| Piú votate - Mars in JPEG2000 |
MartianHole-0002.jpgThe "Martian Black Hole" (extra detail mgnf)72 visitePer i commenti su questo frame, Vi invitiamo a leggere l'articolo pubblicato su TruePlanets dal titolo:The “Martian Black Hole”, ovvero: una ricostruzione alternativa circa la possibile natura di un rilievo marziano inquietante…
(riesame critico del frame Mars Reconnaissance Orbiter PSP_003647_1745) - del Dr Paolo C. Fienga e di Lunar Explorer Italia.
MareKromium
(4 voti)
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Dunes-PIA14876.gifMoving Rippled Patch of Sand in Becquerel Crater (a GIF-Movie by NASA/JPL-Caltech/Univ. of Ariz./JHUAPL)201 visitenessun commentoMareKromium
(3 voti)
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Dunes-PIA14879.gifMoving Rippled Dune-Front in Hershel Crater (a GIF-Movie by NASA/JPL-Caltech/Univ. of Ariz./JHUAPL)191 visitenessun commentoMareKromium
(3 voti)
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Dunes-PIA14877-PCF-LXTT.jpgRippled Dune-Front in Hershel Crater (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)207 visiteThe Eastern Margin of a Rippled Dune located inside Herschel Crater moved an average distance of 3 meters (such as about 3 yards) between March 3rd, 2007 and December 1st, 2010MareKromium
(3 voti)
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Dunes-PIA14876-PCF-LXTT.jpgRippled Patch of Sand in Becquerel Crater (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)190 visiteA Rippled Patch of Sand in Becquerel Crater on Mars moved about 2 meters (such as about 2 yards) between November 24th, 2006 and September 5th, 2010. Becquerel Crater is located just north of the equator in the Arabia Terra region.
MareKromium
(3 voti)
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ESP_023045_1380-PCF-LXTT-00.jpgFlow Features inside Newton Crater (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)175 visitenessun commentoMareKromium
(3 voti)
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Claritas_Fossae-PIA14461-PCF-LXTT.jpgFeatures of Claritas Fossae (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)196 visiteThe Claritas Fossae Region is characterised by systems of "Graben" running mainly North-West to South-East. A Graben forms when a block of the Planet's Crust drops down between two Faults, due to extension, or pulling, of the Crust itself.
MareKromium
(3 voti)
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Crack_of_Unknown_Origin-ESP_022298_1555-GB-PCF-LXTT-01.jpgPossible Evidence of relatively recent Seismic Activity on Mars (credits for the Research and additional process.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)241 visitenessun commentoMareKromium
(3 voti)
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ESP_019997_1975_RED_abrowse-01.jpgCollapse Pit (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)118 visitenessun commentoMareKromium
(3 voti)
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ESP_019997_1975_RED_abrowse-02.jpgCollapse Pit (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)131 visitenessun commentoMareKromium
(3 voti)
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PSP_008338_1525_Erratic_Boulder-EB-LXTT-3.jpgLayers and "Monolith-like" Erratic Boulder in Uzboi Vallis (an Image-Mosaic in High-Def-3D by Elisabetta Bonora - Lunexit Team)102 visitenessun commentoMareKromium
(3 voti)
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PSP_004006_1900-Cerberus_Fossae-MF-LXTT.jpgTrough in Cerberus Fossae (RAW Natural Colors; credits for the additional process. and color.: Dr Marco Faccin - Lunexit Team)119 visiteAcquisition date: June, 4th, 2007
Mars Local Mars (M.L.T.): 15:05 (early afternoon)
Latitude (centered): 10,1° North
Longitude (East): 157,6°
Range to target site: 280,4 Km (such as 175,3 miles)
Original image scale range: 28,1 cm/pixel (with 1 x 1 binning) so objects ~84 cm across are resolved
Map projected scale: 25 cm/pixel and North is up
Map projection: EQUIRECTANGULAR
Emission Angle: 9,2°
Sun-Mars-Spacecraft (i.e.: Phase) Angle: 64,7°
Solar Incidence Angle (S.I.A.): 57 °, with the Sun about 33° above the Local Horizon
Solar Longitude: 251,1° (Northern Autumn)MareKromium
(3 voti)
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