- published: 13 Sep 2014
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Galaxy groups and clusters are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation. They form the densest part of the large-scale structure of the Universe. In models for the gravitational formation of structure with cold dark matter, the smallest structures collapse first and eventually build the largest structures, clusters of galaxies. Clusters are then formed relatively recently between 10 billion years ago and now. Groups and clusters may contain ten to thousands of individual galaxies. The clusters themselves are often associated with larger, non-gravitationally bound, groups called superclusters.
Groups of galaxies are the smallest aggregates of galaxies. They typically contain no more than 50 galaxies in a diameter of 1 to 2 megaparsecs (Mpc)(see 1022 m for distance comparisons). Their mass is approximately 1013solar masses. The spread of velocities for the individual galaxies is about 150 km/s. However, this definition should be used as a guide only, as larger and more massive galaxy systems are sometimes classified as galaxy groups. Groups are the most common structures of galaxies in the universe, comprising at least 50% of the galaxies in the local universe. Groups have a mass range between those of the very large elliptical galaxies and clusters of galaxies.
Crash Course (also known as Driving Academy) is a 1988 made for television teen film directed by Oz Scott.
Crash Course centers on a group of high schoolers in a driver’s education class; many for the second or third time. The recently divorced teacher, super-passive Larry Pearl, is on thin ice with the football fanatic principal, Principal Paulson, who is being pressured by the district superintendent to raise driver’s education completion rates or lose his coveted football program. With this in mind, Principal Paulson and his assistant, with a secret desire for his job, Abner Frasier, hire an outside driver’s education instructor with a very tough reputation, Edna Savage, aka E.W. Savage, who quickly takes control of the class.
The plot focuses mostly on the students and their interactions with their teachers and each other. In the beginning, Rico is the loner with just a few friends, Chadley is the bookish nerd with few friends who longs to be cool and also longs to be a part of Vanessa’s life who is the young, friendly and attractive girl who had to fake her mother’s signature on her driver’s education permission slip. Kichi is the hip-hop Asian kid who often raps what he has to say and constantly flirts with Maria, the rich foreign girl who thinks that the right-of-way on the roadways always goes to (insert awesomely fake foreign Latino accent) “my father’s limo”. Finally you have stereotypical football meathead J.J., who needs to pass his English exam to keep his eligibility and constantly asks out and gets rejected by Alice, the tomboy whose father owns “Santini & Son” Concrete Company. Alice is portrayed as being the “son” her father wanted.
The Milky Way is the galaxy that contains our Solar System. Its name "milky" is derived from its appearance as a dim glowing band arching across the night sky whose individual stars cannot be distinguished by the naked eye. The term "Milky Way" is a translation of the Latin via lactea, from the Greek γαλαξίας κύκλος (galaxías kýklos, "milky circle"). From Earth, the Milky Way appears as a band because its disk-shaped structure is viewed from within. Galileo Galilei first resolved the band of light into individual stars with his telescope in 1610. Until the early 1920s, most astronomers thought that the Milky Way contained all the stars in the Universe. Following the 1920 Great Debate between the astronomers Harlow Shapley and Heber Curtis, observations by Edwin Hubble showed that the Milky Way is just one of many galaxies—now estimated to number as many as 200 billion galaxies in the observable universe.
The Milky Way is a barred spiral galaxy that has a diameter usually considered to be about 100,000–120,000 light-years but may be 150,000–180,000 light-years. The Milky Way is estimated to contain 100–400 billion stars, although this number may be as high as one trillion. There are probably at least 100 billion planets in the Milky Way. The Solar System is located within the disk, about 27,000 light-years from the Galactic Center, on the inner edge of one of the spiral-shaped concentrations of gas and dust called the Orion Arm. The stars in the inner ≈10,000 light-years form a bulge and one or more bars that radiate from the bulge. The very center is marked by an intense radio source, named Sagittarius A*, which is likely to be a supermassive black hole.
Coordinates: 38°52′59″N 77°0′59″W / 38.88306°N 77.01639°W / 38.88306; -77.01639
The National Aeronautics and Space Administration (NASA) is the agency of the United States Federal Government responsible for the civilian space program as well as aeronautics and aerospace research.
President Dwight D. Eisenhower established the National Aeronautics and Space Administration (NASA) in 1958 with a distinctly civilian (rather than military) orientation encouraging peaceful applications in space science. The National Aeronautics and Space Act was passed on July 29, 1958, disestablishing NASA's predecessor, the National Advisory Committee for Aeronautics (NACA). The new agency became operational on October 1, 1958.
