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Images of 'Mro' found, 93

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A young boy from the ethnic Mro community, in Thanchi, Bandarban, Bangladesh. October 8, 2008. (photo)

A young boy from the ethnic Mro community, in Thanchi, Bandarban, Bangladesh. October 8, 2008. (photo)

UIG799710

Martian dunes at the end of winter - March: Late Winter view of Dunes: Detail on dunes in the southern hemisphere of Mars. With the end of winter, the Sun melts the carbon dioxide ice present all winter. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on March 21, 2016. HIRISE is a 50 cm telescope that observes visible and near infrared. Sand dunes cover much of this terrain, which has large boulders lying on flat areas between the dunes. It is now late winter here in the Southern hemisphere, and these dunes are just getting enough sunlight to start defrosting their seasonal cover of carbon dioxide. Spots form where pressurized carbon dioxide gas escapes to the surface

Martian dunes at the end of winter - March: Late Winter view of Dunes: Detail on dunes in the southern hemisphere of Mars. With the end of winter, the Sun melts the carbon dioxide ice present all winter. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on March 21, 2016. HIRISE is a 50 cm telescope that observes visible and near infrared. Sand dunes cover much of this terrain, which has large boulders lying on flat areas between the dunes. It is now late winter here in the Southern hemisphere, and these dunes are just getting enough sunlight to start defrosting their seasonal cover of carbon dioxide. Spots form where pressurized carbon dioxide gas escapes to the surface

PIX4580064

Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

PIX4580071

The Jhum ghar is a temporary housing for living, treating and storing crops. The village of Tindu, in Thanchi, Bandar Ban, Bangladesh. October 9, 2008. (photo)

The Jhum ghar is a temporary housing for living, treating and storing crops. The village of Tindu, in Thanchi, Bandar Ban, Bangladesh. October 9, 2008. (photo)

UIG798757

Avalanches sur Mars - Mars: avalanches on North Polar Scarps - Detail on a cliff in the region of the north pole of Mars. Part of the surface, consisting of dust and carbon dioxide frost, has become detached creating dust avalanches

Avalanches sur Mars - Mars: avalanches on North Polar Scarps - Detail on a cliff in the region of the north pole of Mars. Part of the surface, consisting of dust and carbon dioxide frost, has become detached creating dust avalanches

PIX4616545

This color-enhanced view of NASA's Curiosity rover on the surface of Mars was taken by the HiRISE on NASA's Mars Reconnaissance Orbiter as the satellite flew overhead.

This color-enhanced view of NASA's Curiosity rover on the surface of Mars was taken by the HiRISE on NASA's Mars Reconnaissance Orbiter as the satellite flew overhead.

UIG866639

Martian dune erosion - Mars: Disappearing and Shrinking Dome Dunes - Dune sur Mars photographed by the HIRISE camera of the Mars Reconnaissance probe orbiting on January 30, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. This false - color image from the HIRISE (High Resolution Imaging Science Experiment) camera on Mars Recognition Orbiter was taken on January 30, 2008

Martian dune erosion - Mars: Disappearing and Shrinking Dome Dunes - Dune sur Mars photographed by the HIRISE camera of the Mars Reconnaissance probe orbiting on January 30, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. This false - color image from the HIRISE (High Resolution Imaging Science Experiment) camera on Mars Recognition Orbiter was taken on January 30, 2008

PIX4616448

The coldest place on Mars - Coolest place on Mars: Detail of the ice cap of the southern pole of Mars, composed mainly of carbon dioxide. This dry ice accumulates on the surface mainly in winter, the temperature of this area can sometimes drop to 130 degrees Celsius below zero. Image obtained on August 29, 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this coolest landscape on Earth and Mars

The coldest place on Mars - Coolest place on Mars: Detail of the ice cap of the southern pole of Mars, composed mainly of carbon dioxide. This dry ice accumulates on the surface mainly in winter, the temperature of this area can sometimes drop to 130 degrees Celsius below zero. Image obtained on August 29, 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this coolest landscape on Earth and Mars

