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Baltimore, USA, shuttle view 02 - 2001 - Baltimore, Maryland (USA), viewed by shuttle STS-98 in February 2001

Baltimore, USA, shuttle view 02 - 2001 - Baltimore, Maryland (USA), viewed by shuttle STS-98 in February 2001

PIX4673311

Earth seen by Apollo 11 - July 1969 - Earth seen by Apollo 11 - July 1969 - North Montana with the Rocky Mountains seen from the Apollo module

Earth seen by Apollo 11 - July 1969 - Earth seen by Apollo 11 - July 1969 - North Montana with the Rocky Mountains seen from the Apollo module

PIX4673339

Manhattan, New York, view from space - Manhattan, New York City, seen from space - Manhattan Island to New York seen from the International Space Station March 26, 2005. Manhattan Island and its easily recognizable Central Park (center left) are featured in this image. Some of the other New York City boroughs (including parts of Queens and Brooklyn) are also shown, as are two small sections of the New Jersey side of the Hudson River (lower left and lower right). This astronaut photograph taken from International space station was acquired March 26, 2005

Manhattan, New York, view from space - Manhattan, New York City, seen from space - Manhattan Island to New York seen from the International Space Station March 26, 2005. Manhattan Island and its easily recognizable Central Park (center left) are featured in this image. Some of the other New York City boroughs (including parts of Queens and Brooklyn) are also shown, as are two small sections of the New Jersey side of the Hudson River (lower left and lower right). This astronaut photograph taken from International space station was acquired March 26, 2005

PIX4673344

Manhattan Island, New York, view from space - 11/09/2001 - Smoke plume from Manhattan, New York City - 11/09/2001 - The smoke plume escaping from Manhattan Island to New York seen from the International Space Station on 11 September 2001 11 September 2001 - One of a series of pictures taken of metropolitan New York City (and other parts of New York as well as New Jersey) by one of the Expedition Three crew members onboard the International Space Station (ISS) at various times during the day of September 11, 2001. The image shows a smoke plume rising from the Manhattan area. The orbital outpost was flying at an altitude of approximately 250 miles. The image was recorded with a digital still camera

Manhattan Island, New York, view from space - 11/09/2001 - Smoke plume from Manhattan, New York City - 11/09/2001 - The smoke plume escaping from Manhattan Island to New York seen from the International Space Station on 11 September 2001 11 September 2001 - One of a series of pictures taken of metropolitan New York City (and other parts of New York as well as New Jersey) by one of the Expedition Three crew members onboard the International Space Station (ISS) at various times during the day of September 11, 2001. The image shows a smoke plume rising from the Manhattan area. The orbital outpost was flying at an altitude of approximately 250 miles. The image was recorded with a digital still camera

PIX4673355

New York and Long Island views from space - New York City seen from space - New York, Long Island and reflections of the Sun seen from space shuttle Endeavour in February 2000. New York City, Long Island and sunglint. Image taken from space shuttle Endeavour in February 2000

New York and Long Island views from space - New York City seen from space - New York, Long Island and reflections of the Sun seen from space shuttle Endeavour in February 2000. New York City, Long Island and sunglint. Image taken from space shuttle Endeavour in February 2000

PIX4673392

East American Coast Night View - 04/2011 - Cities on east coast of the USA by night 04/2011 - Part of East American Coast View from International Space Station (ISS) on April 6, 2011. Light pollution in New York (right), Philadelphia, Baltimore, Washington DC, Richmond (extreme left) and Norfolk (bottom) contrasts with the darkness of the Atlantic Ocean. The Atlantic Seaboard Conurbation (ASC) on East Coast of the United States. The ASC extends over 1,000 kilometers (600 miles) and includes the major economic, governmental, and cultural centers of Boston, Massachusetts; New York, New York; Philadelphia, Pennsylvania; Baltimore, Maryland; and Washington, District of Columbia. This astronaut photograph includes every metropolitan area in the ASC except for Boston (located off the image to the northeast). This night image highlights the position and extent of each metropolitan area through urban lighting patterns. Two other large metropolitan areas are visible in the image - - Norfolk and

