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Saturn by the Hubble Space Telecope - natural colors - 11/1999 - Saturn seen from the Hubble Space Telescope in november 1999 - The Saturn Planet observed with the Hubble Space Telescope in November 1999. Saturn is 120,000 km in diameter

Saturn by the Hubble Space Telecope - natural colors - 11/1999 - Saturn seen from the Hubble Space Telescope in november 1999 - The Saturn Planet observed with the Hubble Space Telescope in November 1999. Saturn is 120,000 km in diameter

PIX4624826

Solar sail near an exoplanet - Artist view - Solar sail and exoplanet - Artist view - View of a probe using solar wind and photons emitted by the Sun as a means of propulsion. The radiation pressure of sunlight on a huge expanse of very thin reflective material can gradually build up enough speed to reach another star

Solar sail near an exoplanet - Artist view - Solar sail and exoplanet - Artist view - View of a probe using solar wind and photons emitted by the Sun as a means of propulsion. The radiation pressure of sunlight on a huge expanse of very thin reflective material can gradually build up enough speed to reach another star

PIX4640485

Star Vega in Lyra - Star Vega in Lyra - 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 in the northern hemisphere after Sirius. Due to the precession of the equinoxes, Vega will take the place of the polar star indicating the north in the year 14,000. Vega (Alpha Lyrae) is the brightest star of Lyra constellation, located at 25.4 light years from the Sun. It is the second most luminous star in northern hemisphere. Because of the precession of the equinoxes, Vega will point north celestial pole in year 14,000

Star Vega in Lyra - Star Vega in Lyra - 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 in the northern hemisphere after Sirius. Due to the precession of the equinoxes, Vega will take the place of the polar star indicating the north in the year 14,000. Vega (Alpha Lyrae) is the brightest star of Lyra constellation, located at 25.4 light years from the Sun. It is the second most luminous star in northern hemisphere. Because of the precession of the equinoxes, Vega will point north celestial pole in year 14,000

Jerry Lodriguss

PIX4571757

Star Sky and Planet Venus - Starry sky with Venus - The brilliant Venus planet seen in the sky of Namibia. Brilliant planet Venus seen in Namibia

Star Sky and Planet Venus - Starry sky with Venus - The brilliant Venus planet seen in the sky of Namibia. Brilliant planet Venus seen in Namibia

Sebastian Voltmer

PIX4635006

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606678

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606690

Total Eclipse of Sun. 11/08/1999 - Total Solar Eclipse of 1999 Aug. 1

Total Eclipse of Sun. 11/08/1999 - Total Solar Eclipse of 1999 Aug. 1

Oshin Zakarian

PIX4627642

Mission Perseus - Return of J.P. Haignere - Jean - Pierre Haignere - Perseus mission - Jean - Pierre Haignere seen at the time of his return to Kazakhstan, after a six-month stay spent in space. The Perseus mission took place from 20 February to 28 August 1999 aboard the Mir station. ESA astronaut Jean-Pierre Haignere shortly after completion of the record - breaking “” Perseus”” mission to the Mir space station, on August 28 1999. With 6 Months in space, Jean-Pierre Haignere set a new duration record for a non - Russian astronaut. The “” Perseus”” mission occured from February 20 1999 till August 28 1999

Mission Perseus - Return of J.P. Haignere - Jean - Pierre Haignere - Perseus mission - Jean - Pierre Haignere seen at the time of his return to Kazakhstan, after a six-month stay spent in space. The Perseus mission took place from 20 February to 28 August 1999 aboard the Mir station. ESA astronaut Jean-Pierre Haignere shortly after completion of the record - breaking “” Perseus”” mission to the Mir space station, on August 28 1999. With 6 Months in space, Jean-Pierre Haignere set a new duration record for a non - Russian astronaut. The “” Perseus”” mission occured from February 20 1999 till August 28 1999

PIX4598458

Galaxy clusters 1ES 0657 - 55 in the Carene - Gravitational lens in galaxy cluster 1ES 0657 - 55 - False color image of the distant galaxy cluster 1ES 0657 - 55 in the southern constellation of Carene obtained by the VLT. A gravitational mirage is visible in the form of a green arc at the top right of the image; it is the image of an even farther away galaxy curved and amplified by the gravity of this cluster. An Arc at z = 3.23 in galaxy cluster 1ES 0657 - 55. The galaxy cluster 1ES 0657 - 55 is located in the southern constellation Carina (The Keel), south of the Milky Way band. Its redshift has been measured as z = 0.29. It is a source of strong and very hot X - ray emission and has an asymmetric galaxy distribution, indicating a large mass and recent formation

Galaxy clusters 1ES 0657 - 55 in the Carene - Gravitational lens in galaxy cluster 1ES 0657 - 55 - False color image of the distant galaxy cluster 1ES 0657 - 55 in the southern constellation of Carene obtained by the VLT. A gravitational mirage is visible in the form of a green arc at the top right of the image; it is the image of an even farther away galaxy curved and amplified by the gravity of this cluster. An Arc at z = 3.23 in galaxy cluster 1ES 0657 - 55. The galaxy cluster 1ES 0657 - 55 is located in the southern constellation Carina (The Keel), south of the Milky Way band. Its redshift has been measured as z = 0.29. It is a source of strong and very hot X - ray emission and has an asymmetric galaxy distribution, indicating a large mass and recent formation

PIX4565630

Spiral galaxy ESO 269 - 57 in Centaurus - Galaxy ESO 269 - 57 in Centaurus - The spiral galaxy ESO 269 - 57 is about 155 million years away - light from Earth. The picture shows the complex structure of ESO 269 - 57, with an inner “” ring””, of several tightly wound spiral arms, surrounded by two outer ones that appear to split into several branches. Many blue and diffuse objects are visible - most are star - forming regions. The galaxy type is Sa (r) and its distance is about 155 million light - years. It extends over about 4 arcmin in the sky, corresponding to almost 200,000 light - years across. Many other galaxies are visible in the background. This three - colour composite was obtained with VLT ANTU and FORS1 in the morning of March 27, 1999

