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    VIRGOCosmos In Brief - Aktualní novinky vesmírného výzkumu v kostce
    VIRGO
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    Weekly Space Hangout - Jan 27, 2017: Kimberly Cartier & Exoplanet WASP 103b
    https://www.youtube.com/watch?v=j_3_BJ0uAzc
    VIRGO
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    Asteroid 2017 BH 30 (průměr ~ 7-10 m) proletí v pondělí ráno kolem 04:51 UT asi 40 000 km od Země (0.17 LD)
    Nejbližší průlet kolem Měsíce (~ 280 000 km) v pondělí +/- 09:21 UT



    Objeven dnes díky prohlídce Catalina Sky Survey 29/01/17).
    IAU Minor Planet Center
    http://www.minorplanetcenter.net/db_search/show_object?object_id=2017+BH30

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    Water Underground | How did our planet get its water?
    http://blogs.egu.eu/network/water-underground/2017/01/26/how-did-our-planet-get-its-water/

    Planet Earth makes its own water from scratch deep in the mantle | New Scientist
    https://www.newscientist.com/...75-planet-earth-makes-its-own-water-from-scratch-deep-in-the-mantle/
    VIRGO
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    Latest SETI Talks - Exocomets: Now you see them, now you don't - Barry Welsh, UC Berkeley
    Exocomets: Now you see them, now you don't - Barry Welsh(SETI Talks 2017)
    https://www.youtube.com/watch?v=FsCRNq0lGts


    Present technology does not enable us to view images of these kilometer-sized infalling bodies, but the evaporation of gaseous products
    liberated from exocomets that occurs close to a star can potentially cause small disruptions in the ambient circumstellar disk plasma.
    For circumstellar disks that are viewed “edge-on” this evaporating material may be directly observed through transient (night-to-night
    and hour-to-hour) gas absorption features seen at rapidly changing velocities. Using high resolution spectrographs mounted to large
    aperture ground-based telescopes, we have discovered 15 young stars that harbor swarms of exocomets. In this lecture we briefly describe
    the physical attributes of comets in our own solar system and the instrumental observing techniques to detect the presence of evaporating
    exocomets present around stars with ages in the 10 – 100 Myr range. We note that this work has particular relevance to the dramatic
    fluctuations in the flux recorded towards “Tabby’s star” by the NASA Kepler Mission, that may be explained through the piling up of
    swarms of exocomets in front of the central star.
    OMNIHASH
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    VIRGO: škoda, že je to superzemě s minimální dobou oběhu a pravděpodobně s vázanou rotací na slunce.
    VIRGO
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    Tohle světlo a barvy snad uvidíme příští rok na Velké výpravě... :)



    VIRGO
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    Does anyone know the context of this picture?...



    :)))
    VIRGO
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    https://www.newscientist.com/round-up/ligodetection/

    To celebrate the one-year anniversary of a discovery that changed the face of astronomy,
    on 7 February we feature the exclusive world premiere of a new documentary.

    LIGO Detection trailer
    https://www.youtube.com/watch?v=1xX4x3WyXRo
    VIRGO
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    VIRGO: A ještě jedno video s komentářem, protože téma si to zaslouží.
    It's Faster! Flickering Quasars Used To Measure Universe Expansion
    https://www.youtube.com/watch?v=ql5I48S29gA
    VIRGO
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    VIRGO
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    NEBULA
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    VIRGO: to je nádhera! :)
    VIRGO
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    ATNF Daily Astronomy Picture
    http://www.atnf.csiro.au/ATNF-DailyImage/archive/2017/24-Jan-2017.html
    Resolved magnetic structures in the disk-halo interface of NGC 628
    by George Heald (CASS)

    Spiral galaxies host large-scale magnetic fields that evolve over millions of years via turbulence in the Interstellar Medium and the rotation of the galaxy itself.
    These galactic-sized magnetic fields contain an ordered component, primarily located in the regions between the spiral arms, where randomness imposed by the star
    formation process is low. Such ordered magnetic fields and their directionality can be efficiently observed with cm-wavelength radio synchrotron radiation, and its
    degree of linear polarisation. The above picture shows an optical image of the face-on spiral galaxy NGC628 as observed with the Calar Alto 1.23-m telescope in Spain,
    superimposed with flow lines showing the direction of the ordered large-scale magnetic field as observed with the Jansky Very Large Array (JVLA) at radio frequencies
    between 2-4 GHz. The image is presented as part of new work by a team including George Heald (CASS) that was recently accepted for publication. The research also
    found evidence for two drivers of magnetic turbulence in the disk-halo region of NGC 628, namely, Parker instabilities and superbubbles.

    VIRGO
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    Clingy Alien Planets May Fling Their Moons Out of Orbit
    http://www.space.com/35460-clingy-alien-planets-may-lose-moons.html

    Alien planets that orbit especially close to their stars have a bigger chance of losing their moons, which may reduce
    the chances that habitable alien moons will survive for very long around those planets, a new study finds.

