Solar Nebula Research Paper

The Standard Model of particle physics is a theory concerning the electromagnetic, weak and strong forces, as well as classifying all the subatomic particles known. It was developed as a collaborative effort of scientists around the world during the latter half of the 20th century. Because of its success in explaining wide variety of experimental results, the Standard Model is often referred to as a "theory of almost everything". Although the Standard Model is quite consistent, it does not address some profound questions about the nature of the universe and it does leave some phenomena unexplained. One of these phenomena that the Standard Model doesn't explain is gravity. (CERN, 2015)

no one is really sure what causes gravity, but the effects have been studied by many

Gravity and centripetal force are fighting against each other to maintain celestial bodies in an orbit around the Sun. The 1% of the mass in our Solar System that didn’t get sucked into the Sun is what makes up our planets, asteroids, and moons. The centripetal force acting on the planets aligns them with the Sun’s equator and creates the mostly flat orbit of the Solar System.

The Earth revolves around the sun due to the gravitational force between them, so the Earth is pulled by the gravitation between it and the Sun. The Sun moves in an orbit as well due to the same gravitational force between it and the planet, which is the same as in real life. Also, the Moon revolves around the Earth like the moon revolves around the planet. It can be observed that the moon moves faster when the planet (Earth) is closer to the sun. This can be confirmed using Kepler’s Second Law (Equal Areas) because it states that the speed of the planet constantly changes and becomes faster when it is closer to the sun because it is in an elliptical

The cloud would spin around space. A nearby star had exploded causing the cloud to shrink. A mass formed in the middle of gas. The mass became known as the Sun. Gas and clouds around the Sun created whirlpools. As the whirlpools spun it created masses around the Sun. This became known as the planets, which created the Solar System.

8. Gravity is the force that is keeping the asteroid in orbit around the sun. The force of gravity will pull the asteroid inward, but because the asteroid is constantly moving forward- it is sort of a constant state of perfectly balanced tug-of-war.

First, Sir Isaac Newton discovered gravity after observing an apple fall to the ground. However, one of his most notable contributions is not the discovery of gravity but his discovery that gravitation is universal. The force of gravitational attraction is directly dependent upon the masses of both objects and inversely proportional to the square of the distance that separates their centers.

Before Newton talked about gravitation the main knowledge of scientists was a elementary knowledge of optics, mechanics and astronomy.Copernicus Kepler and Galileo provided the background knowledge of the stars and planets, but Newton used their data to discover the whole gravitational system.10Newton reasoned that the planets and all other physical objects in the universe moved through mutual attraction of gravity.Newton said that every other object in the universe affected every other object through gravity.This explained why the planets move in an orderly fashion. Newton found that “the force of gravity towards the whole planet did arise from and was compounded of the forces of gravity towards all it’s parts, and towards every one part was in the inverse proportion of the squares of the distances from this part.”Newton proves all of this mathematically. This was known to be the single most important contribution to physics that ever has been made.11

Discoveries of what were termed “nebulae” began in the early 17th century. The first of these discoveries was the Orion Nebula, which looked like a normal star to the naked eye. French scholar Peiresc discovered it in 1610 using one of the first telescopes to be made. Later, in 1656, Christiaan Huygens observed the interior of the Orion Nebula and determined that it consisted of a compact quadruple star system instead of a singular star. During the 18th and 19th century, nebulas were discovered even though astronomers were mainly scanning the sky for comets. Some major astronomers who contributed greatly to the discovery of nebulas, among other things, during the 18th and 19th century were Messier and the Herschel family. Though the instrumentation available to astronomers during the 18th and 19th century were highly advanced compared to earlier times, they weren’t advanced enough to detect the motion of extragalactic objects or their composition. This lack of precision instrumentation, and thus the dissociation from motion of stars/star-clusters/nebulae, were the main reasons astronomers during this

Gravity is the force which attracts an object to the center of the earth, and toward any other physical object having mass. Issac Newton and Albert Einstein both contributed to today's knowledge of gravity.Newton started working in 1687 by scratch, he knew nothing about gravity it until he saw an apple fall. Newton dint have much friends growing up because he would lock himself in his room and brainstorming ideas about how gravity could work. A few decades later Einstein started brainstorming off Newtons work to get an even better understanding of it.

Several unresolved problems remain concerning the Orion Nebula. The fate of the protoplanetary disks, for example, is presently impossible to predict. Without a more detailed understanding of how planets actually form, it cannot be assumed that the events within the Orion Nebula are analogous to the events that led to the formation of the planets in the solar system. Furthermore, the detection of water in the nebula has revealed the need to revise the theory of star formation to

The Carina Nebula is located in the Milky Way Galaxy in the constellation Carina in the Carina-Sagittarius Arm. It is sometimes referred to as the Eta Argus, referencing the former constellation, Argo Navis, which represented Jason and the Argonauts. It has been estimated at around 7500 ly (light-years) from earth. It was discovered in 1751-52 by Nicolas Louis de Lacaille and was later found to be one of the largest emission stars in the galaxy. Its entire mass is around 900,000 solar masses which is equivalent to 270 million pounds. It contains several open clusters of stars along with many O-type stars. It used to contain thousands of more stars than it does today, but many self-destructed. It is home to the Trumpler 14 and Trumpler 16

Within the constellation of Orion is what appears to the human eye as a hazy star, but is in fact the Orion Nebula, a cosmic cloud composed of dust and brightly glowing gas around 20-30 light years in diameter. This nebula, often called M42 or NGC 1976, is one of the most studied stellar ‘nurseries’ and is located in the Orion constellation, a part of the ‘sword’ hanging from the three-starred ‘belt,’ approximately 1,500 light years away from Earth.

Throughout the universe, there are dense molecular or dust clouds, known as interstellar clouds, and they are the first stage of a star. These clouds are incredibly large, containing thousands of times the mass of the Sun, and while they start out stable, for them to one day become a star, they must become unstable. Once this happens, they are no longer able to withstand their own gravity and they break into smaller pieces. The trigger for these events are still unknown, but astronomers think it is caused by some external event that forces the cloud to the next stage: cloud fragments.

[And that defines North, South Polls of the magnet, and Head to Feet are in equal ratio with Sky, Earth, and States: Gravity, levity gravity force toward the earth toward and levity force toward the sky example Smock, Gases and Time Space