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    VIRGOCosmos In Brief - Aktualní novinky vesmírného výzkumu v kostce
    VIRGO
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    The Humans to Mars Summit 2017 Is Live Now!
    The George Washington University, Washington D.C.
    https://h2m.exploremars.org/

    Rec: https://livestream.com/viewnow/HumansToMars2017
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    Methane-munching microbes living in the deep biosphere for 400 million years: An analogue for extra-terrestrial life | Science Bulletin
    http://sciencebulletin.org/archives/12895.html

    In numerous cracks down to depths of 1700 meter that have been partly sealed by crystals grown in them, an international team of researchers
    led by Dr. Henrik Drake from Linnaeus University, Sweden, has traced fundamental ancient microbial processes, including production and consumption
    of the greenhouse gas methane. The multi-disciplinary approach included micro-scale measurement of stable isotopes coupled with geochronology within
    minerals formed in response to microbial activity at several Swedish granitic rock sites. This is the most extensive study on ancient microbial
    activity in the continental crust yet and the findings suggest that microbial methane formation and consumption are widespread in the bedrock.
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    Waves of lava seen in Io’s largest volcanic crater | Berkeley News
    http://news.berkeley.edu/2017/05/10/waves-of-lava-seen-in-ios-largest-volcanic-crater/

    Taking advantage of a rare orbital alignment between two of Jupiter’s moons, Io and Europa, researchers have obtained
    an exceptionally detailed map of the largest lava lake on Io, the most volcanically active body in the solar system.

    Loki Patera is about 200 kilometers across. The hot region of the patera has a surface area of 21 500 square kilometers,
    larger than Lake Ontario.

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    Cruise stage of Mars 2020 Rover under construction at NASA JPL.

    VIRGO
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    Asteroid 2014 JO25 Gets Some Sweet Radar Love | Lights in the Dark
    https://lightsinthedark.com/2017/05/10/asteroid-2014-jo25-gets-some-sweet-radar-love/

    This is our best look yet at asteroid 2014 JO25, which made its closest pass by Earth for at least the next 500 years on April 19, 2017. The animation
    is composed of radar observations made from NASA’s Goldstone facility in California when the asteroid was between 1.53 and 1.61 million miles away.

    VIRGO
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    http://newsroom.unsw.edu.au/...ldest-evidence-life-land-found-348-billion-year-old-australian-rocks

    Fossils discovered by UNSW scientists in ancient hot spring deposits in the Pilbara have pushed back by 580 million years
    the earliest known evidence for microbial life on land.

    Fossils discovered by UNSW scientists in 3.48 billion year old hot spring deposits in the Pilbara region of Western Australia
    have pushed back by 580 million years the earliest known existence of microbial life on land.

    Previously, the world’s oldest evidence for microbial life on land came from 2.7- 2.9 billion-year-old deposits in South Africa
    containing organic matter-rich ancient soils.

    ---

    Australian Fossils Hint At Where To Search For Life On Mars : The Two-Way : NPR
    http://www.npr.org/...17/05/09/527575457/australian-fossils-hint-at-where-to-search-for-life-on-mars

    It could also suggest where to look in the search for life on Mars.

    NASA is currently considering where to land the rover on its 2020 Mars Exploration Mission, and one of the sites is
    a "hot spring-type setting," about the same age as the early Earth, Djokic says.

    "If you're going to look for life on Mars, we know it was preserved on hot springs here on the ancient earth," she says.
    "So there's a good chance if it ever developed on Mars, then it would probably be preserved in hot springs there, too."

    Djokic and her colleagues participated in a February NASA workshop that narrowed down the landing-site candidates to three
    from eight, including the hot springs-like site.

    Studies on ancient fossils are often controversial, and this one is no exception. MIT's Tanja Bosak, who specializes in
    signatures of microbial processes in ancient sedimentary rocks, tells NPR that she is thinks more evidence is needed to prove
    the bubbles were formed through biological stabilization. She says relating the results to Mars "is taking this a step too far."

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    TRAPPIST-1 Planets Have No Large Moons, Study Argues - Seeker
    https://www.seeker.com/space/planets/trappist-1-planets-have-no-large-moons-study-argues

    The conditions for habitable exoplanets in the TRAPPIST-1 system might depend on the presence of large moons — and Earth reveals clues to why.

