Compressed distance uses a square-root transform to fit all eight planets. Switch to linear in the Solar System tab to see why the inner planets disappear near the Sun.
Astronomy & Space Simulator
Travel through an interactive solar system, compare planets, follow the Moon’s phases, and discover just how vast space really is.
Positions at the selected date
Heliocentric ecliptic coordinates, approximate radial distance and speed. Distances use AU; longitudes and latitudes use degrees.
| Planet | Sun distance (AU) | Longitude (°) | Latitude (°) | Speed (km/s) |
|---|
Two worlds, side by side.
Choose any two planets. The size illustration uses the same diameter scale for both circles.
Circles share a diameter scale (largest circle = 160 px). Colors and textures are illustrative.
The Moon is always changing.
See how the illuminated portion changes across a 29.53-day lunar cycle.
Travel through the lunar cycle
Estimated upcoming phases
Idealized dates in UTC; not suitable for planning observations.
Space is mostly… space.
Measure distances between worlds at the selected simulator date, or explore their average distances from the Sun.
Distances are between modeled 3D heliocentric positions, not fixed orbital radii. Actual light-time calculations require more precise ephemerides.
Average Sun distance (AU)
1 AU = 149.6 million km. Bars show mean semimajor axis, not the changing distance between planets.
What if the Sun were a small ball?
Set the Sun’s model diameter to see how tiny the planets would be and how far away their mean orbits would sit. Sizes and distances in this table share one true scale.
| Planet | Planet diameter (mm) | Orbit radius (m) |
|---|
Mean orbit radius is the semimajor axis; planetary positions and actual separations change over time.
Planet diameters span almost 30×, while orbit sizes span nearly 80× from Mercury to Neptune. One single view cannot keep both realistic and readable.