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'Nebulosa' images and/or videos results page 1 of 17

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Agrostis nebulosa/Nebulosa Agrostide/Not Japanese
Strix nebulosa
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Echidna nebulosa
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Strix nebulosa
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Neofelis nebulosa/Panthere nebuleuse/Panthere longibande/Clouded leopard
Clouded leopard, Neofelis nebulosa.,1834 (engraving)
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Strix nebulosa/Lapone Owl/Great Gray Owl
Strix nebulosa/Lapone Owl/Great Gray Owl
Strix nebulosa/Lapone Owl/Great Gray Owl
Strix nebulosa/Lapone Owl/Great Gray Owl
The Clouded Tiger, F. Nebulosa, Hand-Colored Engraving, 1825
Neofelis nebulosa/Panthere nebuleuse/Panthere longibande/Clouded leopard
Clouded leopard, Neofelis nebulosa (Felis macrocelis). Vulnerable. Handcoloured steel engraving from Georg Friedrich Treitschke's Gallery of Natural History, Naturhistorischer Bildersaal des Thierreiches, Liepzig-1842.
Clouded Leopard, Neofelis nebulosa, leopard cub standing, front view
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Strix nebulosa/Lapone Owl/Great Grey Owl/Lapland Owl
Side view of Clouded Leopard cub, Neofelis nebulosa, with head facing left in profile
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Japanese Garden/Not Japanese/Agrostis nebulosa/Nebula Agrostid/Alyssum maritimum/Maritime Alyssus
Neofelis nebulosa diardi, plate from A Monograph of the Felidae, or Family of the Cats, by Daniel Giraud Elliot, 1833 (hand-coloured litho)
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Strix nebulosa, great grey owl, Plate 351 from John James Audubon's Birds of America, original double elephant folio, 1827-30 (hand-coloured aquatint)
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Clouded leopard, Neofelis nebulosa (Felis macrocelis). Handcoloured copperplate engraving from Rene Primevere Lesson's Complements de Buffon, Pourrat Freres, Paris, 1838.
Insect: Diptere variety, dark-winged midges with a clematite aristoloche plant. Lithograph by John Curtis (1791-1862) published in “British Entomology”, a collection of 770 illustrations and descriptions of British insects, London, England, 1824 to 1839. Tanypus nebulosus, Anatopynia nebulosa, Clouded-winged Midge, with common birthwort, Aristolochia clematitis. Handcoloured copperplate by John Curtis (1791-1862) for his own “” British Entomology, 770 Illustrations and Descriptions of the Genera of Insects found in Great Britain and Ireland,” London, from 1824 to 1839.
CLOUDED LEOPARD
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The right ascensions and declinations of the principal fixed stars in both hemisphears to year 1678, 1678 (engraving)
Horsehead Nebula (B33) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergeant star belonging to the Orion Baudrier. Towards the center of the image, a reflexion nebula, NGC 2023. The Horsehead Nebula (also known as Barnard 33 in nebula IC 434) is a dark nebula in the Orion constellation at approximately 1,500 light years from Earth. On bottom left of the image is the Flame Nebula (NGC 2024) with star Alnitak which belongs to the Belt of Orion; in the center, the reflection nebula NGC 2023. Dunkelwolke (B33) vor einer HII - Region (Nebel) im Sternbild Orion
Nebulae IC 1283 - 84 and NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - These nebulae are located in Sagittarius at a distance of about 5900 light years from Earth. Image made with Siding Spring's 3.9m telescope. Our view towards the centre of the Galaxy is obscured by extensive clouds of interstellar dust in the direction of the constellation of Sagittarius. The large - scale, patchy nature of the obscuration can be seen with the unaided eye and it is evident on smaller scales from the uneven distribution of background stars across this picture. Light from bright stars within the dust produces the two blue reflection nebulae (NGC 6589 and 6590), and these stars are members of a loose open cluster of stars, NGC 6595 (Sharpless 37) which is at a distance of about 5,900 light years. A large, almost transparent cloud of hydrogen, mixed with traces of dust, glows with a characteristic magenta hue over most of the field of view. This is known as IC 1283, 1284 and 4700 and is likely at a similar distance to NCC 6595
Orion Nebula
Nebula Omega (M17) in Sagittarius - The Omega Nebula (M17) in the constellation Sagittarius - View of the nebula Omega (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. The Omega Nebula, Messier object 17 (M17), NGC 6618, in the constellation Sagittarius is a bright nebula, criss - crossed by clouds and lanes of opaque dust and gas. It is also known as the Swan Nebula and the Horseshoe Nebula. At a distance of 5700 light - years, M17 is also a source of radio noise
Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. This object derives its name from its looped shape reminiscent of the Greek letter when the nebula is seen in a telescope. The gas cloud is unusual in that it does not appear to be illuminated by the bright stars that commonly found in emission nebulae such as this. However, the nebulosity is very bright, so the exciting stars must be hidden within the cloud, an idea confirmed by the infrared brightness of the nebula. It is about 6000 light years distant
Nebula M78 in Orion - M78 nebula in Orion - The nebula M78 (NGC 2068) is located about 1300 years - light from Earth and extends over 4 years - light. M78, (NGC 2068) is part of the Orion complex, a large region of star - forming gas and dust centred around M42 and M43. It is the brightest diffuse reflection nebula in the sky, and fairly easy to see with binoculars (and almost visible to the naked eye, claim some observers). M78 is some 1600 light - years away and around 4 light - years across
The Filamentary Nebula.
