Neutron Star

  

Copyright © Philip M. Parker, INSEAD. Terms of Use.

Neutron Star

Definition: Neutron Star

Neutron Star

Noun

1. A star that has collapsed under its own gravity; it is composed of neutrons.

Source: WordNet 1.7.1 Copyright © 2001 by Princeton University. All rights reserved.
 



Specialty Definitions: Neutron Star

DomainDefinitions

Physics

The imploded core of a massive star produced by a supernova explosion. (typical mass of 1.4 times the mass of the sun, radius of about 5 miles, density of a neutron.) According to astronomer and author Frank Shu, "A sugar cube of neutron-star stuff on Earth would weigh as much as all of humanity!" Neutron stars can be observed as pulsars. (references)

Space

A star (approximately sun-sized or larger), a remnant of a supernova explosion, in which gravity has caused all matter to collapse to a giant nucleus, composed only of neutrons. The collapse is also expected to greatly amplify any magnetic field present in the pre-collapse star, as well as speed up enormously any rate of rotation. It is believed that pulsars, pulsating radio sources with very precise pulsation periods, are neutron stars of radius about 10 km and rotation period about 1 second. Their magnetic axis spins and beams radio waves, in a way similar to the way a lighthouse beams its light. We detect pulsars when the Earth is in one of the directions swept by the beams. (references)

Source: compiled by the editor from various references; see credits.

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Specialty Definition: Neutron star

(From Wikipedia, the free Encyclopedia)

A neutron star is the collapsed remnant of a Type II or Ib supernova. Neutron stars are typically about 20 km in diameter, have greater than 1.4 times the mass of our Sun (otherwise they'd be white dwarfs) and less than about 3 times the mass of our Sun (otherwise they'd be black holes), and spin very rapidly (one revolution can take anything from thirty seconds to a hundredth of a second). Neutron stars are the densest objects known. Due to its small size and high density, a neutron star possesses a surface gravitational field about 2×1011 times that of Earth.

The matter at the surface of a neutron star is composed of ordinary nuclei as well as ionized electrons. Proceeding inward, one encounters nuclei with ever increasing numbers of neutrons; such nuclei would quickly decay on Earth, but are kept stable by tremendous pressures. Proceeding deeper, one comes to a point called neutron drip where free neutrons leak out of nuclei. In this region we have nuclei, free electrons, and free neutrons. The nuclei become smaller and smaller until the core is reached, by definition the point where they disappear altogether. The exact nature of the superdense matter in the core is still not well understood. Some researchers refer to this theoretical substance as neutronium. It could be a superfluid mixture of neutrons with a few protons and electrons, other high energy particles like pions and kaons may be present, and even sub-atomic quark matter is possible. However so far observations have not indicated nor ruled out such exotic states of matter.

Some neutron stars that can be observed:

Neutron stars rotate extremely rapidly after their creation due to the conservation of angular momentum; like an ice skater pulling in his arms, the slow rotation of the original star's core speeds up as it shrinks. A newborn neutron star can rotate several times a second; sometimes, when they orbit a companion star and are able to accrete matter from it, they can increase this to several thousand times per second, distorting into an oblate spheroid shape despite their own immense gravity (an equatorial bulge).

Over time, neutron stars slow down because their rotating magnetic fields radiate energy; older neutron stars may take several seconds or minutes for each revolution.

The rate at which a neutron star slows down its rotation is usually constant and very small: the observed rates are between 10-12 and 10-19 seconds for each century. In other words, a neutron star now rotating in 1 second will rotate in 1.000000000001 seconds after a century.

Sometimes a neutron star will undergo a glitch: a rapid and unexpected increase of its rotation speed (of the same, extremely small scale as the constant slowing down). Glitches are thought to be the effect of internal re-organizations of the matter composing the neutron star, something similar to starquakes. Such a starquake would register as grade 20 or 25 on the Richter scale.

