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Nebula M43 in Orion - M43 nebula in Orion - Nebula M43 (NGC 1982) is part of the great Nebula of Orion (M42), a vast region of star formation. This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula people of bright young stars accompanied by very young stars still surrounded by their cocoon of dust. The NASA/ESA Hubble Space Telescope has taken a close - up view of an outer part of the Orion Nebula's little brother, Messier 43. This nebula, which is sometimes referred to as De Mairan's Nebula after its discoverer, is separated from the famous Orion Nebula (Messier 42) by only a dark lane of dust. Both nebulae are part of the massive stellar nursery called the Orion molecular cloud complex, which includes several other nebulae, such as the Horsehead Nebula (Barnard 33) and the Flame Nebula (NGC 2024). This view shows several of the brilliant hot young stars in this less - studied region and it also reveals many of the curious features around even younger stars that are still cocooned by dust. This picture was created from images taken using the Wide Field Channel of Hubble's Advanced Camera for Surveys. Images through yellow (F555W, coloured blue) and near - infrared (F814W, coloured red) filters were combined. The exposure times were 1000 s per filter and the field of view is about 3.3 arcminutes across
Nebula M43 in Orion - M43 nebula in Orion - Nebula M43 (NGC 1982) is part of the great Nebula of Orion (M42), a vast region of star formation. This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula people of bright young stars accompanied by very young stars still surrounded by their cocoon of dust. The NASA/ESA Hubble Space Telescope has taken a close - up view of an outer part of the Orion Nebula's little brother, Messier 43. This nebula, which is sometimes referred to as De Mairan's Nebula after its discoverer, is separated from the famous Orion Nebula (Messier 42) by only a dark lane of dust. Both nebulae are part of the massive stellar nursery called the Orion molecular cloud complex, which includes several other nebulae, such as the Horsehead Nebula (Barnard 33) and the Flame Nebula (NGC 2024). This view shows several of the brilliant hot young stars in this less - studied region and it also reveals many of the curious features around even younger stars that are still cocooned by dust. This picture was created from images taken using the Wide Field Channel of Hubble's Advanced Camera for Surveys. Images through yellow (F555W, coloured blue) and near - infrared (F814W, coloured red) filters were combined. The exposure times were 1000 s per filter and the field of view is about 3.3 arcminutes across

PIX4618093: Nebula M43 in Orion - M43 nebula in Orion - Nebula M43 (NGC 1982) is part of the great Nebula of Orion (M42), a vast region of star formation. This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula people of bright young stars accompanied by very young stars still surrounded by their cocoon of dust. The NASA/ESA Hubble Space Telescope has taken a close - up view of an outer part of the Orion Nebula's little brother, Messier 43. This nebula, which is sometimes referred to as De Mairan's Nebula after its discoverer, is separated from the famous Orion Nebula (Messier 42) by only a dark lane of dust. Both nebulae are part of the massive stellar nursery called the Orion molecular cloud complex, which includes several other nebulae, such as the Horsehead Nebula (Barnard 33) and the Flame Nebula (NGC 2024). This view shows several of the brilliant hot young stars in this less - studied region and it also reveals many of the curious features around even younger stars that are still cocooned by dust. This picture was created from images taken using the Wide Field Channel of Hubble's Advanced Camera for Surveys. Images through yellow (F555W, coloured blue) and near - infrared (F814W, coloured red) filters were combined. The exposure times were 1000 s per filter and the field of view is about 3.3 arcminutes across / Bridgeman Images

ID: PIX4618093

Nebula M43 in Orion - M43 nebula in Orion - Nebula M43 (NGC 1982) is part of the great Nebula of Orion (M42), a vast region of star formation. This image obtained by the Hubble Space Telescope (HST) shows a detail of the nebula people of bright young stars accompanied by very young stars still surrounded by their cocoon of dust. The NASA/ESA Hubble Space Telescope has taken a close - up view of an outer part of the Orion Nebula's little brother, Messier 43. This nebula, which is sometimes referred to as De Mairan's Nebula after its discoverer, is separated from the famous Orion Nebula (Messier 42) by only a dark lane of dust. Both nebulae are part of the massive stellar nursery called the Orion molecular cloud complex, which includes several other nebulae, such as the Horsehead Nebula (Barnard 33) and the Flame Nebula (NGC 2024). This view shows several of the brilliant hot young stars in this less - studied region and it also reveals many of the curious features around even younger st

Common purple clover, red clover or honeysuckle trefoil, Trifolium pratense. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.
Common purple clover, red clover or honeysuckle trefoil, Trifolium pratense. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

FLO4618125: Common purple clover, red clover or honeysuckle trefoil, Trifolium pratense. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816. / Bridgeman Images

ID: FLO4618125

Common purple clover, red clover or honeysuckle trefoil, Trifolium pratense. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

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
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

PIX4618132: 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 / Bridgeman Images

ID: PIX4618132

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

Nebula M78 in Orion - M78 nebula in Orion - The nebula M78 (NGC 2068) is located about 1600 years - light from Earth and extends over 4 years - light. Image obtained with a telescope 61 cm in diameter. M78 (NGC 2068) is a reflection nebula in the constellation Orion at about 1,600 light years away. Image obtained with a RC 24”” telescope
Nebula M78 in Orion - M78 nebula in Orion - The nebula M78 (NGC 2068) is located about 1600 years - light from Earth and extends over 4 years - light. Image obtained with a telescope 61 cm in diameter. M78 (NGC 2068) is a reflection nebula in the constellation Orion at about 1,600 light years away. Image obtained with a RC 24”” telescope

