emission nebula oor Fins
emission nebula
en
A nebula composed of ionized gases which produce visible light (as distinct from a reflection nebula, which reflects the light produced by neighboring stars).
Vertalings in die woordeboek Engels - Fins
Emissiosumu
en
cloud of ionized gas emitting light of various colors
ionisoituneen vedyn alue
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
voorbeelde
Advanced filtering
Voorbeelde moet herlaai word.
So most people have no idea of the difference between an emission nebula and a planetary nebula.
Tapasimme ennen sotaaQED QED
The North America Nebula (NGC 7000 or Caldwell 20) is an emission nebula in the constellation Cygnus, close to Deneb (the tail of the swan and its brightest star).
Ongelmana on, että yleinen oikeudellinen kehys koostuu säännöistä, joiden sitovuus vaihtelee (asetukset, direktiivit, Euroopan yhteisöjen tuomioistuimen tuomiotWikiMatrix WikiMatrix
This emission nebula visible in the sky even to the naked eye.
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This object is known as an emission nebula.
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This emission nebula visible in the sky even to the naked eye.
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Accordingly, the vast, cloud-like objects that glow with this light from hydrogen (and other) atoms are known as emission nebulae.
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It is an emission nebula, composed of clouds of gas that are made to glow by the radiation emanating from stars within.
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The result is a strikingly colourful emission nebula, called LHA 120-N55, in which the stars are adorned with a mantle of glowing gas.
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Barnard’s Loop, a faint emission nebula thought to be the remnant of a supernova, appears as a faint reddish arc encircling the bright Orion Nebula.
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Star clusters, emission nebulae and active star-forming regions are just some of the riches observed in this region lying some 4000 light-years from Earth.
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NGC 2035 is an HII region, or emission nebula, consisting of clouds of gas that glow due to the energetic radiation given off by young stars.
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In the lower part of this emission nebula, a finger of gas pokes out from the cloud, pointing directly at the central star powering the Trifid.
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Australian astronomer Colin Gum discovered it on photographs taken at the Mount Stromlo Observatory near Canberra, and included it in his catalogue of 84 emission nebulae, published in 1955.
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Emission nebulae like IC 2944 are composed mostly of hydrogen gas that glows in a distinctive shade of red, due to the intense radiation from the many brilliant newborn stars.
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The bluish patch next to the red emission nebula shows the light from the recently formed stars being scattered — reflected in many different directions — by the microscopic particles in the nebula.
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Directly above them, the dazzling constellation of Orion (The Hunter) dominates the view, as giant clouds and arcs of ionised gas — called emission nebulae, and seen here as red patches — encompass the imagined form of mythological hunter.
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The associated nebula containing this clutch of bright stars is known as an emission nebula, meaning that gas within it has been heated up by stars until the gas emits its own light, just like the neon gas used in electric store signs.
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When the green [O III] emission from nebulae was first observed, astronomers thought they had discovered a new element that they dubbed nebulium.
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Below, in the round, pink-reddish area typical of an emission nebula, the gas at the Trifid’s core is heated by hundreds of scorching young stars until it emits the red signature light of hydrogen, the major component of the gas, just as hot neon gas glows red-orange in illuminated signs all over the world.
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“The emission lines of molecules present in the Orion Nebula were transformed into musical notes, transposing the 'chords' from the skies into sound chords.
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At the place of this star we see today a nearly spherical nebula, represented in the Figure above by two grey-scale images (reverse colour scale: dark shading shows bright emission).
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22 sinne gevind in 10 ms. Hulle kom uit baie bronne en word nie nagegaan nie.