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ESP_024227_1595-2.jpg
ESP_024227_1595-2.jpgUnnamed Crater in Ladon Valles (Absolute Natural Colors; credits for the additional process. and color.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)218 visiteMars Local Time: 14:25 (Early Afternoon)
Coord. (centered): 20,5° South Lat. and 330,0° East Long.
Spacecraft altitude: 260,9 Km (such as about 163,1 miles)
Original image scale range: 52,2 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 57 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 1,3°
Sun-Mars-Spacecraft (or "Phase") Angle: 41,6°
Solar Incidence Angle: 43° (meaning that the Sun is about 47° above the Local Horizon)
Solar Longitude: 6,8° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Drr Gianluigi Barca and Paolo C. Fienga - Lunar Explorer Italia
MareKromium
ZZ-Mercury-Craters-Unnamed_Crater_with_Hollows-PIA15069-PCF-LXTT.jpg
ZZ-Mercury-Craters-Unnamed_Crater_with_Hollows-PIA15069-PCF-LXTT.jpgUnnamed Crater with "Hollows" in Caloris Basin (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)218 visiteThis stunning, and as of yet Unnamed, Crater lies within the Caloris Basin. Its fFoor provides another example of the beautiful "Hollows" found on Mercury and has an etched appearance similar to that found in the Crater Tyagaraja. This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's Surface at resolutions much higher than the 250-meter/pixel (820 feet/pixel) morphology base map or the 1-kilometer/pixel (0,6 miles/pixel) color base map. It is not possible to cover all of Mercury's Surface at this high resolution during MESSENGER's one-year mission, but several areas of high scientific interest are generally imaged in this mode each week.

Date acquired: October, 28th, 2011
Image Mission Elapsed Time (MET): 228326267
Image ID: 943690
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 38,44° North
Center Longitude: 175,6° East
Resolution: 42 meters/pixel
Scale: this Unnamed Crater is approximately 38 Km (about 24 miles) across
Solar Incidence Angle: 76,1° (meaning that the Sun, at the time the picture was taken, was about 13,9° above the Local Horizon)
Emission Angle: 40,0°
Sun-Mercury-MESSENGER (or "Phase") Angle: 116,1°
MareKromium
ESP_024074_1425-PCF-LXTT-01.jpg
ESP_024074_1425-PCF-LXTT-01.jpgFeatures of Electris Region (CTX "B" - Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 218 visiteMars Local Time: 14:27 (Early Afternoon)
Coord. (centered): 37,1° South Lat. and 189,4° East Long.
Spacecraft altitude: 255,3 Km (such as about 159,6 miles)
Original image scale range: 25,5 cm/pixel (with 1 x 1 binning) so objects ~ 77 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 6,3°
Sun-Mars-Spacecraft (or "Phase") Angle: 46,6°
Solar Incidence Angle: 51° (meaning that the Sun is about 39° above the Local Horizon)
Solar Longitude: 0,9° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromium
ESP_011337_2360-PCF-LXTT.jpg
ESP_011337_2360-PCF-LXTT.jpgUnnamed Fresh Northern Crater (CTX in Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team - Inset: credits: NASA/JPL-Caltech-Univ. of Arizona)218 visiteMars Local Time: 15:29 (Early Afternoon)
Coord. (centered): 55,6° North Lat. and 150,6° East Long.
Spacecraft altitude: 311,4 Km (such as about 194,6 miles)
Original image scale range: 31,3 cm/pixel (with 1 x 1 binning) so objects ~ 93 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 7,7°
Sun-Mars-Spacecraft (or "Phase") Angle: 77,2°
Solar Incidence Angle: 70° (meaning that the Sun is about 20° above the Local Horizon)
Solar Longitude: 180,6° (Northern Fall)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromium
ESP_024475_2650-PCF-LXTT-01.jpg
ESP_024475_2650-PCF-LXTT-01.jpgFeatures of the North Polar Erg (CTX Frame "B" - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)218 visiteMars Local Time: 12:27 (early afternoon)
Coord. (centered): 84,7° North Lat. and 0,8° East Long.