PIX4580080

Mars: Sedimentary layers in Becquerel crater - Mars: Periodic Layering in Becquerel Crater - Detail on sedimentary layers in Becquerel crater (Arabia Terra region), obtained on June 10, 2007 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This image in false colors shows sedimentary rocks in pink, sand in blue. The study of these sedimentary depot strata suggests that the climate of Mars is linked to the inclination of the axis of rotation of the planet. Rhythmic bedding in sedimentary bedrock within Becquerel crater on Mars is suggested by the patterns in this image from the High Resolution Imaging Science Experiment (HiRise) camera on Nasa's Mars Reconnaissance Orbiter. Three dimensional analysis based on stereo pairs of images confirmed the regularity of repetition in the thickness of the beds. In the top half of this image, some of the rhythm is apparent as a series of bundles of about 10 individual layers per bundle. By corresponding to a known 10 - to - one p

Mars: Sedimentary layers in Becquerel crater - Mars: Periodic Layering in Becquerel Crater - Detail on sedimentary layers in Becquerel crater (Arabia Terra region), obtained on June 10, 2007 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. This image in false colors shows sedimentary rocks in pink, sand in blue. The study of these sedimentary depot strata suggests that the climate of Mars is linked to the inclination of the axis of rotation of the planet. Rhythmic bedding in sedimentary bedrock within Becquerel crater on Mars is suggested by the patterns in this image from the High Resolution Imaging Science Experiment (HiRise) camera on Nasa's Mars Reconnaissance Orbiter. Three dimensional analysis based on stereo pairs of images confirmed the regularity of repetition in the thickness of the beds. In the top half of this image, some of the rhythm is apparent as a series of bundles of about 10 individual layers per bundle. By corresponding to a known 10 - to - one p

PIX4616532

Mars Recognition Orbiter and the Comet, Artist view (photo)

Mars Recognition Orbiter and the Comet, Artist view (photo)

Steven Hobbs

PIX6039537

Traces of flow on Mars - Mars: gullies on impact crater wall - Gullies along a wall of an impact crater (Hale crater). These ravines are thought to indicate the presence of liquid water in the Martian basement. Image obtained by the Mars Reconnaissance Orbiter probe on August 3, 2009. Gullies, on Earth, are usually formed through the action of liquid water. Whether gullies form under today's cold dry conditions on Mars is a major question that planetary scientists are trying to answer. The gullies pictured here in Hale crater are great examples of what a typical Martian gully looks like. Wide V - shaped channels running downhill (from top to bottom) where the material that carved the gully flowed. At the bottom of the channel this material empties out onto a fan - shaped mound. Several gullies are visible here and the fans from each gully overlap one other in complicated ways. Image taken on August 3, 2009 by the HIRISE camera on Nasa's Mars Reconnaissance Orbiter

Traces of flow on Mars - Mars: gullies on impact crater wall - Gullies along a wall of an impact crater (Hale crater). These ravines are thought to indicate the presence of liquid water in the Martian basement. Image obtained by the Mars Reconnaissance Orbiter probe on August 3, 2009. Gullies, on Earth, are usually formed through the action of liquid water. Whether gullies form under today's cold dry conditions on Mars is a major question that planetary scientists are trying to answer. The gullies pictured here in Hale crater are great examples of what a typical Martian gully looks like. Wide V - shaped channels running downhill (from top to bottom) where the material that carved the gully flowed. At the bottom of the channel this material empties out onto a fan - shaped mound. Several gullies are visible here and the fans from each gully overlap one other in complicated ways. Image taken on August 3, 2009 by the HIRISE camera on Nasa's Mars Reconnaissance Orbiter

PIX4616548

Dunes near the north pole on Mars - Dunes at North Polar Cap on Mars: Image obtained on March 26, 2014 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. Formative down-slope winds descending on Mars' North Polar ice cap likely play an important role in transporting sediment from the base of the ice cap into the dune fields that sit beyond the ice cap. The deep chasm that formed on the polar cap edge is identified as an area of strong down-slope winds and has a clear connection to Mars' largest dune field, Olympia Undae. Repeat HiRise images from this chasm that specifically targets the dunes, provides the basis to evaluate the sand fluxes which are associated with the dune and ripple movement in this area

