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Tharsis bulgeLive Science
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76% Informative
A long-lost moon could explain why Mars is so different from the other rocky planets in the solar system.
Nerio 's mass altered the shape of Mars with its gravity, raising tides in the magma oceans.
Because Mars is smaller than Earth , it cooled much more quickly and its tidal bulges became locked into the resulting form of the planet.
It could have been obliterated by a collision, leaving behind the current moons Phobos and Deimos .
VR Score
87
Informative language
92
Neutral language
35
Article tone
formal
Language
English
Language complexity
57
Offensive language
not offensive
Hate speech
not hateful
Attention-grabbing headline
not detected
Known propaganda techniques
not detected
Time-value
long-living
External references
3
Source diversity
3