Dark Nebula LDN 673 in Aquarius - LDN 673 dark nebula in Aquila - This telescopic close - up looks towards the region at a fragmented Aquila dark cloud complex identified as LDN 673, stretching across a field of view slightly wider than the full moon. In the scene, visible indications of energetic outflows associated with young stars include the small red tinted nebulosity RNO 109 at top left and Herbig - Haro object HH32 above and right of center. The dark clouds in Aquila are estimated to be some 600 light - years away
Cone and Hubble Nebulae in the Unicorn - Cone and Hubble nebulae in Monoceros - The Cone nebula, at the bottom left, is an H II region located about 2600 years - light from Earth. The bright star in the middle left is S Monocerotis, a star of magnitude 4.7. Lower right, the Hubble nebula, overexposed. This large area of emission nebulosity and patch of blue reflection nebulosity also contains the Cone Nebula, a dark nebula at the lower right corner of the red nebulae. At the bottom right of the frame is NGC 2261, Hubble's Variable Nebula, in this image looking like an overexposed mis - shaped star because of the extreme processing needed to bring out the faint nebulosity in the Cone Nebula
Nebula NGC 3372 in Carene - Nebula NGC 3372 in Carina - The nebula of the Carene is located about 7000 years - light from Earth. It is home to many hot stars, including the star Eta Carinae (on the left, the brightest star in the picture). In the right center, a cluster of young stars, Trumpler 14. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372). The bright star on the left of the image is Eta Carinae, which is one of the most massive and luminous stars known
Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Trifid is located in Sagittarius constellation between 5000 and 10 000 light - years away
Eagle Nebula (IC 4703) and star cluster M16 in the Snake - This wide - field image of the Eagle Nebula was taken at the National Science Foundation's 0.9 - meter telescope on Kitt Peak with the NOAO Mosaic CCD camera. Located in the constellation of Serpens, the Serpent, the Eagle Nebula is a very luminous open cluster of stars surrounded by dust and gas. The three pillars at the center of the image, made famous in an image by the Hubble Space Telescope, are being sculpted by the intense radiation from the hot stars in the cluster. This image was created by combining emission - line images in Hydrogen - alpha (green), Oxygen [O III] (blue) and Sulfur [S II] (red)
Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Trifid is located in Sagittarius constellation between 5000 and 10 000 light - years away
Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Measuring some forty light years across, this nebula contains enough gas to make many thousands of suns. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Trifid is located in Sagittarius constellation between 5000 and 10 000 light - years away
Horse's Head Nebula - The Horsehead nebula in Orion - The Horse's Head Nebula, Barnard 33, is a dark nebula located in front of the IC 434 emission nebula at about 1500 years - light of the Earth in the constellation Orion. Lower left is the reflexion nebula, NGC 2023. The Horsehead nebula is located in the constellation of Orion, slightly below the left - most star of the three that form the Hunter's belt. It is part of a vast molecular cloud of dust and gas that includes the Great Orion Nebula and extends throughout the entire constellation as well. Here we see the Horsehead as it appeared 1,500 years ago, due to distance and the time it takes light to travel
Orion Nebula (M42 - 43) - The Orion Nebula - Located 1500 years ago - the Orion Nebula is the closest region to the formation of stars of the Sun. Image obtained with Siding Spring's 3.9m telescope. The Orion Nebula is famous for a number of reasons. It is the nearest bright nebula to us and can be seen with the naked eye. Its brightness led to it being the first nebula ever photographed (in 1882) and its proximity (1500 light years) means that we know more about it than any other star - forming region. It is also in a very active stage of star formation and it is perfectly placed for us to explore the intimate details of the birth of stars. The inner regions are glowing mainly in the red light of excited hydrogen, which together with some green emission from oxygen give the centre of the nebula a yellowish colour. The energy for this spectacular display comes from the small cluster of stars in the brightest part of the nebula. Three, five - minute exposures were used to make this picture using the Anglo - Australian Telescope at Siding Spring
