|
|
Mercury |
Venus |
Earth |
Mars |
Jupiter |
Saturn |
Uranus |
|
|
diameter (Earth=1) |
0.382 |
0.949 |
1 |
0.532 |
11.209 |
9.44 |
4.007 |
3.883 |
|
Diameter (km) |
4,878 |
12,104 |
12,756 |
6,787 |
142,800 |
120,000 |
51,118 |
49,528 |
|
mass (Earth=1) |
0.055 |
0.815 |
1 |
0.107 |
318 |
95 |
15 |
17 |
|
mean distance
from Sun (AU) |
0.39 |
0.72 |
1 |
1.52 |
5.20 |
9.54 |
19.18 |
30.06 |
|
orbital period
(Earth years) |
0.24 |
0.62 |
1 |
1.88 |
11.86 |
29.46 |
84.01 |
164.8 |
|
eccentricity (e) |
0.2056 |
0.0068 |
0.0167 |
0.0934 |
0.0483 |
0.0560 |
0.0461 |
0.0097 |
|
mean orbital
velocity (km/sec) |
47.89 |
35.03 |
29.79 |
24.13 |
13.06 |
9.64 |
6.81 |
5.43 |
|
rotation
period (in Earth days) |
58.65 |
-243 # |
1 |
1.03 |
0.41 |
0.44 |
-0.72 # |
0.72 |
|
inclination of
axis (degrees) |
0.0 |
177.4 |
23.45 |
23.98 |
3.08 |
26.73 |
97.92 |
28.8 |
|
mean temp at
surface (C) |
-180 to 430 |
465 |
-89 to 58 |
-82 to 0 |
-150 |
-170 |
-200 |
-210 |
|
gravity at
equator (Earth=1) |
0.38 |
0.9 |
1 |
0.38 |
2.64 |
0.93 |
0.89 |
1.12 |
|
escape
velocity (km/sec) |
4.25 |
10.36 |
11.18 |
5.02 |
59.54 |
35.49 |
21.29 |
23.71 |
|
mean density (water=1) |
5.43 |
5.25 |
5.52 |
3.93 |
1.33 |
0.71 |
1.24 |
1.67 |
|
atmospheric
composition |
none |
CO2 |
N2+O2 |
CO2 |
H2+He |
H2+He |
H2+He |
H2+He |
|
rings |
no |
no |
no |
no |
yes |
yes |
yes |
yes |
The orbital eccentricity
(e) is a number which measures how elliptical
orbits are. If e=0, the orbit is a circle. Most planets have eccentricities
close to 0, so they have orbits which are nearly circular.