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Sign of the zodiac: the sagittarius (Astrological sign: sagittarius) Private collection
The Lactee Way and the Sagittarius - Part of the Sagittarius constellation - The lactee path and the “theiere” in the Sagittarius. The milky way and the “” teapot””” in Sagittarius
Lactee route in Sagittarius and Scorpio - Milky way in Sagittarius and Scorpiu
Sagittarius, 2007 (oil on belgian linen)
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The Lactee Way and the Sagittarius - Part of the Sagittarius constellatio
Sagittarius serpentarius/Sagittarius messenger/Serpentary/Secretary Bird
The constellation Sagittarius.
Sagittarius serpentarius
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Sagittarius serpentarius/Sagittarius messenger/Serpentary/Secretary Bird
Sagittarius serpentarius/Sagittarius messenger/Serpentary/Secretary Bird
Nebula Omega (M17) in Sagittarius - The Omega Nebula (M17) in the constellation Sagittarius - View of the nebula Omega (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. The Omega Nebula, Messier object 17 (M17), NGC 6618, in the constellation Sagittarius is a bright nebula, criss - crossed by clouds and lanes of opaque dust and gas. It is also known as the Swan Nebula and the Horseshoe Nebula. At a distance of 5700 light - years, M17 is also a source of radio noise
SAGITTARIUS (ROSSUM)
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Nebulae IC 1283 - 84 and NGC 6589 - 90 in Sagittarius - Nebulosity in Sagittarius, NGC 6589 - 90 - These nebulae are located in Sagittarius at a distance of about 5900 light years from Earth. Image made with Siding Spring's 3.9m telescope. Our view towards the centre of the Galaxy is obscured by extensive clouds of interstellar dust in the direction of the constellation of Sagittarius. The large - scale, patchy nature of the obscuration can be seen with the unaided eye and it is evident on smaller scales from the uneven distribution of background stars across this picture. Light from bright stars within the dust produces the two blue reflection nebulae (NGC 6589 and 6590), and these stars are members of a loose open cluster of stars, NGC 6595 (Sharpless 37) which is at a distance of about 5,900 light years. A large, almost transparent cloud of hydrogen, mixed with traces of dust, glows with a characteristic magenta hue over most of the field of view. This is known as IC 1283, 1284 and 4700 and is likely at a similar distance to NCC 6595
Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. This object derives its name from its looped shape reminiscent of the Greek letter when the nebula is seen in a telescope. The gas cloud is unusual in that it does not appear to be illuminated by the bright stars that commonly found in emission nebulae such as this. However, the nebulosity is very bright, so the exciting stars must be hidden within the cloud, an idea confirmed by the infrared brightness of the nebula. It is about 6000 light years distant
Horoscope: the sign of the sagittarius.
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Horoscope: the sign of sagittarius.
ZODIAC/SAGITTARIUS/MAXIM
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Sagittarius - Astrology (fresco)
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Sagittarius, 1999 (gouache on paper)
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Sagittarius (w/c on paper)
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Sagittarius serpentarius/Snake
Sagittarius serpentarius/Snake
The constellation of Sagittarius, 1488
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Jupiter in Sagittarius (fresco)
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The Sagittarius, 1893 (illustration)
The constellation Sagittarius, 1603
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Lactee route in Sagittarius - Scutum, parts of Ophiuchus, Sagittarius and the galactic bulg
Globular cluster M55 in Sagittarius - globular star cluster Messier 55 - Star cluster located about 17,000 years ago - light from Earth. Infrared image obtained by the Vista telescope. This striking view of the globular star cluster Messier 55 in the constellation of Sagittarius (The Archer) was obtained in infrared light with the VISTA survey telescope at Eso's Paranal Observatory in Chile. This vast ball of ancient stars is located at a distance of about 17,000 light - years from Earth
