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Honoring Copernicus - Three New Elements Added To The Periodic Table - 0 views

  • November 4, 2011, the General Assembly of the International Union of Pure and Applied Physics (IUPAP) is meeting at the Institute of Physics in London, to approve the names of three new elements
  • Element 110, darmstadtium (Ds),
  • Element 112. copernicium (Cn).
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  • Element111, roentgenium (Rg)
  • Are these new elements? Probably not.
  • As a general rule, these “new elements” are given names by their discoverer – which also leads to international debate
  • elements can be named after a mythological concept, a mineral, a place or a country, a property or a very known scientist… even an astronomer
  • element 112, this extremely radioactive synthetic element can only be created in a laboratory
  • Copernicium was created on February 9, 1996 by the Gesellschaft für Schwerionenforschung
  • its original name – ununbium – didn’t get changed until almost two years ago when a German team of scientists provided enough information to prove its existence
  • the rules were that it had to end in “ium” and it couldn’t be named for a living person.
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Chemistry's Biggest Loser: Official Atomic Weights Change For 19 Elements | Popular Sci... - 0 views

  • Improved measurements of different elements and their isotopes have changed the official atomic weights of 19 elements
  • The changes are relatively small, and they're part of a regular effort to update atomic weights
  • Every atom of an element
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  • silver as an example
  • has the same number of protons
  • Silver has 47
  • not every atom of an element necessarily has the same number of neutrons
  • different versions of an element's atoms are called isotopes
  • Silver occurs as silver-109 and silver-107
  • Chemists calculate the atomic weight of an element that you see on the periodic table from the masses of its isotopes, giving more common isotopes more weight than less common isotopes
  • doesn't necessarily mean every sample of silver on Earth has an atomic weight of exactly
  • samples of elements vary from place to place
  • erences play an important role in many sciences
  • They help chemists trace the origin of different materials
  • and date archaeological findings
  • The latest atomic weights measurements differ too little from their predecessors to really change science
  • do it?"
  • If it's just small changes, why
  • should give the best numbers there are
  • some new idea will come up that needs more accurate data
  • Molybdenum, Losing 0.0122
  • Atomic weights are relative, so they don't have units
  • Thorium, Losing 0.000322
  • Yttrium and Niobium, Tied, Losing 0.00001
  • Selenium, Gaining 0.0088
  • Cadmium, Gaining 0.0026
  • Holmium, Thulium and Praseodymium, All Tied, Gaining 0.00001
  • The changes in weights mostly come from continuing improvements in atomic mass measurements
  • advances in the technology behind mass spectrometers
  • not all about measuring more accurately
  • thorium, the IUPAC decided to recognize an isotope, thorium-230, that it previously thought was too rare to include in atomic weight calculations
  • The last time international chemistry
  • really altered the periodic table was in 2009, when IUPAC decided to list the atomic weights of some elements as ranges, instead of single numbers
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Search for element 113 concluded at last - 0 views

  • do not occur in nature and must be produced through experiments involving nuclear reactors or particle accelerators
  • via processes of nuclear fusion or neutron absorption
  • Elements 93 to 103 were discovered by the Americans, elements 104 to 106 by the Russians and the Americans, elements 107 to 112 by the Germans, and the two most recently named elements, 114 and 116, by cooperative work of the Russians and Americans.
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  • On August 12, those experiments bore fruit: zinc ions travelling at 10% the speed of light collided with a thin bismuth layer to produce a very heavy ion followed by a chain of six consecutive alpha decays identified as products of an isotope of the 113th element
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Japanese Team Claims Discovery Of Elusive Element 113, And May Get To Name It | Popular... - 0 views

  • Japanese researchers claim they’ve seen conclusive evidence of the long-sought element 113, a super-heavy, super-unstable element near the bottom of the periodic table
  • not yet verified by the International Union of Pure and Applied Chemistry
  • if the IUPAC grants its blessing, the researchers could be the first team from Asia to name one of nature’s fundamental atoms.
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  • Super-heavy elements do not occur in nature and have to be discovered in the lab, using particle accelerators, nuclear reactors, ion separators and other complex equipment
  • Science have been hunting for 113 for nine years, and have claimed to see it a few times already — but the evidence has never been this clear,
  • the team used a customized gas-filled recoil ion separator paired with a semiconductor detector that can pick out atomic reaction products
  • created element 113 by speeding zinc ions through a linear accelerator until they reached 10 percent of the speed of light.
  • ions then smashed into a piece of bismuth. When the zinc and bismuth atoms fused, they produced an atom with 113 protons
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ESTCube-1 - Wikipedia, the free encyclopedia - 0 views