PIX4618171: Nebula M78 in Orion - M78 nebula in Orion - The nebula M78 (NGC 2068) is located about 1600 years - light from Earth and extends over 4 years - light. Image obtained with a telescope 61 cm in diameter. M78 (NGC 2068) is a reflection nebula in the constellation Orion at about 1,600 light years away. Image obtained with a RC 24”” telescope / Bridgeman Images

ID: PIX4618171

Nebula M78 in Orion - M78 nebula in Orion - The nebula M78 (NGC 2068) is located about 1600 years - light from Earth and extends over 4 years - light. Image obtained with a telescope 61 cm in diameter. M78 (NGC 2068) is a reflection nebula in the constellation Orion at about 1,600 light years away. Image obtained with a RC 24”” telescope

Marsh St. John 's-Wort, Hypericum elodes. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.
Marsh St. John 's-Wort, Hypericum elodes. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

FLO4618189: Marsh St. John 's-Wort, Hypericum elodes. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816. / Bridgeman Images

ID: FLO4618189

Marsh St. John 's-Wort, Hypericum elodes. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula - The Tarantula Nebula (or 30 Sea bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with the large field camera of the 2.2m ESO/MPG telescope in Chile. Composite colour image of the Tarantula Nebula in the Large Magellanic Cloud (LMC) and its surroundings. The LMC is a satellite galaxy to our Milky Way system, located in the southern constellation Dorado (The Swordfish) at a distance of approximately 170,000 light - years. The image is based on 15 exposures in the visual part of the spectrum with the Wide Field Imager (WFI) camera on the 2.2 - m MPG/ESO telescope at the La Silla Observatory
Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula - The Tarantula Nebula (or 30 Sea bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with the large field camera of the 2.2m ESO/MPG telescope in Chile. Composite colour image of the Tarantula Nebula in the Large Magellanic Cloud (LMC) and its surroundings. The LMC is a satellite galaxy to our Milky Way system, located in the southern constellation Dorado (The Swordfish) at a distance of approximately 170,000 light - years. The image is based on 15 exposures in the visual part of the spectrum with the Wide Field Imager (WFI) camera on the 2.2 - m MPG/ESO telescope at the La Silla Observatory

PIX4618203: Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula - The Tarantula Nebula (or 30 Sea bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with the large field camera of the 2.2m ESO/MPG telescope in Chile. Composite colour image of the Tarantula Nebula in the Large Magellanic Cloud (LMC) and its surroundings. The LMC is a satellite galaxy to our Milky Way system, located in the southern constellation Dorado (The Swordfish) at a distance of approximately 170,000 light - years. The image is based on 15 exposures in the visual part of the spectrum with the Wide Field Imager (WFI) camera on the 2.2 - m MPG/ESO telescope at the La Silla Observatory / Bridgeman Images

ID: PIX4618203

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula - The Tarantula Nebula (or 30 Sea bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with the large field camera of the 2.2m ESO/MPG telescope in Chile. Composite colour image of the Tarantula Nebula in the Large Magellanic Cloud (LMC) and its surroundings. The LMC is a satellite galaxy to our Milky Way system, located in the southern constellation Dorado (The Swordfish) at a distance of approximately 170,000 light - years. The image is based on 15 exposures in the visual part of the spectrum with the Wide Field Imager (WFI) camera on the 2.2 - m MPG/ESO telescope at the La Silla Observatory

Tarantula Nebula (NGC 2070) in the constellation of Bream - The Tarantula Nebula in Dorado - Tarantula Nebula in the large Magellan cloud seen with the FORS2 instrument on the KUEYEN telescope (VLT) February 1, 2000. The Tarantula Nebula (or 30 bream) is the largest star-forming region of the Magellan Grand Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. The Tarantula Nebula in the Large Magellanic Cloud, as obtained with FORS2 at KUEYEN (VLT) on the night of January 31 - February 1, 2000. It is a composite of three exposures
Tarantula Nebula (NGC 2070) in the constellation of Bream - The Tarantula Nebula in Dorado - Tarantula Nebula in the large Magellan cloud seen with the FORS2 instrument on the KUEYEN telescope (VLT) February 1, 2000. The Tarantula Nebula (or 30 bream) is the largest star-forming region of the Magellan Grand Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. The Tarantula Nebula in the Large Magellanic Cloud, as obtained with FORS2 at KUEYEN (VLT) on the night of January 31 - February 1, 2000. It is a composite of three exposures

PIX4618210: Tarantula Nebula (NGC 2070) in the constellation of Bream - The Tarantula Nebula in Dorado - Tarantula Nebula in the large Magellan cloud seen with the FORS2 instrument on the KUEYEN telescope (VLT) February 1, 2000. The Tarantula Nebula (or 30 bream) is the largest star-forming region of the Magellan Grand Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. The Tarantula Nebula in the Large Magellanic Cloud, as obtained with FORS2 at KUEYEN (VLT) on the night of January 31 - February 1, 2000. It is a composite of three exposures / Bridgeman Images

