CNET Do-It-Yourself Camera and Music Phone Projects: 24 Cool by Ari Hakkarainen

By Ari Hakkarainen

Dial up the leisure in your cellular phoneHere's your likelihood to take the sound and imaginative and prescient of your cellular phone to new heights-with 24 easy-to-execute tasks you've gotten by no means dreamed attainable. Ever imagine you'll hearken to tune and podcasts in your cellphone? you could! Ever imagine you may take electronic pictures of stronger caliber along with your cellphone? good, after all you could, and CNET selfmade digicam and track telephone initiatives will allow you to do it all.Produced along side CNET.com, where you opt for the most recent in tech and shopper electronics, and written by means of high-tech specialist Ari Hakkarainen, this ebook leads you step-by-step via each one undertaking. If you've ever desired to take images together with your cell phone that may make expert shutterbugs jealous, or amp up the musical functions of your hand-held, this quintessential how-to is simply the e-book you need!Take better caliber photosRecord domestic video clips in your cellular phoneShare your pictures with friends and family with no incurring community chargesDownload and hear tune and podcastsSave cash by means of studying how one can obtain loose song and ringtones in your phoneRecord your individual ringtonesWatch television in your phoneAnd even more!

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30 Fig. 11 (Top) Russell’s original diagram published in 1913 made use of photographically acquired spectral data to illustrate the relationship of luminosity (Y-axis) to spectral class (X-axis). It was known as the Russell diagram for several years until it was found that the Danish astronomer Ejnar Hertzsprung had published the same findings independently in 1911. It then became known as the Hertzsprung-Russell diagram. (Bottom) Modern graphic of the “theoretical” HRD with calculated surface temperatures as the X-axis plotted against luminosity as the Y-axis 2 A Series of Firsts, from Daguerreotypes to Dry Plates The Photographic Exploration of Deep Space and the Realm of the Nebulae 3 The late nineteenth century saw two transitions in astrophotography.

Although the Sun was photographed by Fizeau and Foucault in 1845 using Daguerre’s method, other stars would pose a more serious challenge for the early daguerreotypists because they were far fainter subjects. Sharp stellar images would require considerably longer exposures and a substantially more sensitive photographic medium. During the next few years an unlikely pair of innovators would push the available technology to capture the first successful images of distant stars. American astronomer William Cranch Bond (1789–1859) was the first director of the Harvard College Observatory.

Stars may pulsate or exhibit outbursts or flares. The science of variable stars has not only contributed to our knowledge about stars but has become the cornerstone of several diverse areas in astronomy, from cosmology to exoplanet discovery. Variable star research is also a field where amateurs, and particularly women, have historically made enormous contributions. One of the great contributors was American Henrietta Swan Leavitt (1868–1921). Leavitt graduated Radcliffe College in 1892. Her only exposure to astronomy was a course she took in her senior year.

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