Since that time, most US space exploration efforts have been led by NASA, including the Apollo moon-landing missions, the Skylab space station, and later the Space Shuttle. Currently, NASA is supporting the International Space Station and is overseeing the development of the Orion Multi-Purpose Crew Vehicle, the Space Launch System and Commercial Crew vehicles. The agency is also responsible for the Launch Services Program (LSP) which provides oversight of launch operations and countdown management for unmanned NASA launches.
A galaxy is a gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter. The word galaxy is derived from the Greek galaxias (γαλαξίας), literally "milky", a reference to the Milky Way. Galaxies range in size from dwarfs with just a few thousand (103) stars to giants with one hundred trillion (1014) stars, each orbiting their galaxy's own center of mass. Galaxies, are categorized according to their visual morphology, including elliptical,spiral, and irregular. Many galaxies are thought to have black holes at their active centers. The Milky Way's central black hole, known as Sagittarius A*, has a mass four million times greater than the Sun. As of July 2015, EGSY8p7 is the oldest and most distant observed galaxy with a light travel distance of 13.2 billion light-years from Earth, and observed as it existed 570 million years after the Big Bang. Previously, as of May 2015, EGS-zs8-1 was the most distant known galaxy, estimated to have a light travel distance of 13.1 billion light-years away and to have 15% of the mass of the Milky Way.
Galaxies are generally found in clusters. Unlike stars, which rarely come into close contact, galaxies interact often, producing spectacular sights of tangled star filaments called “tidal tales”. These three ESA videos feature many examples of merging and colliding galaxies: 1. The Leo Triplet; 2. Merging spiral galaxies; 3. Colliding Galaxies
"Galaxy groups and clusters" are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation. They form the densest part of the large-scale structure of the Universe. In models for the gravitational formation of structure with cold dark matter, the smallest structures collapse first and eventually build the largest structures, clusters of galaxies. Clusters are then formed relatively recently between 10 billion years ago and now. Groups and clusters may contain ten to thousands of individual galaxies. The clusters themselves are often associated with larger, non-gravitationally bound, groups called superclusters. Groups of galaxies are the smallest aggregates of galaxies. They typically contain no more than 50 galaxies in a di...
Superclusters – regions of space that are densely packed with galaxies – are the biggest structures in the Universe. But scientists have struggled to define exactly where one supercluster ends and another begins. Now, a team based in Hawaii has come up with a new technique that maps the Universe according to the flow of galaxies across space. Redrawing the boundaries of the cosmic map, they redefine our home supercluster and name it Laniakea, which means ‘immeasurable heaven’ in Hawaiian. Read the research paper: http://dx.doi.org/10.1038/nature13674 Read Nature's news story: http://www.nature.com/news/earth-s-new-address-solar-system-milky-way-laniakea-1.15819
Active galaxies pour out lots of energy, due to their central supermassive black holes gobbling down matter. Galaxies tend not to be loners, but instead exist in smaller groups and larger clusters. Our Milky Way is part of the Local Group, and will one day collide with the Andromeda galaxy. Clusters of galaxies also clump together to form superclusters, the largest structures in the Universe. In total, there are hundreds of billions of galaxies in the Universe. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Black Holes at the Center of Galaxies 2:26 Galaxies Are a Part of Small/Large Clusters 9:47 The Milky Way is Part of the Local Group 6:45 Galaxy Clusters Clump Together to Create Superclusters 11:03 Hundreds of Billion...
Welcome!! ~ Feel free to Like & Subscribe ~ - A galaxy cluster, or cluster of galaxies, is a structure that consists of anywhere from hundreds to thousands of galaxies that are bound together by gravity with typical masses ranging from 1014–1015 solar masses. They are the largest known gravitationally bound structures in the universe and were believed to be the largest known structures in the universe until the 1980s, when superclusters were discovered. One of the key features of clusters is the intracluster medium (ICM). The ICM consists of heated gas between the galaxies and has a peak temperature between 2–15 keV that is dependent on the total mass of the cluster. Galaxy clusters should not be confused with star clusters, such as open clusters, which are structures of stars within galax...
An international team of astronomers has discovered an enormous galaxy cluster producing stars at a fantastic pace. Galaxy clusters, the Universe's largest structures, are groups of galaxies bound by gravity with a supermassive black hole at the center. Most galaxy clusters produce few stars. But the newly described Phoenix Cluster is experiencing a period of rapid star formation. Science Bulletins is a production of the National Center for Science Literacy, Education, and Technology (NCSLET), part of the Department of Education at the American Museum of Natural History Related Links: NASA: The Remarkable Phoenix Cluster nasa.gov/mission_pages/chandra/multimedia/phoenix_cluster.html Chandra X-Ray Observatory: Phoenix Cluster chandra.harvard.edu/photo/2012/phoenix/ South Pole Telescope...
