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    VIRGOCosmos In Brief - Aktualní novinky vesmírného výzkumu v kostce
    VIRGO
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    Lawrence Krauss reads from The Greatest Story Ever Told...So Far
    https://www.youtube.com/watch?v=a4tB4QbVVmE
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    Rise of the Super Telescopes: The Overwhelmingly Large Telescope - Universe Today
    http://www.universetoday.com/...800/rise-of-the-super-telescopes-the-overwhelmingly-large-telescope/

    Adaptive Optics Discoveries
    https://www.youtube.com/watch?v=F6hmLcJOkzM
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    Sols 1623-1624: MAHLI Diagnostics & Remote Sensing: Curiosity Mission Update by Lauren Edgar
    http://www.flickr.com/photos/105796482@N04/32321734204/sizes/l

    Today’s two-sol plan is devoted to MAHLI diagnostics and remote sensing. It’s another late slide sol, so planning started three and half hours later than usual.
    The plan kicks off with arm activities to better understand the fault that MAHLI experienced last week. Then ChemCam will investigate “Dunn Brook,” a target that
    is just above “Chase Brook” from the weekend plan, and is shown in the above Mastcam image. The target shows some interesting color variations so ChemCam will be
    used to investigate changes in composition. We’ll also acquire a ChemCam observation of “Leighton,” to study the coarse sand grains at the crest of a ripple. Then
    Navcam will look for dust devils and clouds, in response to orbital observations that suggest recent increasing atmospheric opacity. On the second sol, Mastcam
    will acquire a multispectral observation on “Dunn Brook,” and will be used to document the previous APXS locations at “Tomhegan” and “Waweig.” We’ll also acquire
    a Mastcam image for deck monitoring to assess the movement of fines, and an upper tier Navcam mosaic to enable us to target features on Mt. Sharp. The second sol
    includes a number of environmental monitoring observations, using both Mastcam and Navcam to monitor the color and opacity of the atmosphere and search for dust
    devils. The plan also includes an APXS thermal characterization test and a number of change detection observations.

    By Lauren Edgar: Lauren is a Research Geologist at the USGS Astrogeology Science Center and a member of the MSL science team.

    VIRGO
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    Bright fireball spotted over Santos, São Paulo, Brazil on February 28, 2017
    Fireball 28/02/2017 - Santos/SP
    https://www.youtube.com/watch?v=PRTRVUMoY2Y
    VIRGO
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    Recent Claims Invalid: Emergent Gravity Might Deliver A Universe Without Dark Matter
    https://www.forbes.com/.../02/28/is-dark-matter-about-to-be-killed-by-emergent-gravity/#2018cc775359

    Gravity is one of the four fundamental forces of nature, which means it’s not derived from anything else – it just is. At least,
    that's according to our presently accepted theories. But this may be about to change.

    Physicists today describe the gravitational interaction through Einstein’s Theory of General Relativity, which dictates the effects of gravity are due to the curvature of space-time.
    But it's already been 20 years since Ted Jacobson demonstrated that General Relativity resembles thermodynamics, which is a framework to describe how very large numbers of individual,
    constituent particles behave. Since then, physicists have tried to figure out whether this similarity is a formal coincidence or hints at a deeper truth: that space-time is made of
    small elements whose collective motion gives rise to the force we call gravity. In this case, gravity would not be a truly fundamental phenomenon, but an emergent one.

    The problem is, if emergent gravity just reproduces General Relativity, there’s no way to test the idea. What we need instead is a prediction from emergent gravity that deviates from
    General Relativity.

    Such a prediction was made two months ago by Erik Verlinde in his new paper. Verlinde pointed out that emergent gravity in a universe with a positive cosmological constant – like the
    one we live in – would only approximately reproduce General Relativity. The microscopic constituents of space-time, Verlinde claims, also react to the presence of matter in a way that
    General Relativity does not capture: they push inwards on matter. This creates an effect similar to that ascribed to particle dark matter, which pulls normal matter in by its
    gravitational attraction.

