{"id":788401,"date":"2024-09-05T07:04:50","date_gmt":"2024-09-05T12:04:50","guid":{"rendered":"https:\/\/spaceweekly.com\/?p=788401"},"modified":"2024-09-05T07:04:50","modified_gmt":"2024-09-05T12:04:50","slug":"jupiters-moon-slammed-and-tipped-by-giant-asteroid","status":"publish","type":"post","link":"https:\/\/spaceweekly.com\/?p=788401","title":{"rendered":"Jupiter\u2019s moon slammed and tipped by giant asteroid?"},"content":{"rendered":"


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A new study shows that some 4 billion years ago, a giant asteroid slammed into Jupiter\u2019s moon, Ganymede, shifting its axis. Ganymede is the largest of Jupiter\u2019s moons and the largest moon in our solar system. Image via Hirata Naoyuki (CC BY)\/ Kobe University.<\/figcaption><\/figure>\n

Jupiter\u2019s moon slammed and tipped by ancient asteroid<\/h3>\n

Some 4 billion years ago, a behemoth asteroid \u2013 perhaps 20 times larger than Earth\u2019s dinosaur-killer \u2013 slammed into Jupiter\u2019s moon Ganymede. The incredible impact would have sent ejecta flying outward, creating concentric circles of debris around the impact site. On September 3, 2024, Kobe University said the impact caused Ganymede to shift on its axis as a result.<\/p>\n

The scientists published their results in the peer-reviewed journal Scientific Reports<\/em> on September 3, 2024.<\/p>\n

Furrows on Ganymede<\/h3>\n

In images of Ganymede, you can see long lines called furrows covering much of one side of the moon (see image below). These ancient markings are partly covered by craters from more recent impact events. Previously, scientists in the \u201980s determined that these furrows were the concentric rings of ejecta pointing back to the site of a major impact. Hirata Naoyuki, the lead author of the new study, said: <\/p>\n

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The Jupiter moons Io, Europa, Ganymede and Callisto all have interesting individual characteristics. But the one that caught my attention was these furrows on Ganymede. We know that this feature was created by an asteroid impact about 4 billion years ago. But we were unsure how big this impact was and what effect it had on the moon.<\/p>\n<\/blockquote>\n

\"Left
Ganymede, the largest moon of Jupiter and the largest in our solar system, was hit by an asteroid (near the red cross) some 4 billion years ago. It left behind furrows on the planets surface, which appear as parallel lines in the inset at right. Image via Hirata Naoyuki (CC BY)\/ Kobe University.<\/figcaption><\/figure>\n

Jupiter\u2019s moon Ganymede and the new discovery<\/h3>\n

Ganymede is our solar system\u2019s largest moon. In fact, it\u2019s even larger than the planet Mercury. And beneath Ganymede\u2019s icy surface lies an ocean of liquid water. Also, if we lived on Jupiter, we would only ever see one side of Ganymede, just like we do with Earth\u2019s moon. That\u2019s because both satellites are tidally locked to their planets.<\/p>\n

While examining the furrows on Ganymede, Hirata noticed the impact site is on the opposite side of the moon from Jupiter. This reminded him of a discovery that New Horizons made at Pluto. On Pluto, a huge basin named Sputnik Planitia is likely the result of a giant impact that tilted Pluto\u2019s axis. The press release said: <\/p>\n

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Drawing from similarities with an impact event on Pluto that caused the dwarf planet\u2019s rotational axis to shift and that we learned about through the New Horizons space probe, this implied that Ganymede, too, had undergone such a reorientation. <\/p>\n<\/blockquote>\n

Hirata\u2019s many simulations of impact events on moons and asteroids helped him calculate an impact that would have put this reorientation into motion.<\/p>\n

The giant impact<\/h3>\n

Hirata calculated the asteroid would have had to be around 195 miles (300 km) in diameter. And it would have created an initial crater between 875 to 1,000 miles (1,400 to 1,600 km) in diameter. (That\u2019s before the ejecta settles back in.) This is the size of impact that would be necessary to change the mass distribution to shift the moon\u2019s rotational axis to where it is now. Hirata said:<\/p>\n

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I want to understand the origin and evolution of Ganymede and other Jupiter moons. The giant impact must have had a significant impact on the early evolution of Ganymede, but the thermal and structural effects of the impact on the interior of Ganymede have not yet been investigated at all. I believe that further research applying the internal evolution of ice moons could be carried out next.<\/p>\n<\/blockquote>\n

\"Top
In the top image, we see the distribution of furrows in the hemisphere that always faces away from Jupiter. At bottom is a cylindrical projection map of Ganymede. Gray regions represent younger terrain without furrows. The furrows (green lines) are only on old terrain (black). Image via Hirata Naoyuki (CC BY)\/ Kobe University.<\/figcaption><\/figure>\n

JUICE on route to Jupiter<\/h3>\n

ESA\u2019s JUICE space mission is currently speeding toward Jupiter and its moons. A decade from now, we may know more about Ganymede and better understand what happened during its giant impact some 4 billion years ago.<\/p>\n

Bottom line: About 4 billion years ago, a huge asteroid \u2013 20 times larger than Earth\u2019s dinosaur-killer \u2013 struck Ganymede and tilted the moon\u2019s orientation.<\/p>\n

Source: Giant impact on early Ganymede and its subsequent reorientation<\/p>\n

Via Kobe University<\/p>\n

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Kelly Kizer Whitt<\/h4>\n

View Articles\n <\/p><\/div>\n

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About the Author:<\/h6>\n

Kelly Kizer Whitt has been a science writer specializing in astronomy for more than two decades. She began her career at Astronomy Magazine, and she has made regular contributions to AstronomyToday and the Sierra Club, among other outlets. Her children\u2019s picture book, Solar System Forecast, was published in 2012. She has also written a young adult dystopian novel titled A Different Sky. When she is not reading or writing about astronomy and staring up at the stars, she enjoys traveling to the national parks, creating crossword puzzles, running, tennis, and paddleboarding. Kelly lives in Wisconsin.<\/p>\n<\/p><\/div>\n<\/p><\/div>\n


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