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Bilder zu 'Appearing' gefunden, 1,933

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Japan: Hidesaburo Ueno (Ueno Hidesaburo, c. 1871 - May 21, 1925) was an agricultural scientist, famous in Japan as the guardian of Hachiko, a devoted dog

Japan: Hidesaburo Ueno (Ueno Hidesaburo, c. 1871 - May 21, 1925) was an agricultural scientist, famous in Japan as the guardian of Hachiko, a devoted dog

PFH1773518

Japan: The monument to Chuken Hachiko 'Faithful dog Hachiko' at Shibuya being venerated on a rainy day one year after Hachiko's death, 9 March, 1936

Japan: The monument to Chuken Hachiko 'Faithful dog Hachiko' at Shibuya being venerated on a rainy day one year after Hachiko's death, 9 March, 1936

PFH1773521

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's h

Tethys, Saturn satellite, seen by the Cassini probe - Saturn's moon Tethys seen by Cassini spacecraft - The southern pole of the Tethys satellite photographed by the Cassini probe on September 24, 2005. Mosaic of nine images. With this full - disk mosaic, Cassini presents the best view yet of the south pole of Saturn's moon Tethys. The giant rift Ithaca Chasma cuts across the disk. Much of the topography seen here, including that of Ithaca Chasma, has a soft, muted appearance. It is clearly very old and has been heavily bombarded by impacts over time. Many of the fresh - appearing craters (ones with crisp relief) exhibit unusually bright crater floors. The origin of the apparent brightness (or “” albedo”) contrast is not known. It is possible that impacts punched through to a brighter layer underneath, or perhaps it is brighter because of different grain sizes or textures of the crater floor material in comparison to material along the crater walls and surrounding surface. The moon's h

PIX4625583

Cuba, Florida and Bahamas viewed by the Envisat satellite - Cuba, Florida and Bahamas from satellite Envisat - Florida (top left), Cuba (bottom) and the Bahamas viewed by the Envisat satellite on 24 January 2004. The shallow blue waters of the Bahamas as seen from Envisat 800 km away in space, acquired by the Medium Resolution Imaging Spectrometer (MERIS) on 24 January 2004. The Bahamas consist of a chain of islands and shallow water banks extending 1400 km from Florida to the island of Hispaniola. All the islands are surrounded by coral reefs - 5% of all the world's coral reefs are concentrated here. At the top left of the image is the southern tip of Florida, reaching from the circular Lake Okeechobee down through the Everglades all the way to Key West. The top of the curved archipelago of islands and associated coral reefs known as the Florida Keys is also visible. At the image base is the island of Cuba, 145 km south of Florida: the shaded area on the south face of the island is th

Cuba, Florida and Bahamas viewed by the Envisat satellite - Cuba, Florida and Bahamas from satellite Envisat - Florida (top left), Cuba (bottom) and the Bahamas viewed by the Envisat satellite on 24 January 2004. The shallow blue waters of the Bahamas as seen from Envisat 800 km away in space, acquired by the Medium Resolution Imaging Spectrometer (MERIS) on 24 January 2004. The Bahamas consist of a chain of islands and shallow water banks extending 1400 km from Florida to the island of Hispaniola. All the islands are surrounded by coral reefs - 5% of all the world's coral reefs are concentrated here. At the top left of the image is the southern tip of Florida, reaching from the circular Lake Okeechobee down through the Everglades all the way to Key West. The top of the curved archipelago of islands and associated coral reefs known as the Florida Keys is also visible. At the image base is the island of Cuba, 145 km south of Florida: the shaded area on the south face of the island is th

