MERCURY, THE WINGED MESSENGER

Mercury was known to the Romans as the messenger to the gods.
It is the closest planet to the sun and hurtles round our star every 88 days. It is the second smallest planet, after Pluto. Mercury has an iron core that extends three quarters of the way to its surface. This suggests that at one time Mercury was considerably larger. It appears that a hefty blow from a stray object in its distant past may have blown much of its original rocky shell off into space. This is not the only scar Mercury displays from major collisions. The Caloris Basin is one of the largest impact craters in the solar system. At 800 miles across it is bigger than the British Isles. The impact was so great that the shock waves created rocky ridges on the other side of the planet.

Although the Mercurian year is very short, the days (and nights) drag on. Mercury spins on its axis quite slowly and only fits in one and a half days to its year. If you were to visit the planet you would have to suffer interminably long nights where the temperature drops to -280 degrees Farenheit. At dawn the temperature would quickly soar and as the huge sun edged its way across the sky the barren landscape would heat up to 800 degrees farenheit.

A visitor to the planet would also witness some of the most peculiar sunsets in the solar system.
Sometimes Mercury's rapid motion round the sun outpaces it's genteel rotation. If this happens at sunset, the sun will dip below the horizon then pop back up again for a couple of days before sinking back down again plunging you into the long cold night.


Mercury Statistics
 Equatorial radius (km)2,439.7 
 Mean distance from the Sun (km)57,910,000 
 Mean distance from the Sun (Earth = 1)0.3871 
 Rotational period (days)58.6462 
 Orbital period (days)87.969 
 Mean surface temperature179°C 
 Maximum surface temperature427°C 
 Minimum surface temperature-173°C 
 Atmospheric composition
Helium
Sodium
Oxygen
Other

42% 
42% 
15% 
1% 

OBSERVING MERCURY

Mercury is one of the hardest planets to see. Most of the time it is lost in the glare of the sun and only on a few occasions each year does it become visible.



Return to Planets Page




Return to Home Page

Return to Home Page