A beautiful shot of micro-penitentes on Mt Rainier near Seattle, WA as photographed by Mark Sanderson in 2006 ( CC3.0, license and original file and description here ). What I love about this image is the lack of anything familiar that could indicate the scale of the features - aside from the notes from the photographer. They could be cm across or km! This is a familiar feeling from looking at images that come back from spacecraft that challenge our preconceptions. Today, PhD student Giang reflects on his recently published work trying to understand whether such textures could arise on Mars and if so, how big would they be and in what directions would they be orientated? Such models are needed to help us interpret what we see.
By Giang Nguyen
Perhaps it’s a mental coping mechanism from the summer heat, but I’ve been thinking a lot about ice. The behaviour of water ice across the solar system is studied by many people in the PVL group, and I am no exception. I’ve been looking at how water affects the atmosphere since my undergrad where I studied terrestrial weather systems. Later, the work for my Master’s consisted of surveying the icy conditions of the Martian north polar cap to look for surface-atmosphere interaction. Finally, with my PhD well on its way, I’ve been tasked with studying the atmospheric conditions of possible icy worlds beyond our solar system.
As you might guess, water is somewhat an important volatile for the propagation of life on Earth. Since there isn’t another planetary body within the solar system that is like Earth, it is helpful to look at the most extreme conditions Earth has to offer for clues. From my introductory paragraph, you’re probably thinking that I’m going to talk about Earth’s arctic polar conditions but that won’t be the case. The geography of interest here is actually high-altitude deserts, chiefly the Atacama desert located within South America’s Andes mountains.