The Nautical Twilight with the Moon in ALMA
After the sunset starts the nautical twilight and the sky assumes a beautiful pallet of blueish and orange colors, giving space to appearing the first stars of the some constellations. In the foreground, is also visible one antenna (DV-21) of 12 meters in diameter, pointing to some place of the cold Universe, and its right side the Moon. This are the first tests to experiment the largest configuration that ALMA can support, with antennas spread over distances up to 16 km. The array thus simulates a giant, single telescope much larger than any that could actually be built. In fact, ALMA has a maximum resolution which is even better than that achieved, at visible wavelengths, by the Hubble Space Telescope.
The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of radio telescopes in the Atacama desert of northern Chile. Since a high and dry site is crucial to millimeter wavelength operations, the array has been constructed on the Chajnantor plateau at 5,000 meters altitude, near Llano de Chajnantor Observatory and Atacama Pathfinder Experiment. Consisting of 66 12-meter (39 ft), and 7-meter (23 ft) diameter radio telescopes observing at millimeter and submillimeter wavelengths, ALMA is expected to provide insight on star birth during the early universe and detailed imaging of local star and planet formation. ALMA is a single telescope of revolutionary design, composed initially of 66 high-precision antennas, and operating at wavelengths of 0.32 to 3.6 mm. Its main 12-metre array has fifty antennas, 12 metres in diameter, acting together as a single telescope — an interferometer. An additional compact array of four 12-metre and twelve 7-metre antennas complements this. The 66 ALMA antennas can be arranged in different configurations, where the maximum distance between antennas can vary from 150 metres to 16 kilometres, which will give ALMA a powerful variable “zoom”. It will be able to probe the Universe at millimetre and submillimetre wavelengths with unprecedented sensitivity and resolution, with a vision up to ten times sharper than the Hubble Space Telescope, and complementing images made with the VLT Interferometer. Light at these wavelengths comes from vast cold clouds in interstellar space, at temperatures only a few tens of degrees above absolute zero, and from some of the earliest and most distant galaxies in the Universe. Astronomers can use it to study the chemical and physical conditions in molecular clouds — the dense regions of gas and dust where new stars are being born. Often these regions of the Universe are dark and obscured in visible light, but they shine brightly in the millimetre and submillimetre part of the spectrum. ALMA is the most powerful telescope for observing the cool Universe — molecular gas and dust.
ALMA will study the building blocks of stars, planetary systems, galaxies and life itself. By providing scientists with detailed images of stars and planets being born in gas clouds near our Solar System, and detecting distant galaxies forming at the edge of the observable Universe, which we see as they were roughly ten billion years ago, it lets astronomers address some of the deepest questions of our cosmic origins.
Image taken taken in 14/10/2015 from Chajnantor plateau, Atacama desert, Chile.
A Romantic Scene in a Lovely Sky
In this colorful lovely scene captured at the twilight, we can see two skywatchers enjoying his passion about the Universe, with a Crescent Moon shining between the clouds and above the Auxiliary Telescopes (ATs) of VLT.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Cerro Paranal Shadow projected in Cerro Armazones
Above the horizon we can see Cerro Armazones mountain illuminated by the sunset reddish color that is reflected in the land and high clouds, also with the projected shadow of Cerro Paranal. With an altitude of 3060 meterss in the central part of Chiles Atacama Desert, some 130 kilometers south of the town of Antofagasta and about 20 kilometers from Cerro Paranal, home of ESOs Very Large Telescope. Cerro Armazones will be the baseline site for the planned 39-metre-class European Extremely Large Telescope (E-ELT), with a planned construction period of about a decade. The telescope’s “eye” will be almost half the length of a soccer pitch in diameter and will gather 15 times more light than the largest optical telescopes operating today. The telescope has an innovative five-mirror design that includes advanced adaptive optics to correct for the turbulent atmosphere, giving exceptional image quality. The main mirror will be made up from almost 800 hexagonal segments.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Moon Corona in the Twilight of Very Large Telescope
After sunset a partial cloudy sky can promote the appearance of a beautiful show of colors, as well as some optical phenomenon, specially if we have a night of Moonlight that can show an effect called “Corona”, produced by the diffraction of light coming from the Moon by individual small water droplets and sometimes tiny ice crystals of a cloud. In the foreground, we can see three of four movable Auxiliary Telescopes available in the Very Large Telescope platform.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Ghostly Shapes on the Starry Sky of VLT
After sunset a partial cloudy sky can promote the appearance of a beautiful show of colors, specially if we have a night of Moonlight that can illuminate and show a strange game of ghostly shapes in the clouds, combined with a starry sky as a background. In the foreground, we can see three of four movable Auxiliary Telescopes available in the Very Large Telescope platform.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Cerro Armazones, the home for the European Extremely Large Telescope (E-ELT)
Above the horizon we can see Cerro Armazones mountain iluminated by the sunset redish color that is reflected in the land and high clouds . With an altitude of 3060 metres in the central part of Chiles Atacama Desert, some 130 kilometres south of the town of Antofagasta and about 20 kilometres from Cerro Paranal, home of ESOs Very Large Telescope. Cerro Armazone will be the baseline site for the planned 39-metre-class European Extremely Large Telescope (E-ELT), with a planned construction period of about a decade. The telescope’s “eye” will be almost half the length of a soccer pitch in diameter and will gather 15 times more light than the largest optical telescopes operating today. The telescope has an innovative five-mirror design that includes advanced adaptive optics to correct for the turbulent atmosphere, giving exceptional image quality. The main mirror will be made up from almost 800 hexagonal segments.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Belt of Venus above the DIMM tower in Cerro Paranal
In the foreground, we can see the white Meteorological Tower of Paranal. The small dome contains a telescope dedicated to monitoring the atmospheric seeing conditions, known as a Differential Image Motion Monitor (DIMM.) In the background is strongly visible the Earth’s shadow, the shadow that the Earth itself casts on its atmosphere. This shadow is visible in the opposite half of the sky to the sunset or sunrise, and is seen right above the horizon as a dark blue band. Immediately above, a pink band that is visible above the dark blue of the Earth’s shadow is called “Belt of Venus”, and is caused by backscattering of refracted sunlight due to fine dust particles high in the atmosphere.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Atacama Desert View with Cerro Armazones
From left to right and above the horizon we can see in this panoramic view of Atacama desert, the Cerro Armazones mountain, illuminated by the sunset reddish color that is reflected in the land and high clouds, coming from the right edge of the image in the opposite direction, where it is located the Pacific Ocean. With an altitude of 3060 meters in the central part of Chiles Atacama Desert, some 130 kilometers south of the town of Antofagasta and about 20 kilometers from Cerro Paranal, home of ESOs Very Large Telescope. Cerro Armazones will be the baseline site for the planned 39-meter-class European Extremely Large Telescope (E-ELT), with a planned construction period of about a decade. The telescope’s “eye” will be almost half the length of a soccer pitch in diameter and will gather 15 times more light than the largest optical telescopes operating today. The telescope has an innovative five-mirror design that includes advanced adaptive optics to correct for the turbulent atmosphere, giving exceptional image quality. The main mirror will be made up from almost 800 hexagonal segments.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Twilight and Sun Pillar in Cerro Paranal
After the sunset, in the beginning of twilight, a partial cloudy sky can promote an impressive combination of beautiful colors. Sometimes, we can see a phenomenon called Sun Pillar. A sun pillar is a vertical shaft of light extending upward from the sun. This great moment was captured in Cerro Paranal, where stands the VLT Telescope.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Profile of Antenna DV-21 from ALMA in the Twilight
After the sunset starts the nautical twilight and the sky assumes a beautiful pallete of blueish and orange colors, giving space to appearing the first stars of the some constelalltions. In the foreground, is also visible one antenna (DV-21) of 12 meters in diameter, pointing to some place of the cold Universe. This are the first tests to experiment the largest configuration that ALMA can support, with antennas spreaded over distances up to 16 km. The array thus simulates a giant, single telescope much larger than any that could actually be built. In fact, ALMA has a maximum resolution which is even better than that achieved, at visible wavelengths, by the Hubble Space Telescope.