Dunes near the north pole on Mars - Dunes at North Polar Cap on Mars: Image obtained on March 26, 2014 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. Formative down-slope winds descending on Mars' North Polar ice cap likely play an important role in transporting sediment from the base of the ice cap into the dune fields that sit beyond the ice cap. The deep chasm that formed on the polar cap edge is identified as an area of strong down-slope winds and has a clear connection to Mars' largest dune field, Olympia Undae. Repeat HiRise images from this chasm that specifically targets the dunes, provides the basis to evaluate the sand fluxes which are associated with the dune and ripple movement in this area

PIX4580075

Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The co

Glaciers under Martian crateres - Buried glaciers on Mars - Computer reconstructed views of three Martian crateres in the Hellas region that house glaciers. The images show the crateres as they appear today with a layer of Martian soil covering the ice with water and, on the right, the glaciers updated according to radar measurements obtained by the Mars Reconnaissance Orbiter probe (MRO). These glaciers would have a thickness of 250 to 450 meters. Each image covers 20 km wide. This computer graphic image shows three craters in the eastern Hellas region of Mars containing concealed glaciers detected by radar. The images shows how the surface looks today with the ice covered with a layer of Martian soil and what the ice may look like underneath. The image was created using image data from the Context Camera on the Mars Reconnaissance Orbiter (MRO) spacecraft combined with results from the SHARAD radar sounder on MRO and HRSC digital elevation map from the Mars Express spacecraft. The co

PIX4616544

The Claritas Fossae region is characterised by systems of "graben" running mainly north-west to south-east. A graben forms when a block of the planet's crust drops down between two faults, due to extension, or pulling, of the crust. MRO.

The Claritas Fossae region is characterised by systems of "graben" running mainly north-west to south-east. A graben forms when a block of the planet's crust drops down between two faults, due to extension, or pulling, of the crust. MRO.

UIG866579

This image from NASA's Mars Reconnaissance Rover (MRO) shows a degraded impact crater in the southern highlands.

This image from NASA's Mars Reconnaissance Rover (MRO) shows a degraded impact crater in the southern highlands.

UIG866547

These dark sand dunes in the North polar region, basking in the sunshine of late spring, have shed most of their seasonal layer of winter ice. MRO.

These dark sand dunes in the North polar region, basking in the sunshine of late spring, have shed most of their seasonal layer of winter ice. MRO.

UIG866576

This image covers a region of Mars near Nili Fossae that contains some of the best exposures of ancient bedrock on Mars. MRO.

This image covers a region of Mars near Nili Fossae that contains some of the best exposures of ancient bedrock on Mars. MRO.

UIG866577

Martian dunes in winter - March: Winter view of Dunes - Detail on dunes in a crater located in the southern hemisphere of Mars. Clearly, areas covered with gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on November 25, 2006. HIRISE is a 50 cm telescope that observes visible and near infrared. Dunes within a crater on Mars are visible in this HiRise image. This crater is located in the southern hemisphere where it was winter at the time this image was taken on November 25, 2006. This observation documents new seasonal processes occurring on dunes at this latitude, as well as other interesting phenomena. The bright tones are interpreted as carbon dioxide or water frost. This is generally concentrated on the east - facing slopes of the dunes, which are in shadow and therefore cooler. Some dark spots on the dunes may be areas that have defrosted more than surrounding terrain. Landslides and dark - toned streaks are seen on many of the west -

Martian dunes in winter - March: Winter view of Dunes - Detail on dunes in a crater located in the southern hemisphere of Mars. Clearly, areas covered with gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on November 25, 2006. HIRISE is a 50 cm telescope that observes visible and near infrared. Dunes within a crater on Mars are visible in this HiRise image. This crater is located in the southern hemisphere where it was winter at the time this image was taken on November 25, 2006. This observation documents new seasonal processes occurring on dunes at this latitude, as well as other interesting phenomena. The bright tones are interpreted as carbon dioxide or water frost. This is generally concentrated on the east - facing slopes of the dunes, which are in shadow and therefore cooler. Some dark spots on the dunes may be areas that have defrosted more than surrounding terrain. Landslides and dark - toned streaks are seen on many of the west -

