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Titan-Regions-Sinlap_Region-LS28_PSS_LASoderblom_VIMSRADAR20070323.jpg
Titan-Regions-Sinlap_Region-LS28_PSS_LASoderblom_VIMSRADAR20070323.jpgSinlap Region and Guabonito Crater58 visiteIn this composite image, Titan’s surface areas are correlated.
The top pair is composed by Cassini’s radar images, while the bottom pair shows Cassini’s VIMS images. Each of the four panels corresponds to an area about 200 Km wide.
The left views show the Sinlap Crater; the brown features in the bottom panel correspond to the large dune fields visible in the top panel.

The right views show the Guabonito Region situated at about 150 Km East of the Huygens Landing Site.
MareKromium
MarteARTE-05.jpg
MarteARTE-05.jpgHippo!58 visiteUna semplice roccia curiosa, la cui forma ci ricorda il "muso" di un ippopotamo mentre emerge dal..."fango marziano"!MareKromium
NGC-2244.jpg
NGC-2244.jpgNGC 2244 - The "Rosette Nebula"58 visite"...Se oltre un certo limite della Conoscenza ci può essere solo Dio, allora io credo che oltre un certo limite dell'ignoranza ci debba essere soltanto l'uomo..."

P.C. Floegers - "Conversations"
MareKromium
M-081-PIA09579.jpg
M-081-PIA09579.jpgThe M 81 Galaxy is "Pretty in Pink"58 visiteThe perfectly picturesque Spiral Galaxy known as Messier 81, or M81, looks sharp in this new composite from NASA's Spitzer (SST) and Hubble Space Telescopes (HST) and NASA's Galaxy Evolution Explorer.
M81 is a "grand design" spiral galaxy, which means its elegant arms curl all the way down into its center. It is located about 12 MLY away in the Ursa Major Constellation and is one of the brightest galaxies that can be seen from Earth through telescopes.

The colors in this picture represent a trio of light wavelengths: blue is ultraviolet light captured by the Galaxy Evolution Explorer; yellowish white is visible light seen by Hubble; and red is infrared light detected by Spitzer.
The blue areas show the hottest, youngest stars, while the reddish-pink denotes lanes of dust that line the spiral arms. The orange center is made up of older stars.
MareKromium
OPP-SOL1196-1F234369336EFF84GZP1212R0M1-1.jpg
OPP-SOL1196-1F234369336EFF84GZP1212R0M1-1.jpgDark "Streak" (context image) - Sol119658 visiteNella Cerchiatura Rossa ci appare, come ben segnalatoci dal Dr Gianluigi Barca (che ringraziamo per la costante attenzione e dedizione), un "dark streak" (o "striscia di colore scuro") la cui natura è davvero difficile - se non impossibile - da definire.

Le nostre ipotesi le troverete nel frame che segue.
MareKromium
OPP-SOL1196-1P234361359EFF8400P2629L6M1.jpg
OPP-SOL1196-1P234361359EFF8400P2629L6M1.jpgEarly morning's horizon (2) - Sol 119658 visitenessun commentoMareKromium
VDB-152.jpg
VDB-152.jpgvdB-152 - Reflection Nebula in Cepheus58 visite"...(Multa) non quia difficilia sunt non audemus, sed quia non audemus difficilia sunt..."

(Seneca)

"...Ci sono svariate imprese che noi non osiamo (affrontare) le quali non sono (in sè) difficili; ma esse, in realtà, lo diventano proprio perchè noi non abbiamo il coraggio di affrontarle..." (trad. libera)
MareKromium
SNR-N132D-PIA09604.jpg
SNR-N132D-PIA09604.jpgThe "Shock-Waves" of N132D58 visiteSupernovae are the explosive deaths of the universe's most massive stars. In death, these volatile creatures blast tons of energetic waves into the cosmos, destroying much of the dust surrounding them.
This false-color composite from NASA's Spitzer Space Telescope and NASA's Chandra X-ray Observatory shows the remnant of one such explosion. The remnant, called N132D, is the wispy pink shell of gas at the center of this image. The pinkish color reveals a clash between the explosion's high-energy shockwaves and surrounding dust grains.
In the background, small organic molecules called polycyclic aromatic hydrocarbons are shown as tints of green. The blue spots represent stars in our galaxy along this line of sight.
N132D is located 163.000 LY away in the Large Magellanic Cloud.
In this image, infrared light at 4,5 microns is mapped to blue, 8,0 microns to green and 24 microns to red. Broadband X-ray light is mapped purple. The infrared data were taken by Spitzer's infrared array camera and multiband imaging photometer, while the X-ray data were captured by Chandra.
MareKromium
SOL1232-2M235734246EFFAU00P2956M2M1.jpg
SOL1232-2M235734246EFFAU00P2956M2M1.jpgInteresting Soil... (1) - Sol 123258 visitenessun commentoMareKromium
SOL1232-2M235735230EFFAU00P2956M2M1.jpg
SOL1232-2M235735230EFFAU00P2956M2M1.jpgInteresting Soil... (5) - Sol 123258 visitenessun commentoMareKromium
OPP-SOL1214-1P235957410EFF85NOP2445L2M1.jpg
OPP-SOL1214-1P235957410EFF85NOP2445L2M1.jpgThe Inner Wall of Victoria - Sol 121458 visitenessun commento4 commentiMareKromium
OPP-SOL1213-1P235878503EFF85MYP2442L2M1.jpg
OPP-SOL1213-1P235878503EFF85MYP2442L2M1.jpgThe Inner Wall of Victoria - Sol 121358 visitenessun commentoMareKromium
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