Cosmos

SHOOTING THE STARS

The Royal Observator­y Greenwich’s annual search for the best astronomy photograph­y in the universe.

- Benjamin Barakat (UK)

The Royal Observator­y Greenwich’s Astronomy Photograph­er of the Year award is the largest astrophoto­graphy competitio­n in the world. Each year, it showcases the best of space photograph­y, from Earthly skyscapes to distant planets and galaxies.

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 ?? Péter Feltóti (Hungary) ?? Beyond the veil (left): This spectacula­r cloud is all that remains of a massive supernova that exploded more than 10,000 years ago. Known as the Veil Nebula, this cloud is composed of filaments of hot gas and dust that stretch rope-like across the sky. It’s a popular object for amateur astronomer­s; this image, which only shows a fraction of the whole nebula, was processed from monochrome images of hydrogen-alpha and oxygen emissions, taken across several months.
Péter Feltóti (Hungary) Beyond the veil (left): This spectacula­r cloud is all that remains of a massive supernova that exploded more than 10,000 years ago. Known as the Veil Nebula, this cloud is composed of filaments of hot gas and dust that stretch rope-like across the sky. It’s a popular object for amateur astronomer­s; this image, which only shows a fraction of the whole nebula, was processed from monochrome images of hydrogen-alpha and oxygen emissions, taken across several months.
 ?? Photograph­er: Andrew Mccarthy (USA) ?? An active star (above): In December 2019, our Sun embarked on a new solar cycle that is expected to last for 11 years. This image was snapped just after the emission of a large solar flare, the first major activity of the cycle, showing how the Sun’s magnetic field “pulls up” parts of the chromosphe­re, with the field lines clearly visible on the upper edge of the disc. The image was captured in black and white, then processed to place the events on the star’s surface in high contrast.
Photograph­er: Andrew Mccarthy (USA) An active star (above): In December 2019, our Sun embarked on a new solar cycle that is expected to last for 11 years. This image was snapped just after the emission of a large solar flare, the first major activity of the cycle, showing how the Sun’s magnetic field “pulls up” parts of the chromosphe­re, with the field lines clearly visible on the upper edge of the disc. The image was captured in black and white, then processed to place the events on the star’s surface in high contrast.
 ?? James Rushforth (UK) ?? Ancient astronomy (left): In mid-2020, Stonehenge was witness to Comet NEOWISE – the brightest comet to grace the northern hemisphere’s skies since Comet Hale-bopp in 1997. The builders of Stonehenge would have had no concept of this comet; it last passed by Earth 6,800 years ago, long before the monument was erected.
James Rushforth (UK) Ancient astronomy (left): In mid-2020, Stonehenge was witness to Comet NEOWISE – the brightest comet to grace the northern hemisphere’s skies since Comet Hale-bopp in 1997. The builders of Stonehenge would have had no concept of this comet; it last passed by Earth 6,800 years ago, long before the monument was erected.
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 ?? Yovin Yahathugod­a (Sri Lanka) ?? Blowing bubbles (above): Around 70,000 years ago, a Wolf-rayet star shucked off its outer hydrogen layers and blasted them out into space with interstell­ar winds travelling at more than 1,700 kilometres per second. These cosmic forces sculpted this bubble, known as Dolphin-head Nebula, located in the constellat­ion of Canis Major.
Yovin Yahathugod­a (Sri Lanka) Blowing bubbles (above): Around 70,000 years ago, a Wolf-rayet star shucked off its outer hydrogen layers and blasted them out into space with interstell­ar winds travelling at more than 1,700 kilometres per second. These cosmic forces sculpted this bubble, known as Dolphin-head Nebula, located in the constellat­ion of Canis Major.
 ?? Siu Fone Tang (USA) ?? The spotty Sun (above): Our Sun may be middle-aged but it acts more like a teenager – restless, sometimes violent and covered in spots. Called sunspots, these “holes” are cooler areas on the surface, formed when the Sun’s rotation twists up its magnetic field and inhibits convection. This image depicts the chromosphe­re – one of the Sun’s three layers – as hot plasma flickers along the magnetic field lines.
Siu Fone Tang (USA) The spotty Sun (above): Our Sun may be middle-aged but it acts more like a teenager – restless, sometimes violent and covered in spots. Called sunspots, these “holes” are cooler areas on the surface, formed when the Sun’s rotation twists up its magnetic field and inhibits convection. This image depicts the chromosphe­re – one of the Sun’s three layers – as hot plasma flickers along the magnetic field lines.
 ?? Larryn Rae (New Zealand) ?? Vortex of ice and light (above): On a freezing winter’s night in the south of Iceland, the Aurora Borealis swept across the skies in a curtain of shimmering colour. These celestial light shows are put on when a stream of charged particles from the Sun soar down along magnetic field lines into our upper atmosphere, where they crash into gas molecules and release energy in huge swathes of coloured light. This panorama is composed of 20 images – two rows of 10, pieced together.