Galactic Center Region - The Galactic Center - The Galactic Center Region of the center of our galaxy seen the Chandra, Spitzer and Hubble satellites. The galactic center (Sagittarius A*) is located in the white area in the middle to the right of the image. In yellow, near-infrared images obtained by the Hubble Space Telescope; in red, infrared images obtained by the Spitzer Space Telescope; in blue and purple, X-ray observations obtained by the Chandra Space Telescope. Nasa's Great Observatories - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory - have collaborated to produce an unprecedented image of the central region of our Milky Way galaxy. In this spectacular image, observations using infrared light and X-ray light see through the obscuring dust and reveal the intense activity near the galactic core. Note that the center of the galaxy is located within the bright white region to the right of and just below the middle of the image. The entire image width covers about one-half a degree, about the same angular width as the full moon. Each telescope's contribution is presented in a different color: - Yellow represents the near-infrared observations of Hubble. These observations outline the energetic regions where stars are being born as well as reveal hundreds of thousands of stars. - Red represents the infrared observations of Spitzer. The radiation and winds from stars create glowing dust clouds that exhibit complex structures from compact, spherical globules to long, stringy filaments. - Blue and violet represent the X-ray observations of Chandra. X-rays are emitted by gas heated to millions of degrees by stellar explosions and by outflows from the supermassive black hole in the galaxy's center. The bright blue blob on the left side is emission from a double star system containing either a neutron star or a black hole. When these views are brought together, this composite image provides one of the most detailed
Globular cluster Terzan 5 in Sagittarius - Globular cluster Terzan 5 in Sagittarius - The globular cluster Terzan 5 is located in the constellation Sagittarius. Its stars are not all at the same time and show great age differences between 6 and 12 billion years. Image obtained by the Hubble Space Telescope (HST). Deep within the Milky Way lies the ancient globular cluster Terzan 5. This NASA/ESA Hubble Space Telescope image shows the cluster in wonderful detail, but it is the chaotic motions of its stars that make it particularly interesting to astronomers. Terzan 5 has an exceptionally dense core. As a result, it is thought to have one of the highest stellar collision rates for a globular cluster. And packed in at such close quarters, many stars are pushed so close together that they form tight binary systems. Interestingly, studies of individual stars within the cluster reveal that they can be split into two age groups: 6 and 12 billion years old. Some astronomers have hypothesised that the younger crowd may have been stripped away from a dwarf galaxy
Sign of the Zodiac - Sagittarius
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ZODIAC TILE/SAGITTARIUS
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Sign of the zodiac: the sagittarius.
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Sagittarius serpentarius/Snake
Astrology - Zodiac - Sagittarius
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Zodiac sign: Sagittarius.
Sagittarius (colour litho)
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Open cluster M25 (IC 4725) in Sagittariu - Open cluster M25 (IC 4725) in Sagittariu
Globular cluster M22 in Sagittariu - Globular cluster M22 in Sagittariu
Exoplanete OGLE-2013-BLG-0341L Bb - Artist's view: OGLE-2013-BLG-0341L Bb is an exoplanet about twice the mass of the Earth gravitating around the red dwarf OGLE-2013-BLG-0341L B, a secondary component of the binary star OGLE-2013-BLG-0341L located in the constellation. OGLE-2013-BLG-0341LBB, is located in the constellation Sagittarius, about 3,000 light-years away. It is twice the mass of Earth, and orbits one of the stars in the binary system at almost exactly the same distance from which Earth orbits the Sun. But its star is 400 times dimmer than our Sun, so the exoplanet is very cold - around minus 213 degrees Celsius
