'mysterious' Dents on Phobos' Surface in Mars

Phobos Is a larger satellite and is closer to the surface of Mars than any other satellite in the solar system. Phobos Satellite has a rough outer shell, many deep dents on the surface and has a size ratio 17:22:18 (.

Phobos satellite

Photo source: ESA / DLR / FU Berlin (G. Neukum)

Photos of grooves

Photo source: NASA

The spacecraft flying in Viking 1 Is one of the first spacecraft to go to Mars. This photo was taken on June 10, 1977. The image taken from the. Viking 1 Spacecraft shows all streaks of stripes, deep dents on the surface of the. Phobos Satellite. Astronomers find long parallel grooves that create deep cracks or ". Long stretches " that are caused by Mars's gravitational gravity.

Deep indentations on the surface

Photo source: ESA / DLR / FU Berlin (G. Neukum)

The rear image of the moon Mars has shown a ". Second family " of deep grooves. On July 23, 2008,. Mars Express 's high-resolution Stereo Camera On-board Stereo camera Captured the highest resolution full-disc image of the surface of the moon. Phobos . These images show more clearly small, difficult-to-recognize grooves and are not parallel to tidal channels.

Affected by a large "dent"

Photo source: NASA / JPL-Caltech / University of Arizona.

The Giant Stickney Crater Is the largest feature on the surface of. Phobos , with a length of nearly 9.5 km (. 6 miles ). Underneath the Stickney Crater Is a lunar moon Shaped " Dent " - looking like the shape of a partially deflated ball. The above color photo was taken with the. HiRISE ( High Resolution Imaging Science Experiment ) camera on the Mars Reconnaissance Orbit ship.

Grooves on Phobos surface

Photo source: NASA / JPL-Caltech / University of Arizona.

Researchers believe that these grooves are not entirely caused by gravity. Instead, they think that this groove may be caused by small series of induced impacts. Furthermore, those small dents are not affected by small asteroids or comets, but could be caused by Mars fragments on the moon when large impacts occur on the planet itself.

Moon model "concave" in orbit

Photo source: ESA / DLR / FU Berlin-Neukum; Note: M. Nayak & E. Asphaug.

Recently, researchers at the University of California in. Santa Cruz Decided to test another hypothesis: "What. If the fragments are the cause of a series of small" holes "on. Phobos ' surface? not by Mars ". The illustration above clearly describes the sequence of events and scientists have noted the origin of the moons on Mars. (. The trajectory illustration is drawn in the wrong ratio. )

Predict the shape of the dents.

Photo source: ESA / DLR / FU Berlin-Neukum; Note: M. Nayak & E. Asphaug.

Michael Nayak And Erik Asphaug At the University of California and. Santa Cruz Conducted computer simulations to verify hypotheses about the origin of. Phobos Tracks. The simulation performed on the computer creates a model that describes the basics or initial impact that causes large indents and blows dirt into space. Following are the second and subsequent impacts that moon debris will return to. Phobos' Surface. Model a series of dents in the left-hand image that is similar to the predicted model (. Right ).