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OPP-SOL2093-GB-LXTT.jpgDark Horizon - Sol 2093 (possible True Colors; credits: Dr G. Barca - Lunexit Team)131 visitenessun commentoMareKromium
(1 voti)
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FIGURA_14.JPGReady for "Scouting"...65 visiteUn missile "Scout" pronto al lancio; da notare la doppia dicitura "USA-Italia".
MareKromium
(1 voti)
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FIGURA_12.JPGThe "Santa Rita" Platform62 visiteNotate la circostanza per cui gli helipads (o anche helidecks - e cioè le aree di landing e take-off sulla e dalla piattaforma riservate agli elicotteri) della Santa Rita sono state riadattate a sostegno per le antenne.
MareKromium
(1 voti)
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FIGURA_13.jpgThe "San Marco Platform", in 199559 visiteDa non dimenticare che il 1995 è stato l'anno del rinnovo dell'accordo Italia - Kenya, relativo al mantenimento ed al'impiego del "Broglio Space Center" e delle altre strutture (incluse quelle terrestri) ad esso collegate.MareKromium
(1 voti)
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Hestia_Rupes-PIA00469.jpgComplex Network of Narrow Fractures near Hestia Rupes Region (possible Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)60 visiteThis is a Magellan radar image covering an about 105- Km (approx. 63-mile) by 45-Km (approx. 27-mile) Region near Hestia Rupes on the North-Western corner of Aphrodite Terra.
The complex network of narrow (such as <1 Km) Fractures in the center of the image extends for approx. 50 Km (about 31 miles). This network exhibits tributary-like branches similar to those observed in river systems on Earth. However, the angular intersections of the tributaries suggest tectonic control.
These features appear to be due to drainage of lava along preexisting fractures and subsequent collapse of the Surface. The underlying tectonic fabric can be observed in the North-East trending Ridges which predate the Plains.MareKromium
(1 voti)
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FIGURA_03.JPGLifting-up of a "Scout" missile59 visiteSollevamento di un razzo "Scout" sulla rampa della piattaforma San Marco.MareKromium
(1 voti)
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FIGURA_04.jpgLuigi Broglio59 visiteL'ingegner Luigi Broglio in Florida, in visita al John F. Kennedy Space Center di Cape Canaveral.MareKromium
(1 voti)
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Rhea-4229274308_c987cf73d9_o.jpgLarge Crater on Rhea (possible True Colors; credits: Dr M. Faccin - Lunexit Team)59 visitenessun commentoMareKromium
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OPP-SOL2091-GB.jpgCrossing and Crunching... - Sol 2091 (Natural Colors; credits: Dr G. Barca - Lunexit Team)110 visitenessun commentoMareKromium
(1 voti)
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OPP-SOL553-1P177276938EFF58D4P2353L2M1.jpgThe Sandy Waves of Meridiani - Sol 533 (Natural Color View - credits: Dr Paolo C. Fienga - Lunexit Team)83 visitenessun commentoMareKromium
(1 voti)
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OPP-SOL553-1P177276971EFF58D4P2353R2M1.jpgThe Sandy Waves of Meridiani - Sol 533 (Natural Color View - credits: Dr Paolo C. Fienga - Lunexit Team)63 visitenessun commentoMareKromium
(1 voti)
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PSP_001398_2615_RED_abrowse.jpgExposure of NPLD with "Unconformities" (Natural - but enhanced - Colors; credits: Dr Paolo C. Fienga - Lunexit Team)85 visiteThis image shows a portion of the North Polar Layered Deposits (NPLD). The NPLD are layers that have been deposited over an extensive area at both Poles, possibly throughout Martian History. They likely contain ice-rich and dust-rich layers, with the darker layers being probably more dust-rich than the bright layers.
The NPLD holds clues to past climate regimes similar to ice cores on Earth. Several of the layers occur in fairly regular sequences, as seen in this image, suggesting that Mars underwent cyclic climate changes in the past.
Towards the top left side of the image, there is a series of layers that appears truncated at an angle, forming what geologists call "Angular Uncomformity". They typically form by first laying down a series of continuous beds. Then erosion cuts through the beds at an angle. Aferwards, a new set of beds are laid over this partially eroded sequence. A similar Unconformity exists at the bottom right of the image.MareKromium
(1 voti)
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