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Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - Image of the nebula of the Carene (NGC 3372), a very vast region of star formation, obtained by combining light through 3 different filters that highlight oxygen in blue, hydrogen in green, and sulfur in red. The colors also represent different gas temperatures, warm, blue, colder in red. The bright star in the center of the image is Eta Carinae, a super massive star. Image obtained with the Curtis - Schmidt telescope of the Cerro Tololo Observatory. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372), combining the light from 3 different filters tracing emission from oxygen (blue), hydrogen (green), and sulphur (red). The color is also representative of the temperature in the ionized gas: blue is relatively hot and red is cooler. The Carina Nebula is a good example of how very massive stars rip apart the molecular clouds that give birth to them. The bright sta

Nebula NGC 3372 in the Carene in false colours - NGC 3372 Carina nebula - Image of the nebula of the Carene (NGC 3372), a very vast region of star formation, obtained by combining light through 3 different filters that highlight oxygen in blue, hydrogen in green, and sulfur in red. The colors also represent different gas temperatures, warm, blue, colder in red. The bright star in the center of the image is Eta Carinae, a super massive star. Image obtained with the Curtis - Schmidt telescope of the Cerro Tololo Observatory. This image shows a giant star - forming region in the southern sky known as the Carina Nebula (NGC 3372), combining the light from 3 different filters tracing emission from oxygen (blue), hydrogen (green), and sulphur (red). The color is also representative of the temperature in the ionized gas: blue is relatively hot and red is cooler. The Carina Nebula is a good example of how very massive stars rip apart the molecular clouds that give birth to them. The bright sta

PIX4618865

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

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

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

d'Antonio, Biagio (c.1446-1516)

COU6085979

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

d'Antonio, Biagio (c.1446-1516)

COU6085981

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight 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 d

Elephant tube nebula (VDB 142) in Cephee - The Elephant Trunk Nebula (VDB 142) in Cepheus - IC1396, VDB 142. Nebula located about 2700 years - light from Earth. Image obtained with a telescope 40 cm in diameter, through 3 different filters that highlight 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 d

PIX4622303

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

d'Antonio, Biagio (c.1446-1516)

COU6085984

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 2)

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 2)

LCV7247022

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 3)

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 3)

LCV7247024

Seneschal Lane, Douglas, Isle of Man, 1932-34 (b/w photo)

Seneschal Lane, Douglas, Isle of Man, 1932-34 (b/w photo)

Frowde, John James (1868-1946)

MNX5052680

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

d'Antonio, Biagio (c.1446-1516)

COU6085996

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

d'Antonio, Biagio (c.1446-1516)

COU6086004

Framed Youth — Revenge of the Teenage Perverts 1986 (Credits)

Framed Youth — Revenge of the Teenage Perverts 1986 (Credits)

LCV7247019

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 4)

Framed Youth — Revenge of the Teenage Perverts 1986 (Part 4)

LCV7247025

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

d'Antonio, Biagio (c.1446-1516)

COU6085990

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

d'Antonio, Biagio (c.1446-1516)

COU6086057

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

Chest and spalliera with the arms of Vaggia Nerli and Lorenzo Morelli (The Nerli Chest), 1472 (tempera on poplar with gilding)

d'Antonio, Biagio (c.1446-1516)

COU6086061

Nebula IC 4628 in Scorpio - Nebula IC 4628 in Scorpius - Nebula has a low light emission, IC 4628 (or Gum 56) is alongside the open cluster Collinder 316, which houses many young hot stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). This beautiful, arc - like rim of nebulosity is in the far southern sky, out of sight from most of the USA and Europe. It is quite faint and has often been overlooked because of it, even by southern observers. However, it is in a rich region in Scorpius. This richness is reflected in the number of names associated with the objects in the field illustrated here. There is a large scattered star cluster, Collinder 316 which extends over most of the picture. It encloses Trumpler 24, more or less the same cluster under another name, and all of this is part of the Sco OB1 association, a much larger gathering of very hot, intrinsically luminous stars in this part of the sky. The nebula itself is als

