Mars’ moon Phobos tagged posts

Experiments unravelling the Mystery of Mars’ Moon Phobos. What causes the Weathering of the Mars moon Phobos?

© NASA/JPL-Caltech/University of Arizona

There is no weather in space – but there is weathering: Celestial bodies are bombarded by high energy particles. On the Mars moon Phobos, the situation is complicated: It is hit by particles from the sun, but it is partly shielded by Mars. New experiments explain what is going on, in 2024 a space mission will reach Phobos and check the results.

Of course, there is no weather in our sense of the word in space — nevertheless, soil can also “weather” in the vacuum of space if it is constantly bombarded by high-energy particles, such as those emitted by the sun...

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Anomalous Grooves on Martian moon Phobos explained by Impacts

In this spacecraft image of Phobos, red arrows indicate a chain of small craters whose origin researchers were able to trace back to a primary impact at the large crater known as Grildrig. Credit: ESA/Mars Express, modified by Nayak & Asphaug; copyrighted image

In this spacecraft image of Phobos, red arrows indicate a chain of small craters whose origin researchers were able to trace back to a primary impact at the large crater known as Grildrig. Credit: ESA/Mars Express, modified by Nayak & Asphaug; copyrighted image

Some of the mysterious grooves on Mars’ moon Phobos are the result of debris ejected by impacts eventually falling back onto the surface to form linear chains of craters, according to a new study. One set of grooves on Phobos are thought to be stress fractures resulting from the tidal pull of Mars. The new study addresses another set of grooves that do not fit that explanation. “These grooves cut across the tidal fields, so they require another mechanism...

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Scientists are closer to solving the mystery of how Mars’ moon Phobos formed: Phobos in the mid- and far-ultraviolet

Phobos as observed by MAVEN's Imaging Ultraviolet Spectrograph. Orange shows mid-ultraviolet (MUV) sunlight reflected from the surface of Phobos, exposing the moon's irregular shape and many craters. Blue shows far ultraviolet light detected at 121.6 nm, which is scattered off of hydrogen gas in the extended upper atmosphere of Mars. Phobos, observed here at a range of 300km, blocks this light, eclipsing the ultraviolet sky. Credit: CU/LASP and NASA

Phobos as observed by MAVEN’s Imaging Ultraviolet Spectrograph. Orange shows mid-ultraviolet (MUV) sunlight reflected from the surface of Phobos, exposing the moon’s irregular shape and many craters. Blue shows far ultraviolet light detected at 121.6 nm, which is scattered off of hydrogen gas in the extended upper atmosphere of Mars. Phobos, observed here at a range of 300km, blocks this light, eclipsing the ultraviolet sky. Credit: CU/LASP and NASA

At the end of 2015, NASA’s Mars Atmosphere and Volatile Evolution (MAVEN) mission made a series of close approaches to the Martian moon Phobos, collecting data from within 300 miles of the moon. Among the data returned were spectral images of Phobos in the ultraviolet...

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