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Mars: Sedimentary layers in Becquerel crater - Mars: Periodic Layering in Becquerel Crater - Detail on sedimentary layers in Becquerel crater (Arabia Terra region), obtained on June 10, 2007 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This image in false colors shows sedimentary rocks in pink, sand in blue. The study of these sedimentary depot strata suggests that the climate of Mars is linked to the inclination of the axis of rotation of the planet. Rhythmic bedding in sedimentary bedrock within Becquerel crater on Mars is suggested by the patterns in this image from the High Resolution Imaging Science Experiment (HiRise) camera on Nasa's Mars Reconnaissance Orbiter. Three dimensional analysis based on stereo pairs of images confirmed the regularity of repetition in the thickness of the beds. In the top half of this image, some of the rhythm is apparent as a series of bundles of about 10 individual layers per bundle. By corresponding to a known 10 - to - one p

PIX4616532

Mars: Sedimentary layers in Becquerel crater - Mars: Periodic Layering in Becquerel Crater - Detail on sedimentary layers in Becquerel crater (Arabia Terra region), obtained on June 10, 2007 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This image in false colors shows sedimentary rocks in pink, sand in blue. The study of these sedimentary depot strata suggests that the climate of Mars is linked to the inclination of the axis of rotation of the planet. Rhythmic bedding in sedimentary bedrock within Becquerel crater on Mars is suggested by the patterns in this image from the High Resolution Imaging Science Experiment (HiRise) camera on Nasa's Mars Reconnaissance Orbiter. Three dimensional analysis based on stereo pairs of images confirmed the regularity of repetition in the thickness of the beds. In the top half of this image, some of the rhythm is apparent as a series of bundles of about 10 individual layers per bundle. By corresponding to a known 10 - to - one p

PIX4616532

 
Clusters of distant galaxies RDCS1252.9 - 2927 - Distant galaxy cluster RDCS1252.9 - 2927 - This cluster of galaxies is 9 billion years old - light in the constellation Hydra, and is the most massive known to date. It probably contains several thousand galaxies. Image obtained by the Hubble Space Telescope and the VLT. The image shows the entire galaxy cluster (1/15 of a degree, corresponding to about 7 million light - years, across). The cluster probably contains many thousands of galaxies. Most of the other galaxies in the image, including most of the blue galaxies, are foreground or background galaxies. The image, which is made with an additional infrared exposure taken with the European Southern Observatory's Very Large Telescope, shows mature galaxies in a massive cluster that existed when the cosmos was 5000 million years old. The cluster, called RDCS1252.9 - 2927, is as massive as '300 trillion' suns and is the most massive known cluster for its epoch. Dominating the core are a

PIX4565578

Clusters of distant galaxies RDCS1252.9 - 2927 - Distant galaxy cluster RDCS1252.9 - 2927 - This cluster of galaxies is 9 billion years old - light in the constellation Hydra, and is the most massive known to date. It probably contains several thousand galaxies. Image obtained by the Hubble Space Telescope and the VLT. The image shows the entire galaxy cluster (1/15 of a degree, corresponding to about 7 million light - years, across). The cluster probably contains many thousands of galaxies. Most of the other galaxies in the image, including most of the blue galaxies, are foreground or background galaxies. The image, which is made with an additional infrared exposure taken with the European Southern Observatory's Very Large Telescope, shows mature galaxies in a massive cluster that existed when the cosmos was 5000 million years old. The cluster, called RDCS1252.9 - 2927, is as massive as '300 trillion' suns and is the most massive known cluster for its epoch. Dominating the core are a

PIX4565578

 
Acropolis, Beule Gate

SAP672495

Acropolis, Beule Gate

SAP672495

 
Swan Lace - detail - This delicate Hubble Space Telescope image shows a tiny portion of the Cygnus loop, a supernova remnant in the constellation of Cygnus, the Swan. Measurements on this super - detailed image of a cosmic veil shows that the original supernova explosion took place only 5000 years ago. The Cygnus loop, also known as the Veil Nebula, is well - known to amateur astronomers as a challenging target for larger telescopes. It has a diameter of about 3 degrees (corresponding to 6 full moons). This spectacular nebula was created when a massive star ended its days in an immense supernova explosion. A bubble of dust and gas was expelled into space and has continued to expand outwards ever since. The Cygnus Loop consists of two main arcs, designated NGC 6992/95 for the Eastern arc and NGC 6960 for the Western arc (also called the Witch's Broom Nebula). The tiny area of the Hubble image is seen in the upper left - hand corner of the nebula, at the outer edge of one of the large fi

