Deuteronilus Mensae is a region on Mars 937 km across and centered at 43°54′N337°24′W / 43.9°N 337.4°W / 43.9; -337.4. It covers 344°–325° West and 40°–48° North.[1] Deuteronilus region lies just to the north of Arabia Terra and is included in the Ismenius Lacus quadrangle. It is along the dichotomy boundary, that is between the old, heavily cratered southern highlands and the low plains of the northern hemisphere. The region contains flat-topped knobby terrain that may have been formed by glaciers at some time in the past. Deuteronilus Mensae is to the immediate west of Protonilus Mensae and Ismeniae Fossae.[2][3] Glaciers persist in the region in modern times, with at least one glacier estimated to have formed as recently as 100,000 to 10,000 years ago.[4] Recent evidence from the radar on the Mars Reconnaissance Orbiter has shown that parts of Deuteronilus Mensae do indeed contain ice.[5][6][7]
^Patrick Moore; Garry Hunt (1997). The atlas of the solar system. Chancellor. ISBN 978-0-7537-0014-3.
^Baker, M. et al. 2010. Flow patterns of lobate debris aprons and lineated valley fill north of Ismeniae Fossae, Mars: Evidence for extensive mid-latitude glaciation in the Late Amazonian. Icarus: 207. 186–209.
^"Breathtaking views of Deuteronilus Mensae on Mars".
^Rincon, Paul (19 December 2007). "'Active glacier found' on Mars". BBC News.
^"HiRISE | Merging Lobate Debris Aprons of Deuteronilus Mensae (PSP_009535_2240)".
^Plaut, J., A. Safaeinili,, J. Holt, R. Phillips, J. Head, J., R. Seu, N. Putzig, A. Frigeri. 2009. Radar evidence for ice in lobate debris aprons in the midnorthern latitudes of Mars. Geophys. Res. Lett. 36. doi:10.1029/2008GL036379.
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DeuteronilusMensae is a region on Mars 937 km across and centered at 43°54′N 337°24′W / 43.9°N 337.4°W / 43.9; -337.4. It covers 344°–325° West and...
latitudes are 47.06° N and 39.87° N. Protonilus Mensae is between DeuteronilusMensae and Nilosyrtis Mensae; all lie along the Martian dichotomy boundary...
in Aeolis Mensae, between 10 N and 10 S latitude and 240 W and 210 W longitude. Two good examples of fretted terrain are DeuteronilusMensae and Protonilus...
material. DeuteronilusMensae Geology of Mars Glacier Ismenius Lacus quadrangle Martian dichotomy Protonilus Mensae The Color Palette of Nilosyrtis Mensae at...
dichotomy boundary includes the regions called DeuteronilusMensae, Protonilus Mensae, and Nilosyrtis Mensae. All three regions have been studied extensively...
Terra Sabaea. The Ismenius Lacus quadrangle contains DeuteronilusMensae and Protonilus Mensae, two places that are of special interest to scientists...
to be caused by glacial movement. Areas on Mars called DeuteronilusMensae and Protonilus Mensae contain many examples of concentric crater fill. Concentric...
regions that are named from ancient names: DeuteronilusMensae, Protonilus Mensae, and Nilosyrtis Mensae. Well-developed hollows, as seen by HiRISE under...
glacier-like features called lobate debris aprons in an area called DeuteronilusMensae, which display widespread evidence of ice lying beneath a few meters...
covered with a thin layer of rocks. In addition, radar studies in DeuteronilusMensae show that all lobate debris aprons examined in that region contain...
in Mamers Valles, a channel found along the dichotomy boundary in DeuteronilusMensae. They may be an easy way for future colonists of Mars to find water...
cratered uplands of the Arabia Terra, from the Cerulli crater to the DeuteronilusMensae near the edge of Mars' vast northern lowlands. Through their midsection...
west of Moreux crater. The regions of plateaus known as DeuteronilusMensae and Protonilus Mensae are to the northwest and northeast of Ismeniae Fossae...
270°W and 360°W. Parts of the fretted terrain are called DeuteronilusMensae and Protonilus Mensae. In fretted terrain, the land seems to transition from...
regions that are named from ancient places: DeuteronilusMensae, Protonilus Mensae, and Nilosyrtis Mensae. Lobate debris aprons, lineated valley fill...
scientists released the results of a radar study of an area called DeuteronilusMensae that found widespread evidence of ice lying beneath a few meters...
Schneeberger, D. M. (1989). "Transitional Morphology in the West DeuteronilusMensae Region of Mars: Implications for Modification of the Lowland/Upland...
mantling in the mid-latitudes. It was first investigated in the DeuteronilusMensae (Ismenius Lacus quadrangle) region, but it occurs in other places...
mid-latitudes of the planet Mars. It was first investigated in the DeuteronilusMensae (Ismenius Lacus quadrangle) region, but it occurs in other places...
near the northern dichotomy boundary. The Nilosyrtis Mensae, Protonilus Mensae and DeuteronilusMensae bear many examples of LVF. Ismenius Lacus quadrangle...
discovered in the mid-latitudes of Mars. First investigated in the DeuteronilusMensae (Ismenius Lacus quadrangle) region, but it occurs in other places...
discovered in the mid-latitudes of Mars. First investigated in the DeuteronilusMensae region, but it occurs in other places as well. The remnants consist...
with no more than 10% dust by volume and that fretted valleys in DeuteronilusMensae contain thick glaciers covered by a mantle of rocky debris. Kieffer...
"Lineated valley fill (LVF) and lobate debris aprons (LDA) in the DeuteronilusMensae northern dichotomy boundary region, Mars: Constraints on the extent...
Lineated valley fill (LVF) and lobate debris aprons (LDA) in the DeuteronilusMensae northern dichotomy boundary region, Mars: Constraints on the extent...
HiRISE under HiWish program Image is of the top of a debris apron in DeuteronilusMensae. Close up of field of high center polygons with scale, as seen by...
; Schneeberger, Dale M. (1989). "Transitional morphology in West DeuteronilusMensae, Mars: Implications for modification of the lowland/upland boundary"...
"Lineated valley fill (LVF) and lobate debris aprons (LDA) in the DeuteronilusMensae northern dichotomy boundary region, Mars: Constraints on the extent...
"Lineated valley fill (LVF) and lobate debris aprons (LDA) in the DeuteronilusMensae northern dichotomy boundary region, Mars: Constraints on the extent...
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