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ETP - Experience the Planets

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Colin Chapman Colin Chapman's picture
ETP - Experience the Planets
Found this fantastic site, basically exploring each of the planets in our solar system using some great artwork. It only launched a handful of months ago, so there are only 1-2 images per planet so far, but they're great, and they're downloadable! it should prove indispensible as the site develops. http://www.experiencetheplanets.com/ Colin

Radioactive Ape Designs: ENnie and Indie Award nominated publisher of Atomic Highway!
http://radioactiveapedesigns.com

wint-R-mute wint-R-mute's picture
Re: ETP - Experience the Planets
wow. great find. thanks for posting!
Tunips Tunips's picture
Re: ETP - Experience the Planets
"Ambient music ahead" How considerate. I like it already.
GreyBrother GreyBrother's picture
Re: ETP - Experience the Planets
There swells my Wallpaper folder :) Thanks, work collegues already asked about it (Yes, my computer spends that much time on the desktop)
nick012000 nick012000's picture
Re: ETP - Experience the Planets
Did Triton get hit with a RKKV or something in the "Death of Triton" picture?

+1 r-Rep , +1 @-rep

Eleazar Eleazar's picture
Re: ETP - Experience the Planets
Looks to me like it's the artist's vision of Triton as it passes its Roche limit. Triton is on a "reverse" orbit compared to the spin of Neptune, so it's slowing down, and will eventually get pulled into the planet. As I understand it, the Roche limit is when a smaller planetary-type body is so close to a larger one that it's gravity is no longer sufficient to hold it together, and the larger body's power tears it apart. I'm sure wikipedia can explain it better, or maybe NASA has an entry on it. Here we go: http://imagine.gsfc.nasa.gov/docs/dictionary.html#R From that website, I quote: "Roche limit The smallest distance from a planet or other body at which purely gravitational forces can hold together a satellite or secondary body of the same mean density as the primary. At less than this distance the tidal forces of the larger object would break up the smaller object." (Hopefully listing the webpage is sufficient citation - I really don't feel like looking up MLA rules or whatnot.)
Arenamontanus Arenamontanus's picture
Re: ETP - Experience the Planets
One way of thinking about the Roche limit is that the tidal force on the side of the moon that faces the planet (and on the opposite side) becomes larger than the moon's gravity. So pieces start to fall off. The reason orbital direction matters for speeding up or slowing down moons is that they cause a bulge on the planet by tidal forces. That bulge might be moved ahead of them by rotation, in which case it drags the moon with it (weakly slowing the rotation of the planet and moving the moon to a higher orbit, the case we have in the Earth-Moon system), or it might lag and hence drag the moon to a lower orbit (where the forces are stronger, accelerating the process). In reality things get complicated by the oblateness of planets and other small factors.
Extropian