Planet Distance Now
See the current approximate distance from Earth and the Sun to every major planet, calculated in your browser from NASA/JPL low-precision orbital elements.
Planet distances from Earth change every day because Earth and the planets orbit the Sun at different speeds.
Use the Planet Distance Now
Calculating...
Distances are center-to-center approximations calculated from NASA/JPL Table 1 orbital elements (valid 1800–2050). Values refresh every 60 seconds. For precision ephemerides, use NASA JPL Horizons. Approaching or receding speed is the change in Earth–planet distance per second (range rate).
How Far Each Planet Gets From Earth (2000–2050)
Closest, average and farthest Earth–planet distance from the same orbital model, with the one-way light time at the average distance.
| Planet | Closest | Average | Farthest | Light time (avg) |
|---|---|---|---|---|
| Mercury | 0.549 AU 82M km |
1.039 AU 155M km |
1.452 AU 217M km |
8.6 min |
| Venus | 0.265 AU 40M km |
1.137 AU 170M km |
1.736 AU 260M km |
9.5 min |
| Mars | 0.373 AU 56M km |
1.696 AU 254M km |
2.675 AU 400M km |
14.1 min |
| Jupiter | 3.952 AU 591M km |
5.260 AU 787M km |
6.454 AU 966M km |
43.7 min |
| Saturn | 8.041 AU 1,203M km |
9.575 AU 1,432M km |
11.032 AU 1,650M km |
1 h 20 min |
| Uranus | 17.290 AU 2,587M km |
19.377 AU 2,899M km |
21.089 AU 3,155M km |
2 h 41 min |
| Neptune | 28.820 AU 4,311M km |
29.916 AU 4,475M km |
31.101 AU 4,653M km |
4 h 9 min |
Mars Closest Approaches 2027–2050
Mars comes closest about every 26 months, near opposition. Approaches near Mars' perihelion (2035, 2050) are the closest; dates are UTC.
| Date | Distance (AU) | Million km | Million mi | Light time |
|---|---|---|---|---|
| Feb 20, 2027 | 0.678 | 101.4 | 63.0 | 5.6 min |
| Mar 29, 2029 | 0.647 | 96.8 | 60.2 | 5.4 min |
| May 12, 2031 | 0.553 | 82.8 | 51.4 | 4.6 min |
| Jul 5, 2033 | 0.423 | 63.3 | 39.3 | 3.5 min |
| Sep 11, 2035 | 0.380 | 56.9 | 35.4 | 3.2 min |
| Nov 11, 2037 | 0.494 | 73.8 | 45.9 | 4.1 min |
| Dec 28, 2039 | 0.611 | 91.4 | 56.8 | 5.1 min |
| Feb 5, 2042 | 0.672 | 100.5 | 62.4 | 5.6 min |
| Mar 14, 2044 | 0.667 | 99.8 | 62.0 | 5.5 min |
| Apr 24, 2046 | 0.597 | 89.3 | 55.5 | 5 min |
| Jun 12, 2048 | 0.474 | 70.9 | 44.1 | 3.9 min |
| Aug 15, 2050 | 0.374 | 56.0 | 34.8 | 3.1 min |
Quick answer
Planet distances from Earth change every day because Earth and the planets orbit the Sun at different speeds. Venus can come as close as about 0.27 AU (40 million km) and Mars about 0.37 AU (56 million km), while Neptune never gets nearer than about 28.8 AU (4.3 billion km).
Examples
| Planet | Closest (million km) | Farthest (million km) |
|---|---|---|
| Mercury | 82 | 217 |
| Venus | 40 | 260 |
| Mars | 56 | 400 |
| Jupiter | 591 | 966 |
| Saturn | 1,200 | 1,650 |
| Neptune | 4,310 | 4,650 |
Open the live table to see today's distance to every planet in AU, km or miles, sorted closest to farthest, with light travel time.
Summary
This tool calculates the approximate current distance from Earth to each planet using simplified Keplerian orbital elements and the date/time on your device. Planetary positions are computed from published mean orbital elements, then the Earth-to-planet straight-line distance is derived from their heliocentric coordinates. Results update every minute and are expressed in both astronomical units (AU) and millions of kilometers.
How it works
- Your browser reads the current date and time.
- Each planet's heliocentric position is estimated from NASA/JPL Table 1 mean orbital elements and secular rates, a low-precision model valid from 1800 through 2050.
- The Earth-Moon barycenter position is computed with the same model.
- The center-to-center straight-line distance is derived from the 3-D heliocentric coordinates.
- The approach or recession speed is the change in that distance over two hours, and the next closest approach is the first minimum found by stepping forward one day at a time and refining it.
- Results are displayed in AU, millions of kilometers or millions of miles and refresh every 60 seconds. Pick a date to see past or future distances instead.
Use cases
- Satisfy curiosity about how far Mars or Jupiter is from Earth right now.
- Support classroom discussions about the dynamic nature of planetary distances.
- Compare which major planets are currently nearest to or farthest from Earth.
- Understand why communication delays to Mars missions vary so dramatically.
- Illustrate how the solar system is in constant motion.