Sometimes I complain about the earthly weather, but mostly I like to post about astronomy and space events. Hope you enjoy the articles.
By: Susie77, 7:22 PM GMT on August 29, 2013
Courtesy of NASA
Data from a NASA airborne science mission reveals evidence of a large and previously unknown canyon hidden under a mile of Greenland ice.
The canyon has the characteristics of a winding river channel and is at least 460 miles (750 kilometers) long, making it longer than the Grand Canyon. In some places, it is as deep as 2,600 feet (800 meters), on scale with segments of the Grand Canyon. This immense feature is thought to predate the ice sheet that has covered Greenland for the last few million years.
"One might assume that the landscape of the Earth has been fully explored and mapped," said Jonathan Bamber, professor of physical geography at the University of Bristol in the United Kingdom, and lead author of the study. "Our research shows there's still a lot left to discover."
Bamber's team published its findings Thursday in the journal Science.
The scientists used thousands of miles of airborne radar data, collected by NASA and researchers from the United Kingdom and Germany over several decades, to piece together the landscape lying beneath the Greenland ice sheet.
A large portion of this data was collected from 2009 through 2012 by NASA's Operation IceBridge, an airborne science campaign that studies polar ice. One of IceBridge's scientific instruments, the Multichannel Coherent Radar Depth Sounder, can see through vast layers of ice to measure its thickness and the shape of bedrock below.
In their analysis of the radar data, the team discovered a continuous bedrock canyon that extends from almost the center of the island and ends beneath the Petermann Glacier fjord in northern Greenland.
At certain frequencies, radio waves can travel through the ice and bounce off the bedrock underneath. The amount of times the radio waves took to bounce back helped researchers determine the depth of the canyon. The longer it took, the deeper the bedrock feature.
"Two things helped lead to this discovery," said Michael Studinger, IceBridge project scientist at NASA's Goddard Space Flight Center in Greenbelt, Md. "It was the enormous amount of data collected by IceBridge and the work of combining it with other datasets into a Greenland-wide compilation of all existing data that makes this feature appear in front of our eyes."
The researchers believe the canyon plays an important role in transporting sub-glacial meltwater from the interior of Greenland to the edge of the ice sheet into the ocean. Evidence suggests that before the presence of the ice sheet, as much as 4 million years ago, water flowed in the canyon from the interior to the coast and was a major river system.
"It is quite remarkable that a channel the size of the Grand Canyon is discovered in the 21st century below the Greenland ice sheet," said Studinger. "It shows how little we still know about the bedrock below large continental ice sheets."
The IceBridge campaign will return to Greenland in March 2014 to continue collecting data on land and sea ice in the Arctic using a suite of instruments that includes ice-penetrating radar.
For more information about NASA's Operation IceBridge, visit:
By: Susie77, 4:26 PM GMT on August 15, 2013
Around the world, amateur astronomers are turning their telescopes toward minor constellation Delphinus where a new star has appeared. Koichi Itagaki of Yamagata, Japan, discovered the nova on August 14th. At the time, the stellar brightness was +6.3. Since then it has continued to brighten, possibly crossing the 6th magnitude threshold of naked-eye visibility. John Chumack photographed the surging nova on August 15th from the John Bryan State Park in Yellow Springs, Ohio:
"The nova is hard to see naked eye unless you are in a very dark sky and know exactly where to look," says Chumack, "but this is a very bright nova visible in binoculars." He used a 16-inch Newtonian telescope to take the picture.
Backyard astronomers who wish to see this nova should point their GOTO telescopes to coordinates 20:23:30.7, +20:46:06 (J2000). More information and updates are available from Sky and Telescope.
By: Susie77, 12:46 PM GMT on August 09, 2013
Courtesy of Space.com
By Joe Rao, SPACE.com Skywatching Columnist | August 09, 2013 06:15am ET
Every August, just when many people go vacationing in the country where skies are dark, the best-known meteor shower, makes its appearance.
