'Melipal' immagini e video risultati

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Immagini di 'Melipal' trovate, 33

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Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

UIG2915902

Southern Cross Unit Telescope 3 (photo)

Southern Cross Unit Telescope 3 (photo)

UIG2915900

Southern Cross Unit Telescope 3 & Moon Unit Telescope 2 (photo)

Southern Cross Unit Telescope 3 & Moon Unit Telescope 2 (photo)

UIG2915884

Moon Unit Telescope 2 & Southern Cross Unit Telescope 3 (photo)

Moon Unit Telescope 2 & Southern Cross Unit Telescope 3 (photo)

UIG2915879

Auxiliary Telescope, Sun Unit Telescope 1, Moon Unit Telescope 2 & Southern Cross Unit Telescope 3 (photo)

Auxiliary Telescope, Sun Unit Telescope 1, Moon Unit Telescope 2 & Southern Cross Unit Telescope 3 (photo)

UIG2915910

Sun Unit Telescope 1, Moon Unit Telescope 2 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2 (photo)

UIG2915878

Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

UIG2915883

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3 & Venus Unit Telescope 4 (photo)

UIG2915909

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

UIG2915897

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

Sun Unit Telescope 1, Moon Unit Telescope 2, Southern Cross Unit Telescope 3, Venus Unit Telescope 4 (photo)

UIG2915896

Observatory of Paranal, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - domes of 8.2m Kueyen and Melipal telescopes; in the background, the VST. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. This picture shows Kueyen and Melipal, two of the four 8,2m telescopes, with in the background, the VST. March 2008

Observatory of Paranal, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - domes of 8.2m Kueyen and Melipal telescopes; in the background, the VST. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. This picture shows Kueyen and Melipal, two of the four 8,2m telescopes, with in the background, the VST. March 2008

Stephane Guisard

PIX4657027

Paranal Observatory - Chile - 2005 - View of the VLT, Very Large Telescope, consists of 4 main telescopes of 8.2m in diameter and 1.8m in diameter. From left to right, the telescopes ANTU, Kueyen, MELIPAL, the auxiliary telescope AT1, the VST, AT2 and YEPUN

Paranal Observatory - Chile - 2005 - View of the VLT, Very Large Telescope, consists of 4 main telescopes of 8.2m in diameter and 1.8m in diameter. From left to right, the telescopes ANTU, Kueyen, MELIPAL, the auxiliary telescope AT1, the VST, AT2 and YEPUN

PIX4656736

Paranal Observatory - Chile - 2001 - View of the VLT, Very Large Telescope, consists of 4 main telescopes of 8.2m in diameter. From left to right, the telescopes ANTU, Kueyen, MELIPAL and YEPUN. Located in the Atacama desert in northern Chile, at an altitude of 2,635 meters, it studies the sky in wavelengths ranging from ultraviolet to infrared

Paranal Observatory - Chile - 2001 - View of the VLT, Very Large Telescope, consists of 4 main telescopes of 8.2m in diameter. From left to right, the telescopes ANTU, Kueyen, MELIPAL and YEPUN. Located in the Atacama desert in northern Chile, at an altitude of 2,635 meters, it studies the sky in wavelengths ranging from ultraviolet to infrared

PIX4656676

Paranal Observatory - Chile - Aerienne view of the VLT, Very Large Telescope, consists of 4 main telescopes measuring 8.2m in diameter. Here the YEPUN telescope is in the foreground, in the background, from left to right, the ANTU, Kueyen and MELIPAL telescopes. Located in the Atacama desert in northern Chile, at an altitude of 2,635 meters, it studies the sky in wavelengths ranging from ultraviolet to infrared

Paranal Observatory - Chile - Aerienne view of the VLT, Very Large Telescope, consists of 4 main telescopes measuring 8.2m in diameter. Here the YEPUN telescope is in the foreground, in the background, from left to right, the ANTU, Kueyen and MELIPAL telescopes. Located in the Atacama desert in northern Chile, at an altitude of 2,635 meters, it studies the sky in wavelengths ranging from ultraviolet to infrared

PIX4656657

Paranal Observatory - Chile - 2000 - View of the VLT, Very Large Telescope, consists of 4 main telescopes of 8.2 m in diameter. Here the YEPUN telescope is in the foreground, in the background, from left to right, the ANTU, Kueyen and MELIPAL telescopes. Located in the Atacama desert in northern Chile, at an altitude of 2,635 meters, it studies the sky in wavelengths ranging from ultraviolet to infrared

Paranal Observatory - Chile - 2000 - View of the VLT, Very Large Telescope, consists of 4 main telescopes of 8.2 m in diameter. Here the YEPUN telescope is in the foreground, in the background, from left to right, the ANTU, Kueyen and MELIPAL telescopes. Located in the Atacama desert in northern Chile, at an altitude of 2,635 meters, it studies the sky in wavelengths ranging from ultraviolet to infrared