The Milky Way is our neighborhood in the universe. It’s a galaxy and there are many others out there. Galaxies contain gas, dust, and billions of stars or more. They come in four main shapes: elliptical, spiral, peculiar, and irregular. Galaxies can collide, and grow in size by eating each other. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Milky Way is a Galaxy (One of Many) 2:04 Galaxies Have Four Main Shapes 3:18 Galaxies Can Collide 6:05 -- PBS Digital Studios: http://youtube.com/pbsdigitalstudios Follow Phil on Twitter: https://twitter.com/badastronomer Want to find Crash Course elsewhere on the internet? Facebook - http://www.facebook.com/YouTubeCrashCourse Twitter - http://www.twitter.com/TheCrashCourse Tumb...
The VLT Survey Telescope (VST) at ESO's Paranal Observatory in Chile has imaged a fascinating collection of interacting galaxies in the Hercules galaxy cluster. The sharpness of the new picture, and the hundreds of galaxies captured in great detail in less than three hours of observations, attest to the great power of the VST and its huge camera OmegaCAM to explore the nearby Universe. The Hercules galaxy cluster (also known as Abell 2151) lies about 500 million light-years away in the constellation of Hercules. It is unlike other nearby galactic assemblies in many ways. As well as being rather irregular in shape, it contains a wide variety of galaxy types, particularly young, star-forming spiral galaxies, and there are no giant elliptical galaxies in sight. The new image was taken with ...
There are two types of star clusters. Open (or galactic) clusters are sparsely populated, fairly young groups of tens to hundreds of stars that have formed out of a nebula and that are slowly “evaporating” into space. Globular clusters are very old, densely packed groups of millions of star on the outskirts of galaxies. This program combines 3 ESA videos with news about Star Clusters: 1. Extreme star cluster; 2. Globular Clusters; 3. Omega Centauri
Galaxies are generally found in clusters. Unlike stars, which rarely come into close contact, galaxies interact often, producing spectacular sights of tangled star filaments called “tidal tales”. These three ESA videos feature many examples of merging and colliding galaxies: 1. The Leo Triplet; 2. Merging spiral galaxies; 3. Colliding Galaxies
"Galaxy groups and clusters" are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation. They form the densest part of the large-scale structure of the Universe. In models for the gravitational formation of structure with cold dark matter, the smallest structures collapse first and eventually build the largest structures, clusters of galaxies. Clusters are then formed relatively recently between 10 billion years ago and now. Groups and clusters may contain ten to thousands of individual galaxies. The clusters themselves are often associated with larger, non-gravitationally bound, groups called superclusters. Groups of galaxies are the smallest aggregates of galaxies. They typically contain no more than 50 galaxies in a di...
Superclusters – regions of space that are densely packed with galaxies – are the biggest structures in the Universe. But scientists have struggled to define exactly where one supercluster ends and another begins. Now, a team based in Hawaii has come up with a new technique that maps the Universe according to the flow of galaxies across space. Redrawing the boundaries of the cosmic map, they redefine our home supercluster and name it Laniakea, which means ‘immeasurable heaven’ in Hawaiian. Read the research paper: http://dx.doi.org/10.1038/nature13674 Read Nature's news story: http://www.nature.com/news/earth-s-new-address-solar-system-milky-way-laniakea-1.15819
Active galaxies pour out lots of energy, due to their central supermassive black holes gobbling down matter. Galaxies tend not to be loners, but instead exist in smaller groups and larger clusters. Our Milky Way is part of the Local Group, and will one day collide with the Andromeda galaxy. Clusters of galaxies also clump together to form superclusters, the largest structures in the Universe. In total, there are hundreds of billions of galaxies in the Universe. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Black Holes at the Center of Galaxies 2:26 Galaxies Are a Part of Small/Large Clusters 9:47 The Milky Way is Part of the Local Group 6:45 Galaxy Clusters Clump Together to Create Superclusters 11:03 Hundreds of Billion...
Welcome!! ~ Feel free to Like & Subscribe ~ - A galaxy cluster, or cluster of galaxies, is a structure that consists of anywhere from hundreds to thousands of galaxies that are bound together by gravity with typical masses ranging from 1014–1015 solar masses. They are the largest known gravitationally bound structures in the universe and were believed to be the largest known structures in the universe until the 1980s, when superclusters were discovered. One of the key features of clusters is the intracluster medium (ICM). The ICM consists of heated gas between the galaxies and has a peak temperature between 2–15 keV that is dependent on the total mass of the cluster. Galaxy clusters should not be confused with star clusters, such as open clusters, which are structures of stars within galax...
