A History of the Orion Neblua

1716 Words4 Pages
bulb-icon

Recommended: Formation of planets in from nebula

A nebula is a space dust that appears as a hazy bright, colorful patch in the sky. The Orion Nebula goes way back from millions of years ago and is made up of mostly hydrogen, but also helium, carbon, nitrogen, and oxygen (Wiley 1). The Orion Nebula is also known as M42, Messier 42, and NGC 1976 (Ivan P. 1). Even though the Orion Nebula may have a giant black hole in the middle of it, The Orion Nebula is still the brightest nebulae because it can be seen with the naked eye during certain times of the year and has the three brightest stars in it.
The Orion Nebula is not a difficult nebulae to find. It can be seen best during the colder months of January and February (Ivan P. 1). It is one of the many more noticeable star patterns in the sky during the winter (Franknoi 1). The three stars in it's center make it easier to find than most (Franknoi 1). If you live in the Northern Hemisphere, you can find the Orion Nebula in the southwest sky between Latitudes 86 and -75 degrees (Ivan P. 1). The Orion Nebula is 1,270 light years away from the earth (Fuller 1). The Orion Nebula is also between Jupiter and the brightest star, Sirius (Fuller 1). The Orion Nebula is fourteen light-years across (Ivan P. 1). If you really want to see the Orion Nebula up close then you need to use the Hubble Space Telescope to view it (Fuller 1). Since the Orion Nebula is so easy to find, it is a useful aid in finding other stars surrounding it including Sirius, Aldebaran, and Procyon (Garza 1). The Orion Nebula was also one of the first nebulae to be photographed (Britannica 1). Henry Drapper was the photographer and took the photograph in 1880 (Britannica 1).
The Orion Nebula originated from the Greeks. Orion has always been associated with mythology (I...

... middle of paper ...

...'s Sharpest View of the Orion Nebula." Www.spacetelescope.org. NASA, 2004. Web. 27 Mar. 2014. .
Templeton, Matthew. "Trapezium, BM Orionis, and Young Stellar Objects." Www.aavos.org/vsots_bmori. N.p., 4 Apr. 2012. Web. 24 Mar. 2014. .
Than, Ker. "The Splendor of Orion: A Star Factory Unveiled." Space.com. N.p., 11 Jan. 2006. Web. 25 Mar. 2014. .
Wiley, John. "Taking a Shine to Nebulae." Www.dummies.com/how-to/content/taking-a-shine-to-nebulae.html. N.p., 2014. Web. 27 Mar. 2014. .
Zimmerman, Kim Ann. "Orion Constellation: Facts About the Hunter." Space.com. N.p., 19 July 2012. Web. 26 Mar. 2014. .

Show More
Related

  • An Analysis of Robert Ji-Song Ku's Leda

    1958 Words  | 4 Pages

    "Leda and the Constellation Cygnus." Department of Engineering, University of Michigan. 17 February 1999 http://windows.ivv.nasa.gov/mythology/cygnus.html.

    Read More

  • Lagoon Nebula Essay

    886 Words  | 2 Pages

    The Lagoon Nebula featured as Nasa’s astronomy picture of the day was photographed by John Nemcik using various filters to capture the light emitted by the Hydrogen, Sulfur, and Oxygen. While photographed showing beautiful vibrant, eye-catching colors, the Nebula would appear naturally appear gray to human eye due to poor color sensitivity existing at low-light levels (spacetelescope.org). The Lagoon Nebula is home to the formation of new stars, as well as several other interesting phenomena such as Bok globules, and the hourglass nebula. It is these regions of the nebula that make it a continuous area of interest and study for astronomers.

    Read More

  • Night Sky Research Paper

    835 Words  | 2 Pages

    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.

    Read More

  • The Lady of Luminosity: Henrietta Swan Leavitt

    1178 Words  | 3 Pages

    Waller, William H. The Milky Way: An Insider's Guide. Princeton, N.J: Princeton UP, 2013. 42+. Print.

    Read More

  • The Importance Of God In 'The Star'

    977 Words  | 2 Pages

    Nebula away so that it can avoid certain things. In the short story, “The Star,” the priest stated,

    Read More

  • Black Holes

    1549 Words  | 4 Pages

    2, Alter Dinsmore, Cleminshaw H. Clarence, Philips G John. Pictorial Astronomy. United States: Sidney Feinberg, 1963.