  • scheduled to be launched to orbit in second half of 2013
  • Student Satellite is an educational project that university and high school students can participate in
  • The CubeSat standard for nanosatellites was followed during the engineering of ESTCube-1, resulting in a 10x10x11.35 cm cube, with a volume of 1 liter and a mass of 1.048 kg.
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  • According to the CubeSat standard there are three different sized CubeSats corresponding to size 1U, 2U and 3U. Base side lengths are the same but height is 2 to 3 times bigger than 1U CubeSats
  • Mass is also set in CubeSat standard, the highest possible mass for 1U CubeSat is 1300 grams, 2U CubeSat 2600 grams and 3U CubeSat 4000 grams
  • CubeSat base side length must be 100.0±0.1 millimeters and satellite height must be 113.5±0.1 mm
  • the Estonian satellite
  • a 1U CubeSat
  • Although
  • its main purpose was to educate students, the satellite does have a scientific purpose.
  • On board of the satellite is an electric solar wind sail (e-sail) which was created by a Finnish scientist Pekka Janhunen
  • it is the first real experimentation of the e-sail
  • 10 meters of e-sail 50 to 20 micrometers thick wire of high-technology structure so-called Heytether will be deployed from the satellite.
  • The deployment of the Heytether can be detected by decrease of the satellite's speed of rotation or by a on-board camera
  • To control the loaded solar wind sail elements interaction with the plasma surrounding the earth and the effect it has on the spacecraft spinning speed the spacecraft has two on-board nanotechnologic electron emitters/gun
  • The electron emitters are connected to the e-sail element and by shooting out electrons it loads the e-sail element positively to 500 volts
  • The positive ions in the plasma push the e-sail element and have an influence on the satellites rotation speed
  • The effect of the e-sail is measured by the change in rotation speed
  • The camera is used to take a picture of Earth and the successfully deployed Heytether. [edit]
  • ESTCube-1 will be sent to orbit by the European Space Agency's rocket Vega in spring of 2013
  • Start in spring of 2013
  • Half an hour after the satellites deployment from the start capsule satellites antennas will be opened and radio transmitter and important subsystems will be switched on
  • First days or weeks will be used to test the satellite and set it to work on full capacity.
  • Orienting the satellite so the on-board camera will be faced to earth
  • trying to take a picture of Estonia
  • Rotating the satellite on an axis with a speed of 1 revolution per second
  • E-sail element deployment from the satellite by a centrifugal force and confirming the deployment via the on-board camera
  • Activating the electron emitter and loading the e-sail
  • Measuring the e-sails and Lorentz force by satellites revolutions per second
  • If possible using the negatively charged e-sail to take the satellite off orbit and burn it in the earths atmosphere
  • If everything goes perfect the mission can be completed within a few weeks to a month
  • Lifespan of the satellite
  • Measurements and weight
  • Scientific purpose
  • Communicating with the satellite
  • held by two International Amateur Radio Unions three registered frequencies
  • Periodic but very slow communication is done on a telegraphic signal on a frequency of 437.250 MHz
  • the most important satellite parameters are transmitted every 3 to 5 minutes
  • For fast connections FSK-modulation radio signal on a frequency of 437.505 MHz with a 9600 baud connection speed and AX.25 standard is used.
  • Somewhat slow connection speed is caused by the usage of amateur radio frequencies which allow a maximum of 25 kiloherz bandwidth
  • Fast connection is used only when the satellite has been given a specific
  • Using the GFSK-modulation maximum possible connection speed is 19,200 bits per second
  • Software
  • FreeRTOS on the satellite's Command and Data Handling System and camera module
  • TinyOS on the satellite's communication module
  • Financing and costs
  • Cheapest possibility to send a satellite onto orbit is offered by European Space Agency. Because Estonia is an associated member of ESA most of the launch expenses (about 70,000 euros) will be covered from Estonian member fee for educational expenses. With the launch total expenses for the project are approximately 100,000 euros.
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A planetary system from the early Universe - 0 views