Spiral galaxy ESO 269 - 57 in Centaurus - Galaxy ESO 269 - 57 in Centaurus - The spiral galaxy ESO 269 - 57 is about 155 million years away - light from Earth. The picture shows the complex structure of ESO 269 - 57, with an inner “” ring””, of several tightly wound spiral arms, surrounded by two outer ones that appear to split into several branches. Many blue and diffuse objects are visible - most are star - forming regions. The galaxy type is Sa (r) and its distance is about 155 million light - years. It extends over about 4 arcmin in the sky, corresponding to almost 200,000 light - years across. Many other galaxies are visible in the background. This three - colour composite was obtained with VLT ANTU and FORS1 in the morning of March 27, 1999

PIX4613539

Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. Image obtained by the 2,2m MPG telescope in Chile on March 25, 1999. Colour composite image of the peculiar galaxy Centaurus A (NGC 5128), obtained with the Wide - Field Imager (WFI) camera at the ESO/MPG 2.2 - m telescope on La Silla. It is based on a total of nine 3 - min exposures made on March 25, 1999, through different broad - band optical filters. The elliptical shape and the central dust band, the imprint of a galaxy collision, are well visible. North is up and East is to the left

Centaurus A elliptical galaxy (NGC 5128) in the Centaurus - Galaxy Centaurus A (NGC 5128) - The galaxy NGC 5128 is located about 13 million years away from Earth. Image obtained by the 2,2m MPG telescope in Chile on March 25, 1999. Colour composite image of the peculiar galaxy Centaurus A (NGC 5128), obtained with the Wide - Field Imager (WFI) camera at the ESO/MPG 2.2 - m telescope on La Silla. It is based on a total of nine 3 - min exposures made on March 25, 1999, through different broad - band optical filters. The elliptical shape and the central dust band, the imprint of a galaxy collision, are well visible. North is up and East is to the left

PIX4612257

Star Sirius in the Great Dog - Sirius in Canis Major - Sirius is the main star in the constellation Big Dog. Seen from the Earth, Sirius is the brightest star in the sky after the Sun. Sirius, the Dog Star, is the brightest star in the night sky at mag - 1.44 and it dominates the constellation of Canis Major. Sirius is a binary star with a white dwarf companion named Sirius B, “” The Pup”. It is an eight - magnitude star that is separated from Sirius by only a couple of arc seconds making it difficult to observe in a telescope because of the primary's great brilliance

Star Sirius in the Great Dog - Sirius in Canis Major - Sirius is the main star in the constellation Big Dog. Seen from the Earth, Sirius is the brightest star in the sky after the Sun. Sirius, the Dog Star, is the brightest star in the night sky at mag - 1.44 and it dominates the constellation of Canis Major. Sirius is a binary star with a white dwarf companion named Sirius B, “” The Pup”. It is an eight - magnitude star that is separated from Sirius by only a couple of arc seconds making it difficult to observe in a telescope because of the primary's great brilliance

Jerry Lodriguss

PIX4571719

ISS: Unity and Zarya modules 06/1999 - ISS first modules: Unity and Zarya 06/1999 - Unity and Zarya modules photographs from the Discovery shuttle. 03/06/1999 A STS - 96 crew member aboard Discovery recorded this image of the International Space Station (ISS) with a 70 mm camera during a fly - around following separation of the two spacecraft. Lake Hulun Nur in the People's Republic of China is visible in the lower left portion of the frame. Jun 03 1999

ISS: Unity and Zarya modules 06/1999 - ISS first modules: Unity and Zarya 06/1999 - Unity and Zarya modules photographs from the Discovery shuttle. 03/06/1999 A STS - 96 crew member aboard Discovery recorded this image of the International Space Station (ISS) with a 70 mm camera during a fly - around following separation of the two spacecraft. Lake Hulun Nur in the People's Republic of China is visible in the lower left portion of the frame. Jun 03 1999

PIX4599813

Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This image was obtained by the 2,2m MPG telescope in La Silla in 1999. NGC 4945 is a barred spiral galaxy in the Centaurus Group of galaxies, located only six times farther away than the prominent Andromeda Galaxy. The thin disk galaxy is oriented nearly edge - on, and shrouded in dark dust. NGC 4945 is thought to be quite similar to our own Milky Way Galaxy. X - ray observations reveal, however, that NGC 4945 has an unusual, energetic, Seyfert 2 nucleus that might house a large black hole. Image obtained by the 2.2m MPG telescope at La Silla observatory

Barree spiral galaxy NGC 4945 in Centaurus - Barred spiral galaxy NGC 4945 in Centaurus - The barree spiral galaxy NGC 4945 is located about 13 million years away - light from Earth. This image was obtained by the 2,2m MPG telescope in La Silla in 1999. NGC 4945 is a barred spiral galaxy in the Centaurus Group of galaxies, located only six times farther away than the prominent Andromeda Galaxy. The thin disk galaxy is oriented nearly edge - on, and shrouded in dark dust. NGC 4945 is thought to be quite similar to our own Milky Way Galaxy. X - ray observations reveal, however, that NGC 4945 has an unusual, energetic, Seyfert 2 nucleus that might house a large black hole. Image obtained by the 2.2m MPG telescope at La Silla observatory

PIX4612016

Spiral galaxies NGC 3314 A and B in Hydra - Galaxy pair NGC 3314 in Hydra - NGC 3314 is a pair of spiral galaxies distant about 140 million years - Earth light. These galaxies are not interacting but just perfectly aligned in front of each other from Earth. Through an extraordinary chance alignment, a face - on spiral galaxy lies precisely in front of another larger spiral. This line - up provides us with the rare chance to visualize dark material within the front galaxy, seen only because it is silhouetted against the object behind it. NGC 3314 lies about 140 million light - years from Earth, in the direction of the southern hemisphere constellation Hydra. The bright blue stars forming a pinwheel shape near the center of the front galaxy have formed recently from interstellar gas and dust. In many galaxies, interstellar dust lies only in the same regions as recently formed blue stars. However, in the foreground galaxy, NGC 3314a, there are numerous additional dark dust lanes that are

