The gigantic lava flows off of the solar system’s biggest known volcano
Cool image time! The photo to the right, cropped, reduced, and annotated to post here, was taken on October 30, 2021 by the high resolution camera on Mars Reconnaissance Orbiter (MRO). The picture covers a very tiny section of the southeast flank of Olympus Mons, the largest known volcano in the solar system. The arrow indicates the direction of the downward slope.
Olympus Mons itself is about 400 miles wide 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 mountain’s flanks, almost 200 miles long from caldera edge to base, drop about 54,000 feet. That average drop of about 270 feet every mile is not particular steep, but its continuous nature over such a very very long distance makes its quite daunting.
You can see evidence of that slope in the photo. The downward pointing lobes each indicate the volcano’s last separate lava flows that ceased moving when each froze in place, probably several tens of millions of years ago. These lobes were also placed on top of many earlier flows from the volcano’s past eruptions that probably continued for several billion years, beginning 3.5 billion years ago.
The overview map helps provide a sense of scale by placing this image on that mountain flank.
The white rectangular box shows the area covered by today’s full image. The larger white rectangle is the area covered by an December 18, 2016 image taken by MRO’s context camera. The blue dot near the bottom of that large rectangle marks the location of an earlier cool image, posted in May 2021, showing the volcano’s now frozen lava flow as it begins its precipitous drop off that flank.
Make sure you look at the full image as well as that December 18 context camera image. The extent of this flow is amazing. Its age, relatively young for Mars, can be roughly measured by the number of craters on this surface. The low number of craters suggest this surface is only a few million years old.
The large extent of Olympus Mons lava flanks is also another indication that lava flows farther and faster in Mars’ low gravity than it does on Earth.
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Cool image time! The photo to the right, cropped, reduced, and annotated to post here, was taken on October 30, 2021 by the high resolution camera on Mars Reconnaissance Orbiter (MRO). The picture covers a very tiny section of the southeast flank of Olympus Mons, the largest known volcano in the solar system. The arrow indicates the direction of the downward slope.
Olympus Mons itself is about 400 miles wide 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 mountain’s flanks, almost 200 miles long from caldera edge to base, drop about 54,000 feet. That average drop of about 270 feet every mile is not particular steep, but its continuous nature over such a very very long distance makes its quite daunting.
You can see evidence of that slope in the photo. The downward pointing lobes each indicate the volcano’s last separate lava flows that ceased moving when each froze in place, probably several tens of millions of years ago. These lobes were also placed on top of many earlier flows from the volcano’s past eruptions that probably continued for several billion years, beginning 3.5 billion years ago.
The overview map helps provide a sense of scale by placing this image on that mountain flank.
The white rectangular box shows the area covered by today’s full image. The larger white rectangle is the area covered by an December 18, 2016 image taken by MRO’s context camera. The blue dot near the bottom of that large rectangle marks the location of an earlier cool image, posted in May 2021, showing the volcano’s now frozen lava flow as it begins its precipitous drop off that flank.
Make sure you look at the full image as well as that December 18 context camera image. The extent of this flow is amazing. Its age, relatively young for Mars, can be roughly measured by the number of craters on this surface. The low number of craters suggest this surface is only a few million years old.
The large extent of Olympus Mons lava flanks is also another indication that lava flows farther and faster in Mars’ low gravity than it does on Earth.
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.
“That average drop of about 270 feet every mile is not particular steep, . . .”
Works out to about a 5% grade. That is very respectable, especially if you want to move something up it.
Blair Ivey: On Earth a 5% grade might be hearty, but in Mars’ 38% gravity it is more equivalent to a 2% grade.