    A new study looks at the possibilities of large moons in TRAPPIST-1, a notoriously crowded exoplanet system that may have habitable planets within it.
    Earlier this year, observations from NASA's Spitzer Space Telescope indicated that seven planets here could be rocky and have liquid water on their
    surfaces, making TRAPPIST-1 the system with the most potentially habitable planets.

    But even before NASA's discovery, TRAPPIST-1 was known and pondered by scientists, including the author of the new paper, Stephen Kane, an associate
    professor of astronomy at San Francisco State University who specializes in exoplanets.

    "I have several publications now on exomoons, and for many years I've been thinking about how the ability of a planet to host a moon scales with
    the presence of nearby planets and proximity to the host star," Kane said in an e-mail. "The discovery of the TRAPPIST-1 system prompted me to finally
    calculate whether or not planets in compact planetary systems can actually harbor moons."

    For TRAPPIST-1, Kane found that the planets are so tightly packed together that large moons would likely be impossible. While the rotational axes of
    the planets would quickly change and have more chaotic climates, he said, life could still evolve — it just might take a longer time.

    Kane's methodology involved studying the influences of two parameters: the Hill radius, or the area in space in which a planet exerts gravitational
    influence based on its mass and distance from the host star, and the Roche limit, which identifies where the gravitational effect near a planet is
    too strong for a moon to survive.

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    2 asteroids recently discovered will have a near-Earth flyby tomorrow

    Asteroid 2017 JX1 was first observed at Mt. Lemmon Survey on 2017-05-04. Flyby May 11 at 02:47 UT. Dist: 3.71 LD. Size: 12-39 m.
    IAU Minor Planet Center
    http://www.minorplanetcenter.net/db_search/show_object?object_id=2017%20JX1

    Asteroid 2017 HU49 was first observed at Mt. Lemmon Survey on 2017-04-30. Flyby May 11 at 21:42 UT. Dist: 5.55 LD. Size: 10-33 m.
    IAU Minor Planet Center
    http://www.minorplanetcenter.net/db_search/show_object?object_id=2017%20HU49

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    Current NEO statistics/Highlights of April
    NEOs News - April |
    http://www.neoshield.eu/neos-news-april-2017/

    VIRGO
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    New Radar Images of Asteroid 2014 JO25
    https://www.youtube.com/watch?v=7mLVEgwFH-U


    This movie of asteroid 2014 JO25 was generated using radar data collected by NASA's
    70-meter wide Deep Space Network antenna at Goldstone, California on April 19, 2017.
    VIRGO
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    Two bright fireballs captured over São Paulo, Brazil on May 6 and May 8, 2017

    https://www.youtube.com/watch?v=zK8F1JJKuYo
    VIRGO
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    Two James Webb instruments are best suited for exoplanet atmospheres | Penn State University
    http://news.psu.edu/...0/2017/05/09/two-james-webb-instruments-are-best-suited-exoplanet-atmospheres

    Batalha and Michael Line, assistant professor, School of Earth and Space Science, Arizona State University, developed a mathematical model
    to predict the quantity of information that different Webb instruments could extract about an exoplanet's atmosphere.

    Their model predicts that using a combination of two infrared instruments — the Near Infrared Imager and Slitless Spectrograph (NIRISS) and
    the G395 mode on the Near Infrared Spectrograph (NIRSpec) — will provide the highest information content about an exoplanet's atmosphere.

    NIRISS is a versatile camera and spectrograph that will observe infrared wavelengths similar to those the Hubble Telescope covers. NIRISS,
    according to Batalha and Line, should be combined with the G395 mode on NIRSpec, which will observe targets in longer infrared wavelengths
    at Webb's highest resolution.

    VIRGO
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    Cassini: The Grand Finale: Cloud Bands Streak Across Titan
    https://saturn.jpl.nasa.gov/resources/7673/

    NASA's Cassini spacecraft captured this view of bands of bright, feathery methane clouds drifting across Saturn's moon Titan on May 7, 2017.

    The view was obtained during a distant (non-targeted) flyby, during which Cassini passed 488 000 kilometers above the moon's surface. Although
    Cassini will have no further close, targeted flybys of Titan, the spacecraft continues to observe the giant moon and its atmosphere from a distance.

    The dark regions at top are Titan's hydrocarbon lakes and seas.

    The image was taken on May 7, 2017, at a distance of 508 000 kilometers. The view is an orthographic projection centered on 57 degrees north latitude,
    48 degrees west longitude. An orthographic view is most like the view seen by a distant observer. Image scale is about 3 kilometers per pixel.

