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COSMOGRAFO VELOZ
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Toma mi alma...
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WONDERFUL!
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Fotografía de la puesta de Sol tomada desde Estambul, Turquía. El tiempo de exposición es de 1/1250 segundos y 100 de ISO. Se utilizó una cámara Canon EOS 7D Mark II y un objetivo Canon EF 100-400mm. Crédito: Ender Gökçebay. Comparte Esta Publicación: Comparte en TwitterComparte en ...
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Saturn's Rings in Infrared
This mosaic of Saturn's rings was acquired by Cassini's visual and infrared mapping spectrometer instrument on Sept. 15, 2006, while the spacecraft was in the shadow of the planet looking back towards the rings from a distance of 2.16 million kilometers (1.34 million miles).

Data at wavelengths of 1.0 micron, 1.75 micron and 3.6 microns were combined in the blue, green and red channels to make the pseudo-color image shown here.

The brightest feature in the mosaic is the F ring, located at the outer edge of the main rings. The F ring is overexposed and appears white in this image. Of the main A, B and C rings; the C ring is the most prominent and reddish in color, becoming saturated close to the sun. The more opaque A and B rings are muddy in color and very dark in this geometry.

By contrast, the normally faint D ring, located just interior to the C ring, is quite bright and blue, indicating the presence of very small ring particles. Similarly, a narrow, green ringlet in the Cassini Division, as well as the greenish G ring and blue E ring -- located at increasing distances outside the F ring -- are predominantly composed of small particles. The faint reddish band immediately outside the F ring is likely to be an artifact caused by the extremely bright F ring.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The visual and infrared mapping spectrometer team is based at the University of Arizona where this image was produced.
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Jean-Philippe Cazard
27 de julio a las 16:48 ·
Protubérance solaire Halpha - 26/07/2016 - 16:33TU à 17:40TU
L127/635 + Daystar Quark + IR/UV-Cut ASI 174MM
Animation en meilleure résolution ici :
www.astrosurf.com/astrophoto/047577.html
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Southern Color
The Cassini spacecraft samples a bit of Saturn's southern hemisphere along with a spread of the planet's main rings.

Working outward from the planet, the C, B, and A rings are visible in this natural color image. The rings have been brightened relative to the planet to enhance their visibility.

This view looks toward the sunlit side of the rings from about 59 degrees below the ringplane. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were acquired with the Cassini spacecraft wide-angle camera on April 23, 2009 at a distance of approximately 1 million kilometers (621,000 miles) from Saturn. Image scale is 58 kilometers (36 miles) per pixel.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo.
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July 14 is 5 Imix/Imox. Those who are able to connect to the beyond, to alternate realities, are either ahead or out of their time. Ho can take you to the many worlds of Imix faster than you think, so take a measured breath before you plunge in. To survive such a trip with your mind fully intact does take a fair amount of psychic strength and stability; luckily you have Caban’s level-headed essence to ground you today as you explore different dimensions of your life, of the questions or worries you may have, or possibilities for the kind of future you want to create.
from Maya Calendar Portal
El 14 de julio es 5 IMIX / imox. Aquellos que son capaces de conectar al más allá, a realidades alternas, o son por delante o por fuera de su tiempo. Ho te puede llevar a los muchos mundos de imix más rápido de lo que crees, así que toma una medida aliento antes de que lo hagas. Para sobrevivir en este tipo de viaje con la mente totalmente intacta necesita una buena cantidad de fuerza psíquica y la estabilidad; por suerte tienes de caban de esencia a tierra hoy explorando diferentes dimensiones de tu vida, de las preguntas o preocupaciones puede Tienen, o las posibilidades para la clase de futuro que queremos crear.
Calendario Maya de portal
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#Saturn’s clouds help explore fluid dynamics, a branch of physics that studies the motion of gases and liquids.

Photo taken by +NASA's #Cassini mission.
Saturn's clouds are full of raw beauty, but they also represent a playground for a branch of physics called fluid dynamics, which seeks to understand the motion of gases and liquids.
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Bursting at the Seams
Dramatic plumes, both large and small, spray water ice out from many locations along the famed "tiger stripes" near the south pole of Saturn's moon Enceladus. The tiger stripes are fissures that spray icy particles, water vapor and organic compounds.

More than 30 individual jets of different sizes can be seen in this image and more than 20 of them had not been identified before. At least one jet spouting prominently in previous images now appears less powerful.

This mosaic was created from two high-resolution images that were captured by the narrow-angle camera when NASA's Cassini spacecraft flew past Enceladus and through the jets on Nov. 21, 2009. (For other images captured during the same flyby, see PIA11686 and PIA11687). Imaging the jets over time will allow Cassini scientists to study the consistency of their activity.

The south pole of the moon lies near the limb in the top left quadrant of the mosaic, near the large jet that is second from left. Lit terrain seen here is on the leading hemisphere of Enceladus (504 kilometers, 313 miles across).

Cassini scientists continue to study the question of whether reservoirs of liquid water exist beneath the surface of the moon. See PIA11114 and PIA08386 to learn more.

The view was obtained at a distance of approximately 14,000 kilometers (9,000 miles) from Enceladus and at a sun-Enceladus-spacecraft, or phase, angle of 145 degrees. Image scale is 81 meters (267 feet) per pixel.
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J-p Metsavainio
28 de julio de 2015 ·
The emission nebula IC 410 as an experimental 3D study.
There are a flythrough video, stereo images and more info in my blog, please have a look: http://www.astroanarchy.blogspot.fi/…/an-experimental-3d-st…

https://lh3.googleusercontent.com/…/s400…/IC410_Animated.gif
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Mmmm...really?
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Kiril Demerdjiev's profile photo
 
Здрасти много си приличаме
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Stormy...
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