-
parts of
Deuteronilus Mensae do
indeed contain ice. It is now
widely believed that ice ac****ulated in many
areas of Mars,
including Deuteronilus Mensae...
- dichotomy. The
Martian dichotomy boundary includes the
regions called Deuteronilus Mensae,
Protonilus Mensae, and
Nilosyrtis Mensae. All
three regions have...
- program. CTX
Context image of
Deuteronilus Mensae showing location of next two images.
Eroded terrain in
Deuteronilus Mensae, as seen by HiRISE, under...
-
Vastitas Borealis, and
Terra Sabaea. The
Ismenius Lacus quadrangle contains Deuteronilus Mensae and
Protonilus Mensae, two
places that are of
special interest...
-
complex geologic history of
parts of Isidis,
especially areas near the
Deuteronilus contact. This
contact is the
supposed edge of a vast
Martian ocean. The...
- This year two
groups of
hills on Mars were
named (Ariadnes
Colles and
Deuteronilus Colles). As of May 2015, 43 such
groups are named: 22 on Mars, 16 on...
-
widely believed to be
caused by
glacial movement.
Areas on Mars
called Deuteronilus Mensae and
Protonilus Mensae contain many
examples of
concentric crater...
-
found in
Mamers Valles, a
channel found along the
dichotomy boundary in
Deuteronilus Mensae. They may be an easy way for ****ure
colonists of Mars to find...
-
around Mars
except through the
Tharsis volcanic region. The lower, the '
Deuteronilus',
follows the
Vastitas Borealis formation. A
study in June 2010 concluded...
- the mid-latitudes of the
planet Mars. It was
first investigated in the
Deuteronilus Mensae (Ismenius
Lacus quadrangle) region, but it
occurs in
other places...