East American Coast Night View - 04/2011 - Cities on east coast of the USA by night 04/2011 - Part of East American Coast View from International Space Station (ISS) on April 6, 2011. Light pollution in New York (right), Philadelphia, Baltimore, Washington DC, Richmond (extreme left) and Norfolk (bottom) contrasts with the darkness of the Atlantic Ocean. The Atlantic Seaboard Conurbation (ASC) on East Coast of the United States. The ASC extends over 1,000 kilometers (600 miles) and includes the major economic, governmental, and cultural centers of Boston, Massachusetts; New York, New York; Philadelphia, Pennsylvania; Baltimore, Maryland; and Washington, District of Columbia. This astronaut photograph includes every metropolitan area in the ASC except for Boston (located off the image to the northeast). This night image highlights the position and extent of each metropolitan area through urban lighting patterns. Two other large metropolitan areas are visible in the image - - Norfolk and

PIX4673429

Utah - Nevada - Colorado - Wyoming (USA) seen by Shuttle 03 - 1994 - Utah - Nevada - Colorado - Wyoming (USA) seen by shuttle STS - 62 in March 199

Utah - Nevada - Colorado - Wyoming (USA) seen by Shuttle 03 - 1994 - Utah - Nevada - Colorado - Wyoming (USA) seen by shuttle STS - 62 in March 199

PIX4673486

Lake Powell - Utah: Lake Powell, Utah, USA, seen from the International Space Station (ISS) on September 6, 2016. This panorama, photographed by an astronaut aboard the International Space Station, shows almost the full length of Lake Powell, the reservoir on the Colorado River in southern Utah and northern Arizona. Note south is at the top left of the image. Image acquired on September 6, 2016.

Lake Powell - Utah: Lake Powell, Utah, USA, seen from the International Space Station (ISS) on September 6, 2016. This panorama, photographed by an astronaut aboard the International Space Station, shows almost the full length of Lake Powell, the reservoir on the Colorado River in southern Utah and northern Arizona. Note south is at the top left of the image. Image acquired on September 6, 2016.

PIX4673489

Bingham Canyon Copper Mine - USA - Bingham Canyon Mine - Utah: The Bingham Canyon Mine is an open-pit copper mine located southwest of the city of Salt Lake City, Utah. With a width of 4 km and a depth of more than 800 m, it is one of the largest mines in the world. Mining began at the site in 1906. Image taken from the International Space Station (ISS) on 20 September 2007. The Bingham Canyon Mine, more commonly known as Kennecott Copper Mine among locals, is an open-pit mining operation extracting a large porphyry copper deposit southwest of Salt Lake City, Utah, in the Oquirrh Mountains. The mine is the largest man-made excavation in the world and is considered to have produced more copper than any other mine in history - more than 19 million tonnes. Astronaut photograph was acquired on September 20 2007 from the International Space Station (ISS)

Bingham Canyon Copper Mine - USA - Bingham Canyon Mine - Utah: The Bingham Canyon Mine is an open-pit copper mine located southwest of the city of Salt Lake City, Utah. With a width of 4 km and a depth of more than 800 m, it is one of the largest mines in the world. Mining began at the site in 1906. Image taken from the International Space Station (ISS) on 20 September 2007. The Bingham Canyon Mine, more commonly known as Kennecott Copper Mine among locals, is an open-pit mining operation extracting a large porphyry copper deposit southwest of Salt Lake City, Utah, in the Oquirrh Mountains. The mine is the largest man-made excavation in the world and is considered to have produced more copper than any other mine in history - more than 19 million tonnes. Astronaut photograph was acquired on September 20 2007 from the International Space Station (ISS)

PIX4673491

Hurricane Florence - 09/2018

Hurricane Florence - 09/2018

PIX5894680

The Full Moon over earth, 2016 (photograph)

The Full Moon over earth, 2016 (photograph)