  • A group of European astronomers has discovered an ancient planetary system that is likely to be a survivor from one of the earliest cosmic eras, 13 billion years ago. The system consists of the star HIP 11952 and two planets, which have orbital periods of 290 and 7 days, respectively. Whereas planets usually form within clouds that include heavier chemical elements, the star HIP 11952 contains very little other than hydrogen and helium. The system promises to shed light on planet formation in the early universe – under conditions quite different from those of later planetary systems, such as our own
  • widely accepted that planets are formed in disks of gas and dust that swirl around young stars
  • many open questions remain
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  • what it actually takes to make a planet
  • With a sample of, by now, more than 750 confirmed planets
  • astronomers have some idea of the diversity among planetary systems
  • certain trends have emerged
  • Statistically, a star that contains more “metals” - in astronomical parlance, the term includes all chemical elements other than hydrogen and helium – is more likely to have planets.
  • suggests a key question
  • Originally, the universe contained almost no chemical elements other than hydrogen and helium
  • what about planet formation under conditions like those of the very early universe
  • ? If metal-rich stars are more likely to form planets
  • stars with a metal content so low that they cannot form planets at all
  • then when
  • should we expect the very first planets to form
  • a group of astronomers
  • has discovered a planetary system that could help provide answers to those questions
  • part of a survey targeting especially metal-poor stars
  • identified two giant planets around a star known by its catalogue number as HIP 11952
  • at a distance of about 375 light-years from Earth
  • these planets
  • are not unusual
  • What is unusual is the fact that they orbit such an extremely metal-poor and, in particular, such a very old star!
  • planets around such a star should be extremely rare
  • Compared to other exoplanetary systems
  • not only one that is extremely metal-poor
  • at an estimated age of 12.8 billion years, also one of the oldest systems known so far.
  • In 2010 we found the first example of such a metal-poor system, HIP 13044. Back then, we thought it might be a unique case; now, it seems as if there might be more planets around metal-poor stars than expected
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Apollo Moon Rocks Challenge Lunar Water Theory: Scientific American - 0 views

  • The discovery of "significant amounts" of water in moon rock samples collected by NASA's Apollo astronauts is challenging a longstanding theory about how the moon formed
  • Since the Apollo era, scientists have thought the moon came to be after a Mars-size object smashed into Earth early in the planet's history, generating a ring of debris that slowly coalesced over millions of years
  • That process, scientists have said, should have flung away the water-forming element hydrogen into space
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  • a new study suggests the accepted scenario is not possible given the amount of water found in moon rocks collected from the lunar surface in the early 1970s
  • By "water," the researchers don't mean liquid water, but hydroxyl, a chemical that includes the hydrogen and oxygen ingredients of water.
  • Those water-forming elements would have been on the moon all along
  • the impact scenario is the best formation scenario for the moon, but we need to reconcile the theory of hydrogen
  • Past studies have suggested water-forming elements came to the moon from outside sources long after the moon's crust cooled
  • The solar wind — a stream of particles emanating from the sun — as well as meteorites and comets were pegged as possible sources ofwater depositson the moon in recent studies
  • that explanation does not account for the amount of water found in the Apollo samples
  • Because they found hydroxyl deep inside each sampled rock, the scientists say they have eliminated the solar wind moon water explanation
  • those particles can penetrate the surface only slightly
  • An impact from an asteroid or comet could push the hydrogen in further, but it would not be as pristine as the samples the researchers observed, because it would have melted from the heat of the asteroid collision
  • Researchers probed samples from the late Apollo missions, including the famous "Genesis Rock" that was named for its advanced age of 4.5 billion years, about the same time the moon is thought to have formed
  • Using an infrared spectrometer, the researchers found water embedded in the Genesis Rock
  • implies that the various landing sites of Apollo 15, 16 and 17 each had water present
  • Hui's research flies in the face of past analyses of Apollo rocks that found they were very dry, except for a small bit of water attributed to the rock containers leaking when they were returned to Earth
  • Past instruments that analyzed these samples, however, were not very sensitive
  • older spectrometers had a sensitivity of around 50 parts per million (ppm), while his instruments were able to detect water at concentrations of about 6 ppm in anorthosites and 2.7 ppm in troctolites, which are both igneous rocks found in the moon's crust.
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Four white dwarf stars caught in the act of consuming 'earth-like' exoplanets - 0 views

