supernova remnant oor Indonesies
supernova remnant
en
(astronomy) A nebula that is formed from supernova explosion debris.
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Sisa-sisa supernova
en
remnants of an exploded star
Scattered among the stars of the Milky Way are supernova remnants each one the remains of a colossal stellar explosion.
Tersebar antara bintang-bintang dari Bima Sakti Adalah sisa-sisa supernova Masing-masing sisa-sisa ledakan bintang kolosal.
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Supernova remnant: Radio image in red, X-ray in blue, visible light in green
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A supernova remnant (SNR) is the structure resulting from the explosion of a star in a supernova.
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The expelled matter may form nebulae called supernova remnants.
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Scattered among the stars of the Milky Way are supernova remnants each one the remains of a colossal stellar explosion.
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And inside that supernova remnant is going to be a little black hole that has a mass roughly three times the mass of the Sun.
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And inside that supernova remnant is going to be a little black hole that has a mass roughly three times the mass of the Sun.
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One of the best observed young supernova remnants was formed by SN 1987A, a supernova in the Large Magellanic Cloud that was observed in February 1987.
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This feature is approximately 25 light-years in width and has the attributes of a supernova remnant from an explosive event that occurred between 35,000 and 100,000 BC.
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It is called a pulsar, described as a spinning supernova remnant so compressed that the electrons and protons in the atoms of the original star have been squeezed together to produce neutrons.
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It consists of three components, the supernova remnant Sagittarius A East, the spiral structure Sagittarius A West, and a very bright compact radio source at the center of the spiral, Sagittarius A* ("Sagittarius A-star").
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So, if a star starts its life off with much more mass than the mass of the Sun, it's going to end its life by exploding and leaving behind these beautiful supernova remnants that we see here.
Tapi mungkin aku yang lamaQED QED
Elements with greater than 26 protons are formed by supernova nucleosynthesis in supernovae, which, when they explode, blast these elements as supernova remnants far into space, where they may become incorporated into planets when they are formed.
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Astronomers, such as Harvard’s Robert Kirshner, believe that understanding supernova remnants like the Crab Nebula is important because they can be used to measure the distance to other galaxies, which is currently an area of intense research.
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Recently, the detection of characteristic gamma rays originating from the decay of neutral pions in two supernova remnants has shown that pions are produced copiously after supernovas, most probably in conjunction with production of high energy protons that are detected on Earth as cosmic rays.
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And some stars die spectacularly in a supernova explosion, leaving remnants like that.
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See the discussion The M102 Controversy for more details. Open cluster Globular cluster Nebula Planetary nebula Supernova remnant Galaxy Other He independently discovered four others, originally discovered by someone else but unknown to him at the time and included in the Messier catalogue: M71, discovered by Jean-Philippe de Chéseaux in the 1740s; M80, discovered by Messier about two weeks earlier than Méchain's observation; and M81 and M82, discovered originally by Johann Bode.
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It's a remnant of a supernova.
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These massive stars produce supernova explosions, resulting in expanding remnants that interact powerfully with the surrounding gas.
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The remnant of a supernova is a dense neutron star, or, if the stellar mass was at least three times that of the Sun, a black hole.
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White dwarfs are the remnants of low-mass stars and, if they form a binary system with another star, they can cause large stellar explosions known as type Ia supernova.
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On April 15, 1979, the first type II supernova found in the M100 galaxy was discovered; however the star SN 1979C faded quickly; later observations from x-ray to radio wavelengths revealed its remnant.
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22 sinne gevind in 9 ms. Hulle kom uit baie bronne en word nie nagegaan nie.