    In the past 20 years or so, astronomers have confirmed the existence of more than 3,400 worlds outside Earth's solar system.
    These discoveries have revealed that many exoplanets are very different from those seen in Earth's solar system; for instance,
    about 40 percent of exoplanets discovered to date orbit their stars at least 10 times closer than Earth orbits the sun.
    (In comparison, Mercury is at most about three times closer than Earth is to the sun.)

    In Earth's solar system, there are far more moons than planets, with Jupiter alone having at least 67 moons. Previous work has
    suggested that exomoons, or moons around exoplanets, could be as big or larger than Earth. If an exoplanet happens to lie in
    a star's habitable zone — the area in which worlds have surface temperatures warm enough to host liquid water — then an Earth-
    size exomoon around such a planet could potentially harbor life.
    VIRGO
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    Objective: To deflect asteroids, thus preventing their collision with Earth | EurekAlert! Science News
    https://www.eurekalert.org/pub_releases/2017-01/snrc-otd012517.php

    An international project, led by Spain's National Research Council, (CSIC) provides information on the effects a projectile impact would have on an asteroid.
    The aim of the project is to work out how an asteroid might be deflected so as not to collide with the Earth. The research, published in The Astrophysical Journal,
    focuses on the study of the asteroid Chelyabinsk, which exploded over Russian skies in 2013 after passing through the atmosphere.

    The probability that a kilometre-sized asteroid could have devastating consequences after impact with the Earth is statistically small. What is more frequent,
    and repeatedly discovered, is that objects a few tens of meters across reach the Earth's atmosphere.

    The results of this study indicate that the composition, internal structure, density and other physical properties of the asteroid are "fundamental in
    determining the success of a mission in which a kinetic projectile would be launched to deflect the orbit of a dangerous asteroid."
    VIRGO
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    https://www.paulanthonywilson.com/...phere-transit-of-the-directly-imaged-exoplanet-beta-pictoris-b/

    This summer will be the first time that we’ll be able to observe the Hill sphere of a directly imaged exoplanet as it passes in
    front of its host star! The exoplanet, Beta Pictoris b, is a young (~20 million years old) planet orbiting the star beta Pictoris.

    As chance would have it, we see the orbit of beta Pic b (the exoplanet) nearly edge-on from Earth. This means that as beta Pic b
    moves along its orbit it will come very close to transiting the host star. Although the planet itself won’t pass exactly in front
    of it’s host star, the Hill sphere of beta Pic b will.

    During this event, any material in the Hill sphere (e.g. left-over debris from planet formation, rings, gas torus around satellites,
    etc.) could be detectable. This summer, my colleagues and I will monitor this transit event using the HST in the far-UV.

    This will be the first time that a Hill sphere of a directly imaged planet will be observed in the far-UV.
    The next such transit will not happen again for another 20 years!


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    Earth’s water must have arrived here earlier than we thought | New Scientist
    https://www.newscientist.com/...2118993-earths-water-must-have-arrived-here-earlier-than-we-thought/

    The arrival of water on our planet wasn’t a last-minute job.

    Water came to Earth on icy comets after most of the planet and its core were formed, about 4.5 billion years ago,
    according to a leading theory.

    But now an analysis of isotopes from meteorites born earlier, when the solar system was formed, seems to imply
    that the wet stuff got here much sooner. To pin down when meteorites could have delivered Earth’s water, Mario
    Fisher-Gödde and Thorsten Kleine at the University of Münster, Germany, looked at the Tagish Lake meteorites that
    fell in British Columbia, Canada, in January 2000. They compared the abundance of ruthenium isotopes in these
    meteorites with the abundance in Earth’s mantle.

    “Meteorites impacted Earth during formation and they can leave signatures,” says Katherine Bermingham, at
    the University of Maryland. “Ruthenium isotopes are stable. That means they can act as fingerprints.”

    VIRGO
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    Isotopic similarities seen in materials that formed Earth, moon | UChicago News
    https://news.uchicago.edu/article/2017/01/25/isotopic-similarities-seen-materials-formed-earth-moon

    Where did the materials that make up the Earth and moon come from—and when did they arrive?

    Most scientific models contend the Earth formed gradually by addition from an assortment of moon-
    to Mars-sized masses that had a vast array of isotopic characteristics. New research published Jan. 26
    in Nature maintains the Earth, as well as the moon and certain meteorites, were formed from materials
    that were more similar, holding almost indistinguishable isotopic characteristics.

    VIRGO
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    WOOW!

    Scientists have detected a habitable zone in one of our nearest solar systems - ScienceAlert
    http://www.sciencealert.com/we-just-found-a-habitable-zone-on-an-exoplanet-14-light-years-away

    An exoplanet with the prime conditions for life could be located just 14 light-years away, scientists report,
    in one of the closest neighbouring solar systems to our own.

    New research suggests that a planet circling the star Wolf 1061 falls within what's called the star's habitable zone -
    making it one of the most likely neighbouring candidates for a planet that supports life.

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