The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of radio telescopes in the Atacama desert of northern Chile. Since a high and dry site is crucial to millimeter wavelength operations, the array has been constructed on the Chajnantor plateau at 5,000 meters altitude, near Llano de Chajnantor Observatory and Atacama Pathfinder Experiment. Consisting of 66 12-meter (39 ft), and 7-meter (23 ft) diameter radio telescopes observing at millimeter and submillimeter wavelengths, ALMA is expected to provide insight on star birth during the early universe and detailed imaging of local star and planet formation. ALMA is a single telescope of revolutionary design, composed initially of 66 high-precision antennas, and operating at wavelengths of 0.32 to 3.6 mm. Its main 12-metre array has fifty antennas, 12 metres in diameter, acting together as a single telescope — an interferometer. An additional compact array of four 12-metre and twelve 7-metre antennas complements this. The 66 ALMA antennas can be arranged in different configurations, where the maximum distance between antennas can vary from 150 metres to 16 kilometres, which will give ALMA a powerful variable “zoom”. It will be able to probe the Universe at millimetre and submillimetre wavelengths with unprecedented sensitivity and resolution, with a vision up to ten times sharper than the Hubble Space Telescope, and complementing images made with the VLT Interferometer. Light at these wavelengths comes from vast cold clouds in interstellar space, at temperatures only a few tens of degrees above absolute zero, and from some of the earliest and most distant galaxies in the Universe. Astronomers can use it to study the chemical and physical conditions in molecular clouds — the dense regions of gas and dust where new stars are being born. Often these regions of the Universe are dark and obscured in visible light, but they shine brightly in the millimetre and submillimetre part of the spectrum. ALMA is the most powerful telescope for observing the cool Universe — molecular gas and dust.
ALMA will study the building blocks of stars, planetary systems, galaxies and life itself. By providing scientists with detailed images of stars and planets being born in gas clouds near our Solar System, and detecting distant galaxies forming at the edge of the observable Universe, which we see as they were roughly ten billion years ago, it lets astronomers address some of the deepest questions of our cosmic origins.
Image taken taken in 14/10/2015 from Chajnantor plateau, Atacama desert, Chile.
Stunning view of the Milky Way above ALMA along with the Moonset
In the background we can see the heart of our Galaxy full of gas and dust, star clusters and emission nebulae, as well as the orange star Antares from Scorpius constellation and the dark dust that connects this region to the main arm of Milky Way. Below at right, a faint white light called the Zodiacal Light is very well visible, coming up as a backlight behind the antenna of ALMA (DV-21) with12 meters in diameter, is capturing the wavelengths from vast cold clouds in the interstellar space. Above the horizon we also can see an orange glow coming from the moonset. This are the first tests to experiment the largest configuration that ALMA can support, with antennas spread over distances up to 16 km. The array thus simulates a giant, single telescope much larger than any that could actually be built. In fact, ALMA has a maximum resolution which is even better than that achieved, at visible wavelengths, by the Hubble Space Telescope.
The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of radio telescopes in the Atacama desert of northern Chile. Since a high and dry site is crucial to millimeter wavelength operations, the array has been constructed on the Chajnantor plateau at 5,000 meters altitude, near Llano de Chajnantor Observatory and Atacama Pathfinder Experiment. Consisting of 66 12-meter (39 ft), and 7-meter (23 ft) diameter radio telescopes observing at millimeter and submillimeter wavelengths, ALMA is expected to provide insight on star birth during the early universe and detailed imaging of local star and planet formation. ALMA is a single telescope of revolutionary design, composed initially of 66 high-precision antennas, and operating at wavelengths of 0.32 to 3.6 mm. Its main 12-metre array has fifty antennas, 12 metres in diameter, acting together as a single telescope — an interferometer. An additional compact array of four 12-metre and twelve 7-metre antennas complements this. The 66 ALMA antennas can be arranged in different configurations, where the maximum distance between antennas can vary from 150 metres to 16 kilometres, which will give ALMA a powerful variable “zoom”. It will be able to probe the Universe at millimetre and submillimetre wavelengths with unprecedented sensitivity and resolution, with a vision up to ten times sharper than the Hubble Space Telescope, and complementing images made with the VLT Interferometer. Light at these wavelengths comes from vast cold clouds in interstellar space, at temperatures only a few tens of degrees above absolute zero, and from some of the earliest and most distant galaxies in the Universe. Astronomers can use it to study the chemical and physical conditions in molecular clouds — the dense regions of gas and dust where new stars are being born. Often these regions of the Universe are dark and obscured in visible light, but they shine brightly in the millimetre and submillimetre part of the spectrum. ALMA is the most powerful telescope for observing the cool Universe — molecular gas and dust. ALMA will study the building blocks of stars, planetary systems, galaxies and life itself. By providing scientists with detailed images of stars and planets being born in gas clouds near our Solar System, and detecting distant galaxies forming at the edge of the observable Universe, which we see as they were roughly ten billion years ago, it lets astronomers address some of the deepest questions of our cosmic origins.
Image taken taken in 14/10/2015 from Chajnantor plateau, Atacama desert, Chile.
Twilight Above the interferometer VLTI
Nautical twilight, above the Very Large Telescope platform. Near the horizon the bright moon is shining above the Antu telescope, the first one near the center. At his left, above the horizon are visible some of the Auxiliary Telescopes (ATs) of 1.8 m aperture. At the right side of Antu, is the telescope Kueyen, with a mirror of 8.2m diameter. Both, are opening and preparing for a night of observations. This telescopes are generally used separately, but can be used together to achieve a very high angular resolution. Looking from outside, they are reflecting a silver color coming from the moon reflection on its metalic surface. In the ground, at the left side of the image, we can see part of the interferometer (VLTI) complex, where the movable Auxiliary Telescopes can be placed.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 15/10/2015 from Cerro Paranal, Atacama desert, Chile.
Sun Pillar in Cerro Paranal
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Very Large Telescope Platform in the Twilight
Nautical twilight, above the Very Large Telescope platform. Near the horizon the bright moon is shining above the Antu telescope, the first one near the center. At his left, above the horizon are visible some of the Auxiliary Telescopes (ATs) of 1.8 m aperture. At the right side of Antu, the telescopes Kueyen, Melipal and Yepun, with mirrors of 8.2m diameter, are opening and preparing for a night of observations. This telescopes are generally used separately, but can be used together to achieve a very high angular resolution. Looking from outside, they are reflecting a silver color coming from the moon reflection on its metalic surface. In the ground, at the left side of the image, we can see part of the interferometer (VLTI) complex, where the movable Auxiliary Telescopes can be placed.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred meters. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 15/10/2015 from Cerro Paranal, Atacama desert, Chile.
Stargazing with Passion – Twilight and Crescent Moon on VLT
In this colorful lovely scene captured at the twilight, we can see two skywatchers enjoying his passion about the Universe, with a Crescent Moon shining between the clouds and above the Auxiliary Telescopes (ATs) of VLT.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Milky Way Arm Crossing Antu, Kueyen and Melipal Telescopes
Milky Way arm of gas and dust lying behind the Very Large Telesope Antu, Kueyen e Melipal, while it is capturing the light coming from space. At the right edge of the image, we can see the VLT Survey Telescope (VST), that is the latest telescope to be added to ESO’s Paranal Observatory in the Atacama Desert of northern Chile.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 15/10/2015 from Cerro Paranal, Atacama desert, Chile.
A Planet of Very Large Telescopes
After sunset a partial cloudy sky can promote the appearance of a beautiful show of colors, specially if we have a night of Moonlight that can illuminate and show a strange game of ghostly shapes in the clouds, combined with a starry sky as a background with the Milky Way. In the foreground, we can see in this fish-eye fulldome picture some of the Auxiliary Telescopes availabe in the VLT plataform and the Antu 8.2m diameter Large Telescope.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 16/10/2015 from Cerro Paranal, Atacama desert, Chile.
Twilight With a New Large Configuration of Antennas in ALMA
After the sunset starts the nautical twilight and the sky assumes a beautiful pallete of blueish and orange colors, giving space to appearing the first stars of the some constelalltions. In the foreground, is also visible one antenna (DV-21) of 12 meters in diameter, pointing to some place of the cold Universe. This are the first tests to experiment the largest configuration that ALMA can support, with antennas spreaded over distances up to 16 km. The array thus simulates a giant, single telescope much larger than any that could actually be built. In fact, ALMA has a maximum resolution which is even better than that achieved, at visible wavelengths, by the Hubble Space Telescope.
The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of radio telescopes in the Atacama desert of northern Chile. Since a high and dry site is crucial to millimeter wavelength operations, the array has been constructed on the Chajnantor plateau at 5,000 meters altitude, near Llano de Chajnantor Observatory and Atacama Pathfinder Experiment. Consisting of 66 12-meter (39 ft), and 7-meter (23 ft) diameter radio telescopes observing at millimeter and submillimeter wavelengths, ALMA is expected to provide insight on star birth during the early universe and detailed imaging of local star and planet formation. ALMA is a single telescope of revolutionary design, composed initially of 66 high-precision antennas, and operating at wavelengths of 0.32 to 3.6 mm. Its main 12-metre array has fifty antennas, 12 metres in diameter, acting together as a single telescope — an interferometer. An additional compact array of four 12-metre and twelve 7-metre antennas complements this. The 66 ALMA antennas can be arranged in different configurations, where the maximum distance between antennas can vary from 150 metres to 16 kilometres, which will give ALMA a powerful variable “zoom”. It will be able to probe the Universe at millimetre and submillimetre wavelengths with unprecedented sensitivity and resolution, with a vision up to ten times sharper than the Hubble Space Telescope, and complementing images made with the VLT Interferometer. Light at these wavelengths comes from vast cold clouds in interstellar space, at temperatures only a few tens of degrees above absolute zero, and from some of the earliest and most distant galaxies in the Universe. Astronomers can use it to study the chemical and physical conditions in molecular clouds — the dense regions of gas and dust where new stars are being born. Often these regions of the Universe are dark and obscured in visible light, but they shine brightly in the millimetre and submillimetre part of the spectrum.