ID: PIX4618210

Tarantula Nebula (NGC 2070) in the constellation of Bream - The Tarantula Nebula in Dorado - Tarantula Nebula in the large Magellan cloud seen with the FORS2 instrument on the KUEYEN telescope (VLT) February 1, 2000. The Tarantula Nebula (or 30 bream) is the largest star-forming region of the Magellan Grand Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. The Tarantula Nebula in the Large Magellanic Cloud, as obtained with FORS2 at KUEYEN (VLT) on the night of January 31 - February 1, 2000. It is a composite of three exposures

Sneezewort yarrow, Achillea ptarmica. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Claves and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.
Sneezewort yarrow, Achillea ptarmica. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Claves and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

FLO4618226: Sneezewort yarrow, Achillea ptarmica. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Claves and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816. / Bridgeman Images

ID: FLO4618226

Sneezewort yarrow, Achillea ptarmica. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Claves and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

Marigold, Calendula officinalis. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.
Marigold, Calendula officinalis. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

FLO4618234: Marigold, Calendula officinalis. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816. / Bridgeman Images

ID: FLO4618234

Marigold, Calendula officinalis. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

Great globe thistle, Echinops sphaerocephalus (Sea urchin with round heads) Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.
Great globe thistle, Echinops sphaerocephalus (Sea urchin with round heads) Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

FLO4618244: Great globe thistle, Echinops sphaerocephalus (Sea urchin with round heads) Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816. / Bridgeman Images

ID: FLO4618244

Great globe thistle, Echinops sphaerocephalus (Sea urchin with round heads) Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

Tarantula (NGC 2070) in the LMC - The nebula around 30 Doradus (NGC 2070) in the LMC - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. The brightest cluster of stars in this picture was believed until recently to contain a single, uniquely massive object with the mass equivalent to 1000 suns, and was named as a star, 30 Doradus. Sophisticated image analysis techniques have been used to show that 30 Doradus is a very compact group of stars, many of which are massive, but not unimaginably so. The radiation from this star cluster is sufficient to excite a huge cloud of hydrogen gas in its vicinity so that it glows with its distinctive red colour. This picture is essentially a one minute exposure. A longer exposure would show that the curving tendrils of nebulosity are the brightest parts of the huge Tarantula nebula, one of the largest star - forming regions known anywhere
Tarantula (NGC 2070) in the LMC - The nebula around 30 Doradus (NGC 2070) in the LMC - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. The brightest cluster of stars in this picture was believed until recently to contain a single, uniquely massive object with the mass equivalent to 1000 suns, and was named as a star, 30 Doradus. Sophisticated image analysis techniques have been used to show that 30 Doradus is a very compact group of stars, many of which are massive, but not unimaginably so. The radiation from this star cluster is sufficient to excite a huge cloud of hydrogen gas in its vicinity so that it glows with its distinctive red colour. This picture is essentially a one minute exposure. A longer exposure would show that the curving tendrils of nebulosity are the brightest parts of the huge Tarantula nebula, one of the largest star - forming regions known anywhere

PIX4618266: Tarantula (NGC 2070) in the LMC - The nebula around 30 Doradus (NGC 2070) in the LMC - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. The brightest cluster of stars in this picture was believed until recently to contain a single, uniquely massive object with the mass equivalent to 1000 suns, and was named as a star, 30 Doradus. Sophisticated image analysis techniques have been used to show that 30 Doradus is a very compact group of stars, many of which are massive, but not unimaginably so. The radiation from this star cluster is sufficient to excite a huge cloud of hydrogen gas in its vicinity so that it glows with its distinctive red colour. This picture is essentially a one minute exposure. A longer exposure would show that the curving tendrils of nebulosity are the brightest parts of the huge Tarantula nebula, one of the largest star - forming regions known anywhere / Bridgeman Images

ID: PIX4618266

Tarantula (NGC 2070) in the LMC - The nebula around 30 Doradus (NGC 2070) in the LMC - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. The brightest cluster of stars in this picture was believed until recently to contain a single, uniquely massive object with the mass equivalent to 1000 suns, and was named as a star, 30 Doradus. Sophisticated image analysis techniques have been used to show that 30 Doradus is a very compact group of stars, many of which are massive, but not unimaginably so. The radiation from this star cluster is sufficient to excite a huge cloud of hydrogen gas in its vicinity so that it glows with its distinctive red colour. This picture is essentially a one minute exposure. A longer

Tarantula Nebula in the Great Magellan Cloud - Tarantula nebula (NGC 2070) in Dorado - NGC 2070, the Tarantula Nebula is a vast star-forming region located north of the Great Magellan Cloud galaxy, in the southern hemisphere about 170,000 years - light from Earth. Image obtained by combining light through different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min). The largest emission nebula in the sky, the Tarantula Nebula (also known as NGC 2070 or 30 Doradus) is located in the Large Magellanic Cloud (LMC) in the southern hemisphere at about 170,000 light year from Earth. Image obtained with different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min)
Tarantula Nebula in the Great Magellan Cloud - Tarantula nebula (NGC 2070) in Dorado - NGC 2070, the Tarantula Nebula is a vast star-forming region located north of the Great Magellan Cloud galaxy, in the southern hemisphere about 170,000 years - light from Earth. Image obtained by combining light through different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min). The largest emission nebula in the sky, the Tarantula Nebula (also known as NGC 2070 or 30 Doradus) is located in the Large Magellanic Cloud (LMC) in the southern hemisphere at about 170,000 light year from Earth. Image obtained with different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min)

