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    VIRGOCosmos In Brief - Aktualní novinky vesmírného výzkumu v kostce
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    NASA : The 2017 Total Solar Eclipse
    https://www.youtube.com/watch?v=2VaTYQvB6so


    Multimedia | NOAA NESDIS
    https://www.nesdis.noaa.gov/content/multimedia

    Follow the Moon's Shadow across the Northern Hemisphere
    https://www.youtube.com/watch?time_continue=1&v=uZMvd-WZH1A
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    Za pár minut:

    NASA TV Public-Education
    https://www.youtube.com/watch?v=wwMDvPCGeE0
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    Join Cassini's end of mission celebration with CSIRO | Cosmos
    https://cosmosmagazine.com/society/join-cassini-s-end-of-mission-celebration-with-csiro

    CSIRO is giving 30 social media superstars the opportunity to celebrate the end
    of Cassini's 20 year mission with the team at Canberra Deep Space Complex.
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    Could the total solar eclipse reveal a comet? | The Planetary Society
    http://www.planetary.org/blogs/guest-blogs/2017/20170816-solar-eclipse-comet.html

    We're less than a week away from one of the most talked-about astronomical events in many years - the "Great" North American solar eclipse! The Internet
    abounds with articles that discuss how eclipses work, give you a map of the path of totality for this eclipse, and even tell you about some of the planets
    you might see during the eclipse. This is all fantastically exciting, but there's one more possibility that would put the cherry on the eclipse cake...

    Now, be forewarned: the odds are heavily stacked against us, and the level of skill required for any individual to pull this off might range from "little"
    to "legendary." But with that in mind, there does exist a chance—a slim chance—that we could see a comet next to the Sun during the eclipse!

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    Closer look at red supergiant Antares suggests convection not enough to remove surface material
    https://phys.org/news/2017-08-closer-red-supergiant-antares-convection.html

    A trio of researchers with Universidad Católica del Norte and the Max-Planck-Institut für Radioastronomie has found evidence that suggests
    that convection alone cannot account for the amount of material that is pulled from the surface of a red supergiant. In their paper published
    in the journal Nature, K. Ohnaka, G. Weigelt and K.-H. Hofmann describe their study of the supergiant Antares, what they found and why they
    now believe there is an unknown force pulling some parts of the star's surface into space. Gail Schaefer with Georgia State University offers
    a News & Views piece on the work done by the team in the same journal issue.

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    Tuning Up RV: A Test Case at Tau Ceti
    https://www.centauri-dreams.org/?p=38293

    The new work on Tau Ceti, which analyzes radial velocity data showing four planets there,
    looks to be a step forward in this workhouse method for planetary detection. With radial velocity,
    we’re analyzing tiny variations in the movement of a star as it is affected by the planets around it.
    These are tiny signals, and the new Tau Ceti paper discusses working with variations as low as 30
    centimeters per second. It’s a good number, but we’ll want better — to detect a true Earth analog
    around a Sun-like star, we need to get this number into the 10 cm/s range.

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    UTA astrophysicists predict Earth-like planet may exist in star system only 16 light years away - UTA News Center
    http://www.uta.edu/news/releases/2017/08/New%20planet%20Suman%20Satyal.php

    Astrophysicists at the University of Texas at Arlington have predicted that an Earth-like planet may be lurking in a star system just 16 light years away.

    The team investigated the star system Gliese 832 for additional exoplanets residing between the two currently known alien worlds in this system. Their
    computations revealed that an additional Earth-like planet with a dynamically stable configuration may be residing at a distance ranging from 0.25 to 2.0
    astronomical unit (AU) from the star.

    “According to our calculations, this hypothetical alien world would probably have a mass between 1 to 15 Earth's masses,” said the lead author Suman Satyal,
    UTA physics researcher, lecturer and laboratory supervisor. The paper is co-authored by John Griffith, UTA undergraduate student and long-time UTA physics
    professor Zdzislaw Musielak.