PIX4656654

Paranal Observatory - The VLT - 2006 - View of the VLT, Very Large Telescope, consists of 4 main telescopes measuring 8.2m in diameter. From left to right, the telescopes ANTU, Kueyen, MELIPAL and YEPUN. In the foreground, the 4 auxilliary telescopes measuring 1.8m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, the VLT studies the sky in wavelengths ranging from ultraviolet to infrared

Paranal Observatory - The VLT - 2006 - View of the VLT, Very Large Telescope, consists of 4 main telescopes measuring 8.2m in diameter. From left to right, the telescopes ANTU, Kueyen, MELIPAL and YEPUN. In the foreground, the 4 auxilliary telescopes measuring 1.8m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, the VLT studies the sky in wavelengths ranging from ultraviolet to infrared

Stephane Guisard

PIX4656740

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656703

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656715

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656691

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656709

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656712

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656706

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

View of the VLT, Very Large Telescope, consists of 4 main telescopes 8.2m in diameter. Located in the Atacama desert in northern Chile, at an altitude of 2,635 metres, it studies the sky in wavelengths ranging from ultraviolet to infrared - This european observatory accomodates the Very Large Telescope (VLT) since 1998. Four 8.2m telescopes are used besides several other telescopes from 1.8m to 4m. The four giant telescopes are named ANTU, KUEYEN, MELIPAL and YEPUN. Cerro Paranal is 2600 meters in altitude in Atacama desert: Observatoire du Paranal-Le VLT - The Very Large Telescope (VLT)

L. Weinstein

PIX4656710

Paranal Observatory, Chile: The Very Large Telescope (VLT) and its auxiliary telescopes seen on August 9, 2014. In the sky the galaxy of Andromede is visible. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Paranal Observatory, Chile: The Very Large Telescope (VLT) and its auxiliary telescopes seen on August 9, 2014. In the sky the galaxy of Andromede is visible. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Alex Tudorica

PIX4657492

Telescope Yepun - Paranal Observatory, Chile - Yepun and the Magellanic clouds - Paranal Observatory, Chile: The 8,2m diameter telescope Yepun and an auxiliary telescope seen on August 8, 2014. In the sky the clouds of Magellan. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Telescope Yepun - Paranal Observatory, Chile - Yepun and the Magellanic clouds - Paranal Observatory, Chile: The 8,2m diameter telescope Yepun and an auxiliary telescope seen on August 8, 2014. In the sky the clouds of Magellan. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Alex Tudorica

PIX4657504

Paranal Observatory, Chile - Paranal and the Full Moon: The Very Large Telescope (VLT) seen on 11 August 2014 lit by the full moon. The full Moon shines over the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Paranal Observatory, Chile - Paranal and the Full Moon: The Very Large Telescope (VLT) seen on 11 August 2014 lit by the full moon. The full Moon shines over the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode of operation

Alex Tudorica

PIX4657499

Paranal Observatory, Chile - Sunrise at VLT - Paranal Observatory, Chile: The Very Large Telescope (VLT) and an auxiliary telescope seen at the end of the night on August 9, 2014. In the sky the galaxy of Andromede is visible. The morning has arrived at the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode

Paranal Observatory, Chile - Sunrise at VLT - Paranal Observatory, Chile: The Very Large Telescope (VLT) and an auxiliary telescope seen at the end of the night on August 9, 2014. In the sky the galaxy of Andromede is visible. The morning has arrived at the Very Large Telescope (VLT), the flagship optical observatory of the European Southern Observatory (ESO) and the most advanced one in the world now. The four 8m telescopes telescopes, named Antu (Sun), Kueyen (Moon), Melipal (Southern Cross), and Yepun (Venus) form a very versatile observatory. They can be used as a single large telescope that adds (incoherently) the light from all four, in order to achieve the light gathering ability of a single 16m telescope. Also, their light can be combined in a coherent manner in order to achieve a solving power equivalent to the one of a telescope with a diameter as large as the baseline between the units. Of course, all the telescopes can be used individually, which is usually the default mode

Alex Tudorica

PIX4657511

Spiral galaxy NGC 7424 in the Crane - Galaxy NGC 7424 in Grus - The barree spiral galaxy NGC 7424 is located about 40 million years away from Earth. NGC 7424 extends over nearly 100,000 light years, like our galaxy. Numerous bright blue clusters of massive young stars are visible along the spiral arms. Image obtained by the telescope MELIPAL of the VLT on October 9, 2004 Composite colour - coded image of spiral galaxy, NGC 7424, at a distance of 40 million light - years. This galaxy is classified as “” SAB (rs) cd””, meaning that it is intermediate between normal spirals (SA) and strongly barred galaxies (SB) and that it has rather open arms with a small central region. It also shows many ionised regions as well as clusters of young and massive stars. Ten young massive star clusters can be identified whose size span the range from 1 to 200 light - years. The galaxy itself is roughly 100,000 light - years across, that is, quite similar in size to our own Milky Way galaxy. Images obtaine

