• úvod
  • témata
  • události
  • tržiště
  • diskuze
  • nástěnka
  • přihlásit
    registrace
    ztracené heslo?
    VIRGOCosmos In Brief - Aktualní novinky vesmírného výzkumu v kostce
    VIRGO
    VIRGO --- ---
    http://www.ifa.hawaii.edu/info/press-releases/robo_ao2/

    The University of Hawaiʻi's 2.2 meter (88-inch) telescope on Maunakea will soon be producing images nearly as sharp
    as those from the Hubble Space Telescope, thanks to a new instrument using the latest image sharpening technologies.
    Astronomer Christoph Baranec, at the University of Hawaiʻi's Institute for Astronomy (IfA), has been awarded a nearly
    $1 million grant from the National Science Foundation to build an autonomous adaptive optics system called Robo-AO-2
    for the UH telescope.

    VIRGO
    VIRGO --- ---
    Astrobiology: Hunting aliens : Nature : Nature Research
    http://www.nature.com/nature/journal/v546/n7660/full/546596a.html

    Ramin Skibba enjoys a profile of the woman heading the search for life off Earth.

    VIRGO
    VIRGO --- ---
    Institute for Astronomy celebrates 50 years of discovery : University of Hawaiʻi System News
    http://www.hawaii.edu/news/2017/06/29/institute-for-astronomy-celebrates-50-years/

    Institute for Astronomy celebrates 50 years of discovery
    https://www.youtube.com/watch?v=bGyBofPm84E
    VIRGO
    VIRGO --- ---
    https://www.nasa.gov/image-feature/jpl/pia21335/zoom-in-on-epimetheus

    This zoomed-in view of Epimetheus, one of the highest resolution ever taken, shows a surface covered in craters, vivid reminders of the hazards of space.

    Epimetheus (70 miles or 113 kilometers across) is too small for its gravity to hold onto an atmosphere. It is also too small to be geologically active.
    There is therefore no way to erase the scars from meteor impacts, except for the generation of new impact craters on top of old ones. This view looks toward
    anti-Saturn side of Epimetheus. North on Epimetheus is up and rotated 32 degrees to the right. The image was taken with the Cassini spacecraft narrow-angle
    camera on Feb. 21, 2017 using a spectral filter which preferentially admits wavelengths of near-infrared light centered at 939 nanometers. The view was acquired at
    a distance of approximately 15 000 kilometers from Epimetheus and at a Sun-Epimetheus-spacecraft, or phase, angle of 71 degrees. Image scale is 89 meters per pixel.

    VIRGO
    VIRGO --- ---
    New Mysteries Surround New Horizons’ Next Flyby Target -

    The data show that MU69 might not be as dark or as large as some expected

    https://www.nasa.gov/feature/new-mysteries-surround-new-horizons-next-flyby-target

    NASA’s New Horizons spacecraft doesn’t zoom past its next science target until New Year’s
    Day 2019, but the Kuiper Belt object, known as 2014 MU69, is already revealing surprises.

    VIRGO
    VIRGO --- ---
    All About Exoplanets | DiscoverMagazine.com
    http://discovermagazine.com/rapid/2017/05/all-about-exoplanets

    As research to find life on other planets continues, the best is yet to come. In DM free,
    downloadable PDF, we explore exoplanet discovery, as well as decades of research on mass extinctions.

    VIRGO
    VIRGO --- ---
    Woow!!

    Proxima Centauri: What do we know? – by Mikko Tuomi – Red Dots
    https://reddots.space/proxima-centauri-what-do-we-know-by-mikko-tuomi/

    Following the announcement of the discovery of Proxima b, the Red Dots campaign aims at detecting additional
    small planetary sized companions to Proxima Centauri. But we already have hints of variability in the star’s
    radial velocities not explained by the presence of Proxima b alone. There is more to the star than Proxima b.

    VIRGO
    VIRGO --- ---
    VIRGO:
    ESOcast 115 Light: Meet one of the most energetic objects in the Universe
    https://www.youtube.com/watch?v=kjbM9FVIXOY
    VIRGO
    VIRGO --- ---
    Zářivá spirála s aktivním srdcem | ESO Česko
    http://www.eso.org/public/czechrepublic/news/eso1720/?lang

    Dalekohled ESO/VLT pořídil úchvatný záběr spirální galaxie s příčkou M 77 (Messier 77). Snímek sice zachycuje krásy galaxie
    například v podobě zářících ramen protkaných temnými oblaky prachu, ale není schopen odhalit pravou neklidnou povahu M 77.

    VIRGO
    VIRGO --- ---
    It is not clear what might have caused the AMC-9 satellite to become unresponsive.

    A satellite may be falling apart in geostationary orbit [Updated] | Ars Technica
    https://arstechnica.com/.../07/a-large-satellite-appears-to-be-falling-apart-in-geostationary-orbit/

    In the early hours of 1st July, the SES Satellite Control reestablished contact to AMC-9. SES and the satellite
    manufacturer Thales are working around the clock to evaluate the status and define the next steps.