    The astrophysicists published their findings this week as “Dynamics of a probable Earth-Like Planet in the GJ 832 System” in The Astrophysical Journal.

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    Woow! Dva dni před koncem CRF kampaně mají přes 80% financí!

    Laser SETI: First Ever All-Sky All-the-Time Search | Indiegogo
    https://www.indiegogo.com/projects/laser-seti-first-ever-all-sky-all-the-time-search-science#/

    LaserSETI
    https://vimeo.com/229780383
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    Eclipse – Crossroads in the sky
    https://www.youtube.com/watch?v=B50qwsy3JyM
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    Superhmotná černá díra požírá kosmickou medúzu | ESO Česko
    http://www.eso.org/public/czechrepublic/news/eso1725/?lang

    Přístroj MUSE pro dalekohled ESO/VLT objevil nový způsob zásobování černých děr hmotou

    Pozorování takzvaných 'medúzovitých galaxií' pomocí dalekohledu ESO/VLT odhalila dosud neznámý způsob, jakým superhmotné černé díry získávají hmotu.
    Zdá se, že mechanismus vzniku struktur tvořených plynem i hvězdami a připomínajících chapadla medúzy, které daly těmto objektům jméno, rovněž umožňuje,
    aby se plyn dostal až do centrální oblasti galaxie, stal se kořistí černé díry a jasně se rozzářil. Výsledky byly publikovány ve vědeckém časopise Nature.

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    Can Radio Telescopes Find Axions?
    http://aasnova.org/2017/08/16/can-radio-telescopes-find-axions/

    In the search for dark matter, the most commonly accepted candidates are invisible, massive particles commonly referred to as WIMPs. But as time
    passes and we still haven’t detected WIMPs, alternative scenarios are becoming more and more appealing. Prime among these is the idea of axions.

    Axions are a type of particle first proposed in the late 1970s. These theorized particles arose from a new symmetry introduced to solve ongoing
    problems with the standard model for particle physics, and they were initially predicted to have more than a keV in mass. For this reason, their
    existence was expected to be quickly confirmed by particle-detector experiments — yet no detections were made.

    Today, after many unsuccessful searches, experiments and theory tell us that if axions exist, their masses must lie between 10-6–10-3 eV. This is
    minuscule — an electron’s mass is around 500,000 eV, and even neutrinos are on the scale of a tenth of an eV!

    But enough of anything, even something very low-mass, can weigh a lot. If they are real, then axions were likely created in abundance during the
    Big Bang — and unlike heavier particles, they can’t decay into anything lighter, so we would expect them all to still be around today. Our universe
    could therefore be filled with invisible axions, potentially providing an explanation for dark matter in the form of many, many tiny particles.

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    Cassini: The Grand Finale: Nine Ways Cassini Matters: No. 6
    https://saturn.jpl.nasa.gov/news/3089/nine-ways-cassini-matters-no-6/

    There is a diffuse ring that is created out of the bits of water ice jetted out by the moon Enceladus (the E ring).
    There are rings that were created because of the material thrown off when meteorites hit moons (such as the G ring
    and the two rings discovered by Cassini in images from 2006—the Janus-Epimetheus ring and the Pallene ring). There
    are rings controlled by interactions with moons, like the F ring, which is regularly perturbed by Prometheus, and
    the narrow ringlets that share the Encke Gap with Pan.

    In addition to the rings’ origins, Cassini’s close-up examination has also revealed propeller-shaped features that
    mark the locations of hidden moonlets. The processes involved in the formation of such objects are thought to be
    similar to how planets form in disks around young stars.

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    Gaia's first full-colour all-sky map
    ESA Science & Technology: Sneak peek of Gaia's sky in colour
    http://sci.esa.int/gaia/59404-sneak-peek-of-gaias-sky-in-colour/

    While surveying the positions of over a billion stars, ESA's Gaia mission is also measuring their colour,
    a key diagnostic to study the physical properties of stars. A new image provides a preview of Gaia's first
    full-colour all-sky map, which will be unleashed in its highest resolution with the next data release in 2018.

