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The first mission to Mercury

MESSENGER's successful entry into Mercury's orbit marks a major milestone in understanding the planet's origin, composition, and geological history. The spacecraft has captured stunning images of Mercury's previously unexplored hemisphere, revealing its intricate details.

SourceIOP Publishing·JournalPhysics World·DateFeb 1, 2011

Volcanic activity shaped Mercury after all

Researchers from Brown University have discovered evidence of past volcanic activity on Mercury, suggesting that the planet underwent intense changes to its landscape around 3-4 billion years ago. The findings were made possible by detailed images from NASA's MESSENGER spacecraft and provide new insights into Mercury's geologic history.

SourceBrown University·JournalScience·DateJul 3, 2008

Mercury's shifting, rolling past

Researchers propose that mantle convection played a role in forming Mercury's lobate scarps, contrary to earlier theories. The simulations suggest that upwellings from mantle convection take on a linear roll shape, distinct from other planets' features.

SourceVirginia Tech·JournalNature Geoscience·DateMar 17, 2008

Mercury in color!

MESSENGER's Wide Angle Camera captures high-resolution color views of Mercury, showcasing subtle variations indicative of different rock types and mineral compositions. The images provide valuable information for understanding Mercury's formation and evolution.

Astronomer finds that Mercury has molten core

Researchers have found strong evidence that Mercury's core is molten, a discovery that could explain the planet's weak magnetic field. The study used a novel technique to detect tiny twists in Mercury's spin, which occurred as the sun's gravity exerted alternating torques on the planet.

SourceCornell University·JournalScience·DateMay 3, 2007

Eating planets gives stars indigestion

When a star swallows a planet, it can experience profound effects on its evolution, including changes in spin rate and emission of infrared radiation. The simulations show that large planets can survive for thousands of years before being vaporized by the heat, leaving behind tell-tale signs such as high lithium abundance.

SourceNew Scientist·JournalThe New Scientist·DateNov 9, 1999