PIX4616480

Martian dunes in Spring - March: Frost - covered dunes in crater - Detail on dunes in a crater located near the north pole of Mars. Clearly, areas covered with carbon dioxide gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on January 1, 2010. HIRISE is a 50 cm telescope that observes visible and near infrared Dunes are often found on crater floors. In the winter time at high northern latitudes the terrain is covered by carbon dioxide ice (dry ice). In the spring as this seasonal ice evaporates many unusual features unique to Mars are visible. On the floor of this crater where there are no dunes, the ice forms an uninterrupted layer. On the dunes however, dark streaks form as surface material from below the ice is mobilized and deposited on top of the ice. In some cases this mobile material probably slides down the steep face of the dune, while in other cases it may be literally blown out in a process of gas release similar to removing a c

Martian dunes in Spring - March: Frost - covered dunes in crater - Detail on dunes in a crater located near the north pole of Mars. Clearly, areas covered with carbon dioxide gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on January 1, 2010. HIRISE is a 50 cm telescope that observes visible and near infrared Dunes are often found on crater floors. In the winter time at high northern latitudes the terrain is covered by carbon dioxide ice (dry ice). In the spring as this seasonal ice evaporates many unusual features unique to Mars are visible. On the floor of this crater where there are no dunes, the ice forms an uninterrupted layer. On the dunes however, dark streaks form as surface material from below the ice is mobilized and deposited on top of the ice. In some cases this mobile material probably slides down the steep face of the dune, while in other cases it may be literally blown out in a process of gas release similar to removing a c

PIX4616489

This observation shows a fresh, approximately 7.5 kilometer diameter crater that resides in a larger crater in the Southern hemisphere. MRO.

This observation shows a fresh, approximately 7.5 kilometer diameter crater that resides in a larger crater in the Southern hemisphere. MRO.

UIG866559

The formation of the large outflow channels on Mars have been attributed to catastrophic discharges of ground water. This is known as chaotic terrain. MRO.

The formation of the large outflow channels on Mars have been attributed to catastrophic discharges of ground water. This is known as chaotic terrain. MRO.

UIG866558

Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

PIX4616482

Tracks from the first drives of NASA's Curiosity rover are visible in this image captured by the HiRISE camera on NASA's Mars Reconnaissance Orbiter.

Tracks from the first drives of NASA's Curiosity rover are visible in this image captured by the HiRISE camera on NASA's Mars Reconnaissance Orbiter.

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An ethnic woman grazing her goat, at Bandarban, Bangladesh. June 26, 2005. They do not get sufficient agricultural commodities easily, therefore impact of poverty is apparent in their lives. (photo)

An ethnic woman grazing her goat, at Bandarban, Bangladesh. June 26, 2005. They do not get sufficient agricultural commodities easily, therefore impact of poverty is apparent in their lives. (photo)

UIG799727

The Nili Fossae region of Mars is one of the largest exposures of clay minerals discovered by the OMEGA spectrometer on Mars Express and mapped in greater detail by the CRISM spectrometer on MRO.

The Nili Fossae region of Mars is one of the largest exposures of clay minerals discovered by the OMEGA spectrometer on Mars Express and mapped in greater detail by the CRISM spectrometer on MRO.

UIG866563

These before-and-after images show the effects of weights from the entry vehicle of NASA's Curiosity rover hitting the surface of Mars. MRO.

These before-and-after images show the effects of weights from the entry vehicle of NASA's Curiosity rover hitting the surface of Mars. MRO.

UIG866627

Known since at least 2003, this is a wonderful case of aeolian sandstone that preserves its original sand dune bedform shapes and lies unconformably over a previously-eroded surface of layered sedimentary rock. MRO.