PIX4618301: Tarantula Nebula in the Great Magellan Cloud - Tarantula nebula (NGC 2070) in Dorado - NGC 2070, the Tarantula Nebula is a vast star-forming region located north of the Great Magellan Cloud galaxy, in the southern hemisphere about 170,000 years - light from Earth. Image obtained by combining light through different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min). The largest emission nebula in the sky, the Tarantula Nebula (also known as NGC 2070 or 30 Doradus) is located in the Large Magellanic Cloud (LMC) in the southern hemisphere at about 170,000 light year from Earth. Image obtained with different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min) / Bridgeman Images

ID: PIX4618301

Tarantula Nebula in the Great Magellan Cloud - Tarantula nebula (NGC 2070) in Dorado - NGC 2070, the Tarantula Nebula is a vast star-forming region located north of the Great Magellan Cloud galaxy, in the southern hemisphere about 170,000 years - light from Earth. Image obtained by combining light through different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min). The largest emission nebula in the sky, the Tarantula Nebula (also known as NGC 2070 or 30 Doradus) is located in the Large Magellanic Cloud (LMC) in the southern hemisphere at about 170,000 light year from Earth. Image obtained with different filters (SII 5x 2min, Ha 20x 2min, [OIII] 11x 2min, H - beta 10x 2min, L (IR) 2x 2min, IR 4x 2min, R 8x 2min, G 5x 2min)

Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula, NGC 2070, is a vast star-forming region located north of the Great Magellan Cloud galaxy in the southern hemisphere about 170,000 years - light from Earth. Image obtained with Siding Spring's 3.9m telescope. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a monstrous stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula contains some of the most massive stars known
Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula, NGC 2070, is a vast star-forming region located north of the Great Magellan Cloud galaxy in the southern hemisphere about 170,000 years - light from Earth. Image obtained with Siding Spring's 3.9m telescope. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a monstrous stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula contains some of the most massive stars known

PIX4618312: Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula, NGC 2070, is a vast star-forming region located north of the Great Magellan Cloud galaxy in the southern hemisphere about 170,000 years - light from Earth. Image obtained with Siding Spring's 3.9m telescope. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a monstrous stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula contains some of the most massive stars known / Bridgeman Images

ID: PIX4618312

Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula, NGC 2070, is a vast star-forming region located north of the Great Magellan Cloud galaxy in the southern hemisphere about 170,000 years - light from Earth. Image obtained with Siding Spring's 3.9m telescope. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a monstrous stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula contains some of the most massive stars known

Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula, NGC 2070, is a vast star-forming region located north of the Great Magellan Cloud galaxy in the southern hemisphere about 170,000 years - light from Earth. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a monstrous stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula contains some of the most massive stars known
Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula, NGC 2070, is a vast star-forming region located north of the Great Magellan Cloud galaxy in the southern hemisphere about 170,000 years - light from Earth. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a monstrous stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula contains some of the most massive stars known

PIX4618320: Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula, NGC 2070, is a vast star-forming region located north of the Great Magellan Cloud galaxy in the southern hemisphere about 170,000 years - light from Earth. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a monstrous stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula contains some of the most massive stars known / Bridgeman Images

ID: PIX4618320

Around the Tarantula Nebula - Around the Tarantula nebula in the Large Magellanic Cloud - The Tarantula Nebula, NGC 2070, is a vast star-forming region located north of the Great Magellan Cloud galaxy in the southern hemisphere about 170,000 years - light from Earth. Image obtained with the 1.2m Schmidt UK Telescope from Siding Spring. Known as the Tarantula Nebula for its spidery appearance, the 30 Doradus complex is a monstrous stellar factory. It is the largest emission nebula in the sky, and can be seen far down in the southern sky at a distance of about 170,000 light - years, in the southern constellation Dorado. It is part of one of the Milky Way's neighbouring galaxies, the Large Magellanic Cloud. The Tarantula Nebula contains some of the most massive stars known

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud
Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

PIX4618377: Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud / Bridgeman Images

ID: PIX4618377

Nebula NGC 2170 in Unicorn - Nebula NGC 2170 in Monoceros - Nebula by reflexion located in the constellation Unicorn. This rich collection of predominantly reflection and sparse emission nebulosity exists in the western part of a vast star forming region known as the Mon R 2 association. The “” R”” designation stands for reflection and indicates an association of stars illuminating reflection nebulae. Most of the members of Mon R 2 are type B stars located along an east - west line stretching across 2 degrees of the winter sky, situated about 8 degrees east of the Orion Nebula. The Mon R 2 association resides at a distance of 830 pc and formed about 6 to 10 million years ago along the edge of the Mon R2 molecular cloud

