The Moon and Mercury, the closest planet to the Sun, may contain significantly more water ice than previously thought, according to a new analysis of data from NASA spacecraft. The potential ice deposits are found in craters near the poles of both worlds. In the past, telescopic observations and orbiting spacecraft have found glacier-like ice deposits on Mercury, but as of yet not on the Moon. The new work raises the possibility that thick ice-rich deposits also exist on the Moon.
- The research may not only help resolve the question regarding the Moon’s apparent low ice abundance relative to Mercury, but it could also have practical applications.
- The poles of Mercury and the Moon are among the coldest places in our solar system. Unlike Earth, the spin axes of Mercury and the Moon are oriented such that, in their polar regions, the Sun never rises high above the horizon. Consequently, polar topographic depressions, such as impact craters, never see the Sun.
- For decades it has been postulated these so-called permanently shadowed regions are so cold that any ice trapped within them can potentially survive for billions of years. Previous observations of the poles of Mercury with Earth-based radar revealed a signature characteristic of thick, pure ice deposits. Later, MESSENGER spacecraft imaged these ice deposits.
- Mercury’s ice deposits appear to be much less patchy than those on the Moon, and relatively fresh, perhaps emplaced or refreshed within the last tens of millions of years.
- Previous radar and imaging studies of the Moon, whose polar thermal environments are very similar to those of Mercury, found only patchy, shallow ice deposits.
- The airless surfaces of Mercury and the Moon are scarred by many impact craters. These craters form when meteoroids or comets impact the surface. The team analysed simple craters that are formed by smaller, less energetic impactors.
- These depressions are held together by the strength of the surface dust layer, or regolith and tend to be more circular and symmetrical than large craters. The scientists exploited this inherent symmetry to estimate the thickness of ice trapped within simple craters.
- The study used elevation data obtained by MESSENGER and LRO to measure approximately 15,000 simple craters with diameters ranging from 2.5 kilometre (km) to 15 km on Mercury and the Moon.
- Researchers found that craters become up to 10 per cent shallower near the north pole of Mercury and the south pole of the Moon, but not the north pole of the Moon. The researchers concluded that the most probable explanation for these shallower craters is the accumulation of previously undetected thick ice deposits on both worlds.
- They found that the pole-facing slopes of these craters are slightly shallower than their equator-facing slopes, and that the shallowing is more significant in regions that promote ice stability because of Mercury’s orbit around the Sun.
- The topographic signal detected by the scientists is relatively more prominent in smaller simple craters, but does not preclude the possibility that ice may be more widespread in larger craters across the lunar pole.