Known since at least 2003, this is a wonderful case of aeolian sandstone that preserves its original sand dune bedform shapes and lies unconformably over a previously-eroded surface of layered sedimentary rock. MRO.

UIG866575

Some of the weirdest and least-understood landscapes on Mars are on the floor of the deep Hellas impact basin. MRO.

Some of the weirdest and least-understood landscapes on Mars are on the floor of the deep Hellas impact basin. MRO.

UIG866574

Women from an ethnic community bathing in the fountain, at Chimbuk, in Bandarban, Bangladesh. June 25, 2005. They do not get sufficient facilities in almost all aspects of life, therefore impact of poverty is apparent in their lives. (photo)

Women from an ethnic community bathing in the fountain, at Chimbuk, in Bandarban, Bangladesh. June 25, 2005. They do not get sufficient facilities in almost all aspects of life, therefore impact of poverty is apparent in their lives. (photo)

UIG799726

Most of the ethnic people of Bangladesh live in hill tract districts like Bandarban, Rangamati, Khagrachori. Mro people and their life style are quite remarkable. They are very hard working and have their own lifestyle, culture and social distinction. They make their own clothing, cultivate crops, collect water from river or fountain. Bandarban, Bangladesh. 2007. (photo)

Most of the ethnic people of Bangladesh live in hill tract districts like Bandarban, Rangamati, Khagrachori. Mro people and their life style are quite remarkable. They are very hard working and have their own lifestyle, culture and social distinction. They make their own clothing, cultivate crops, collect water from river or fountain. Bandarban, Bangladesh. 2007. (photo)

UIG797306

Rhythmic patterns of sedimentary layering in Danielson Crater on Mars result from periodic changes in climate related to changes in tilt of the planet. MRO.

Rhythmic patterns of sedimentary layering in Danielson Crater on Mars result from periodic changes in climate related to changes in tilt of the planet. MRO.

UIG866594

Most of the ethnic people of Bangladesh live in hill tract districts like Bandarban, Rangamati, Khagrachori. Mro people and their life style are quite remarkable. They are very hard working and have their own lifestyle, culture and social distinction. They make their own clothing, cultivate crops, collect water from river or fountain. Bandarban, Bangladesh. 2007. (photo)

Most of the ethnic people of Bangladesh live in hill tract districts like Bandarban, Rangamati, Khagrachori. Mro people and their life style are quite remarkable. They are very hard working and have their own lifestyle, culture and social distinction. They make their own clothing, cultivate crops, collect water from river or fountain. Bandarban, Bangladesh. 2007. (photo)

UIG797302

Most of the ethnic people of Bangladesh live in hill tract districts like Bandarban, Rangamati, Khagrachori. Mro people and their life style are quite remarkable. They are very hard working and have their own lifestyle, culture and social distinction. They make their own clothing, cultivate crops, collect water from river or fountain. Bandarban, Bangladesh. 2007. (photo)

Most of the ethnic people of Bangladesh live in hill tract districts like Bandarban, Rangamati, Khagrachori. Mro people and their life style are quite remarkable. They are very hard working and have their own lifestyle, culture and social distinction. They make their own clothing, cultivate crops, collect water from river or fountain. Bandarban, Bangladesh. 2007. (photo)

UIG797305

This color view of the parachute and back shell that helped deliver NASA's Curiosity rover to the surface of the Red Planet was taken by the HiRISE camera on NASA's Mars Reconnaissance Orbiter.

This color view of the parachute and back shell that helped deliver NASA's Curiosity rover to the surface of the Red Planet was taken by the HiRISE camera on NASA's Mars Reconnaissance Orbiter.

UIG866666

This image hows the funnel-shaped terminus of Lethe Vallis, a winding channel in the Elysium Planitia region of Mars. MRO.

This image hows the funnel-shaped terminus of Lethe Vallis, a winding channel in the Elysium Planitia region of Mars. MRO.

UIG866560

This scene is from early spring in the northern hemisphere of Mars. These dunes are covered with a layer of seasonal carbon dioxide ice (dry ice). MRO.

This scene is from early spring in the northern hemisphere of Mars. These dunes are covered with a layer of seasonal carbon dioxide ice (dry ice). MRO.