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    A comparison of Arecibo Observatory radar images of Venus from 1988 and 2012. Via Ed Rivera-Valentín.

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    Experiments cast doubt on how the Earth was formed | EurekAlert! Science News
    https://www.eurekalert.org/pub_releases/2017-08/gc-ecd081117.php

    New geochemical research indicates that existing theories of the formation of the Earth may be mistaken. The results of experiments to show how zinc
    (Zn) relates to sulphur (S) under the conditions present at the time of the formation of the Earth more than 4 billion years ago, indicate that there
    is a substantial quantity of Zn in the Earth's core, whereas previously there had been thought to be none. This implies that the building blocks of
    the Earth must be different to what has been supposed. The work is presented at the Goldschmidt geochemistry conference in Paris.

    The researchers, from the Institut de Physique du Globe de Paris (IPGP) melted mixtures of iron-rich metal and silicate compounds, containing Zn and S,
    at high temperatures and pressures up to 80 GPa and 4100K* to experimentally simulate core-mantle differentiation at the time of the Earth's formation.
    They then measured how these elements were distributed (partitioned) between the core and mantle of their experiments. When they fed their results into
    computer models of the Earth's formation, they found that none of the canonical models can sufficiently reproduce the S/Zn ratio of the present-day mantle.
    This means that the current estimates of the Earth's composition, including its core, need to be modified, and therefore the way the core and mantle
    - i.e. the Earth - formed may also need to be revised.
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    TRAPPIST-1 is no longer the exoplanet dream we once hoped | Alphr
    http://www.alphr.com/space/1006622/trappist-1-is-no-longer-the-exoplanet-dream-we-once-hoped

    TRAPPIST-1, the star system 39 light years away that could hold the potential for Earth-like planets to exist, may not be all that great after all. Initial
    reports suggested that this nearby system could hold up to seven possibly habitable planets but new findings suggest TRAPPIST-1 is too old to sustain life.

    Researchers originally believed the TRAPPIST-1 system was around 500 million years old due to its compact nature. Now though, it’s believed that the TRAPPIST-1
    star is actually between 5.4 and 9.8 billion years old. This makes the TRAPPIST-1 system over twice as old as our Solar System – which was formed around 4.5
    billion years ago.

    "Our results really help constrain the evolution of the TRAPPIST-1 system, because the system has to have persisted for billions of years. This means the planets
    had to evolve together, otherwise, the system would have fallen apart long ago," said Adam Burgasser, an astronomer at the University of California who worked on
    the research paper.

    Because TRAPPIST-1 is now a lot older than previously thought, researchers have begun to question if it really is the holy grail of new planets that it was once
    thought to be. The TRAPPIST-1 star may be more stable than other dwarf stars, meaning that being closer to it isn’t as dangerous as first thought, but because
    of its age, it’s likely that the close-orbiting planets have been completely irradiated by long exposure to the star.

    PIA21430
    https://www.youtube.com/watch?v=_HfgHhMg6vY
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    (úterý 15/08)

    On this day in 1977: A Big Ear radio radio telescope received a narrowband 72-sec radio signal from space. Its origin is still unknown.



    CEO Bill Diamond with scientists Seth Shostak and Gerry Harp about the 40th anniversary of Wow! signal.
    https://www.facebook.com/SETIInstitute/videos/10155469445160535/

    Due to technical difficulties the LIVE was interrupted, for watching 2nd part, use this link:
    https://www.facebook.com/SETIInstitute/videos/10155469479165535/
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    The Air out There: Astronomers Aim to Find Atmospheres of Alien Earths - Scientific American
    https://www.scientificamerican.com/...out-there-astronomers-aim-to-find-atmospheres-of-alien-earths/

    Is our nearest neighboring exoplanet, Proxima b, an "Earth next door," or is it a lifeless rock?

