Explanation: The mysterious blue reflection nebula found in catalogs as VdB 152 or Ced 201 really is very faint. It lies at the tip of the long dark nebula Barnard 175 in a dusty complex that has also been called Wolf's Cave. At the center of this deep and widefield telescopic view, the cosmic apparitions are nearly 1,400 light-years away along the northern Milky Way in the royal constellation Cepheus. Near the edge of a large molecular cloud, pockets of interstellar dust in the region block light from background stars or scatter light from the embedded bright star giving the the nebula its characteristic blue color. Ultraviolet light from the star is also thought to cause a dim reddish luminescence in the nebular dust. Though stars do form in molecular clouds, this star seems to have only accidentally wandered into the area, as its measured velocity through space is very different from the cloud's velocity. Another dense, obscuring dark nebula, LDN 1221, is easy to spot at the upper right in the frame, while the more colorful planetary nebula Dengel-Hartl 5 is just below center. Faint reddish emission from an ancient supernova remnant can also be traced (lower right to upper left) against the dust-rich complex in Cepheus.
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07/09/2019
Science & Technology - Astronomy picture of the day : In Wolf's Cave
06/09/2019
Science & Technology - Astronomy picture of the day : Recycling Cassiopeia A
Image Credit: X-ray - NASA, CXC, SAO; Optical - NASA,STScI
Explanation: Massive stars in our Milky Way Galaxy live spectacular lives. Collapsing from vast cosmic clouds, their nuclear furnaces ignite and create heavy elements in their cores. After a few million years, the enriched material is blasted back into interstellar space where star formation can begin anew. The expanding debris cloud known as Cassiopeia A is an example of this final phase of the stellar life cycle. Light from the explosion which created this supernova remnant would have been first seen in planet Earth's sky about 350 years ago, although it took that light about 11,000 years to reach us. This false-color image, composed of X-ray and optical image data from the Chandra X-ray Observatory and Hubble Space Telescope, shows the still hot filaments and knots in the remnant. It spans about 30 light-years at the estimated distance of Cassiopeia A. High-energy X-ray emission from specific elements has been color coded, silicon in red, sulfur in yellow, calcium in green and iron in purple, to help astronomers explore the recycling of our galaxy's star stuff. Still expanding, the outer blast wave is seen in blue hues. The bright speck near the center is a neutron star, the incredibly dense, collapsed remains of the massive stellar core.
05/09/2019
Science & Technology - Astronomy picture of the day : The Large Cloud of Magellan
Image Credit & Copyright: Alessandro Cipolat Bares
Explanation: The 16th century Portuguese navigator Ferdinand Magellan and his crew had plenty of time to study the southern sky during the first circumnavigation of planet Earth. As a result, two fuzzy cloud-like objects easily visible to southern hemisphere skygazers are known as the Clouds of Magellan, now understood to be satellite galaxies of our much larger, spiral Milky Way galaxy. About 160,000 light-years distant in the constellation Dorado, the Large Magellanic Cloud (LMC) is seen here in a remarkably deep, colorful, image. Spanning about 15,000 light-years or so, it is the most massive of the Milky Way's satellite galaxies and is the home of the closest supernova in modern times,SN 1987A. The prominent patch below center is 30 Doradus, also known as the magnificent Tarantula Nebula, a giant star-forming region about 1,000 light-years across.
Science & Technologie - Astronomie - HOJE, AUJOURD'HUI, TODAY : Triangle Lune Jupiter Antarès
Jeudi 5 septembre à la nuit tombante, la Lune, Jupiter et Antarès forment un triangle visible à l’œil nu.
Alors que la journée se termine en ce jeudi 5 septembre, recherchez sur l’horizon sud sud-ouest la Lune au premier quartier. A peu près à la même hauteur mais plus à l’est, la brillante planète Jupiter se repère facilement même avant la nuit. Ces deux astres matérialisent deux des trois sommets d’un triangle céleste remarquable et presque équilatéral.
Pour voir le troisième sommet du triangle, il faut attendre que la nuit s’installe un peu, vers 21h (heure de Paris). Vous distinguerez alors sans peine la brillante étoile orangée Antarès située dans la constellation du Scorpion, plus près de l’horizon. L’ensemble s’observe jusqu’aux environs de 22h30, heure à laquelle Antarès se couche.Notre satellite, une planète géante gazeuse et une étoile supergéante joliment colorée, voilà un joli trio à observer pour faire sa rentrée astronomique !
Stelvision
04/09/2019
Science & Technology - Astronomy picture of the day : The Spider Nebula in Infrared
Explanation: Will the spider ever catch the fly? Not if both are large emission nebulas toward the constellation of the Charioteer (Auriga). The spider-shaped gas cloud on the left is actually an emission nebula labelled IC 417, while the smaller fly-shaped cloud on the right is dubbed NGC 1931 and is both an emission nebula and a reflection nebula. About 10,000 light-years distant, both nebulas harbor young, open star clusters. For scale, the more compact NGC 1931 (Fly) is about 10 light-years across. The featured picture in scientifically-assigned, infrared colors combines images from the Spitzer Space Telescope and the Two Micron All Sky Survey (2MASS). Spitzer is celebrating its 16th year orbiting the Sun near the Earth.