Spiral galaxy NGC 7424 in the Crane - Galaxy NGC 7424 in Grus - The barree spiral galaxy NGC 7424 is located about 40 million years away from Earth. NGC 7424 extends over nearly 100,000 light years, like our galaxy. Numerous bright blue clusters of massive young stars are visible along the spiral arms. Image obtained by the telescope MELIPAL of the VLT on October 9, 2004 Composite colour - coded image of spiral galaxy, NGC 7424, at a distance of 40 million light - years. This galaxy is classified as “” SAB (rs) cd””, meaning that it is intermediate between normal spirals (SA) and strongly barred galaxies (SB) and that it has rather open arms with a small central region. It also shows many ionised regions as well as clusters of young and massive stars. Ten young massive star clusters can be identified whose size span the range from 1 to 200 light - years. The galaxy itself is roughly 100,000 light - years across, that is, quite similar in size to our own Milky Way galaxy. Images obtaine

PIX4613160

Barree spiral galaxy NGC 613 in the Sculptor - Barred spiral galaxy NGC 613 in Sculptor - Image of the barree spiral galaxy NGC 613 realized by the Very Large Telescope in December 2001. Unlike most barred spirals, this galaxy has multiple arms. It's assumed that a black hole sits in its center. Barred spiral galaxy NGC 613 obtained with the FORS1 and FORS2 multi - mode instruments (at VLT MELIPAL and YEPUN, respectively) on December 16 - 18, 2001. It is a composite of three exposures in different wavebands. NGC 613 is a beautiful barred spiral galaxy in the southern constellation Sculptor. This galaxy is inclined by 32 degrees and, contrary to most barred spirals, has many arms that give it a tentacular appearance. Prominent dust lanes are visible along the large - scale bar. Extensive star - formation occurs in this area, at the ends of the bar, and also in the nuclear regions of the galaxy. The gas at the centre, as well as the radio properties are indicative of the presence of a ma

Barree spiral galaxy NGC 613 in the Sculptor - Barred spiral galaxy NGC 613 in Sculptor - Image of the barree spiral galaxy NGC 613 realized by the Very Large Telescope in December 2001. Unlike most barred spirals, this galaxy has multiple arms. It's assumed that a black hole sits in its center. Barred spiral galaxy NGC 613 obtained with the FORS1 and FORS2 multi - mode instruments (at VLT MELIPAL and YEPUN, respectively) on December 16 - 18, 2001. It is a composite of three exposures in different wavebands. NGC 613 is a beautiful barred spiral galaxy in the southern constellation Sculptor. This galaxy is inclined by 32 degrees and, contrary to most barred spirals, has many arms that give it a tentacular appearance. Prominent dust lanes are visible along the large - scale bar. Extensive star - formation occurs in this area, at the ends of the bar, and also in the nuclear regions of the galaxy. The gas at the centre, as well as the radio properties are indicative of the presence of a ma

PIX4609353

Spiral galaxy NGC 1792 in Dove - Spiral galaxy NGC 1792 in Columba - NGC 1792 is located in the southern constellation Dove. Image obtained by the VLT in December 2001 NGC 1792 is located in the southern constellation Columba (The Dove). It is a starburst spiral galaxy. Its optical appearance is quite chaotic, due to the patchy distribution of dust throughout the disc of this galaxy. It is very rich in neutral hydrogen gas - fuel for the formation of new stars - and is indeed rapidly forming such stars. The galaxy is characterized by unusually luminous far - infrared radiation; this is due to dust heated by young stars. Image taken on 16 - 18 December 2001 with the VLT

Spiral galaxy NGC 1792 in Dove - Spiral galaxy NGC 1792 in Columba - NGC 1792 is located in the southern constellation Dove. Image obtained by the VLT in December 2001 NGC 1792 is located in the southern constellation Columba (The Dove). It is a starburst spiral galaxy. Its optical appearance is quite chaotic, due to the patchy distribution of dust throughout the disc of this galaxy. It is very rich in neutral hydrogen gas - fuel for the formation of new stars - and is indeed rapidly forming such stars. The galaxy is characterized by unusually luminous far - infrared radiation; this is due to dust heated by young stars. Image taken on 16 - 18 December 2001 with the VLT

PIX4609960

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Stephane Guisard

PIX4657141

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama Desert in the northern part of Chile. March 2008

Stephane Guisard

PIX4657134

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. The Very Large Telescope (VLT) and auxiliary telescopes. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama desert in the northern part of Chile. March 2008

Paranal Observatory, Chile 03/2008 - Paranal Observatory, Chile 03/2008 - Panorama of the Paranal Observatory at dusk. The Very Large Telescope (VLT) and auxiliary telescopes. March 2008. Paranal Observatory is an astronomical observatory located on the top of Cerro Paranal in the Atacama desert in the northern part of Chile. March 2008

Stephane Guisard

PIX4657128

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