Neutron stars also have very intense magnetic fields - about 1012 times stronger than Earth's. Neutron stars may "pulse" due to electrons accelerated near the magnetic poles, which are not aligned with the rotation axis of the star. These electrons travel outward from the neutron star, until they reach the point at which they would be forced to travel faster than the speed of light in order to still co-rotate with the star. At this radius, the electrons must stop, and they release some of their kinetic energy in the form of X-rays and gamma-rays. External viewers see these pulses of radiation whenever the magnetic pole is visible. The pulses come at the same rate as the rotation of the neutron star, and thus, appear periodic. Neutron stars which emit such pulses are called pulsars.

When pulsars were first discovered, they were believed by some to be evidence of extra-terrestrial intelligences. Because of their highly regular pattern of emmisions, they were initially thought to be beacons of some type.

Another class of neutron star, known as the magnetar, exists. These have a magnetic field of above 1014 gauss, strong enough to wipe a credit card from the distance of the Sun away and strong enough to be fatal from the distance of the moon away. By comparison, Earth's natural magnetic field is .5 gauss, and on Earth a fatal magnetic field is only a theoretical possibility; some of the strongest fields generated are actually used in medical imaging. A small neodymium based rare earth magnet has a field of a few thousand gauss, and most media used for data storage take several hundred gauss to erase.

The processes in a magnetar involve the rotation of the neutron star tangling field lines until they become exceptionally dense, giving rise to a resonant magnetic field.

See also:

Neutron Star was a 1966 Hugo award winning short story by Larry Niven

Source: adapted by the editor from Wikipedia, the free encyclopedia under a copyleft GNU Free Documentation License (GFDL) from the article "Neutron star."

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Synonyms within Context: Neutron Star

ContextSynonyms within Context (source: adapted from Roget's Thesaurus).

Density

Superdense matter, condensed states of matter; dwarf star, neutron star.

Source: adapted from Roget's Thesaurus.

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Crosswords: Neutron Star

English words defined with "neutron star": pulsar. (references)
Specialty definitions using "neutron star": binary starsS-Process. (references)

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Commercial Usage: Neutron Star

DomainTitle

Books

  • Neutron Star (reference)

  • Neutron star matter : phase transition to a neutron solid? (reference)

  • Physics of Neutron Star Interiors (Lecture Notes in Physics, 578) (reference)

  • The Neutron Star Black Hole Connection (NATO Science Series. Series C, Mathematical and Physical Sciences, V. 567) (reference)

  • Theory of Neutron Star Magnetospheres (Theoretical Astrophysics) (reference)

    (more book examples)

Source: compiled by the editor from various references; see credits.

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Photo Album: Neutron Star

ThumbnailDescription & Credit

First direct look, in visible light, at a lone neutron star (RX J185635-3754). (Produced with the Wide-Field Planetary Camera 2, Hubble Space Telescope.).Credit: NASA.

Source: compiled by the editor from various references; see credits.

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Frequency of Internet Keywords: Neutron Star

The following statistics estimate the number of searches per day across the major English-language search engines as identified by various trade publications. Hyperlinks lead to commercial use of the expression at Amazon.com.
 
ExpressionFrequency
per Day

neutron star

76

density neutron star

4

neutron star star type

3

information neutron star

3

black hole neutron star

2
Source: compiled by the editor from various references; see credits.

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Modern Translations: Neutron Star

Language Translations for "neutron star"; alternative meanings/domain in parentheses.

Dutch

  

neutronenster. (various references)

   

German

  

neutronenstern. (various references)

   

Japanese Kanji 

  

中性子星 (a neutron star). (various references)

   

Japanese Katakana 

  

ちゅうせいしせい (a neutron star). (various references)

   

Pig Latin

  

eutronnay arstay

   

Spanish

  

estrella de neutrones. (various references)

Source: compiled by the editor from various translation references.