UIG866586

Most of the ethnic people of Bangladesh live in hill tract districts like Bandarban, Rangamati, Khagrachori. Mro people and their life style are quite remarkable. They are very hard working and have their own lifestyle, culture and social distinction. They make their own clothing, cultivate crops, collect water from river or fountain. Bandarban, Bangladesh. 2007. (photo)

Most of the ethnic people of Bangladesh live in hill tract districts like Bandarban, Rangamati, Khagrachori. Mro people and their life style are quite remarkable. They are very hard working and have their own lifestyle, culture and social distinction. They make their own clothing, cultivate crops, collect water from river or fountain. Bandarban, Bangladesh. 2007. (photo)

UIG797301

An elderly man from the ethnic Mro community warms himself beside a bonfire, in a cold winter morning, in Bandarban, Bangladesh. January 4, 2007. (photo)

An elderly man from the ethnic Mro community warms himself beside a bonfire, in a cold winter morning, in Bandarban, Bangladesh. January 4, 2007. (photo)

UIG799950

Mars Reconnaissance Orbiter - Artist View - Mars Reconnaissance Orbiter - Artist view - The American Mars Reconnaissance Orbiter probe (MRO) was launched in August 2005 and began its observations from Mars in October 2006. Artwork of Mars Reconnaissance Orbiter (MRO) as it orbits over the martian north pole. The spacecraft was launched in August 2005 and began the first observations of March in October 2006

Mars Reconnaissance Orbiter - Artist View - Mars Reconnaissance Orbiter - Artist view - The American Mars Reconnaissance Orbiter probe (MRO) was launched in August 2005 and began its observations from Mars in October 2006. Artwork of Mars Reconnaissance Orbiter (MRO) as it orbits over the martian north pole. The spacecraft was launched in August 2005 and began the first observations of March in October 2006

Steven Hobbs

PIX4606683

Murong Woman in Lama, Bandarban, Bangladesh. July 29, 2010 (photo)

Murong Woman in Lama, Bandarban, Bangladesh. July 29, 2010 (photo)

UIG2619304

Cane baskets (photo)

Cane baskets (photo)

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A woman from the ethnic Murong (also Mro or Mru) community, in Lama, Bandarban, Bangladesh. July 29, 2010 (photo)

A woman from the ethnic Murong (also Mro or Mru) community, in Lama, Bandarban, Bangladesh. July 29, 2010 (photo)

UIG2619302

Daily life (photo)

Daily life (photo)

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Two women from the ethnic Murong (also Mro or Mru) community (photo)

Two women from the ethnic Murong (also Mro or Mru) community (photo)

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Three women from the ethnic Murong (also Mro or Mru) community (photo)

Three women from the ethnic Murong (also Mro or Mru) community (photo)

UIG2619673

Three Mro women returns home from the Lama bazaar. Lama (photo)

Three Mro women returns home from the Lama bazaar. Lama (photo)

UIG2619678

Children from the ethnic Murong (also Mro or Mru) community (photo)

Children from the ethnic Murong (also Mro or Mru) community (photo)

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A little girl from the ethnic Murong (also Mro or Mru) community (photo)

A little girl from the ethnic Murong (also Mro or Mru) community (photo)

UIG2620177

A mother and child at the window of their hut (photo)

A mother and child at the window of their hut (photo)

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Children (photo)

Children (photo)

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Woman crossing a mountain stream (photo)

Woman crossing a mountain stream (photo)

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Woman (photo)

UIG2619303

Women at a bazaar (photo)

Women at a bazaar (photo)

UIG2619305

Two women (photo)

Two women (photo)

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Elderly man (photo)

Elderly man (photo)

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The Lama bazaar (photo)

The Lama bazaar (photo)

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Children (photo)

Children (photo)

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A scene from Lama bazaar (photo)

A scene from Lama bazaar (photo)

UIG2619675

Elderly woman (photo)

Elderly woman (photo)

UIG2619292

Children (photo)

Children (photo)

UIG2619293

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