A new analysis of seismic data from the InSight mission to Mars has revealed some surprises. The first: the top 300 meters of the subsurface beneath the InSight landing site near the Martian equator contains little to no ice. "We find that Mars' crust is weak and porous, the sediments are not well-cemented, and there's no ice or not much ice filling the pore spaces," said geophysicist Vashan Wright of the Scripps Institution of Oceanography at the University of California San Diego. Wright and co-authors published the U.S. National Science Foundation-supported analysis in Geophysical Research Letters.