Hale Crater

Scaled Image

Image Credit: NASA/JPL/ASU

About this image

This VIS image shows part of the floor of Hale Crater. The mountains in the image are part of the elongated central peak of the crater. It is believed that Hale Crater was formed by an oblique impact, which caused its more oval form and central peak elongation.

Please see the THEMIS Data Citation Note for details on crediting THEMIS images.

Context

Image ID:

V66105007 (View data in Mars Image Explorer)

Latitude: -35.5732

Longitude: 323.646

Orbit Number: 66105

Captured: 2016-11-07 23:04

Posted to Web: Fri, 2016-12-16

Instrument: VIS

Image Width: 512 pixels (18 km)

Image Height: 1824 pixels (63 km)

Vertical Resolution: 0.034752 km/pixel

Horizontal Resolution: 0.0352408 km/pixel

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