Ptolemaic Solar System ptolemaic model science learning hub System Solar Ptolemaic

Ptolemaic Solar System ptolemaic model science learning hub System Solar Ptolemaic

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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

For this reason, for many years astronomers considered the possibility that hydrocarbon lakes and seas might exist on this fantastic moon-world. Data that finally arrived courtesy of the joint NASA and European Space Agency's (ESA's) Cassini-Huygens mission lived up to their expectations. Since arriving at the Saturn system in 2004, the Cassini spacecraft has revealed more than 620,000 square miles of Titan's long-hidden, bewildering surface--and it has shown that almost two percent of Titan's entire surface is covered in liquid.



and finally

The new study is based on data gathered by Cassini's radar instrument during flybys of Titan between 2007 and 2015.

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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.



Mars may be circled by many moons smaller than 160 to 330 feet in diameter, and a ring of dust has been predicted to circle Mars between Phobos and Deimos.



Saturn is the smaller of the two gas-giant planets dwelling in the outer regions of our Solar System, far from the friendly light and warmth of our incandescent golden Star, the Sun. The larger of the two gas-giants is Jupiter, which is also the largest planet in our Solar System. Some scientists think that the two gas giants do not have solid surfaces hidden beneath their immense and heavy gaseous envelopes, although others think that they probably do contain relatively small cores of rocky-icy material. The two other large denizens of the outer limits of our Sun's family are Uranus and Neptune, which are classified as ice-giants, because they have large icy cores buried beneath their heavy atmospheres which, though massive, are not nearly as heavy as the gaseous atmospheres borne by the two gas-giants.