ALMA is the most powerful telescope for observing the cool Universe — molecular gas and dust. ALMA will study the building blocks of stars, planetary systems, galaxies and life itself. By providing scientists with detailed images of stars and planets being born in gas clouds near our Solar System, and detecting distant galaxies forming at the edge of the observable Universe, which we see as they were roughly ten billion years ago, it lets astronomers address some of the deepest questions of our cosmic origins.
Image taken taken in 14/10/2015 from Chajnantor plateau, Atacama desert, Chile.
A Close-up of ALMA Antenna DV-21 and the Crescent Moon with Earthshine
After the sunset starts the nautical twilight and the sky assumes a beautiful pallete of blueish and orange colors, giving space to appearing the first stars of the some constelalltions. In the foreground, is also visible one antenna (DV-21) of 12 meters in diameter, pointing to some place of the cold Universe and at his right side, the Crescent Moon with the strong Earthshine effect very well visible.
The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of radio telescopes in the Atacama desert of northern Chile. Since a high and dry site is crucial to millimeter wavelength operations, the array has been constructed on the Chajnantor plateau at 5,000 meters altitude, near Llano de Chajnantor Observatory and Atacama Pathfinder Experiment. Consisting of 66 12-meter (39 ft), and 7-meter (23 ft) diameter radio telescopes observing at millimeter and submillimeter wavelengths, ALMA is expected to provide insight on star birth during the early universe and detailed imaging of local star and planet formation.
ALMA is a single telescope of revolutionary design, composed initially of 66 high-precision antennas, and operating at wavelengths of 0.32 to 3.6 mm. Its main 12-metre array has fifty antennas, 12 metres in diameter, acting together as a single telescope — an interferometer. An additional compact array of four 12-metre and twelve 7-metre antennas complements this. The 66 ALMA antennas can be arranged in different configurations, where the maximum distance between antennas can vary from 150 metres to 16 kilometres, which will give ALMA a powerful variable “zoom”. It will be able to probe the Universe at millimetre and submillimetre wavelengths with unprecedented sensitivity and resolution, with a vision up to ten times sharper than the Hubble Space Telescope, and complementing images made with the VLT Interferometer. Light at these wavelengths comes from vast cold clouds in interstellar space, at temperatures only a few tens of degrees above absolute zero, and from some of the earliest and most distant galaxies in the Universe. Astronomers can use it to study the chemical and physical conditions in molecular clouds — the dense regions of gas and dust where new stars are being born. Often these regions of the Universe are dark and obscured in visible light, but they shine brightly in the millimetre and submillimetre part of the spectrum. ALMA is the most powerful telescope for observing the cool Universe — molecular gas and dust. ALMA will study the building blocks of stars, planetary systems, galaxies and life itself. By providing scientists with detailed images of stars and planets being born in gas clouds near our Solar System, and detecting distant galaxies forming at the edge of the observable Universe, which we see as they were roughly ten billion years ago, it lets astronomers address some of the deepest questions of our cosmic origins.
Image taken taken in 14/10/2015 from Chajnantor plateau, Atacama desert, Chile.
Twlight on VLT and the Southern Crescent Moon
Twilight behind the Yepun VLT Telescope (at left) and Survey Telescope VST (at right) while they start opening his doors, preparing for a night of research. The faint and inverted crescent moon of the southern hemisphere, can be seen in the center of the image.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 15/10/2015 from Cerro Paranal, Atacama desert, Chile.
Sunset Between the VLT Telescopes
Sunset rays illuminating with an orange light the left face of Antu Telescope (the first one). In the foreground, at right, we can see the Melipal Telescope few minutes before start opening his doors to the Universe. The faint and inverted crescent moon of the southern hemisphere, can be seen at the left upper edge of the telescope, surrounded by the blue sky of twilight.
The Very Large Telescope (VLT) is a telescope operated by the ESO – European Southern Observatory on Cerro Paranal in the Atacama Desert of northern Chile. The VLT is the world’s most advanced optical instrument, consisting of four Unit Telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution. The four separate optical telescopes are known as Antu, Kueyen, Melipal and Yepun, which are all words for astronomical objects in the Mapuche language, with optical elements that can combine them into an astronomical interferometer (VLTI), which is used to resolve small objects. The interferometer is complemented by four movable Auxiliary Telescopes (ATs) of 1.8 m aperture. The 8.2m diameter Unit Telescopes can also be used individually. With one such telescope, images of celestial objects as faint as magnitude 30 can be obtained in a one-hour exposure. This corresponds to seeing objects that are four billion (four thousand million) times fainter than what can be seen with the unaided eye. The telescopes can work together, to form a giant ‘interferometer’, the ESO Very Large Telescope Interferometer, allowing astronomers to see details up to 25 times finer than with the individual telescopes. The light beams are combined in the VLTI using a complex system of mirrors in underground tunnels where the light paths must be kept equal to distances less than 1/1000 mm over a hundred metres. With this kind of precision the VLTI can reconstruct images with an angular resolution of milliarcseconds, equivalent to distinguishing the two headlights of a car at the distance of the Moon.
Image taken taken in 15/10/2015 from Cerro Paranal, Atacama desert, Chile.
1% of Crescent Moon above the Medieval Village of Monsaraz
The Crescent Moon with 1% of light, lying behind the castle and medieval village of Monsaraz. 19/04/2015 Monsaraz | Alqueva Dark Sky Reserve – Portugal
Milky Way and GTC in Twilight
Vertical vision of our great Milky Way above the GTC – Gran TeCan Canarias Telescope during the twilight in observatory Roque de Los Muchachos. Above the dome we can see the main stars of constellation Scorpius.
Sharing the Passion of Shooting the Beauty of the Night Sky
Sharing the Passion of Shooting the Night Sky- Image captured in the land of Museu da Luz, Mourão – Alqueva Dark Sky Reserve. Canon EOS 60da- ISO1600, Exp. 30 sec 11mm at f/2.8. Taken in 13/09/2014 23.40
Enjoying Venus corona above the Giant´s Causeway – Northen Ireland
In the image we can see a Skygazer enjoying the planet venus with a visible corona phenomenon between the Giant’s Causeway, near Bushmills, in northeast coast of Northen Ireland. Is an area of about 40,000 interlocking basalt columns, the result of an ancient volcanic eruption, 60 million years ago. It was declared a World Heritage Site byUNESCO in 1986. Near the top edge of the image we can see the Pleiades star cluster.
Corona, is produced by the diffraction of light from either the Sun, the Moon or some bright planets by individual small water droplets and sometimes tiny ice crystals of a cloud.
ISO 2000, 30 sec, 16mm at f/2.8. In 20/03/2015 at 20:17
Moonrise in Monsaraz Castle
EN: Full Moonrise behind the medieval village and castle of Monsaraz | Sky of Monsaraz
PT: Nascer da lua cheia por detrás da vila e castelo medieval de Monsaraz | Céu de Monsaraz
Silhouette of Noudar Church in a Starry Trail Background
Silhouette of Noudar Church in a Starry Trail Background
Included in the great Alqueva Dark Sky Reserve – first site in the world to receive the “Starlight Tourism Destination” certification – Noudar Natural Park is located in a farm estate called Herdade da Coitadinha spreads across 1000 hectare, ‘over-the-hills’ between the winding rivers Ardila and Múrtega and lodged among hills and summits near the town of Barrancos (Alentejo, Portugal) and in the border with Spain. The road from the Park’s entrance to the Noudar Castle goes through an extensive holm oak grove (‘montado’) area, ending with a majestic view over the water lines. In Noudar, life presents itself in a state of wilderness and absolute purity.
The Castle of Noudar and the church of Nossa Senhora do Desterro is located between the Múrtega and the Ardila rivers which flow towards the West. Its construction was finished in 1307, during the reign of Don Dinis. The place was chosen because of its natural defenses, easy access and the closeness of a water spring of excellent quality – Fonte da Figueira, located roughly 250 meters to the East of the castle, under the hilltop known as Forca (“the Gallows”). Good and plentiful farming land and cattle grazing fields can also be found near the castle. This medieval fortress was very important for border defense against the kingdom of Castile during the early 14th Century.