  • astrophysicists have pinpointed four white dwarf stars surrounded by dust from shattered planetary bodies which once bore striking similarities to the composition of the Earth
  • White dwarfs are the final stage of life of stars like our Sun, the residual cores of material left behind after their available fuel for nuclear reactions has been exhausted
  • researchers found that the most frequently occurring elements in the dust around these four white dwarfs were oxygen, magnesium, iron and silicon – the four elements that make up roughly 93 per cent of the Earth.
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  • even more significant observation was that this material also contained an extremely low proportion of carbon, which matched very closely that of the Earth and the other rocky planets orbiting closest to our own Sun
  • first time that such low proportions of carbon have been measured in the atmospheres of white dwarf stars
  • clear evidence that these stars once had at least one rocky exoplanet which they have now destroyed
  • must also pinpoint the last phase of the death of these worlds.
  • atmosphere of a white dwarf is made up of hydrogen and/or helium
  • heavy elements that come into their atmosphere are dragged downwards to their core and out of sight within a matter of days
  • astronomers must literally be observing the final phase of the death of these worlds as the material rains down on the stars at rates of up to 1 million kilograms every second.
  • clear evidence that these stars once had rocky exoplanetary bodies which have now been destroyed
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10 Amazing Things NASA's Huge Mars Rover Can Do | NASA, Mars Science Laboratory & Curio... - 0 views

  • Mast Camera (MastCam)
  • capture high-resolution color pictures and video of the Martian landscape, which scientists will study and laypeople will gawk at
  • Mars Hand Lens Imager (MAHLI)
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  • will function much like a high-powered magnifying glass
  • instrument will take color pictures of features as tiny as 12.5 microns — smaller than the width of a human hair
  • MAHLI sits on the end of Curiosity's five-jointed, 7-foot (2.1-meter) robotic arm
  • Mars Descent Imager (MARDI)
  • small camera located on Curiosity's main body, will record video of the rover's descent to the Martian surface
  • will click on a mile or two above the ground, as soon as Curiosity jettisons its heat shield. The instrument will then take video at five frames per second until the rover touches down. The footage will help the MSL team plan Curiosity's Red Planet rovings, and it should also provide information about the geological context of the landing site, the 100-mile-wide
  • Sample Analysis at Mars (SAM)
  • makes up about half of the rover's science payload.
  • a suite of three separate instruments — a mass spectrometer, a gas chromatograph and a laser spectrometer
  • will search for carbon-containing compounds, the building blocks of life as we know it
  • look for other elements associated with life on Earth, such as hydrogen, oxygen and nitrogen
  • The rover's robotic arm will drop samples into SAM via an inlet on the rover's exterior
  • Chemistry and Mineralogy (CheMin)
  • CheMin will identify different types of minerals on Mars and quantify their abundance
  • will help scientists better understand past environmental conditions on the Red Planet
  • CheMin has an inlet on Curiosity's exterior to accept samples delivered by the rover's robotic arm
  • will shine a fine X-ray beam through the sample, identifying minerals' crystalline structures based on how the X-rays diffract
  • Chemistry and Camera (ChemCam)
  • This instrument will fire a laser at Martian rocks from up to 30 feet (9 meters) away and analyze the composition of the vaporized bits
  • help the mission team determine from afar whether or not they want to send the rover over to investigate a particular landform
  • The laser sits on Curiosity's mast, along with a camera and a small telescope
  • Three spectrographs sit in the rover's body, connected to the mast components by fiber optics
  • spectrographs will analyze the light emitted by excited electrons in the vaporized rock samples
  • Alpha Particle X-Ray Spectrometer (APXS)
  • sits at the end of Curiosity's arm, will measure the abundances of various chemical elements in Martian rocks and dirt
  • APXS will shoot out X-rays and helium nuclei. This barrage will knock electrons in the sample out of their orbits, causing a release of X-rays. Scientists will be able to identify elements based on the characteristic energies of these emitted X-rays
  • Dynamic Albedo of Neutrons (DAN)
  • located near the back of Curiosity's main body, will help the rover search for ice and water-logged minerals beneath the Martian surface
  • The instrument will fire beams of neutrons at the ground, then note the speed at which these particles travel when they bounce back. Hydrogen atoms tend to slow neutrons down, so an abundance of sluggish neutrons would signal underground water or ice
  • should be able to map out water concentrations as low as 0.1 percent at depths up to 6 feet (2 m).
  • Radiation Assessment Detector (RAD)
  • instrument will measure and identify high-energy radiation of all types on the Red Planet, from fast-moving protons to gamma rays
  • designed specifically to help prepare for future human exploration of Mars
  • will allow scientists to determine just how much radiation an astronaut would be exposed to on Mars
  • Rover Environmental Monitoring Station (REMS)
  • partway up Curiosity's mast, is a Martian weather station
  • measure atmospheric pressure, humidity, wind speed and direction, air temperature, ground temperature and ultraviolet radiation.
  • integrated into daily and seasonal reports
  • MSL Entry, Descent and Landing Instrumentation (MEDLI)
  • MEDLI isn't one of Curiosity's 10 instruments
  • will measure the temperatures and pressures the heat shield experiences as the MSL spacecraft streaks through the Martian sky
  • will tell engineers how well the heat shield, and their models of the spacecraft's trajectory, performed
  • data to improve designs for future Mars-bound spacecraft
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Astronomers discover first Thorne-Zytkow object, a bizarre type of hybrid star -- Scien... - 0 views

