BBC: The Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft, launched by NASA in November 2013, has been exploring the Red Planet’s upper atmosphere since it arrived there in September 2014. As reported at the 46th Lunar and Planetary Science Conference being held this week in Texas, last December MAVEN detected the presence of a bright UV auroral glow in Mars’s northern hemisphere, similar to the northern lights that can be observed on Earth. However, the high-energy particles responsible for the phenomenon appear to penetrate much deeper into the atmosphere of Mars than they do on Earth, perhaps because Mars lacks Earth’s protective magnetic field. The aurora sighting, and the detection of dust at altitudes of 150–300 km, may help further MAVEN‘s mission of determining how Mars’s atmosphere evolved.
The finding that the Saturnian moon may host layers of icy slush instead of a global ocean could change how planetary scientists think about other icy moons as well.
Modeling the shapes of tree branches, neurons, and blood vessels is a thorny problem, but researchers have just discovered that much of the math has already been done.
January 29, 2026 12:52 PM
Get PT in your inbox
PT The Week in Physics
A collection of PT's content from the previous week delivered every Monday.
One email per week
PT New Issue Alert
Be notified about the new issue with links to highlights and the full TOC.
One email per month
PT Webinars & White Papers
The latest webinars, white papers and other informational resources.