A very small solar system body made mostly of ices mixed with smaller amounts of dust and rock. Most comets are no larger than a few kilometers across.the main body of the comet is called the nucleus, and it can contain water, methane, nitrogen, and other ices. When a comet is heated by the sun, its ices began to melt off. The mixture of ice crystals and dust blows away from the comet nucleus in the solar wind, creating a pair of tails. The dust tail is what we usually see when we view comets from earth. The tail happens when gas molecules interact with the solar wind. The tail is not usually seen by the naked eye but can be imaged. Comets normally orbit around the sun and have come from the further outer solar system.The nucleus of a comet
Brian Doyle’s, “The Meteorites” was a short essay about a camp counselor and his unforgettable summer. Doyle uses very poignant arguments to explain his love for his campers. Each camper is introduced with a short synopsis, allowing the reader to get a feeling for what the children are like. The counselor was in charge of a flock of 5-6 year olds. The second paragraph introduces the main argument: how this summer camp made him love the boys as if they were his own. The paragraph goes continues the counselor is pulled aside by one of the shyest and quietest that was speaking up for the most outspoken of the group. He was asking for help because one David (outspoken on) had an accident in his pants and needed to be clean. This puzzled the
A comet is a small icy body that travels in an elliptical orbit around the sun. Halley’s Comet, or 1P/Halley, is the most well-known “periodic” comet that orbits the solar system and returns to Earth’s vicinity approximately every seventy-six years. It is one of the only comets that can be seen from Earth that is visible to the naked-eye, and can appear twice in one’s lifetime. The comet’s last visit was in the year 1986, and it is calculated to return mid-2061.
Our Solar System was formed approximately 4.6 billion years ago during the Big Bang with the collapse of an interstellar body (Lammer et al., 2009). During these supernova explosions, the dusts and gases that were expelled were mixed and processed to form the planets of our system (Lammer et al., 2009, Nisbet and Sleep, 2001).
The Kuiper Belt is an icy-bodied disc shapes area of the Solar System. Kuiper Belt has a circular shape, to be exact, it is a curved plane. It is over 4.5 to 7.4 billion kilometers from Sun. This is roughly 30 to 50 times the distance of Earth from Sun. The Kuiper Belt has been said to resemble the Asteroid Belt that lies between Mars and Jupiter. The difference between the Kuiper Belt and the Asteroid Belt is that the bodies are icier due to their distance from the Sun. The Kuiper Belt objects includes Pluto and other comets that orbit beyond Neptune. Most Kuiper Belt objects are made up of frozen volatiles such as methane, water and ammonia. In 1950 astronomer Gerald Kuiper predicted the existence of the Kuiper Belt and the find was named
Halley’s Comet or Comet Halley is a comet who orbits earth every 74.5 years! This comet is also the most known comet ever to be documented! Halley is very interesting comet.
This paper is an overview of the Kepler spacecraft and its mission in space. According to the National Aeronautics and Space Association (NASA), Kepler, named after Renaissance astronomer Johannes Kepler, “is a space observatory launched…to discover Earth-like planets orbiting other stars.” Kepler does this by searching for planets within our galaxy that have a similar size to Earth within a habitable zone. A habitable zone is a distance between the planet and its star where water can exist on the planet’s surface. Additionally, Kepler is aimed at searching for planets with similar one-year orbits like that of Earth. As technology advances on Earth, increased standards of living and life expectancies have taken a toll on Earth’s fleeting, finite resources. Kepler potentially provides scientists with information regarding planets that can serve as a future home when resources have diminished and information that can foreshadow inevitabilities about Earth through older, Earth-like planets.
The universe is a shooting gallery and earth is the bullseye. The earth is always under threat of a doomesday asteroid that will wipe out civilization. There are over one thousand asteroids traveling toward earth and only three quarters are accounted for. Where are the other one forth? No one knows because the government doesn't fund NASA astrologists enough to cover the astroids. Just one impact could end civilization as we know it. No matter where it hits everything would die, even bacteria. To give an estimate how much is spent on asteroid detection. It is said to be less than the cost to operate a single McDonald's franchise. Total disaster would occur no matter where the asteroid hit. Land, sea it doesn't matter. Ocean impact would create a number of things. First, a Tsunami(tidal wave) would be created on impact. The wave would be hundreds for feet high traveling hundreds of miles per hour. It would start to slow down crashing ashore through all coastal city. Then, finally wash up hundreds for miles inland. " The mid-Atlantic Ocean impact ranging from 400 meters to 5 kilometers in diameter. This would generate a tsunami that would sweep across the upper East Coast of the United States to the Appalachian Mountains."(Gottschalk 1) The blast of the impact would equal a 300 gigaton blast of T.N.T. Also, 2.4 seconds after impact, a small fireball with a temperature of 5000'C would sweep across long island. A land fall strike would cause total divistation. The asteroid would create a earth trembling impact causing earth quakes around the world. The binding flash will show impact and the crater would be twenty miles across. Then, a blanket of dust and debris would blanket the earth and block the sun's light. This would occur for hundreds of years and the climate would be disrupted. Global killer no matter where it hits. The end of the world is only 28 years, 10 months, 19 days, 1 hour, 45 minutes, and 39 seconds away. An asteroid named XF11 is on route to hit earth directly. October is the month and 2038 is the year. Discovered by Jim Scotti on December 6, 1997 while looking at star with the Arizona Spacewatch Group. The asteroid "is predicted to pass at a rather comfortable distance of about 600,000 miles (about 960,000 kilometers) in 2028," "reported Dr. Donald K.