More about Alqueva Dark Sky Reserve:
Alqueva is the first site in the world to receive the “Starlight Tourism Destination” certification. This certification, awarded by the Starlight Foundation is supported by UNESCO, UNWTO and IAC. Starlight destinations are visitable places characterized by excellent quality for the contemplation of starry skies, and the practice of tourist activities based on this resource. www.darkskyalqueva.com
Waning Crescent Moon above Noudar Castle Church
Waning Crescent Moon above Noudar Castle Church
Included in the great Alqueva Dark Sky Reserve – first site in the world to receive the “Starlight Tourism Destination” certification – Noudar Natural Park is located in a farm estate called Herdade da Coitadinha spreads across 1000 hectare, ‘over-the-hills’ between the winding rivers Ardila and Múrtega and lodged among hills and summits near the town of Barrancos (Alentejo, Portugal) and in the border with Spain. The road from the Park’s entrance to the Noudar Castle goes through an extensive holm oak grove (‘montado’) area, ending with a majestic view over the water lines. In Noudar, life presents itself in a state of wilderness and absolute purity.
The Castle of Noudar and the church of Nossa Senhora do Desterro is located between the Múrtega and the Ardila rivers which flow towards the West. Its construction was finished in 1307, during the reign of Don Dinis. The place was chosen because of its natural defenses, easy access and the closeness of a water spring of excellent quality – Fonte da Figueira, located roughly 250 meters to the East of the castle, under the hilltop known as Forca (“the Gallows”). Good and plentiful farming land and cattle grazing fields can also be found near the castle. This medieval fortress was very important for border defense against the kingdom of Castile during the early 14th Century.
More about Alqueva Dark Sky Reserve:
Alqueva is the first site in the world to receive the “Starlight Tourism Destination” certification. This certification, awarded by the Starlight Foundation is supported by UNESCO, UNWTO and IAC. Starlight destinations are visitable places characterized by excellent quality for the contemplation of starry skies, and the practice of tourist activities based on this resource. www.darkskyalqueva.com
Venus at Dawn above Noudar Castle
Venus at Dawn above Noudar Castle
Included in the great Alqueva Dark Sky Reserve – first site in the world to receive the “Starlight Tourism Destination” certification – Noudar Natural Park is located in a farm estate called Herdade da Coitadinha spreads across 1000 hectare, ‘over-the-hills’ between the winding rivers Ardila and Múrtega and lodged among hills and summits near the town of Barrancos (Alentejo, Portugal) and in the border with Spain. The road from the Park’s entrance to the Noudar Castle goes through an extensive holm oak grove (‘montado’) area, ending with a majestic view over the water lines. In Noudar, life presents itself in a state of wilderness and absolute purity.
The Castle of Noudar and the church of Nossa Senhora do Desterro is located between the Múrtega and the Ardila rivers which flow towards the West. Its construction was finished in 1307, during the reign of Don Dinis. The place was chosen because of its natural defenses, easy access and the closeness of a water spring of excellent quality – Fonte da Figueira, located roughly 250 meters to the East of the castle, under the hilltop known as Forca (“the Gallows”). Good and plentiful farming land and cattle grazing fields can also be found near the castle. This medieval fortress was very important for border defense against the kingdom of Castile during the early 14th Century.
More about Alqueva Dark Sky Reserve:
Alqueva is the first site in the world to receive the “Starlight Tourism Destination” certification. This certification, awarded by the Starlight Foundation is supported by UNESCO, UNWTO and IAC. Starlight destinations are visitable places characterized by excellent quality for the contemplation of starry skies, and the practice of tourist activities based on this resource. www.darkskyalqueva.com
Biggest & Brightest Full Moon of the Year 2014
Image of the biggest and brightest full Moon of the year 2014, captured on August 10. Astronomers call it a perigee moon, but the popular term is “supermoon.” The image was captured from Alqueva, Dark Sky Reserve, Portugal on 10/09/2014 at 20:39. Canon 50D – ISO640; Exp. 1/400 secs. f/7 at 560mm ( Astro Professional APO ED80).
ISS transiting the Summer Triangle
ISS crossing the arm of Milky Way reaching a magnitude of -3.2 above the land of Vila Boim, in Alentejo. In the top of the image, the path of International Space Station is transiting between the stars that forming the well known Summer Triangle, in that moment as seen from Earth, the ISS was reaching the Zenith, the point above our heads, the moment when it is also more close to us..
Canon 60Da – ISO 200, Exp.208 Secs at f/4 with a 11mm lens and a Vixen Polarie travel mount. Taken in 02-08-2014 at 22h30, during an exposure of consecutive 3.4 minutes.
A colorful life, full of stars!
In this picture captured in Alentejo, we can see the main stars of Big Dipper, Ursa Minor and Cassiopeia, scratching the colorful skies of a celestial blue in a twilight of moonlight. In the land, a house full of life, space and water, is the ideal spot for a skygazer who loves to appreciate the beauty of Alentejo skies.
Canon 50D – f/4 ISO 800 Exp. 20 Secs 11mm. Taken in 07-08-2014 between 22:17 and 1:04 Sum of 466 images with a total time of 2.6h.
A Moonlite scene from Alvão
Taken in the top of Alvão mountain range, Vila Real, Portugal. The full moon helped to light up all the rocky scene in the landscape. In the sky, we can see the stars that forming the asterism of summer triangle. Canon 60D – ISO640; 11mm at f/2.8; Exp. 15 secs. Taken in 8-06-2014 at 25:51
Crescent Moon and Jupiter in the Twilight of Fonte-de-Telha
Sequence of a Crescent Moon Earthshine, captured in the nautical twilight until the moon sets behind the trees of a small pine forest in Fonte-de-Telha, Almada. Portugal, facing to the Atlantic Ocean. Above the Moon and the treetop, is visible the disc of planet Jupiter, accompanied with two of its main moons (Ganymede and Europa).
Canon 50D – ISO640; Exp. 4 secs. f/3.5 at 70mm. In 31/05/2014 at 21:37. Sequence of 858 images.
“Honey Moon” in Lisbon
Canon 60Da – ISO1000; Exp. 1/40s; f/2.8 at 200mm Canon L lens (f/2.8). In 13/06/2014 at 21:33
The Full Moon of June – Friday 13th – 2014, well know as “Honey Moon”, was captured in Lisbon, from Algés region. “With the sun’s path across the sky at its highest during this month of the summer solstice, the moon is at its lowest, which keeps the lunar orb close to the horizon and makes it appear more amber than other full moons this year.” (NG). In the foreground we can see the Christ the King monument, in Lisbon, in a clifftop 133 metres above the sea, and behind it, the full moon rising in the east horizon.
The study predictions for this particular position have been kindly maded by my friend and portuguese author of many astronomy books, Dr. Guilherme de Almeida. Thank you Guilherme for the great spot you found. Image below: Canon 50D – ISO2000; Exp. 1/15 secs. f/7 at 560mm ( Astro Professional APO ED80). In 13/06/2014 at 21:34
See below the poster with the entire sequence image, made this night. More image here
Ferry Moon
The May´s Moon captured in the twilight and 34 minutes after reaching their total fullness, with the disk 100% illuminated by the Sun, rising above Barreiro city, in Setúbal, Portugal, visible in the horizon with one of its Ferry boats crossing the Tagus River in the foreground. Canon 60Da – ISO400; Exp. 1/125s; f/4.5 at 200mm Canon L lens (f/2.8).
Full Worm Moon Sequence in the Lighthouse
The full Moon in this sequence, well known as “Worm Moon”, for signaling the coming of spring in the northern hemisphere, was captured in Cape Espichel lighthouse. Opened in 1790, in 1865 was powered by olive oil, changing to fuel in 1886, when its light began to be fueled by glowing vapor of oil, much later in 1926 by electricity. Measures 32 meters high and lies at an altitude of 168m above the see level. Presently, its luminous range is 42 nautical miles, about 67 km.
Canon 60Da – 35mm at f/4 ISO500; 1/5 sec. Sequence of 93 images with 2-minute intervals each other, taken in 16/03/2014 between 19:16 and 20:42. Cabo Espichel, Sesimbra, Portugal.
Comet Lovejoy in Serra D´Aire
This image shows the peculiar landscape of Algar do Ladoeira, in Serra de Santo António, near Serra de Aires with a view to the comet c/2013 R1 well known as the comet Lovejoy, specially, after the dead of comet ISON who was suposed to be the comet of the century, but unfortunately was to young to resist the power our Sun. To help identify the comet in the picture, please see below the annotated version of the picture. Canon 50D – ISO1600 f/2.8; Exp:10 sec. 35mm, taken in 07/12/2013 at 18h30.
