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'Lunetta' images and/or videos results

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Images of 'Lunetta' found, 990

 
Chateau - Abbadia Observatory - Abbadia Castle - Property of the Academy of Sciences, located in Hendaye, in the Atlantic Pyrenees, this castle was the home of Antoine d'Abbadie (1810 - 1897), a scholar and explorer. It was built between 1864 and 1879 by the architect Eugene Viollet-le-Duc (1814 - 1879), instead of an astronomical observatory dating back to 1858. The castle houses a new observatory, equipped with a Meridian bezel of 2.05 m focal length, with which d'Abbadie participated in the elaboration of the map of the sky “”. Passionate about astronomy, Antoine d'Abbadie made many trips, notably to observe total eclipses of the Sun in Norway (1851), Spain (1860) and Algeria (1867). In 1882 he observed Venus's passage before the Sun from the West Indies. He was president of the Academy of Sciences in 1891 and 1892. Abbadia Castle, owned by the French Academy of Sciences, was built by Eugene Viollet le Duc between 1864 and 1879. It houses a former astronomy observatory.

Sebastien Beaucourt

PIX4566964

Chateau - Abbadia Observatory - Abbadia Castle - Property of the Academy of Sciences, located in Hendaye, in the Atlantic Pyrenees, this castle was the home of Antoine d'Abbadie (1810 - 1897), a scholar and explorer. It was built between 1864 and 1879 by the architect Eugene Viollet-le-Duc (1814 - 1879), instead of an astronomical observatory dating back to 1858. The castle houses a new observatory, equipped with a Meridian bezel of 2.05 m focal length, with which d'Abbadie participated in the elaboration of the map of the sky “”. Passionate about astronomy, Antoine d'Abbadie made many trips, notably to observe total eclipses of the Sun in Norway (1851), Spain (1860) and Algeria (1867). In 1882 he observed Venus's passage before the Sun from the West Indies. He was president of the Academy of Sciences in 1891 and 1892. Abbadia Castle, owned by the French Academy of Sciences, was built by Eugene Viollet le Duc between 1864 and 1879. It houses a former astronomy observatory.

Sebastien Beaucourt

PIX4566964

 
Chateau - Abbadia Observatory - Abbadia Castle - Property of the Academy of Sciences, located in Hendaye, in the Atlantic Pyrenees, this castle was the home of Antoine d'Abbadie (1810 - 1897), a scholar and explorer. It was built between 1864 and 1879 by the architect Eugene Viollet-le-Duc (1814 - 1879), instead of an astronomical observatory dating back to 1858. The castle houses a new observatory, equipped with a Meridian bezel of 2.05 m focal length, with which d'Abbadie participated in the elaboration of the map of the sky “”. Passionate about astronomy, Antoine d'Abbadie made many trips, notably to observe total eclipses of the Sun in Norway (1851), Spain (1860) and Algeria (1867). In 1882 he observed Venus's passage before the Sun from the West Indies. He was president of the Academy of Sciences in 1891 and 1892. Abbadia Castle, owned by the French Academy of Sciences, was built by Eugene Viollet le Duc between 1864 and 1879. It houses a former astronomy observatory.

Sebastien Beaucourt

PIX4566979

Chateau - Abbadia Observatory - Abbadia Castle - Property of the Academy of Sciences, located in Hendaye, in the Atlantic Pyrenees, this castle was the home of Antoine d'Abbadie (1810 - 1897), a scholar and explorer. It was built between 1864 and 1879 by the architect Eugene Viollet-le-Duc (1814 - 1879), instead of an astronomical observatory dating back to 1858. The castle houses a new observatory, equipped with a Meridian bezel of 2.05 m focal length, with which d'Abbadie participated in the elaboration of the map of the sky “”. Passionate about astronomy, Antoine d'Abbadie made many trips, notably to observe total eclipses of the Sun in Norway (1851), Spain (1860) and Algeria (1867). In 1882 he observed Venus's passage before the Sun from the West Indies. He was president of the Academy of Sciences in 1891 and 1892. Abbadia Castle, owned by the French Academy of Sciences, was built by Eugene Viollet le Duc between 1864 and 1879. It houses a former astronomy observatory.