Barnard's Loop detail and M78 nebula in Orion - Barnard's Loop detail and M78 nebula in Orion - Barnard's Loop is a very low emission nebula, very large, that surrounds the great Orion nebula. Here, the brightest part of the Loop, with lower left the cluster of stars NGC 2112, and to the right the nebula by refexion M78. Also visible is a dark nebula LDN 1622 at the top left of the image. Barnard's Loop is an extremely faint emission nebula which is part of an amazing, even larger complex of nebulosity in the constellation of Orion. This photo shows only the brightest central portion of the loop which runs diagonally across the frame here from lower left to upper right. NGC 2112, a ninth magnitude open cluster 11 arc minutes in diameter and containing about 50 stars, is seen at lower left - center, and reflection nebulae M78 and NGC 2071 are at lower right. An interesting dark nebula, LDN 1622, lies at the upper left of the image, surrounded by very faint emission nebulosity, with a hint of reflection nebulosity on the outlying western edge
Nebula NGC 6334 in Scorpio - Cat's Paw nebula (NGC 6334) in Scorpius - The nebula NGC 6334 is located about 5500 years - light from Earth. Image made with a 130 mm Astrophysics bezel, one hour of laying. NGC 6334 is the Cat's Paw nebula in Scorpius.It is a large area of emission nebulosity more than a half of a degree in size located about 3 degrees northwest of Lambda and Upsilon Scorpii, the stinger in the Scorpion's tail, which are also called the Cat's Eyes. To the upper left of NGC 6334 is an area almost devoid of stars which is dark nebula B 257. Radio source RCW 127 is also located in NGC 6334
Nebulae of the horse's head and M42 in Orion - Horsead nebula and Orion nebula - Dark Nebula of the horse's head (IC434 - B33). On the right, the large Orion nebula (M42) is a vast region of star formation. This large complex of nebulosity is located about 1,500 light years away in Orion. The Orion complex is a gigantic stellar nursery where stars are forming out of the dust and gas in the region. Young energetic stars excite the gas in the region ionizing it and causing it to glow in the hydrogen - alpha and oxygen III emission lines. The brightest star in the photo at left at magnitude 1.8 is Alnilam, the middle star of the three distinctive stars in the belt of Orion. At the bottom is the Flame, NGC 2024, and the dark nebula B33, the Horsehead Nebula. Top right is a patch of blue reflection nebulosity NGC 1973 - 4 - 5 and the beautiful Orion Nebula, M 42
Orion Nebula - M42 - M43 - The Great Nebula in Orion - Located 1500 years - light, the Orion Nebula is the closest region to the formation of stars of the Sun. The Orion Nebula is the greatest of all HII clouds visible from our location within the Milky Way. With a gaseous repository of 10,000 suns, and illuminated by a cluster of hot young stars, the clouds of M42 glow with fantastic colors and shapes, giving us a birds eye view of one of the greatest star forming nurseries in our part of the galaxy. At a distance of 1500 light years, the Orion nebula is the nearest star - forming region to the Sun
Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained with a telescope of 61 cm. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name. Image taken with a 24 - inch telescope
Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained with a bezel Astro - Physics 130 EDT, 12x6min of poses. M20, The Trifid Nebula, in the constellation of Sagittarius, is a remarkable object - large, bright and beautiful. It is a complex of red emission, blue reflection, and dark nebulae about the size of the full moon. It was shot at 1,000 mm of focal length with 130 mm of aperture at f/8 (Astro - Physics 130EDT apochromatic refractor) with a Canon 20Da DSLR and only 12 x 6 minutes of exposure at ISO 1600
Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star with a brightness 35,000 times greater than the Sun. Its mass is 20 times the solar mass. Partly obscured by the glare of zeta is the curious yellowish nebula NGC 2024, whose energy comes from stars hidden in the dark lane, while other nebulae simply reflect the light of embedded hot stars and appear blue. All these objects are about 1500 light years distant
Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the Trifide nebula (M20 or NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Trifid nebula is located in Sagittarius constellation between 5000 and 10 000 light - years away. Stars, the Sun included, were born within clouds of dusty gas such as the Trifid Nebula. Within it a number of young hot stars have already formed. The hottest cause the gas, mostly hydrogen, to emit its characteristic red light. Around the red emission nebula the gas contains many dust grains which preferentially reflect the blue component of starlight, and to the north (top) of the nebula can be seen a bright star which illuminates part of the dust to create a region of blue reflection. In some parts of the nebula there are so many dust grains that they hide the glowing gas, producing the three dark lanes which give the object its name
Spiral nebula Messier 51
Horsehead Nebula (B33) in Orion - Horsehead nebula in Orion - The horse head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emission nebula about 1500 years - light of the Earth in the constellation Orion. Lower left is the reflexion nebula, NGC 2023. This curious dark nebula is one of the best - known images in astronomy, probably because of its chance likeness to a recognisable form. The horse - head shape is an extension of a large cloud of dust which fills the lower part (east) of the picture and hides the light of stars beyond. The outer surface of the dusty gas (IC 434) runs roughly north - south and is illuminated by sigma Orionis (off the top of the picture) which causes the hydrogen there to fluoresce, outlining the horse - head shape. The diffuse haze to the left of the image (north) is scattered light from the bright star zeta Orionis. Though conspicuous here, the Horsehead is very difficult to see visually, even with a large telescope. A bright star is partially enveloped in the dust cloud and its scattered light is seen as the large, irregular blue reflection nebula, NGC 2023. All these objects are about 1500 light years distant
Nebulae NGC 2024 and Horse's Head - Flame nebula and the Horsehead Nebula - This image shows the nebula NGC 2024 (left), the small nebula NGC 2023 (right middle) and the nebula of the horse's head (top right). The bright star on the top left is the star Alnitak. Visible infrared composite image. This image shows the spectacular star - forming region known as the Flame Nebula, or NGC 2024, in the constellation of Orion (the Hunter) and its surroundings. The view also includes the glow of the reflection nebula NGC 2023, middle right, and the ghostly outline of the Horsehead Nebula (Barnard 33) towards the upper right. The bright bluish star top left is one of the three bright stars forming the Belt of Orion, Alnitak. The image was created from VISTA in the near - infrared part of the spectrum and optical datas
Horsehead Nebula (IC 434) in Orion - Horsehead Nebula (B33) in Orion - The horse's head nebula, Barnard 33, is a dark nebula located in front of the IC 434 emitting nebula about 1500 years - light from Earth in the constellation Orion. At the bottom left, the nebula NGC 2024 with just above the star Alnitak, a supergiant star belonging to the Baudrier of Orion. Towards the center of the image, a reflexion nebula, NGC 2023. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. This distinctive red emission nebula (IC 434) is the result of radiation from sigma Orionis interacting with the surface of a dusty cloud of gas from which projects the dark shape of the head of a horse. Sigma is the second brightest star in the picture and is at about the same distance from the Sun as the nebula. The brightest star here is zeta Orionis, easily visible to the unaided eye as the easternmost star in the line of three which form Orion's Belt. Alnitak (Zeta Orionis) is a supergiant star with a brightness 35,000 times greater than the Sun. Its mass is 20 times the solar mass. Partly obscured by the glare of zeta is the curious yellowish nebula NGC 2024, whose energy comes from stars hidden in the dark lane, while other nebulae simply reflect the light of embedded hot stars and appear blue. All these objects are about 1500 light years distant. This photograph was produced by combining three separate photographs taken with the 1.2m UK Schmidt Telescope through different coloured filters
Nebula IC 1274 in Sagittariu - Nebula IC 1274 in Sagittariu