Solar System - Science Olympiad Exam Questions And Answers (Verified And Updated)

Solar System - Science Olympiad Exam Questions And Answers (Verified And Updated) How did the terrestrial planets form? - answerIn the proto-Solar-Sytem, after the sun formed, the rest of the materials orbiting close around it began to clump together too. However, closer to the sun, lighter materials like gases blew away and only rocky material was left, causing the four terrestrial planets, and some of their moons, to form. What are the characteristics of Terrestrial Planets? - answerSolid bodies with a core surrounded by a mantle and crust. Comprised mostly of heavier materials, like rocks, stones, and heavy metals like nickel and iron. They are smaller in size than the gas giants and very dense in comparison. How old is the Solar System? - answer4.6 billion years. How did Mercury form? - answerLike the rest of the terrestrial planets, Mercury was formed 4.55 billion years ago and is primarily rocky. After the sun's formation, the rocks and metals very close it it began to come together to form Mercury. However, all of Mercury's gases and atmosphere were blown away, leading to it being small, but even more rocky than the other planets. How did Venus form? - answerVenus, like Mercury, was formed by rocks and metals coming together to form a large planet. However, solar winds are too weak to blow away Venus' atmosphere, and the heat has led to a greenhouse gas effect, causing the planet to be especially hot, even more so than Mercury, though being further away. How did Earth form? - answerEarth formed in the same way as the rest of the terrestrial planets. However, another large body slammed into Earth (which used to be larger) and the material from that body and the chunk of Earth blown off formed the moon, which is why is has such a large size in comparison to Earth. How did Mars form? - answerMars was most likely very similar to Earth, and it had formed the same way as well. It possibly even had large oceans. However, for unknown reasons, they have dried up, leading to Mars' nickname as "The Red Planet." How did the Moon form? - answerLong ago, when the Earth was younger, and larger, another body slammed into it. This body blew into pieces that began to orbit the Earth, along with chunks of Earth blown off from the impact. Together, these formed the Moon, being responsible for its relatively large size. What are the surface features of Mercury? - answerMercury's surface is made of volcanic basalt (a hint towards prior geologic activity) and is very smooth. However, Mercury has a no real atmosphere, allowing almost any incoming asteroids to impact, though they are stopped by it's thick mantle. As a result, Mercury looks like a smooth, dark grey planet peppered with large and small round imprints. Mercury also has ridges all across it's surface. As the magma on Mercury cools, it shrinks, since solids are more compact than liquids. Mercury's surface is also made up of intercrater plains, accounting for almost half of the planet's surface area. Intercrater plains are made up of flatter lands containing older more shallow craters, while smooth plains are made up of newer land and more recent deeper craters. Smooth plains make up around 15% of mercury's surface What are the internal features of Mercury? - answerMercury has an extremely large core relative to its size. The core is mostly iron and iron compounds and is about 1800 km in diameter. The mantle and crust are only 600 km in Diameter, and are mostly silicates. This is because the temperature of the early son evaporated and destroyed a large portion of the rocky material, causing the core to be larger than it normally would be, as it is the size of a core in what would be a much larger planet. The core seems to have a liquid outer core and superdense solid liquid core. Features to look for in identifying Mercury? - answerDark Grey surface, round, shallow imprints into the surface, a relatively smooth surface, a relatively large core of iron and iron compounds, and a planet about 2500 km in diameter. Surface features of Venus? - answerVenus' surface appears red due to the carbon dioxide in the atmosphere, but its surface is covered in lava from volcanic activity, basaltic rocks, and sulfuric acid. It has very few craters, since the extremely heavy atmosphere destroys any craters that would impact. Only strong asteroids can survive, of which there are very few. There are two "continents"- Ishtar Terra and Aphrodite Terra. These are the few parts of Venus with solid land, and are made of mostly rough, patchy rocks with valleys and canyons. The rest of the surface is mostly melted rock- lava and magma. Internal features of Venus'? - answerVenus' internal surface is mostly normal, with a metallic core, rocky mantle and crust. However, about 300-500 million years ago, there seems to have been a "resurfacing" in which large amounts of magma rose from the mantle to the surface, causing "lava oceans" along the surface. Features to look for to identify Venus? - answerBright orange or red surface, lava oceans, a pinkish, tan, atmosphere, few craters due to an atmosphere, about 38,000 km in circumference. There are two continents on the planet, made of rough, patchy soil. A large belt of lava surrounding the planet.