Spiral galaxies NGC 3314 A and B in Hydra - Galaxy pair NGC 3314 in Hydra - NGC 3314 is a pair of spiral galaxies distant about 140 million years - Earth light. These galaxies are not interacting but just perfectly aligned in front of each other from Earth. Through an extraordinary chance alignment, a face - on spiral galaxy lies precisely in front of another larger spiral. This line - up provides us with the rare chance to visualize dark material within the front galaxy, seen only because it is silhouetted against the object behind it. NGC 3314 lies about 140 million light - years from Earth, in the direction of the southern hemisphere constellation Hydra. The bright blue stars forming a pinwheel shape near the center of the front galaxy have formed recently from interstellar gas and dust. In many galaxies, interstellar dust lies only in the same regions as recently formed blue stars. However, in the foreground galaxy, NGC 3314a, there are numerous additional dark dust lanes that are

PIX4610557

Jerry Lodriguss and Astro Bezel - Physics 130 EDT - Astro - Physic's 130 EDT f/8 refractor - Astrophotographer Jerry Lodriguss and his Astro - Physic's 130 ED

Jerry Lodriguss and Astro Bezel - Physics 130 EDT - Astro - Physic's 130 EDT f/8 refractor - Astrophotographer Jerry Lodriguss and his Astro - Physic's 130 ED

Jerry Lodriguss

PIX4567108

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606692

Space Telescope XMM - Newton - Artist view - XMM - Newton space telescope. Artwork - The XMM - Newton space telescope is a European satellite that observes the Universe in X-ray and was launched and put into orbit in December 1999. XMM - Newton is an european X - Ray observatory launched in december 1999

Space Telescope XMM - Newton - Artist view - XMM - Newton space telescope. Artwork - The XMM - Newton space telescope is a European satellite that observes the Universe in X-ray and was launched and put into orbit in December 1999. XMM - Newton is an european X - Ray observatory launched in december 1999

D. Ducros

PIX4645569

Space Telescope XMM - Newton - Artist view - XMM - Newton space telescope. Artwork - The XMM - Newton space telescope is a European satellite that observes the Universe in X-ray and was launched and put into orbit in December 1999. XMM - Newton is an european X - Ray observatory launched in december 1999

Space Telescope XMM - Newton - Artist view - XMM - Newton space telescope. Artwork - The XMM - Newton space telescope is a European satellite that observes the Universe in X-ray and was launched and put into orbit in December 1999. XMM - Newton is an european X - Ray observatory launched in december 1999

D. Ducros

PIX4645542

Shooting Star-Illustration - Leonid meteor storm Artwork - Artist's view of a rain by Leonides

Shooting Star-Illustration - Leonid meteor storm Artwork - Artist's view of a rain by Leonides

S. Numazawa

PIX4599315

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

Mars Polar Lander - Artist view - Mars Polar Lander spaceprobe - Artist view - The American Mars Polar Lander probe, launched on January 3, 1999, was scheduled to land in December 1999 near the southern polar cap of Mars. Contact with the probe was interrupted on 3 December 1999, when it entered the Martian atmosphere. The Mars Polar Lander is shown on the surface of Mars. The spacecraft was launched in january 1999 to Mars to land near the southern polar cap in December 1999 and carry out a three - month mission to search for traces of subsurface water in this frozen, layered terrain. The contact with the spacecraft was lost on December 9, 1999, shortly after it entered the Martian atmosphere

PIX4606673

ISS: Unity and Zarya modules 06/1999 - ISS first modules: Unity and Zarya 06/1999 - Unity and Zarya modules photographs from the Discovery shuttle. 03/06/1999 A STS - 96 crew member aboard Discovery handling a 70 mm camera recorded this image of the International Space Station (ISS) during a fly - around following separation of the two spacecraft. Jun 03 1999

ISS: Unity and Zarya modules 06/1999 - ISS first modules: Unity and Zarya 06/1999 - Unity and Zarya modules photographs from the Discovery shuttle. 03/06/1999 A STS - 96 crew member aboard Discovery handling a 70 mm camera recorded this image of the International Space Station (ISS) during a fly - around following separation of the two spacecraft. Jun 03 1999

PIX4599820

Galaxies NGC 5090 - NGC 5091 in Centaurus - Interacting galaxies NGC 5090 - 5091 in Centaurus - NGC 5090 is an elliptical galaxy and NGC 5091 a spiral galaxy. These two galaxies interact and lie about 150 million light years away from Earth. This image was obtained by the ANTU telescope of the VLT on March 29, 1999. NGC 5090 is an elliptical galaxy interacting with the spiral galaxy NGC 5091. Both are located at about 150 million light - years away. Image taken with ANTU telescope (VLT) on March 29, 1999

Galaxies NGC 5090 - NGC 5091 in Centaurus - Interacting galaxies NGC 5090 - 5091 in Centaurus - NGC 5090 is an elliptical galaxy and NGC 5091 a spiral galaxy. These two galaxies interact and lie about 150 million light years away from Earth. This image was obtained by the ANTU telescope of the VLT on March 29, 1999. NGC 5090 is an elliptical galaxy interacting with the spiral galaxy NGC 5091. Both are located at about 150 million light - years away. Image taken with ANTU telescope (VLT) on March 29, 1999

PIX4612149

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

Detail of the globular cluster 47 Toucan - Starfield in the globular cluster 47 Tucanae, NGC 104 - The globular cluster 47 Toucan (or NGC 104) is visible to the naked eye from the southern hemisphere. Located about 15000 years ago - light it contains several million stars, some of which are among the older stars known today. This image obtained by the Hubble Space Telescope shows a detail of this cluster near its center; about 35,000 stars are visible. This image shows the Hubble telescope's close - up look at a swarm of 35, 000 stars near the club's central region. The stars are tightly packed together: They are much closer together than our Sun and its closest stars. The picture, taken by the Wide Field and Planetary Camera 2, depicts the stars' natural colors and tells scientists about their composition and age. For example, the red stars denote bright red giants nearing the end of their lives; the more common yellow stars are similar to our middle - aged Sun