PIX5894690

Prominent Hill open pit mine - Australia

Prominent Hill open pit mine - Australia

PIX5894695

Open pit coal mines in New South Wales with Maules Creek Coal Mine at left and Boggabri coal mine at right. Image taken from the international space station in september 2018

Open pit coal mines in New South Wales with Maules Creek Coal Mine at left and Boggabri coal mine at right. Image taken from the international space station in september 2018

PIX5894699

Agriculture in Brazil in 2014

Agriculture in Brazil in 2014

PIX5894715

Agriculture in Brazil (photo)

Agriculture in Brazil (photo)

PIX5894717

Rio Doce, Brazil

Rio Doce, Brazil

PIX5894718

Phalaborwa Copper Mine - Republic South Africa

Phalaborwa Copper Mine - Republic South Africa

PIX5894538

Sivash Lagoons - Crimea

Sivash Lagoons - Crimea

PIX5894560

Crimea and the sea Image taken from the international space station in june 2018

Crimea and the sea Image taken from the international space station in june 2018

PIX5894565

Volcan Tambora. Ile de Sumbawa, indonesia

Volcan Tambora. Ile de Sumbawa, indonesia

PIX5894592

Nisyros - Grece

Nisyros - Grece

PIX5894625

SLS rocket launch - Artemis 1 - 11/2022 (photography)

SLS rocket launch - Artemis 1 - 11/2022 (photography)

PIX7331205

SLS rocket launch - Artemis 1 - 11/2022 (photography)

SLS rocket launch - Artemis 1 - 11/2022 (photography)

PIX7331206

Artemis 1 - Orion, the Moon and the Earth - 28/11/2022 (photography)

Artemis 1 - Orion, the Moon and the Earth - 28/11/2022 (photography)

PIX7331212

Telfer gold and copper mine - Australia, 2022 (photography)

Telfer gold and copper mine - Australia, 2022 (photography)

PIX7331236

Agriculture in Bolivia (photo)

Agriculture in Bolivia (photo)

PIX5973634

Escondida Mine, Chile (photo)

Escondida Mine, Chile (photo)

PIX5973639

Palabora Mine (Phalaborwa Copper Mine), South Africa (photo)

Palabora Mine (Phalaborwa Copper Mine), South Africa (photo)

PIX5973666

Tambora Volcano, Sumbawa Island, Indonesia (photo)

Tambora Volcano, Sumbawa Island, Indonesia (photo)

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Tambora Volcano, Sumbawa Island, Indonesia (photo)

Tambora Volcano, Sumbawa Island, Indonesia (photo)

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Tenoumer Impact Crater, Mauritania (photo)

Tenoumer Impact Crater, Mauritania (photo)

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Turow Coal Mine, Poland (photo)

Turow Coal Mine, Poland (photo)

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Ernest henry mine, 2018 (photo)

Ernest henry mine, 2018 (photo)

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ISS: The new Nauka module - 07/2021 (photo)

ISS: The new Nauka module - 07/2021 (photo)

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Actress Yulia Peresild in the International Space Station, 2021 (photo)

Actress Yulia Peresild in the International Space Station, 2021 (photo)

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Actress Yulia Peresild in the International Space Station, 2021 (photo)

Actress Yulia Peresild in the International Space Station, 2021 (photo)

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Star Cluster NGC 1872 in Dorado - Star Cluster NGC 1872 in Dorado - The NGC 1872 cluster is located in the galaxy of the Great Magellan Cloud. It is a cluster of globular shape, but young, composed of warm, blue stars. Image obtained by the Hubble Space Telescope. This Hubble Space Telescope picture shows NGC 1872, a rich cluster of thousands of stars lying in our small neighbouring galaxy, the Large Magellanic Cloud. This little - studied cluster is located in the constellation of Dorado. The Scottish astronomer James Dunlop was probably the first to spot NGC 1872 in 1826 with a small telescope near Sydney in Australia. Star clusters are usually classed as either open or globular but NGC 1872 has characteristics of both - - it is as rich as a typical globular but is much younger, and, like many open clusters, has bluer stars. Such intermediate clusters are common in the Large Magellanic Cloud