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    Beyond the stars Green Bank telescopes search for signs of life - West Virginia Press Association : West Virginia Press Association
    http://wvpress.org/breaking-news/beyond-stars-green-bank-telescopes-search-signs-life/

    The GBT, completed in 2000, is taller than the Statue of Liberty, the Great Pyramids of Giza and just smaller than the Washington Monument.
    The surface area of the dish itself is 2.3 acres. The entire telescope is on wheels — 16 to be exact — and weighs almost 17 million pounds.

    That makes it the heaviest wheel and track system in the world. And unlike the other telescopes, the dish of the GBT moves. In fact, it always moves.

    “It can move 360 degrees all the way around,” Holstine said. “But we generally only move it 270 degrees because in the center of this is a cable wrap,
    but it can see the whole sky.” The part of the dish that doesn’t move side-to-side moves up and down, going from 95 degrees all the way to 4 degrees.

    “It can see 85 percent of the celestial sphere,” Holstine said. “Almost everything there is to see in the universe.”

    https://www.wired.com/2009/10/gbt-nrao-tour/



    VIRGO
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    The Scientific Truth About Planet Nine, So Far
    https://www.forbes.com/...rtswithabang/2017/05/09/the-scientific-truth-about-planet-nine-so-far/amp/

    ...The full suite of data allows us to place better restrictions on where we think Planet Nine ought to be, and the most likely scenarios place it somewhere
    in the constellation of Taurus. As we approach the June solstice, that constellation becomes more visible, meaning that the coming months will be the best time
    for potential Planet Nine-hunters, both amateur and professional, to get to work. Mike Brown is also keeping a blog, himself, about the current status of
    the efforts to find Planet Nine; despite his wild optimism about the scenario, his reporting thus far is accurate and not overhyped.

    VIRGO
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    https://www.scientificamerican.com/article/scientists-push-to-orbit-pluto/
    After New Horizons’ 2015 encounter with the dwarf planet, researchers are hoping to go back—to stay

    Fusion-Enabled Pluto Orbiter and Lander - Princeton Satellite Systems, Inc.
    https://www.youtube.com/watch?v=IlydFJtWeXg
    VIRGO
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    News | NASA Delivers Detectors for ESA's Euclid Spacecraft
    https://www.jpl.nasa.gov/news/news.php?feature=6840

    Three detector systems for the Euclid mission, led by ESA (European Space Agency), have been delivered to Europe for the spacecraft's near-infrared instrument.
    The detector systems are key components of NASA's contribution to this upcoming mission to study some of the biggest questions about the universe, including
    those related to the properties and effects of dark matter and dark energy -- two critical, but invisible phenomena that scientists think make up the vast
    majority of our universe.

    VIRGO
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    News | Merging Galaxies Have Enshrouded Black Holes
    https://www.jpl.nasa.gov/news/news.php?feature=6841

    Black holes get a bad rap in popular culture for swallowing everything in their environments. In reality, stars,
    gas and dust can orbit black holes for long periods of time, until a major disruption pushes the material in.

    A merger of two galaxies is one such disruption. As the galaxies combine and their central black holes approach
    each other, gas and dust in the vicinity are pushed onto their respective black holes. An enormous amount of high-
    energy radiation is released as material spirals rapidly toward the hungry black hole, which becomes what
    astronomers call an active galactic nucleus (AGN).

    A study using NASA's NuSTAR telescope shows that in the late stages of galaxy mergers, so much gas and dust falls
    toward a black hole that the extremely bright AGN is enshrouded. The combined effect of the gravity of the two
    galaxies slows the rotational speeds of gas and dust that would otherwise be orbiting freely. This loss of energy
    makes the material fall onto the black hole.

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    Surprise! When a brown dwarf is actually a planetary mass object | Carnegie Institution for Science
    https://carnegiescience.edu/news/surprise-when-brown-dwarf-actually-planetary-mass-object

    Sometimes a brown dwarf is actually a planet—or planet-like anyway. A team led by Carnegie’s Jonathan Gagné,
    and including researchers from the Institute for Research on Exoplanets (iREx) at Université de Montréal,
    the American Museum of Natural History, and University of California San Diego, discovered that what astronomers
    had previously thought was one of the closest brown dwarfs to our own Sun is in fact a planetary mass object.
    Their results are published by The Astrophysical Journal Letters.

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