PIX4564266

Mission Perseus - Return of J.P. Haignere - Jean - Pierre Haignere - Perseus mission - Jean - Pierre Haignere seen at the time of his return to Kazakhstan, after a six-month stay spent in space. The Perseus mission took place from 20 February to 28 August 1999 aboard the Mir station. ESA astronaut Jean-Pierre Haignere shortly after completion of the record - breaking “” Perseus”” mission to the Mir space station, on August 28 1999. With 6 Months in space, Jean-Pierre Haignere set a new duration record for a non - Russian astronaut. The “” Perseus”” mission occured from February 20 1999 till August 28 1999

Mission Perseus - Return of J.P. Haignere - Jean - Pierre Haignere - Perseus mission - Jean - Pierre Haignere seen at the time of his return to Kazakhstan, after a six-month stay spent in space. The Perseus mission took place from 20 February to 28 August 1999 aboard the Mir station. ESA astronaut Jean-Pierre Haignere shortly after completion of the record - breaking “” Perseus”” mission to the Mir space station, on August 28 1999. With 6 Months in space, Jean-Pierre Haignere set a new duration record for a non - Russian astronaut. The “” Perseus”” mission occured from February 20 1999 till August 28 1999

PIX4598447

Claude Nicollier in the shuttle Discovery STS - 103 1999 - Astronaut Claude Nicollier in Discovery - 1999 - Astronaut Claude Nicollier, mission specialist representing the European Space Agency (ESA), on Discovery's mid deck prior to a space walk in the weightlessness of space

Claude Nicollier in the shuttle Discovery STS - 103 1999 - Astronaut Claude Nicollier in Discovery - 1999 - Astronaut Claude Nicollier, mission specialist representing the European Space Agency (ESA), on Discovery's mid deck prior to a space walk in the weightlessness of space

PIX4647908

Shuttle Discovery in orbit and satellite 06/1999 - Shuttle Discovery with a satellite 06/1999 - STARSHINE (Student - Tracked Atmospheric Research Satellite for Heuristic International Networking Experiment) leaves Shuttle Discovery. The Student - Tracked Atmospheric Research Satellite for Heuristic International Networking Experiment (STARSHINE) satellite leaves the cargo bay of Discovery near the completion of the STS-96. Jun 05 1999

Shuttle Discovery in orbit and satellite 06/1999 - Shuttle Discovery with a satellite 06/1999 - STARSHINE (Student - Tracked Atmospheric Research Satellite for Heuristic International Networking Experiment) leaves Shuttle Discovery. The Student - Tracked Atmospheric Research Satellite for Heuristic International Networking Experiment (STARSHINE) satellite leaves the cargo bay of Discovery near the completion of the STS-96. Jun 05 1999

PIX4647712

ISS: Unity and Zarya modules 06/1999 - ISS first modules: Unity and Zarya 06/1999 - Unity and Zarya modules photographs from the Discovery shuttle. 03/06/1999 STS - 96 crew member aboard Discovery recorded this distant image of the International Space Station (ISS) with a 70 mm camera following separation of the two spacecraft. Russia's Lake Baykal, not far from the Mongolian border, can be seen in the background of the horizon view of Earth. Jun 03 1999

ISS: Unity and Zarya modules 06/1999 - ISS first modules: Unity and Zarya 06/1999 - Unity and Zarya modules photographs from the Discovery shuttle. 03/06/1999 STS - 96 crew member aboard Discovery recorded this distant image of the International Space Station (ISS) with a 70 mm camera following separation of the two spacecraft. Russia's Lake Baykal, not far from the Mongolian border, can be seen in the background of the horizon view of Earth. Jun 03 1999

PIX4599821

Sirius A and Sirius B in the Big Dog - Sirius A and Sirius B seen in X - ray - Sirius A and Sirius B in the Big Dog seen in X-ray by the Chandra telescope. The brightest source on this image is Sirius B, a white dwarf star whose surface, heated at a temperature of 25,000 degres, emits huge X-rays. The other point is Sirius A, the brightest star in the sky in visible light, but practically non-existent in this wavelength. An X - ray image of the Sirius star system located 8.6 light years from Earth. This image shows two sources and a spike - like pattern due to the support structure for the transmission grating. The bright source is Sirius B, a white dwarf star that has a surface temperature of about 25,000 degrees Celsius which produces very low energy X - rays. The dim source at the position of Sirius A, a normal star more than twice as massive as the Sun, may be due to ultraviolet radiation from Sirius A leaking through the filter on the detector. In contrast, Sirius A is the brighte

Sirius A and Sirius B in the Big Dog - Sirius A and Sirius B seen in X - ray - Sirius A and Sirius B in the Big Dog seen in X-ray by the Chandra telescope. The brightest source on this image is Sirius B, a white dwarf star whose surface, heated at a temperature of 25,000 degres, emits huge X-rays. The other point is Sirius A, the brightest star in the sky in visible light, but practically non-existent in this wavelength. An X - ray image of the Sirius star system located 8.6 light years from Earth. This image shows two sources and a spike - like pattern due to the support structure for the transmission grating. The bright source is Sirius B, a white dwarf star that has a surface temperature of about 25,000 degrees Celsius which produces very low energy X - rays. The dim source at the position of Sirius A, a normal star more than twice as massive as the Sun, may be due to ultraviolet radiation from Sirius A leaking through the filter on the detector. In contrast, Sirius A is the brighte

PIX4571724

Jupiter and Saturn in the Taurus -06/11/1999 - Jupiter and Saturn between the Hyades and Pleiades - Jupiter and Saturn between the Hyades and Pleiades, 1999-2000. November 6, 199

Jupiter and Saturn in the Taurus -06/11/1999 - Jupiter and Saturn between the Hyades and Pleiades - Jupiter and Saturn between the Hyades and Pleiades, 1999-2000. November 6, 199

