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Four Breathtaking Solar Eclipses You Can See From Other Planets. Boo 2 A Madea Halloween (2017) Ipod Download. On August 2. 1st, millions of Earthlings will gather to watch as a total solar eclipse sweeps across the centerline of the United States over the course of 9. For many, it’ll be once- in- a- life- time spectacle.

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But if you had a spacecraft on hand, you wouldn’t need to wait decades for the next total solar eclipse to arrive at a town near you—you could simply jet off to Mars, Jupiter, Saturn, or even Pluto. That’s because there’s a veritable zoo of solar eclipses occurring all across our solar system, all the time. To be fair, none of these extraterrestrial eclipses is quite like the total solar eclipse here on Earth, where a quirk of celestial geometry causes the Moon to stack perfectly over the Sun, leaving a fiery ring of coronal jets to illuminate the sky. Some satellites, like Mars’ moon Phobos, are too small to engulf the Sun from the perspective of an observer on the planet, resulting in what astronomers call a transit. In other cases, like that of Saturn’s moon Titan, the angular size of the satellite in the sky is far greater than that of the Sun, resulting in a solar occultation.

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But that’s just the basics—eclipses, it turns out, come in all shapes and sizes, and studying them can tell us a lot about our cosmic neighborhood. Tiny transits at Mars. For most other planets, we have to imagine what a solar eclipse would look like from the surface (or, in the case of a gas giant, the cloud- tops). But when it comes to Mars, we’ve actually seen quite a few. In 2. 00. 4, NASA’s Spirit and Opportunity rovers captured six solar transits events from the surface of Mars—four involving the potato- shaped moon Phobos, another two starring the even runtier satellite Deimos.

They were, according to a paper published in Nature the following year, the first direct images of satellites transiting the Sun from the surface of another planet. Before NASA’s rovers landed, “the uncertainty about where Phobos would be at any given time was about as big as Phobos.” Once eclipse observations had improved the orbits of the two moons, the European Space Agency’s Mars Express Orbiter was able to point its camera accurately enough to capture high- res images of both, Lemmon said.

Eclipse- watching on Mars has only gotten better, especially since NASA’s Curiosity rover landed in Gale Crater in August 2. Just look at this footage Curiosity captured in 2. Phobos racing across the Sun, transforming our beloved star into an eerie cyclops monster over the course of 3. I think that’s the best shot of an eclipse . Even though Spirit and Opportunity refined the positions of Mars’ moons more than a decade ago, there’s still plenty we can learn by watching their transits.“Even now, while there’s no missing where Phobos and Deimos are, their orbits are changing all the time due to the push and pull of gravity,” from Mars, Lemmon explained. That is why Phobos is spiraling in toward Mars and will eventually be destroyed.”Indeed, eclipses may be critical to figuring out how soon Phobos faces annihilation—and when Deimos will be cast away into deep space.

Hazy eclipses at Saturn. With. 62 confirmed moons, Saturn’s skies offer myriad eclipse- viewing opportunities, from tiny solar transits to massive occultations to moons stacked atop other moons. But of all the gas giant’s many satellites, few produce an eclipse as otherworldly as Titan, a massive methane cauldron that challenges our understanding of the kinds of places life might emerge.

It was the Voyager 1 spacecraft that spotted the first solar occultation at Titan in 1. The Astrophysical Journal. As Titan swept across the Sun, Voyager captured some of the light that filtered through its hazy atmosphere, which scientists used to confirm that the moon’s skies are composed mostly of nitrogen. Since NASA’s Cassini probe arrived in orbit around Saturn in 2. Titan eclipses, which we’ve used to probe the chemistry of the moon’s thick haze. Some of what we’ve learned even has implications for understanding planets beyond our solar system. In 2. 01. 4, analyzing visible and infrared spectra collected by Cassini during solar occultations, researchers demonstrated that Titan absorbs, refracts, and scatters sunlight in ways that may obscure information about deeper parts of the atmosphere.

This, the researchers wrote in a paper published in PNAS, could have ramifications for elucidating the atmospheres of exoplanets, particularly “super Earths.” “Haze has a dramatic effect on the transit spectra,” the researchers wrote, noting that it “substantially impacts the amount of information that can be gleaned.” This information could prove incredibly useful when the James Webb Space Telescope starts peering into the atmospheres of distant planets over the next few years. But as valuable at the science is, astronomers are mostly drawn to Saturnian eclipses because of their sheer beauty.“In most cases, we imaged eclipses because they are just wondrous events, at Saturn as they are on Earth,” Cassini imaging lead Carolyn Porco told Gizmodo. Because of Uranus’ funky tilt, its poles are alternately illuminated during its 8. Sun. The moons, which circle Uranus in the band of rings stretched across the planet’s equator, only align edge- on with the Sun ever 4. Ice Giant. Rare, but not impossible to catch. In 2. 00. 6, just as Uranus was approaching its summer equinox, the Hubble Space Telescope caught a never- before- seen- glimpse of the moon Ariel traversing the face of the ice giant and casting a shadow, or umbra, on the planet’s blue- green cloud tops. From the “surface” of Uranus, it would have looked like a solar eclipse.“These observations were planned only to study the atmosphere of Uranus – the detection of Ariel and its shadow were purely serendipitous,” Heidi Hammel, Executive Vice President of AURA, who helped analyze the image while working at the Space Science Institute, told Gizmodo.

