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Trachyandesite and trachyte are the most common rocks on Mount Melbourne, with basalt being less common[50] and mostly occurring around its base. The rocks define a mildly alkaline suite[21] rich in potassium, unlike the rocks elsewhere in the volcanic field. The rest of the volcanic field also features alkali basalts, basanite and mugearite. Phenocrysts include aegirine, amphibole, anorthoclase, augite, clinopyroxene, fayalite, hedenbergite, ilmenite, kaersutite, magnetite, olivine, plagioclase and sanidine.[84][85][86] Gneiss,[55] granulite, harzburgite, lherzolite and tholeiite xenoliths are found in the volcanic field[52] and form the core of many lava bombs.[34] Inclusions in xenoliths indicate that the gaseous components of the Mount Melbourne volcanic field magmas consist mainly of carbon dioxide.[87] The rocks in the volcanic field have porphyritic to vitrophyric textures.[86] The trachytes and mugearites formed through magmatic differentiation in a crustal magma chamber[7] from alkali basalts,[88] defining an alkali basalt-trachyte differentiation series.[89] Basalts were mainly erupted early in the history of the volcano.[7] During the last hundred thousand years the magma chamber became established; this allowed both the differentiation of trachytes and the occurrence of large eruptions.[90] A gap in the rock spectrum ("Daly gap") with a scarcity of benmoreite and mugearite has been noted at Mount Melbourne and other volcanoes in the region.[42] There is no agreement on which processes contributed to petrogenesis in the Mount Melbourne volcanic field[91] but diverse mantle domains and assimilation and fractional crystallization processes appear to have played a role.[92] The magmatic system that feeds Mount Melbourne appears to have a composition distinct from the one associated with the Mount Melb













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<p style=3D"color:#FFFFFF;font-size:7px;">Trachyandesite and trachyte are t=
he most common rocks on Mount Melbourne, with basalt being less common[50] =
and mostly occurring around its base. The rocks define a mildly alkaline su=
ite[21] rich in potassium, unlike the rocks elsewhere in the volcanic field=
. The rest of the volcanic field also features alkali basalts, basanite and=
 mugearite. Phenocrysts include aegirine, amphibole, anorthoclase, augite, =
clinopyroxene, fayalite, hedenbergite, ilmenite, kaersutite, magnetite, oli=
vine, plagioclase and sanidine.[84][85][86] Gneiss,[55] granulite, harzburg=
ite, lherzolite and tholeiite xenoliths are found in the volcanic field[52]=
 and form the core of many lava bombs.[34] Inclusions in xenoliths indicate=
 that the gaseous components of the Mount Melbourne volcanic field magmas c=
onsist mainly of carbon dioxide.[87] The rocks in the volcanic field have p=
orphyritic to vitrophyric textures.[86]

The trachytes and mugearites formed through magmatic differentiation in a c=
rustal magma chamber[7] from alkali basalts,[88] defining an alkali basalt-=
trachyte differentiation series.[89] Basalts were mainly erupted early in t=
he history of the volcano.[7] During the last hundred thousand years the ma=
gma chamber became established; this allowed both the differentiation of tr=
achytes and the occurrence of large eruptions.[90] A gap in the rock spectr=
um ("Daly gap") with a scarcity of benmoreite and mugearite has been noted =
at Mount Melbourne and other volcanoes in the region.[42] There is no agree=
ment on which processes contributed to petrogenesis in the Mount Melbourne =
volcanic field[91] but diverse mantle domains and assimilation and fraction=
al crystallization processes appear to have played a role.[92] The magmatic=
 system that feeds Mount Melbourne appears to have a composition distinct f=
rom the one associated with the Mount Melb</p>
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