PIX4672985

Nebula NGC 281 in Cassiopee - Nebula NGC 281 in Cassiopeia - NGC 281 is a star-forming region about 10,000 light years away from Earth in the constellation Cassiopee. At the center of this nebula is the cluster of stars IC 1590 whose stars are only a few million years old. A composite of X-ray images obtained by the Chandra Space Telescope in purple and infrared by Spitzer in red green and blue. High - mass stars are important because they are responsible for much of the energy pumped into our galaxy over its lifetime. Unfortunately, these stars are poorly understood because they are often found relatively far away and can be obscured by gas and dust. The star cluster NGC 281 is an exception to this rule. It is located about 6,500 light years from Earth and, remarkably, almost 1,000 light years above the plane of the galaxy, giving astronomers a nearly unfettered view of the star formation within IT.This composite image of NGC 281 contains X - ray data from Chandra, in purple, with inf

Nebula NGC 281 in Cassiopee - Nebula NGC 281 in Cassiopeia - NGC 281 is a star-forming region about 10,000 light years away from Earth in the constellation Cassiopee. At the center of this nebula is the cluster of stars IC 1590 whose stars are only a few million years old. A composite of X-ray images obtained by the Chandra Space Telescope in purple and infrared by Spitzer in red green and blue. High - mass stars are important because they are responsible for much of the energy pumped into our galaxy over its lifetime. Unfortunately, these stars are poorly understood because they are often found relatively far away and can be obscured by gas and dust. The star cluster NGC 281 is an exception to this rule. It is located about 6,500 light years from Earth and, remarkably, almost 1,000 light years above the plane of the galaxy, giving astronomers a nearly unfettered view of the star formation within IT.This composite image of NGC 281 contains X - ray data from Chandra, in purple, with inf

PIX4617483

Sylvia Sidney By Alfredo Valente, 1940'S. Sylvia Sidney Was Born In New York City, In The Bronx, On August 8, 1910 With The Birth Name Of Sophia Kosow. As An Early Teen, Sylvia Had Decided That She Wanted A Stage Career. She Was Enrolled In The Theater Guild'S School For Acting. Sylvia Later Admitted That When She Decided To Become A Stage Actress At 15, It Wasn'T Being Starstruck That Occurred To Her, But The Expression Of Beauty That Encompassed Acting. All She Wanted Was To Be Identified With Good Productions. On The Strength Of Her Performance In New York, Sylvia Appeared In A Play At The Famed Poli Theater In Washington, D.C. More Stage Productions Followed, Each Better Than The Last And It Wasn'T Long Before The Film Moguls Were At The Doorstep. Sylvia Was Appearing In The Stage Production Of Crime When She Made Her First Appearance On The Silver Screen In 1927. Her Last Film For The Silver Screen Was Mars Attack! In 1996. In 1998 She Was Clia In The Tv Series Fantasy Island. Syl

Sylvia Sidney By Alfredo Valente, 1940'S. Sylvia Sidney Was Born In New York City, In The Bronx, On August 8, 1910 With The Birth Name Of Sophia Kosow. As An Early Teen, Sylvia Had Decided That She Wanted A Stage Career. She Was Enrolled In The Theater Guild'S School For Acting. Sylvia Later Admitted That When She Decided To Become A Stage Actress At 15, It Wasn'T Being Starstruck That Occurred To Her, But The Expression Of Beauty That Encompassed Acting. All She Wanted Was To Be Identified With Good Productions. On The Strength Of Her Performance In New York, Sylvia Appeared In A Play At The Famed Poli Theater In Washington, D.C. More Stage Productions Followed, Each Better Than The Last And It Wasn'T Long Before The Film Moguls Were At The Doorstep. Sylvia Was Appearing In The Stage Production Of Crime When She Made Her First Appearance On The Silver Screen In 1927. Her Last Film For The Silver Screen Was Mars Attack! In 1996. In 1998 She Was Clia In The Tv Series Fantasy Island. Syl

