The Large Magellanic Cloud
Hubble captures bubbles and baby stars
The NASA/ESA Hubble Space Telescope captures a complex network of gas clouds and star clusters within our neighbouring galaxy, the Large Magellanic Cloud. This region of energetic star birth is one of the most active in the nearby Universe.
 © NASA/ESA/J. M. Apellániz (Instituto de Astrofísica de Andalucía, Spain).
|
This broad vista of young stars and gas clouds in our neighbouring galaxy, the Large Magellanic Cloud, was captured by the NASA/ESA Hubble Space Telescope’s Advanced Camera for Surveys (ACS). This region is named LHA 120-N 11, informally known as N11, and is one of the most active star-forming regions in the nearby Universe. This picture is a mosaic of ACS data from five different positions and covers a region of about 6 arcmin across.
The Large Magellanic Cloud contains many bright bubbles of glowing gas. One of the largest and most spectacular is LHA 120-N 11, from the catalogue compiled in 1956 by the late astronomer and astronaut Karl Henize. It is informally known as N11.
Close up, N11’s billowing pink clouds of glowing gas resemble a puffy swirl of fairground candyfloss. From further away, its distinctive overall shape led some observers to nickname it the Bean Nebula. The dramatic and colourful features in the nebula are the telltale signs of star birth.
N11 is a well-studied region that extends across 1000 light-years. It is the second largest star-forming region within the Large Magellanic Cloud and has produced some of the most massive stars known.
It is the process of star birth that gives N11 its distinctive look. Three successive generations of stars, each of which formed further away from the centre of the nebula than the last, have created shells of gas and dust. These shells were blown away from the newborn stars in the turmoil of their energetic birth and early life, creating the ring shapes so prominent in this image.
Beans are not the only terrestrial shapes to be found in this spectacular high-resolution image from Hubble. At upper left is the red bloom of nebula LHA 120-N 11A. Its roseate petals of gas and dust are illuminated from within, thanks to the radiation from the massive hot stars at its centre. N11A is relatively compact and dense and is the site of the most recent burst of star development in the region.
Other star clusters abound in N11, including NGC 1761 at the bottom of the image – a group of massive hot young stars busily pouring out intense ultraviolet radiation into space.
Although it is much smaller than our own Galaxy, the Large Magellanic Cloud is a vigorous region of star formation. Studying these stellar nurseries helps astronomers to understand a lot more about how stars are born and their ultimate development and lifespan.
Both the Large Magellanic Cloud and its smaller companion, the Small Magellanic Cloud, are easily seen with the unaided eye and have always been familiar to people living in the southern hemisphere. The credit for bringing these galaxies to the attention of Europeans is usually given to Portuguese explorer Fernando de Magellan and his crew, who viewed it on their 1519 sea voyage. However, the Persian astronomer Abd Al-Rahman Al Sufi and the Italian explorer Amerigo Vespucci recorded the Large Magellanic Cloud even earlier, in 964 and 1503, respectively.
Source: ESA - European Space Agency
Close up, N11’s billowing pink clouds of glowing gas resemble a puffy swirl of fairground candyfloss. From further away, its distinctive overall shape led some observers to nickname it the Bean Nebula. The dramatic and colourful features in the nebula are the telltale signs of star birth.
N11 is a well-studied region that extends across 1000 light-years. It is the second largest star-forming region within the Large Magellanic Cloud and has produced some of the most massive stars known.
It is the process of star birth that gives N11 its distinctive look. Three successive generations of stars, each of which formed further away from the centre of the nebula than the last, have created shells of gas and dust. These shells were blown away from the newborn stars in the turmoil of their energetic birth and early life, creating the ring shapes so prominent in this image.
Beans are not the only terrestrial shapes to be found in this spectacular high-resolution image from Hubble. At upper left is the red bloom of nebula LHA 120-N 11A. Its roseate petals of gas and dust are illuminated from within, thanks to the radiation from the massive hot stars at its centre. N11A is relatively compact and dense and is the site of the most recent burst of star development in the region.
Other star clusters abound in N11, including NGC 1761 at the bottom of the image – a group of massive hot young stars busily pouring out intense ultraviolet radiation into space.
Although it is much smaller than our own Galaxy, the Large Magellanic Cloud is a vigorous region of star formation. Studying these stellar nurseries helps astronomers to understand a lot more about how stars are born and their ultimate development and lifespan.
Both the Large Magellanic Cloud and its smaller companion, the Small Magellanic Cloud, are easily seen with the unaided eye and have always been familiar to people living in the southern hemisphere. The credit for bringing these galaxies to the attention of Europeans is usually given to Portuguese explorer Fernando de Magellan and his crew, who viewed it on their 1519 sea voyage. However, the Persian astronomer Abd Al-Rahman Al Sufi and the Italian explorer Amerigo Vespucci recorded the Large Magellanic Cloud even earlier, in 964 and 1503, respectively.
