Mercury

Pete's Pages

Home page

Observatory

Telescopes

CCD Cameras

Focusing CCD Cameras

Software

Sundrie astronomy equipment

Palm Pilot atronomy software

CCD Images

Lists,Data & Tables

Astronomy links


Back to Lists & Tables.
Mercury
Venus
Mars
Minor Planets.

Jupiter
Saturn
Uranus
Neptune
Pluto
 
DATA
Distance from the SUN Mean: 57.9 million Km (0.387 au.)
Max: 69.7 million Km (0.467 au.)
Min: 45.9 Km (0.306 au.)
Sidereal period  87.969 days  
Syodic period 115.88 days
Rotation period 58.6461 days
Mean orbital velocity 47.87 Km/sec
Axial inclination Negligible
Orbital inclnation 7 deg 0.0 min 15 sec
Diameter Equatorial: 4878 Km
Apparent Diameter from Earth max : 12 sec .9
min: 4 sec .5
Reciprocal Mass (Sun = 1) 6000000
Density (water =1) 5.44
Mass (Earth = 1) 0.055
Volume (Earth = 1) 0.150
Escape Velocity 4.25 km/sec
Surface gravity (Earth = 1) 0.38
Mean surface temperature Day: +350°C
Night: -183°C
Oblateness Negligible
Albedo 0.06
Maximum Magnitude -1.9
Mean Diameter of Sun as seen from Mercury 1 deg 22 min 40 sec


Predicted transites of Mercury accross the Sun

Date Time of mid transit (UT)
7 May 2003 7h 53m
8 November 2006 21h 42m
9 May 2016 14h 59m
11 November 2019 15h 21m



Description.

Mercury is the innermost of all the planets, and the fastest to go around the Sun. It is the second smallest both in size & mass, the smallest being Pluto. It is virtually without atmosphere. What little atmosphere it does have was probably captured from Solar winds. (The stream of atomic particles thrown out by the Sun.) Mercury has a weak magnetic field of unknown origin. Mercury, seen close up by NASA's Mariner 10 space probe in 1974\1975, resembles that of the Moon. It is heavily cratered by meteorite impacts & has vast lava seas as well as mountainous regions. The surface facing the sun is very hot at about 400°C while the surface not facing the Sun is at -170 °C. This is because there is no atmosphere to circulate the heat around the planet. Mercury rotates on it's axis very slowly, only one & half times for every revolution around the Sun. This means its day is very long, 59 Earth days & its year is very short, 88 Earth days. Its orbit is very eccentric as well so its speed varies greatly. These variations produce some unique effects. As seen from Mercury the Sun would rise in the East, stop, then set in the East. Then it would rise again, move slowly across the sky & set in the West. Then it would rise in the West, stop, then set finally in the West. Mercury has no satellites.

This document maintained by pete.cox@zetnet.co.uk.
Material Copyright © 2000 Pete