- published: 17 Sep 2015
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A neutron star is a type of compact star that can result from the gravitational collapse of a massive star after a supernova. Neutron stars are the densest and smallest stars known to exist in the Universe; with a radius of only about 11–11.5 km (7 miles), they can have a mass of about twice that of the Sun.
Neutron stars are composed almost entirely of neutrons, which are subatomic particles with no net electrical charge and with slightly larger mass than protons. Neutron stars are very hot and are supported against further collapse by quantum degeneracy pressure due to the phenomenon described by the Pauli exclusion principle, which states that no two neutrons (or any other fermionic particles) can occupy the same place and quantum state simultaneously.
A neutron star has a mass of at least 1.1 and perhaps up to 3 solar masses (M☉), though the highest observed mass is 2.01 M☉. Neutron stars typically have a surface temperature around 7005600000000000000♠6×105 K. Neutron stars have overall densities of 7017370000000000000♠3.7×1017 to 7017590000000000000♠5.9×1017 kg/m3 (7014260000000000000♠2.6×1014 to 7014409999999999999♠4.1×1014 times the density of the Sun), which is comparable to the approximate density of an atomic nucleus of 7017300000000000000♠3×1017 kg/m3. The neutron star's density varies from below 7009100000000000000♠1×109 kg/m3 in the crust—increasing with depth—to above 7017600000000000000♠6×1017 or 7017800000000000000♠8×1017 kg/m3 deeper inside (denser than an atomic nucleus). A normal-sized matchbox containing neutron-star material would have a mass of approximately 5 trillion tons or 1000 km3 of Earth rock.
"Neutron Star Collision (Love Is Forever)" is a song by the English alternative rock band Muse, featured on the soundtrack to the 2010 film The Twilight Saga: Eclipse. Recorded by the band in 2010, the song was released as the lead single from the album on 17 May 2010. The song is available to purchase as a digital download from the band's official website, among several other digital sources.
The single became a top ten hit in Italy. It was also certified gold by Federation of the Italian Music Industry.
The song was first announced on Stephenie Meyer's official website. BBC Radio 1 aired the full song at 7.30pm on 17 May 2010, during Zane Lowe's show, accompanied by an interview with Matt Bellamy. Matt Bellamy explained that the song was written after he split with his longtime girlfriend at the end of 2009, and was based on his feelings at the beginning of their relationship. A 30-second preview of the music video is displayed on the official MTV website. While Muse featured on the Twilight and New Moon soundtracks previously (with "Supermassive Black Hole" and a special remix of "I Belong to You" respectively), this marks the first time the band has produced the lead single for a movie.
The neutron is a subatomic particle, symbol n or n0, with no net electric charge and a mass slightly larger than that of a proton. Protons and neutrons, each with mass approximately one atomic mass unit, constitute the nucleus of an atom, and they are collectively referred to as nucleons. Their properties and interactions are described by nuclear physics.
The nucleus consists of Z protons, where Z is called the atomic number, and N neutrons, where N is the neutron number. The atomic number defines the chemical properties of the atom, and the neutron number determines the isotope or nuclide. The terms isotope and nuclide are often used synonymously, but they refer to chemical and nuclear properties, respectively. The atomic mass number, symbol A, equals Z+N. For example, carbon has atomic number 6, and its abundant carbon-12 isotope has 6 neutrons, whereas its rare carbon-13 isotope has 7 neutrons. Some elements occur in nature with only one stable isotope, such as fluorine (see stable nuclide). Other elements occur as many stable isotopes, such as tin with ten stable isotopes. Even though it is not a chemical element, the neutron is included in the table of nuclides.
Spaceflight (also written space flight) is ballistic flight into or through outer space. Spaceflight can occur with spacecraft with or without humans on board. Examples of human spaceflight include the U.S. Apollo Moon landing and Space Shuttle programs and the Russian Soyuz program, as well as the ongoing International Space Station. Examples of unmanned spaceflight include space probes that leave Earth orbit, as well as satellites in orbit around Earth, such as communications satellites. These operate either by telerobotic control or are fully autonomous.
Spaceflight is used in space exploration, and also in commercial activities like space tourism and satellite telecommunications. Additional non-commercial uses of spaceflight include space observatories, reconnaissance satellites and other Earth observation satellites.