    Verlinde’s idea is interesting and solves two problems that had plagued previous attempts at emergent gravity.

    First, he conjectures that the deviations from General Relativity come about because the microscopic constituents of space-time have an additional type of entropy. In the thermodynamic
    formulation of gravity, the entropy – that is the number of possible microscopic configurations – which a volume can maximally have is proportional to the surface area of that volume.
    This is also often referred to as a “holographic” entropy because it demonstrates that all what happens inside the volume can entirely be encoded on its surface. The additional entropy
    that Verlinde introduces instead grows with the volume itself.

    The modification to General Relativity then comes about because matter – so the conjecture goes – reduces the new, volume-scaling entropy in its environment. The entropy decrease leads
    to a decrease in volume which, in turn creates a force pushing inwards on the matter. This force, Verlinde shows, is similar to the force normally attributed to dark matter – which pulls
    in normal matter from its additional gravitational mass.
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    https://www.nasa.gov/feature/goddard/2017/study-hints-at-change-in-water-fingerprint-of-comet

    Astronomers from NASA’s Goddard Space Flight Center in Greenbelt, Maryland, observed the Oort cloud comet C/2014 Q2, also called Lovejoy,
    when it passed near Earth in early 2015. Through NASA’s partnership in the W. M. Keck Observatory on Mauna Kea, Hawaii, the team observed
    the comet at infrared wavelengths a few days after Lovejoy passed its perihelion – or closest point to the sun.

    VIRGO
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    Spontaneous “dust traps”: astronomers discover a missing link in planet formation
    http://www.ras.org.uk/...ntaneous-dust-traps-astronomers-discover-a-missing-link-in-planet-formation

    Planets are thought to form in the disks of dust and gas found around young stars. But astronomers have struggled to assemble
    a complete theory of their origin that explains how the initial dust develops into planetary systems. A French-UK-Australian
    team now think they have the answer, with their simulations showing the formation of 'dust traps' where pebble-sized fragments
    collect and stick together, to grow into the building blocks of planets. They publish their results in the journal Monthly
    Notices of the Royal Astronomical Society.

    VIRGO
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    Constraining the Chemistry of Carbon-Chain Molecules in Spacesu201708 | www.cfa.harvard.edu/
    https://www.cfa.harvard.edu/news/su201708

    The interstellar medium of the Milky Way contains 5-10% of the total mass of the galaxy (excluding its dark matter) and consists primarily of hydrogen gas. There are small
    but important contributions from other gases as well, including carbon-bearing molecules both simple, like carbon monoxide and carbon dioxide, and complex like ethene,
    benzene, propynal, methanol and other alcohols, and cyanides. There are even some very large molecules like polycyclic aromatic hydrocarbons and buckyballs with fifty or
    more carbon atoms. Some species like the cyanides have relative abundances similar to what is seen in comets in our Solar System, suggesting that local carbon chemistry
    is not unique.

    Astronomers think complex interstellar molecules are probably produced on dust grains, although some molecules might be produced in the gas phase. About one percent by mass
    of the interstellar material, these tiny grains are composed predominantly of silicates and provide the gas molecules with surfaces on which to react with other molecules.
    Carbon chain molecules are particularly interesting because they are thought to be the starting point for a significant fraction of the known complex chemicals in
    the interstellar medium. It is even suspected that carbon-chain species are a key stage in the formation of polycyclic aromatic hydrocarbons. Carbon-chain molecular
    chemistry thus provides insight into a large subset of interstellar chemistry.

    VIRGO
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    A remarkable galactic hybrid | ESA/Hubble
    https://www.spacetelescope.org/images/potw1709a/

    This NASA/ESA Hubble Space Telescope image showcases the remarkable galaxy UGC 12591. Classified as an S0/Sa galaxy, UGC 12591 sits somewhere
    between a lenticular and a spiral. It lies just under 400 million light-years away from us in the westernmost region of the Pisces–Perseus
    Supercluster, a long chain of galaxy clusters that stretches out for hundreds of light-years — one of the largest known structures in the cosmos.