This year, the Perseid meteor shower is expected to reach its peak overnight on Monday (Aug. 12), and there are some key tips to keep in mind for your "shooting stars" viewing.
Peak activity for the Perseids is unfortunately predicted for the daylight hours across North America, so stargazers with clear skies are encouraged to seek out the meteor display during the pre-dawn hours of Monday and again during the early morning hours of Tuesday (Aug. 13). At these times, the absence of bright moonlight can maximize your chances of spotting a meteor.
At mid-northern latitudes, moonset on Sunday evening (Aug. 11) occurs at about 10:15 p.m. local time and around 10:50 p.m. the following night. Since dawn doesn't break until around 4:30 a.m. local time that means there will be between five-and a-half to six hours of dark, moonless skies for the two best viewing nights for the Perseids.
Take full advantage of this year's favorable lunar circumstances. Next year, a bright waning gibbous moon will flood the after-midnight night sky with its light and seriously hinder the Perseids.
Perseids: the remains of a comet
We know today that the Perseid meteor shower is actually created by the remains of the Comet Swift-Tuttle. Discovered back in 1862, this comet takes approximately 130 years to circle the sun. And in much the same way that the Comet Tempel-Tuttle leaves a trail of debris along its orbit to produce the Leonid meteor shower of November, Comet Swift-Tuttle produces a similar debris trail along its orbit to cause the Perseids display.
Every year during mid-August, the Earth passes near the orbit of Swift-Tuttle and crosses the comet's debris stream. The comet material left behind then ram's into our atmosphere at approximately 37 miles per second (about 133,000 mph/214,000 km/h) to create bright streaks of light in our mid-summer night skies.
Comet Swift-Tuttle made its most recent appearance more than 20 years ago, in December 1992. Its orbit is highly elongated and as such it takes roughly 130 years to make one trip around the sun.
For several years before and after its 1992 return, the Perseids were a far more prolific shower, appearing to produce brief outbursts of as many as several hundred meteors per hour, many of which were dazzlingly bright and spectacular. The most likely reason was that the Perseids parent comet was itself passing through the inner solar system and that the streams of Perseid meteoroids in the comet's vicinity were larger and more thickly clumped together, leading to brighter meteors as well as much-higher-than-normal meteor rates.
But now, with the comet now having retreated nearly 3.2 billion miles (5.1 billion km) back out into space, Perseid activity has returned to normal.
Perseid meteor clumps
A very good meteor shower will produce about one meteor per minute for a given observer under a dark country sky. However, any light pollution from city lights or moonlight considerably reduces the count.
The August Perseids are among the strongest of the readily observed annual meteor showers, and at maximum activity nominally yield 90 or 100 meteors per hour. However, observers with exceptional skies often record even larger numbers.
But while 90 to 100 meteors per hour correspond to at least one meteor per minute, keep in mind that this is only a statistical average. In reality, what usually is seen is what some have called, "the clumping effect." Sometimes you'll see two or even three Perseids streak across the sky in quick succession, all within less than minute. This is usually followed by a lull of several minutes or more, before the sky suddenly bears fruit once again.
When and where to look
Typically during an overnight watch, the Perseids are capable of producing a number of bright, flaring and fragmenting meteors, which leave fine trains in their wake. On the night of shower maximum, the Perseid radiant is not far from the famous "Double Star Cluster" of Perseus.
Low in the northeast during the early evening, it rises higher in the sky until morning twilight ends observing. Shower streakers appearing close to the radiant have foreshortened tracks; those appearing farther away are often brighter, have longer tracks, and move faster across the sky. About five to 10 of the meteors seen in any given hour will not fit this geometric pattern, and may be classified as sporadic or as members of some other (minor) shower.
Perseid meteor shower activity increases sharply in the hours after midnight, so plan your observing times accordingly. We are then looking more nearly face-on into the direction of the Earth’s motion as it orbits the sun, and the radiant is also higher up.