Nebula IC 4628 in Scorpio - Nebula IC 4628 in Scorpius - Nebula has a low light emission, IC 4628 (or Gum 56) is alongside the open cluster Collinder 316, which houses many young hot stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). This beautiful, arc - like rim of nebulosity is in the far southern sky, out of sight from most of the USA and Europe. It is quite faint and has often been overlooked because of it, even by southern observers. However, it is in a rich region in Scorpius. This richness is reflected in the number of names associated with the objects in the field illustrated here. There is a large scattered star cluster, Collinder 316 which extends over most of the picture. It encloses Trumpler 24, more or less the same cluster under another name, and all of this is part of the Sco OB1 association, a much larger gathering of very hot, intrinsically luminous stars in this part of the sky. The nebula itself is als

Tom Davis

PIX4622673

Saturn en jour vue par Cassini - Backlit Saturn seen by Cassini - Mosaic of 141 photos obtained by the Cassini probe on 19 July 2013 at a distance of 1.2 million km from the planet. The Cassini probe was then in the shadow of the Planet Saturn; this portrait of the Giant Planet highlights its ring system and seven of its satellites appear in the image. The planets Mars, Venus and Earth are also visible. On July 19, 2013, Nasa's Cassini spacecraft slipped into Saturn's shadow and turned to image the planet, seven of its moons, its inner rings - and, in the background, our home planet, Earth. With both Cassini's wide-angle and narrow-angle cameras aimed at Saturn, Cassini was able to capture 323 images in just over four hours. This final mosaic uses 141 of those wide-angle images. Images taken using the red, green and blue spectral filters of the wide-angle camera were combined and mosaicked together to create this natural-color view. This image spans about 404,880 miles (651,591 kilomet

Saturn en jour vue par Cassini - Backlit Saturn seen by Cassini - Mosaic of 141 photos obtained by the Cassini probe on 19 July 2013 at a distance of 1.2 million km from the planet. The Cassini probe was then in the shadow of the Planet Saturn; this portrait of the Giant Planet highlights its ring system and seven of its satellites appear in the image. The planets Mars, Venus and Earth are also visible. On July 19, 2013, Nasa's Cassini spacecraft slipped into Saturn's shadow and turned to image the planet, seven of its moons, its inner rings - and, in the background, our home planet, Earth. With both Cassini's wide-angle and narrow-angle cameras aimed at Saturn, Cassini was able to capture 323 images in just over four hours. This final mosaic uses 141 of those wide-angle images. Images taken using the red, green and blue spectral filters of the wide-angle camera were combined and mosaicked together to create this natural-color view. This image spans about 404,880 miles (651,591 kilomet

PIX4625315

Around the Nares Detroit - Canada - Greenland - Nares strait area - Canada - Greenland - This radar image from Envisat shows the northeast tip of Ellesmere Island (left) in the Canadian Arctic and the northwestern extremity of Greenland - the largest island on the planet (right). At the bottom of the image, the waters, which appear in green and purple, form the detroit of Nares, which flies north to form the Robeson Canal. It drains the Lincoln Sea (in the upper left corner) which is part of the Arctic Ocean. The white and blue area on the right side of the image is a portion of the Greenland ice cap, the second largest concentration of frozen fresh water on Earth after the Antarctic polar cap. The largest floating glacier in the northern hemisphere, the Petermann Glacier, is reddish in colour, and runs at the bottom of the image in the centre towards the detroit of Nares. The Petermann Glacier lost a 29 km2 block between July 10 and 25, 2008. Standard radar images are not in colour be

Around the Nares Detroit - Canada - Greenland - Nares strait area - Canada - Greenland - This radar image from Envisat shows the northeast tip of Ellesmere Island (left) in the Canadian Arctic and the northwestern extremity of Greenland - the largest island on the planet (right). At the bottom of the image, the waters, which appear in green and purple, form the detroit of Nares, which flies north to form the Robeson Canal. It drains the Lincoln Sea (in the upper left corner) which is part of the Arctic Ocean. The white and blue area on the right side of the image is a portion of the Greenland ice cap, the second largest concentration of frozen fresh water on Earth after the Antarctic polar cap. The largest floating glacier in the northern hemisphere, the Petermann Glacier, is reddish in colour, and runs at the bottom of the image in the centre towards the detroit of Nares. The Petermann Glacier lost a 29 km2 block between July 10 and 25, 2008. Standard radar images are not in colour be