Rosette nebula (NGC 2237) in the Unicorn - The Rosette nebula in Monoceros - The Rosette nebula is a vast cloud of dust and gas. In its center, the cluster of stars NGC 2244. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The north is at top. Discovered by John Flamsteed about 1690, the Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. Star formation is still in progress in this vast cloud of interstellar matter. Although various values for its distance occur in the literature, an avarage value of about 5,500 light - years is generally accepted. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory
Rosette nebula (NGC 2237) in the Unicorn - The Rosette nebula in Monoceros - The Rosette nebula is a vast cloud of dust and gas. In its center, the cluster of stars NGC 2244. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The north is at top. Discovered by John Flamsteed about 1690, the Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. Star formation is still in progress in this vast cloud of interstellar matter. Although various values for its distance occur in the literature, an avarage value of about 5,500 light - years is generally accepted. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory

PIX4618434: Rosette nebula (NGC 2237) in the Unicorn - The Rosette nebula in Monoceros - The Rosette nebula is a vast cloud of dust and gas. In its center, the cluster of stars NGC 2244. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The north is at top. Discovered by John Flamsteed about 1690, the Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. Star formation is still in progress in this vast cloud of interstellar matter. Although various values for its distance occur in the literature, an avarage value of about 5,500 light - years is generally accepted. This image is based on data acquired by the Oschin Telescope at the Mount Palomar Observatory / Bridgeman Images

ID: PIX4618434

Rosette nebula (NGC 2237) in the Unicorn - The Rosette nebula in Monoceros - The Rosette nebula is a vast cloud of dust and gas. In its center, the cluster of stars NGC 2244. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The north is at top. Discovered by John Flamsteed about 1690, the Rosetta Nebula is a vast cloud of dust and gas, extending over an area of more than 1 degree across, or about 5 times the area covered by the full moon. Within the nebula, open star cluster NGC 2244 is situated, consisted of the young stars which recently formed from the nebula's material, and the brightest of which make the nebula shine by exciting its atoms to emit radiation. Star formation is still in progress in this vast cloud of interstellar matter. Although various values for its distance occur in the literature, an avarage value of about 5,500 light - years is generally accepted. This image is based on data acquired by the Oschin Telescope at the Mo

The Rosette Nebula in the Unicorn - The Rosette Nebula and NGC 2244 cluster - The Rosette Nebula is a vast cloud of dust and gas located about 5500 years from Earth. Towards the center of the nebula, a cluster of blue stars, NGC 2244 formed less than a million years ago. Image obtained by Siding Spring's 3.9m telescope. In the hollowed - out centre of the Rosette nebula lies NGC 2244, the cluster of young stars recently formed there. The cluster has itself created the cavity, radiation pressure and stellar winds from the stars blowing the gas and dust away from the young cluster. The hottest (and brightest) members of the group are seen as distinctly blue on this photograph, a colour corresponding to a surface temperature around 20,000K which may be compared with the Sun's 5500K. The nebula and its cluster is at a distance of about 4500 light years and shows many streaks and globules of dust, remnants of the cloud from which the stars formed
The Rosette Nebula in the Unicorn - The Rosette Nebula and NGC 2244 cluster - The Rosette Nebula is a vast cloud of dust and gas located about 5500 years from Earth. Towards the center of the nebula, a cluster of blue stars, NGC 2244 formed less than a million years ago. Image obtained by Siding Spring's 3.9m telescope. In the hollowed - out centre of the Rosette nebula lies NGC 2244, the cluster of young stars recently formed there. The cluster has itself created the cavity, radiation pressure and stellar winds from the stars blowing the gas and dust away from the young cluster. The hottest (and brightest) members of the group are seen as distinctly blue on this photograph, a colour corresponding to a surface temperature around 20,000K which may be compared with the Sun's 5500K. The nebula and its cluster is at a distance of about 4500 light years and shows many streaks and globules of dust, remnants of the cloud from which the stars formed

PIX4618457: The Rosette Nebula in the Unicorn - The Rosette Nebula and NGC 2244 cluster - The Rosette Nebula is a vast cloud of dust and gas located about 5500 years from Earth. Towards the center of the nebula, a cluster of blue stars, NGC 2244 formed less than a million years ago. Image obtained by Siding Spring's 3.9m telescope. In the hollowed - out centre of the Rosette nebula lies NGC 2244, the cluster of young stars recently formed there. The cluster has itself created the cavity, radiation pressure and stellar winds from the stars blowing the gas and dust away from the young cluster. The hottest (and brightest) members of the group are seen as distinctly blue on this photograph, a colour corresponding to a surface temperature around 20,000K which may be compared with the Sun's 5500K. The nebula and its cluster is at a distance of about 4500 light years and shows many streaks and globules of dust, remnants of the cloud from which the stars formed / Bridgeman Images

ID: PIX4618457

The Rosette Nebula in the Unicorn - The Rosette Nebula and NGC 2244 cluster - The Rosette Nebula is a vast cloud of dust and gas located about 5500 years from Earth. Towards the center of the nebula, a cluster of blue stars, NGC 2244 formed less than a million years ago. Image obtained by Siding Spring's 3.9m telescope. In the hollowed - out centre of the Rosette nebula lies NGC 2244, the cluster of young stars recently formed there. The cluster has itself created the cavity, radiation pressure and stellar winds from the stars blowing the gas and dust away from the young cluster. The hottest (and brightest) members of the group are seen as distinctly blue on this photograph, a colour corresponding to a surface temperature around 20,000K which may be compared with the Sun's 5500K. The nebula and its cluster is at a distance of about 4500 light years and shows many streaks and globules of dust, remnants of the cloud from which the stars formed