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Misspellings: Neutron Star

Misspellings

"Neutron Star" is suggested in spellcheckers for the following: nuetron star. (additional references)

Source: compiled by the editor, based on several corpora (additional references).

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Anagrams: Neutron Star

Scrabble® Enable2K-Verified Anagrams

Words within the letters "a-e-n-n-o-r-r-s-t-t-u"

-1 letter: nonstarter.

-2 letters: turnstone.

-3 letters: antrorse, entrants, neutrons, outearns, outrates, outstare, resonant, rostrate, taunters, tonneaus, torrents, tortures, unornate, unreason.

-4 letters: arenous, arouser, atoners, attorns, attunes, entrant, entrust, errants, natrons, natters, natures, neurons, neuston, neutron, nonarts, nonuser, notates, nutates, nutters, outearn, outeats, outrate, outsert, ranters, rattens, ratters, rattons, restart, retorts, returns, roaster, rotates, rotters, rouster, routers, runners, santour, saunter, senator, serrano, snorter, soutane, starter, stature, stentor, stertor, stouten, stouter, stunner, tanners, tannest, taunter, tautens, tenants, tenours, tenutos, tetanus, toaster, tonneau, tonners, tonsure, torrent, torture, tourers, touters, treason, trouser, truants, truster, trustor, turners, turnons, turrets, unstate.

-5 letters: anenst, antres, arouse, arrest, arseno, astern, astute, atoner, atones, attorn, attune, errant, natron, natter, nature, nestor, neuron, nonart, nonets, nonuse, notate, noters, nurser, nutant, nutate, nutter, oaters, orates, ornate, ottars, otters, ouster, outate, outeat, outers, outran, outsat, outset, ranter, rarest, raster, rasure, raters, ratten, ratter, ratton, reason, reruns, resort, retorn, retort, retros, return, roster, rostra, rotate, rotten, rotter, rottes, rouens, rouser, router, routes, runner, santur, sartor, senora, setout, snarer, snorer, soarer, sonant, sonnet, sorner, sorter, sourer, souter, starer, stater, stator, statue, sterna, stoner, stoure, strunt, suntan, tanner, tarots, tarres, tarter, taster, taters, taunts, tauten, tauter, tenant, tenons, tenors, tenour, tensor, tenuto, terras, teston, tetras, toners, tonner, tonnes, torten, tortes, toters, tourer, touter, treats, tronas, trones, trouts, truant, truest, tuners, turner, turnon, turret, tutors, unrent, unrest, unseat, unsent, untorn, urares, urates, utters.

 Words containing the letters "a-e-n-n-o-r-r-s-t-t-u"
 

+2 letters: renaturations.

 

+3 letters: macronutrients, pretournaments.

 

+4 letters: nonbarbiturates.

 

+5 letters: counterarguments, counterirritants, counterreactions, countersignature, neurotransmitter, nonarchitectures.

Source: compiled by the editor from various references; see credits.

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Alternative Orthography: Neutron Star


Hexadecimal (or equivalents, 770AD-1900s) (references)

4E 65 75 74 72 6F 6E      53 74 61 72

Leonardo da Vinci (1452-1519; backwards) (references)

    

Binary Code (1918-1938, probably earlier) (references)

01001110 01100101 01110101 01110100 01110010 01101111 01101110 00100000 01010011 01110100 01100001 01110010

HTML Code (1990) (references)

&#78 &#101 &#117 &#116 &#114 &#111 &#110 &#32 &#83 &#116 &#97 &#114

ISO 10646 (1991-1993) (references)

004E 0065 0075 0074 0072 006F 006E      0053 0074 0061 0072

Encryption (beginner's substitution cypher): (references)

48718786848180253866784

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INDEX

1. Definition
2. Crosswords
3. Usage: Commercial
4. Images: Photo Album
5. Expressions: Internet
6. Translations: Modern
7. Derivations
8. Anagrams
9. Orthography
10. Bibliography


  

Copyright © Philip M. Parker, INSEAD. Terms of Use.