Categories
planetary geology

The Waters of Mars

No, not the super awesome episode of Doctor Who. And forgive me if I keep this short and only semi-coherent. I’ve spent most of my day staring at thin sections of fossilized sea varmint poop (you heard me right) so… yeah. It’s the glamor. That’s why I chose this educational path.

However, Mars is much more glamorous than peloids. Fortuitously enough, the geological colloquium today featured Bryan Hynek, who researches Mars. He did an interesting talk about Martian river valleys, and also the existence of an early ocean on Mars.

Mostly what struck me about the river valley portion was just how much higher resolution imaging has done for the field. In one example, he showed an area that had an extremely small drainage density when calculated from pictures taken by the Viking (if I remember correctly) mission. With the newer, higher resolution data a lot more tributaries are apparent and the drainage density in that area climbed up to something you’d expect to find in Utah. Which isn’t to say Mars was a watery paradise back in the Noachian, but it had actively flowing water. Looking at the river valley distribution and age, it was mostly concentrated in the early history of the planet, but it’s still interesting to think of Mars as a significantly wet planet.

This lead in to looking at the possibility of a Martian ocean, which isn’t really a new idea. Using climate models, it’s apparently not really possible to create the sort of drainage networks that have been found without an ocean. This is actually not an idea I’d been exposed to before, probably because I don’t read nearly enough about planetary geology. Bryan also looked at river deltas (some of the pictures had the classic bird’s foot shape like the Mississippi delta) that emptied into the probable site of the ocean and used that to estimate the sea level and thus the shoreline. He had a striking picture of Mars with elevations up to the proposed sea level filled in with blue. There’s something jarring about seeing a third of the red planet hidden under and ocean.

There are still a lot of questions to be answered (like the big issue of constructing an atmosphere for the Noachian epoch that would have made this possible and sourcing all of the gases), and doesn’t really do much for the question of if there’s water on Mars today – but it’s a lot of fun to think about if nothing else. And cool. Let’s not forget cool. And it made me remember all sorts of terminology from geomorphology that I’d almost managed to forget.

Oh yes, and evidence of moraines left by retreating glaciers on the volcanoes. Pitterpat goes my heart.

I’ll add it to my list of things to do as soon as time travel is invented, right after (3) Pet a [herbivorous] dinosaur – (4) Go sailing on Mars. Do not forget respirator.

Categories
geomorph planetary geology

Mars Geomorph Porn

There’s a lovely blog post over at The Planetary Society explaining a couple of images from IAG’s Planetary Geomorphology Working Group’s May 2010 featured images.

This is some cool stuff, since it’s very much connected to the ongoing “water on Mars” debate, and the geomorphological argument has to do with water leaching minerals over a fairly long period of time. Another of the images that the blog post doesn’t cover looks at:

However, with the addition of infrared color, two distinct units of altered minerals can be discerned, and using spectroscopic information, these have been identified. Here at NE Syrtis, there is a unique stratigraphy of iron sulfate overlying carbonate, which is being exposed by the erosion of overlying lavas (Mustard and Ehlmann, 2010). This suggests a transition in the aqueous alteration environment from neutral-to-alkaline to acidic that is preserved in the rock record.

Aqueous alteration environment… squee! With of course the added fun of wondering what might have caused the pH of that environment to go from neutral-ish to acidic. Interesting stuff, to be sure.

I didn’t know about the images of the month, but I’m going to start checking them out for sure! Geomorphology was one of my favorite undergrad classes, and there’s some very neat stuff on that site. For example, comparison of catastrophic flood bed forms on Earth and Mars that was April’s set of images. Looking at land features via aerial/satellite imagery isn’t perfect, but I think it’s great to see our knowledge of our own planet being applied to the images we’re getting from Mars.

Categories
astro stuff planetary geology

The canyons of Mars

Super cool post over at Phil Plait’s blog in regards to an oblique view of an exposed section in the Gale Crater on Mars, courtesy of NASA. This is some exciting stuff if you’re a sed/strat nerd like me. Outcrops are the bread and butter of any geologist – unless you’ve got the money to drill cores or shoot seismic, subsurface geology is inferred from outcrops – and this one looks quite beautiful.

I just wish NASA would tell us a little more:

Layers near the bottom of the mound contain clay and sulfate minerals that indicate wet conditions. Overlying rock layers contain sulfates with little or no clay, consistent with these layers forming in an environment in which water was evaporating and Mars was drying out.

Since of course I’m immediately dying to know what sorts of clays, and which sulfate minerals. I’m thinking that when they’re talking about sulfates consistent with Mars drying out, it’d be sulfate evaporites like gypsum, barite, or anhydrite. Which then allows my fevered imagination to bring forth images of the Paradox Formation in eastern Utah and Colorado.

Of course, I have to stop myself from getting carried away here. The Paradox Formation is in places thousands of feet thick and covers an enormous area, which is what allows it to have such a profound tectonic effect on the landscape. Looking at that outcrop, I’m having a hard time getting a sense of just how thick the evaporites would be, but probably not that much. But what it does say, about the existence of water on the surface of Mars in the past, is pretty huge. And of course – letting my imagination run just a little wild here – opens the possibility of more evaporite deposits lurking under the surface, and bigger ones, and somewhere out there, one of the salt tectonic guys is going, “squee!”