Martian stratovolcanoes Zephyria Tholus and Elysium Mons
While stratovolcanoes are common on Earth, they’re extremely rare on other planets of solar system.
on Mars, almost all volcanoes are shield, except few cinder cones and two stratovolcanoes (of those, one is also a shield). on Venus there are no stratovolcanoes at all, but there are pancakes domes, that can’t be found on Earth and Mars. It should be noted, however, that Venus has an atmospheric pressure that is 90 times the one of Earth, so possibly stratovolcanoes might have been squished from the start, developing into shield instead.
The only pure stratovolcano on Mars is named Zephyria Tholus.
https://onehundredmountains.blogspot.com/2011/05/meizan-from-outer-space.html
Meizan from outer spaceA new candidate for the “Mt Fuji of Mars” is proposed. And why stop there… ?
Sumimasen: a few posts ago, I did something ill-considered. It was reckless to designate Mons Olympus, the largest volcano on the Red Planet, as "the Mt Fuji of Mars" (火星富士). For even the briefest glance shows that the Martian mountain (below) looks nothing like Mt Fuji. It isn’t even the same kind of volcano.
And, if you do seek a Mars-Fuji, there are better choices. Take Zephyria Tholus, for instance, an “unusually symmetrical cone located in the Aeolis region of Mars … with a flat-floored summit crater”.
As you’d expect from this description, Zephyria is likely to be a stratovolcano. That is certainly the conclusion of Emily Lewis and James Head, two savants from Brown University who analysed the radar data from NASA’s Mars Orbiter.
Just like the real Mt Fuji, the Martian cone (above) has slightly concave upper slopes and its edifice is “dissected” by two huge erosion gullies. Even the height is Fuji-like: about 3,000 metres today and perhaps as tall as 3,900 metres in the past.
Like Fuji’s, the summit crater plunges about 200 metres deep. However – and this is where the comparison does get a bit stretched – Zephyria’s cauldron is about eight or nine times wider than the Japanese one. Also, its summit slopes are only about half as steep as Fuji’s.
All in all, Zephyria would look squatter than Fuji. That, say Lewis and Head, is only to be expected of Martian volcanoes – the low gravity and thin atmosphere allow eruptive debris to fly further, resulting in a more spread-out edifice. You see, Mars is a foreign planet; they do things differently there.
Yet proposing Zephyria as Mars-Fuji shouldn’t be too controversial. It only extends the Japanese custom of awarding the “Fuji” suffix to any mountain that looks remotely conical. Thus, there is hardly a Japanese prefecture without its own Fuji, from one end of the archipelago to the other: Rishiri-Fuji, Ezo-Fuji, Tsugaru-Fuji …
The point about all these honorary Mt Fujis is that they share the elegance of their original. In short they are “Meizan”. The word is Japanese, but it can apply to any mountain of note, anywhere. When they relabelled Mt Rainier (below) as “Tacoma-Fuji”, homesick émigrés from Japan implicitly recognised that.
So did Fukada Kyūya, the maven of Meizan. Encouraged by the success of his One Hundred Mountains in Japan (Nihon Hyakumeizan), he was busy compiling a Sekai no Hyakumeizan (One Hundred Mountains of the World) when he died in 1971.
But why stop with the world? As Lewis and Head show, other planets have Meizan too. Indeed, there should be more than enough for a One Hundred Mountains of the Solar System (太陽系の百名山). Now which would they be, I wonder.... ?
The other stratovolcano (though is an half shield), Elysium Mons, might have characteristics similar to Mount Etna, a large shield base with a tiny stratocone on the top (though Etna has FOUR tiny stratocone on the top of a still active large shield)
From wikipedia: https://repress.alummah.news/browses.php?q=https%253A%252F%252Fen.wikipedia.org%252Fwiki%252FVolcanology_of_Mars
Elysium volcanic province
A smaller volcanic center lies several thousand kilometers west of Tharsis in Elysium. The Elysium volcanic complex is about 2,000 kilometers in diameter and consists of three main volcanoes, Elysium Mons, Hecates Tholus, and Albor Tholus. The northwestern edge of the province is characterized by large channels (Granicus and Tinjar Valles) that emerge from several grabens on the flanks of Elysium Mons. The grabens may have formed from subsurface dikes. The dikes may have fractured the cryosphere, releasing large volumes of ground water to form the channels. Associated with the channels are widespread sedimentary deposits that may have formed from mudflows or lahars.[37] The Elysium group of volcanoes is thought to be somewhat different from the Tharsis Montes, in that development of the former involved both lavas and pyroclastics.[38]
Elysium Mons is the largest volcanic edifice in the province. It is 375 km across (depending on how one defines the base) and 14 km high. It has single, simple caldera at its summit that measures 14 km wide and 100 m deep. The volcano is distinctly conical in profile, leading some to call it a stratocone;[39] however, given the predominantly low slopes, it is probably a shield. Elysium Mons is only about one-fifth the volume of Arsia Mons.[37]
Hecates Tholus is 180 km across and 4.8 km high. The slopes of the volcano are heavily dissected with channels, suggesting that the volcano is composed of easily erodible material such as volcanic ash. The origin of the channels is unknown; they have been atrributed to lava, ash flows, or even water from snow or rainfall.[40] Albor Tholus, the southernmost of the Elysium volcanoes, is 150 km in diameter and 4.1 km high. Its slopes are smoother and less heavily cratered than the slopes of the other Elysium volcanoes.[41]