A spaceflight typically begins with a rocket launch, which provides the initial thrust to overcome the force of gravity and propels the spacecraft from the surface of the Earth. Once in space, the motion of a spacecraft—both when unpropelled and when under propulsion—is covered by the area of study called astrodynamics. Some spacecraft remain in space indefinitely, some disintegrate during atmospheric reentry, and others reach a planetary or lunar surface for landing or impact.
The Goddard Space Flight Center (GSFC) is a major NASA space research laboratory established on May 1, 1959 as NASA's first space flight center. GSFC employs approximately 10,000 civil servants and contractors, and is located approximately 6.5 miles (10.5 km) northeast of Washington, D.C. in Greenbelt, Maryland, USA. GSFC, one of ten major NASA field centers, is named in recognition of Dr. Robert H. Goddard (1882–1945), the pioneer of modern rocket propulsion in the United States.
GSFC is the largest combined organization of scientists and engineers in the United States dedicated to increasing knowledge of the Earth, the Solar System, and the Universe via observations from space. GSFC is a major U.S. laboratory for developing and operating unmanned scientific spacecraft. GSFC conducts scientific investigation, development and operation of space systems, and development of related technologies. Goddard scientists can develop and support a mission, and Goddard engineers and technicians can design and build the spacecraft for that mission. Goddard scientist John C. Mather shared the 2006 Nobel Prize in Physics for his work on COBE.
In the aftermath of a 8 – 20 solar mass star’s demise we find a weird little object known as a neutron star. Neutrons stars are incredibly dense, spin rapidly, and have very strong magnetic fields. Some of them we see as pulsars, flashing in brightness as they spin. Neutrons stars with the strongest magnetic fields are called magnetars, and are capable of colossal bursts of energy that can be detected over vast distances. Crash Course Astronomy Poster: http://store.dftba.com/products/crashcourse-astronomy-poster -- Table of Contents A Star Can Collapse to Form a Neutron Star 0:59 Neutron Star Characteristics 2:24 Pulsars 5:56 Magnetars 8:15 -- PBS Digital Studios: http://youtube.com/pbsdigitalstudios Follow Phil on Twitter: https://twitter.com/badastronomer Want to find Crash Course...
Neutron Stars are some of the strangest things in the Universe. Not quite massive enough to become black holes they are basically atoms as big as mountains with properties so extreme it's mind-blowing. And if you get too close to a neutron star you are in big trouble… Lots of you told us youtube doesn't tell you when we release new content. So we made a newsletter. No spam ever: http://eepurl.com/2bzP1 (Never miss a new video again) The music of the video can be found here: https://www.epicmountainmusic.bandcamp.com/track/neutron-star & https://www.soundcloud.com/epicmountain Videos, explaining things. Like evolution, time, space, global energy or our existence in this strange universe. We are a team of designers, journalists and musicians who want to make science look beautiful. ...
Stars are not eternal and unchanging - they are born, live their lives, and then die. The way a star dies depends on its mass. A low mass star ends as a white dwarf. A high mass star becomes a black hole. But in between, a star becomes a neutron star. In this video we talk about which stars become neutron stars, and the physics behind their formation. Hosted by Liliana de Castro Written by Michael Harrison Produced by Kimberly Hatch Harrison
#HowTheUniverseWorks A neutron star is one of the most dangerous objects in the universe. Neutron stars are the densest things besides black holes. A stone sized piece of this star would weigh 100 million metric tons. Full Episodes Streaming FREE on Science GO: https://www.sciencechannelgo.com/how-the-universe-works/ Subscribe to Science Channel: http://bit.ly/SubscribeScience Check out SCI2 for infinitely awesome science videos. Every day. http://bit.ly/SCI2YT Join Us on Facebook: http://www.facebook.com/ScienceChannel Follow Us on Twitter: http://www.twitter.com/sciencechannel
National Geographic End of the World: Evacuate Earth What would we do if the Earth were about to be destroyed? EVACUATE EARTH examines this terrifying and scientifically plausible scenario by exploring the technologies we would devise to carry as many humans as possible to safety. In EVACUATE EARTH, we envision a scenario in which a neutron star - tiny and incredibly dense- is flying straight toward our solar system. When it arrives in 75 years, it will pull our planets out of their orbits and shred the planet we live on. Our only choice is band together, create a vast ship and a new drive to power it, and find a new planet in the closest possible solar system to escape to. After a journey of almost a century, the ship will deliver mankind's remnants to our new home, and the human story w...