Common arrowhead, Sagittaria sagittifolia. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Claves and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.
Common arrowhead, Sagittaria sagittifolia. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Claves and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

FLO4618461: Common arrowhead, Sagittaria sagittifolia. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Claves and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816. / Bridgeman Images

ID: FLO4618461

Common arrowhead, Sagittaria sagittifolia. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Claves and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

Rosette and Cone Nebulae - The Cone and Rosette region - Large field image of the Cone nebula (centre left) and the Rosette nebula (top right), in the constellation Unicorn. This wide field image shows the rich colorful Cone nebula region (at the center - left of the image) and the Rosette Nebula (at the top right). They are both located in the Monoceros constellation, very close to the better known Orion constellation
Rosette and Cone Nebulae - The Cone and Rosette region - Large field image of the Cone nebula (centre left) and the Rosette nebula (top right), in the constellation Unicorn. This wide field image shows the rich colorful Cone nebula region (at the center - left of the image) and the Rosette Nebula (at the top right). They are both located in the Monoceros constellation, very close to the better known Orion constellation

PIX4618480: Rosette and Cone Nebulae - The Cone and Rosette region - Large field image of the Cone nebula (centre left) and the Rosette nebula (top right), in the constellation Unicorn. This wide field image shows the rich colorful Cone nebula region (at the center - left of the image) and the Rosette Nebula (at the top right). They are both located in the Monoceros constellation, very close to the better known Orion constellation / Bridgeman Images

ID: PIX4618480

Rosette and Cone Nebulae - The Cone and Rosette region - Large field image of the Cone nebula (centre left) and the Rosette nebula (top right), in the constellation Unicorn. This wide field image shows the rich colorful Cone nebula region (at the center - left of the image) and the Rosette Nebula (at the top right). They are both located in the Monoceros constellation, very close to the better known Orion constellation

Black bryony, Dioscorea communis (Tamus communis) Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.
Black bryony, Dioscorea communis (Tamus communis) Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

FLO4618555: Black bryony, Dioscorea communis (Tamus communis) Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816. / Bridgeman Images

ID: FLO4618555

Black bryony, Dioscorea communis (Tamus communis) Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

Fig, Ficus carica. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.
Fig, Ficus carica. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

FLO4618620: Fig, Ficus carica. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816. / Bridgeman Images

ID: FLO4618620

Fig, Ficus carica. Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

Nebulae around the cluster NGC 2264 - The Cone nebula at the top is an H II region located about 2600 light years away from Earth. The bright star in the center is S Monocerotis, a star of magnitude 4.7. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed
Nebulae around the cluster NGC 2264 - The Cone nebula at the top is an H II region located about 2600 light years away from Earth. The bright star in the center is S Monocerotis, a star of magnitude 4.7. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed

PIX4618628: Nebulae around the cluster NGC 2264 - The Cone nebula at the top is an H II region located about 2600 light years away from Earth. The bright star in the center is S Monocerotis, a star of magnitude 4.7. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed / Bridgeman Images

ID: PIX4618628

Nebulae around the cluster NGC 2264 - The Cone nebula at the top is an H II region located about 2600 light years away from Earth. The bright star in the center is S Monocerotis, a star of magnitude 4.7. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed

Bulrush or club-rush, Schoenoplectus lacustris (Bull-rush, Scirpus lacustris). Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.
Bulrush or club-rush, Schoenoplectus lacustris (Bull-rush, Scirpus lacustris). Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

FLO4618633: Bulrush or club-rush, Schoenoplectus lacustris (Bull-rush, Scirpus lacustris). Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816. / Bridgeman Images

ID: FLO4618633

Bulrush or club-rush, Schoenoplectus lacustris (Bull-rush, Scirpus lacustris). Handcoloured copperplate engraving after an illustration by Richard Duppa from his The Clours and Orders of the Linnaean System of Botany, Longman, Hurst, London, 1816.

Nebula of the cone NGC 2264 in the Unicorn - Nebula of the cone NGC 2264 in the Unicorn - The nebula of the Cone, is a region H II located about 2600 years - light from Earth
Nebula of the cone NGC 2264 in the Unicorn - Nebula of the cone NGC 2264 in the Unicorn - The nebula of the Cone, is a region H II located about 2600 years - light from Earth

PIX4618649: Nebula of the cone NGC 2264 in the Unicorn - Nebula of the cone NGC 2264 in the Unicorn - The nebula of the Cone, is a region H II located about 2600 years - light from Earth / Bridgeman Images

ID: PIX4618649

Nebula of the cone NGC 2264 in the Unicorn - Nebula of the cone NGC 2264 in the Unicorn - The nebula of the Cone, is a region H II located about 2600 years - light from Earth

Louis XIV of France (1638-1715), 1701 - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th et 18th centuries” by Georges Duplessis (1834-1899), edition 1867
Louis XIV of France (1638-1715), 1701 - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th et 18th centuries” by Georges Duplessis (1834-1899), edition 1867

FLO4616714: Louis XIV of France (1638-1715), 1701 - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th et 18th centuries” by Georges Duplessis (1834-1899), edition 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616714

Louis XIV of France (1638-1715), 1701 - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th et 18th centuries” by Georges Duplessis (1834-1899), edition 1867