PIX4587736

Shuttle Discovery in orbit - 06/1999 - Space shuttle Discovery in orbit 05/06/199

Shuttle Discovery in orbit - 06/1999 - Space shuttle Discovery in orbit 05/06/199

PIX4647711

Discovery shuttle in orbit - 12/1999 - Discovery shuttle and moon above the earth - STS103 Discovery above Earth. Dec 1999

Discovery shuttle in orbit - 12/1999 - Discovery shuttle and moon above the earth - STS103 Discovery above Earth. Dec 1999

PIX4647880

Total Eclipse of Sun. 11/08/1999 - Total Solar Eclipse of 1999 Aug. 1

Total Eclipse of Sun. 11/08/1999 - Total Solar Eclipse of 1999 Aug. 1

Oshin Zakarian

PIX4627611

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

Interacting galaxies Arp 81 - Interacting galaxies Arp 81 - Arp 81 is located about 300 million light years away from Earth in the constellation Dragon. This pair of interacting galaxies is composed of NGC 6621 on the left and NGC 6622 on the right. NGC 6621 is the largest of the two galaxies. The collision, seen here about 100 million years later, caused intense star flames. Image obtained by the Hubble Space Telescope on 15 March 1999. NGC 6621/2 (VV 247, Arp 81) is a strongly interacting pair of galaxies, seen about 100 million years after their closest approach. It consists of NGC 6621 (to the left) and NGC 6622 (to the right). NGC 6621 is the larger of the two, and is a very disturbed spiral galaxy. The encounter has pulled a long tail out of NGC 6621 that has now wrapped behind its body. The collision has also triggered extensive star formation between the two galaxies. Scientists believe that Arp 81 has a richer collection of young massive star clusters than the notable Antennae

PIX4612937

Discovery shuttle in orbit - 12/1999 - Discovery shuttle and moon above the earth - STS103 Discovery Dec 1999

Discovery shuttle in orbit - 12/1999 - Discovery shuttle and moon above the earth - STS103 Discovery Dec 1999

PIX4647929

Allee de Von Karman - Von Karman vortices - Allee of Karman swirls in the clouds caused by the encounter between the wind and the mountain peak of Alejandro Selkirk Island (Juan Fernandez Archipelago) off Chile. False colour image obtained by Landsat 7 satellite on 15 September 1999. Each of these swirling clouds is the result of a meteorological phenomenon known as a von Karman vortex. These vortices appeared over Alexander Selkirk Island in the southern Pacific Ocean. Rising precipitously from the surrounding waters, the island's highest point is nearly a mile (1.6 km) above sea level. As wind - driven clouds encounter this obstacle, they flow around it to form large, spinning eddies. This false color image was acquired by Landsat 7 satellite on September 15, 1999

Allee de Von Karman - Von Karman vortices - Allee of Karman swirls in the clouds caused by the encounter between the wind and the mountain peak of Alejandro Selkirk Island (Juan Fernandez Archipelago) off Chile. False colour image obtained by Landsat 7 satellite on 15 September 1999. Each of these swirling clouds is the result of a meteorological phenomenon known as a von Karman vortex. These vortices appeared over Alexander Selkirk Island in the southern Pacific Ocean. Rising precipitously from the surrounding waters, the island's highest point is nearly a mile (1.6 km) above sea level. As wind - driven clouds encounter this obstacle, they flow around it to form large, spinning eddies. This false color image was acquired by Landsat 7 satellite on September 15, 1999

PIX4674986

Center of the Orion Nebula - Trapeze - Orion nebula center - Mosaic of infrared images showing the center of the Orion Nebula, the Trapeze region. 4 massive stars form the Trapeze but the image also shows the cluster of stars associated with it, constitutes a thousand stars of about 1 million years old. Mosaic of 81 infrared images obtained by the ISAAC instrument at the VLT. Colour composite mosaic image of the central part of the Orion Nebula, based on 81 images obtained with the infrared multi - mode ISAAC instrument on the ESO Very Large Telescope (VLT) at the Paranal Observatory. The famous Trapezium stars are seen near the centre and the photo also shows the associated cluster of about one thousand stars, about a million years old

Center of the Orion Nebula - Trapeze - Orion nebula center - Mosaic of infrared images showing the center of the Orion Nebula, the Trapeze region. 4 massive stars form the Trapeze but the image also shows the cluster of stars associated with it, constitutes a thousand stars of about 1 million years old. Mosaic of 81 infrared images obtained by the ISAAC instrument at the VLT. Colour composite mosaic image of the central part of the Orion Nebula, based on 81 images obtained with the infrared multi - mode ISAAC instrument on the ESO Very Large Telescope (VLT) at the Paranal Observatory. The famous Trapezium stars are seen near the centre and the photo also shows the associated cluster of about one thousand stars, about a million years old

PIX4617863

Colliding spiral galaxies NGC 2207 and IC 2163 - Colliding galaxies NGC 2207 and IC 2163 - The galaxies NGC 2207 (left) and IC 2163 (right) form a pair of colliding galaxies approximately 114 million light years away. Currently IC 2163 is moving away from NGC 2207, but it is likely that within several billion years these two galaxies will eventually merge into a single massive galaxy. Image obtained by the Hubble Space Telescope in 1998. The larger and more massive galaxy is cataloged as NGC 2207 (on the left in the Hubble Heritage image), and the smaller one on the right is IC 2163. Strong tidal forces from NGC 2207 have distorted the shape of IC 2163, flinging out stars and gas into long streamers stretching out a hundred thousand light - years towards the right - hand edge of the image. The calculations indicate that IC 2163 is swinging past NGC 2207 in a counterclockwise direction, having made its closest approach 40 million years ago. However, IC 2163 does not have sufficient ener