Jupiter is a very interesting planet. It is very much different from our planet Earth. Its days are a lot shorter than and Earth day. Then the years though are very long. The giant, Jupiter, is named after and old Greek god. Jupiter actually has rings, though very little. It is one of my favorite planet’s.
Solar nebula is a rotating flattened disk of gas and dust in which the outer part of the disk became planets while the center bulge part became the sun. Its inner part is hot, which is heated by a young sun and due to the impact of the gas falling on the disk during its collapse. However, the outer part is cold and far below the freezing point of water. In the solar nebula, the process of condensation occurs after enough cooling of solar nebula and results in the formation into a disk. Condensation is a process of cooling the gas and its molecules stick together to form liquid or solid particles. Therefore, condensation is the change from gas to liquid. In this process, the gas must cool below a critical temperature. Accretion is the process in which the tiny condensed particles from the nebula begin to stick together to form bigger pieces. Solar nebular theory explains the formation of the solar system. In the solar nebula, tiny grains stuck together and created bigger grains that grew into clumps, possibly held together by electrical forces similar to those that make lint stick to your clothes. Subsequent collisions, if not too violent, allowed these smaller particles to grow into objects ranging in size from millimeters to kilometers. These larger objects are called planetesimals. As planetesimals moved within the disk and collide with one another, planets formed. Because astronomers have no direct way to observe how the Solar System formed, they rely heavily on computer simulations to study that remote time. Computer simulations try to solve Newton’s laws of motion for the complex mix of dust and gas that we believe made up the solar nebula. Merging of the planetesimals increased their mass and thus their gravitational attraction. That, in turn, helped them grow even more massive by drawing planetesimals into clumps or rings around the sun. The process of planets building undergoes consumption of most of the planetesimals. Some survived planetesimals form small moons, asteroids, and comets. The leftover Rocky planetesimals that remained between Jupiter and Mars were stirred by Jupiter’s gravitational force. Therefore, these Rocky planetesimals are unable to assemble into a planet. These planetesimals are known as asteroids. Formation of solar system is explained by solar nebular theory. A rotating flat disk with center bulge is the solar nebula. The outer part of the disk becomes planets and the center bulge becomes the sun.
Comets and asteroids. They are some of the first celestial bodies that humans observed and truly thought about. From ancient cultures interpreting these near-Earth objects as signs of disaster, to 18th century Europeans studying their paths, to even the extinction of the dinosaurs, comets and asteroids have always been prevalent in the majority of Earth’s history. These objects have intrigued the human race for generations, and continue to do so today. These similar subjects of fascination have many unique and interesting characteristics and a rich history with Earth.
I was born with an inherent fascination for all things celestial. Ever since I was young, I have been staring at the night sky trying to find constellations, or using my juvenile imagination to create my own. My efforts to find, view, and mentally catalogue everything the heavenly bodies have to offer has led me to employ some over-the-top measures, but the most extreme of them all might be the night I stayed awake through the wee hours of the morning to catch a glimpse of a meteor shower. Over the course of an entire year, the memory of this stupefying event is still as lucent and vivid as it was that very night so long ago.
Imagine standing in the field with your friend looking at the stars, as the cool breeze blows through the group you see a white bright streak flying by. One of the voices says, “Hey! Its Halley’s Comet!” Now fast forward seventy-five years, as you sit on your porch with your wife you see a familiar looking streak cruising through the vast dark blue sky. You realise that Halley’s Comet has come back to say hello.
The last of the features of the comet are the tails. Most comets have two tails. One tail is made from dust particles and the other, called ion tail, is made gases. As a comet approaches the sun, the frozen gas becomes unfrozen which causes the dust particles to become free. Light pressure from the sun and some other forces cause these materials to move away from the head of the comet and in the opposite direction from the sun. According to Charles A. Schweighauser in his book, entitled Astronomy from A to Z: A Dictionary of Celestial Objects and Ideas, he states that we see comet heads and tails because they not only reflect sunlight, but they also fluoresce—give off their own light—when comets are near the sun. The tails from the comet may be up to 150 million kilometers long each or together.
Nuclear fusion occurs when two atomic nuclei collide with enough energy to bind together to form one nucleus. Nuclear fusion occurs in the core of our sun, and is the source of its tremendous heat. In the sun hydrogen nuclei, single protons, fuse together and form a new nucleus. In the conversion, a small amount of mass is converted into energy. It is this energy that heats the sun.
The idea behind the Solar Nebular Hypothesis is that the solar system was condensed from an enormous cloud of hydrogen, helium, and a few other elements and rocks. Around five billion years this cloud of materials began to spin and contract together into a disk shape under their own gravitational forces. The particles started combined together, protoplanets, to eventually form planets. A great mass of the material eventually began to form together, protosun, and make up the sun.