This, he explained, is due to the fact that at Uranus, Ariel is roughly ten times bigger in the sky than the distant Sun. As Uranus continued to approach the summer equinox, there were other eclipses of other large moons, including Umbriel, Titania, and Oberon. But Ariel’s eclipse was the money shot, and it’s likely to stay that way for a while—the next equinox at Uranus won’t be until 2. Maybe, if we’re lucky, the weird world will have had another visitor by then. Years of solar eclipse at Pluto. Pluto may seem like a cosmic castaway, taking 2. Sun. Thankfully, it’s got Charon, a moon approximately half its size with which it’s locked in an endless gravitational embrace.

And because Charon is so close—just 1. Pluto—when eclipse season hits, eclipses happen a lot.“When Pluto’s in eclipse season, twice during its 2. Pluto and Charon essentially orbit around each other every six days, you get an eclipse every six days,” Planetary Society astronomer Bruce Betts told Gizmodo. Before the New Horizons spacecraft zipped past Pluto in 2. Charon’s incessant photobombing.“The last eclipse season was not that long ago, and astronomers used the event—Charon in front of Pluto, Pluto in front of Charon—to resolve the two bodies,” Betts said.

For comparison, this is what Pluto looks like today, two years after the New Horizons flyby.“The whole thing is pretty amazing,” Betts said, noting that the sunlight is so weak at Pluto astronomers had struggled to get any resolution at all on the icy world. Or Neptune’s mysterious moon Despina, which a citizen scientist discovered transiting the sun when he re- analyzed old data from the Voyager 2 flyby in 2. Then, there’s the eclipse here on Earth. And it’s not only the size of our Moon, but the Moon at this point in time—in early lunar history, the Moon was too close.” So, as you’re making your travel plans to hit the centerline of the eclipse on August 2. But it’s also more than an Earthly phenomena. It’s a connection to a far grander celestial choreography that promises to dazzle observers for eons to come.

DVD FAQThis is the June 2. Internet DVD FAQ for the rec. Usenet newsgroups.(See below for what's new.) Send corrections, additions, and new questions to.

Jim Taylor < jtfrog@usa. This FAQ is usually updated at least once a month.

If. you are looking at a version more than a few months old, it's probably an out- of- date copy. Where can I get statistics?? Aren't discs. too fragile to be rented?? Will it work in all. Does it work. with NTSC, PAL, and SECAM??

Doesn't it compress. Can't. DVDs hold four hours per side?? Do they. all have 5. Why do I get. 2- channel surround audio? What do I do?? Why do. I get a pink or black square?? How. can I play them?

New MPEG LA pricing. Also mentioned RF activation. Hopefully nothing major broke. For the absurdly curious, here's the list of. The most current version is on the Web at < dvddemystified.

A text version was once posted periodically as . You can also get a text version.

FAQ by using the . Translations to a. If you'd like to translate the DVD FAQ into another language (Klingon. Jim. Also see 6. 4.

DVD info in other languages. Take a gander at. Earl's Famous DVD. Technology Exposition Web Page Extravaganza Supreme Deluxe. Or you might prefer.

DVD Q& A. If you type . It's the most accurate source of DVD information in. If you find something you think is in error, please. Jim know. There's plenty of other good. DVD on the Internet.

Pointers to other DVD sites are scattered throughout the FAQ and in section. The DVD FAQ is written by Jim Taylor, the author of DVD. Everything You Ever Wanted to Know About DVD, and Blu- ray Disc Demystified. Jim has been in the DVD. DVD business. In 1. DVD. began writing articles to let others know about this amazing new technology. Jim. received the 2.

DVD Pro Discus Award for Outstanding Contribution to the. Industry, was named one of the 2. DVD executives by DVD Report. Digital Media Hall of Fame, and was. Pioneers of DVD in the October 2. One to One. magazine.

Jim has worked with interactive media for over 2. CD- ROMs, Web sites, and DVDs, along with. He writes articles and. DVD for publications such as. Widescreen Review and serves as. Chairman of the IDMA/DVD Association.

Jim was formerly. DVD Evangelist at Microsoft, and is currently Chief Technologist at. Sonic Solutions, the leading developer of DVD. BD creation software.

Since you asked, here are the stats as of March 2. Size: 5. 98 KBNumber of words: 6. Number of external links: 1,9.

If you're wondering why it's all in one big piece instead of broken into. FAQ. I realize this. Web. TV browsers. I might break it up some day.

DVD is movies on a shiny disc, and much more. It's an optical disc storage technology.