An international team of astronomers has discovered an enormous galaxy cluster producing stars at a fantastic pace. Galaxy clusters, the Universe's largest structures, are groups of galaxies bound by gravity with a supermassive black hole at the center. Most galaxy clusters produce few stars. But the newly described Phoenix Cluster is experiencing a period of rapid star formation. Science Bulletins is a production of the National Center for Science Literacy, Education, and Technology (NCSLET), part of the Department of Education at the American Museum of Natural History Related Links: NASA: The Remarkable Phoenix Cluster nasa.gov/mission_pages/chandra/multimedia/phoenix_cluster.html Chandra X-Ray Observatory: Phoenix Cluster chandra.harvard.edu/photo/2012/phoenix/ South Pole Telescope...
The Milky Way is our neighborhood in the universe. It’s a galaxy and there are many others out there. Galaxies contain gas, dust, and billions of stars or more. They come in four main shapes: elliptical, spiral, peculiar, and irregular. Galaxies can collide, and grow in size by eating each other. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents Milky Way is a Galaxy (One of Many) 2:04 Galaxies Have Four Main Shapes 3:18 Galaxies Can Collide 6:05 -- PBS Digital Studios: http://youtube.com/pbsdigitalstudios Follow Phil on Twitter: https://twitter.com/badastronomer Want to find Crash Course elsewhere on the internet? Facebook - http://www.facebook.com/YouTubeCrashCourse Twitter - http://www.twitter.com/TheCrashCourse Tumb...
The VLT Survey Telescope (VST) at ESO's Paranal Observatory in Chile has imaged a fascinating collection of interacting galaxies in the Hercules galaxy cluster. The sharpness of the new picture, and the hundreds of galaxies captured in great detail in less than three hours of observations, attest to the great power of the VST and its huge camera OmegaCAM to explore the nearby Universe. The Hercules galaxy cluster (also known as Abell 2151) lies about 500 million light-years away in the constellation of Hercules. It is unlike other nearby galactic assemblies in many ways. As well as being rather irregular in shape, it contains a wide variety of galaxy types, particularly young, star-forming spiral galaxies, and there are no giant elliptical galaxies in sight. The new image was taken with ...
There are two types of star clusters. Open (or galactic) clusters are sparsely populated, fairly young groups of tens to hundreds of stars that have formed out of a nebula and that are slowly “evaporating” into space. Globular clusters are very old, densely packed groups of millions of star on the outskirts of galaxies. This program combines 3 ESA videos with news about Star Clusters: 1. Extreme star cluster; 2. Globular Clusters; 3. Omega Centauri
Lecture given by Prof Joydeep Bagchi (IUCAA) during the Radio Astronomy Winter school held at IUCAA-NCRA, December 2016.
TITLE: Mechanical Approach to Discrete Cosmology: Theory and Applications ABSTRACT: We consider the late Universe deep inside the cell of uniformity. At these scales, the Universe is highly inhomogeneous and is filled with discrete distributed structures (galaxies, groups and clusters of galaxies), which perturb the background Friedmann model. We investigate such Universe in the mechanical approach. This means that the peculiar velocities of the inhomogeneities in the form of galaxies as well as fluctuations of other perfect fluids are nonrealistic. Under such condition, we investigate the theory of scalar perturbations. We derive the main equations and apply them to a number of models, starting with the ΛCDM model. We demonstrate that within our approach, the theory of scalar perturbatio...
Welcome!! ~ Feel free to Like & Subscribe ~ - A galaxy cluster, or cluster of galaxies, is a structure that consists of anywhere from hundreds to thousands of galaxies that are bound together by gravity with typical masses ranging from 1014–1015 solar masses. They are the largest known gravitationally bound structures in the universe and were believed to be the largest known structures in the universe until the 1980s, when superclusters were discovered. One of the key features of clusters is the intracluster medium (ICM). The ICM consists of heated gas between the galaxies and has a peak temperature between 2–15 keV that is dependent on the total mass of the cluster. Galaxy clusters should not be confused with star clusters, such as open clusters, which are structures of stars within galax...
