-
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...
- 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...
- 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...
-
around Mars
except through the
Tharsis volcanic region. The lower, the '
Deuteronilus',
follows the
Vastitas Borealis formation. A
study in June 2010 concluded...
- as
Major Syrtis Wayne Coyne as the
Alien Super-Being
Michael Ivins as
Deuteronilus Kliph Scurlock as
Orcus Steve Burns as
Astronaut Scott Booker as Sirenum...
-
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...
-
south latitudes are 47.06° N and 39.87° N.
Protonilus Mensae is
between Deuteronilus Mensae and
Nilosyrtis Mensae; all lie
along the
Martian dichotomy boundary...
-
widely believed to be
caused by
glacial movement.
Areas on Mars
called Deuteronilus Mensae and
Protonilus Mensae contain many
examples of
concentric crater...
- S.; Schneeberger, D. M. (1989). "Transitional
Morphology in the West
Deuteronilus Mensae Region of Mars:
Implications for
Modification of the Lowland/Upland...