Clouds and Fog in Caldera de Taburiente
Captured in a height of 2,200 meters from the sea level we can see the clouds and Fog near the border of Caldera de Taburiente – a very large volcanic crater with about 10 km across. Above the horizon the sun sets behind the silhouette mountains of Roque de Los Muchachos, where stands a huge complex with the some of the largest telescopes in the world. The picture was taken in Pico de La Cruz, La Palma, Canary Island.
Canon 60Da – ISO250; 24mm at f/4; Exp. 1/250 secs. in 26/09/2013 at: 20h11
Colorful Twilight in Roque de Los Muchachos
In this colorful twilight view captured after the sunset from the top of El Roque de Los Muchachos, home to one of the most extensive fleets of telescopes to be found anywhere in the world, we can see a startrail with an amazing view of planet Venus (the brightest trail at left), reflected in the “ocean of clouds” below the land. On earth, the bright trail was left by the lights of a car that was moving inside the observatory area, where is visible from left to right, the Telescopio Nazionale Galileo. TNG is a 3.6m alt-azimuth telescope with a Ritchey-Chretien optical configuration and a flat tertiary mirror feeding two opposite Nasmyth foci and represents the largest Italian optical/infrared telescope. On the right edge of the picture stands the Gran Telescope Canarias (GTC) with a 10,4 meters primary mirror reflecting telescope was designed to incorporate the most up-to-date technology and it is one of the most advanced telescopes in the world, actually, the largest one until now in the optical-infrared system
| Canon 50D – ISO1600; 13mm at f/5; Exp. 30 secs. Sum of 14 images taken in 30/09/2013 between 20:59 and 21:06.
Observatories, Earth Shadow and Belt of Venus
In this picture captured few minutes after the sunset from Roque de Los Muchachos, in La Palma Canary Island, we can see the Earth shadow, a dark blue band that rises upwards from the horizon. The band is the shadow of the Earth on the atmosphere. Immediately above, where the evening air is still lit, glows a pink band called the anti-twilight arch, or “Belt of Venus”. On Earth, stands part of a huge complex with 15 telescopes, some of the largest telescopes in the world. From left to right, the grey dome open is the shelter for the Nordic Optical Telescope (NOT) a modern 2.6-m optical/IR telescope, next, the small white house is the home for Automatic Transit Circle (ATC), an old meridian circle built by Grubb-Parsons in 1950 but completely refurbished and automatized in the 70’s of the past century by the Copenhagen University Observatory (CUO). It main task is to observe evenly bodies at their transit across the meridian. At his right, the big white dome belongs to the great William Herschel Telescope (WHT), the largest optical telescope of its kind in Europe, with a primary mirror of 4.2 meters in diameter, is one of the most scientifically productive telescopes in the world. Next, the small shape in the background near the first white tower is from Liverpool Telescope, a 2 meter diameter optical astronomical telescope, constructed especially for robotic use. The telescope is especially to study variable astronomical phenomena. Now, the first white Tower is from Dutch Open Telescope (DOT) an innovative optical telescope with a primary mirror of 45 cm diameter, for high-resolution imaging of the solar atmosphere. Next far, the silver small dome is from Mercator Telescope, a 1.2 m quasi-robotic telescope which scientific niche is focussed on monitoring variable celestial phenomena with a large range in typical time-scales (pulsating stars, gravitational lenses, Gamma Ray Bursts, active Galactic Nuclei), immediately adjacent to the next tower (just in the picture) we can see the Swedish 1-m Solar Telescope (SST), the largest solar telescope in Europe and number one in the world when it comes to high spatial resolution. The last white domes belongs to Isaac Newton Telescope (INT) with a 2.54-meter primary mirror and the Jacobus Kapteyn Telescope (JKT) with a parabolic primary mirror of 1.0 m diameter.
| Canon 60Da – ISO400; 24mm at f/4; Exp. 1/80 secs. in 30/09/2013 at: 20h10 AM
A Road to Big Dipper
The Big Dipper (Ursa Major) lies in the “end” of the road to Roque de Los Muchachos, where a stargazer is enjoying the great sky of La Palma. The excellent quality of the sky for astronomy in the Canaries is determined and protected by Law. As a result, the observatories of the Instituto de Astrofísica de Canarias (IAC) are an “astronomy reserve” which has been available to the international community since 1979. I´ve used a diffuse filter in the camera lens, to increase and highlight the main stars of Ursa Major.
| Canon 60Da – ISO2500; 24mm at f/2; Exp. 15 secs. in 30/09/2013 at: 06h42 AM
Venus and Saturn in Libra from Los Andenes
The Nautical Twilight seen from Los Andenes, near Roque de Los Muchahos, in La Palma, where we could see the strong light of planet Venus (the strongest light in the picture) inside the stellar asterism with a trapezium shape, that forms the Libra constellation. In the same imaginary line which conects Venus to the Zubenelgenubi star, we can find the planet Saturn, the third brightest object in the picture (at the right side of the image) almost with the same brightness of Antares, from Scorpius constellation, visible in the top of the picture as an orange star. Below the horizon, we found an ocean of clouds, located inside the Caldera. The rocky silhouette is part of Roque de Los Muchachos, where stands a huge complex with the some of the largest telescopes in the world.
| Canon 60Da – ISO640; 24mm at f/2; Exp. 10 secs. in 29/09/2013 at: 20h58 AM
Zodiacal Light, Milky Way and William Herschel Telescope
In this mosaic of 25 images, we can see the rocky silhouette between Los Andenes and Roque de Los Muchachos, where is the home to one of the most extensive fleets of telescopes to be found anywhere in the world, and where 15 telescopes from 19 nations are using the best night sky in Europe to explore the cosmos. The William Herschel Telescope (WHT) is one of them, with a primary mirror of diameter 4.2 meters, the telescope can be seen below right in the picture, with is dome opened, seems to pointing to the triangle formed in the middle of the picture by the smooth band of Zodiacal light (at left) which is crossing the Milky Way smooth region (at right), below the Orion constellation. These smooth bands are also important to let us find objects, like M44 above the rocks, and following the zodical light we find the planet Jupiter, the brightest star in the image. In the middle of Milky Way band, we can find the Rosette nebula. The Moon is shining in Cancer constellation, behind the rocks and below right to the star cluster M44 (NGC2632), so creating a blueish glow – more strong and evident – in the left half part of the picture.
| Mosaico – Canon 60Da – ISO2500; 24mm at f/2; Exp. 15 secs. in 30/09/2013 at: 05h50 AM Mosiac of 25 images.
Sirius in a Lovely Morning Scene
A lovely moonlite scene captured in La Palma moutains, in Los Canarios, Fuencaliente, facing to the Atlantic Ocean. While Sirius, the brightest star in the northen hemisphere is shining blue and strong in the morning sky, the Teide volcano seems to emerge from the clouds in the horizon, with 3718 km is the highest point above sea level in the islands of the Atlantic Ocean and the world’s third largest volcano. In the image, is also visible the entire constellation of Canis Major, and below right the Sirius, is clearly visible the star cluster M41.
Canon 60Da – ISO1250; 24mm at f/2.8; Exp. 15 secs. in 28/09/2013 at: 4h22 AM
Lost in the Beach – Planets Alignment wiht Crescent Moon
I could be “lost in the beach” on the evening of 7 September, but actually I was claiming such a beautiful peaceful moment, enjoying the alignment between planets, Saturn (in the top left corner), Venus and Spica star (in the center image), and as it we following down this imagined diagonal line, we can finally find the Crescent Moon above the horizon.
Canon 50D – ISO160; f/4; Exp. 1.30 seconds for each sequence “startrail” image; at 24mm. Picture taken in 07-09-2013 at 20h38
Below you will find a resume with all publications – printed and online – related to this particular photograph.
Please refer the i-frame above, generated automatically from the overview page Press.
After the Dark, comes the light
This is a panoramic photograph captured at dawn on the big lake Alqueva. In addition to the characteristic tones of a nautical twilight, in this case, morning, it is still possible to identify at left in the picture, the Big Dipper, lying down as it shaped farewell until next night … it is now time to rest, and give rise to the birth of the Sun King who will reign all day, filling with Life and Light, this beautiful planet that is our EARTH, from another perspective, seen as a small blue dot suspended in the Universe (the well known Pale Blue Dot).