Star Cluster NGC 1872 in Dorado - Star Cluster NGC 1872 in Dorado - The NGC 1872 cluster is located in the galaxy of the Great Magellan Cloud. It is a cluster of globular shape, but young, composed of warm, blue stars. Image obtained by the Hubble Space Telescope. This Hubble Space Telescope picture shows NGC 1872, a rich cluster of thousands of stars lying in our small neighbouring galaxy, the Large Magellanic Cloud. This little - studied cluster is located in the constellation of Dorado. The Scottish astronomer James Dunlop was probably the first to spot NGC 1872 in 1826 with a small telescope near Sydney in Australia. Star clusters are usually classed as either open or globular but NGC 1872 has characteristics of both - - it is as rich as a typical globular but is much younger, and, like many open clusters, has bluer stars. Such intermediate clusters are common in the Large Magellanic Cloud

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Earth from space - Earth from space - Image of Earth recomposed from different satellite images Composite images obtained with data collected from several satellites

Earth from space - Earth from space - Image of Earth recomposed from different satellite images Composite images obtained with data collected from several satellites

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Samantha Cristoforetti in weightlessness - Samantha Cristoforetti in ISS: Italian astronaut Samantha Cristoforetti performs sports on board the International Space Station (ISS). Samantha Cristoforetti is to date the longest time in space, with a flight lasting 199 days and 16 hours.

Samantha Cristoforetti in weightlessness - Samantha Cristoforetti in ISS: Italian astronaut Samantha Cristoforetti performs sports on board the International Space Station (ISS). Samantha Cristoforetti is to date the longest time in space, with a flight lasting 199 days and 16 hours.

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Samantha Cristoforetti in weightlessness - Samantha Cristoforetti in ISS: Italian astronaut Samantha Cristoforetti brushes his teeth in the International Space Station (ISS). 5/12/2014

Samantha Cristoforetti in weightlessness - Samantha Cristoforetti in ISS: Italian astronaut Samantha Cristoforetti brushes his teeth in the International Space Station (ISS). 5/12/2014

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Samantha Cristoforetti in weightlessness - Samantha Cristoforetti in ISS: Italian astronaut Samantha Cristoforetti observes the Earth from Cupola, the panoramic dome of the International Space Station (ISS). Samantha Cristoforetti is to date the longest time in space, with a flight lasting 199 days and 16 hours.

Samantha Cristoforetti in weightlessness - Samantha Cristoforetti in ISS: Italian astronaut Samantha Cristoforetti observes the Earth from Cupola, the panoramic dome of the International Space Station (ISS). Samantha Cristoforetti is to date the longest time in space, with a flight lasting 199 days and 16 hours.

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Thomas Pesquet in weightlessness - Thomas Pesquet in ISS: French astronaut Thomas Pesquet takes pictures of the Earth in the International Space Station (ISS). 28 December 2016 - Thomas Pesquet of ESA (European Space Agency) is taking pictures in the International Space Station

Thomas Pesquet in weightlessness - Thomas Pesquet in ISS: French astronaut Thomas Pesquet takes pictures of the Earth in the International Space Station (ISS). 28 December 2016 - Thomas Pesquet of ESA (European Space Agency) is taking pictures in the International Space Station

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Exit in space by Thomas Pesquet - Thomas Pesquet EVA: The French astronaut Thomas Pesquet during his first extravehicular ride. 13 January 2017 - Thomas Pesquet first extravehicular activity on january 13 2017

Exit in space by Thomas Pesquet - Thomas Pesquet EVA: The French astronaut Thomas Pesquet during his first extravehicular ride. 13 January 2017 - Thomas Pesquet first extravehicular activity on january 13 2017

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Planetary nebula NGC 2440 in the stern - View of planetary nebula NGC 2440 in the stern obtained by the Hubble space telescope on 6 February 2007. The star in the center of the image is a white dwarf, a star at the end of life that expels the outer layers of its material all around it. Our Sun could have a similar fate in five billion years. This star is one of the hottest in history; its temperature is 200,000 degres Celsius. NGC 2440 is located about 4000 years from Earth

