New Maps of Mercury Show Icy Looking Craters on the Solar System's Innermost Planet A NASA spacecraft bolsters the case that ice lines the inside of
polar craters on Mercury
But some places on Mercury are slightly more stable.Inside
polar craters on the diminutive planet are regions that never see the light of day, shaded as they are by the craters» rims.
Not exact matches
Many scientists think these permanently shadowed regions, such as the floors
on impact
craters in the Moon's
polar regions, could hold large deposits or water ice.
The researchers discovered that the reflective features
on the map match
polar craters seen by Mariner 10 if the positions deduced from the spacecraft are about 1.5 degrees in error.
A spent rocket stage that NASA sent hurtling into the moon last year in hopes of kicking up water from a
polar crater delivered
on that mission, revealing that at least a moderate portion of its target was indeed made of ice.
Among them: How do the materials trapped in
polar craters arrive
on the moon?
On Tuesday, the team successfully executed the last of seven daring orbit correction maneuvers that kept MESSENGER aloft long enough for the spacecraft's instruments to collect critical information on Mercury's crustal magnetic anomalies and ice - filled polar craters, among other feature
On Tuesday, the team successfully executed the last of seven daring orbit correction maneuvers that kept MESSENGER aloft long enough for the spacecraft's instruments to collect critical information
on Mercury's crustal magnetic anomalies and ice - filled polar craters, among other feature
on Mercury's crustal magnetic anomalies and ice - filled
polar craters, among other features.
Most recently,
on May 12, Hubble's Wide Field Camera 3 captured the surface of Mars in stunning detail, revealing russet deserts pockmarked with
craters and bright frosty
polar caps shrouded in a thin haze of clouds.
Scientists thought most of Vesta outside the south
polar region might be flat like the Moon, yet some of the
craters outside that region formed
on very steep slopes and have nearly vertical sides, with landslides often occurring in the regolith, the deep layer of crushed rock
on the surface.
On March 21, 2012, the MESSENGER team also revealed new supporting evidence that many permanently shadowed
craters in Mercury's
polar regions may harbor water ice insulated with a thin layer of soil or dust, or some other radar - reflecting volatile substance such as sulfur.
The most conspicuous feature
on Vesta is a giant impact
crater located around its south
polar region, which is 310 miles (499 kilometers) across and nearly 12 miles (19 km) deep around a «bull's - eye» central peak rising 11 miles (or 18 km) above the exposed mantle rock of the
crater floor — that is characteristic of rock rebounding from an impact.