Canon 60Da – ISO 1000, 35mm lens at f/2.8, Exp 13 secs. Panoramic of 13 images, taken in 15/06/2013 at 04:45 AM
The Alqueva´s Dawn sky
Taken just before dawn, in the region of Lake Alqueva and near the Chapel of St. Peter, in Mourão, where stars mingle with the rich tones of morning nautical twilight. On the left, the most visible reflection in the water belongs to the star Capella, as the extreme right over the horizon and through the tree, almoste hiden, is the Pleiades (M45). The upper cluster of stars in the image belongs to the central region of the constellation Perseus.
Canon 60Da – ISO1600 exp 15 seconds. 35 mm f/2.8 15/06/2013 at 04:34 AM
From Moon to the Planets
Panoramic view over Almada City and Lisbon at the Nautical Twilight, with the Full moon rising above the Eastern horizon (right side of the image), while at the same time but in the opposite direction, the planets Venus, Mercury and Jupiter, are aligned in a triangle formation, setting in the Western horizon (left side of the image).In this panoramic picture is also visible the smooth light transition in the sky, with the end of Nautical Twilight and the beginning of Astronomical Twilight (almost night), at right. Facing to North, is visible the great lighted Monument Christ the King and at the left side of it, part of the 25 April Bridge that connects Almada to Lisbon.
Canon 50D – ISO200; f/4; Exp. 1,6 Sec; 35mm. Panoramic of 10 images with about 200º, taken at 21h42 in 25/05/2013. Below is the image with identification:
Photographing a beautiful twilight
Self portrait of the conjunction between Jupiter (the Brightest star in the image) and Crescent Moon with the disc only 3% illuminated by the Sun. Near the horizon, is visible the city of Lisbon.
Canon 50D – ISO400; Exp. 1,6sec. F/4; 35mm. 11/05/2013 21h48
A “Macro” Picture of the Moon – Planets Alignment
Self portrait of the conjunction between Jupiter (the Brightest star in the image) and Crescent Moon with the disc only 3% illuminated by the Sun, and where is visible the Earthshine effect. Venus, also in conjunction, was covered by the cloudy band in the Lisbon horizon. While I was enjoying this beautiful and gold moment, holding my camera, I remembered to take a “Macro photo of the moon, maybe the first macro-moon shot from planet earth :=) “, but is it possible ?, yes it is, just take a look to the second picture, I only have to approach my lens camera, to the lunar limb :=) Images taken from Capuchos, Almada, Portugal.
Canon 50D – ISO400; Exp. 2sec. F/4; 35mm. 11/05/2013 21h41 and 21h43.
Below you will find a resume with all publications – printed and online – related to this particular photograph.
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Jupiter, Moon Earthshine and Venus, Aligned in Capuchos
Alignment between Jupiter, Crescent Moon and Venus, captured from Capuchos village, in Almada, Portugal. Jupiter is the bright star in the left upper corner. Venus is the bright star near the yellow/orange sky, and the cloudy band. Near the horizon is visible the city of Lisbon.
Canon 50D – ISO200; Exp. 1.3sec. f/4 at 35mm. In 11/05/2013 at 21:24
Milky Rocky
A stargazer above the rocky region of Portinho da Arrábida, Portugal, with the Milky Way behind it, visible in the dawn. Canon 60Da – ISO 1600; Exp.15 Seg; f/2.8; 24mm. In 11/05/2013 at 05h10 AM.
Milky Way in Daylight
A rocky region of Portinho da Arrábida, Portugal, with the center of Milky Way behind it, visible at the dawn – almost in the daylight – with the stars of Saggitarius and Scorpius clearly visible, while the sky is turning blue, slowly. Canon 60Da – ISO 1600; Exp.15 Sec; f/2.8; 24mm. In 11/05/2013 at 05h14 AM.
Below is the image with the sky identification.
Below you will find a resume with all publications – printed and online – related to this particular photograph.
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Lonely Canoe
Nautical Twilight and a smooth zodiacal light in the direction of Jupiter, visible near the center image, as the brightest star. Image captured in the Pegrogão´s Albufeira, a region of great Alqueva´s Lake, covered by the Dark Sky Reserve.
Canon 50D – ISO1250 ; f/4 ; Exp. 30s. ; 10mm. 27/04/2013 at 21h29
Smooth zodiacal light in the Lake
Nautical Twilight and a smooth zodiacal light in the direction of Jupiter, visible near the center image, as the brightest star. Image captured in the Pegrogão´s Albufeira, a region of great Alqueva´s Lake, covered by the Dark Sky Reserve. Canon 50D – ISO1250 ; f/4 ; Exp. 30s. ; 10mm. 27/04/2013 at 21h25
Canoeing family
A Canoeing family preparing for a moonlight ride in the lake. Canon 50D – ISO640; f/4; Exp. 1/60s; 10mm. 27/04/2013 20h58
Starry cloudy twilight
Panorama of a Starry cloudy twilight above the Pedrogão´s Albufeira, in Moura, a region of great Alqueva´s Lake, covered by the Dark Sky Reserve. Jupiter, visible near the center image and low in the horizon, is the brightest star. Above it, is visible the entire constellation of Auriga.
Canon 60Da – ISO1250, f/2; Exp. 13s ; 24mm. 27/04/2013 22h52 AM
Sunset Jupiter
After the sunset, in the begining of twilight, only the brightest stars can emerge from the blue lighted sky, normally only the planets have light enough to do this, like we can see in the upper left corner, with the planet Jupiter shining against this dramatic sky and landscape, captured in the Contenda homestead.
Canon 50D – ISO200, f/10; Exp. 20s ; 10mm. 26/04/2013 20h43
Crepuscular Rays in Tomina
Image captured near Convento da Tomina region, a area inside the great Contenda homestead, near Moura and Barrancos, Portugal. In the sky we could see the dramatic effect of the phenomenon known as “Crepuscular rays, in atmospheric optics, are rays of sunlight that appear to radiate from the point in the sky where the sun is located. These rays, which stream through gaps in clouds (particularly stratocumulus) or between other objects, are columns of sunlit air separated by darker cloud-shadowed regions. Despite seeming to converge at a point, the rays are in fact near-parallel shafts of sunlight, and their apparent convergence is a perspective effect (similar, for example, to the way that parallel railway lines seem to converge at a point in the distance).”
“The name comes from their frequent occurrences during crepuscular hours (those around dawn and dusk), when the contrasts between light and dark are the most obvious. Crepuscular comes from the Latin word “crepusculum”, meaning twilight.”
Canon 50D – ISO500, f/13; Exp. 1/320s ; 10mm. 26/04/2013 19h16
Below you will find a resume with all publications – printed and online – related to this particular photograph.
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The Moon shining like a Ray of light
Nautical twilight at dawn in Monsaraz. The moon shining in the stargazer like a cosmic ray of light.
Canon 60Da – ISO1250; 24mm; f/2.8; 13 secs. 06/04/2013 at 06h04 AM.
Twilight meteor in the Moonlite
Twilight at dawn in Monsaraz with the moonlite. In the left upper corner we could see the trail of a shooting star.
Canon 60Da – ISO1600 Lens 24mm f/2; Exp. 15 secs. 06/04/2013 at 05h47
Comet PanSTARRS over Almada
After a few days of rain and clouds in the horizon, I can finally photograph the comet PanSTARRS in the portuguese sky. Actually, I was arrived from a weekend photo trip and was exausted, but the sky was totally clear, so, I found some “extra forces” to delay my sleep, and I´ve tried to find this view from my home window.
Near and below the comet there was two stars with a magnitude of +6.3. (HIP2734 / HIP 2832).The image was captured in the city of Almada, near Lisbon, Portugal.
Canon 50D, f/5; 1,60sec. ISO1000 at 133mm and 108mm. 17/03/2013 at 19h43
The Orada´s Convent
Night Sky image of the Convent of Orada, in Monsaraz, with it´s great cross. Canon 50D – ISO2500; 24mm; f/4; 30 secs. 13/01/2013 at 06h35 AM.
The Convent of Orada
Night Sky image of the Convent of Orada, in Monsaraz, with it´s great cross in the left side of the image. Canon 50D – ISO2500; 11mm; f/4.5; 30 secs. 13/01/2013 at 06h25 AM.
Nautical Sky
Image taken near the nautical center of Monsaraz, during the Nautical Twilight, a special moment when the first stars appear in the sky. Few moments after I took the image, I saw a strong Zodiacal Light coming from the direction of the mountain. See the short time lapse movie. Canon 50D – ISO1000; f/4; exp. 15 secs; Lens 10mm.
Twilight in the Alqueva´s Lake
Twilight in the Alqueva´s Lake, Monsaraz. Portugal. Canon 50D – IOS125; f/7.1; Exp. 2 secs; 10mm lens.
The beauty deep sky shining above the land
Image taken near a small part of the largest manmade lake in Europe (250 sq km) and one of the world’s largest, called Alqueva. Around this area, we also can find some of the darkest sky regions in Portugal, like Monsaraz, inserted in Dark Sky Reserve Alqueva, the world’s first certified ‘Starlight Tourism Destination’.