    Tracking information received on 29 June had suggested that at least two separate objects were located in the vicinity
    of AMC-9. Their source has still to be determined. The new piece of information was included by Thales and SES in their
    investigations.

    VIRGO
    VIRGO --- ---
    Radio emission detected from a gamma-ray pulsar
    https://phys.org/news/2017-07-radio-emission-gamma-ray-pulsar.html

    A team of astronomers led by Yogesh Maan of the Netherlands Institute for Radio Astronomy (ASTRON) has discovered radio emission from the gamma-ray pulsar known as
    J1732−3131. The study, presented in a paper published June 26 on arXiv.org, provides more details about J1732−3131, which was originally detected as a radio-quiet pulsar.

    Located nearly 2,000 light years away from the Earth, J1732−3131 has a rotation period of about 196 milliseconds and is one such gamma-ray pulsar with hart-to-identify
    radio emission. The pulsar was found thanks to the data provided by the large area telescope (LAT) onboard NASA's Fermi Gamma-ray Space Telescope. So far, only a faint
    radio signal from this pulsar was detected at 34 MHz in 2012.

    More recently, Maan's team, motivated by previous faint detections, conducted follow-up observations of J1732−3131 between March 2014 and April 2015, using the Ooty radio
    telescope (ORT), located in Muthorai, India. This 530-meter-long and 30-meter-wide cylindrical paraboloid telescope allowed the researchers to observe the pulsar at 327 MHz,
    which resulted in detection of a faint periodic radio signal.

    VIRGO
    VIRGO --- ---
    APOD: 2017 July 5 - Aphelion Sunrise
    https://apod.nasa.gov/apod/ap170705.html

    VIRGO
    VIRGO --- ---
    Now in HD: the Earth’s Turbulent Core | CNRS News
    https://news.cnrs.fr/articles/now-in-hd-the-earths-turbulent-core

    Taking a deep dive into our planet’s turbulent core 3000 kilometers below surface level, geophysicists have
    emerged with high-definition 3D simulations showing the hidden mechanisms that govern the Earth’s magnetic field.

    Tequat_l299_st2ns_big67
    https://vimeo.com/223309160
    VIRGO
    VIRGO --- ---
    Artist's rendition of how the Tunguska event might have looked from the windows of a nearby airliner.

    https://futurism.com/anniversary-of-the-tunguska-event-what-really-happened/

    VIRGO
    VIRGO --- ---
    Teda letos probíhají doslova noktiluminiscenční orgie...

    After delayed start, magnificent noctilucent clouds are back in full effect
    https://watchers.news/2017/07/04/2017-noctilucent-clouds-season-late-start/

    VIRGO
    VIRGO --- ---
    BepiColombo’s journey to Mercury
    https://www.youtube.com/watch?v=0Yp-q1wqgig


    Animation visualising BepiColombo’s 7.2 year journey to Mercury.

    This animation is based on a launch date of 5 October, marking the start of the launch window in October 2018. It illustrates
    the gravity assist flybys that the spacecraft will make at Earth, Venus and Mercury before arriving at Mercury in December 2025.
    VIRGO
    VIRGO --- ---
    Fastest stars in the Milky Way are ‘runaways’ from another galaxy | University of Cambridge
    http://www.cam.ac.uk/research/news/fastest-stars-in-the-milky-way-are-runaways-from-another-galaxy

    A group of astronomers have shown that the fastest-moving stars in our galaxy – which are travelling so fast
    that they can escape the Milky Way – are in fact runaways from a much smaller galaxy in orbit around our own.

    The researchers, from the University of Cambridge, used data from the Sloan Digital Sky Survey and computer simulations to demonstrate
    that these stellar sprinters originated in the Large Magellanic Cloud (LMC), a dwarf galaxy in orbit around the Milky Way.

    These fast-moving stars, known as hypervelocity stars, were able to escape their original home when the explosion of one star in a binary
    system caused the other to fly off with such speed that it was able to escape the gravity of the LMC and get absorbed into the Milky Way.
    The results are published in the Monthly Notices of the Royal Astronomical Society, and will be presented today (5 July) at the National
    Astronomy Meeting in Hull.

    Astronomers first thought that the hypervelocity stars, which are large blue stars, may have been expelled from the centre of the Milky Way
    by a supermassive black hole. Other scenarios involving disintegrating dwarf galaxies or chaotic star clusters can also account for the speeds
    of these stars but all three mechanisms fail to explain why they are only found in a certain part of the sky.

    To date, roughly 20 hypervelocity stars have been observed, mostly in the northern hemisphere, although it’s possible that there are many more
    that can only be observed in the southern hemisphere.

    VIRGO
    VIRGO --- ---
    JAYME: Teda na první výstřel skvělý! :o
    JAYME
    JAYME --- ---
    JAYME: první obdobný pokus v noci. zatím nic moc. 300mm je prostě málo. příště zkusím aspoň stack více fotek dle návodu z netu.

    Kliknutím sem můžete změnit nastavení reklam