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How hard did it rain on Mars?

Researchers found that heavy rainfall on early Mars carved out river-like channels and altered impact craters, similar to Earth's effects. The study used physics principles to understand the relationship between Martian atmosphere pressure, raindrop size, and rainfall intensity.

SourceElsevier·JournalIcarus·DateMay 16, 2017

Pluto follows its cold, cold heart

Research suggests Pluto's subsurface ocean could be responsible for its current location. The 'heart' region, Sputnik Planitia, may have accumulated ice that made the planet roll over, creating cracks and tensions in the crust. This process, called true polar wander, allows planets to reorient without changing their spin axis.

SourceUniversity of Arizona·JournalNature·DateNov 16, 2016

Two planets orbit nearby ancient star

Astronomers have discovered two new planets orbiting a nearby ancient star, Kapteyn's Star, which is just 13 light years away from Earth. One planet, Kapteyn b, is thought to be warm enough to support liquid water on its surface, while the second, Kapteyn c, is a more massive super-Earth with uncertain habitability.

SourceCarnegie Institution for Science·JournalMonthly Notices of the Royal Astronomical Society·DateJun 3, 2014

Disappearing homing pigeon mystery solved

Researchers discovered that homing pigeons rely on 'loft-specific infrasonic map cues' to navigate, which are disrupted when release sites are shielded from these low-frequency signals. This finding resolves a long-standing puzzle and sheds new light on the birds' impressive navigation abilities.

SourceThe Company of Biologists·JournalJournal of Experimental Biology·DateJan 30, 2013

Bouncing on Titan

The probe dug a 12 cm deep hole before bouncing out onto a flat surface, sliding 30 cm across the surface due to friction. The probe wobbled back and forth five times before coming to rest, suggesting the surface was soft enough to make a hole but hard enough to support wobbling

SourceEuropean Space Agency·JournalPlanetary and Space Science·DateOct 11, 2012