    Remotely sniffing the air of these tantalizing worlds is no easy task, and is unlikely to occur sooner than the end of this decade, if not well into the next.
    The first observations could be made by NASA’s infrared James Webb Space Telescope, launching in 2018, followed in the mid-2020s by a new generation of ground-
    based “Extremely Large Telescopes” with 30-meter mirrors. However, the payoff could be immense: In a forthcoming paper submitted to The Astrophysical Journal,
    the Harvard-Smithsonian Center for Astrophysics astronomer Caroline Morley and colleagues conclude that with a total investment of as little as a week of
    observing time Webb could conceivably deliver statistically significant detections of Earth-like atmospheric conditions upon a handful of small planets transiting
    nearby red dwarf stars. Or, of course, Webb could find instead that those worlds are airless rocks. Whether such investments will happen at all is far from certain:
    With a nominal lifetime of only five years and astronomers worldwide clamoring to use it, the telescope is destined to become the most oversubscribed and in-demand
    scientific instrument humans have ever built.

    In the meantime some researchers are focusing on ways to use Webb to simply detect an atmosphere—or rule one out—upon the closest potentially life-friendly red-dwarf
    world. Find that Proxima b has managed to keep an appreciable atmosphere in spite of the barrage of physical insults from its stellar host, and you have taken a big
    step toward showing the universe is filled with biologically promising red-dwarf worlds. Finding it has no atmosphere could, by contrast, bolster the case that red
    dwarfs are by and large dead-ends in the search for alien life.

    “It may sound arrogant, but using Webb to prove that Proxima b has an atmosphere would be one of the biggest scientific achievements it could make,” says Ignas
    Snellen, an astronomer at the University of Leiden. “If Webb does that, I think the project would have to be considered a success, no matter what else it does.”

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    Cosmology Results from The Dark Energy Survey! | astrobites
    https://astrobites.org/2017/08/14/cosmology-results-from-the-dark-energy-survey/

    The Dark Energy Survey (DES) is a 5-year long endeavor meant to map astrophysical objects over 1/8th of the total night sky visible from Earth (5000 square degrees!),
    making it one of the largest all-sky surveys ever undertaken from the Earth. DES, which has been in operation since 2013 and is being considered the natural successor
    to the Sloan Digital Sky Survey (SDSS), uses the 4m Blanco Telescope at the Cerro Tololo Inter-American Observatory (CTIO) in Chile for its observations.

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    The Cosmic Velocity Web
    http://www.ifa.hawaii.edu/info/press-releases/velocity_web/

    The cosmic web - the distribution of matter on the largest scales in the universe - has usually been defined through the distribution of galaxies.
    Now, a new study by a team of astronomers from France, Israel, and Hawaii demonstrates a novel approach. Instead of using galaxy positions, they
    mapped the motions of thousands of galaxies. Because galaxies are pulled toward gravitational attractors and move away from empty regions, these
    motions allowed the team to locate the denser matter in clusters and filaments and the absence of matter in regions called voids.

    Matter was distributed almost homogeneously in the very early universe, with only miniscule variations in density. Over the 14 billion year history
    of the universe, gravity has been acting to pull matter together in some places and leave other places more and more empty. Today, the matter forms
    a network of knots and connecting filaments referred to as the cosmic web. Most of this matter is in a mysterious form, the so-called "dark matter".
    Galaxies have formed at the highest concentrations of matter and act as lighthouses illuminating the underlying cosmic structure.

    The newly defined cosmic velocity web defines the structure of the universe from velocity information alone. In those regions with abundant observations,
    the structure of the velocity web and the web inferred from the locations of the galaxy lighthouses are similar. This agreement provides strong confirmation
    of the fundamental idea that structure developed from the growth of initially tiny fluctuations through gravitational attraction.

    The cosmic velocity web analysis was led by Daniel Pomarede, Atomic Energy Center, France, with the collaboration of Helene Courtois at the University
    of Lyon, France; Yehuda Hoffman at the Hebrew University, Israel; and Brent Tully at the University of Hawai'i Institute for Astronomy.

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