  • While normal red supergiants derive their energy from nuclear fusion in their cores, TŻOs are powered by the unusual activity of the absorbed neutron stars in their cores
  • Thorne-Żytkow objects (TŻOs) are hybrids of red supergiant and neutron stars that superficially resemble normal red supergiants,
  • They differ, however, in their distinct chemical signatures
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  • TŻOs are thought to be formed by the interaction of two massive stars―a red supergiant and a neutron star formed during a supernova explosion―in a close binary system
  • the most commonly held theory suggests that, during the evolutionary interaction of the two stars
  • the much more massive red supergiant essentially swallows the neutron star, which spirals into the core of the red supergiant
  • Studying these objects
  • represents a completely new model of how stellar interiors can work
  • In these interiors we also have a new way of producing heavy elements in our universe
  • The astronomers
  • examined the spectrum of light emitted from apparent red supergiants, which tells them what elements are present
  • When the spectrum of one
  • star -- HV 2112
  • were quite surprised by some of the unusual features
  • took a close look at the subtle lines in the spectrum they found that it contained excess rubidium, lithium and molybdenum
  • Past research has shown that normal stellar processes can create each of these elements
  • high abundances of all three of these at the temperatures typical of red supergiants is a unique signature of TŻOs
  • careful to point out that HV 2112 displays some chemical characteristics that don't quite match theoretical models
  • There are some minor inconsistencies between some of the details of what we found and what theory predicts
  • But the theoretical predictions are quite old, and there have been a lot of improvements in the theory since then
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Astronomers find sun's 'long-lost brother,' pave way for family reunion -- ScienceDaily - 0 views

