Explanation: An unusual type of solar eclipse occurred in 2012. Usually, it is the Earth’s Moon that eclipses the Sun. That year, most unusually, the planet Venus took a turn. Like a solar eclipse by the Moon, the phase of Venus became a continually thinner crescent as Venus became increasingly better aligned with the Sun. Eventually, the alignment became perfect and the phase of Venus dropped to zero. The dark spot of Venus crossed our parent star. The situation could technically be labelled a Venusian annular eclipse with an extraordinarily large ring of fire. Pictured here during the occultation, the Sun was imaged in three colours of ultraviolet light by the Earth-orbiting Solar Dynamics Observatory, with the dark region toward the right corresponding to a coronal hole. Hours later, as Venus continued in its orbit, a slight crescent phase appeared again. The next Venusian transit across the Sun will occur in 2117. </center>
THE ORIONID meteor shower promises to dazzle stargazers with a spectacular display of shooting stars TONIGHT. But what is the best time too watch the meteor shower?
When its the Orionids meteor shower?
If you can’t view it, either it being cloudy or heavey lit area, Slooh will be Live streaming the event from tonight. Join Paul Cox, Dr. Paige Godfrey, and Bob Berman for a decidedly casual and far-ranging chat as as we train our telescopes on the Orionids. SLOOH Live Event of the Orionid Meteor Shower
The Orionids light up the night sky every year towards the end of October in “one of the most beautiful showers of the year”, according to Nasa.
The meteor shower will peak in the early of hours of Saturday (October 20) and once again in the early hours of Sunday (October 22). Sporadic meteors have already been dashing across the night sky from October 15 and should remain visible until November.
During the peak, stargazers can expect anywhere up to 50 meteors per hour, though this year Nasa believes that the numbers may not be as spectacular.
Nasa’s Jane Houston Jones said: “The Orionids peak on October 20, a dark, moonless night. Look near Orion’s club in the hours before dawn and you may see up to 10 to 15 meteors per hour. “Use binoculars to look for bright asteroid 7 Iris in the constellation Aries. Newbies to astronomy should be able to spot this magnitude 6.9 asteroids even from the city.”
What is the best time to view the Orionids meteor shower?
The peak of the Orionids will be visible anywhere on Earth in the early morning hours of tonight and tomorrow night, usually after midnight and just before dawn.
The best time for skywatchers to head outside is usually around 2am when the shower is at its most intense.
Star gazers will be aided this year by the lack of moonlight which should keep the skies clear of any hindering light pollution.
But Storm Brian will make the sky overcast tonight much of the UK as the weather bomb unleashes strong winds and rainstorms.
A Met Office spokesman said: “There’s quite a lot of cloud around this evening and overnight. The best chance of seeing them will be in the early hours before dawn.” He said that the clearest skies will be from 3am in the eastern part of England across East Anglia, the South East, Lincolnshire and the Midlands.”
To get the best views, stay away from any sources of light pollution and give your eyes some time to adjust to the dark of space.
Where will the Orionid meteor shower appear?
The Orionids derive their name from there point of origin next to the Orion constellation, which ascends in the east.
But the shower’s radiant point is mostly irrelevant because the meteors will shoot out in all sorts of directions, and usually remain unseen until about 30 degrees from the radiant.
However, if you spot a streaking meteor, you should be able to trace its path back to its origin next to Orion’s club.
What are the Orionids?
The spectacular shooting stars are remnants of the prolific Halley’s Comet, which visits Earth every 74 to 79 years.
When the comet passes through the solar system, chunks (Debris) of ice and rock break off from the comet thanks to the sun, and trail in the comet’s path. The first recorded reports of the shower date back to 1839, when it was spotted in America.
The Orionids are incredibly fast meteors and crash into Earth’s atmosphere at a speed of 66 km/s. Many of the falling stars leave ionised trails of glowing gas in their path.
Global Aurora at Mars Image Credit: MAVEN, LASP, University of Colorado, NASAExplanation: A strong solar event last month triggered intense global aurora at Mars. Before (left) and during (right) the solar storm, these projections show the sudden increase in ultraviolet emission from martian aurora, more than 25 times brighter than auroral emission previously detected by the orbiting MAVEN spacecraft. With a sunlit crescent toward the right, data from MAVEN’s ultraviolet imaging spectrograph is projected in purple hues on the right side of Mars globes simulated to match the observation dates and times. On Mars, solar storms can result in planet-wide aurora because, unlike Earth, the Red Planet isn’t protected by a strong global magnetic field that can funnel energetic charged particles toward the poles. For all those on the planet’s surface during the solar storm, dangerous radiation levels were double any previously measured by the Curiosity rover. MAVEN is studying whether Mars lost its atmosphere due to its lack of a global magnetic field.