PIX4666074

Nebula NGC 3372 in the Carene - NGC 3372 Carina nebula - The Carene Nebula (NGC 3372) is a very large region of star formation visible in the southern hemisphere. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). The bright star in the center of the image is Eta Carinae, a super massive star. The Carina Nebula (also known as the Great Nebula in Carina, the Eta Carinae Nebula, or NGC 3372) is a large bright nebula that surrounds several open clusters of stars. Eta Carinae and HD 93129A, two of the most massive and luminous stars in our Milky Way galaxy, are among them. The nebula lies at an estimated distance between 6,500 and 10,000 light years from Earth. It is located in the constellation of Carina. The nebula contains multiple O - type stars. This nebula is one of the largest H II regions in the Milky Way. It has a visual magnitude of 1.0. The nebula is one of the largest diffuse nebulae in our skies. Although it is some fou

Nebula NGC 3372 in the Carene - NGC 3372 Carina nebula - The Carene Nebula (NGC 3372) is a very large region of star formation visible in the southern hemisphere. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). The bright star in the center of the image is Eta Carinae, a super massive star. The Carina Nebula (also known as the Great Nebula in Carina, the Eta Carinae Nebula, or NGC 3372) is a large bright nebula that surrounds several open clusters of stars. Eta Carinae and HD 93129A, two of the most massive and luminous stars in our Milky Way galaxy, are among them. The nebula lies at an estimated distance between 6,500 and 10,000 light years from Earth. It is located in the constellation of Carina. The nebula contains multiple O - type stars. This nebula is one of the largest H II regions in the Milky Way. It has a visual magnitude of 1.0. The nebula is one of the largest diffuse nebulae in our skies. Although it is some fou

Tom Davis

PIX4619112

Total Eclipse of Moon 27 - 09 - 1996 - Total lunar eclipse September 27, 1996 - This montage illustrates the progression of the Moon in Earth's shadow cone. The image on the right corresponds to its complete entry into the shadow (beginning of the totalite), the central at the maximum of the totalite and the one on the left at the end of the totalite. During this eclipse, the southern pole of the Moon is passing a little above the center of the Earth's shadow cone. Thus, the southern pole of the Moon is the darkest, while the north pole is brighter. Note the color degrade for the right and left poses: from dark red towards the center of the shadow cone to white on the periphery of this cone, with an intermediate greenish orange degrade. This highlights the fact that blue is more diffuse than green by the Earth's atmosphere - hence the absence of blue on the image, because this color is lost in the Earth's atmosphere and therefore does not reach the surface of the Moon - and that green

Total Eclipse of Moon 27 - 09 - 1996 - Total lunar eclipse September 27, 1996 - This montage illustrates the progression of the Moon in Earth's shadow cone. The image on the right corresponds to its complete entry into the shadow (beginning of the totalite), the central at the maximum of the totalite and the one on the left at the end of the totalite. During this eclipse, the southern pole of the Moon is passing a little above the center of the Earth's shadow cone. Thus, the southern pole of the Moon is the darkest, while the north pole is brighter. Note the color degrade for the right and left poses: from dark red towards the center of the shadow cone to white on the periphery of this cone, with an intermediate greenish orange degrade. This highlights the fact that blue is more diffuse than green by the Earth's atmosphere - hence the absence of blue on the image, because this color is lost in the Earth's atmosphere and therefore does not reach the surface of the Moon - and that green

Laurent Laveder

PIX4579217

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation.

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus - Nebula IC 2948 is a vast nebula located about 6000 years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars. Image obtained through 3 different filters that highlight oxygen (blue), hydrogen (green), and sulfur (red). Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch - American astronomer who first drew attention to them as the possible sites of star formation.