Source: ESA - European Space Agency
The Large Magellanic Cloud
Hubble captures bubbles and baby stars
The NASA/ESA Hubble Space Telescope captures a complex network of gas clouds and star clusters within our neighbouring galaxy, the Large Magellanic Cloud. This region of energetic star birth is one of the most active in the nearby Universe.
© NASA/ESA/J. M. Apellániz (Instituto de Astrofísica de Andalucía, Spain).
|
This broad vista of young stars and gas clouds in our neighbouring galaxy, the Large Magellanic Cloud, was captured by the NASA/ESA Hubble Space Telescope’s Advanced Camera for Surveys (ACS). This region is named LHA 120-N 11, informally known as N11, and is one of the most active star-forming regions in the nearby Universe. This picture is a mosaic of ACS data from five different positions and covers a region of about 6 arcmin across.
The Large Magellanic Cloud contains many bright bubbles of glowing gas. One of the largest and most spectacular is LHA 120-N 11, from the catalogue compiled in 1956 by the late astronomer and astronaut Karl Henize. It is informally known as N11.
Close up, N11’s billowing pink clouds of glowing gas resemble a puffy swirl of fairground candyfloss. From further away, its distinctive overall shape led some observers to nickname it the Bean Nebula. The dramatic and colourful features in the nebula are the telltale signs of star birth.
N11 is a well-studied region that extends across 1000 light-years. It is the second largest star-forming region within the Large Magellanic Cloud and has produced some of the most massive stars known.
It is the process of star birth that gives N11 its distinctive look. Three successive generations of stars, each of which formed further away from the centre of the nebula than the last, have created shells of gas and dust. These shells were blown away from the newborn stars in the turmoil of their energetic birth and early life, creating the ring shapes so prominent in this image.
Beans are not the only terrestrial shapes to be found in this spectacular high-resolution image from Hubble. At upper left is the red bloom of nebula LHA 120-N 11A. Its roseate petals of gas and dust are illuminated from within, thanks to the radiation from the massive hot stars at its centre. N11A is relatively compact and dense and is the site of the most recent burst of star development in the region.
Other star clusters abound in N11, including NGC 1761 at the bottom of the image – a group of massive hot young stars busily pouring out intense ultraviolet radiation into space.
Although it is much smaller than our own Galaxy, the Large Magellanic Cloud is a vigorous region of star formation. Studying these stellar nurseries helps astronomers to understand a lot more about how stars are born and their ultimate development and lifespan.
Both the Large Magellanic Cloud and its smaller companion, the Small Magellanic Cloud, are easily seen with the unaided eye and have always been familiar to people living in the southern hemisphere. The credit for bringing these galaxies to the attention of Europeans is usually given to Portuguese explorer Fernando de Magellan and his crew, who viewed it on their 1519 sea voyage. However, the Persian astronomer Abd Al-Rahman Al Sufi and the Italian explorer Amerigo Vespucci recorded the Large Magellanic Cloud even earlier, in 964 and 1503, respectively.
Source: ESA - European Space Agency
Close up, N11’s billowing pink clouds of glowing gas resemble a puffy swirl of fairground candyfloss. From further away, its distinctive overall shape led some observers to nickname it the Bean Nebula. The dramatic and colourful features in the nebula are the telltale signs of star birth.
N11 is a well-studied region that extends across 1000 light-years. It is the second largest star-forming region within the Large Magellanic Cloud and has produced some of the most massive stars known.
It is the process of star birth that gives N11 its distinctive look. Three successive generations of stars, each of which formed further away from the centre of the nebula than the last, have created shells of gas and dust. These shells were blown away from the newborn stars in the turmoil of their energetic birth and early life, creating the ring shapes so prominent in this image.
Beans are not the only terrestrial shapes to be found in this spectacular high-resolution image from Hubble. At upper left is the red bloom of nebula LHA 120-N 11A. Its roseate petals of gas and dust are illuminated from within, thanks to the radiation from the massive hot stars at its centre. N11A is relatively compact and dense and is the site of the most recent burst of star development in the region.
Other star clusters abound in N11, including NGC 1761 at the bottom of the image – a group of massive hot young stars busily pouring out intense ultraviolet radiation into space.
Although it is much smaller than our own Galaxy, the Large Magellanic Cloud is a vigorous region of star formation. Studying these stellar nurseries helps astronomers to understand a lot more about how stars are born and their ultimate development and lifespan.
Both the Large Magellanic Cloud and its smaller companion, the Small Magellanic Cloud, are easily seen with the unaided eye and have always been familiar to people living in the southern hemisphere. The credit for bringing these galaxies to the attention of Europeans is usually given to Portuguese explorer Fernando de Magellan and his crew, who viewed it on their 1519 sea voyage. However, the Persian astronomer Abd Al-Rahman Al Sufi and the Italian explorer Amerigo Vespucci recorded the Large Magellanic Cloud even earlier, in 964 and 1503, respectively.
