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Gracie-the-Mixed-Breed
http://cdn-www.dailypuppy.com/dog-im...05-01_w450.jpg
My name is Gracie. I have a lot personally and spunk. My dog dad is mixed with Cocker Spaniel and Jack Russell terrier and my dog mom is Dachshund and Chihuahua. I love to go camping and hiking with my human family. I may be small with chunky legs but this helps a lot on mountain trails. I have no problem keeping up but my family has the problem of keeping up with me. I also love when my mom takes me to a pet store where I can check out all the toys and other dogs. More... |
Four Fashionable Fosters Part 4: Chanel - May 01, 2011
http://goodmorningkitten.com/media/k...kitten1217.jpg
Four Fashionable Fosters Part 4: Chanel Jaime says: Chanel had such spunk! She had an amazing personality and never failed to make me laugh. She was always up to no good, but I never cared because it always kept me entertained. Definitely a determined little kitten. And she LOVED to run. That girl had speed when she really set her heart on it. She also had the cutest little "mew"; it was so high pitched but loud! Chanel's favorite thing was to curl up in my lap when she finally got sleepy. :-) Four Fashionable Fosters Part 3: Dior Four Fashionable Fosters Part 2: Prada Four Fashionable Fosters Part 1: Armani Courtesy of: Jaime Sundquist http://feeds.feedburner.com/~r/TheDa...~4/-CqFJ1xUBFU More... |
White House Correspondents Dinner: Obama Takes On Trump, Birthers, The Media, And Mor
President Barack Obama exercised his revenge Saturday after weeks of attacks from his would-be Republican challenger Donald Trump, joking that the billionaire businessman could bring change to the White House, transforming it from a stately mansion into...(read more)http://blackamericans.com/aggbug.aspx?PostID=275423
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Why is Qatar buying up London landmarks?
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Maguire hails team effort
Wigan coach Michael Maguire was left satisfied with his side's all-round effort after they thrashed Crusaders 48-16 on Sunday.
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Hale Crater
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Electrical Circuit Between Saturn and Enceladus
This artist's concept shows a glowing patch of ultraviolet light near Saturn's north pole that occurs at the "footprint" of the magnetic connection between Saturn and its moon Enceladus. The footprint and magnetic field lines are not visible to the naked eye, but were detected by the ultraviolet imaging spectrograph and the fields and particles instruments on NASA's Cassini spacecraft. The footprint, newly discovered by Cassini, marks the presence of an electrical circuit that connects Saturn with Enceladus and accelerates electrons and ions along the magnetic field lines. In this image, the footprint is in the white box marked on Saturn, with the magnetic field lines in white and purple. A larger white square above Enceladus shows a cross-section of the magnetic field line between the moon and the planet. This pattern of energetic protons was detected by Cassini's magnetospheric imaging instrument (MIMI) on Aug. 11, 2008. The patch near Saturn's north pole glows because of the same phenomenon that makes Saturn's well-known north and south polar auroras glow: energetic electrons diving into the planet's atmosphere. However, the "footprint" is not connected to the rings of auroras around Saturn's poles (shown as an orange ring around the north pole in this image). The Cassini plasma spectrometer complemented the MIMI data, with detection of field-aligned electron beams in the area. A team of scientists analyzed the charged particle data and concluded that the electron beams had sufficient energy flux to generate a detectable level of auroral emission at Saturn. Target locations were provided to Cassini's ultraviolet imaging spectrograph team. On Aug. 26, 2008, the spectrograph obtained images of an auroral footprint in Saturn's northern hemisphere. The newly discovered auroral footprint measured about 1,200 kilometers (750 miles) in the longitude direction and less than 400 kilometers (250 miles) in latitude, covering an area comparable to that of California or Sweden. It was located at about 65 degrees north latitude. In the brightest image the footprint shone with an ultraviolet light intensity of about 1.6 kilorayleighs, far less than the Saturnian polar auroral rings. This is comparable to the faintest aurora visible at Earth without a telescope in the visible light spectrum. Scientists have not yet found a matching footprint at the southern end of the magnetic field line. The background star field and false color images of Saturn and Enceladus were obtained by Cassini's imaging science subsystem. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif. manages the mission for NASA's Science Mission Directorate, Washington, D.C. The ultraviolet imaging spectrograph team is based at the University of Colorado, Boulder. The magnetospheric imaging team is based at the Johns Hopkins University Applied Physics Laboratory, Laurel, Md. The Cassini plasma spectrometer team is based at the Southwest Research Institute, San Antonio, Texas.
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Hayden Panettiere
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