Mercury

Mercury combines a strongly heated dayside with polar craters whose floors remain permanently shaded. Radar reflections, MESSENGER’s hydrogen measurements and temperature models support deposits of water ice in these cold traps. Its low axial tilt makes that contrast possible: proximity to the Sun does not illuminate every piece of ground. The polar deposits preserve a record of volatile delivery and survival on a largely airless rocky planet.

Mean diameter
4,879 km
Rotation
58.65 Earth days
Year
0.24 Earth years
Mercury

NASA VTAD · reference globe

MESSENGER view of Caloris, one of Mercury’s largest impact basins. NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington/Brown University

Caloris basin

An impact followed by lava

A basin about 1,550 kilometres wide preserves a sequence of impact, lava flooding and younger craters. Read the overlapping terrain in MESSENGER’s observations.

More investigations

Through the instruments

Open an image for the full frame and its source.

Missions & milestones

3 launch records · 11 linked events

14 related records

Programs (1)
About these records

The source cohort includes dedicated missions, attempts and reviewed scientific flybys or gravity assists. Launch outcomes describe the recorded flight. They do not establish whether an old spacecraft is operating today. Events show published targets unless the record confirms an outcome.

Mercury & Earth

Earth12,742 km
Mercury4,878.8 km

Mean diameters on one scale. Separation is omitted.

Rotation
58.65 Earth days · sidereal rotation
Solar day
175.94 Earth days
Orbital period
88 Earth days
Surface gravity
3.70 m/s² 0.38 × Earth
Mean distance from the Sun
0.39 AU
Surface pressure
Tenuous exosphere

Earth–Mercury radio time

One way8.34 min
There and back16.68 min

Choose a reference Earth–Mercury separation. Radio travel time is calculated in vacuum; the range is illustrative, not a current ephemeris.