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    VIRGOCosmos In Brief - Aktualní novinky vesmírného výzkumu v kostce
    VIRGO
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    NASA’S First Asteroid Deflection Mission Enters Next Design Phase
    https://www.nasa.gov/feature/nasa-s-first-asteroid-deflection-mission-enters-next-design-phase

    The first-ever mission to demonstrate an asteroid deflection technique for planetary defense -- the Double Asteroid Redirection
    Test (DART) -- is moving from concept development to preliminary design phase, following NASA’s approval on June 23.

    Dart Moon Collision
    https://www.youtube.com/watch?v=8zooPRmgUPI
    VIRGO
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    Hidden red dwarf discovered in dust of giant star | University of Hertfordshire
    http://www.herts.ac.uk/about-us/news/2017/july/hidden-red-dwarf-discovered-in-dust-of-giant-star

    Observations of the brightest star in the infrared sky by a team of astronomers, including researchers
    from the University of Hertfordshire, have revealed that the dust surrounding it hides a small red dwarf star.

    CW Leonis, a red giant star 500 times the size of the Sun is located in the Leo constellation 300 light years away.
    This is an evolving star that is ejecting significant amounts of dust forming an enveloping cloud many times the size
    of our solar system. It has been the subject of hundreds of studies over the years, but only now has the existence
    of a smaller red dwarf star been found within the dust cloud.

    From 1994 to 2000, using a one meter telescope at the Observatory of Torino, Professor Richard Smart at the University
    of Hertfordshire observed a minute wobble in the motion of CW Leonis that defied explanation. This wobble was very small -
    equivalent to the side of a 10p coin on the Moon as seen from the Earth - but it was detectable.

    A recent study of the dust around CW Leonis revealed a swirl pattern that was hypothesised to be due to the presence of
    an unseen companion star. Introducing the companion resolved the 17-year-old mystery of the wobble. The research has
    been accepted for publication in Monthly Notices of the Royal Astronomical Society (MNRAS).
    VIRGO
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    MACH in VR: 7 Big Questions About The Cosmos
    https://www.youtube.com/watch?v=uujewwFiS-s


    Why Are Distant Galaxies Aligned?
    https://www.youtube.com/watch?v=TbeJUcABezw
    VIRGO
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    Střechu kůlny prorazil meteorit starý 4,5 miliardy let – Novinky.cz
    https://www.novinky.cz/...a-skoly/442548-strechu-kulny-prorazil-meteorit-stary-4-5-miliardy-let.html
    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.​
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