Sebastien Beaucourt

PIX4566979

 
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Sacrifice and Drunkenness of Noah, 1425-1430 (fresco)

Uccello, Paolo (1397-1475) (and workshop)

Antonio Quattrone

MEP2627447

Sacrifice and Drunkenness of Noah, 1425-1430 (fresco)

Uccello, Paolo (1397-1475) (and workshop)

Antonio Quattrone

MEP2627447

 
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Sassetti Chapel, 1482-1486 (fresco)

Ghirlandaio, Domenico (Domenico Bigordi) (1449-94)

Antonio Quattrone

MEP2627830

Sassetti Chapel, 1482-1486 (fresco)

Ghirlandaio, Domenico (Domenico Bigordi) (1449-94)

Antonio Quattrone

MEP2627830

 
Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) in the center left, and M110 (NGC 205) below. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image made with an amateur instrument, a 130 mm bezel, several composite images. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

Jerry Lodriguss

PIX4608685

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) in the center left, and M110 (NGC 205) below. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image made with an amateur instrument, a 130 mm bezel, several composite images. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

Jerry Lodriguss

PIX4608685

 
Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) at the top center, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image obtained with an apochromatic bezel Televue 127is. 22 hours of laying. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

PIX4608828

Spiral Galaxy M31 in Andromede - Spiral galaxy M31 in Andromeda - The galaxy of Andromede is located about 2 million years ago - light from Earth. Two satellite galaxies accompany it: M32 (NGC 221) at the top center, and M110 (NGC 205) at the bottom. Like the lactee path, the Andromede galaxy belongs to the local group, making up about thirty galaxies. Image obtained with an apochromatic bezel Televue 127is. 22 hours of laying. M31, the Great galaxy in Andromeda, is a gigantic collection of more than 300 billion stars and is located about 2 million light years from Earth. Companion dwarf elliptical galaxies M32 and M110 are also visible. M31 and its companions are part of our local group of galaxies, which includes the Milky Way and Magellanic Clouds, and M33. The Andromeda Galaxy is headed towards our Milky Way Galaxy and is expected to collide with it and possibly merge into a gigantic elliptical galaxy in about 3 billion years

PIX4608828

 
Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. Image made with an amateur instrument, a 130 mm bezel. The Pinwheel Galaxy, M33, is a very large, beautiful, face - on spiral galaxy. It is more difficult to observe at magnification than its size and magnitude would indicate under skies that are not dark because of it's fairly low surface brightness. Still, under very dark and transparent skies, M33 can be seen with the unaided eye by keen - eyed observers. Several emission nebulae inside of M33 can be seen as pink patches in this photo. The largest and most prominent emission nebula is NGC 604 which is almost 1,500 light - years in diameter. Such clouds are star factories where gas condenses under gravitational attraction and stars are born. It is one of the largest clouds of ionized hydrogen g

Jerry Lodriguss

PIX4609277

Spiral galaxy M33 in the Triangle - Spiral galaxy M33 in Triangulum - M33, (NGC 598), the galaxy of the Triangle, is located about 2 million years ago - light from Earth. It belongs to the local group, just like our galaxy or Andromede galaxy. Image made with an amateur instrument, a 130 mm bezel. The Pinwheel Galaxy, M33, is a very large, beautiful, face - on spiral galaxy. It is more difficult to observe at magnification than its size and magnitude would indicate under skies that are not dark because of it's fairly low surface brightness. Still, under very dark and transparent skies, M33 can be seen with the unaided eye by keen - eyed observers. Several emission nebulae inside of M33 can be seen as pink patches in this photo. The largest and most prominent emission nebula is NGC 604 which is almost 1,500 light - years in diameter. Such clouds are star factories where gas condenses under gravitational attraction and stars are born. It is one of the largest clouds of ionized hydrogen g

Jerry Lodriguss

PIX4609277

 
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  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
Usage restrictions from our Content Partners
  • Not available to clients invoiced in Italy
St. Francis Receiving the Rule of the Order by Pope Honorius III, 1482-1485 (fresco)

Ghirlandaio, Domenico (Domenico Bigordi) (1449-94)

Antonio Quattrone

MEP2627771

St. Francis Receiving the Rule of the Order by Pope Honorius III, 1482-1485 (fresco)

Ghirlandaio, Domenico (Domenico Bigordi) (1449-94)

