Orbital Data for the Planets & Dwarf Planets
| Planet |
Semimajor Axis (AU) |
Orbital Period (yr) |
Orbital Speed (km/s) |
Orbital
Eccentricity
(e) |
Inclination of Orbit to Ecliptic (°) |
Rotation Period (days) |
Inclination of Equator to Orbit (°) |
| Mercury |
0.3871 |
0.2408 |
47.9 |
0.206 |
7.00 |
58.65 |
0 |
| Venus |
0.7233 |
0.6152 |
35.0 |
0.007 |
3.39 |
-243.01* |
177.3 |
| Earth |
1.000 |
1 |
29.8 |
0.017 |
0.00 |
0.997 |
23.4 |
| Mars |
1.5273 |
1.8809 |
24.1 |
0.093 |
1.85 |
1.026 |
25.2 |
| Jupiter |
5.2028 |
11.862 |
13.1 |
0.048 |
1.31 |
0.410 |
3.1 |
| Saturn |
9.5388 |
29.458 |
9.6 |
0.056 |
2.49 |
0.426 |
26.7 |
| Uranus |
19.1914 |
84.01 |
6.8 |
0.046 |
0.77 |
-0.746* |
97.9 |
| Neptune |
30.0611 |
164.79 |
5.4 |
0.010 |
1.77 |
0.718 |
29.6 |
|
| Ceres |
2.76596 |
4.599 |
17.882 |
0.07976 |
10.587 |
0.378 |
~3 |
| Pluto |
39.5294 |
248.54 |
4.7 |
0.248 |
17.15 |
-6.4* |
122.5 |
| Haumea |
43.335 |
285.4 |
4.484 |
0.18874 |
28.19 |
0.163 |
? |
| Makemake |
45.791 |
309.88 |
4.419 |
0.159 |
28.96 |
? |
? |
| Eris |
67.6681 |
557 |
3.436 |
0.44177 |
44.187 |
> 8 hrs ? |
? |
* Negative values of rotation period indicate that the
planet rotates in the direction opposite to that in which it orbits
the Sun. This is called retrograde rotation.
The semimajor axis (the average distance to the Sun) is given in units
of the Earth's average distance to the Sun, which is called an AU.
For example, Neptune is 30 times more distant from the Sun than the
Earth, on average. Orbital periods are also given in units of the
Earth's orbital period, which is a year.
The eccentricity (e) is a number which
measures how elliptical orbits are. If e = 0, the orbit is a circle.
Most of the planets have eccentricities close to 0, so they must have
orbits which are nearly circular.


Shop Windows to the Universe Science Store!
The
Winter 2010 issue of The Earth Scientist, which includes articles on meteor cratering, classroom glaciers, podcasts in the classroom, and pyro-cumulonimbus clouds, is available in our
online store.
You might also be interested in:

Most objects in orbits move along an elliptical path. An ellipse is a shape that can be thought of as a "stretched out" circle or an oval. An ellipse can be very long and thin, or it can be quite
...more
In 2006 the International Astronomical Union (IAU) approved a new classification scheme for planets and smaller objects in our Solar System. Their scheme includes three classes of objects: "small solar
...more
Pluto is a frigid ball of ice and rock that orbits far from the Sun on the frozen fringes of our Solar System. Considered a planet, though a rather odd one, from its discovery in 1930 until 2006, it was
...more
Makemake is a dwarf planet in our Solar System. Makemake was discovered on March 31, 2005 by a team of astronomers led by Mike Brown of the California Institute of Technology. The International Astronomical
...more
Eris is a dwarf planet that was discovered in 2005. Eris is a trans-Neptunian object (TNO) that orbits the Sun on the frozen fringes of our Solar System beyond the Kuiper Belt. Eris takes 557 years to
...more
When one object is in orbit around another object, the orbit is usually an elliptical orbit. For example, all of the planets in our Solar System move around the Sun in elliptical orbits. An ellipse is
...more
Kepler's second law he again discovered by trial and error. After some experimentation, Kepler realized that the line connecting the planet and the Sun sweeps out equal area in equal time. Look at the
...more