Planetary Radio: Space Exploration, Astronomy and Science
Planetary Radio: Space Exploration, Astronomy and Science

The Ancient Snows of Mars

When she was learning to forecast the weather in Hawaii, Brown University grad student Kat Scanlon didn’t suspect it would help her uncover evidence for rain or, more likely, snow that helped shape the surface of Mars billions of years ago. Learn more about your ad choices. Visit megaphone.fm/adchoi

Featured Speakers

The Planetary Society HostBill Nye Guest

Topics Discussed

Episode Summary

Executive Summary: This episode covers Curiosity rover progress on Mars, Bill Nye’s concerns about NASA education and web consolidation, and Brown grad student Kat Scanlon’s research suggesting ancient Martian valley networks were shaped by orographic precipitation—likely snow rather than rain. The show ties Mars climate history to habitability, discusses MAVEN’s atmospheric findings, and closes with a night-sky update and space trivia.

Main Topics: Curiosity rover’s first-year progress on Mars: Emily Lakdawalla reports that Curiosity has finally driven west of its landing site, resumed its trek toward Mount Sharp, and is stopping for science and imaging along the way. Curiosity’s imaging of Phobos and Deimos: A new animation and full-resolution frame show Curiosity capturing the moons passing each other, an early example of high-value visual science from the rover’s cameras. NASA education/public outreach and website consolidation: Bill Nye describes concerns that NASA’s education/public outreach budget was cut to zero and argues that mission teams still provide essential content for broader education efforts. Ancient Martian precipitation and orographic snow: Kat Scanlon explains how climate modeling showed Mars valley networks align with precipitation patterns expected from atmospheric flow over topography, supporting snow or rain as a shaping mechanism. Mars climate, atmospheric pressure, and habitability: The discussion explores why a warm, rainy early Mars is hard to justify physically, how snowmelt or episodic warming might work, and what this means for possible early life. Night sky update and space trivia: Bruce Betts gives a seasonal planet lineup, recalls historic space milestones, and presents trivia about the Vega missions and recovered orbital objects.

Key Arguments: Curiosity has moved beyond its landing site and is now making real progress toward Mount Sharp, showing the rover is fully operational and productive. The rover’s route is scientifically informed: the visually impressive layered hills ahead are likely windblown sediments, while more interesting water-related minerals are lower and farther along the path. NASA’s mission-driven communications remain crucial because outside organizations depend on NASA for accurate information about missions and discoveries. A physically robust early-Mars warm-rain scenario is hard to support with current climate models because the young Sun was dimmer and greenhouse mechanisms are insufficiently convincing. Kat Scanlon’s modeling suggests that precipitation patterns on early Mars matched valley network locations, supporting snow/rain driven erosion rather than groundwater alone. If Mars had a thicker atmosphere, the modeled precipitation would fall in the wrong places for key valley systems, so topography can help constrain ancient atmospheric pressure. Ancient snowfall and meltwater are relevant to habitability because they affect how water moves, how long it persists, and whether conditions could support prebiotic chemistry or microbial life.

Data Points: Curiosity travel distance: just over 1 kilometer - Described as the rover’s distance traveled after about one Earth year on Mars. Curiosity drill holes: 2 - Emily notes the rover has drilled two holes so far. Age of Martian precipitation event: about 3.7 billion years ago - Kat Scanlon says the valley networks date to the ancient period when precipitation may have fallen. Atmospheric pressure scenario: 2 bars - Kat explains that if early Mars had twice Earth’s atmospheric pressure, precipitation would fall in the wrong place for some valley networks. Lower pressure constraint: below 1.6 bars - She cites other work suggesting early Mars pressure had to be under roughly 1.6 bars. Mars climate model resolution: about 2 degrees of latitude/longitude - Kat describes the coarse resolution of general circulation models before downscaling. Topographic dataset coverage: 100-meter coverage - THEMIS is described as giving 100-meter global coverage used in the study. Topographic dataset coverage: 5-meter coverage - CTX is described as providing 5-meter coverage over much of Mars. NASA websites: 2,500 - Bill Nye mentions the scale of NASA’s website footprint during discussion of consolidation. X-15 space threshold: 50 miles - Bruce Betts notes Joe Engle’s X-15 flight crossed the US Air Force space threshold.

Pivotal Quotes: "“the wind directions the model predicted as being the most common in each of these places... were also... exactly lit up where we see all the valley networks.”" — Kat Scanlon: Explaining the key result that climate-model winds and topography-based precipitation matched Martian valley network locations. "“Mars may have been warm enough to rain every now and then, but nobody has yet come up with a physically very robust way to prove that Mars could have had a warm climate at that time.”" — Kat Scanlon: Summarizing why the team considers snow and episodic warming more plausible than persistent rain. "“NASA is the best brand that the United States has.”" — Bill Nye: Arguing for preserving NASA’s identity and mission-linked communication structure while consolidating websites.

Implications: The episode suggests Mars may have had localized snow-driven erosion and a more complex climate than once thought, sharpening habitability questions. It also underscores the importance of mission data, modeling, and NASA outreach for understanding planetary evolution.

🔓 Sign Up for Unlimited Episode Search

About Planetary Radio: Space Exploration, Astronomy and Science

View all episodes from Planetary Radio: Space Exploration, Astronomy and Science