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may be unreliable if the small crater population is dominated by secondary craters (craters formed by material ejected from larger impacts). Images showing no large craters with diameters larger than 500 meters superimposed on western
Cerberus plains lavas indicate the same surface is younger than 49
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lie both over and under lavas, suggesting the deposition of this formation was contemporaneous with volcanism. Statistics of small craters indicate lavas in the western
Cerberus plains may be less than a million years old, but the model
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High resolution images show the bulk of the
Cerberus plains is covered by platy-ridged and inflated lavas, which are interpreted as insulated sheet flows. Eastern Cerberus plains lavas originate at
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are both incised into pristine lavas and embayed by pristine lavas, indicating that
Athabascan fluvial events were contemporaneous with volcanic eruptions. Deposits of the
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Geological history of the
Cerberus Plains, Mars (Ph.D dissertation)
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fissures and shields. Some flows extend for 2000 km through
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53:plains and may be sand drifts. The volcano
34:Cerberus is dark area to left of center
146:. USGS Astrogeology Research Program.
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160:- zoomable map centered on Cerberus
144:Gazetteer of Planetary Nomenclature
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18:Cerberus (Martian albedo feature)
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68:into Amazonis Planitia. The
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74:Medusae Fossae Formation
174:Albedo features on Mars
122:Lanagan P. D. (2004).
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82:Ma (million years).
132:2004PhDT........16L
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92:Geography of Mars
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109:pds.jpl.nasa.gov
70:Athabasca Valles
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112:. Retrieved
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66:Marte Vallis
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55:Elysium Mons
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158:Google Mars
168:Categories
140:"Cerberus"
114:2013-04-12
105:"Cerberus"
79:isochrons
179:Cerberus
86:See also
51:Amazonis
47:Cerberus
39:Cerberus
128:Bibcode
98:Sources
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