Source: ESA - European Space Agency
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The Large Magellanic Cloud
Hubble captures bubbles and baby stars
The NASA/ESA Hubble Space Telescope captures a complex network of gas clouds and star clusters within our neighbouring galaxy, the Large Magellanic Cloud. This region of energetic star birth is one of the most active in the nearby Universe.
© NASA/ESA/J. M. Apellániz (Instituto de Astrofísica de Andalucía, Spain).
|
This broad vista of young stars and gas clouds in our neighbouring galaxy, the Large Magellanic Cloud, was captured by the NASA/ESA Hubble Space Telescope’s Advanced Camera for Surveys (ACS). This region is named LHA 120-N 11, informally known as N11, and is one of the most active star-forming regions in the nearby Universe. This picture is a mosaic of ACS data from five different positions and covers a region of about 6 arcmin across.
The Large Magellanic Cloud contains many bright bubbles of glowing gas. One of the largest and most spectacular is LHA 120-N 11, from the catalogue compiled in 1956 by the late astronomer and astronaut Karl Henize. It is informally known as N11.
Close up, N11’s billowing pink clouds of glowing gas resemble a puffy swirl of fairground candyfloss. From further away, its distinctive overall shape led some observers to nickname it the Bean Nebula. The dramatic and colourful features in the nebula are the telltale signs of star birth.
N11 is a well-studied region that extends across 1000 light-years. It is the second largest star-forming region within the Large Magellanic Cloud and has produced some of the most massive stars known.
It is the process of star birth that gives N11 its distinctive look. Three successive generations of stars, each of which formed further away from the centre of the nebula than the last, have created shells of gas and dust. These shells were blown away from the newborn stars in the turmoil of their energetic birth and early life, creating the ring shapes so prominent in this image.
Beans are not the only terrestrial shapes to be found in this spectacular high-resolution image from Hubble. At upper left is the red bloom of nebula LHA 120-N 11A. Its roseate petals of gas and dust are illuminated from within, thanks to the radiation from the massive hot stars at its centre. N11A is relatively compact and dense and is the site of the most recent burst of star development in the region.
Other star clusters abound in N11, including NGC 1761 at the bottom of the image – a group of massive hot young stars busily pouring out intense ultraviolet radiation into space.
Although it is much smaller than our own Galaxy, the Large Magellanic Cloud is a vigorous region of star formation. Studying these stellar nurseries helps astronomers to understand a lot more about how stars are born and their ultimate development and lifespan.
Both the Large Magellanic Cloud and its smaller companion, the Small Magellanic Cloud, are easily seen with the unaided eye and have always been familiar to people living in the southern hemisphere. The credit for bringing these galaxies to the attention of Europeans is usually given to Portuguese explorer Fernando de Magellan and his crew, who viewed it on their 1519 sea voyage. However, the Persian astronomer Abd Al-Rahman Al Sufi and the Italian explorer Amerigo Vespucci recorded the Large Magellanic Cloud even earlier, in 964 and 1503, respectively.
Source: ESA - European Space Agency
Close up, N11’s billowing pink clouds of glowing gas resemble a puffy swirl of fairground candyfloss. From further away, its distinctive overall shape led some observers to nickname it the Bean Nebula. The dramatic and colourful features in the nebula are the telltale signs of star birth.
N11 is a well-studied region that extends across 1000 light-years. It is the second largest star-forming region within the Large Magellanic Cloud and has produced some of the most massive stars known.
It is the process of star birth that gives N11 its distinctive look. Three successive generations of stars, each of which formed further away from the centre of the nebula than the last, have created shells of gas and dust. These shells were blown away from the newborn stars in the turmoil of their energetic birth and early life, creating the ring shapes so prominent in this image.
Beans are not the only terrestrial shapes to be found in this spectacular high-resolution image from Hubble. At upper left is the red bloom of nebula LHA 120-N 11A. Its roseate petals of gas and dust are illuminated from within, thanks to the radiation from the massive hot stars at its centre. N11A is relatively compact and dense and is the site of the most recent burst of star development in the region.
Other star clusters abound in N11, including NGC 1761 at the bottom of the image – a group of massive hot young stars busily pouring out intense ultraviolet radiation into space.
Although it is much smaller than our own Galaxy, the Large Magellanic Cloud is a vigorous region of star formation. Studying these stellar nurseries helps astronomers to understand a lot more about how stars are born and their ultimate development and lifespan.
Both the Large Magellanic Cloud and its smaller companion, the Small Magellanic Cloud, are easily seen with the unaided eye and have always been familiar to people living in the southern hemisphere. The credit for bringing these galaxies to the attention of Europeans is usually given to Portuguese explorer Fernando de Magellan and his crew, who viewed it on their 1519 sea voyage. However, the Persian astronomer Abd Al-Rahman Al Sufi and the Italian explorer Amerigo Vespucci recorded the Large Magellanic Cloud even earlier, in 964 and 1503, respectively.
Source: ESA - European Space Agency