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Inizio > SOLAR SYSTEM > 433-Eros: Pictures, Facts and Legends
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433-Eros From orbit: the Giant Gouge (natural colors; credits: Lunexit)
This picture was taken from NEAR on February 15, 2000, while the Spacecraft was passing directly over the large gouge that creates Eros's characteristic peanut shape. 

It is a mosaic of individual images showing features as small as 120 feet (35 meters) across. Although most of the asteroid is in shadow, we are able to see inside the gouge. Many narrow parallel troughs closely follow the shape of the gouge. Although they appear curvilinear from this view, they are most likely oriented parallel to the length of the asteroid. 
The strong lighting contrast along the terminator (the line separating day from night on Eros) makes it easy to see that most of the surface is saturated with impact craters. Inside the gouge, however, only smaller craters are present, indicating that the area within the gouge is younger than the surface along the terminator. 
This implies that the event that caused the gouge must have happened more recently than the formation of the rest of the surface of Eros.

(Mosaic of images 0126023473, 0126023535, 0126023721, 0126023783, 0126023845, 0126023907, 0126024093, 0126024155)
Parole chiave: Asteroids - 433-Eros

433-Eros From orbit: the Giant Gouge (natural colors; credits: Lunexit)

This picture was taken from NEAR on February 15, 2000, while the Spacecraft was passing directly over the large gouge that creates Eros's characteristic peanut shape.

It is a mosaic of individual images showing features as small as 120 feet (35 meters) across. Although most of the asteroid is in shadow, we are able to see inside the gouge. Many narrow parallel troughs closely follow the shape of the gouge. Although they appear curvilinear from this view, they are most likely oriented parallel to the length of the asteroid.
The strong lighting contrast along the terminator (the line separating day from night on Eros) makes it easy to see that most of the surface is saturated with impact craters. Inside the gouge, however, only smaller craters are present, indicating that the area within the gouge is younger than the surface along the terminator.
This implies that the event that caused the gouge must have happened more recently than the formation of the rest of the surface of Eros.

(Mosaic of images 0126023473, 0126023535, 0126023721, 0126023783, 0126023845, 0126023907, 0126024093, 0126024155)

20000214g.jpg 20000217b.jpg 20000217c.jpg 0-433-EROS-01.gif 19981105.jpg
Informazioni sul file
Nome del file:20000217c.jpg
Nome album:MareKromium / 433-Eros: Pictures, Facts and Legends
Valutazione (4 voti):55555(Mostra dettagli)
Parole chiave:Asteroids / - / 433-Eros
Copyright:NASA - NEAR/SHOEMAKER Mission e Lunexit per la colorizzazione ed il processing addizionale
Dimensione del file:21 KiB
Data di inserimento:Ago 08, 2008
Dimensioni:512 x 345 pixels
Visualizzato:60 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=21360
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