    Read More

  • Solar Nebula Cause Planet Formation

    532 Words  | 2 Pages

    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.

    Read More

  • Cosmic Life and Death of a Star

    1612 Words  | 4 Pages

    If the nebula is dense enough, certain regions of it will begin to gravitationally collapse after being disturbed. As it collapses the particles begin to move more rapidly, which on a molecular level is actually heat, and photons are emitted that drive off the remaining dust and gas. Once the cloud has collapsed enough to cause the core temperature to reach ten-million degrees Celsius, nuclear fusion starts in its core and this ball of gas and dust is now a star. It begins its life as a main sequence star and little does it know its entire life has already been predetermined.

    Read More

  • Stellar Evolution

    2295 Words  | 5 Pages

    Shklovskii, Iosif S. Stars: Their Birth, Life, and Death. Moscow: Central Press for Literature in Physics and Mathematics, 1975.

    Read More

  • Solar Nebular Hypothesis

    313 Words  | 1 Pages

    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.

    Read More

  • Story Of Orion Research Paper

    789 Words  | 2 Pages

    His left foot is formed by Saiph and the right formed by Rigel. In order from left to right, Orion’s belt is made from the stars of Alnitak, Alnilam,and Mintaka. These are important stars that make out the shape of the constellation Orion the

    Read More

  • The Hydra

    675 Words  | 2 Pages

    ...s one of the oldest and most original constellations there can be dating back to Ptolemy and the times of the ancient Greeks.

    Read More

  • The Milky Way Galaxy

    1798 Words  | 4 Pages

    The first person to ever observe the Milky Way was Greek philosopher, Democritus, who said the galaxy may consist of distant stars. In 1610, Galileo Galilei used a telescope to study the Milky Way and came to the conclusion that it was composed of billions and billions of faint stars. Then, in 1750, Thomas Wright c...

    Read More

  • Essay On Nebulae

    640 Words  | 2 Pages

    Nebulae are cosmic clouds of dust and gas floating in space. The word nebula is Latin and means cloud. Originally the word nebula referred to any extended astronomical object, not including comets, planets, or satellites. But over time the word nebula became reduced to mean interstellar cloud of dust and gas. Calling it that does not do a nebula justice. Most nebulae are commonly made up of hydrogen and helium gasses, dust, and plasma. Nebulae are the building blocks of our universe; they contain all the things stars need to form. Scientists classify nebulae in to one of two major categories; bright and dark. From there they narrow it down more to planetary nebulae, emission nebulae, reflection nebulae, dark nebulae, and supernova remnants. Bright nebulae are close enough to stars to glow, and dark nebulae are to far away from stars to do so. Dark nebulae are only visible if a star cluster or other bright object provides a backdrop. Sometimes they are part of a bright nebula. A good example of this phenomenon would be the Trifid Nebula. It is a bright nebula divided into three sections by dark “alleys” spanning across it. Getting down into the smaller categories, planetary nebulae form when a star cannot support itself by fusion reactions in its center. Gravity forces the outer layers of the sun in on its core, making the insides heat up and condense. The heat from the center blows the outsides away in a stellar wind over a few thousand years. When the star finishes the only thing left of it is the core. The core then heats the distant gasses and they glow because of this. Despite planetary nebula being called planetary nebula, planets have nothing to do with them. They are a very common nebula in our galaxy, as there are an es...

    Read More

  • Orion: Orion The Star

    703 Words  | 2 Pages

    The great Orion Nebula lies just in front of the Orion Molecular Cloud, a particularly active source of star birth. The Hubble Space Telescope has imaged many proto-planetary disks around the stars forming there. The Orion Nebula is visible to the unaided eye in the region just below Orion's belt, often referred to as Orion's sword. Binoculars or a small telescope can reveal the true splendor of the Orion Nebula. Brightly glowing clouds surround the Trapezium, a dense multiple star recently born within the nebula. The Trapezium forms the center of a star cluster that may include more than 300 young stars. Closer to the belt, there lies one of Orion's most famous features, the Horsehead Nebula. It is difficult to observe, however, without a high-power telescope, and unless specific viewing conditions are

    Read More

More about A History of the Orion Neblua

Open Document