Image credit: ESA/Hubble & NASA Text credit: European Space Agency
This beautiful Hubble image reveals a young super star cluster known as Westerlund 1, only 15,000 light-years away in our Milky Way neighborhood, yet home to one of the largest stars ever discovered.
Stars are classified according to their spectral type, surface temperature, and luminosity. While studying and classifying the cluster’s constituent stars, astronomers discovered that Westerlund 1 is home to an enormous star. Originally named Westerlund 1-26, this monster star is a red supergiant (although sometimes classified as a hypergiant) with a radius over 1,500 times that of our sun. If Westerlund 1-26 were placed where our sun is in our solar system, it would extend out beyond the orbit of Jupiter.
Most of Westerlund 1’s stars are thought to have formed in the same burst of activity, meaning that they have similar ages and compositions. The cluster is relatively young in astronomical terms —at around three million years old it is a baby compared to our own sun, which is some 4.6 billion years old.
Explanation: Can you find which day is the winter solstice? Each panel shows one day. With 360 movie panels, the sky over (almost) an entire year is shown in time lapse format as recorded by a video camera on the roof of the Exploratorium museum in San Francisco, California. The camera recorded an image every 10 seconds from before sunrise to after sunset and from mid-2009 to mid-2010. A time stamp showing the local time of day is provided on the lower right. The videos are arranged chronologically, with July 28 shown on the upper left, and January 1 located about half way down. In the videos, darkness indicates night, blue depicts clear day, while gray portrays pervasive daytime cloud cover. Many videos show complex patterns of clouds moving across the camera’s wide field as that day progresses. The initial darkness in the middle depicts the delayed dawn and fewer daylight hours of winter. Although every day lasts 24 hours, nighttime lasts longest in the northern hemisphere in December and the surrounding winter months. Therefore, finding the panel with the longest night will locate the day of winter solstice — which happens to be today in the northern hemisphere. As the videos collectively end, sunset and then darkness descend first on the winter days just above the middle, and last on the mid-summer near the bottom.
Our magnificent Milky Way Galaxy sprawls across this ambitious all-sky panorama. In fact, at 800 million pixels the full resolution mosaic strives to show all the stars the eye can see in planet Earth’s night sky. As part of ESO’s Gigagalaxy Zoom Project, Serge Brunier recorded images with a digital camera over several months of 2008 and 2009 at exceptional astronomical sites—the Atacama Desert in the southern hemisphere and the Canary Islands in the northern hemisphere. The individual frames were stitched together and mapped into a single, flat, apparently seamless 360 by 180 degree view. The final result is oriented so the plane of our galaxy runs horizontally through the middle with the bulging Galactic Center at image center. Below and right of center are the Milky Way’s satellite galaxies, the Magellanic Clouds. The Andromeda galaxy is just below center about 1/6 of the way from the left edge. Also visible are bright planets (with spikes around them) and even a comet.
Sculpted by stellar winds and radiation, the star factory known as Messier 17 lies some 5,500 light-years away in the nebula-rich constellation Sagittarius. At that distance, this 1/3 degree wide field of view spans over 30 light-years. The sharp composite, color image, highlights faint details of the region’s gas and dust clouds against a backdrop of central Milky Way stars. Stellar winds and energetic light from hot, massive stars formed from M17 stock of cosmic gas and dust have slowly carved away at the remaining interstellar material producing the cavernous appearance and undulating shapes. M17 is also known as the Omega Nebula or the Swan Nebula.
Image Credit: ESA/Hubble and NASA Beautiful island universe Messier 94 lies a mere 15 million light-years distant in the northern constellation of the hunting dogs, Canes Venatici. A popular target for earth-based astronomers, the face-on spiral galaxy is about 30,000 light-years across, with spiral arms sweeping through the outskirts of its broad disk. But this Hubble Space Telescope field of view spans about 7,000 light-years or so across M94’s central region. The sharp close-up examines the galaxy’s compact, bright nucleus and prominent inner dust lanes, surrounded by a remarkable bluish ring of young, massive stars. The massive stars in the ring are all likely less than 10 million years old, indicating the galaxy experienced a well-defined era of rapid star formation. As a result, while the small, bright nucleus is typical of the Seyfert class of active galaxies, M94 is also known as a starburst galaxy. Because M94 is relatively nearby, astronomers can explore in detail the reasons for the galaxy’s burst of star formation.