Colliding spiral galaxies NGC 2207 and IC 2163 - Colliding galaxies NGC 2207 and IC 2163 - The galaxies NGC 2207 (left) and IC 2163 (right) form a pair of colliding galaxies approximately 114 million light years away. Currently IC 2163 is moving away from NGC 2207, but it is likely that within several billion years these two galaxies will eventually merge into a single massive galaxy. Image obtained by the Hubble Space Telescope in 1998. The larger and more massive galaxy is cataloged as NGC 2207 (on the left in the Hubble Heritage image), and the smaller one on the right is IC 2163. Strong tidal forces from NGC 2207 have distorted the shape of IC 2163, flinging out stars and gas into long streamers stretching out a hundred thousand light - years towards the right - hand edge of the image. The calculations indicate that IC 2163 is swinging past NGC 2207 in a counterclockwise direction, having made its closest approach 40 million years ago. However, IC 2163 does not have sufficient ener

PIX4610001

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. The NASA Hubble Space Telescope photo shows three regions of star birth: the long, sweeping tail and spiral arms of NGC 7319 [near center]; the gaseous debris of two galaxies, NGC 7318B and NGC 7318A [top right]; and the area north of those galaxies, dubbed the northern starburst region [top left]. The clusters' bluish color indicates that they're relatively young. Their ages span from about 2 million to more than 1 billion years old. The brilliant star clusters in NGC 7318B's spiral arm (about 30,000 light - years long) and the northern sta

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. The NASA Hubble Space Telescope photo shows three regions of star birth: the long, sweeping tail and spiral arms of NGC 7319 [near center]; the gaseous debris of two galaxies, NGC 7318B and NGC 7318A [top right]; and the area north of those galaxies, dubbed the northern starburst region [top left]. The clusters' bluish color indicates that they're relatively young. Their ages span from about 2 million to more than 1 billion years old. The brilliant star clusters in NGC 7318B's spiral arm (about 30,000 light - years long) and the northern sta

PIX4565466

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained by the ANTU telescope of the VLT in Chile in March 1999. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Image obtained with ANTU telescope (VLT) in March 1999

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classic spiral and a barree spiral. Image obtained by the ANTU telescope of the VLT in Chile in March 1999. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Image obtained with ANTU telescope (VLT) in March 1999

PIX4612419

Tognini prepares to return to Earth 07/1999 - Tognini prepares for Columbia's descent to Earth - Michel Tognini prepares to return to Earth after his space mission aboard the Columbia Shuttle. 27/07/1999. Michel Tognini, mission specialist representing France's Centre National d'Etudes Spatiales (CNES), prepares for Colombia's descent to Earth on the fifth and final day of the STS - 93 mission. Jul 27 1999

Tognini prepares to return to Earth 07/1999 - Tognini prepares for Columbia's descent to Earth - Michel Tognini prepares to return to Earth after his space mission aboard the Columbia Shuttle. 27/07/1999. Michel Tognini, mission specialist representing France's Centre National d'Etudes Spatiales (CNES), prepares for Colombia's descent to Earth on the fifth and final day of the STS - 93 mission. Jul 27 1999

PIX4647516

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained in 1999 by the European telescope Antu of the VLT in Chile. NGC 1365 is one of the most prominent “” barred”” galaxies in the sky. It is a supergiant galaxy with a diameter of about 200,000 light - years, seen in the direction of the southern constellation Fornax. It is a major member of the Fornax Cluster of Galaxies. The distance is about 60 million light - years. A massive straight bar runs through this galaxy and contains the nucleus at the centre. It consists mostly of older stars that give a reddish colour to the bar.The gravitational perturbation from the bar causes interstellar gas and dust clouds to form a pair of spiral arms that extend from the ends of the bar. Young luminous hot stars, born out of the inter

Barree spiral galaxy NGC 1365 in the Furnace - Barred spiral galaxy NGC 1365 in Fornax - NGC 1365 is a barree spiral galaxy that extends over 200,000 years - light. Located 60 million years ago - light, it belongs to the cluster of galaxies of the Furnace. Image obtained in 1999 by the European telescope Antu of the VLT in Chile. NGC 1365 is one of the most prominent “” barred”” galaxies in the sky. It is a supergiant galaxy with a diameter of about 200,000 light - years, seen in the direction of the southern constellation Fornax. It is a major member of the Fornax Cluster of Galaxies. The distance is about 60 million light - years. A massive straight bar runs through this galaxy and contains the nucleus at the centre. It consists mostly of older stars that give a reddish colour to the bar.The gravitational perturbation from the bar causes interstellar gas and dust clouds to form a pair of spiral arms that extend from the ends of the bar. Young luminous hot stars, born out of the inter

PIX4609836

Spiral galaxy ESO 510 - 13 in Hydra - Spiral galaxy ESO 510 - 13 in Hydra - The spiral galaxy ESO 510 - 13 is about 150 million years away - light from Earth and extends over about 100,000 years - light. Image obtained by the ANTU telescope of the VLT on March 15, 1999. The peculiar spiral galaxy ESO 510 - 13 resembles the famous “” Sombrero”” galaxy, but its equatorial dust plane is pronouncedly warped. Its distance is about 170 million light - years and the size is 100,000 light - years. This three - colour composite was obtained with VLT ANTU and FORS in the morning of March 15, 1999

Spiral galaxy ESO 510 - 13 in Hydra - Spiral galaxy ESO 510 - 13 in Hydra - The spiral galaxy ESO 510 - 13 is about 150 million years away - light from Earth and extends over about 100,000 years - light. Image obtained by the ANTU telescope of the VLT on March 15, 1999. The peculiar spiral galaxy ESO 510 - 13 resembles the famous “” Sombrero”” galaxy, but its equatorial dust plane is pronouncedly warped. Its distance is about 170 million light - years and the size is 100,000 light - years. This three - colour composite was obtained with VLT ANTU and FORS in the morning of March 15, 1999

PIX4613547

Project Daedalus - Vue d'artiste - Daedalus project - Artist view - Daedalus was an interstellar space probe project written in the 1970s. The aim was to make a probe capable of examining the Barnard star system in order to study possible planets. This hypothetical fusion - powered vehicle was designed by the British Interplanetary Society in the seventies. This interstellar unmanned spacecraft had to be able to reach the Barnard's star and to study its hypothetical planetary system

