| Risultati della ricerca nelle immagini - "Region" |
04-C_Mars03_Mountains.jpgMars Mountains79 visiteContrary to some reports, the phototelevision cameras on Mars-3 were functional after the dust storm subsided, in December. At least four photographic surveys have been reported (December 12 and 14, February 28 and March 12). Images were returned by pulse-code modulation over the decimeter-band telemetry channel, after the centimeter-band pulse-position modulation system failed.
The decimeter transmitter suffered from intermittant failures and was used very cautiously. Only after important science data was gathered, a small number of images at LR were transmitted (using a 256-line mode). The color image of Mars (picture n. 1) is a composite from the 52 mm camera, using its program of cycling red, green and blue glass filters.
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094-PolarSite.jpgSouth Polar Winter53 visiteUn'immagine "virtuale" NASA che avrebbe dovuto rappresentare un'area del Polo Sud di Marte la quale fosse idonea per un landing.
Ovviamente noi non abbiamo idea se la superficie di Marte nella sua Regione Sud-Polare sia simile a quanto ipotizzato dalla NASA in questo frame o no, ma una cosa è certa: il frame NASA è errato dal punto di vista della luminosità apparente del paesaggio il quale, sempre secondo i loro Scienziati, dovrebbe essere cupo e molto polveroso.
Noi siamo intervenuti solo sulla luminosità, abbattendola.MareKromium
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62-smart-1_data1002887_016_H.jpgSmall craters53 visitenessun commento
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63-smart-1_data1002887_024_H.jpgHeavily cratered Lunar Region54 visitenessun commento
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APOLLO 16-4136-A.jpgAS 16-4136 - Cratered Region near Mandel'shtam (1)53 visiteThis view looks southward near Mandel'shtam on the Lunar Far-Side. Most young lunar craters wider than about 40 Km have flows on their rims that resemble lava flows or mud flows on Earth. The unnamed crater near the top is about 14 Km wide and was recognized by H. J. Moore (1972) as being the smallest crater known to have such flows. Flows in the middle of the picture surged downhill off the high rim of the crater making lobes and tongues and leaving behind drained channels with levees.
In the area to the right of the crater, enlarged in the next frame, are some thin lobate flows that apparently rode over small hills, as if these flows were propelled outward from the crater with sufficient velocity to climb the hills. Ejecta deposits farther than about 1 Km from the rim are radially lineated and are smoother than the ground immediately surrounding the crater. The crisp, blocky zone around the crater is typical of many fresh craters.
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APOLLO 16-4136-B.jpgAS 16-4136 - Cratered Region near Mandel'shtam (2)53 visiteThis enlarged view of part of frame AS 16-4136 shows some of the smooth flows that originate near the crest of the crater rim at the left side of photograph. Arrows point to the lower ends of two flows.
The origin of the flow material is controversial.
It was probably molten material generated by shock-wave compression of lunar rocks and ejected at relatively low velocities during the late stages of the formation of the impact crater; or it may have resulted from the flow of rock debris mixed with a fluidizing agent such as gas or water; or it may have been volcanically generated lava.
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APOLLO_12_AS_12-50-7438-1.jpgAS 12-50-7438 - Lunar Terminator (True Colors; credits: Dr Marco Faccin)96 visitenessun commentoMareKromium
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APOLLO_13_-_AS_13-60-8648-PCF-LXTT.jpgAS 13-60-8648 - The "Mare Moscoviense" (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)338 visiteImage Collection: 70mm Hasselblad
Mission: Apollo 13
Magazine: 60
Magazine Letter: L
Latitude (centered): approx. 24° North
Longitude: approx. 144° East
Film Type: SO-368
Film Width: 70 mm
Film Color: color
Feature(s): Mare Moscoviense RegionMareKromium
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Acheron_Fossae-PIA13604.jpgAcheron Fossae (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)112 visiteOrbit Number: 38929
Latitude (centered): 38,754° North
Longitude (East): 224,903°
Instrument: VIS
Captured: September, 23rd, 2010
Mars Local Time: 18:09 (late afternoon)MareKromium
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Acidalia_Planitia-Unusual_Landforms-M0300102-PCF-LXTT-00.jpgUnusual Landforms in Acidalia Planitia (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)134 visitenessun commentoMareKromium
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Acidalia_Planitia-Unusual_Landforms-M0300102-PCF-LXTT-01.jpgUnusual Landforms in Acidalia Planitia (EDM n.1 - Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)141 visitenessun commentoMareKromium
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Acidalia_Planitia-Unusual_Landforms-M0300102-PCF-LXTT-02.jpgUnusual Landforms in Acidalia Planitia (EDM n.2 - Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)132 visitenessun commentoMareKromium
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