03/09/2019
Science & Technology - Astronomy picture of the day : Unusual Signal Suggests Neutron Star Destroyed by Black Hole
Explanation: What created this unusual explosion? Three weeks ago, gravitational wave detectors in the USA and Europe -- the LIGO and Virgo detectors -- detected a burst of gravitational radiation that had the oscillating patternexpected when a black hole destroys a neutron star. One object in event S190814sv was best fit with a mass greater than five times the mass of the Sun -- making it a good candidate for a black hole, while the other object appeared to have a mass less than three times the mass of the Sun -- making it a good candidate for a neutron star. No similar event had been detected with gravitational waves before. Unfortunately, no light was seen from this explosion, light that might have been triggered by the disrupting neutron star. It is theoretically possible that the lower mass object was also a black hole, even though no clear example of a black hole with such a low mass is known. The featured video was created to illustrate a previously suspected black hole - neutron star collision detected in light in 2005, specifically gamma-rays from the burst GRB 050724. The animated video starts with a foreground neutron star orbiting a black hole surrounded by an accretion disk. The black hole's gravity then shreds the neutron star, creating a jet as debris falls into the black hole. S190814sv will continue to be researched, with clues about the nature of the objects involved possibly coming from future detections of similar systems.
02/09/2019
Science & Technology - Astronomy picture of the day : The Moon and Jupiter over the Alps
Image Credit & Copyright: Giorgia Hofer (Cortina Astronomical Association)
Explanation: What are those bright lights in the sky ahead? When hiking a high mountain pass in northern Italy three weeks ago, a conjunction between our Moon and the distant planet Jupiter was visible as both rose together in the southwest after sunset. The picturesque mountains in the distance are Tre Cime di Lavaredo (Three Peaks of Lavaredo), a UNESCO World Heritage Site and three of the best known mountain peaks in Italy, the Dolomites, and the entire Alps. In the foreground on the left is Locatelli Hut, a refuge for tired hikers as it is located over an hour from nearest parking lot. The bright sky object on the upper left is Saturn. The entire scene was captured on a single 8-second exposure. Jupiter and Saturn will remain prominent in the western sky after sunset this month, while the Moon, in its monthly orbit around the Earth, will pass near Jupiter again in about four days.
Science & Technologie - Aeronautique - Avions du futur : L'Aeroscraft ML 866, un dirigeable de luxe
Le dirigeable joue l'éternel retour : économique, spacieux et capable d'emporter d'énormes charges, il présente de bons atouts. Mais il a aussi quelques défauts : il est lent, difficile à manœuvrer (surtout par grand vent) et il est vraiment très encombrant. L'idée reste cependant toujours valable, notamment pour des transports de fret et pour des missions de surveillance. L'entreprise Aeros, spécialiste du domaine, a présenté un projet pour une sorte de yacht aérien de luxe, l'Aeroscraft ML 866. Son avenir est incertain mais il illustre la persistance de l'idée d'utiliser des « aéronefs » plus légers que l'air.
© Aeros
01/09/2019
Science & Technologie - Aeronautique - Avions du futur : le retour de l'hélice grâce à l'open rotor ?
Le concept de « rotor ouvert » (open rotor) est à l'étude chez plusieurs motoristes, comme Snecma (du groupe Safran). L'idée n'est pas nouvelle puisqu'elle a été testée, sous le nom de UDF (pour unducted fan), dans les années 1980... et abandonnée. Mais la voilà de nouveau sur les rails, avec l'espoir d'une réduction de la consommation de 25 %.
Comme dans un réacteur double flux actuel, la partie centrale est une turbine qui assure une poussée avec un flux d'air chaud et accéléré. Autour, une « soufflante », entraînée par cette même turbine, fonctionne un peu comme une hélice. Elle produit un flux annulaire autour du flux chaud. Le principe de l'open rotor est d'ôter le carénage du réacteur et d'installer une soufflante prenant la forme de deux propulseurs à pales contrarotatives (tournant en sens inverse).
© Snecma
Science & Technology - Astronomy picture of the day : M45: The Pleiades Star Cluster
Image Credit & Copyright: Marco Lorenzi (Glittering Lights)
Explanation: Have you ever seen the Pleiades star cluster? Even if you have, you probably have never seen it as dusty as this. Perhaps the most famous star cluster on the sky, the bright stars of the Pleiades can be seen without binoculars from even the depths of a light-polluted city. With a long exposure from a dark location, though, the dust cloud surrounding the Pleiades star cluster becomes very evident. The featured exposure took over 12 hours and covers a sky area several times the size of the full moon. Also known as the Seven Sisters and M45, the Pleiades lies about 400 light years away toward the constellation of the Bull (Taurus). A common legend with a modern twist is that one of the brighter stars faded since the cluster was named, leaving only six stars visible to the unaided eye. The actual number of Pleiades stars visible, however, may be more or less than seven, depending on the darkness of the surrounding sky and the clarity of the observer's eyesight.
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