DVD is. essentially a bigger, faster CD that can hold high- quality digital video, better- than- CD. DVD encompasses home. DVD has. widespread support from all major electronics companies, all major computer. With this. unprecedented support, DVD became the most successful consumer electronics. In 2. 00. 7, ten. DVD playback devices worldwide.

DVD players, DVD PCs, and DVD game consoles. It's important to understand the difference between the physical formats. DVD- ROM and DVD- R) and the application formats (such as.

DVD- Video and DVD- Audio). DVD- ROM is the base format that holds data.

DVD- Video. (often simply called DVD) defines how video programs such as movies are stored. DVD- Video player or a DVD computer (see. The difference is similar to that between CD- ROM and Audio CD. DVD- ROM. includes recordable variations: DVD- R/RW, DVD- RAM, and DVD+R/RW (see. The application formats include DVD- Video, DVD- Video. Recording (DVD- VR), DVD+RW Video Recording (DVD+VR), DVD- Audio Recording (DVD- AR). Tales Of An Immoral Couple (2017) Full Divx Movies here.

DVD- Audio (DVD- A), and Super Audio. CD (SACD). There are also special application formats for game consoles such as. Sony Play. Station 2 and Microsoft Xbox. A report from DVD Forum Steering Committee. DVD, as. an international standard, is simply three letters.

Nevertheless, Toshiba. DVD Forum Web site—. No one agrees on that one either.)Over 2 hours of high- quality digital video (a double- sided, dual- layer. VHS quality. video). Support for widescreen movies on standard or widescreen TVs (4: 3 and 1.

Up to 8 tracks of digital audio (for multiple languages, commentaries. Up to 3. 2 subtitle/karaoke tracks. Automatic seamless branching of video (for multiple story lines or ratings. Up to 9 camera angles (different viewpoints can be selected during.

On- screen menus and simple interactive features (for games, quizzes. Multilingual identifying text for title name, album name, song name, cast. Instant rewind and fast forward (no . Resistant to heat. Compact size (easy to handle, store, and ship; players can be portable. Noncomedogenic. Note: Most discs do not contain all features (multiple. Some discs may not allow searching or.

Most players support a standard set of features: Language choice (for automatic selection of video scenes, audio tracks. Special effects playback: freeze, step, slow, fast, and scan. Parental lock (for denying playback of discs or scenes with objectionable. Programmability (playback of selected sections in a desired sequence). Random play and repeat play. Digital audio output (PCM stereo and Dolby Digital). Recognition and output of DTS Digital Surround audio tracks.

Playback of audio CDs.* Must be supported by additional content on the. Some players include additional features: Component video output (YUV or RGB) for higher quality picture.

Progressive- scan component output (YUV or RGB) for highest quality analog. Digital video output (SDI, 1. DVI/HDMI) for perfect digital picture. This is a. player feature, not a DVD disc feature. DVD has the capability to produce near- studio- quality video and. CD- quality audio. DVD is vastly superior to consumer videotape and.

However, quality. As compression experience and technology. DVD. authoring software becomes widely available we also see more shoddily produced. A few low- budget DVDs even use MPEG- 1 encoding (which is no better than. VHS) instead of higher- quality MPEG- 2. DVD video is usually encoded from digital studio master tapes to MPEG- 2.

The encoding process uses lossy compression that removes. The resulting. video, especially when it is complex or changing quickly, may sometimes contain.

At. average video data rates of 3. Mbps (million bits/second), compression. Higher data rates can result in. Mbps. As MPEG compression technology improves, better quality is being.

Video from DVD sometimes contains visible artifacts such as color. Artifacts are sometimes caused by poor MPEG.

TV, bad. cables, electrical interference, sloppy digital noise reduction, improper. Most DVDs exhibit few visible MPEG compression. If you think otherwise, you are. Some early DVD demos were not very good, but this is simply an indication of.

DVD can be if not properly processed and correctly reproduced. In- store. demos should be viewed with a grain of salt, since most salespeople are. Most TVs have the sharpness set too high for the clarity of DVD.

This. exaggerates high- frequency video and causes distortion, just as the treble. For best. quality the sharpness control should be set very low. Brightness should also not. Some DVD players output video with a black- level setup of 0 IRE. Japanese standard) rather than 7. IRE (US standard). On TVs that are not.

There may be. an option in the player menu to use standard black level. DVD video has. exceptional color fidelity, so muddy or washed- out colors are almost always a.

DVD player or disc. DVD audio quality is superb.

DVD includes the option of PCM (pulse code. CD. As with video, audio quality.

In spite of. compression, Dolby Digital and DTS can be close to or better than CD quality. Vagueness of the DVD specification and inadequate testing of players and. Some movie discs don't function fully. Poorly compressed audio or video may be. These predictions were woefully optimistic.

The first. players appeared in Japan in November, 1. U. S. Prices for the. By the end of 2. 00.

In 2. 00. 3 players became available.