Pistol star - Massive star in the constellation Sagittarius - The massive star Pistol star in Sagittarius - Pistol star is one of the most massive stars in our galaxy. Located about 25,000 years ago - the light of the Earth in the constellation of Sagittarius, this star shines like 10 million Sun consuming in six seconds as much energy as our star in a year. This star is masked by the numerous interstellar dust present in the Sagittarius near the galactic center and appears only in infrared wavelengths, as in this image obtained with the NICMOS instrument embark on the Hubble space telescope. The nebula that surrounds it (in the shape of a gun), extends over 4 years - light. Image obtained in 1997. Astronomers using Nasa's Hubble Space Telescope have identified what may be the most luminous star known “” a celestial mammoth which releases up to 10 million times the power of the Sun and is big enough to fill the diameter of Earth's orbit. The star unleashes as much energy in six seconds as our Sun does in one year. The image, taken with the Near - Infrared Camera and Multi - Object Spectrometer (NICMOS) aboard Hubble, also reveals a bright nebula, created by extremely massive stellar eruptions. The nebula is so big (four light - years) that it would almost span the distance from the Sun to Alpha Centauri, the nearest star to Earth's solar system. The astronomers estimate that when the titanic star was formed one to three million years ago, it may have weighed up to 200 times the mass of the Sun before shedding much of its mass in violent eruptions. The star, called the “” Pistol Star”” (for the pistol shaped nebula surrounding it), is approximately 25,000 light - years from Earth near the center of our Milky Way galaxy. The Pistol Star is not visible to the eye, but is located in the direction of the constellation Sagittarius, hidden behind the great dust clouds along the Milky Way
Globular cluster M54 in Sagittarius - M54, globular cluster in Sagittariu
Globular cluster M70 in Sagittarius - Globular cluster M70 in Sagittarius - Star cluster located about 29,000 years away from Earth. Image obtained by the Hubble Space Telescope (HST). The NASA/ESA Hubble Space Telescope has captured the brilliance of the compact centre of Messier 70, a globular cluster. Messier 70 orbits close to the Milky Way's center, around 30 000 light - years away from the Solar System. Messier 70 is only about 68 light - years in diameter and can be seen, albeit very faintly, with binoculars in dark skies in the constellation of Sagittarius (The Archer). This picture was obtained with the Wide Field Camera of Hubble's Advanced Camera for Surveys. The field of view is around 3.3 by 3.3 arcminutes
Globular cluster M70 in Sagittarius - Globular cluster M70 in Sagittarius - Star cluster located about 29,300 years - light from Earth. Star cluster located at about 29,000 light years away
Globular cluster M54 in Sagittariu - M54 globular cluster in Sagittariu
Globular cluster M55 in Sagittarius - Globular cluster M55 in Sagittarius - Star cluster located about 17,000 years away from Earth. Star cluster located at about 17,000 light years away
Open cluster M21 in Sagittarius - Open cluster M21 in Sagittarius - The cluster of stars M21 (NGC 6531) is composed of about sixty stars located in the constellation Sagittarius. Image obtained by the Oschin telescope of Mount Palomar through several filters and composed. The open cluster M21, or NGC 6531, in the constellation Sagittarius shows a strong central concentration and a wide range of star brightnesses, despite its limited membership of probably fewer than 60 stars. Most likely quite young (for a star cluster, that means only a few million years), its distance is uncertain. M21 is quite close on the sky to M20, the Trifid Nebula
Nebula IC 1274 in Sagittariu - Nebula IC 1274 in Sagittariu
Constellations of the Telescopium and Sagittarius - The Telescope is a small constellation of the southern hemisphere located just above Sagittarius
Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. Image obtained by the VST (VLT Survey Telescope) in Chile in June 2011. The first released VST image shows the spectacular star - forming region Messier 17, also known as the Omega Nebula or the Swan Nebula, as it has never been seen before. This vast region of gas, dust and hot young stars lies in the heart of the Milky Way in the constellation of Sagittarius (The Archer). The VST field of view is so large that the entire nebula, including its fainter outer parts, is captured - - and retains its superb sharpness across the entire image
Nebula M20 in Sagittarius - View of the nebula Trifide (M20/ngc 6514) in the constellation Sagittarius
Centre de la nebula de la Lagoon (M8) dans le Sagittarius - In the heart of the Lagoon Nebula - Centre de la nebula de la Lagoon (M8) vue par le telescope Hubble (HST). This close - up shot of the centre of the Lagoon Nebula (Messier 8) clearly shows the delicate structures formed when the powerful radiation of young stars interacts with the hydrogen cloud they formed from. This image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. Light from glowing hydrogen (through the F658N filter) is coloured red. Light from ionised nitrogen (through the F660N filter) is coloured green and light through a yellow filter (F550M) is coloured blue. The exposure times through each filter are 1560 s, 1600 s and 400 s respectively. The blue - white flare at the upper - left of the image is scattered light from a bright star just outside the field of view. The field of view is about 3.3 by 1.7 arcminutes