    VIRGO
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    A New Binary Star Asteroid Belt Teaches Us About How Planets Form
    https://www.forbes.com/...-binary-star-asteroid-belt-teaches-us-about-how-planets-form/#6e9615d64d6d

    The system is called SDSS 1557. It consists of a white dwarf about the mass of our Sun, orbited by a large brown dwarf
    about 60 times more massive than Jupiter. Recently astronomers have observed a rocky asteroid belt surrounding the system.

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    Science checkout continues for ExoMars orbiter / ExoMars / Space Science / Our Activities / ESA
    http://www.esa.int/...ctivities/Space_Science/ExoMars/Science_checkout_continues_for_ExoMars_orbiter

    Next week, the ExoMars orbiter will devote two days to making important calibration measurements
    at the Red Planet, which are needed for the science phase of the mission that will begin next year.

    VIRGO
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    Long fireball north north west of hawley, Tx 2-26-17 8:55 pm
    https://www.youtube.com/watch?v=B6Fy8KEgEVA
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    https://www.nasa.gov/feature/goddard/2017/first-solar-images-from-noaas-goes-16-satellite

    The first images from the Solar Ultraviolet Imager or SUVI instrument aboard NOAA’s GOES-16 satellite
    have been successful, capturing a large coronal hole on Jan. 29, 2017.

    First Solar Imagery from GOES-16
    https://www.youtube.com/watch?v=Xa0vI4kwx9k
    VIRGO
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    Space in Images - 2017 - 02 - The evolution of SN 1987A
    http://www.esa.int/spaceinimages/Images/2017/02/The_evolution_of_SN_1987A

    VIRGO
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    First ultra-compact dwarf galaxy in the group NGC 5044 found
    https://phys.org/news/2017-02-ultra-compact-dwarf-galaxy-group-ngc.html

    A team of astronomers led by Favio Faifer of the National University of La Plata, Argentina, has discovered the first ultra-compact dwarf (UCD) galaxy
    in an X-ray bright galaxy group designated NGC 5044. The finding was presented Feb. 21 in a paper published online on the arXiv pre-print repository.

    Located some 116 million light years away, NGC 5044 is an early-type massive elliptical galaxy residing at the center of an X-ray bright group also named
    NGC 5044. This group contains about 150 members, most of which are dwarf galaxies. Although the group's center galaxy has been the subject of several past
    studies, its globular cluster and UCD system remain unexplored.

    UCDs are very compact galaxies with high stellar populations, containing about 100 million stars. They display masses, colors, and metallicities between
    those of globular clusters and early-type dwarf galaxies. These ultra-compact stellar systems could provide important insights on the formation and evolution
    of galaxies in the universe.

    That is why Faifer's team observed the NGC 5044 with the Gemini Multi-Object Spectrograph (GMOS) at the Gemini South telescope in Chile. They obtained deep
    images of several fields around NGC 5044, which allowed them to detect the presence of a UCD.

    "From the photometric and spectroscopic analysis of a deep field taken with Gemini+GMOS, we have been able to detect and confirm the first UCD in the NGC 5044
    group," the researchers wrote in the paper.

    The radial velocity and angular proximity (2.83 arcmin) of this UCD indicate that this object is associated with galaxy NGC 5044. The newly discovered UCD
    was designated NGC 5044-UCD1.

    The researchers found that the metallicity of NGC 5044-UCD1 is within the range displayed by other UCD detected in constellations Virgo and Fornax, but
    considerably lower than that of the confirmed stripped nuclei described in previous studies. They also studied the star formation history of this UCD and
    found that this object is approximately 11.7 billion years old.

