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Bilder zu 'Ost-Berlin (Ost-Berlin)' gefunden, 2,891

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Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case …, 1985 (photo)

Sächsische Zeitung

IMO8757629

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case …, 1985 (photo)

Saxony, GDR, historical, Turn, upheaval, Autumn 89, Fall of the Wall Case …, 1985 (photo)

Sächsische Zeitung

IMO8757619

Jan. 21, 1954 - Eastern Berliners Demonstrate For Murdered Jewish German Communists. President Pieck Speaks: At the same time as the Jews were being persecuted by the Soviets in all the Communist states - the GDR Government - the Eastern German Association ordered a demonstration by Eastern Berliners in” Memory” of two well known German Communists murdered 34 years ago - Karl Liebknecht and Rosa Luxenburg. A greet parade was held through the streets of East Berlin at which pictures of the” Martyrs” were carried. East German President Pieck made a speech at which he gave the unusual Soviet denounciations of the West

Jan. 21, 1954 - Eastern Berliners Demonstrate For Murdered Jewish German Communists. President Pieck Speaks: At the same time as the Jews were being persecuted by the Soviets in all the Communist states - the GDR Government - the Eastern German Association ordered a demonstration by Eastern Berliners in” Memory” of two well known German Communists murdered 34 years ago - Karl Liebknecht and Rosa Luxenburg. A greet parade was held through the streets of East Berlin at which pictures of the” Martyrs” were carried. East German President Pieck made a speech at which he gave the unusual Soviet denounciations of the West

ZUM4908934

Erich Honecker (5th from left, GDR SED Chairman of the Council of State) together with Kurt Hager (left, GDR SED member..., 1982 (photo)

Erich Honecker (5th from left, GDR SED Chairman of the Council of State) together with Kurt Hager (left, GDR SED member..., 1982 (photo)

Werner Schulze

IMO8788642

From left to right, front: Willi Stoph (GDR Chairman of the Council of Ministers), Walter ..., 1972 (photo)

From left to right, front: Willi Stoph (GDR Chairman of the Council of Ministers), Walter ..., 1972 (photo)

Werner Schulze

IMO8767992

From left to right, front: Willi Stoph (GDR Chairman of the Council of Ministers), Walter ..., 1972 (photo)

From left to right, front: Willi Stoph (GDR Chairman of the Council of Ministers), Walter ..., 1972 (photo)

Werner Schulze

IMO8767993

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Detail obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is the source region of Kasei Valles which extends 3000 km to the north. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Detail obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is the source region of Kasei Valles which extends 3000 km to the north. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel

PIX4616128

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Image obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is an approximately 100 km long and 10 km wide incision in the Lunae Planum high plateau north of Valles Marineris, the 'Grand Canyon' of Mars. Etus Chasma is the water source region of Kasei Valles, which extends thousands of kilometres to the north, and its southern - most part. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Image obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is an approximately 100 km long and 10 km wide incision in the Lunae Planum high plateau north of Valles Marineris, the 'Grand Canyon' of Mars. Etus Chasma is the water source region of Kasei Valles, which extends thousands of kilometres to the north, and its southern - most part. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel

PIX4616094

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Detail obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is the source region of Kasei Valles which extends 3000 km to the north. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel. The dark material shows a network of light - coloured, incised valleys that look similar to drainage networks known on Earth. It is still debated whether the valleys originate from precipitation, groundwater springs or liquid or magma flows on the surface

March: Echus Chasma - Mars: Echus Chasma - Echus Chasma is a valley located north of Valles Marineris. It is about 100 km long and 10 km wide. Detail obtained by the Mars Express probe in September 2005. The High - Resolution Stereo Camera (HRSC) on board ESA's Mars Express has returned images of Etus Chasma, one of the largest water source regions on the Red Planet. Echus Chasma is the source region of Kasei Valles which extends 3000 km to the north. The data was acquired on 25 September 2005. The pictures are centred at about 1* north and 278* east and have a ground resolution of approximately 17 m/pixel. The dark material shows a network of light - coloured, incised valleys that look similar to drainage networks known on Earth. It is still debated whether the valleys originate from precipitation, groundwater springs or liquid or magma flows on the surface

PIX4616125

Erich Honecker (5th from left, GDR SED Chairman of the Council of State) together with Werner Krolikowski (left, GDR..., 1982 (photo)

Erich Honecker (5th from left, GDR SED Chairman of the Council of State) together with Werner Krolikowski (left, GDR..., 1982 (photo)

Werner Schulze

IMO8788648

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained by the Mars Express probe, shows Tenuis Cavus, the end of this canyon, where layers of water ice mix with Mars dust. At the bottom of the bowl there are numerous sand dunes. Chasma Boreale is a huge canyon in the northern polar cap. The images taken by Mars Express spacecraft show sharp detail of a series of scarps at the head of Chasma Boreale, a giant trough that almost divides the north polar ice cap in two. The trough is about 318 kilometers long and has cliffs that are almost two kilometers high. The images show layers of water ice and dust possibly for the first time in perspective view. Chasma Boreale is cut into the layered material that lies beneath the water ice of the polar cap. For decades, these layered materials were assumed to consist of a mixture of ice and dust. Recent observations could mean tha

Mars: dunes and ice in Chasma Boreale - Mars: dunes and ice in Chasma Boreale - Chasma Boreale is a huge canyon located in the northern polar cap of Mars. This image, obtained by the Mars Express probe, shows Tenuis Cavus, the end of this canyon, where layers of water ice mix with Mars dust. At the bottom of the bowl there are numerous sand dunes. Chasma Boreale is a huge canyon in the northern polar cap. The images taken by Mars Express spacecraft show sharp detail of a series of scarps at the head of Chasma Boreale, a giant trough that almost divides the north polar ice cap in two. The trough is about 318 kilometers long and has cliffs that are almost two kilometers high. The images show layers of water ice and dust possibly for the first time in perspective view. Chasma Boreale is cut into the layered material that lies beneath the water ice of the polar cap. For decades, these layered materials were assumed to consist of a mixture of ice and dust. Recent observations could mean tha

PIX4615964

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