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Danu Montes and Lakshmi Planum (possible Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)
Southwest Lakshmi Planum is bounded on the South by the Danu Montes. 

Lakshmi Planum is an elevated plateau plain that is bounded on all sides by mountain chains. Here, the Danu Mountains have an angular fractured appearance. Chasms slice diagonally across the mountains in the lower left (South-West) corner of the image. Because of the steep slopes and the local relief of the mountains of several kilometers (2-3 miles, these fault-bounded troughs appear to zig-zag through the mountains when, in fact, they are probably straight if viewed from above. 

The radar view provides a perspective that would place the viewer's eye to the right, 27° above the Horizon. Thus, slopes facing to the right can be seen completely, though dark, and slopes facing away to the left appear shortened, often seen only as thin bright lines. In the center of the image is a low volcanic dome (approx. 20 Km - about 12 miles - in diameter). 
This type of volcanic feature frequently occurs on the low plains. This dome on the edge of Lakshmi is deformed and faulted where it has been affected by the forces that created the Danu mountains. 

The image is approx. 75 Km (about 46 miles) on a side. The center is at 60° North Latitude and 324,5° East Longitude.
Parole chiave: Venus from orbit - Lakshmi Planum Regio

Danu Montes and Lakshmi Planum (possible Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)

Southwest Lakshmi Planum is bounded on the South by the Danu Montes.

Lakshmi Planum is an elevated plateau plain that is bounded on all sides by mountain chains. Here, the Danu Mountains have an angular fractured appearance. Chasms slice diagonally across the mountains in the lower left (South-West) corner of the image. Because of the steep slopes and the local relief of the mountains of several kilometers (2-3 miles, these fault-bounded troughs appear to zig-zag through the mountains when, in fact, they are probably straight if viewed from above.

The radar view provides a perspective that would place the viewer's eye to the right, 27° above the Horizon. Thus, slopes facing to the right can be seen completely, though dark, and slopes facing away to the left appear shortened, often seen only as thin bright lines. In the center of the image is a low volcanic dome (approx. 20 Km - about 12 miles - in diameter).
This type of volcanic feature frequently occurs on the low plains. This dome on the edge of Lakshmi is deformed and faulted where it has been affected by the forces that created the Danu mountains.

The image is approx. 75 Km (about 46 miles) on a side. The center is at 60° North Latitude and 324,5° East Longitude.

Hestia_Rupes-PIA00469.jpg Lakhshmi_Planum-PIA00249.jpg Lakshmi_Planum-PIA00249.jpg Landslides-Navka_Region-PIA00262.jpg Montes-Akna_Montes-PCF-LXTT.jpg
Informazioni sul file
Nome del file:Lakshmi_Planum-PIA00249.jpg
Nome album:MareKromium / Venus
Valutazione (2 voti):55555(Mostra dettagli)
Parole chiave:Venus / from / orbit / - / Lakshmi / Planum / Regio
Copyright:NASA/JPL - Magellan Probe Project e Paolo C. Fienga/Lunexit Team per l'additional process. e la colorizzazione
Dimensione del file:168 KiB
Data di inserimento:Gen 11, 2010
Dimensioni:1000 x 1000 pixels
Visualizzato:55 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=26087
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