Lechevallier-Chevignard, Edmond (1825-1902)

Jean Antoine de Mesme (1661-1723), lord of Irval, count of Avaux, French magistrature 17th century, after a painting of 1653, by Philippe de Champaigne (1602-1674) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), extracted from “” Costumes historiques of the 16th, 17th and 18th century by Georges Duplessis (1834-1899), edition 1867
Jean Antoine de Mesme (1661-1723), lord of Irval, count of Avaux, French magistrature 17th century, after a painting of 1653, by Philippe de Champaigne (1602-1674) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), extracted from “” Costumes historiques of the 16th, 17th and 18th century by Georges Duplessis (1834-1899), edition 1867

FLO4616720: Jean Antoine de Mesme (1661-1723), lord of Irval, count of Avaux, French magistrature 17th century, after a painting of 1653, by Philippe de Champaigne (1602-1674) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), extracted from “” Costumes historiques of the 16th, 17th and 18th century by Georges Duplessis (1834-1899), edition 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616720

Jean Antoine de Mesme (1661-1723), lord of Irval, count of Avaux, French magistrature 17th century, after a painting of 1653, by Philippe de Champaigne (1602-1674) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), extracted from “” Costumes historiques of the 16th, 17th and 18th century by Georges Duplessis (1834-1899), edition 1867

Lechevallier-Chevignard, Edmond (1825-1902)

King Charles I of England (1600-1649), based on a portrait of 1635 by Antonie Van Dyck (1599-1641) - Lithography of an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867
King Charles I of England (1600-1649), based on a portrait of 1635 by Antonie Van Dyck (1599-1641) - Lithography of an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867

FLO4616724: King Charles I of England (1600-1649), based on a portrait of 1635 by Antonie Van Dyck (1599-1641) - Lithography of an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616724

King Charles I of England (1600-1649), based on a portrait of 1635 by Antonie Van Dyck (1599-1641) - Lithography of an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867

Lechevallier-Chevignard, Edmond (1825-1902)

French cavalry, 17th century, based on a painting by Sebastien Bourdon (1616-1671) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867
French cavalry, 17th century, based on a painting by Sebastien Bourdon (1616-1671) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867

FLO4616742: French cavalry, 17th century, based on a painting by Sebastien Bourdon (1616-1671) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616742

French cavalry, 17th century, based on a painting by Sebastien Bourdon (1616-1671) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867

Lechevallier-Chevignard, Edmond (1825-1902)

French royal officer, 17th century, after an engraving of 1675, by Jean de Saint Jean - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th et 18th Siecles” by Georges Duplessis (1834-1899), edition 1867
French royal officer, 17th century, after an engraving of 1675, by Jean de Saint Jean - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th et 18th Siecles” by Georges Duplessis (1834-1899), edition 1867

FLO4616759: French royal officer, 17th century, after an engraving of 1675, by Jean de Saint Jean - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th et 18th Siecles” by Georges Duplessis (1834-1899), edition 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616759

French royal officer, 17th century, after an engraving of 1675, by Jean de Saint Jean - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16e, 17th et 18th Siecles” by Georges Duplessis (1834-1899), edition 1867

Lechevallier-Chevignard, Edmond (1825-1902)

Peasant of Lombardy (Italy), 18th century, based on a painting by Fracesco Londonio (1723-1783) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), extracted from “” Costumes historiques des 16e, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867
Peasant of Lombardy (Italy), 18th century, based on a painting by Fracesco Londonio (1723-1783) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), extracted from “” Costumes historiques des 16e, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867

FLO4616827: Peasant of Lombardy (Italy), 18th century, based on a painting by Fracesco Londonio (1723-1783) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), extracted from “” Costumes historiques des 16e, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616827

Peasant of Lombardy (Italy), 18th century, based on a painting by Fracesco Londonio (1723-1783) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), extracted from “” Costumes historiques des 16e, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867

Lechevallier-Chevignard, Edmond (1825-1902)

Officer governor of Marseille and lady of quality, France, 18th century, after a painting of 1754 by Joseph Vernet (1714-1789) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition. 1867
Officer governor of Marseille and lady of quality, France, 18th century, after a painting of 1754 by Joseph Vernet (1714-1789) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition. 1867

FLO4616844: Officer governor of Marseille and lady of quality, France, 18th century, after a painting of 1754 by Joseph Vernet (1714-1789) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition. 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616844

Officer governor of Marseille and lady of quality, France, 18th century, after a painting of 1754 by Joseph Vernet (1714-1789) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition. 1867

Lechevallier-Chevignard, Edmond (1825-1902)

Venitian gondolier, Italy 18th century, based on a painting by Giovanni Antonio Canal dit Canaletto (1697-1768) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “” Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867
Venitian gondolier, Italy 18th century, based on a painting by Giovanni Antonio Canal dit Canaletto (1697-1768) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “” Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867

FLO4616848: Venitian gondolier, Italy 18th century, based on a painting by Giovanni Antonio Canal dit Canaletto (1697-1768) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “” Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616848

Venitian gondolier, Italy 18th century, based on a painting by Giovanni Antonio Canal dit Canaletto (1697-1768) - Lithography based on an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “” Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1867

Lechevallier-Chevignard, Edmond (1825-1902)

