Insane New Images of Mercury's Surface Captured on Probe's Final Flyby
Close up images of Mercury from the Bepicolombo monitoring cameras. (ESA/BepiColombo/MTM) |
During its penultimate flyby of the little, sun-baked globe, ESA's BepiColombo transfer probe has taken breathtaking close-up photos of Mercury from a just 295 kilometers above the planet's surface.
The images depict a world engulfed in extremes, offering close-ups of crater rims ringed by unending daylight and perpetual darkness. It is believed that a layer of ice lies behind those shadows, preserving hints that might provide us with more insight into Mercury's past and possibly its future.
At the European Space Agency's (ESA) annual press
briefing on January 9, Geraint Jones stated, "The BepiColombo team will
put in a lot of effort over the next few weeks to solve as many of Mercury's
mysteries with the data from this flyby as we can."
Close up of Mercury's north pole region, taken by M-CAM 1. (ESA/BepiColombo/MTM) |
The mission will move on to its next phase, preparing
for data gathering in 2027, after completing its series of gravitational aids.
"BepiColombo's main mission phase may only start two years from now,"
Jones added, "but all six of its flybys of Mercury have given us
invaluable new information about the little-explored planet."
As far as planets go, Mercury is a strange ball of rock. It orbits within a
cosmic whisker of our Sun at an average distance of about 58 million kilometers
(36 million miles), hardly bigger than our own Moon.
Its atmosphere, a dismal coating of gas continuously renewed by meteorites and
plasma tearing into its hide, is scourged by radiation and degraded by the
solar wind.
Temperatures can soar to 430 degrees Celsius (more
than 800 degrees Fahrenheit) at high midday. Hidden crevices and the predawn
chill can drop as low as minus 180 degrees Celsius in the absence of a
significant atmosphere to disperse and retain heat.
We can only speculate about the secrets that lie beneath the surface.
mechanisms behind an enigmatic magnetic field. An abundance of carbon that
might form a dense diamond coating. The planet may be gradually getting smaller
due to some sort of action.
BepiColombo was launched in October 2018 with the goal of gathering information
on Mercury's surface features, gaseous exosphere, and magnetism that may help
explain these anomalies and more.
As it traveled, its monitoring cameras captured stunning images of Venus' cloudtops and the surface of the innermost planet.
Mercury's northern hemisphere by M-CAM 1. (ESA/BepiColombo/MTM) |
Together with these most recent photos, astronomers have gathered proof of a globe that has been gradually darkened throughout time, with a history of volcanic eruptions and sporadic regeneration from massive impacts.
A vent around 40 kilometers across in the very center of the Nathair Facula, a feature in one photograph, still shows evidence of Mercury's greatest known volcanic eruption.
Fonteyn Crater, which was formed only 300 million years ago, is nearby and shines with relative youth.
Lava and debris brighten Mercury's surface, as seen by M-Cam 2. (ESA/BepiColombo/MTM) |
The ESA’s Mercury Planetary Orbiter and the Japan Aerospace Exploration Agency’s Mercury Magnetospheric Orbiter will be released by the Bepicolombo Mercury Transfer Module in 2026, with the goal of spending 2027 gathering data from their respective altitudes and orientations above the planet.
These are the closest images of Mercury we will see for some time because neither will approach 480 kilometers from the planet's surface.
However, once BepiColombo settles in to perform its
intended function, our image of the terrible planet is about to get much more
specific.
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