A new study indicates that Mercury may be shrinking 30% faster than previously estimated, resulting in a loss of up to 14 miles (23 kilometers) in its diameter.
The research, published in the journal Geophysical Research Letters, suggests that Mercury's rough surface, shaped by impact debris, has obscured the true extent of its contraction.
Scientists from the German Aerospace Center's Institute of Space Research conducted the study.
The findings are based on data collected by NASA's Messenger spacecraft during its mission in the 2010s.
The joint European and Japanese BepiColombo mission is expected to enter Mercury's orbit in November to further investigate the planet's internal cooling and shrinkage.
Detailed Insights:
Mercury, the smallest and innermost planet in our solar system, has been contracting since its formation approximately 4.5 billion years ago.
This shrinkage is primarily due to the cooling and contraction of its hot iron core, along with its mantle and crust.
The study compared maps of faults and other geological signs of contraction with newer maps highlighting surface roughness.
Researchers discovered that the roughest patches exhibited fewer visible shrinkage wrinkles, suggesting these features were buried under impact debris.
The BepiColombo mission is a collaborative effort between the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA).
It comprises two orbiters: the Mercury Planetary Orbiter (MPO) by ESA and the Mercury Magnetospheric Orbiter (Mio) by JAXA.
The mission will utilize a laser instrument to confirm the extent of Mercury's contraction.
Only two other spacecraft have visited Mercury: NASA's Mariner 10 in the 1970s and NASA's Messenger in the 2010s.
The lead author, Gaku Nishiyama, affiliated with Hokkaido University, suggests the actual shrinkage could be even greater than current estimates.
A greater degree of shrinkage implies Mercury could have a larger metal core, fewer light elements, or a higher initial temperature.
Scientific/Technical Concepts Involved:
Planetary Contraction: The process by which a celestial body reduces in size due to the cooling and subsequent densification of its internal structure.
Impact Craters: Bowl-shaped depressions on a planetary surface formed by the high-velocity collision of meteoroids, asteroids, or comets.
Faults: Fractures in a planet's crust where there has been significant displacement of rock, often indicating tectonic activity or contraction.
Geophysical Research Letters: A scientific journal publishing high-impact, short-format research articles across Earth and space sciences.