Tom Davis

PIX4622599

The 'St Andrew' at Sea in a Moderate Breeze, c.1673 (oil on canvas)

The 'St Andrew' at Sea in a Moderate Breeze, c.1673 (oil on canvas)

Velde, Willem van de, the Younger (1633-1707)

MMM7342592

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus: IC2944 - SHO 70 70 70 Bin 2 - Nebula IC 2948 is a vast nebula located about 6000 light years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars - Image obtained through 3 different filters that highlight oxygen (in blue), hydrogen (in green), and sulfur (in red) - Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch-American astronomer who first drew attention to t

Nebula IC 2948 in Centaurus - Nebula IC 2948 and IC 2944 in Centaurus: IC2944 - SHO 70 70 70 Bin 2 - Nebula IC 2948 is a vast nebula located about 6000 light years from Earth in the southern constellation of Centaurus. It is associated with the cluster of stars IC 2944 near which Bok's blood cells are visible. A Bok's blood cell is a dark interstellar cloud of gases and dust that absorb light. If it condenses enough, it gives birth to new stars - Image obtained through 3 different filters that highlight oxygen (in blue), hydrogen (in green), and sulfur (in red) - Between the Southern Cross and the rich Carina region, on the southern border of Centaurus, is a large, almost featureless emission nebula, IC 2948, with a sprinkling of bright stars, Collinder 249. It is against this uniform, backdrop that we see a brighter region (IC 2944) which hosts small group of dark clouds of the kind known as 'Bok globules'. They are named for the Dutch-American astronomer who first drew attention to t

W. Promper

PIX4622580

No. 4 St Barnabas Square, Douglas, Isle of Man, 1932-34 (b/w photo)

No. 4 St Barnabas Square, Douglas, Isle of Man, 1932-34 (b/w photo)

Frowde, John James (1868-1946)

MNX5052636

Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. Th

Uranus - true and false colors - Voyager 2 - Uranus in true and false colors - Images obtained by the Voyager 2 probe on January 17, 1986 at 9.1 million km from Uranus. On the left image in real colors, the blue color is due to the presence of methane in the atmosphere of the planet; on the right, the false colours show a thick layer of fog around the south pole. The axis of rotation of the planet is different from that of all other planets in the solar system. While for most planets this axis is almost vertical, for Uranus it is almost lying on the plane of its orbit. These two pictures of Uranus - - one in true color (left) and the other in false color - - were compiled from images returned Jan. 17, 1986, by the narrow - angle camera of Voyager 2. The spacecraft was 9.1 million kilometers (5.7 million miles) from the planet, several days from closest approach. The picture at left has been processed to show Uranus as human eyes would see it from the vantage point of the spacecraft. Th

PIX4634727

Young stars in Rho Ophiuchi - Young stars in Rho Ophiuchi - Image of the central part of Rho Ophiuchi obtained in infrared by the Spitzer space telescope. Rho Ophiuchi is a vast dark cloud of molecular hydrogen located 407 years - light from Earth in the constellations of Ophiuchus and Scorpio. More than 300 young stars aged only 300,000 years have been observed. On this picture in false colors highlighting the temperature differences present in this cloud, the younger stars appear in red, the more evolute stars in blue. Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from Nasa's Spitzer Space Telescope. Called “” Rho Oph””” by astronomers, it's one of the closest star - forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new

Young stars in Rho Ophiuchi - Young stars in Rho Ophiuchi - Image of the central part of Rho Ophiuchi obtained in infrared by the Spitzer space telescope. Rho Ophiuchi is a vast dark cloud of molecular hydrogen located 407 years - light from Earth in the constellations of Ophiuchus and Scorpio. More than 300 young stars aged only 300,000 years have been observed. On this picture in false colors highlighting the temperature differences present in this cloud, the younger stars appear in red, the more evolute stars in blue. Newborn stars peek out from beneath their natal blanket of dust in this dynamic image of the Rho Ophiuchi dark cloud from Nasa's Spitzer Space Telescope. Called “” Rho Oph””” by astronomers, it's one of the closest star - forming regions to our own solar system. Located near the constellations Scorpius and Ophiuchus, the nebula is about 407 light years away from Earth. Rho Oph is a complex made up of a large main cloud of molecular hydrogen, a key molecule allowing new