Project Daedalus - Vue d'artiste - Daedalus project - Artist view - Daedalus was an interstellar space probe project written in the 1970s. The aim was to make a probe capable of examining the Barnard star system in order to study possible planets. This hypothetical fusion - powered vehicle was designed by the British Interplanetary Society in the seventies. This interstellar unmanned spacecraft had to be able to reach the Barnard's star and to study its hypothetical planetary system

PIX4607470

Shooting star rain -Leonides 11/1999 - Leonid meteor shower Nov 1999 - Shooting star rain seen above the caravan of Deh Namak, Iran. Leonid meteor shower of Nov. 1999, Deh-Namak caravansary, Semnan, Iran

Shooting star rain -Leonides 11/1999 - Leonid meteor shower Nov 1999 - Shooting star rain seen above the caravan of Deh Namak, Iran. Leonid meteor shower of Nov. 1999, Deh-Namak caravansary, Semnan, Iran

Oshin Zakarian

PIX4598737

central area of M51 taken in picture in 1999

central area of M51 taken in picture in 1999

PIX5620155

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - Image obtained with the Hubble space telescope. This group of 5 galaxies is located about 270 million light years away from Earth. In this image three star-forming regions are visible: in the long arm of NGC 7319 (near the center); the gas debris of two galaxies, NGC 7318B and NGC 7318A (upper right); and in the upper left. Blue indicates that these stars are young. This NASA/ESA Hubble Space Telescope image is a close - up view of the central part of Stephan's Quintet, giving a magnificent view of a gigantic cosmic collision. Stephan's Quintet, as its name implies, is a group of five galaxies (NGC7317, 7318A, 7318B, 7319 and 7320) and lies about 270 million light - years away in the constellation of Pegasus (North - west of the Great Square of Pegasus). A sixth galaxy (NGC 7320C) lies south - east of the other five (upper left - hand corner of the overview image). The galaxy group was the first of its

PIX4565462

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - This group of 5 galaxies is located about 260 million years ago - light from Earth. These galaxies are interacting, however the NGC 7320 galaxy (down in the middle) would be 8 times closer to us. Image obtained with a telescope of 50 cm, cumulative poses of 40 hours. This group of galaxies is located about 260 million light - years away in Pegasus constellation. They are gravitationally interacting with the exception of the interloper NGC 7320 (bottom center) which is a foreground galaxy. Image made with a 20 inches telescope, total exposure 40 Hours

Galaxies Group: Stephan's Quintet in Pegase - Stephan's Quintet group of galaxies - This group of 5 galaxies is located about 260 million years ago - light from Earth. These galaxies are interacting, however the NGC 7320 galaxy (down in the middle) would be 8 times closer to us. Image obtained with a telescope of 50 cm, cumulative poses of 40 hours. This group of galaxies is located about 260 million light - years away in Pegasus constellation. They are gravitationally interacting with the exception of the interloper NGC 7320 (bottom center) which is a foreground galaxy. Image made with a 20 inches telescope, total exposure 40 Hours

R. Gendler

PIX4565481

Detail of the nebula NGC 3372 in the Carene - Eta Carinae nebula detail - Detail of the nebula NGC 3372 near the star Eta Carinae (off field). Region of star formation. Image obtained by the Hubble Space Telescope in April 1999. The Hubble Space Telescope image reveals complex structure in the Carina Nebula (NGC 3372). The picture is dominated by a large, approximately circular feature, which is part of the Keyhole Nebula. This region, about 8000 light - years from Earth, is located adjacent to the famous explosive variable star Eta Carinae, which lies just outside the field of view towards the upper right. The Carina Nebula also contains several other stars that are among the hottest and most massive known, each about 10 times as hot, and 100 times as massive, as our Sun

Detail of the nebula NGC 3372 in the Carene - Eta Carinae nebula detail - Detail of the nebula NGC 3372 near the star Eta Carinae (off field). Region of star formation. Image obtained by the Hubble Space Telescope in April 1999. The Hubble Space Telescope image reveals complex structure in the Carina Nebula (NGC 3372). The picture is dominated by a large, approximately circular feature, which is part of the Keyhole Nebula. This region, about 8000 light - years from Earth, is located adjacent to the famous explosive variable star Eta Carinae, which lies just outside the field of view towards the upper right. The Carina Nebula also contains several other stars that are among the hottest and most massive known, each about 10 times as hot, and 100 times as massive, as our Sun

PIX4618927

Interacting galaxies Arp 297 - Interacting galaxies Arp 297 - Arp 297 is located about 200 million light years away from Earth in the constellation Bovier. This pair of interacting galaxies consists of a large spiral galaxy, NGC 5754, and a small spiral galaxy, NGC 5752, at the bottom of the image. This interaction causes intense star flames within the small galaxy. Image obtained by the Hubble Space Telescope on March 14, 1999. This beautiful pair of interacting galaxies consists of NGC 5754, the large spiral on the right, and NGC 5752, the smaller companion in the bottom left corner of the image. NGC 5754's internal structure has hardly been disturbed by the interaction. The outer structure does exhibit tidal features, as does the symmetry of the inner spiral pattern and the kinked arms just beyond its inner ring. In contrast, NGC 5752 has undergone a starburst episode, with a rich population of massive and luminous star clusters clumping around the core and intertwined with intricat

Interacting galaxies Arp 297 - Interacting galaxies Arp 297 - Arp 297 is located about 200 million light years away from Earth in the constellation Bovier. This pair of interacting galaxies consists of a large spiral galaxy, NGC 5754, and a small spiral galaxy, NGC 5752, at the bottom of the image. This interaction causes intense star flames within the small galaxy. Image obtained by the Hubble Space Telescope on March 14, 1999. This beautiful pair of interacting galaxies consists of NGC 5754, the large spiral on the right, and NGC 5752, the smaller companion in the bottom left corner of the image. NGC 5754's internal structure has hardly been disturbed by the interaction. The outer structure does exhibit tidal features, as does the symmetry of the inner spiral pattern and the kinked arms just beyond its inner ring. In contrast, NGC 5752 has undergone a starburst episode, with a rich population of massive and luminous star clusters clumping around the core and intertwined with intricat