Planetary nebula NGC 2440 in the stern - View of planetary nebula NGC 2440 in the stern obtained by the Hubble space telescope on 6 February 2007. The star in the center of the image is a white dwarf, a star at the end of life that expels the outer layers of its material all around it. Our Sun could have a similar fate in five billion years. This star is one of the hottest in history; its temperature is 200,000 degres Celsius. NGC 2440 is located about 4000 years from Earth

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Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope (HST). The Hubble Space Telescope has captured the sharpest view yet of M57, the Ring Nebula in Lyra, which is the most famous of all planetary nebulae. In this image, the telescope has looked down a tunnel of gas cast off by a dying star thousands of years ago. This photo reveals elongated dark clumps of material embedded in the gas at the edge of the nebula, and the dying central star floating in a blue haze of hot gas. The nebula is about a light - year in diameter, and is located some 2,000 light - years from Earth in the direction of the constellation Lyra

Planetary nebula M57 (NGC 6720) in Lyra - The Ring nebula M57 in Lyra - The planetary nebula of Lyra (M57) is located about 2000 years - light from Earth. A planetary nebula is a gas shell from a small late-life star whose heart collapsed to become a white dwarf and expelled the outer layers of its matter. Image obtained by the Hubble Space Telescope (HST). The Hubble Space Telescope has captured the sharpest view yet of M57, the Ring Nebula in Lyra, which is the most famous of all planetary nebulae. In this image, the telescope has looked down a tunnel of gas cast off by a dying star thousands of years ago. This photo reveals elongated dark clumps of material embedded in the gas at the edge of the nebula, and the dying central star floating in a blue haze of hot gas. The nebula is about a light - year in diameter, and is located some 2,000 light - years from Earth in the direction of the constellation Lyra

R. Gendler

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Saturn and satellites seen by the Hubble-Saturn space telescope observed by the Hubble space telescope on 6 August 1995. At that time the Earth was almost in the same plane as the rings of Saturn which is why they appear seen by the slice. The Titan satellite projects its shadow on the planet and the Tethys satellite is visible just under the rings. On the left side, more images of Titan's move around Saturn

Saturn and satellites seen by the Hubble-Saturn space telescope observed by the Hubble space telescope on 6 August 1995. At that time the Earth was almost in the same plane as the rings of Saturn which is why they appear seen by the slice. The Titan satellite projects its shadow on the planet and the Tethys satellite is visible just under the rings. On the left side, more images of Titan's move around Saturn

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Barree spiral galaxy NGC 1559 - Barred spiral galaxy NGC 1559: The galaxy NGC 1559 is a galaxy of Seyfert located about 50 million light years ago in the constellation Reticule. Image obtained by the Hubble Space Telescope. Roughly 50 million light-years away lies a little galaxy named NGC 1559. Pictured here by Hubble's Wide Field Camera 3, this barred spiral lies in the southern constellation of Reticulum (The Reticule)

Barree spiral galaxy NGC 1559 - Barred spiral galaxy NGC 1559: The galaxy NGC 1559 is a galaxy of Seyfert located about 50 million light years ago in the constellation Reticule. Image obtained by the Hubble Space Telescope. Roughly 50 million light-years away lies a little galaxy named NGC 1559. Pictured here by Hubble's Wide Field Camera 3, this barred spiral lies in the southern constellation of Reticulum (The Reticule)

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Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

Spiral galaxy NGC 1566 in the bream - The Seyfert Galaxy NGC 1566: NGC 1566 is a spiral galaxy located about 40 million light years ago. Its core is very bright. It is an active galaxy called Seyfert, which probably houses a black hole in its heart. Image obtained with the Hubble telescope - NGC 1566 is a galaxy located approximately 40 million light-years away in the constellation of Dorado (The Dolphinfish). NGC 1566 is an intermediate spiral galaxy, meaning that while it does not have a well defined bar-shaped region of stars at its centre - like barred spirals - it is not quite an unbarred spiral either (heic9902o). The small but extremely bright nucleus of NGC 1566 is clearly visible in this image, a telltale sign of its membership of the Seyfert class of galaxies. The centres of such galaxies are very active and luminous, emitting strong bursts of radiation and potentially harbouring supermassive black holes that are many millions of times the mass of the Sun. NGC 1566 is not jus

