How Does Gravity Affect The Formation Of The Solar System

The study of Kuiper Belt will likely continue to provide more information on how our solar system was formed and its origins. The material in the Kuiper Belt are what’s left over after the rocks, dust and gas pulled together form

Jupiter is a VERY important planet. Not only does is it the biggest planet in our solar system, but it keeps thousands of minor planets in their orbits. There is a family of minor planets (or asteroids) in the same plane as Jupiter. These are called Trojan asteroids. Scientists have divided these into two groups the “Greeks” and the “Trojans”. The “Greeks” come before Jupiter and the “Trojans” follow Jupiter. These asteroids are as far away from Jupiter as they are from the sun; because of this they stay and will continue to stay in the positions they are in because the gravitational pull from Jupiter and the sun are the same.

the planets fall around the Sun. Each of these objects balances the Sun 's force of gravity

Although all nine planets are a huge part of the solar system there's a lot more to the solar system than the nine planets. According to scientist the Solar System started out as an enormous cloud of gas and dust. Scientist believe that the cloud of dust and gas began to collapse under the weight of its own gravity and it did. The matter that was kept within itself began moving in a giant circle and at the center of the spinning cloud a tiny star began to form. The star eventually grew larger and collected more dust and gas that collapsed into it. Farther from the center of the mass that was being formed there was many smaller clumps of dust and gas that were also collapsing. The large cloud in the center eventually became the sun while the smaller clumps formed the planets, moons, comets and,

In inspiring people to have the passion in understanding the universal laws that govern us all, Professor Stephen Hawking reminds us on his speech for his 70th birthday to “remember to look up at the stars and not down at your feet” (enoch, 2012). Many scientists have been “looking up” and have discovered answers to the many questions that we have of the universe for ages. They have constructed theories, launched satellites, observed stellar phenomena, and even sent living beings in space to gain more understanding of the existence of everything. After centuries of research and observation, there are still some aspects of Astronomy that are still to be explored. One of them is the evolution of the Solar System, which is composed of the Sun and everything that travels around it. This includes eight planets and their natural satellites such as the Earth’s moon; dwarf planets such as Pluto and Ceres; asteroids; comets and meteoroids (Solar System Exploration, 2014). The Solar System is located in the Milky Way Galaxy, which is a part of a galactic group under the Virgo Supercluster. Figure 1 shows the location of our Solar System in the Universe. Many theories have been proposed on how the Solar System existed, but none has been completely successful. This spans from the time of the Ancient Greeks to the present 21st Century. As of now, the widely accepted theory is the Nebular Theory, which describes how the Solar System started as a large cloud of gas that contracted under

The Kuiper Belt is a ‘belt-like’ disc in our outer Solar System that extends from the orbit of Neptune at about 30 astronomical units (AU) from the Sun to approximately 50 AU [1]. It is like a larger version of the asteroid belt, and is mostly made up of remnants of the formation of our Solar system [2]. As the Kuiper Belt gets further away from the Sun, it also becomes denser. At its section that should be the densest it instead stops suddenly, and this abrupt ending is known as the Kuiper Cliff. The reason for this dramatic falloff is thus unknown [3], but there is one interesting theory. Patryk Lykawka of Kobe University claims that the gravitational pull of a so far unseen planet may be responsible for the behavior of the Kuiper Belt.

The solar system was believed to be formed when a gas cloud and dust in space was disturbed by the explosion of the supernova. The explosion made space waves which squeezed in the cloud of the dust. The Jovian planets include Jupiter, Saturn, Uranus and Neptune. These planets surfaces are not solid. Jovian’s atmosphere in our solar system is mostly made of helium and hydrogen.

Pluto orbits around the sun, all the other planets orbit around the sun. Pluto is large enough to be rounded by its own gravity, all tho it is small still has its self gravity. Pluto is part of History, I think kids should learn about Pluto in school so that is why pluto is part of history. People are pretty much discriminating Pluto. I am hoping to revise Pluto’s extinction.

