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Chance encounters: Mercury probe and sun spacecraft provide new info about Venus
Data from BepiColombo and Solar Orbiter during Venus gravity assists reveal how a magnetic field protects the Venusian atmosphere
Science & Tech
Space exploration missions always have a planned destination, but sometimes they swing by other planets on the way.
Two probes — BepiColombo, headed to Mercury, and Solar Orbiter, en route to the sun — recently passed by Venus at nearly the same time, visiting Earth's sister planet within a day of each other in August 2021. Their combined observations, recently published in the journal Nature Communications (opens in new tab), give astronomers a rare glimpse into the workings of Venus' magnetic field.
"BepiColombo had a perfect view of the different regions within the magnetosheath and magnetosphere," said University of Tokyo astronomer Moa Persson, lead author on the new study, in a press release (opens in new tab).
Earth's magnetic field is a key reason why life has been so successful here. Magnetic fields help deflect high-energy particles streaming from the sun, known as the solar wind, protecting the fragile atmosphere of the planet. Venus isn't quite so lucky — it doesn't have a magnetic field created deep in its core like Earth does.
However, Venus does have something known as an "induced" magnetic field, in which the solar wind interacts with charged particles in Venus' atmosphere to create a magnetosphere surrounding the planet. Solar Orbiter passed by Venus just outside this magnetosphere, observing the solar wind in its calm, undisturbed state. At the same time, BepiColombo zipped through the "stagnation region," the area where the solar wind and atmosphere are expected to interact at Venus.
Together, the probes' observations provided experimental evidence that charged particles are, in fact, slowed down by this region, protecting Venus' atmosphere from erosion by the solar wind.
This is also an important finding for planets beyond our solar system, since astronomers now know there is a way for exoplanets without an internal magnetic field to retain their atmospheres like Venus has — and therefore possibly even harbor life.