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Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its lightning shrinking. Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its brightnes

Spiral Galaxy NGC 2397 - Galaxy Spiral NGC 2397 - The galaxy NGC 2397 is a classic spiral galaxy located about 60 million years ago - light from Earth in the southern constellation of Flying Fish. The central part houses old yellow and red stars while new stars form in the outer arms. This image obtained by the space telescope on 14 October 2006 shows the brightest of these young blue stars. The 2006bc supernova, which exploded in March 2006, is also visible near the central region, while its lightning shrinking. Located nearly 60 million light - years away from Earth, the galaxy NGC 2397 is typical of most spirals, with mostly older, yellow and red stars in its central portion, while star formation continues in the outer, bluer spiral arms. The brightest of these young, blue stars can be seen individually in this high resolution view from the Hubble's Advanced Camera for Surveys (ACS). One typical feature of this Hubble image is the view of supernova SN 2006bc taken when its brightnes

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Barree spiral galaxy NGC 2442 in Flying Fish - Barred spiral galaxy NGC 2442 in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Mosaic of images obtained by the Hubble Space Telescope and the 2.2 m MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This close - up Hubble view of the Meathook Galaxy (NGC 2442) focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These observations were made in 2006 in order to study the aftermath of this supernova. Ground - based data from MPG/ESO 2.2 - metre telescope were used to fill out parts of the edges of this image

Barree spiral galaxy NGC 2442 in Flying Fish - Barred spiral galaxy NGC 2442 in Volans - NGC 2442 is a barree spiral galaxy located about 50 million years ago - light. Its asymmetrical shape suggests that a galaxy interacts with it. Mosaic of images obtained by the Hubble Space Telescope and the 2.2 m MPG/ESO telescope at the La Silla Observatory. NGC 2442 is a barred spiral galaxy about 50 million light years away in the constellation Volans. This close - up Hubble view of the Meathook Galaxy (NGC 2442) focuses on the more compact of its two asymmetric spiral arms as well as the central regions. The spiral arm was the location of a supernova that exploded in 1999. These observations were made in 2006 in order to study the aftermath of this supernova. Ground - based data from MPG/ESO 2.2 - metre telescope were used to fill out parts of the edges of this image

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Spiral galaxy NGC 4402 - Spiral galaxy NGC 4402 - NGC 4402 is located about 60 million light years away from Earth in the galaxy cluster of Our Lady. Image obtained by the Hubble Space Telescope. Close - up of the disc of gas and dust of the spiral galaxy NGC 4402 in the Virgo cluster. Image taken by the Hubble Space Telescope

Spiral galaxy NGC 4402 - Spiral galaxy NGC 4402 - NGC 4402 is located about 60 million light years away from Earth in the galaxy cluster of Our Lady. Image obtained by the Hubble Space Telescope. Close - up of the disc of gas and dust of the spiral galaxy NGC 4402 in the Virgo cluster. Image taken by the Hubble Space Telescope

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Spiral Galaxy NGC 4522 - Galaxy Spiral NGC 4522 - Moving at a speed of 10 million km/h in the Virgin's galaxy cluster, this spiral galaxy loses some of its gas. NGC 4522 is located about 60 million light years away from Earth. Image obtained by the Hubble Space Telescope. NGC 4522 is a spectacular example of a spiral galaxy that is currently being stripped of its gas content. The galaxy is part of the Virgo galaxy cluster and its rapid motion within the cluster results in strong winds across the galaxy as the gas within is left behind. Scientists estimate that the galaxy is moving at more than 10 million kilometers per hour. A number of newly formed star clusters that developed in the stripped gas can be seen in the Hubble image. The stripped spiral galaxy is located some 60 million light - years away from Earth

