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Star and Supernova remnant

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Star and Supernova remnant

Star vs. Supernova remnant

A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity. A supernova remnant (SNR) is the structure resulting from the explosion of a star in a supernova.

Similarities between Star and Supernova remnant

Star and Supernova remnant have 16 things in common (in Unionpedia): Black hole, Crab Nebula, Hydrogen, Interstellar medium, Large Magellanic Cloud, Neutron star, Oxygen, Planetary nebula, Plasma (physics), Pulsar, Shock wave, SN 1006, Supernova, Tycho Brahe, White dwarf, X-ray.

Black hole

A black hole is a region of spacetime exhibiting such strong gravitational effects that nothing—not even particles and electromagnetic radiation such as light—can escape from inside it.

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Crab Nebula

The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant in the constellation of Taurus.

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Hydrogen

Hydrogen is a chemical element with symbol H and atomic number 1.

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Interstellar medium

In astronomy, the interstellar medium (ISM) is the matter and radiation that exists in the space between the star systems in a galaxy.

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Large Magellanic Cloud

The Large Magellanic Cloud (LMC) is a satellite galaxy of the Milky Way.

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Neutron star

A neutron star is the collapsed core of a large star which before collapse had a total of between 10 and 29 solar masses.

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Oxygen

Oxygen is a chemical element with symbol O and atomic number 8.

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Planetary nebula

A planetary nebula, abbreviated as PN or plural PNe, is a type of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from red giant stars late in their lives.

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Plasma (physics)

Plasma (Henry George Liddell, Robert Scott, A Greek English Lexicon, on Perseus) is one of the four fundamental states of matter, and was first described by chemist Irving Langmuir in the 1920s.

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Pulsar

A pulsar (from pulse and -ar as in quasar) is a highly magnetized rotating neutron star or white dwarf that emits a beam of electromagnetic radiation.

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Shock wave

In physics, a shock wave (also spelled shockwave), or shock, is a type of propagating disturbance.

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SN 1006

SN 1006 was a supernova that is likely the brightest observed stellar event in recorded history, reaching an estimated −7.5 visual magnitude, and exceeding roughly sixteen times the brightness of Venus.

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Supernova

A supernova (plural: supernovae or supernovas, abbreviations: SN and SNe) is a transient astronomical event that occurs during the last stellar evolutionary stages of a star's life, either a massive star or a white dwarf, whose destruction is marked by one final, titanic explosion.

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Tycho Brahe

Tycho Brahe (born Tyge Ottesen Brahe;. He adopted the Latinized form "Tycho Brahe" (sometimes written Tÿcho) at around age fifteen. The name Tycho comes from Tyche (Τύχη, meaning "luck" in Greek, Roman equivalent: Fortuna), a tutelary deity of fortune and prosperity of ancient Greek city cults. He is now generally referred to as "Tycho," as was common in Scandinavia in his time, rather than by his surname "Brahe" (a spurious appellative form of his name, Tycho de Brahe, only appears much later). 14 December 154624 October 1601) was a Danish nobleman, astronomer, and writer known for his accurate and comprehensive astronomical and planetary observations.

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White dwarf

A white dwarf, also called a degenerate dwarf, is a stellar core remnant composed mostly of electron-degenerate matter.

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X-ray

X-rays make up X-radiation, a form of electromagnetic radiation.

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The list above answers the following questions

Star and Supernova remnant Comparison

Star has 399 relations, while Supernova remnant has 43. As they have in common 16, the Jaccard index is 3.62% = 16 / (399 + 43).

References

This article shows the relationship between Star and Supernova remnant. To access each article from which the information was extracted, please visit:

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