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.

PlanetClosestAverageFarthestLight 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.

DateDistance (AU)Million kmMillion miLight 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
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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

PlanetClosest (million km)Farthest (million km)
Mercury82217
Venus40260
Mars56400
Jupiter591966
Saturn1,2001,650
Neptune4,3104,650

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

  1. Your browser reads the current date and time.
  2. 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.
  3. The Earth-Moon barycenter position is computed with the same model.
  4. The center-to-center straight-line distance is derived from the 3-D heliocentric coordinates.
  5. 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.
  6. 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.

Frequently Asked Questions

Last updated: 2026-10-09 · Reviewed by Nham Vu