emission nebula oor Noorse Bokmål
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 - Noorse Bokmål
emisjonståke
en
cloud of ionized gas emitting light of various colors
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
voorbeelde
Advanced filtering
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The California Nebula (NGC 1499) is an emission nebula located in the constellation Perseus.
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Barnard's Loop (catalogue designation Sh 2-276) is an emission nebula in the constellation of Orion.
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First observed in the late 19th century by Sherburne Wesley Burnham, Herbig–Haro objects were not recognised as being a distinct type of emission nebula until the 1940s.
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Huggins' observations revealed that the nebula's spectrum was non-continuous and made of a few bright emission lines, first indication that planetary nebulae consist of tenuous ionised gas.
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In many planetary nebulae, molecular emission is greatest at larger distances from the star, where more material is un-ionised, but molecular hydrogen emission in NGC 6543 seems to be bright at the inner edge of its outer halo.
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Detail of emission nebula IC 2944, "The Running Chicken", in Centaurus.
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This emission nebula visible in the sky even to the naked eye.
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This is known as an emission nebula.
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This object is known as an emission nebula.
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Emission Nebulae Emission nebulae are clouds of cosmic gas and dust that have been heated by nearby stars.
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Emission nebulae usually glow red or pink, this is because they’re filled with lots of hydrogen gas.
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The Heart Nebula, like most emission nebulas, is inflated like a bubble by newborn stars in its interior.
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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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NGC 7000 is an emission nebula, meaning that its gaseous hydrogen, oxygen and sulphur are strongly irradiated by ultraviolet light from a nearby star.
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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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It is a beautiful example of an emission nebula, in this case an HII region, indicating active formation of new stars, which can be seen peppering this image.
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The objects were first observed in the late 19th century by Sherburne Wesley Burnham, but were not recognised as being a distinct type of emission nebula until the 1940s.
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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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IC 2944, also known as the Running Chicken Nebula or the Centauri Nebula, is an open cluster with an associated emission nebula found in the constellation Centaurus, near the star Centauri.
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IC 2944, also known as the Running Chicken Nebula or the Lambda Centauri Nebula, is an open cluster with an associated emission nebula found in the constellation Centaurus, near the star Lambda Centauri.
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In the centre of the image is the young open cluster NGC 6193, and to the right is the emission nebula NGC 6188, illuminated by the ionising radiation emitted by the brightest nearby stars.
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Sh2-292 is both an emission nebula and a reflection nebula; much of its light is emitted by ionised gas surrounding its nascent stars, but a significant amount is also reflected from stars outside it.
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In the centre of the final image from the VLT Survey Telescope at ESO’s Paranal Observatory is the young open cluster NGC 6193, and to the right is the emission nebula NGC 6188, illuminated by the ionising radiation emitted by the brightest nearby stars.
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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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