9 interesting facts about Neutron Stars. The spirit of a dead star. If you are interested in the wonders of the Universe, as planets, stars, black holes, theories, our solar system... You should watch this short documentary. In this case, you will enjoy learning the best curiosities about Neutron Stars. Their density, their magnetic field, their diameter, their power... Please, if you liked the video, drop a like and subscribe for more interesting videos about the universe, prehistoric animals and the deep sea. Channel: https://www.youtube.com/user/josepecinausina And if you like cinema... Second Channel: https://www.youtube.com/channel/UCCvsbroLD7oAHjSYUYZ1W8g Also, If you have any particular interest, something you would like to learn about, please comment it and I will make a grea...
Here's just some of what we already know about neutron stars. An upcoming NASA mission will further investigate these unusual objects from the International Space Station. The Neutron star Interior Composition Explorer mission, or NICER, will study the extraordinary environments — strong gravity, ultra-dense matter, and the most powerful magnetic fields in the universe — embodied by neutron stars. NICER is a two-in-one mission. The embedded Station Explorer for X-ray Timing and Navigation Technology, or SEXTANT, demonstration will use NICER data to validate, for the first time in space, pulsar-based navigation. NICER is planned for launch aboard the SpaceX CRS-11, currently scheduled for June 1, 2017. Learn more about the mission at nasa.gov/nicer. This video is public domain and along w...
Hello! Today I'll be testing a suggestion from "AAV" asking what would happen if we orbited a white dwarf around a black hole with a mass equal to that of 100 solar masses? Let's find out! Want this game?!: http://store.steampowered.com/app/230290/
In her Feb. 3 talk, Dr. Victoria Kaspi of McGill University, explored neutron stars -- mysterious celestial objects can shed light on some of the most vexing questions in the universe. More info on Perimeter Public Lectures: http://www.perimeterinstitute.ca/node/92581
I was searching You were on a mission Then our hearts combined like A neutron star collision I have nothing left to lose You took your time to choose Then we told each other With no trace of fear that... Our love would be forever And if we die We die together And lie, I said never Cause our love would be forever The world is broken Halos fail to glisten You try to make a difference But no one wants to listen Hail, The preachers, fake and proud Their doctrines will be cloud Then they'll dissipate Like snowflakes in an ocean Love is forever And we'll die, we'll die together And lie, I say never Cause our love could be forever Now I've got nothing left to lose You take your time to choose I can tell you now without a trace of fear That my love will be forever and we'll die we'll die to...
I have always been intrigued by the beauty of space. All art assets procedurally generated. Coded in C++ using the Cinder library. Music by Newton Faulkner. More info: http://illogictree.com/blog/2011/02/neutron-star/
Music video by Muse performing Neutron Star Collision (Love is forever) Band version, Twilight Official Soundtrack. © 2010 Warner Music UK Limited.
I love MUSE, but I hate twilight. I think you agree. I was extremely disappointed in Muse to see this music video with all the clips from twilight in it- so I made my own edit of the video WITH NO TWILIGHT! THE MUSE ONLY VERSION. w00t, right? Anyway, it's not perfect and if you have any suggestions I'd love to hear them. Download it, watch it, listen to it, share it with everyone you know, and post it everywhere so it doesn't get taken down. I'll upload videos for DOWNLOAD in various formats at: http://collinwinget.co.cc/muse.html
The video to "Neutron Star Collision" without any of the Twilight bullshit. Enjoy!
This animation shows the unique triple-star system with a superdense neutron star and two white dwarf stars. The neutron star is a pulsar, emitting lighthouse-like beams of radiation as it spins on its axis. These beams, in blue, are seen sweeping through space as the neutron star rotates. At the start, you see this pulsar and its close companion white dwarf in orbit around their common center of mass. The animation zooms outward, showing this pair also in orbit with a more-distant, cooler white dwarf, and illustrates the motions of these three bodies. The entire system would fit within Earth's orbit around the Sun.
Binary systems containing neutron stars are born when the cores of two orbiting stars collapse in supernova explosions. Neutron stars pack the mass of our sun into the size of a city. They are so dense and packed so tightly that the boundaries atoms nuclei disappear. In such systems, Einstein's theory of general relativity predicts that neutron stars emit gravitational radiation, ripples of space-time. This causes the orbits to shrink and gradually brings the neutron stars closer together. Shown here is such a system after about 1 billion years, when two equal-mass neutron whirl around each other at 60,000 times a minute. The stars merge in a few milliseconds, sending out a burst of gravitational waves and a brief, intense gamma-ray burst. This animation shows a neutron star merger and th...