Spacecraft altitude: 320,7 Km (such as about 200,4 miles)
Original image scale range: 64,2 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 92 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: POLAR STEREOGRAPHIC
Emission Angle: 0,1°
Phase Angle: 78,0°
Solar Incidence Angle: 78° (meaning that the Sun is about 12° above the Local Horizon)
Solar Longitude: 16,1° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium
SOL520-2N172517486EDNABAKP1585L0M1-PCF-LXTT.jpg
SOL520-2N172517486EDNABAKP1585L0M1-PCF-LXTT.jpgLate Morning on Mars - Sol 520 (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)218 visiteLeft Navigation Camera Non-linearized Downsampled EDR acquired on Sol 520 of Spirit's mission to Gusev Crater at approximately 10:15:32 Mars Local Solar Time.MareKromium
ESP_024997_1155_RED-PCF-LXTT-01.jpg
ESP_024997_1155_RED-PCF-LXTT-01.jpgSouthern Dunefield partially covered with Frost (CTX Frame "B" - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)218 visiteCoord. (centered): 64,2° North Lat. and 194,5° East Long.MareKromium
ESP_024421_1530-PCF-LXTT-00.jpg
ESP_024421_1530-PCF-LXTT-00.jpgLayered Features inside Terby Crater (CTX Frame "A" - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)218 visiteCoord. (centered): 27,1° South Lat. and 75,0° East Long.MareKromium
101955-Bennu-011.png
101955-Bennu-011.png101955 Bennu - Just like Itokawa (Natural Colors; credits for the additional process. and color.: E. Bonora & Marco Faccin)218 visiteNotate la posizione "anomala" e "sporgente" dei mega-boulders (mega-macigni) visibili. Bizzarro, vero?!? La "causa" della nascita di 101955 Bennu? Aggregazione Gravitazionale di detriti. Così come Itokawa. Asteroidi fragili, polverosi e senza crateri. Ere di "lavoro" (miliardi di anni terrestri) e questo ne é un (altro esempio di) risultato.MareKromium
APOLLO 11 AS 11-37-5525.jpg
APOLLO 11 AS 11-37-5525.jpgAS 11-37-5525 - Red Anomaly (7)217 visiteLa "caccia" (fotografica) alla sfera rossa continua - almeno così pensiamo - ma, purtroppo, gli astronauti non sono fortunati e non riescono a riprenderla. Si vede chiaramente l'ombra della Bandiera. Non c'è traccia di ombre anomale.
APOLLO 11 AS 11-40-5869.jpg
APOLLO 11 AS 11-40-5869.jpgAS 11-40-5869 - Going down the ladder (5)217 visite..."artefatta" è molto diversa da queste ed avremo occasione di vederne alcune (AS 11-40-5881HR e svariati frames delle Missioni Apollo 16 e 17). Una precisazione: quando parliamo di foto "falsa/alterata" noi non intendiamo nè implichiamo che essa NON sia stata scattata effettivamente sulla Luna.
Noi intendiamo ed implichiamo che essa potrebbe essere stata "manipolata" DOPO.
Quando? In sede di sviluppo, per esempio.
AA-Anomaly - Saturn_s Sky from Cassini-Huygens.jpg
AA-Anomaly - Saturn_s Sky from Cassini-Huygens.jpgA bright light in the Space of Saturn: Saturn overexposed (1)217 visiteMa adesso che ci troviamo nello Spazio Esterno; che non c'è nessuna atmosfera di sorta da chiamare in causa e non ci sono neppure vecchie Sonde che possono precipitare ed alle quali si potrebbe "dare la colpa" per la presenza di "strisce di luce nel cielo", che cosa si inventeranno le Agenzie Spaziali per negare ancora l'evidenza?
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