After several hundreds of millions of years of slow, gradual migration, Jupiter and Saturn, the two inmost giant planets, crossed their mutual 1:2 mean-motion resonance of orbital motion. This resonance increased their orbital eccentricities to such an extent, that it destabilized the entire planetary system. The arrangement of the giant planets altered quickly and very radically. Jupiter shifted Saturn out towards its present position, and this relocation caused mutual gravitational encounters between Saturn and the two ice giants, which subsequently propelled the planets Neptune and Uranus onto much more eccentric orbits. These ice giants then ploughed into the planetesimal disk, scattering tens of thousands of planetesimals from their formerly stable orbits in the outer Solar System. This disruption almost entirely scatters the primordial disk, removing almost 99% of its mass, a scenario which explains the modern-day absence of a dense trans-Neptunian population. Some of the planetesimals were thrown into the inner Solar System, producing a sudden influx of impacts on the terrestrial planets: yes! It is the Late Heavy

Scientists have been researching about outer space for years but still don’t know as much as one may think. Scientists still do not know much about the early solar system. Scientists believed that the solar system was reshuffled around in the past which would explain the Kuiper belt and the Oort cloud of icy bodies, the inner planets being destroyed by asteroids and why there isn’t any super Earths around in this solar system. But scientists recently discovered something that may change their theory. In Michael D. Lemonick’s “Plant Nine from Outer Space,” Lemonick claims that scientists may have found a planet with ten times the mass of Earth that is beyond Pluto and may be the reason why objects from the Kuiper belt are following similar orbits

The nebular hypothesis stating a cloud of dust condensed to the solar system. Next, the protoplanet stating that as the cloud cold it created and formed “whirlpools” to form planets. After that the planetesimal hypothesis states another the planets formed from chunks of the Sun. Each of these hypothesis have problems with them that hinders the status of theory. Plus, each of these have similarities and differences with each other. These hypotheses lead to discussion and resource to prove which one is

7. The inner solar system does not have room for any more planets without chaos taking place. Scientists believe that the solar system is “marginally stable.” Our planets tug on one another, producing a resonance on their orbits. Over time, these resonances have most likely caused collisions between the planets and small debris, which actually helped the planets to clear out their orbital spaces. However, if you were to squeeze in another planet in the inner solar system, the current “stability” would be thrown off, possibly leading to a collision between the planets. The system has basically found a sort of balance over millions of years, and adding another planet would drastically alter that.

Uncovering the mysteries of Jupiter is a crucial step for a greater understanding of our Solar System. Being the massive planet that it is, this mysterious planet may hold many answers to how our the Solar System formed and evolved. The understanding of the origins of the universe includes answers even to the formation of Earth itself. Many believe that the research of Jupiter will lead to discoveries on planet formation and the role of giant planets on the formation f stars and other smaller bodies. Mysteries of Jupiter include its composition, what is under its clouds, what is in its core and its magnetic field. Research on the amount of water in the planet will tell us about the

The terrestrial planets are Mercury, Venus, Earth, and Mars. These four planets are the planets that are closest to the sun. Terrestrial means earthlike; therefore, these planets are all earthlike because they have a solid ground. The terrestrial planets are the middle school years. The knowledge learned here orbits the sun. If the knowledge learned at the sun is not retained, a student may have a

Formally, classified natural satellites or moons include 176 planetary satellites orbiting six of the eight planets. Of the inner planets, Mercury and Venus have no natural satellites; Earth has one large natural satellite, known as the Moon; and Mars has two tiny natural satellites, Phobos and Deimos. The large gas giant planets have extensive systems of natural satellites, including half a dozen comparable in size to Earth 's Moon. The objects in the solar system are classified foremost by their dynamics and motion, while size and composition are important for secondary classification. The solar system itself is, defined by the orbits of its constituent bodies. Classification by motion is more useful for astronomers. In fact, the dynamics of the solar system were a central issue for early astronomers such as Ptolemy in the second century and Nicholaus Copernicus in the 16th century. In what follows, we introduce different classifications of the planetary moons.