  • Astronomers have identified
  • a star that was almost certainly born from the same cloud of gas and dust as our star.
  • The newly developed methods for locating the Sun's 'siblings' will help other astronomers find other "solar siblings," work that could lead to an understanding of how and where our Sun formed, and how our solar system became hospitable for life
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  • team of researcher
  • has identified the first "sibling" of the Sun -- a star that was almost certainly born from the same cloud of gas and dust as our star
  • there is a chance, "small, but not zero," Ramirez said, that these solar sibling stars could host planets that harbor life
  • The solar sibling his team identified is a star called HD 162826, a star 15 percent more massive than the Sun, located 110 light-years away in the constellation Hercules
  • The star is not visible to the unaided eye, but easily can be seen with low-power binoculars, not far from the bright star Vega.
  • The team identified HD 162826 as the Sun's sibling by following up on 30 possible candidates found by several groups around the world looking for solar siblings.
  • All of these observations used high-resolution spectroscopy to get a deep understanding of the stars' chemical make-up.
  • several factors are needed to really pin down a solar sibling
  • . In addition to chemical analysis, his team also included information about the stars' orbits
  • where they had been and where they are going in their paths around the center of the Milky Way galaxy
  • Combining information on both chemical make-up and dynamics of the candidates narrowed the field down to one: HD 162826.
  • By "lucky coincidence,"
  • this star has been studied by the McDonald Observatory Planet Search team
  • for more than 15 years
  • Those studies,
  • together with calculations
  • have ruled out any "hot Jupiters" -- massive planets orbiting close to the star
  • The studies indicate that it's unlikely that a Jupiter analog orbits the star, either, but they do not rule out the presence of smaller terrestrial planets.
  • the project has a larger purpose: to create a road map for how to identify solar siblings
  • "The idea is that the Sun was born in a cluster with a thousand or a hundred thousand stars. This cluster, which formed more than 4.5 billion years ago, has since broken up,"
  • Ivan Ramirez/Tim Jones/McDonald
  • The member stars have broken off into their own orbits around the galactic center, taking them to different parts of the Milky Way today. A few, like HD 162826, are still nearby. Others are much farther
  • even with information on more stars to work with, it's not like "we're going to throw this data into a machine and it's going to spit out the answer,"
  • "You can concentrate on certain key chemical elements that are going to be very useful
  • ." These elements are ones that vary greatly among stars which otherwise have very similar chemical compositions.
  • team has identified the elements barium and yttrium as particularly useful.
  • Once many more solar siblings have been identified, astronomers will be one step closer to knowing where and how the Sun formed.
  • To reach that goal, the dynamics specialists will make models that run the orbits of all known solar siblings backward in time, to find where they intersect: their birthplace.
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Dawn Finds Asteroid Vesta is Rich in Hydrogen - 0 views

  • The giant asteroid Vesta appears to have
  • hydrogen
  • Dawn spacecraft reveals hydrated minerals in a wide area around Vesta’s equator
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  • Dawn did not find actual water ice, there are signs of hydrated minerals such as hydroxyl
  • source of the hydrogen within Vesta’s surface appears to be hydrated minerals delivered by carbon-rich space rocks that collided with Vesta at speeds slow enough to preserve their volatile content
  • pitted terrain – looking much like potholes – mark where the volatiles, perhaps both hydroxyl and water, released from hydrated minerals boiled off
  • Hydroxyl has recently been found on the Moon in permanently shadowed craters at the lunar poles
  • scientists thought there might be a chance that water ice may have
  • around the giant asteroid’s poles
  • unlike Earth’s Moon, however, Vesta has no permanently shadowed polar regions
  • strongest signature for hydrogen actually came from regions near the equator. And there, water ice is not stable
  • The holes that were left as the water escaped stretch as much as 0.6 miles (1 kilometer) across and go down as deep as 700 feet (200 meters
  • collisions converted the hydrogen bound to the minerals into water, which evaporated
  • The pits look just like features seen on Mars, but while water was common on Mars, it was totally unexpected on Vesta in these high abundances
  • ults provide evidence that not only were hydrated materials present, but they played an important role in shaping the asteroid’s geology and the surface we see today
  • the first direct measurements describing the elemental composition of Vesta’s surface
  • elemental investigation by the instrument determined the ratios of iron to oxygen and iron to silicon in the surface materials
  • new findings solidly confirm the connection between Vesta and a class of meteorites found on Earth called the Howardite, Eucrite and Diogenite meteorites
  • have the same ratios for these elements
  • n, more volatile-rich fragments of other objects have been identified in these meteor
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Billion-year-old water could hold clues to life on Earth and Mars - 0 views

