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    VIRGOCosmos In Brief - Aktualní novinky vesmírného výzkumu v kostce
    VIRGO
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    Pulsar Candidate in Andromeda

    NASA's Nuclear Spectroscope Telescope Array, or NuSTAR, has identified a candidate pulsar in Andromeda - the nearest large galaxy to the Milky Way.
    This likely pulsar is brighter at high energies than the Andromeda galaxy's entire black hole population. The inset image shows the pulsar candidate
    in blue, as seen in X-ray light by NuSTAR. The background image of Andromeda was taken by NASA's Galaxy Evolution Explorer in ultraviolet light.

    Andromeda is a spiral galaxy like our Milky Way but larger in size. It lies 2.5 million light-years away in the Andromeda constellation.

    Image credit: NASA/JPL-Caltech/GSFC/JHU

    VIRGO
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    ALMA Reveals Turbulent Birth of Twin Baby Stars
    http://www.almaobservatory.org/...ress-releases/1190-alma-reveals-turbulent-birth-of-twin-baby-stars

    Using the Atacama Large Millimeter/submillimeter Array (ALMA), researchers obtained a critical clue to an underlying problem:
    how are widely separated twin stars formed? The team found very low mass newborn twin stars with misaligned rotation axes.
    This misalignment indicates that they were formed in a pair of fragmented gas clouds produced through turbulence, not via
    evolution of tightly-coupled twin. This finding strongly supports the turbulent fragmentation theory of binary star formation
    down to the substellar regime.

    An international team of astronomers led by Jeong-Eun Lee in Kyung Hee University, Korea, observed the baby twin star system
    IRAS 04191+1523 with ALMA. Thanks to the high resolution of ALMA, the team successfully imaged the rotation of the gas disks
    around the very low mass twin stars and found that the rotation axes of the two stars are misaligned.

    VIRGO
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    VIRGO
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    New faint dwarf galaxy discovered
    https://phys.org/news/2017-07-faint-dwarf-galaxy.html

    Astronomers have detected a new faint dwarf spheroidal galaxy using Japan's Subaru Telescope located in Hawaii. The newly found dwarf, designated d1005+68,
    belongs to a nearby galaxy group known as the M81 Group. The new findings were presented June 22 in a paper published on the arXiv pre-print repository.

    VIRGO
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    Large sample of giant radio galaxies discovered | OUPblog
    https://blog.oup.com/2017/07/giant-radio-galaxies-discovered/

    Recently a team of astronomers from India have reported discovery of a large number of extremely rare kind of galaxies called “giant radio galaxies” (GRGs),
    using a nearly 20 year old radio survey. GRGs are the largest galaxies known in the Universe, which are visible only to radio telescopes. These extremely active
    form of galaxies harbor a super massive black hole ‘central-engine’ at the nucleus, which ejects a pair of high energy particle jets nearly at the speed of light,
    which terminate into two giant radio lobes. These behemoths span nearly three million light years across, or even more sometimes. This size corresponds to stacking
    nearly 33 Milky Way like galaxies in a line!

    VIRGO
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    Under pressure - extreme atmosphere stripping may limit exoplanets’ habitability
    http://www.ras.org.uk/...der-pressure-extreme-atmosphere-stripping-may-limit-exoplanets-habitability

    New models of massive stellar eruptions hint at an extra layer of complexity when considering whether an exoplanet may be habitable or not.
    Models developed for our own Sun have now been applied to cool stars favoured by exoplanet hunters, in research presented by Dr Christina Kay,
    of the NASA Goddard Flight Center, on Monday 3rd July at the National Astronomy Meeting at the University of Hull.

    Coronal mass ejections (CMEs) are huge explosions of plasma and magnetic field that routinely erupt from the Sun and other stars. They are
    a fundamental factor in so called “space weather”, and are already known to potentially disrupt satellites and other electronic equipment on Earth.
    However, scientists have shown that the effects of space weather may also have a significant impact on the potential habitability of planets around
    cool, low mass stars - a popular target in the search for Earth-like exoplanets.
    VIRGO
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    ALICE detector upgrades enter production phase | ALICE Matters
    http://alicematters.web.cern.ch/?q=content%2Fnode%2F1029

    While the extended end-of-year shutdown has concluded and the LHC has been switched on again, the activities for the upgrade of the ALICE detector
    have entered a new phase. The prototypes of the various new components have been tested and validated, so that now production can start.

    This major upgrade will increase the performance of the detector in order to fully exploit the higher interaction rate of about 50 kHz that is expected
    in Run 3 of LHC, after the two-year long shut down (LS2) that will start at the end of 2018.

    VIRGO
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    Zítra je Asteroid day! To zase bude nestíhačka...
    XCHAOS
    XCHAOS --- ---
    An Algorithm Helps Protect Mars Curiosity's Wheels | NASA
    https://www.nasa.gov/feature/jpl/an-algorithm-helps-protect-mars-curiositys-wheels/
    VIRGO
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    This image taken with ALMA and Hubble Space Telescope captures the “Hubble Ultra Deep Field,” the farthest reaches of space. The purple regions are the galaxies
    (collections of stars) captured by the Hubble Space Telescope. And, the orange areas are the distribution of carbon monoxide gas, which is material for stars, taken
    with ALMA. Comparing these two data sets, astronomers will tackle the big mystery of how fast the galaxies in the Universe generated stars about 10 billion years ago.

