Ancient lava flows down the flanks of the solar system’s largest volcano
Cool image time! The photo to the right, cropped, reduced, and sharpened to post here, was taken on October 2, 2022 by the high resolution camera on Mars Reconnaissance Orbiter (MRO). It shows what appears to be very old and eroded lava on the northeast flanks of Olympus Mons, the largest volcano on Mars as well as the entire solar system. About 600 miles across, from the edge to its peak, Olympus rises about 54,000 feet, with an actual height relative to Mars’ “sea level” of just under 70,000 feet, more than twice as high as Mount Everest on Earth.
The white arrow show the downward grade. Several different flows can be seen throughout the picture, some confined to a central channel with smooth aprons of overflows on either side. Others are more broken and less coherent, and suggest that either the flows were inherently different, or are much older and have deteriorated with time.
The white box in the overview map to the right marks this picture’s location, on the northeast flank of the mountain.
The eruptions that created this volcano are thought to have occurred from 2 to 4 billion years ago, though some younger flows only 2 to 115 million years ago are suspected to exist on its northwest quadrant. Because it is a shield volcano, it was created by many eruptions, with lava flowing great distances again and again down its slopes. Thus, the picture above might be showing us many of these flows over time.
In Mars’ low gravity, about 39% of Earth’s, the data suggests that lava flows faster and with less viscosity. It is therefore possible for a single flow to travel several hundred miles, from the caldera down these slopes to the volcano’s edge, before freezing. At the same time, there is also evidence of additional vents along those flanks, which would have contributed their own flows.
Imaging what Mars was like when this volcano was active is difficult. Each eruption would have likely changed the planet’s entire climate.
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Cool image time! The photo to the right, cropped, reduced, and sharpened to post here, was taken on October 2, 2022 by the high resolution camera on Mars Reconnaissance Orbiter (MRO). It shows what appears to be very old and eroded lava on the northeast flanks of Olympus Mons, the largest volcano on Mars as well as the entire solar system. About 600 miles across, from the edge to its peak, Olympus rises about 54,000 feet, with an actual height relative to Mars’ “sea level” of just under 70,000 feet, more than twice as high as Mount Everest on Earth.
The white arrow show the downward grade. Several different flows can be seen throughout the picture, some confined to a central channel with smooth aprons of overflows on either side. Others are more broken and less coherent, and suggest that either the flows were inherently different, or are much older and have deteriorated with time.
The white box in the overview map to the right marks this picture’s location, on the northeast flank of the mountain.
The eruptions that created this volcano are thought to have occurred from 2 to 4 billion years ago, though some younger flows only 2 to 115 million years ago are suspected to exist on its northwest quadrant. Because it is a shield volcano, it was created by many eruptions, with lava flowing great distances again and again down its slopes. Thus, the picture above might be showing us many of these flows over time.
In Mars’ low gravity, about 39% of Earth’s, the data suggests that lava flows faster and with less viscosity. It is therefore possible for a single flow to travel several hundred miles, from the caldera down these slopes to the volcano’s edge, before freezing. At the same time, there is also evidence of additional vents along those flanks, which would have contributed their own flows.
Imaging what Mars was like when this volcano was active is difficult. Each eruption would have likely changed the planet’s entire climate.
Readers!
My annual February birthday fund-raising drive for Behind the Black is now over. Thank you to everyone who donated or subscribed. While not a record-setter, the donations were more than sufficient and slightly above average.
As I have said many times before, I can’t express what it means to me to get such support, especially as no one is required to pay anything to read my work. Thank you all again!
For those readers who like my work here at Behind the Black and haven't contributed so far, please consider donating or subscribing. My analysis of space, politics, and culture, taken from the perspective of an historian, is almost always on the money and ahead of the game. For example, in 2020 I correctly predicted that the COVID panic was unnecessary, that the virus was apparently simply a variation of the flu, that masks were not simply pointless but if worn incorrectly were a health threat, that the lockdowns were a disaster and did nothing to stop the spread of COVID. Every one of those 2020 conclusions has turned out right.
Your help allows me to do this kind of intelligent analysis. I take no advertising or sponsors, so my reporting isn't influenced by donations by established space or drug companies. Instead, I rely entirely on donations and subscriptions from my readers, which gives me the freedom to write what I think, unencumbered by outside influences.
You can support me either by giving a one-time contribution or a regular subscription. There are four ways of doing so:
1. Zelle: This is the only internet method that charges no fees. All you have to do is use the Zelle link at your internet bank and give my name and email address (zimmerman at nasw dot org). What you donate is what I get.
2. Patreon: Go to my website there and pick one of five monthly subscription amounts, or by making a one-time donation.
3. A Paypal Donation or subscription:
4. Donate by check, payable to Robert Zimmerman and mailed to
Behind The Black
c/o Robert Zimmerman
P.O.Box 1262
Cortaro, AZ 85652
You can also support me by buying one of my books, as noted in the boxes interspersed throughout the webpage or shown in the menu above.
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