    VIRGO
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    Scientists reach back in time to discover some of the most power-packed galaxies | Clemson University News and Stories, South Carolina
    http://newsstand.clemson.edu/...ach-back-in-time-to-discover-some-of-the-most-power-packed-galaxies/

    When the universe was young, a supermassive black hole — bloated to the bursting point with stupendous power — heaved out a jet of particle-infused energy
    that raced through the vastness of space at nearly the speed of light. Billions of years later, a trio of Clemson University scientists, led by College of Science
    astrophysicist Marco Ajello, has identified this black hole and four others similar to it that range in age from 1.4 billion to 1.9 billion years old. These objects
    emit copious gamma rays, light of the highest energy, that are billions of times more energetic than light that is visible to the human eye.

    The previously known earliest gamma-ray blazars — a type of galaxy whose intense emission is powered by extremely powerful relativistic jets launched by monstrous
    black holes — were more than 2 billion years old. Currently, the universe is estimated to be approximately 14 billion years old.
    VIRGO
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    First evidence of rocky planet formation in Tatooine system
    http://www.ucl.ac.uk/...cles/0217/270217-First-evidence-of-rocky-planet-formation-in-Tatooine-system

    Published today in Nature Astronomy and funded by the Science and Technology Facilities Council and the European Research Council,
    the study reports on the remains of shattered asteroids orbiting a double sun consisting of a white dwarf and a brown dwarf roughly
    1000 light-years away in a system called SDSS 1557.

    The discovery is remarkable because the debris appears to be rocky and suggests that terrestrial planets like Tatooine – Luke Skywalker’s
    home world in Star Wars – might exist in the system. To date, all exoplanets discovered in orbit around double stars are gas giants,
    similar to Jupiter, and are thought to form in the icy regions of their systems.

    In contrast to the carbon-rich icy material found in other double star systems, the planetary material identified in the SDSS 1557 system
    has a high metal content, including silicon and magnesium. These elements were identified as the debris flowed from its orbit onto the surface
    of the star, polluting it temporarily with at least 1017 g (or 1.1 trillion US tons) of matter, equating it to an asteroid at least 4 km in size.
    VIRGO
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    A Challenge to Our View of How Stars Die
    http://aasnova.org/2017/02/27/a-challenge-to-our-view-of-how-stars-die/

    For the first time ever, we’ve been able to watch the complete metamorphosis of an unusual explosion from one type of
    supernova to another. What do our observations of SN 2014C mean for our understanding of how massive stars end their lives?

    Categorizing Explosions

    Supernovae — the explosions that mark the end of massive stellar lifetimes — are broadly categorized into two types: Type I
    supernovae, which do not show evidence of hydrogen in their spectra, and Type II supernovae, which do.

    The majority of supernovae in both categories have the same cause: the fuel in the star’s core is exhausted, and the core
    subsequently collapses under its own gravity. But a supernova will appear as a Type I or Type II depending upon whether
    or not the star had already lost its outer hydrogen envelope long before the explosion.

    VIRGO
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    Study suggests we reclassify the moon as a planet – reopening a centuries-old debate
    https://theconversation.com/...eclassify-the-moon-as-a-planet-reopening-a-centuries-old-debate-73575

    Every now and then a scientific paper makes a real splash. We had one recently, to judge from recent headlines. “Moon rises to claim
    its place as a planet” said The Sunday Times on February 19, while the Mail Online asked “Is this lunarcy?”. The articles were among
    many responding to the humble paper: “A Geophysical Planet Definition”, which suggested that the criteria for determining what constitutes
    a planet need an overhaul. It argued that the moon, Pluto and several other bodies in the solar system should be upgraded to planets.

    The paper, published in Planetary and Lunar Science, was written by a team including Alan Stern. Stern is famous for NASA’s New Horizons mission,
    which made its spectacular flyby of Pluto in July 2015. The paper is a bit technical, but it basically argues that the geophysics of a body
    should determine whether it is a planet – not just whether it orbits the sun.

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