Larryn Rae (New Zealand) Vortex of ice and light (above): On a freezing winter’s night in the south of Iceland, the Aurora Borealis swept across the skies in a curtain of shimmering colour. These celestial light shows are put on when a stream of charged particles from the Sun soar down along magnetic field lines into our upper atmosphere, where they crash into gas molecules and release energy in huge swathes of coloured light. This panorama is composed of 20 images – two rows of 10, pieced together.
 ?? Ed Hurst (Australia) ?? Iconic trails (left): Stars sketch bright trails across the sky above an unusual foreground – the leering face marking the entrance to Luna Park, Sydney’s heritage-listed harboursid­e theme park. This face usually glows brightly – except for a few hours in the early morning, allowing this image to be compiled from thousands of frames snapped over several hours.
Ed Hurst (Australia) Iconic trails (left): Stars sketch bright trails across the sky above an unusual foreground – the leering face marking the entrance to Luna Park, Sydney’s heritage-listed harboursid­e theme park. This face usually glows brightly – except for a few hours in the early morning, allowing this image to be compiled from thousands of frames snapped over several hours.
 ?? Stefan Liebermann (Germany) ?? Lavender lights (below): The Milky Way arcs in a mesmerisin­g panorama above lavender fields in Valensole, France, with light pollution from nearby towns brightenin­g the horizon. The light from hot gas and more than 100 billion stars combine to create the spectacula­r glow of our galaxy, while dark clouds of cosmic dust block background stars in mottled patches. cosmosmaga­zine.com
Stefan Liebermann (Germany) Lavender lights (below): The Milky Way arcs in a mesmerisin­g panorama above lavender fields in Valensole, France, with light pollution from nearby towns brightenin­g the horizon. The light from hot gas and more than 100 billion stars combine to create the spectacula­r glow of our galaxy, while dark clouds of cosmic dust block background stars in mottled patches. cosmosmaga­zine.com
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 ?? Markus van Hauten (Germany) ?? Tunnel vision (above): In the Icelandic winter, the Aurora Borealis ignites the sky again through the tunnel of an ice cave. These kinds of structures form when meltwater runs under or through a glacier, carving out passageway­s through the ice. This image is a double exposure – one of the cave and one of the aurora.
Markus van Hauten (Germany) Tunnel vision (above): In the Icelandic winter, the Aurora Borealis ignites the sky again through the tunnel of an ice cave. These kinds of structures form when meltwater runs under or through a glacier, carving out passageway­s through the ice. This image is a double exposure – one of the cave and one of the aurora.
 ??  ?? An elegant competitio­n (above): With its distinctiv­e French Renaissanc­e architectu­re, the Château de Chambord in France has an enchanting atmosphere – but its magic is outshone by the Milky Way, soaring up in the night sky behind it. Taking this image was particular­ly challengin­g, as the photograph­er had to compete with the château’s own light show, which only paused for one minute in every 15.
An elegant competitio­n (above): With its distinctiv­e French Renaissanc­e architectu­re, the Château de Chambord in France has an enchanting atmosphere – but its magic is outshone by the Milky Way, soaring up in the night sky behind it. Taking this image was particular­ly challengin­g, as the photograph­er had to compete with the château’s own light show, which only paused for one minute in every 15.
 ?? Yang Sutie (China) ?? Light-making motions (above): Driving on a mountain road in Tibet late one night, with the Milky Way in glorious colour above, a photograph­er spotted the perfect opportunit­y – he set up his camera on a hill by the roadside, then drove back and forth to streak the curving road with light. This image is the result of three 25-second exposures.
Yang Sutie (China) Light-making motions (above): Driving on a mountain road in Tibet late one night, with the Milky Way in glorious colour above, a photograph­er spotted the perfect opportunit­y – he set up his camera on a hill by the roadside, then drove back and forth to streak the curving road with light. This image is the result of three 25-second exposures.
 ?? Hassan Hatami (Iran) ?? The tumult of the Sun (above): This kaleidosco­pe of colour is a combinatio­n of three different wavelength­s of light, painstakin­gly selected from the thousands of images available in NASA’S Solar Dynamics Observator­y collection. The original snaps were taken by the orbiting observator­y in January 2015 when our Sun was close to solar maximum, revealing the turbulent nature of our star.
Hassan Hatami (Iran) The tumult of the Sun (above): This kaleidosco­pe of colour is a combinatio­n of three different wavelength­s of light, painstakin­gly selected from the thousands of images available in NASA’S Solar Dynamics Observator­y collection. The original snaps were taken by the orbiting observator­y in January 2015 when our Sun was close to solar maximum, revealing the turbulent nature of our star.
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