Spiral Galaxy NGC 4522 - Galaxy Spiral NGC 4522 - Moving at a speed of 10 million km/h in the Virgin's galaxy cluster, this spiral galaxy loses some of its gas. NGC 4522 is located about 60 million light years away from Earth. Image obtained by the Hubble Space Telescope. NGC 4522 is a spectacular example of a spiral galaxy that is currently being stripped of its gas content. The galaxy is part of the Virgo galaxy cluster and its rapid motion within the cluster results in strong winds across the galaxy as the gas within is left behind. Scientists estimate that the galaxy is moving at more than 10 million kilometers per hour. A number of newly formed star clusters that developed in the stripped gas can be seen in the Hubble image. The stripped spiral galaxy is located some 60 million light - years away from Earth

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Elliptical galaxy NGC 4696 in Centaur - Elliptical galaxy NGC 4696 - Image of the elliptical galaxy NGC 4696, in Centaur, obtained by the Hubble space telescope. This picture, taken by Hubble's Advanced Camera for Surveys, shows NGC 4696, the largest galaxy in the Centaurus Cluster. The huge dust lane, around 30 000 light - years across, that sweeps across the face of the galaxy makes NGC 4696 look different from most other elliptical galaxies. Viewed at certain wavelengths, strange thin filaments of ionised hydrogen are visible within it. In this picture, these structures are visible as a subtle marbling effect across the galaxy's bright centre

Elliptical galaxy NGC 4696 in Centaur - Elliptical galaxy NGC 4696 - Image of the elliptical galaxy NGC 4696, in Centaur, obtained by the Hubble space telescope. This picture, taken by Hubble's Advanced Camera for Surveys, shows NGC 4696, the largest galaxy in the Centaurus Cluster. The huge dust lane, around 30 000 light - years across, that sweeps across the face of the galaxy makes NGC 4696 look different from most other elliptical galaxies. Viewed at certain wavelengths, strange thin filaments of ionised hydrogen are visible within it. In this picture, these structures are visible as a subtle marbling effect across the galaxy's bright centre

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Lenticular galaxy NGC 4710 in Berenice's Hair - Lenticular galaxy NGC 4710 in Coma Berenices - The galaxy NGC 4710 is located about 60 million years ago - light from Earth, in the galaxy cluster of Our Lady. It's a lenticular galaxy seen from the slice. Image obtained by the Hubble Space Telescope. Edge - on galaxy located at about 60 million light years away. NGC 4710 is a member of the giant Virgo Cluster of galaxies and lies in the northern constellation of Coma Berenices (the Hair of Queen Berenice). It is not one of the brightest members of the cluster, but can easily be seen as a dim elongated smudge on a dark night with a medium - sized amateur telescope. In the 1780s, William Herschel discovered the galaxy and noted it simply as a “” faint nebula””. It is an example of a lenticular or S0 - type galaxy - a type that seems to have some characteristics of both spiral and elliptical galaxies. Image taken by the Hubble Space Telescope

Lenticular galaxy NGC 4710 in Berenice's Hair - Lenticular galaxy NGC 4710 in Coma Berenices - The galaxy NGC 4710 is located about 60 million years ago - light from Earth, in the galaxy cluster of Our Lady. It's a lenticular galaxy seen from the slice. Image obtained by the Hubble Space Telescope. Edge - on galaxy located at about 60 million light years away. NGC 4710 is a member of the giant Virgo Cluster of galaxies and lies in the northern constellation of Coma Berenices (the Hair of Queen Berenice). It is not one of the brightest members of the cluster, but can easily be seen as a dim elongated smudge on a dark night with a medium - sized amateur telescope. In the 1780s, William Herschel discovered the galaxy and noted it simply as a “” faint nebula””. It is an example of a lenticular or S0 - type galaxy - a type that seems to have some characteristics of both spiral and elliptical galaxies. Image taken by the Hubble Space Telescope

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Mars and its satellites - Mars and its moons - Photomontage showing the planet Mars surrounded by its two satellites, Phobos (middle) and Deimos (left)