PIX4612781

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

PIX4567335

Venus in the Pleiades - Venus among the Pleiades, April 3 1999 - Venus among the Pleiades, April 3

Venus in the Pleiades - Venus among the Pleiades, April 3 1999 - Venus among the Pleiades, April 3

PIX4586749

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classical spiral and a barree spiral Image obtained by the ANTU telescope of the VLT in Chile in March 1999. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Image obtained with ANTU telescope (VLT) in March 1999

Spiral Galaxy M83 in Hydra - Spiral galaxy M83 in Hydra - The galaxy M83 (NGC 5236) is located about 15 million years away from Earth. This galaxy is intermediate between a classical spiral and a barree spiral Image obtained by the ANTU telescope of the VLT in Chile in March 1999. M83 (NGC 5236) is located in the southern constellation Hydra at 15 million light years from the sun. It is classified as intermediate between normal and barred spiral galaxies. Image obtained with ANTU telescope (VLT) in March 1999

PIX4612441

Spiral Galaxy NGC 4603 in Centaur - Cepheids in the galaxy NGC 4603 - The spiral galaxy NGC 4603 is located 108 million years - light. Its distance was accurately measured by the Hubble space telescope in 1999 using the study of cepheides, variable stars. More than 36 cepheides have been identified in this galaxy. The bright stars visible in this image are located in front of the galaxy and belong to our lactee path. NGC 4603, a galaxy is 108 million light - years away. Its distance has been accurately measured by astronomers using the pulsating variable stars known as Cepheids. The Hubble space telescope has identified more than 36 Cepheids in NGC 4603. The bright stars visible on this image are in foreground and belong to our galaxy

Spiral Galaxy NGC 4603 in Centaur - Cepheids in the galaxy NGC 4603 - The spiral galaxy NGC 4603 is located 108 million years - light. Its distance was accurately measured by the Hubble space telescope in 1999 using the study of cepheides, variable stars. More than 36 cepheides have been identified in this galaxy. The bright stars visible in this image are located in front of the galaxy and belong to our lactee path. NGC 4603, a galaxy is 108 million light - years away. Its distance has been accurately measured by astronomers using the pulsating variable stars known as Cepheids. The Hubble space telescope has identified more than 36 Cepheids in NGC 4603. The bright stars visible on this image are in foreground and belong to our galaxy

PIX4611662

Venus pres des Pleiades - Venus among the Pleiades, April 6, 1999 - Venus pres de l'amas des Pleiades April 6, 1999. Venus among the Pleiades, April 6, 1999

Venus pres des Pleiades - Venus among the Pleiades, April 6, 1999 - Venus pres de l'amas des Pleiades April 6, 1999. Venus among the Pleiades, April 6, 1999

PIX4586759

Launch of the space telescope XMM - Newton - Artist's view - Launch of XMM - Newton space telescope - The space telescope XMM - Newton is a European satellite that observes the Universe in X-ray; it was launched and put into orbit in December 1999 by an Ariane 5 rocket. XMM - Newton is an european X - Ray observatory launched in december 1999 by an Ariane 5 rocket

Launch of the space telescope XMM - Newton - Artist's view - Launch of XMM - Newton space telescope - The space telescope XMM - Newton is a European satellite that observes the Universe in X-ray; it was launched and put into orbit in December 1999 by an Ariane 5 rocket. XMM - Newton is an european X - Ray observatory launched in december 1999 by an Ariane 5 rocket

D. Ducros

PIX4645580

C. Nicollier and JF. Clervoy in the shuttle Discovery STS-103 - 1999 - C. Nicollier and JF. Clervoy in weightlessness 12/1999 - (19 - 27 December 1999) - - - Astronauts Claude Nicollier (left) and Jean - Francois Clervoy, mission specialists representing the European Space Agency (ESA), move about on Discovery's mid deck in a manner they could not duplicate in Earth - bound training. A photography

C. Nicollier and JF. Clervoy in the shuttle Discovery STS-103 - 1999 - C. Nicollier and JF. Clervoy in weightlessness 12/1999 - (19 - 27 December 1999) - - - Astronauts Claude Nicollier (left) and Jean - Francois Clervoy, mission specialists representing the European Space Agency (ESA), move about on Discovery's mid deck in a manner they could not duplicate in Earth - bound training. A photography

PIX4647909

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

PIX4567343

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

Eclipse of 11/08/1999: observation du soleil - Solar eclipse observation with safe solar glasses. August 11 1999 - Sun observation with protective glasses

PIX4567349

Star cluster in the nebula NGC 3603 - Star cluster in NGC 3603 nebula - Cluster of young stars in the nebula NGC 3603, located about 20,000 years ago - light from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope on 29 December 2005. NGC 3603 is a prominent star - forming region located in the Carina spiral arm of the Milky Way, about 20,000 light - years away from our Solar System. This image from the NASA/ESA Hubble Space Telescope shows a young star cluster surrounded by a vast region of dust and gas. Most of the bright stars in the image are hot blue stars whose ultraviolet radiation and violent winds have blown out an enormous cavity in the gas and dust enveloping the cluster

Star cluster in the nebula NGC 3603 - Star cluster in NGC 3603 nebula - Cluster of young stars in the nebula NGC 3603, located about 20,000 years ago - light from Earth in the southern constellation of Carene. Image obtained by the Hubble Space Telescope on 29 December 2005. NGC 3603 is a prominent star - forming region located in the Carina spiral arm of the Milky Way, about 20,000 light - years away from our Solar System. This image from the NASA/ESA Hubble Space Telescope shows a young star cluster surrounded by a vast region of dust and gas. Most of the bright stars in the image are hot blue stars whose ultraviolet radiation and violent winds have blown out an enormous cavity in the gas and dust enveloping the cluster

PIX4619157

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