Solar System Grade 4 my daughters 4th grade science project solar system Solar 4 System Grade
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Looking inward from Triton, there are seven regular moons, all of which display prograde orbits in planes that are situated close to Neptune's equitorial plane, and some of these small moons orbit within Neptune's rings. It is thought that these seven small moons were re-accreted from the rubble ring that formed after Neptune snared Triton. This would have occurred some time after Triton's orbit had become circular. In addition, Neptune is circled by six more outer irregular moons other than Triton, including Nereid, whose orbits are considerably farther from Neptune and at high inclination: A trio of these moons sport prograde orbits, while the remainder have retrograde orbits. Indeed, Nereid has an unusually close and eccentric orbit for an irregular moon. This suggests that Nereid may have once been a regular moon that was badly disturbed and nudged into its current position when Triton was snared by Neptune's gravity. The duo of outermost Neptunian irregular moons, Psamathe and Neso, have the largest orbits of any natural satellites known in our Solar System to date.
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Dr. Le Gall and her team used the newly acquired depth-sounding information in order to separate the contributions made to the sea's detected temperature by the liquid sea and the seabed, which provided new insights into their compositions.
The inner Solar System is dramatically different from the distant realm of the giant planets. The inner region of our Solar System, where our Earth is situated, is almost entirely moon-less. Of the four relatively small, rocky worlds--Mercury, Venus, our Earth, and Mars--Mercury and Venus are barren of moons, and Mars is orbited by two fascinating, but very small, potato-shaped moons named Phobos and Deimos. The duo of Martian moons are often considered to be captured asteroids that long ago escaped from their birthplace in the Main Asteroid Belt between Mars and Jupiter. According to this scenario, Phobos and Deimos, during their dangerous journey from their original home, were snared by the gravity of their adopted Red Planet when our 4.56 billion-year-old Solar System was young. In the warm and well-lit inner Solar System, only Earth's large Moon is a significant moon-world in its own right.
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The crust of Earth's Moon is 43 miles thick on the near-side hemisphere, and 93 miles on the far-side. It is composed of silicon, magnesium, oxygen, calcium, aluminum, and iron. There are also trace amounts of titanium, uranium, thorium, hydrogen, and potassium.
In order to shed new light on the mysterious origins of the surviving duo of Martian moons, the researchers conducting this study combined their expertise in astrophysics, planetary science, computer science, and mathematics in order to create complex supercomputer models. The models ran a range of hydrodynamic and numerical simulations able to recreate the sequence of ancient events. Their findings strengthen the hypothesis that a horrific blast in the past formed the moons of Mars--originally a collection of moons and moonlets.
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.