Click to watch Playlist: https://www.youtube.com/playlist?list=PLL2LECDSDJ1xddO4qm8NdrFQmxSkZlDjy Check more information about Universe Documentary and keep update here: Facebook: https://www.facebook.com/Life-Sience-219167571854129 Twitter: https://twitter.com/LifeSienceDocu Subscribe here: https://www.youtube.com/channel/UChwJp9TNugZRZSJTW2bQ3CQ Wiki: https://en.wikipedia.org/wiki/Galaxy_groups_and_clusters Galaxy groups and clusters are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation.[2] They form the densest part of the large-scale structure of the Universe. In models for the gravitational formation of structure with cold dark matter, the smallest structures collapse first and eventually build the largest structures...
Galaxy clusters are the largest gravitationally bound objects in our Universe and are unique laboratories to study fundamental questions in astrophysics. Galaxy clusters grow by mergers with smaller subclusters and galaxy groups. In this talk, I will discuss how merging galaxy clusters can act as giant particle accelerators, producing extremely energetic cosmic rays. Host: Charles Alcock Speaker: Reinout van Weeren
How much do we know about this universe we call home? In this New York Real episode London edition, you will meet astrophysicist Maggie Lieu who was selected as the 100 prospective astronaut for Mars One project from 200,000 applicants all over the world. She is working on a PhD within the Astronomy & Space Research group at the University of Birmingham. Her work is focused on using weak gravitational lensing and X-ray observables to determine precise mass measurements of galaxy groups and clusters. On the day we met, we discovered that we both can speak Cantonese - fun fact! Don't worry, this interview is in English. Be inspired to explore our universe and stay curious! Maggie's official website: http://maggielieu.com Maggie on Twitter: @Space_Mog Music: New York Real Opening Theme by ...
Scary Yet Beautiful Facts About SPACE & UNIVERSE - The BIGGEST Star clusters in the Universe 🔴 CLICK to Subscribe ➡ https://goo.gl/cNLxa2 👈👽 🔴 CLICK to DONATE ➡ https://goo.gl/adEY40 👈👽 ►Star clusters or star clouds are groups of stars. Two types of star clusters can be distinguished: globular clusters are tight groups of hundreds or thousands of very old stars which are gravitationally bound, while open clusters, more loosely clustered groups of stars, generally contain fewer than a few hundred members, and are often very young. ►Open clusters become disrupted over time by the gravitational influence of giant molecular clouds as they move through the galaxy, but cluster members will continue to move in broadly the same direction through space even though they are no longer gravitational...
Galaxy clusters are the largest gravitationally bound objects in our Universe and are unique laboratories to study fundamental questions in astrophysics. Galaxy clusters grow by mergers with smaller subclusters and galaxy groups. This talk will discuss how merging galaxy clusters can act as giant particle accelerators, producing extremely energetic cosmic rays. The radio interferometric array of LOFAR consists of many low-cost antennas. This is the main application of LOFAR. There are two distinct antenna types: the Low Band Antenna (LBA) operates between 10 and 90 MHz and the High Band Antenna (HBA) between 110 and 250 MHz. These 'sensors' are organised in aperture array stations. The stations (currently, 36 stations are being constructed in the Netherlands) are distributed over an area a...
Public Astronomy talk “The Universe of Galaxies and STEM Research Opportunities for Young People” by the leading Astronomer in the galaxy formation, Dr. Puragra Guhathakurta (Raja) on Friday, March 18, from 7 pm to 8 pm at VPA Theater, Evergreen Valley College. Introduction by EVC President – Henry Yong The talk will have two distinct segments. The first segment on galaxies will discuss how the very elements in the Periodic Table that form the basis of complex life on Earth were created inside stars and during the explosive death of massive stars. The second segment of the talk will be about the Science Internship Program, the Global SPHERE Network, and the importance of engaging young people in real (i.e., open-ended) STEM research projects outside the traditional classroom. The key e...
Space, Planet, Nibiru, PlanetX, UFO, Moon, Documentaries: https://www.youtube.com/watch?v=Xr4X7-7Qu7g&list;=PL-VOxZxryC3QHP8HznpsYIndGa50kEV50 "What Is the Biggest Thing in the Universe? The Universe Biggest Things In Space" In space, we're used to dealing with large distances and objects. In the cosmic scheme of things, Earth is rather small. Even in our solar system, we are easily dwarfed by the planet Jupiter (more than 1,000 Earths would fit in the planet, according to NASA) and our sun (more than a million Earths would fit in there, according to Cornell University). Even our sun looks puny when it is compared to the biggest stars we know of. The sun is a G-type star, a yellow dwarf — pretty average-size on the cosmic scale. But some “hypergiant” stars are much, much larger. ...