PIX4582633

Swan Lace - detail - This delicate Hubble Space Telescope image shows a tiny portion of the Cygnus loop, a supernova remnant in the constellation of Cygnus, the Swan. Measurements on this super - detailed image of a cosmic veil shows that the original supernova explosion took place only 5000 years ago. The Cygnus loop, also known as the Veil Nebula, is well - known to amateur astronomers as a challenging target for larger telescopes. It has a diameter of about 3 degrees (corresponding to 6 full moons). This spectacular nebula was created when a massive star ended its days in an immense supernova explosion. A bubble of dust and gas was expelled into space and has continued to expand outwards ever since. The Cygnus Loop consists of two main arcs, designated NGC 6992/95 for the Eastern arc and NGC 6960 for the Western arc (also called the Witch's Broom Nebula). The tiny area of the Hubble image is seen in the upper left - hand corner of the nebula, at the outer edge of one of the large fi

PIX4582633

 
Southern Crown Nebula - The tail of the CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Our picture is about 4.5 degrees across and the extremely faint Corona Australis nebula meanders along the Sgr - CRA border nebula in the same E - W direction. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clou

PIX4620260

Southern Crown Nebula - The tail of the CRA reflection nebula - R Coronae Australis is a region of star formations visible in the southern hemisphere. It is located about 500 light years away from Earth. On the right, the globular cluster NGC 6723, located 30 000 light years from Earth in Sagittarius. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. Corona Australis (the southern crown, CRA) is in the far southern sky but visible from the southern states of the USA. The constellation is small but distinctive. The conspicuous globular cluster NGC 6723 is at the western (right) edge of the photograph, but it is in Sagittarius, and is about 30,000 light years distant. Our picture is about 4.5 degrees across and the extremely faint Corona Australis nebula meanders along the Sgr - CRA border nebula in the same E - W direction. Almost all the nebulosity here is starlight, reflected from minute grains of dust, some of which gather into darker condensations ('molecular clou

PIX4620260

 
Galaxy Clusters Abell 1689 - details - Gravitational lenses in Abell 1689 galaxy cluster - Close-up of the various gravitational mirages observed in the Abell 1689 galaxy cluster. Near infrared and visible image obtained by the Hubble space telescope in June 2002. 13 hours of installation. A selection of cropped images from a NASA Hubble Space Telescope Advanced Camera for Surveys view of one of the most massive galaxy clusters known, called Abell 1689. These close - ups show “” lensed”” images of background galaxies that have been brightened and smeared by the gravitational bending of light by the foreground cluster. The yellow - white objects are the cluster galaxies located 2.2 billion light - years away. The blue arcs are the distorted images of background galaxies located billions of light - years farther away than Abell 1689. The distribution of both “” normal”” and dark matter, and the alignment of the background galaxies determine the amount of distortion. In a perfectly aligne

PIX4565586

Galaxy Clusters Abell 1689 - details - Gravitational lenses in Abell 1689 galaxy cluster - Close-up of the various gravitational mirages observed in the Abell 1689 galaxy cluster. Near infrared and visible image obtained by the Hubble space telescope in June 2002. 13 hours of installation. A selection of cropped images from a NASA Hubble Space Telescope Advanced Camera for Surveys view of one of the most massive galaxy clusters known, called Abell 1689. These close - ups show “” lensed”” images of background galaxies that have been brightened and smeared by the gravitational bending of light by the foreground cluster. The yellow - white objects are the cluster galaxies located 2.2 billion light - years away. The blue arcs are the distorted images of background galaxies located billions of light - years farther away than Abell 1689. The distribution of both “” normal”” and dark matter, and the alignment of the background galaxies determine the amount of distortion. In a perfectly aligne