Ocean sur Mars - Region d'Elysium - Mars with ocean - looking at Elysium Mons - Reconstructed view of Mars at the time she had an ocean. This image was created from data obtained by the FUSE satellite and the MOLA instrument on the Mars Global Surveyor probe. Viking sensor images were used for the emergeal zones. This visualization shows how Mars might look with an ocean at - 500m where the lowest point on Mars is about - 8000m and the highest point is about 22000m. Data from The FUSE spacecraft and from the Mars Global Surveyor/MOLA instrument where used to support this theor
Ocean sur Mars - Region d'Elysium - Mars with ocean - looking at Elysium Mons - Reconstructed view of Mars at the time she had an ocean. This image was created from data obtained by the FUSE satellite and the MOLA instrument on the Mars Global Surveyor probe. Viking sensor images were used for the emergeal zones. This visualization shows how Mars might look with an ocean at - 500m where the lowest point on Mars is about - 8000m and the highest point is about 22000m. Data from The FUSE spacecraft and from the Mars Global Surveyor/MOLA instrument where used to support this theor

PIX4616860: Ocean sur Mars - Region d'Elysium - Mars with ocean - looking at Elysium Mons - Reconstructed view of Mars at the time she had an ocean. This image was created from data obtained by the FUSE satellite and the MOLA instrument on the Mars Global Surveyor probe. Viking sensor images were used for the emergeal zones. This visualization shows how Mars might look with an ocean at - 500m where the lowest point on Mars is about - 8000m and the highest point is about 22000m. Data from The FUSE spacecraft and from the Mars Global Surveyor/MOLA instrument where used to support this theor / Bridgeman Images

ID: PIX4616860

Ocean sur Mars - Region d'Elysium - Mars with ocean - looking at Elysium Mons - Reconstructed view of Mars at the time she had an ocean. This image was created from data obtained by the FUSE satellite and the MOLA instrument on the Mars Global Surveyor probe. Viking sensor images were used for the emergeal zones. This visualization shows how Mars might look with an ocean at - 500m where the lowest point on Mars is about - 8000m and the highest point is about 22000m. Data from The FUSE spacecraft and from the Mars Global Surveyor/MOLA instrument where used to support this theor

Young French woman with a little boy, 18th century, by an engraving by Philibert Debucourt (1755-1832) - Lithography after an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1834-1899 67
Young French woman with a little boy, 18th century, by an engraving by Philibert Debucourt (1755-1832) - Lithography after an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1834-1899 67

FLO4616888: Young French woman with a little boy, 18th century, by an engraving by Philibert Debucourt (1755-1832) - Lithography after an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1834-1899 67, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616888

Young French woman with a little boy, 18th century, by an engraving by Philibert Debucourt (1755-1832) - Lithography after an illustration by Edmond Lechevallier-Chevignard (1825-1902), from “Costumes historiques des 16th, 17th and 18th century” by Georges Duplessis (1834-1899), edition 1834-1899 67

Lechevallier-Chevignard, Edmond (1825-1902)

Ferdinand Guillemardet (1765-1809), ambassador of the French republic to Spain 18th century, based on a painting of 1798 by Francisco Goya (1746-1828) - Lithography of an illustration by Edmond Lechevallier-Chevignard (1825-1902), from Georges Duorges Plessis (1834-1899), edition 1867
Ferdinand Guillemardet (1765-1809), ambassador of the French republic to Spain 18th century, based on a painting of 1798 by Francisco Goya (1746-1828) - Lithography of an illustration by Edmond Lechevallier-Chevignard (1825-1902), from Georges Duorges Plessis (1834-1899), edition 1867

FLO4616890: Ferdinand Guillemardet (1765-1809), ambassador of the French republic to Spain 18th century, based on a painting of 1798 by Francisco Goya (1746-1828) - Lithography of an illustration by Edmond Lechevallier-Chevignard (1825-1902), from Georges Duorges Plessis (1834-1899), edition 1867, Lechevallier-Chevignard, Edmond (1825-1902) / Bridgeman Images

ID: FLO4616890

Ferdinand Guillemardet (1765-1809), ambassador of the French republic to Spain 18th century, based on a painting of 1798 by Francisco Goya (1746-1828) - Lithography of an illustration by Edmond Lechevallier-Chevignard (1825-1902), from Georges Duorges Plessis (1834-1899), edition 1867

Lechevallier-Chevignard, Edmond (1825-1902)

Mars with water - Artist's view - Wet Mars - Artwork - View of the region of Kasei Vallis sur Mars at the time when the water was present on the surface of the planet. Kasei Vallis as it may once have been during an early, wet period in March history
Mars with water - Artist's view - Wet Mars - Artwork - View of the region of Kasei Vallis sur Mars at the time when the water was present on the surface of the planet. Kasei Vallis as it may once have been during an early, wet period in March history

PIX4616896: Mars with water - Artist's view - Wet Mars - Artwork - View of the region of Kasei Vallis sur Mars at the time when the water was present on the surface of the planet. Kasei Vallis as it may once have been during an early, wet period in March history / Bridgeman Images

ID: PIX4616896

Mars with water - Artist's view - Wet Mars - Artwork - View of the region of Kasei Vallis sur Mars at the time when the water was present on the surface of the planet. Kasei Vallis as it may once have been during an early, wet period in March history


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