Making a meteor count is as simple as lying in a lawn chair or on the ground and marking on a clipboard whenever a "shooting star" is seen. Watching for the Perseids consists of lying back, gazing up into the stars, and waiting. It is customary to watch the point halfway between the radiant (which will be rising in the northeast sky) and the zenith, though it's all right for your gaze to wander.
Meteor counts should be made on several nights before and after the predicted maximum, so the behavior of the shower during off-peak nights can be determined. Usually, good numbers of meteors should be seen on the preceding and following nights as well. The shower is generally at one-quarter strength one or two nights before and after maximum.
A few Perseids can be seen as much as two weeks before and a week after the peak. The extreme limits, in fact, are said to extend from July 17 to Aug. 24, though an occasional one might be seen almost anytime during the month of August.
No danger in watching
Many years ago, a phone call came into New York's Hayden Planetarium. The caller sounded concerned after hearing a radio announcement of an upcoming Perseid meteor display and wanted to know if it would be dangerous to stay outdoors on the night of the peak of the shower (perhaps assuming there was a danger of getting hit).
These meteoroids, however, are no bigger than sand grains or pebbles, have the consistency of cigar ash and are consumed many miles above our heads. The caller was passed along to the Planetarium's Chief Astronomer who commented that there are only two dangers from observing the Perseid meteor shower: getting drenched with dew and falling asleep!
August is also the month of "The Tears of St. Lawrence," which has a historic link to the Perseids.
Laurentius, a Christian deacon, is said to have been martyred by the Romans in 258 AD on an iron outdoor stove. It was in the midst of this torture that Laurentius cried out: "I am already roasted on one side and, if thou wouldst have me well cooked, it is time to turn me on the other."
The saint’s death was commemorated on his feast day, Aug. 10. King Phillip II of Spain built his monastery place the "Escorial," on the plan of the holy gridiron. And the abundance of shooting stars seen annually between approximately Aug. 8 and 14 have come to be known as St. Lawrence's "fiery tears."
Whether you plan to make detailed meteor counts or just lie back and watch nature put on a show, there should be plenty to during the predawn hours of Aug. 12 and 13. As one long-time meteor enthusiast once noted: "Meteor observing is relaxing and enjoyable, potentially dramatic and just plain fun!"
Editor's Note: If you snap an amazing picture of the 2013 Perseid meteor shower or any other night sky view that you'd like to share for a possible story or image gallery, send photos, comments and your name and location to managing editor Tariq Malik at email@example.com.
Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, the Farmer's Almanac and other publications, and he is also an on-camera meteorologist for News 12 Westchester, N.Y. Follow us @Spacedotcom, Facebookand Google+. Original article on SPACE.com.
By: Susie77, 2:49 PM GMT on August 03, 2013
Courtesy of SpaceWeather
FIRST PERSEIDS OF 2013 (Updated): Earth is entering a broad stream of debris from comet 109P/Swift-Tuttle, source of the annual Perseid meteor shower. Although the shower won't peak until August 12-13, when Earth hits the densest part of the stream, the first Perseids are already arriving. "Despite poor weather over our network of meteor cameras, we have detected six Perseid fireballs since July 30th," reports Bill Cooke, head of NASA's Meteoroid Environment Office. He made this plot showing the orbits of the meteoroids:
In the diagram, the green lines trace the orbits of Perseid meteoroids. All six intersect Earth (the blue dot). The orbit of the parent comet is color-coded purple. An inset shows one of the fireballs shining almost as brightly as the Moon: video.
The shower is just getting started. Rates should remain low for the next week as Earth penetrates the sparse outskirts of the debris stream, then skyrocket to ~100 meteors per hour as the calendar turns to the second week of August. Stay tuned for more fireballs.
The views of the author are his/her own and do not necessarily represent the position of The Weather Company or its parent, IBM.