Irregular galaxy NGC 6822 in Sagittarius - Irregular galaxy NGC 6822 in Sagittarius - The galaxy NGC 6822 is located about 1.8 million years ago - light from Earth. She belongs to our local group. Image obtained with Siding Spring's 3.9m telescope. NGC 6822 is one of the nearest galaxies to the milky Way and is thus a member of a small cluster known as the Local Group to which our Galaxy belongs. It is close enough to be resolved into individual stars, though because of its distance (about 1.8 million light years) only the brightest are seen, even with a telescope as powerful as the AAT. The galaxy seems to be without symmetry and is classified as an irregular. At one end of a prominent bar a few clouds of glowing gas can be seen; at the other, bright bluish stars are scattered out into what appears to be the first signs of a straggling spiral arm
Star field in the constellation Sagittarius - Scattered stars in Sagittarius: Stars in Sagittarius seen by the space telescope Hubble. This stunning image, captured by the NASA/ESA Hubble Space Telescope's Advanced Camera for Surveys (ACS), shows part of the sky in the constellation of Sagittarius (The Archer). The region is rendered in exquisite detail - deep red and bright blue stars are scattered across the frame, set against a background of thousands of more distant stars and galaxies. Two features are particularly striking: the colours of the stars, and the dramatic crosses that burst from the centres of the brightest bodies. While some of the colours in this frame have been enhanced and tweaked during the process of creating the image from the observational data, different stars do indeed glow in different colours. Stars differ in colour according to their surface temperature: very hot stars are blue or white, while cooler stars are redder. They may be cooler because they are smaller, or because they are very old and have entered the red giant phase, when an old star expands and cools dramatically as its core collapses. The crosses are nothing to do with the stars themselves, and, because Hubble orbits above Earth's atmosphere, nor are they due to any kind of atmospheric disturbance. They are actually known as diffraction spikes, and are caused by the structure of the telescope itself. Like all big modern telescopes, Hubble uses mirrors to capture light and form images. Its secondary mirror is supported by struts, called telescope spiders, arranged in a cross formation, and they diffract the incoming light. Diffraction is the slight bending of light as it passes near the edge of an object
Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. This object derives its name from its looped shape reminiscent of the Greek letter when the nebula is seen in a telescope. The gas cloud is unusual in that it does not appear to be illuminated by the bright stars that commonly found in emission nebulae such as this. However, the nebulosity is very bright, so the exciting stars must be hidden within the cloud, an idea confirmed by the infrared brightness of the nebula. As well as exciting the nebula we can see, the embedded stars heat the dust that surrounds them, so M17 is one of the brightest objects in the infrared sky. It is about 6000 light years distant
The Sagittarius (the archer), 1927 (print)
Horoscope: sign of the zodiac, the Sagittarius.
Exoplanete SWEEPS-10: SWEEPS-10 is an exoplanet located towards the galactic center. This hot jupiter is one of the hottest exoplanets discovered to date with a temperature of 1650 degres. SWEEPS-10 is an extrasolar planet orbiting the star SWEPS J175902.00 291323.7 located in the Galactic bulge at a distance of approximately 22,000 light years from Earth. It completes an orbit of its star in just 10 hours, and is categorized as an ultra-short period planet (USPP). Located only 1.2 million kilometers from its star, the planet is among the hottest ever detected; its estimated temperature is approximately 1,650 degrees Celsius. This planet must be at least 1.6 times the mass of Jupiter
The lactee route in the region of Sagittarius. - The lactee route in the region of Sagittarius. Image obtained in Chile
Nebula NGC 6559 in Sagittarius - Nebula NGC 6559 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth
Sagittarius 1967 (Acrylic on canvas)
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