PIX4565586

 
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A large figure, most likely representing Hermes Trismegistus; at his head, a largely illegible scroll; he is embracing a large, stoppered flask (the arms of which bear writing and symbols), which contains a black frog, feathers and tadpoles or droplets of liquid at the top, and eight roundels connected to a central roundel by chains, representing stages in the alchemical process. Seven of the roundels depict figures conducting alchemical experiments involving a large flask containing homunculi atop a furnace; the eighth roundel contains a sun and and moon, corresponding silver and gold figures, and two figures dressed in red robes wielding tools. A large scroll, bearing an inscription: 'Terra stat unda lavat pyr purgat spiritus vivificat'; beneath, a further inscription: 'The mouth of the Collorick beware and thereof be wise'; two walls, enclosing a burst of flame. - a tree, its upper branches bearing inscriptions 'spiritus' and 'anima'; a naked, dragon-tailed woman is straddling its

BL3292659

A large figure, most likely representing Hermes Trismegistus; at his head, a largely illegible scroll; he is embracing a large, stoppered flask (the arms of which bear writing and symbols), which contains a black frog, feathers and tadpoles or droplets of liquid at the top, and eight roundels connected to a central roundel by chains, representing stages in the alchemical process. Seven of the roundels depict figures conducting alchemical experiments involving a large flask containing homunculi atop a furnace; the eighth roundel contains a sun and and moon, corresponding silver and gold figures, and two figures dressed in red robes wielding tools. A large scroll, bearing an inscription: 'Terra stat unda lavat pyr purgat spiritus vivificat'; beneath, a further inscription: 'The mouth of the Collorick beware and thereof be wise'; two walls, enclosing a burst of flame. - a tree, its upper branches bearing inscriptions 'spiritus' and 'anima'; a naked, dragon-tailed woman is straddling its

BL3292659

 
Star Vega in the Lyre - Star Vega in infrared - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical

PIX4571758

Star Vega in the Lyre - Star Vega in infrared - Vega (Alpha Lyrae) is the main star of the constellation Lyra, located only 25.4 light years from the Sun. It is the second brightest star after Sirius in the northern hemisphere. It's seen here in infrared by the Spitzer space telescope. Observed in this wavelength, the dust cloud surrounding the star appears. Nasa's Spitzer Space Telescope captured these images of the star Vega, located 25 light years away in the constellation Lyra. Spitzer was able to detect the heat radiation from the cloud of dust around the star and found that the debris disk is much larger than previously thought. This side - by - side comparison, taken by Spitzer's multiband imaging photometer, shows the warm infrared glows from dust particles orbiting the star at wavelengths of 24 microns (on the left in blue) and 70 microns (on the right in red). Both images show a very large, circular and smooth debris disk. The disk radius extends to at least 815 astronomical

PIX4571758

 
Distant galaxies in the Fornax constellation - Distant galaxies in the Fornax constellation - Image of distant galaxies obtained by the Hubble space telescope in the constellation Forneau in September 2003. This image represents a typical view of our distant universe. In taking this picture, Hubble is looking down a long corridor of galaxies stretching billions of light - years distant in space, corresponding to looking billions of years back in time. The field shown in this picture covers a relatively small patch of sky, a fraction of the area of the full moon, yet it is richly populated with a variety of galaxy types. A handful of large fully formed galaxies are scattered throughout the image. These galaxies are easy to see because they are relatively close to us. Several of the galaxies are spirals with flat disks that are oriented edge - on or face - on to our line of sight, or somewhere in between. Elliptical galaxies and more exotic galaxies with bars or tidal tails are also visi

PIX4613828

Distant galaxies in the Fornax constellation - Distant galaxies in the Fornax constellation - Image of distant galaxies obtained by the Hubble space telescope in the constellation Forneau in September 2003. This image represents a typical view of our distant universe. In taking this picture, Hubble is looking down a long corridor of galaxies stretching billions of light - years distant in space, corresponding to looking billions of years back in time. The field shown in this picture covers a relatively small patch of sky, a fraction of the area of the full moon, yet it is richly populated with a variety of galaxy types. A handful of large fully formed galaxies are scattered throughout the image. These galaxies are easy to see because they are relatively close to us. Several of the galaxies are spirals with flat disks that are oriented edge - on or face - on to our line of sight, or somewhere in between. Elliptical galaxies and more exotic galaxies with bars or tidal tails are also visi

PIX4613828

 
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  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
A large figure, most likely representing Hermes Trismegistus; at his head, a scroll bearing an inscription ('Est lapis occultus secreto fonte sepultus; he is embracing a large, stoppered flask (the arms of which bear writing), which contains a black frog, feathers and tadpoles or droplets of liquid at the top, and eight roundels, seven of which are connected to a central roundel by gold bands, which represent stages in the alchemical process. Seven of the roundels depict figures conducting alchemical experiments involving a large flask containing homunculi atop a furnace; the eighth (detached) roundel contains a sun and moon, corresponding silver and gold figures (Adam and Eve beside the Tree of Knowledge, around which a serpent is entwined), and two figures dressed in red robes wielding tools. The central roundel depicts two men holding a large book, to which the connecting bands are attached. All of the roundels contain inscriptions around their borders. a title 'An Alkemye Scrowle,

BL3292641

A large figure, most likely representing Hermes Trismegistus; at his head, a scroll bearing an inscription ('Est lapis occultus secreto fonte sepultus; he is embracing a large, stoppered flask (the arms of which bear writing), which contains a black frog, feathers and tadpoles or droplets of liquid at the top, and eight roundels, seven of which are connected to a central roundel by gold bands, which represent stages in the alchemical process. Seven of the roundels depict figures conducting alchemical experiments involving a large flask containing homunculi atop a furnace; the eighth (detached) roundel contains a sun and moon, corresponding silver and gold figures (Adam and Eve beside the Tree of Knowledge, around which a serpent is entwined), and two figures dressed in red robes wielding tools. The central roundel depicts two men holding a large book, to which the connecting bands are attached. All of the roundels contain inscriptions around their borders. a title 'An Alkemye Scrowle,

BL3292641

 
Permessi
  • Permission required for non-editorial use (inc book and magazine covers). Please contact us
Map of post Jacobean Scotland in 1755, 10 years after the Battle of Culloden. The land of Culloden and Inverness. A very large and highly finished colored military survey of the kingdom of Scotland, exclusive of the islands, undertaken by order of William Augustus, Duke of Cumberland, and executed by Lieutenant [afterwards Major-General] William Roy, and other officers, under the superintendence of Lieut.-Col. David Watson, Deputy Quarter-Master-General of the Forces, in the years 1747-1755 drawn on a scale of about two inches to a mile: it is divided into 38 compartments which are contained in eight cases: a small map is attached, marked with corresponding divisions, to serve as a key to the arrangement. The Roy Map of Scotland, c.1755 The military survey of Scotland was carried out in the wake of the 1745 Jacobite uprising and was intended to ensure there was no repetition. It is arguably the British Library's greatest cartographic treasure. Various versions survive, all kept in the

BL3287569

Map of post Jacobean Scotland in 1755, 10 years after the Battle of Culloden. The land of Culloden and Inverness. A very large and highly finished colored military survey of the kingdom of Scotland, exclusive of the islands, undertaken by order of William Augustus, Duke of Cumberland, and executed by Lieutenant [afterwards Major-General] William Roy, and other officers, under the superintendence of Lieut.-Col. David Watson, Deputy Quarter-Master-General of the Forces, in the years 1747-1755 drawn on a scale of about two inches to a mile: it is divided into 38 compartments which are contained in eight cases: a small map is attached, marked with corresponding divisions, to serve as a key to the arrangement. The Roy Map of Scotland, c.1755 The military survey of Scotland was carried out in the wake of the 1745 Jacobite uprising and was intended to ensure there was no repetition. It is arguably the British Library's greatest cartographic treasure. Various versions survive, all kept in the

BL3287569

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