Mars and its satellites - Mars and its moons - Photomontage showing the planet Mars surrounded by its two satellites, Phobos (middle) and Deimos (left)

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Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346 in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars in which some stars are only 5 million years old. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the Hubble space telescope in July 2004. In the center of this nebula, a cluster of very young stars, some of them are less than 5 million years old

Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346 in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars in which some stars are only 5 million years old. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the Hubble space telescope in July 2004. In the center of this nebula, a cluster of very young stars, some of them are less than 5 million years old

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Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346 in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars in which some stars are only 5 million years old. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the Hubble space telescope in July 2004. In the center of this nebula, a cluster of very young stars, some of them are less than 5 million years old

Nebula NGC 346 in the Small Magellan Cloud - Nebula NGC 346 in the Small Magellanic Cloud - Photo of the nebula NGC 346 in the galaxy of the Small Magellan Cloud obtained by the Hubble space telescope. At the center of this nebula, a cluster of very young stars in which some stars are only 5 million years old. Nebula NGC 346 in the Small Magellanic Cloud, a nearby irregular galaxy, seen by the Hubble space telescope in July 2004. In the center of this nebula, a cluster of very young stars, some of them are less than 5 million years old

R. Gendler

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Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the nebula of the Carene seen in visible light (top) and infrared (bottom) by the Hubble space telescope. The top image shows a column of gas and dust eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of a nascent star. In the infrared image, the dust clouds radiate little, the nascent star responsible for these jets appears. NGC 3372 is located about 7000 light years away from Earth. Images obtained in July 2009. The pictures demonstrate one example of the broad wavelength range of the new Wide Field Camera 3 (WFC3) aboard the Hubble telescope, extending from ultraviolet to visible to infrared light. Composed of gas and dust, the pillar resides in a tempestuous stellar nursery called the Carina Nebula, located 7500 light - years away in the southern constellation of Carina. The pair of images shows that astronomers are given a much more complete vie

Birth of stars in the nebula NGC 3372 - Star formation in the Carina Nebula - Detail of the nebula of the Carene seen in visible light (top) and infrared (bottom) by the Hubble space telescope. The top image shows a column of gas and dust eroded by ultraviolet radiation emitted by young stars. Jets are also visible, showing the presence of a nascent star. In the infrared image, the dust clouds radiate little, the nascent star responsible for these jets appears. NGC 3372 is located about 7000 light years away from Earth. Images obtained in July 2009. The pictures demonstrate one example of the broad wavelength range of the new Wide Field Camera 3 (WFC3) aboard the Hubble telescope, extending from ultraviolet to visible to infrared light. Composed of gas and dust, the pillar resides in a tempestuous stellar nursery called the Carina Nebula, located 7500 light - years away in the southern constellation of Carina. The pair of images shows that astronomers are given a much more complete vie

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Massive Stars in the Carene - Massive stars in the Carina Nebula - The image shows a cluster of stars named Trumpler 16 which contains two very massive stars, WR 25 at Tr16 - 244. WR 25 is the brightest star on the image. It is a double star composed of a star at least 50 times more massive than the Sun. Tr16 - 244 is the third brightest star in this image (top left of WR 25). It's a triple star. The second bright star in the image, to the left of WR 25, is a small star, which does not belong to this cluster and is located much closer to us. The Carene Nebula is located about 7500 years from Earth

Massive Stars in the Carene - Massive stars in the Carina Nebula - The image shows a cluster of stars named Trumpler 16 which contains two very massive stars, WR 25 at Tr16 - 244. WR 25 is the brightest star on the image. It is a double star composed of a star at least 50 times more massive than the Sun. Tr16 - 244 is the third brightest star in this image (top left of WR 25). It's a triple star. The second bright star in the image, to the left of WR 25, is a small star, which does not belong to this cluster and is located much closer to us. The Carene Nebula is located about 7500 years from Earth

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Spiral galaxy NGC 6744 in the constellation Peacock

Spiral galaxy NGC 6744 in the constellation Peacock

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