From left to right, in the land, we could see the silhouette of the photographer, Babak Tafreshi, that was also making his images of the night sky. Next to the tree, we can see the light of the Monsaraz Castle, also reflected in the calm water of the lake, 30 minutes after the moonset.
Even with some light pollution coming directly from the village castle, the sky above shows a rich variety of deep sky objects that are visible in the infrared camera, like Canon EOS 60Da, as well a lot of star clusters, one asteroid and the Planet Jupiter. From left to right, in the sky, we could identify M46 and M47, M41, and above Sirius the Seagull nebula IC2177. Near the center top image, is visible another infrared emission from Rosette Nebula. Below, the Barnard´s Loop, Horse Head and Orion nebula M42, are strongest emissions indeed. A little bit to the right making the center upper image, is the Lambda Orionis (Sh2 264), Messia. Above the star aldebaran, is visible the open cluster NGC1647 and near to the left, the Vesta asteroid, and above it another open cluster the NGC1746. Below is the brightest sky object capturing in this image, the planet Jupiter, shining near the pleiades M45. In the upper right corner, is located the last infrared brightest deep sky object, the California nebula, NGC1499.
Canon EOS60Da – F/2 15s ISO4000 35mm lens. Mosaic of 24 images. Image taken in 22/12/2012 at 2:58 AM.
The Night Like a Paiting
Image of a colorful startrail captured in the Monsaraz region, inserted in the Alqueva Dark Sky Reserve.
The M45 and the Tree
The M45 Pleiades photographed above a tree in the Monsaraz region. Portugal. Canon EOS60Da – F/2.8 Exp.15s ISO1000 35mm lens. Taken in 22/12/2012 at 1:50 AM.
Dreaming scene at the morning
A dreamy panoramic view of the early morning with fog, on the big lake Alqueva, in Monsaraz. Canon EOS60Da – F/4 Exp.1s ISO125 35mm lens. Panoramic of 5 images taken in 22/12/2012 at 7:06 AM.
Almendres Cromlech startra
In the sky image, is visible the startrails of Orion Constellation above the stone circle, and the shadows of the stones projected in the land, due to the light of the moon, which light up the landscape from the oposite site.
Canon 50D – ISO 2000; f/4; Exp.25s 10mm em 20/12/2012
Alqueva´s Lake at night
Images taken in Portel, one of the regions inside de Alqueva Dark Sky Reserve, The world’s first certified ‘Starlight Tourism Destination’. In the land, we could see one of the world’s largest manmade lakes (250 sq km). In the sky, it´s clearly visible many star clusters as well as the great Andromeda Galaxy and some part of the Milky Way.
Sum of 18 mosaic images, taken with a Canon 50D, 15 sec, at f/1.8, ISO 2500, Lens: 35mm in 16/07/2012 at 2:51 AM
The Lighttrails of the Knights Templar
The castle of Almourol is one of the more emblematic and cenographic medieval military monuments of the reconquest, and the best representation of the influence of the Knights Templar in Portugal. Located on a small islet in the middle of the Tagus River, in Vila Nova da Barquinha, in the centre region of the country. The castle was conquered in 1129 and it was part of the defensive line controlled by the Knights Templar, and a stronghold used during the Portuguese reconquest.
In the scene, at right, is visible the strong path of planet Venus, also reflected in the calm water of the river.
Canon 50D – ISO500 f/4.5 10mm Exp.20″ in 30-04-2012. Sum of 161 images taken between 21h31 and 22h59, in a total time integration of about 54 minutes.
Canon 50D – ISO500 f/4.5 10mm Exp.20″ in 30-04-2012 at 21h45
The Bridge Between Moon and Jupiter
Image of the Crescent Moon with only 1% of the disc iluminated by the Sun, and where it is clearly visible the Earthshine effect. Below the bridge we can see the Planet Jupiter. The image was taken from Almada, facing to Lisbon and to the 25 April bridge.
Canon 50D – ISO500 F/4.5 133mm Exp. 2″ in 22/04/2012 at 21h20
Moon and Mars above Almourol Castle
The castle of Almourol is one of the more emblematic and cenographic medieval military monuments of the reconquest, and the best representation of the influence of the Knights Templar in Portugal. Located on a small islet in the middle of the Tagus River, in Vila Nova da Barquinha, in the centre region of the country. The castle was conquered in 1129 and it was part of the defensive line controlled by the Knights Templar, and a stronghold used during the Portuguese reconquest.
In the scene, is visible the path of Moon and above it, the orange trail of planet Mars.
Canon 50D – ISO500 f/4.5 10mm Exp.15″ in 01-05-2012. Sum of 125 images taken between 00h22 and 00h57, in a total time integration of about 31 minutes.
Sunset Sky Show
View of the conjunction between Venus, Jupiter and the Crescent Moon in a strong Earthshine effect, with the 25 April Bridge, in Lisbon as a background.
Canon 50D – ISO250 f/2.8 Exp. 2″ in 25/03/2012 at 20:38 | Canon 50D- ISO250 f/2.8 Exp. 2.5″ in 25/03/2012 at 20:51
Venus and Moon Portrait
Image from Monsaraz region, one of the locations covered by the great Dark Sky Reserve area and that had the best dark sky measures in the process of Starlight validation.
Covering 3000sq km in southern Portugal the Alqueva Dark Sky Reserve is the first area in the world to be internationally certified as a Starlight Tourism Destination by the Starlight Foundation. More info at: www.darkskyAlqueva.com.
Canon 50D – ISO 500 f/5.6 20mm Exp. 20″ in 25-02-2012 at 19:12
Venus, Jupiter and Moon in the Nautical Twilight
In this image obtained in the nautical twilight, from Almada, Portugal, we can see at left, the path of planet Venus and a few degrees of the Moon, more precisely on it´s left, the path of the planet Jupiter. The photography sequence is the result of the sum of 111 images at intervals of 3 minutes between each, and for about 5 hours, from 18h45 until 00h13, when the moon disappears behind the city buildings.
Canon 50D -ISO400 20mm F/5.6 Exp.2″. Image taken in 29/01/2012
Solar Wall
This image was taken in the Serra de Sintra, near the solar wall, a rock with about 30 meters in height, where climbers usually make climbing and rappelling.
Canon 50D -ISO800 10mm F/4 Exp.25″. Image taken in 12/01/2012 at 00h44
Sintra Enigmatic View
In this image taken in the middle of the Sintra hills, we can see through the branches of trees many stars, below left, the bright star is the planet jupiter, in the same vertical line, near the top left, we find the pleiades and in the oposite location, in the right corner of the image, the Polaris Star. Near the horizon, the orange bright lights come from Sintra´s Village, a UNESCO World Heritage Site, on account of its 19th century Romantic architecture.
Canon 50D -ISO800 10mm F/4 Exp.25″. Image taken in 12/01/2012 at 00h40.
Crescent Moon and Venus at the Ocean
In the image we could see the Crescent Moon in the Sagittarius constellation, and below them, 3º above the horizon, the planet Venus. The Moon shows a strong Earthshine effect, for being just 9% directly iluminated by the Sun. The image was taken in Costa da Caparica beach, facing the Atlantic Ocean.
Canon 50D- ISO640 f/2.5 Exp. 3.2″ 50mm lens in 27/11/2011 at 18h25.
Sintra Village Moonset
Image of the Crescent Moonset, behind the Sintra Village. Located in the the region of Lisbon, Portugal, the village is a UNESCO World Heritage Site, on account of its 19th century Romantic architecture.
Canon 50D -ISO640 16mm F/8 Exp.5s. Sum of 57 images, in a total integration of 5 minutes. Image taken in 29/10/2011 at 19h30.
Draconids Shower
In Portugal with the moon almost full, the Draconids outburst was very faint, altough, I have registered a few meteors that escaped from the light of the moon.
Image taken from Arrábida Mountain range, in Setúbal, Portugal. 08-10-2011 at 21h11.
Canon 50D -ISO640mm 10mm F/4 Exp.30s
Above – Zoomed image
Mountain Starlight
In Portugal with the moon almost full, the Draconids outburst was very faint, altough, I have registered a few meteors that escaped from the light of the moon.
Image taken from Arrábida Mountain range, in Setúbal, Portugal. 08-10-2011between 20h52 and 22h08. Total sum of 142 images.
Canon 50D -ISO640mm 10mm F/4 Exp.30s for each image.