  • A UK-Canadian team of scientists has discovered ancient pockets of water, which have been isolated deep underground for billions of years and contain abundant chemicals known to support life
  • This water could be some of the oldest on the planet and may even contain life
  • the similarity between the rocks that trapped it and those on Mars raises the hope that comparable life-sustaining water could lie buried beneath the red planet's surface
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  • Researchers
  • analysed water pouring out of boreholes from a mine 2.4 kilometres beneath Ontario, Canada
  • found that the water is rich in dissolved gases like hydrogen, methane and different forms – called isotopes – of noble gases such as helium, neon, argon and xenon
  • there is as much hydrogen in the water as around hydrothermal vents in the deep ocean, many of which teem with microscopic life
  • The hydrogen and methane come from the interaction between the rock and water, as well as natural radioactive elements in the rock reacting with the water
  • These gases could provide energy for microbes that may not have been exposed to the sun for billions of years.
  • The crystalline rocks surrounding the water are thought to be around 2.7 billion years old. But no-one thought the water could be the same age, until now
  • Using ground-breaking techniques
  • researchers show that the fluid is at least 1.5 billion years old, but could be significantly older.
  • interconnected fluid system in the deep Canadian crystalline basement that is billions of years old, and capable of supporting life
  • Before this finding, the only water of this age was found trapped in tiny bubbles in rock and is incapable of supporting life
  • the water found in the Canadian mine pours from the rock at a rate of nearly two litres per minute
  • don't yet know if the underground system in Canada sustains life
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Weird World! 'Oozing' Alien Planet Is a Super-Earth Wonder | Exoplanets & 55 Cancri e |... - 0 views

  • A new look at an alien planet that orbits extremely close to its parent star suggests that the rocky world might not be a scorching hot wasteland, as was thought
  • The exotic planet 55 Cancri e is a relatively close alien planet, just 40 light-years away from Earth
  • long thought to harbor surface temperatures as high as 4,800 degrees Fahrenheit (about 2,700 degrees Celsius
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  • 55 Cancri e could be a wetter and weirder place than   though
  • 55 Cancri e has a mass 7.8 times that of Earth, and a width just over twice that of our planet
  • observations suggest that about a fifth of the planet's mass must be made up of light elements and compounds, including water
  • experiences such extreme temperatures and high pressure, these elements and compounds likely exist in what is known as a "supercritical" fluid state,
  • Supercritical fluids can best be imagined as liquid-like gases in high pressure and temperature conditions
  • water becomes supercritical in some steam turbines
  • supercritical carbon dioxide is used to scrub caffeine from coffee beans
  • supercritical fluids could be seeping out from the planet's rocks. And, while conditions on the strange world are not suitable to host life, 55 Cancri e does give exoplanet hunters an interesting example to study
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Engineers build 50 gigapixel camera - 0 views

  • resolution is five times better than 20/20 human vision over a 120 degree horizontal field.
  • capture up to 50 gigapixels of data, which is 50,000 megapixels
  • most consumer cameras
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  • ranging from 8 to 40 megapixels
  • researchers believe that within five years
  • gigapixel cameras should be available to the general public
  • Traditionally, one way of making better optics has been to add more glass elements, which increases complexity
  • camera was developed by
  • Duke's Pratt School of Engineering
  • University of Arizona
  • University of California
  • Distant Focus Corp
  • The camera is so large now because of the electronic control boards and the need to add components to keep it from overheating
  • prototype camera itself is two-and-half feet square and 20 inches dee
  • only about three percent of the camera is made of the optical elements
  • arrange for some overlap
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Astronomers find a new type of planet: The 'mega-Earth' - 0 views

  • Astronomers announced
  • that they have discovered a new type of planet - a rocky world weighing 17 times as much as Earth
  • Theorists believed such a world couldn't form because anything so hefty would grab hydrogen gas as it grew and become a Jupiter-like gas giant
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  • This planet, though, is all solids and much bigger than previously discovered "super-Earths," making it a "mega-Earth."
  • Kepler-10c, circles a sunlike star once every 45 days
  • It is located about 560 light-years from Earth in the constellation Draco
  • The system also hosts a 3-Earth-mass "lava world," Kepler-10b, in a remarkably fast, 20-hour orbit
  • Kepler-10c was originally spotted by NASA's Kepler spacecraft.
  • By measuring the amount of dimming, astronomers can calculate the planet's physical size or diameter
  • Kepler can't tell whether a planet is rocky or gassy
  • Kepler-10c was known to have a diameter
  • , 2.3 times as large as Earth
  • This suggested it fell into a category of planets known as mini-Neptunes, which have thick, gaseous envelopes
  • The team used the HARPS-North instrument on the Telescopio Nazionale Galileo (TNG) in the Canary Islands to measure the mass of Kepler-10c
  • They found that it weighed 17 times as much as Earth - far more than expected.
  • This showed that Kepler-10c must have a dense composition of rocks and other solids.
  • Planet formation theories have a difficult time explaining how such a large, rocky world could develop
  • The early universe contained only hydrogen and helium
  • Heavier elements needed to make rocky planets, like silicon and iron, had to be created
  • When those stars exploded
  • scattered
  • through space, which then could
  • later generations of stars and planets
  • This process should have taken billions of years. However, Kepler-10c shows that the universe was able to form such huge rocks even during the time when heavy elements were scarce.
  • tells us that rocky planets could form much earlier than we thought. And if you can make rocks
  • This research implies that astronomers shouldn't rule out old stars when they search for Earth-like planets
  • if old stars can host rocky Earths too, then we have a better chance of locating potentially habitable worlds in our cosmic neighborhood
  • The Kepler-10 system is about 11 billion years old, which means it formed less than 3 billion years after the Big Bang
  • It's massive enough to have held onto
  • its atmosphere
  • if it ever had it
Mars Base

