end product of the life of sun-like stars - white dwarfs. When such white dwarfs, acting as stellar vampires that suck matter from their companion, become heavier than a given limit, they become unstable and explode. But the process isn't quite as simple as that: As the white dwarf cannibalizes its prey, matter accumulates on its surface. If this layer becomes too dense, it becomes unstable and erupts as a nova. These controlled, mini-explosions eject part of the accumulated matter back into space. The crucial question is thus to know whether the white dwarf can manage to gain weight despite the outburst - that is, if some of the matter taken from the companion stays on the white dwarf, so that it will eventually become heavy enough to explode as a supernova. Combining the NACO images with data obtained with several other telescopes allowed the astronomers to determine the distance to the system - about 25,000 light-years from the Sun - and its intrinsic brightness - over 10,000 times brighter than the Sun. This implies that the vampire white dwarf in this system has a high mass that is near its fatal limit and is still simultaneously being fed by its companion at a high rate. "Whether V445 Puppis will eventually explode as a supernova, or if the current nova outburst has pre-empted that pathway by ejecting too much matter back into space is still unclear," said team member Patrick Woudt of the University of Cape Town in South Africa. "But we have here a pretty good suspect for a future Type Ia supernova!" The findings for V445 Puppis are detailed in the Nov. 20 issue of the Astrophysical Journal. |
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BethanyKismet |
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And for those interested in a visual....
http://www.space.com/common/media/video/player.php?videoRef=SP_091117_vampire-star |
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Mak Manto |
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AvadreiaLacroix wrote:Well, with the moon being out much farther then the Earth is, we could build a radio telescope, such as Big Ear, on the moon, allowing for a far better chance of contact.
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Goff256 |
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Meh, who cares about listening for life? If they're advanced enough to get to us, what are we going to do in the relatively short amount of time it would
take them to get the extra 238k miles? XD
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Mak Manto |
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Well, if advanced life is looking for us, they're probably using ways to search for life out there as well.
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AvadreiaLacroix |
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BethanyKismet wrote:>_> Does it sparkle? |
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BethanyKismet |
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Oh god Ava, I bet it does! o.O
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BethanyKismet |
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Wild Solar System Spotted Around Distant Star
By SPACE.com staff posted: 10 November 2009 10:11 am ET A young star observed by the Spitzer Space Telescope appears to be home to a wild - and young - planetary system that shares some of the frenetic dynamics thought to have shaped the early years of our own solar system. The Spitzer observations suggest young planets circling the star are disturbing smaller comet-like bodies, causing them to collide and kick up a huge halo of dust. The star, called HR 8799, became one of the first of two stars with planets that were directly imaged from Earth in November 2008. Ground-based telescopes at the W.M. Keck Observatory and the Gemini Observatory, both in Hawaii, took images of three planets orbiting in the far reaches of the system. Each of the three distant worlds is roughly 10 times the mass of Jupiter. HR 8799 is younger and more massive than our sun, which is more than 4.5 billion years old and more than 300,000 times the mass of Earth. It is about 129 light-years from Earth, so scientists weren't sure if Spitzer would be able to snap a picture of its debris disk. But to their amazement, it succeeded. The Spitzer team, led by Kate Su of the University of Arizona, Tucson, says the giant cloud of fine dust around the disk is very unusual. The researchers say this dust must be coming from collisions among small bodies similar to the comets or icy bodies that make up today's Kuiper Belt objects in our solar system. "The system is very chaotic and collisions are spraying up a huge cloud of fine dust," Su said. The gravity of the three large planets is throwing the smaller bodies off course, causing them to migrate around and collide with each other. Astronomers think the planets may have yet to reach their final stable orbits, so more violence could be in store. A similar setup has also been seen by Spitzer and the Hubble Space Telescope around the star Fomalhaut, which sits about 25 light-years from Earth. "What's exciting is that we have a direct link between a planetary disk and imaged planets," Su said. "We've been studying disks for a long time, but this star and Fomalhaut are the only two examples of systems where we can study the relationships between the locations of planets and the disks." When our solar system was young, astronomers think it went through similar planet migrations. Jupiter and Saturn moved around quite a bit, throwing comets around, sometimes into Earth. Some say the most extreme part of this phase, called the late heavy bombardment, explains how our planet got water. Wet, snowball-like comets are thought to have crashed into Earth, delivering life's favorite liquid. The Spitzer results are detailed in the Nov. 1 issue of Astrophysical Journal. |
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BethanyKismet |
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Black Holes: Powerhouses of the UniverseBy Clara Moskowitz, Staff Writer posted: 09 November 2009 11:31 am ET