    Looking into the Depths of the Universe with Two Telescopes | NAOJ: National Astronomical Observatory of Japan - English
    http://www.nao.ac.jp/en/gallery/weekly/2017/20170627-alma.html

    VIRGO
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    Huge Storms Disrupted Jupiter’s Fastest Jet Stream in 2016 - Eos
    https://eos.org/research-spotlights/huge-storms-disrupted-jupiters-fastest-jet-stream-in-2016

    Recurrent jet stream disturbances provide glimpses of what lies beneath the gas giant’s thick upper cloud cover.

    VIRGO
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    Rocky planets are probably a whole lot more common in our galaxy than astronomers previously believed—according to the latest release
    of Kepler Space Telescope data last week—a scenario that enhances the prospects for extraterrestrial life in nearby solar systems.

    Kepler Has Taught Us That Rocky Planets Are Common - Astrobiology Magazine
    http://www.astrobio.net/news-exclusive/kepler-taught-us-rocky-planets-common/

    VIRGO
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    This montage of views from NASA's Cassini spacecraft shows three of Saturn's small ring moons: Atlas, Daphnis and Pan at the same scale for ease of comparison.
    Two differences between Atlas and Pan are obvious in this montage. Pan's equatorial band is much thinner and more sharply defined, and the central mass of Atlas
    (the part underneath the smooth equatorial band) appears to be smaller than that of Pan.

    https://www.nasa.gov/image-feature/jpl/pia21449/small-wonders

    VIRGO
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    The rise of LIGO’s space-studying super-team | symmetry magazine
    http://www.symmetrymagazine.org/article/the-rise-of-ligos-space-studying-super-team

    Scientists including astronomers working with the Fermi Large Area Telescope have recorded brief bursts of high-energy photons
    called gamma rays coming from distant reaches of space. They suspect such eruptions result from the merging of two neutron stars—
    the collapsed cores of dying stars—or from the collision of a neutron star and a black hole.

    But gamma rays alone can’t tell them that. The story of the dense, crashing cores would be more convincing if astronomers saw
    a second signal coming from the same event—for example, the release of ripples in space-time called gravitational waves.

    “The Fermi Large Area Telescope detects a few short gamma ray bursts per year already, but detecting one in correspondence to
    a gravitational-wave event would be the first direct confirmation of this scenario,” says postdoctoral researcher Giacomo Vianello
    of the Kavli Institute for Particle Astrophysics and Cosmology, a joint institution of SLAC National Accelerator Laboratory and
    Stanford University.

    Scientists discovered gravitational waves in 2015 (announced in 2016). Using the Laser Interferometer Gravitational-Wave Observatory,
    or LIGO, they detected the coalescence of two massive black holes.

    LIGO scientists are now sharing their data with a network of fellow space watchers to see if any of their signals match up. Combining
    multiple signals to create a more complete picture of astronomical events is called multi-messenger astronomy.​
    VIRGO
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    Planet Nine Is Put on Trial in Absentia | Quanta Magazine
    https://www.quantamagazine.org/planet-nine-is-put-on-trial-in-absentia-20170627/

    Breathless media coverage notwithstanding, the cases for and against a hypothetical Planet Nine in the outskirts of the solar system remain inconclusive.
    VIRGO
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    A map that fills a 500-million year gap in Earth's history
    https://theconversation.com/a-map-that-fills-a-500-million-year-gap-in-earths-history-79838

    Earth is estimated to be around 4.5 billion years old, with life first appearing around 3 billion years ago.

    To unravel this incredible history, scientists use a range of different techniques to determine when and where continents moved,
    how life evolved, how climate changed over time, when our oceans rose and fell, and how land was shaped. Tectonic plates – the huge,
    constantly moving slabs of rock that make up the outermost layer of the Earth, the crust – are central to all these studies.

    Along with our colleagues, we have published the first whole-Earth plate tectonic map of half a billion years of Earth history,
    from 1,000 million years ago to 520 million years ago.

    A map that fills a 500-million year gap in Earth's history
    https://www.youtube.com/watch?v=77NKvC4nkvY
    VIRGO
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    VIRGO:

    The mystique of Barnard's Star | Astronomy Essentials | EarthSky
    http://earthsky.org/astronomy-essentials/barnards-star-closest-stars-famous-stars

    Although very common, red dwarfs like Barnard’s Star are typically dim. Thus they are notoriously faint and hard to study. In fact, not a single red dwarf
    can be seen with the unaided human eye. But because Barnard’s Star is relatively close and bright, it has become a go-to model for all things red dwarf.

    At nearly six light-years’ distance, Barnard’s Star is often cited as the second-closest star to our sun (and Earth). This is true only if you consider
    the triple star system Alpha Centauri as one star.

    Proxima Centauri, the smallest and faintest of Alpha Centauri’s three components, is the closest known star to the sun at just 4.24 light years away.
    It, too, is a red dwarf. So Barnard’s Star is only the second-closest red dwarf star. It is perhaps more important for astronomical purposes, though,
    because Proxima is four times fainter and thus harder to study.

    VIRGO
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    Syfy - Bad Astronomy | The planets, like grains of sand
    http://www.syfy.com/syfywire/the-planets-like-grains-of-sand

    Statistically speaking, for every planet Kepler finds, there are a million more in the galaxy waiting to be discovered.
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