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A little interesting about space life.
The spacecraft Voyager 2 flew past Uranus in 1986, and Neptune in 1989. Voyager 2 sent back images of Neptune to Earth that revealed a strikingly beautiful deep blue planet, that sported stripes and bands, and spot-like storms akin to hurricanes. Neptune's bands and spots are different shades of blue--and these lovely shades of blue are caused by atmospheric methane, not oxygen. Some of Neptune's frothy storms are white, and look like whirling marshmallows.
and here is another
Saturn, along with its frozen retinue of icy rings, dazzling moons, and sparkling moonlets, orbits our Sun about ten times farther out than the Earth. Astronomers received their first collection of detailed data about Titan when the Cassini/Huygens orbiter and lander arrived there in 2004. The Huygens lander successfully obtained revealing images when it drifted down to Titan's tormented, hydrocarbon-slashed surface, as well as when it was still floating slowly and softly down through the moon's thick, foggy, orange atmosphere--which has 1.4 times greater pressure than that of our own planet. These pictures, when combined with other studies using instruments aboard the Cassini orbiter, reveal to curious planetary scientists that Titan's geological features include lakes and river channels filled with methane, ethane, and propane. Titan's strange surface also shows mountains and sand dunes--and it is pockmarked by craters. The rippling dunes form when fierce winds sweep up loose particles from the surface and then tosses them downwind. However, the sands of Titan are not like the sands on our Earth. Titan's "sand" is both bizarre and alien, probably composed of very small particles of solid hydrocarbons--or, possibly, ice imprisoned within hydrocarbons--with a density of about one-third that of the sand on our own planet. Furthermore, Titan's gravity is low. In fact, it is only approximately one-seventh that of Earth. This means that, working in combination with the low density of Titan's sand particles, they carry only the small weight of a mere four percent that of terrestrial sand. Titan's "sand" is about the same light-weight as freeze-dried grains of coffee!
Some of the images focus on the shallow center of a bizarre impact crater dubbed Pwyll. Impact rays and shattered pieces of material scattered over an immense area of the moon tell the tale of a sizeable meteorite that collided violently with Europa relatively recently--"only" about 10 to 100 million years ago. There is also darker debris chaotically scattered around Pwyll. This further suggests that the large crashing meteorite may have dug up some deeply buried material, and tossed it helter-skelter around the crater.
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The team further ascertained the presence of the enormous, embedded lake by drawing a connection between processes seen on Europa and processes seen on our own planet. Ice-piercing radar, that can delve through thick layers of ice sheets, has been used to locate numerous subglacial lakes in Antarctica.
The efforts of planetary scientists to determine the lunar birthday have suggested a range of ages. Some have proposed an early event, about 30 million years after our Solar System formed, while others suggested that it occurred over 50 million years and perhaps as much as 100 million years after our Sun's family took shape.
Full Moon Experienced Through Outer Senses. Now we need to become skilled in how to welcome and embrace the Moon Goddess's moonbeams. Whereas before, what was thought to be the most important, was just the Full Moon as that's what we could see with our outer senses.