DIL4064980

The Hubble Space Telescope's Near Infrared Camera and Multi - Object Spectrometer (NICMOS) has captured a glimpse of a brief stage in the burnout of NGC 7027, a medium - mass star like our sun. THE INFRARED VIEW - - The composite color image of NGC 7027 (on the left) is among the first data of a planetary nebula taken with NICMOS. This picture is actually composed of three separate images taken at different wavelengths. The red color represents cool molecular hydrogen gas, the most abundant gas in the universe. The image reveals the central star, which is difficult to see in images taken with visible light. Surrounding it is an elongated region of gas and dust cast off by the star. This gas (appearing as white) has a temperature of several tens of thousands of degrees Fahrenheit. The object has two “” cones”” of cool molecular hydrogen gas (the red material) glowing in the infrared. The gas has been energized by ultraviolet light from the star - a process known as fluorescence. Most of

The Hubble Space Telescope's Near Infrared Camera and Multi - Object Spectrometer (NICMOS) has captured a glimpse of a brief stage in the burnout of NGC 7027, a medium - mass star like our sun. THE INFRARED VIEW - - The composite color image of NGC 7027 (on the left) is among the first data of a planetary nebula taken with NICMOS. This picture is actually composed of three separate images taken at different wavelengths. The red color represents cool molecular hydrogen gas, the most abundant gas in the universe. The image reveals the central star, which is difficult to see in images taken with visible light. Surrounding it is an elongated region of gas and dust cast off by the star. This gas (appearing as white) has a temperature of several tens of thousands of degrees Fahrenheit. The object has two “” cones”” of cool molecular hydrogen gas (the red material) glowing in the infrared. The gas has been energized by ultraviolet light from the star - a process known as fluorescence. Most of

PIX4623549

Remnants of Supernova of Vails - detail - Pencil Nebula (NGC 2376) - Remnants from a star that exploded thousands of years ago created a celestial abstract portrait, as captured in this image of the Pencil Nebula. Officially known as NGC 2736, the Pencil Nebula is part of the huge Vela supernova remnant, located in the southern constellation Vela. Discovered by Sir John Herschel in the 1840s, the nebula's linear appearance triggered its popular name. The nebula's shape suggests that it is part of the supernova shock wave that recently encountered a region of dense gas. It is this interaction that causes the nebula to glow, appearing like a rippled sheet. In this snapshot, astronomers are looking along the edge of the undulating sheet of gas. This view shows large, wispy filamentary structures, smaller bright knots of gas, and patches of diffuse gas. The Hubble Heritage Team used the Advanced Camera for Surveys in October 2002 to observe the nebula. The region of the Pencil Nebula captu

Remnants of Supernova of Vails - detail - Pencil Nebula (NGC 2376) - Remnants from a star that exploded thousands of years ago created a celestial abstract portrait, as captured in this image of the Pencil Nebula. Officially known as NGC 2736, the Pencil Nebula is part of the huge Vela supernova remnant, located in the southern constellation Vela. Discovered by Sir John Herschel in the 1840s, the nebula's linear appearance triggered its popular name. The nebula's shape suggests that it is part of the supernova shock wave that recently encountered a region of dense gas. It is this interaction that causes the nebula to glow, appearing like a rippled sheet. In this snapshot, astronomers are looking along the edge of the undulating sheet of gas. This view shows large, wispy filamentary structures, smaller bright knots of gas, and patches of diffuse gas. The Hubble Heritage Team used the Advanced Camera for Surveys in October 2002 to observe the nebula. The region of the Pencil Nebula captu

PIX4582819

Wise Collection 2: Scenes at street festival and rally in Calcutta (Kolkata)

Wise Collection 2: Scenes at street festival and rally in Calcutta (Kolkata)

BAF7424530

The Railway Station, c.1862-1909 (oil on canvas)

The Railway Station, c.1862-1909 (oil on canvas)

Frith, William Powell (1819-1909)

ROC5648129

'Jubilee', Herongate, Essex, 1935 (part 1)

'Jubilee', Herongate, Essex, 1935 (part 1)

ESS3483013

Cornwall, East and West Looe (watercolour)

Cornwall, East and West Looe (watercolour)

Rowlandson, Thomas (1756-1827)

CBE8833615

'Jubilee', Herongate, Essex, 1935 (part 1)

'Jubilee', Herongate, Essex, 1935 (part 1)

ESS3483012

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