Mars Science Laboratory: Mars Rock Touched By NASA Curiosity Has Surprises - 0 views

  • The first Martian rock NASA's Curiosity rover has reached out to touch presents a more varied composition than expected from previous missions
  • On Earth, rocks with composition like the Jake rock typically come from processes in the planet's mantle beneath the crust, from crystallization of relatively water-rich magma at elevated pressure.
  • elements
Mars Base

Mars Science Laboratory: Curiosity Rover Preparing for Thanksgiving Activities - 0 views

  • drove for the first time after spending several weeks in soil-scooping activities at one location
  • On Friday, Nov. 16, the rover drove 6.2 feet (1.9 meters) to get within arm's reach of a rock called "Rocknest 3."
  • touched that rock with the Alpha Particle X-Ray Spectrometer (APXS) on its arm, and took two 10-minute APXS readings of data about the chemical elements in the rock
  • ...8 more annotations...
  • Then Curiosity stowed its arm and drove 83 feet (25.3 meters) eastward toward a target called "Point Lake
  • this is
  • first 'touch-and-go' on the same day
  • good sign that the rover team is getting comfortable with more complex operational planning
  • During a Thanksgiving break, the team will use Curiosity's Mast Camera (Mastcam) from Point Lake to examine possible routes and targets to the east
  • priority is to choose a rock for the first use of the rover's hammering drill, which will collect samples of powder from rock interiors
  • the sample-handling mechanism on the rover's arm is still holding some soil from the fifth and final scoop collected at Rocknest
  • so it can be available for analysis by instruments within the rover if scientists choose that option in coming days.
Mars Base

Russia finds 'new bacteria' in Antarctic lake - 0 views

  • Russian scientists believe they have found a wholly new type of bacteria in the mysterious subglacial Lake Vostok in Antarctica
  • The samples obtained from the underground lake in May 2012 contained a bacteria which bore no resemblance to existing type
  • "After putting aside all possible elements of contamination, DNA was found that did not coincide with any of the well-known types in the global database,"
  • ...13 more annotations...
  • discovery comes from samples collected in an expedition in 2012 where a Russian team drilled down to the surface of Lake Vosto
  • believed to have been covered by ice for more than a million years but has kept its liquid state.
  • Lake Vostok is the largest subglacial lake in Antarctica
  • The Russian team last year drilled almost four kilometres (2.34 miles) to reach the lake and take the samples.
  • t the interest surrounded one particular form of bacteria whose DNA was less than 86 percent similar to previously existing forms.
  • "In terms of work with DNA this is basically zero. A level of 90 percent usually means that the organism is unknown."
  • not even possible to find the genetic descendants of the bacteria.
  • "If this had been found on Mars everyone would have undoubtedly said there is life on Mars. But this is bacteria from Earth."
  • new samples of water would be taken from Lake Vostok during a new expedition in May.
  • "If we manage to find the same group of organisms in this water we can say for sure that we have found new life on Earth that exists in no database,"
  • Exploring environments such as Lake Vostok allows scientists to discover what life forms can exist in the most extreme conditions
  • whether life could exist on some other bodies in the solar system.
  • Saturn's moon Enceladus and the Jupiter moon Europa as they are believed to have oceans, or large lakes, beneath their icy shells.
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