Moon, Pleiades, Jupiter, Orion and Sirius
Imagem do rasto da Lua obtido no Alentejo, em Vila Boim, Elvas. Na imagem e possível ver o rasto da Lua em cima e à direita o rasto das Pleiades. No centro da imagem é visível o rasto de Orion e logo abaixo o rasto intenso de Sírius. Sensivelmente ao nível da Lua mas no extremo superior direito da imagem, podemos ver o forte rasto do planeta Júpiter por entre os ramos da árvore. Foi feita uma soma de 90 imagens perto do nascer do dia entre as 05h26 e as 06h14 de 20-09-2011. Cada imagem de 30 segundos, totalizando uma integração de 45 minutos.
Canon 50D -ISO1250 10mm F/5.6 Exp.30s por imagem.
Raining Stars
Rastos de estrelas como chuva caindo sobre um pequeno pinhal na Fonte-de-Telha. Imagem obtida na noite das Perseidas em 13-08-2011 entre as 00h14 e a 01h23. Soma de 75 imagens alternadas cada uma de 25 segundos, totalizando uma integração de 31 minutos. São visiveis diversas constelações como Cepheus, Cassiopeia, Perseus, Andromeda, Pegasus e o planeta Júpiter.
Canon 50D -ISO800mm a 12mm F/6.3 Exp.25s por cada imagem
Moon and Saturn falling in the Ocean
Rasto da Lua e do planeta Saturno a pôr-se na região do Oceano Atlântico. Imagem obtida na Fonte-de-Telha em 03-08-2011 entre as 21h38 e as 22h42. Soma de 331 imagens cada uma de 10 segundos, totalizando uma integração de 55 minutos. São visiveis diversas estrelas como Spica, Porrima, Denebola, Vindemiatrix, Alula Australis e Borealis e o Planeta Saturno.
Canon 50D -ISO400mm a 17mm F/5.6 Exp.10s por cada imagem.
The Light Surrounding the Axis
Rotação das estrelas que circundam a região da estrela polar, registado no Alentejo, em Vila Boim, em 1-07-2011 entre as 00h53 e as 04h41. Soma de 420 imagens cada uma de 30 segundos, totalizando uma integração de 3h30 minutos. São visíveis as distintas cores das estrelas de várias constelações tais como: Ursa Menor, Ursa Maior, Canes Venatici, Draco, Cepheus, Camelopardalis e ainda de Cassiopeia. Em baixo à direita imagem legendada com as principais constelações.
Canon 50D -ISO1250 10mm F/4 Exp.30s por cada imagem.
Total Lunar Eclipse 2011
Eclipse Total da Lua, visto a partir do Portinho da Arrábida. Em Portugal, a lua já nasceu eclipsada e na fase da totalidade, sendo possível ver a mudança de tom no rasto à medida que a Lua sai do cone de sombra da Terra, até ao termino do Eclipse. 15-06-2011 entre as 21h43 e as 22h49. Soma de 357 imagens cada uma de 10 segundos, totalizando uma integração de 59.5 minutos.
Canon 50D -ISO200 16mm F/5 Exp.10s por imagem.
Capuchos Crescent Moon
Lua Crescente com o disco apenas 1% iluminado. Imagem obtida nos Capuchos, em Almada. É possível ver ainda a Costa da Caparica e parte de Lisboa, assim como do Oceano Atlântico.
Canon 50D- Exp.3.2″ F/5 ISO500 a 50mm 04-04-11 20h54
Arrábida – The Vernal Equinox
Imagem do rasto das estrelas no Portinho da Arrábida, obtidas com a maior lua cheia dos últimos 18 anos, no perigeu. No céu são visíveis, as estrelas Sírius, por detrás do pico rochoso, Orion, Procyon, Capella, Castor e Pollux. Imagem obtida em 20-03-2011 entre as 23h05 e as 10h02. Soma de 254 imagens cada uma de 20 segundos, totalizando uma integração de 84 minutos.
This night time lapse photography was made during the Vernal Equinox, March 20, 2011. While the Pleiades, Orion and Sirius star, were getting down behind the Arrábida moutain range, in Portugal, the biggest Moon of the last 18 years was moving in the sky, iluminating all the scene and making a slow motion movement in the rock shadows on the sand. The Moon was also drawing the water from the Atlantic Ocean, due to gravity is noticeable the incoming tide at the end of the video, that was made between 21h30 and 01h00. This is a movie trailer from the “Arrábida Nightscape Project”, by Miguel Claro and Emanuel Magessi Lopes. A special thanks to local assitant, Paulo Lourenço.
Canon 50D -ISO640 10mm F/4.5 Exp.20s por imagem.
Panoramic Full Moon
Panoramic Full Moon image when was at perigee, or closest orbital zone of planet Earth. This was the biggest full moon of the last 20 years, 14% bigger and 30% brighter. The images were obtained at Cape Espichel, Sesimbra, on 19-03-2011.Canon 50D – ISO800 15mm F/6.3 Exp. 25″ às 20:07
Canon 50D – ISO800 15mm F/6.3 Exp. 25″ às 20:07
Jupiter and Crescent Moon
Jupiter e a Lua em fase Crescente junto ao Oceano Atlântico. Imagem obtida na zona da Nato, na Fonte-de-Telha.
Canon 50D -ISO1600 20mm F/5.6 Exp.13s
Star Motion in the Park of the Peace
Imagem do rasto das estrelas na região sudoeste do céu, obtida no Parque da Paz, um refúgio da natureza localizado no meio da cidade de Almada. Imagem obtida em 27-02-2011 entre as 22h22 e as 00h29. Soma de 234 imagens cada uma de 30 segundos, totalizando uma integração de 117 minutos.
São visíveis várias estrelas e respectivas constelações: Logo à esquerda o rasto mais brilhante é da estrela Sírius, seguindo-se logo à direita os rastos da estrelas de Orion, que atravessam o primeiro conjunto rochoso vertical. Logo acima de Orion é ainda visivel o rasto de Procyon e mais à frente em baixo, destaco o rasto das conhecidas Pleiades. Finalmente no canto superior direito, a estrela Capella, com uma tonalidade alaranjada e inconfundível. O rasto rectilíneo inferior que atravessa a imagem, é de alguns aviões que ali passaram.
Canon 50D -ISO500 10mm F/5.6 Exp.30s por imagem.
Moonlit Trees and a Starry Cloudy Sky
Imagens da Lua na fase quase cheia, iluminando as paisagens com uma luz tão intensa que quase parece de dia. Na imagem vertical obtida num pinhal na Fonte-de-Telha podemos ver algumas estrelas brilhantes por entre os ramos de um pinheiro, destacando a Estrela Sírius e a constelação de Orion, totalmente visivel ao centro da imagem e por entre os ramos do pinheiro. Na imagem Horizontal em baixo, é possível observar uma bonita formação de nuvens e à esquerda são visíveis as Pleiades.
Canon 50D – ISO640 10mm F/4 Exp. 15″ 15-02-11 22:16/23:39
Crescent Moon and Earthshine
Imagem da Lua em fase Crescente, com apenas 3% do disco iluminado e onde é visível um forte Earthshine lunar, tornando visível a parte da Lua que nesta fase não se encontra directamente exposta aos raios solares, mas que se torna visível devido à luz reflectida na sua superfície, pelo próprio planeta Terra, que ilumina assim a parte escura da Lua, claramente visível, nesta imagem obtida no Feijó, Almada, em 04-02-2011 às 18h50.
Imagem above: Canon 50D -ISO400 300mm F/5.6 Exp. 2.5″ às 18:50
Image above: Canon 50D -ISO800 300mm F/5.6 Exp. 2″ às 18:58
Crescente Moon and Venus Star Party
Lua Crescente e Vénus na Lagoa de Albufeira, no início da noite de uma Star Party.
Canon 50D-ISO250 50mm F/2 Exp.13s em 11-09-10 20:50
Light Trails in the Forest
Imagem do rasto das estrelas na região Sul do céu, na zona da Via Láctea. Imagem obtida num pinhal da Fonte-de-Telha, na noite das Perseidas, em 13-08-2010 entre as 00h15 e a 01h11am. Soma de 104 imagens cada uma de 30 segundos, totalizando uma integração de 52 minutos. São visíveis várias estrelas. Os rastos no centro inferior da imagem entre os pinheiros, pertencem à constelação de Sagittarius.À direita da imagem, logo por cima da ultima árvore, verticalmente, é possível ver o rasto subtil de um meteoro das perseidas.
Canon 50D -ISO1250 10mm F/4 Exp.30s por cada imagem.
Alinhamento entre Saturno, Marte, Vénus e Lua
Alinhamento entre os planetas Saturno, Vénus, Marte e a Lua. Mercúrio não é visível na imagem por já estar demasiado baixo no horizonte. Imagem obtida na Costa da Caparica.
Canon 50D- Exp.13″ F/5.6 ISO400 20mm 12-08-10 21h3