The brightest lights in the universe often come from the blackest pits of deep space. Black holes, so named because even light cannot escape their gravitational grasp, can only be sensed through their tug on other matter. While black holes themselves are invisible, the regions around them are reigned by powerful magnetic and gravitational forces that create some of the most luminous radiation ever seen. Super-bright anomalies like cosmic rays, plasma jets and gamma-ray bursts pour forth to fly across the universe, and researchers are just beginning to untangle the mysteries of how they arise. Infinitely dense Black holes are extremely dense masses jammed into single points of space. At their centers, all the matter is crushed to infinite density inside a space of zero volume, called a singularity. There, the pull of gravity is thought to be infinitely strong, warping space-time to be infinitely curved. Yet, for all the bizarre happenings inside black holes, if you are sufficiently far enough away from them, they act like any other matter. That means that if the sun were replaced with a black hole of the same mass, all the planets would continue to orbit around it just as usual, scientists have said, though Earth would not be habitable due to lack of sunlight. Black holes are thought to form during the explosive deaths of very massive stars. When a star exhausts all its fuel, it implodes under the crushing force of gravity into a denser and denser ball, eventually reducing down to a black hole. Meanwhile, the outside layers of the star are expelled in a powerful blast called a supernova. Rays, bursts and jets Scientists think some of the energy released by the explosion and formation of a black hole goes toward accelerating particles to great speeds, creating marvels called cosmic rays that fly through the universe at almost the speed of light. We detect some of these particles on Earth, where they still pack such a punch they can knock out electronics systems. Another consequence of black holes and supernovas are short flashes of high-energy gamma-ray light called gamma-ray bursts. They originate in distant galaxies and are the brightest things ever seen in the universe. The bursts likely arise when a very massive, rapidly-rotating star collapses into a black hole during a supernova explosion, and releases a short, intense beam of gamma-ray radiation. And black holes also seem to be to blame for the jets of hot charged gas seen spewing from the hearts of distant galaxies. These galaxies, called blazars, likely have supermassive black holes in their centers that are warping space-time in extreme ways. As dust and gas gets dragged toward a black hole, some of it is spit back out and accelerated by twisted magnetic fields around the black hole to shoot out in luminous jets that can be seen across the universe. "We studied a battery mechanism to extract the energy of a spinning black hole, and it provides a compelling way to power jets in high-energy gammaray sources," said Govind Menon, a professor of physics at Alabama's Troy University. Menon recently wrote the book "High Energy Radiation from Black Holes: Gamma Rays, Cosmic Rays, and Neutrinos," (2009, Princeton University Press) with astrophysicist Charles Dermer of the Space Science Division of the Naval Research Laboratory. The two scientists spoke about the topic Nov. 4 at the 2009 Fermi Symposium in Washington, D.C. The researchers said even more secrets of black holes are likely to be discovered soon thanks to new experiments like the Fermi Gamma-ray Space Telescope, the South Pole IceCube Neutrino Experiment, ground-based TeV (1000 GeV) gamma-ray detectors, and the Pierre Auger Cosmic Ray Observatory in Argentina. "This is a decade of incredible scientific discovery in high-energy astronomy and astroparticle physics," Dermer said. |
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General Ceel |
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updates, updates..... get this thread going.
Join, visit, or advertise your board at the oldest, largest, and most respected Star Wars community on Yuku/Ezboard: The Gungan Council since 1999. What is 1138? |
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BethanyKismet |
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Giant Cannibal Galaxy's Last Meal
By SPACE.com staff posted: 20 November 2009 09:42 am ET
New images show the "last meal" of a giant cannibal galaxy as it gobbles down a smaller spiral galaxy, which has been twisted and warped from being devoured. The giant galaxy, Centaurus A (NGC 5128) is the nearest giant, elliptical galaxy, at a distance of about 11 million light-years. The galaxy hosts a supermassive black hole that is 200 million times the mass of the sun, or 50 times the mass of the black hole at the center of the Milky Way. At the galaxy's center is an opaque dust lane that is thought to be the remains of a cosmic merger between the galaxy and a smaller spiral galaxy full of dust. Between 200 and 700 million years ago, this galaxy is believed to have consumed a smaller spiral, gas-rich galaxy - the contents of which appear to be churning inside Centaurus A's core, likely triggering new generations of stars. First glimpses of the "leftovers" of this meal were obtained thanks to observations with the European Space Agency's Infrared Space Observatory, which revealed a 16,500 light-year-wide structure, very similar to that of a small barred galaxy. More recently, NASA's Spitzer Space Telescope resolved this structure into a parallelogram, which can be explained as the remnant of a gas-rich spiral galaxy falling into an elliptical galaxy and becoming twisted and warped in the process. Galaxy merging is the most common mechanism to explain the formation of such giant elliptical galaxies. The new images, taken by the European Southern Observatory's 3.58-metre New Technology Telescope (NTT) in La Silla, Chile, allow astronomers to get an even sharper view of the structure of this galaxy, completely free of obscuring dust. What the astronomers found in the images was surprising: "There is a clear ring of stars and clusters hidden behind the dust lanes, and our images provide an unprecedentedly detailed view toward it," said Jouni Kainulainen, lead author of the paper reporting these results. "Further analysis of this structure will provide important clues on how the merging process occurred and what has been the role of star formation during it." The technique used to observe Centaurus A could help scientists better understand star formation in galaxies. "These are the first steps in the development of a new technique that has the potential to trace giant clouds of gas in other galaxies at high resolution and in a cost-effective way," said co-author João Alves. "Knowing how these giant clouds form and evolve is to understand how stars form in galaxies." |
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EPIII: ROTS 10th Anniversary: