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The Heir of the Ages, by James Payn (engraving)

The Heir of the Ages, by James Payn (engraving)

Furniss, Harry (1854-1925) (after)

LIP1623196

High Cross With Cathedral, Ireland (photo)

High Cross With Cathedral, Ireland (photo)

DPS3503954

Broughty Castle, c.1860 (oil on panel)

Broughty Castle, c.1860 (oil on panel)

Fraser, Alexander Jnr. (1828-99)

DNE6199911

Gustave Dore Bible: The apparition of the army in the heavens (engraving)

Gustave Dore Bible: The apparition of the army in the heavens (engraving)

Dore, Gustave (1832-83)

LLM5221591

Tantallon Castle, 1869 (w/c)

Tantallon Castle, 1869 (w/c)

Bough, Samuel (1822-78)

DNE6200708

Swan Boats On Pond By Historic Westport House; Westport, County Mayo, Ireland (photo)

Swan Boats On Pond By Historic Westport House; Westport, County Mayo, Ireland (photo)

DPS3503190

WW1 - Large Aerial Dogfight

WW1 - Large Aerial Dogfight

EPL7022253

Red Ivy Growing On The Side Of Muckross House; Killarney, County Kerry, Ireland (photo)

Red Ivy Growing On The Side Of Muckross House; Killarney, County Kerry, Ireland (photo)

DPS3503182

Gustave Dores Don Quixote: "The morn began to spread her smiling looks in the eastern quarter of the skies" (engraving)

Gustave Dores Don Quixote: "The morn began to spread her smiling looks in the eastern quarter of the skies" (engraving)

Dore, Gustave (1832-83)

LLM6008409

Portal Tomb, County Armagh, Ireland (photo)

Portal Tomb, County Armagh, Ireland (photo)

DPS3249530

Bushmills Church, County Antrim, Ireland; Church And Cemetery In Winter (photo)

Bushmills Church, County Antrim, Ireland; Church And Cemetery In Winter (photo)

DPS3250029

The Catholic Cathedral of Our Lady of the Assumption Building Destroyed in an Earthquake, Port-Au-Prince, Haiti (photo)

The Catholic Cathedral of Our Lady of the Assumption Building Destroyed in an Earthquake, Port-Au-Prince, Haiti (photo)

Reynold Mainse

DPS3319764

Muckross house near killarney;County kerry ireland (photo)

Muckross house near killarney;County kerry ireland (photo)

Peter Zoeller

DPS3254731

People relaxing at the Beach at Coney Island in Brooklyn, New York, USA (photo)

People relaxing at the Beach at Coney Island in Brooklyn, New York, USA (photo)

Jenny Acheson

DPS3317434

Orion, c.1825 (card, paper, tissue)

Orion, c.1825 (card, paper, tissue)

Hall, Sydney (fl.1826)

MMM7340893

Leo Major and Leo Minor, c.1825 (card, paper, tissue )

Leo Major and Leo Minor, c.1825 (card, paper, tissue )

Hall, Sydney (fl.1826)

MMM7340886

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 gas in the known universe — 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

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

Yorkshire Moorland, 1942 (Watercolour)

Yorkshire Moorland, 1942 (Watercolour)

Campbell, Nesta Jennings (1876-1951)

TW7290965

BLUNT/PERSEUS/28/1849

BLUNT/PERSEUS/28/1849

Blunt, Charles F. (19th century)

EPL6798931

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 four times as large and even brighter than the famous Orion Nebula, the Carina Nebula is much less well known, due to its location far in the Southern Hemisphere. It was discovered by Nicolas Louis de Lacaille in 1751 - 52 from the Cape of Good Hope. This is an amazingly bright nebula. This image is in the classic “” Hubble palette”” where SII is assigned to red, H - alpha to green, and OIII to blue. RGB frames were taken for star colors — 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

The Meteora, Greece - Kalabaka

The Meteora, Greece - Kalabaka

EPL6921830

NEW YORK FOURTH OF JULY FIREWORKS, 2002-07-04 (photo)

NEW YORK FOURTH OF JULY FIREWORKS, 2002-07-04 (photo)

Peter Morgan

REU8013732

FIREWORKS EXPLODE OVER NEW YORK CITY, 2002-07-04 (photo)

FIREWORKS EXPLODE OVER NEW YORK CITY, 2002-07-04 (photo)

Peter Morgan

REU8011030

III Reich, soldiers in maneuver 1939 (photo)

III Reich, soldiers in maneuver 1939 (photo)

SZT11749217

Spiral Galaxy M31 in Andromede - Detail - The southern arm of the Andromeda galaxy, M31 - View of the southern arm of the Andromede galaxy. Visible to the naked eye, the Andromede galaxy is located about 2 million years away from Earth. In this image obtained in La Palma, one of its two satellite galaxies is visible to the north-east: M32 (NGC 221). Also visible is the star cloud NGC 206, low centre, one of the largest star formations regions of our local group. Like the lactee path, the Andromede galaxy belongs to the local group, which consists of about thirty galaxies. M31 is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. Despite its distance it can be seen as an elongated streak with the unaided eye in northern skies and in a large telescope under good conditions it is clearly resolved into stars and star - forming regions. This picture shows less than half the galaxy but the spiral structure, star clouds and dust lanes are evident. Also here is one of M31's close companions, the compact elliptical galaxy M32 (NGC 221), (top). M31 and its companions belong to the Local Group of about 30 galaxies that includes the Milky Way and M31 as its most massive members as well as the Magellanic Clouds. <BR>This picture is about half a degree across and is of the same region as the frontispiece in Hubble's famous book “” The Realm of the Nebulae”” (Harvard UP, 1936). In his illustration Hubble points out a Cepheid variable star, a globular cluster, a star cloud and open cluster as typical ingredients of a spiral galaxy. The star cloud is so conspicuous that it has its own New General Catalogue number, NGC 206 — Spiral Galaxy M31 in Andromede - Detail - The southern arm of the Andromeda galaxy, M31 - View of the southern arm of the Andromede galaxy. Visible to the naked eye, the Andromede galaxy is located about 2 million years away from Earth. In this image obtained in La Palma, one of its two satellite galaxies is visible to the north-east: M32 (NGC 221). Also visible is the star cloud NGC 206, low centre, one of the largest star formations regions of our local group. Like the lactee path, the Andromede galaxy belongs to the local group, which consists of about thirty galaxies. M31 is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. Despite its distance it can be seen as an elongated streak with the unaided eye in northern skies and in a large telescope under good conditions it is clearly resolved into stars and star - forming regions. This picture shows less than half the galaxy but the spiral structure, star clouds and dust lanes are evident. Also he

Spiral Galaxy M31 in Andromede - Detail - The southern arm of the Andromeda galaxy, M31 - View of the southern arm of the Andromede galaxy. Visible to the naked eye, the Andromede galaxy is located about 2 million years away from Earth. In this image obtained in La Palma, one of its two satellite galaxies is visible to the north-east: M32 (NGC 221). Also visible is the star cloud NGC 206, low centre, one of the largest star formations regions of our local group. Like the lactee path, the Andromede galaxy belongs to the local group, which consists of about thirty galaxies. M31 is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. Despite its distance it can be seen as an elongated streak with the unaided eye in northern skies and in a large telescope under good conditions it is clearly resolved into stars and star - forming regions. This picture shows less than half the galaxy but the spiral structure, star clouds and dust lanes are evident. Also he

PIX4608878

Remains of the supernova Cassiopee A/HST - Cassiopeia A: Colorful, Shredded Remains of Old Supernova Glowing gaseous streamers of red, white, and blue - - as well as green and pink - - illuminate the heavens like Fourth of July fireworks. The colorful streamers that float across the sky in this photo taken by Nasa's Hubble Space Telescope were created by one of the biggest firecrackers seen to go off in our galaxy in recorded history, the titanic supernova explosion of a massive star. The light from the exploding star reached Earth 320 years ago, nearly a century before our United States celebrated its birth with a blow. The dead star's shredded remains are called Cassiopeia A, or “” Cas A”” for short. Cas A is the youngest known supernova remnant in our Milky Way Galaxy and resides 10,000 light - years away in the constellation Cassiopeia, so the star actually blew up 10,000 years before the light reached Earth in the late 1600s. This stunning Hubble image of Cas A is allowing astronomers to study the supernova's remains with great clarity, showing for the first time that the debris is arranged into thousands of small, cooling knots of gas. This material eventually will be recycled into building new generations of stars and planets. Our own Sun and planets are constructed from the debris of supernovae that exploded billions of years ago. This photo shows the upper rim of the supernova remnant's expanding shell. Near the top of the image are dozens of tiny clumps of matter. Each small clump, originally just a small fragment of the star, is tens of times larger than the diameter of our solar system. The colors highlight parts of the debris where chemical elements are glowing. The dark blue fragments, for example, are richest in oxygen; the red material is rich in sulfur. The star that created this colorful show was a big one, about 15 to 25 times more massive than our Sun. Massive stars like the one that created Cas A have short lives. They use up their supply of nuclea — Remains of the supernova Cassiopee A/HST - Cassiopeia A: Colorful, Shredded Remains of Old Supernova Glowing gaseous streamers of red, white, and blue - - as well as green and pink - - illuminate the heavens like Fourth of July fireworks. The colorful streamers that float across the sky in this photo taken by Nasa's Hubble Space Telescope were created by one of the biggest firecrackers seen to go off in our galaxy in recorded history, the titanic supernova explosion of a massive star. The light from the exploding star reached Earth 320 years ago, nearly a century before our United States celebrated its birth with a blow. The dead star's shredded remains are called Cassiopeia A, or “” Cas A”” for short. Cas A is the youngest known supernova remnant in our Milky Way Galaxy and resides 10,000 light - years away in the constellation Cassiopeia, so the star actually blew up 10,000 years before the light reached Earth in the late 1600s. This stunning Hubble image of Cas A is allowing astrono

Remains of the supernova Cassiopee A/HST - Cassiopeia A: Colorful, Shredded Remains of Old Supernova Glowing gaseous streamers of red, white, and blue - - as well as green and pink - - illuminate the heavens like Fourth of July fireworks. The colorful streamers that float across the sky in this photo taken by Nasa's Hubble Space Telescope were created by one of the biggest firecrackers seen to go off in our galaxy in recorded history, the titanic supernova explosion of a massive star. The light from the exploding star reached Earth 320 years ago, nearly a century before our United States celebrated its birth with a blow. The dead star's shredded remains are called Cassiopeia A, or “” Cas A”” for short. Cas A is the youngest known supernova remnant in our Milky Way Galaxy and resides 10,000 light - years away in the constellation Cassiopeia, so the star actually blew up 10,000 years before the light reached Earth in the late 1600s. This stunning Hubble image of Cas A is allowing astrono

PIX4582924

Beaches with Palm Trees, Aitutaki, Cook Island, Polynesia, South Pacific Ocean (photo)

Beaches with Palm Trees, Aitutaki, Cook Island, Polynesia, South Pacific Ocean (photo)

Reboredo, Sergi

SRB1202894

Aereial View of the Coast, Aitutaki, Cook Island, Polynesia, South Pacific Ocean (photo)

Aereial View of the Coast, Aitutaki, Cook Island, Polynesia, South Pacific Ocean (photo)

Reboredo, Sergi

SRB1202893

Beaches with Palm Trees, Aitutaki, Cook Island, Polynesia, South Pacific Ocean (photo)

Beaches with Palm Trees, Aitutaki, Cook Island, Polynesia, South Pacific Ocean (photo)

Reboredo, Sergi

SRB1202892

US Air Show Events, 1956.

US Air Show Events, 1956.

LTT7239398

La Ronde du Sabbat, ca. 1861 (oil on canvas)

La Ronde du Sabbat, ca. 1861 (oil on canvas)

Boulanger, Louis (1806-67)

XOS8984805

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