I have chosen this topic because I myself did not know much about Nebulas and Galaxies; I thought to myself, “It wouldn’t hurt to learn something new.” So, then I decided to write and read about nebulas and galaxies. There are things you may not know about galaxies and nebulas. You may have also thought of questions like, “why are nebulas and galaxies even important to your existence?”, or questions like, “how do they form?” There are many more questions and I might just answer most of your questions. Let’s just say that without galaxies, there would not be a Milky Way, and with-out the Milky Way the solar system would have probably ended up elsewhere. Moreover, galaxies are important to our existence due to the fact that the solar …show more content…
Nebulas and galaxies differ because, nebulas are clouds deep in space made of dirt or so called dust. Galaxies are groups of billions of stars, planets, dirt, and other matter put together by gravitational force people call gravity. Nebulae have many ways of forming in which galaxies do not. Nebulas come in galaxies, emission nebula, reflection nebula, planetary nebulae, dark nebulae, open clusters. As for galaxies come in spirals, irregular and elliptical shapes. Here are some examples of shapes and what they look …show more content…
Nebulas and galaxies are mainly something close to you educational worries. Galaxies are more important because, our solar system is part of a galaxy, and that galaxy is known as the Milky Way. There can be a possibility that new galaxies and nebulae could form and you may be a person whom would be there to see and experience what it may look like, what else it may have, may be new life. Therefore, I finish with a grand ending and I have now explained to you what these two wonderful things called nebulas and also galaxies are for and how they can affect your
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.
Waller, William H. The Milky Way: An Insider's Guide. Princeton, N.J: Princeton UP, 2013. 42+. Print.
The authors' prospected views on the future of our galaxy are rather harsh. The authors argue that a billion terrestrial years from now-in 10 galactic years-the galaxy will look much like it does now. Certain details, however, will be different. As the sun executes its next ten circuits around our galaxy's central hub, our today-familiar constellations will be scrambled one hundred times over. Many of the night stars in the sky will no longer exist. Deneb and Rigel, for example, will explode as supernovae. Sirious will swell into a red giant and puff out a planetary nebula. Alpha Centauri, currently the sun's closest neighbor, will recede from the sun, and its apparent brightness will fade below the threshold of naked-eye visibility.
Nebula away so that it can avoid certain things. In the short story, “The Star,” the priest stated,
Every day we look into the night sky, wondering and dreaming what lies beyond our galaxy. Within our galaxy alone, there are millions upon millions of stars. This may be why it interests us to learn about all that we cannot see. Humans have known the existence of stars since they have had eyes, and see them as white glowing specks in the sky. The mystery lies beyond the white glowing specks we see but, in the things we cannot see in the night sky such as black holes.
The Orion Nebula contains one of the brightest star clusters in the night sky. With a magnitude of 4, this nebula is easily visible from the Northern Hemisphere during the winter months. It is surprising, therefore, that this region was not documented until 1610 by a French lawyer named Nicholas-Claude Fabri de Peiresc. On March 4, 1769, Charles Messier inducted the Orion Nebula, M42, into his list of stellar objects. Then, in 1771, Messier released his list of objects for its first publication in Memoires de l’Academie.1
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.
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.
A star begins as nothing more than a very light distribution of interstellar gases and dust particles over a distance of a few dozen lightyears. Although there is extremely low pressure existing between stars, this distribution of gas exists instead of a true vacuum. If the density of gas becomes larger than .1 particles per cubic centimeter, the interstellar gas grows unstable. Any small deviation in density, and because it is impossible to have a perfectly even distribution in these clouds this is something that will naturally occur, and the area begins to contract. This happens because between about .1 and 1 particles per cubic centimeter, pressure gains an inverse relationship with density. This causes internal pressure to decrease with increasing density, which because of the higher external pressure, causes the density to continue to increase. This causes the gas in the interstellar medium to spontaneously collect into denser clouds. The denser clouds will contain molecular hydrogen (H2) and interstellar dust particles including carbon compounds, silicates, and small impure ice crystals. Also, within these clouds, there are 2 types of zones. There are H I zones, which contain neutral hydrogen and often have a temperature around 100 Kelvin (K), and there are H II zones, which contain ionized hydrogen and have a temperature around 10,000 K. The ionized hydrogen absorbs ultraviolet light from it’s environment and retransmits it as visible and infrared light. These clouds, visible to the human eye, have been named nebulae. The density in these nebulae is usually about 10 atoms per cubic centimeter. In brighter nebulae, there exists densities of up to several thousand atoms per cubic centimete...
Many people think that spiders and arachnids are synonyms with the same meaning and classifications. Through this piece, one will understand various differences and similarities between the two. Spiders are a member of the order, Araneae, class, Arachnids, and the phylum, Anthropods. Within the arachnid class lies much diversity and a few common traits. Spiders are grouped into this class as well as scorpions, ticks, mites, and many more organisms. The order, Araneae, is comprised of spiders. How do spiders and arachnids compare? While spiders and arachnids have many mutual traits, spiders differ in some key categories.
There is not much we can relate to when we watch this galaxy far, far away, but with the
The Universe is a collection of millions of galaxies and extends beyond human imagination. After the big bang, the universe was found to be composed of radiation and subatomic particles. Information following big bang is arguable on how galaxies formed, that is whether small particles merged to form clusters and eventually galaxies or whether the universe systematized as immense clumps of matter that later fragmented into galaxies (Nasa World book, 2013). A galaxy is a massive area of empty space full of dust, gases (mainly 75% Hydrogen and 25%Helium), atoms, about 100-200 billion stars, interstellar clouds and planets, attracted to the center by gravitational force of attraction. Based on recent research, 170 billion galaxies have been estimated to exist, with only tens of thousands been discovered (Deutsch, 2011).
see galaxies, nebulas and black holes millions of light-years away. One of the most interesting
As a source of information that is open to exploration, astronomy is a career field that is often ignored in favour of options such as business or psychology. But when overlooking the possibilities, students can miss out on opportunities they are unable to obtain in any other field. So many could learn so much with the technology that scientists have improved. It’s important to know the facts about the astronomy field, without dumbing it down.
Ever since the beginning of time there have been stars. Not only stars in the sky, but moons, planets, and even galaxies! Astronomy is defined as the branch of science that deals with celestial objects, space, and the physical universe as a whole. In other words it is the study of space, planets, and stars. Throughout the ages, many people have used astronomy to help them learn about the universe, our own planet, and even make predictions about life itself. Understanding astronomy means understanding where it originated, the different groups/cultures that used it, and modern purposes of the science of the stars.