Poslední hybridní zatmění z vesmíru:

Solar Eclipse - October 2013 - YouTube
http://www.youtube.com/watch?v=RvctRZz2yjQ


Solar eclipse 3.11. 2013 from russian satellite Elektro-L - YouTube
http://www.youtube.com/watch?v=wzfj-l0669Y

zajimave:

RETROSPEKTIVNÍ VÝSTAVA PROJEKTŮ "VESMÍRNÉHO ARCHITEKTA" DAVIDA NIXONA
ve čtvrtek 7. 11. 2013 v Galerii NTK

[ GUMAGUAR @ ex~hibit ~~~ ex~po ]

M78, NGC2068 | Kitt Peak National Observatory
M78 is part of the Orion complex, a large region of star-forming gas and dust centered around M42 and M43.
It is the brightest diffuse reflection nebula in the sky, and fairly easy to see with binoculars (and almost
visible to the naked eye, claim some observers). M78 is some 1600 light-years away and around 4 light-years
across. Other parts of this giant molecular cloud have their own labels: NGC2071 to the northeast (upper left),
NGC2067 in close to the northwest (upper right) and NGC2064 (faint, southwest, lower right), as well as other
pieces not in this picture. The present picture is a color composite mosaic of CCD images from the 0.9-meter
telescope of the Kitt Peak National Observatory, near Tucson, Arizona, taken in November 1998.
Image size 22.1x28.3 arc minutes.

Iris Nebula NGC 7023 | Kitt Peak National Observatory
This image was obtained with the wide-field view of the Mosaic Camera on the Mayall 4-meter telescope at Kitt Peak National Observatory
on August 29th, 2009. NGC 7023, also known as the Iris Nebula because of its flower-like shape, is a bright reflection nebula. The bluish
glow of the nebula comes from a hot, massive star at the center of the nebula, named HD 200775. Blue light from the star is scattered off
dust grains in the nebula, giving it its distinctive color. The dust can also be seen on the outer portions of the nebula, where it has a
faint brownish color and blocks out stars behind it. It was observed in the filters B (blue), V (green), R (orange) and Hydrogen-Alpha (
red). The image is rotated 30 degrees CCW from North is up, East is to the left.

The Hockey Stick Galaxy
This image was obtained with the wide-field view of the Mosaic camera on the Mayall 4-meter telescope at Kitt Peak National Observatory.
NGC 4656, also known informally as the "hockey stick galaxy," is a distorted edge-on spiral galaxy. Its distinctive shape is due to a recent
gravitational interaction with the galaxy NGC 4631. It is not yet certain, but these two galaxies may be in the early stages of merging. The
faint object in the upper-left corner may not be part of the galaxy, but instead be a dwarf galaxy in the process of merging with NGC 4656.
The image was generated with observations in the B (blue), V (green), I (orange) and Hydrogen-Alpha (red) filters. In this image, North
is up, East is to the left.

The Ghost Nebula
This image was obtained with the wide-field view of the Mosaic Camera on the Mayall 4-meter telescope
at Kitt Peak National Observatory. vdB 141 is a reflection nebula located in the constellation Cepheus.
Sometimes referred to as the ghost nebula, its awkward name is its catalog number in Sidney van den
Bergh's catalog of reflection nebulae, published in 1966. Several stars are embedded in the nebula. Their
light gives it a ghoulish brown color. North is down and East is to the right. Imaged August 28, 2009.

Part of the constellation Scorpius centred on NGC 6357 which has star cluster Pismis 24 in its centre.
This image is a colour composite taken by the Digitized Sky Survey (DSS), the field of view is 3.8x3.3 degrees.