PIX4621537

Moon Formation: Another Hypotheses of Giant Impact - Moon Formation: Hit-and-run Giant Impact Scenario: The hypothesis of giant impact suggests that the Moon was created from material ejected by a collision between the young Earth and a body the size of Mars named Theia 4.5 billion years ago. This scenario is widely accepted, but analyses of lunar samples have shown a major problem with this theory: the Moon should be composed mainly of Theia materials. The elements of the Moon and the Earth show remarkable similarities. Researchers explored a new collision geometry, changing the impact configuration. Their simulation also integrates a more energetic impact (called “hit and run”) that could tear more matter from Earth and make the pre-lunar debris disc dominate by terrestrial matter - The giant-impact hypothesis, sometimes called the Big Splash, or the Theia Impact suggests that the Moon formed out of the debris left over from a collision between Earth and a body of the size of Mars, a

Moon Formation: Another Hypotheses of Giant Impact - Moon Formation: Hit-and-run Giant Impact Scenario: The hypothesis of giant impact suggests that the Moon was created from material ejected by a collision between the young Earth and a body the size of Mars named Theia 4.5 billion years ago. This scenario is widely accepted, but analyses of lunar samples have shown a major problem with this theory: the Moon should be composed mainly of Theia materials. The elements of the Moon and the Earth show remarkable similarities. Researchers explored a new collision geometry, changing the impact configuration. Their simulation also integrates a more energetic impact (called “hit and run”) that could tear more matter from Earth and make the pre-lunar debris disc dominate by terrestrial matter - The giant-impact hypothesis, sometimes called the Big Splash, or the Theia Impact suggests that the Moon formed out of the debris left over from a collision between Earth and a body of the size of Mars, a

Miller, Ron (b.1947)

PIX4614860

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434239

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434236

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434240

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434243

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434237

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434242

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434235

Drawing Room from Lansdowne House, c.1766-75 (photo)

Drawing Room from Lansdowne House, c.1766-75 (photo)

Adam, Robert (1728-92)

PHL434248

Drawing Room from Lansdowne House, c.1766-75 (photo)

Drawing Room from Lansdowne House, c.1766-75 (photo)

Adam, Robert (1728-92)

PHL434251

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434234

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434238

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434241

Drawing Room from Lansdowne House, c.1766-75 (photo)

Drawing Room from Lansdowne House, c.1766-75 (photo)

Adam, Robert (1728-92)

PHL434252

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Drawing Room from Lansdowne House, c.1766-75 (photo) (detail)

Adam, Robert (1728-92)

PHL434245

Drawing Room from Lansdowne House, c.1766-75 (photo)

Drawing Room from Lansdowne House, c.1766-75 (photo)

Adam, Robert (1728-92)

PHL434246

Drawing Room from Lansdowne House, c.1766-75 (photo)

Drawing Room from Lansdowne House, c.1766-75 (photo)

Adam, Robert (1728-92)

PHL434247

Drawing Room from Lansdowne House, c.1766-75 (photo)

Drawing Room from Lansdowne House, c.1766-75 (photo)

Adam, Robert (1728-92)

PHL434249

Drawing Room from Lansdowne House, c.1766-75 (photo)

Drawing Room from Lansdowne House, c.1766-75 (photo)

Adam, Robert (1728-92)

PHL434250

Prince William Augustus, Duke of Cumberland (17211765)

Prince William Augustus, Duke of Cumberland (17211765)

Morier, David (1705-70) (studio of)

USB1159962

Study of a King Charles Spaniel (oil on canvas)

Study of a King Charles Spaniel (oil on canvas)

Chalon, Henry Bernard (1770-1849)

TW1212975

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