Antonio Quattrone

MEP2627771

 
Horsehead nebula and Orion nebula - Orion nebula and horsehead nebula - On the left, the dark nebula of the horse's head (IC434 - B33). On the right, the large Orion nebula (M42) is a vast region of star formation. These nebulae are located 1500 years of light from Earth. Mosaic of four images obtained with a FSQ 106 bezel, a 50 cm telescope and CCD STL11000 camera, with an H alpha filter. Total installation of 50 hours. 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. The brightest star in the photo at left is Alnilam, the middle star of the three distinctive stars in the belt of Orion. Bottom left is the Flame nebula, NGC 2024, and to its right is dark nebula B33, the Horsehead Nebula. Above at right is a patch of blue reflection nebulosity NGC 1973 - 4 - 5 and the beautiful Orion Nebula, M 42

R. Gendler

PIX4617946

Horsehead nebula and Orion nebula - Orion nebula and horsehead nebula - On the left, the dark nebula of the horse's head (IC434 - B33). On the right, the large Orion nebula (M42) is a vast region of star formation. These nebulae are located 1500 years of light from Earth. Mosaic of four images obtained with a FSQ 106 bezel, a 50 cm telescope and CCD STL11000 camera, with an H alpha filter. Total installation of 50 hours. 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. The brightest star in the photo at left is Alnilam, the middle star of the three distinctive stars in the belt of Orion. Bottom left is the Flame nebula, NGC 2024, and to its right is dark nebula B33, the Horsehead Nebula. Above at right is a patch of blue reflection nebulosity NGC 1973 - 4 - 5 and the beautiful Orion Nebula, M 42

R. Gendler

PIX4617946

 
The center of our galaxy, the milky way - The center of our galaxy, the milky way - This billion pixel mosaic shows the central region of our galaxy, the Lactee Way. The 52 assembled images cover an area that extends from Sagittarius (with the galactic center and nebulae M8 and M20) on the left, to the Scorpio, with the star Antares and the colored cloud of Rho Ophiuchus on the right. Image obtained with a Takahashi FSQ 106 Ed bezel at Cerro Paranal Observatory in Chile; 200 hours of poses. This image is a 1 billion pixel RGB mosaic of the galactic center region (340 million pixels in each R, V and B color). It shows the region spanning from Sagittarius (with the Milky Way center and M8/M20 area on the left) to Scorpius (with colorful Antares and Rho Ophiuchus region on the right) and cat paw nebula (red nebula at the bottom). This mosaic was assembled from 52 different sky fields made from 1200 individual images and 200 hours total exposure time, final image size is 24000x14000 pixels

Stephane Guisard

PIX4636007

The center of our galaxy, the milky way - The center of our galaxy, the milky way - This billion pixel mosaic shows the central region of our galaxy, the Lactee Way. The 52 assembled images cover an area that extends from Sagittarius (with the galactic center and nebulae M8 and M20) on the left, to the Scorpio, with the star Antares and the colored cloud of Rho Ophiuchus on the right. Image obtained with a Takahashi FSQ 106 Ed bezel at Cerro Paranal Observatory in Chile; 200 hours of poses. This image is a 1 billion pixel RGB mosaic of the galactic center region (340 million pixels in each R, V and B color). It shows the region spanning from Sagittarius (with the Milky Way center and M8/M20 area on the left) to Scorpius (with colorful Antares and Rho Ophiuchus region on the right) and cat paw nebula (red nebula at the bottom). This mosaic was assembled from 52 different sky fields made from 1200 individual images and 200 hours total exposure time, final image size is 24000x14000 pixels

Stephane Guisard

PIX4636007

 
Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and

W. Promper

PIX4622329

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus: IC1396, VDB 142. Nebula located about 2700 light years from Earth. Image obtained with a bezel Tele Vue NP127iS, through 3 different filters that demonstrate oxygen, hydrogen, and sulfur - The Elephant Trunk Nebula (IC 1396A) in Cepheus is part of the larger IC 1396 complex which spans a large area of the sky measuring 170 by 140 arc-minutes and is one of the brightest emission nebulae with a magnitude of 3.5. The western portion of IC 1396 contains the Elephant Trunk Nebula (IC 1396A) which is characterized with H-II emissions, dark lanes and globules as well as a small reflection nebula. The IC 1396 complex is technically a star cluster (aka Cr 439, Trumpler 37) owing to the presence of a developing open but loose cluster at the heart of this rich nebulosity. This open star cluster is comprised of 50-100 member stars which vary in brightness spanning an area of approximately 50 'in diameter and

W. Promper

PIX4622329

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