Planet Position Calculator

Compute approximate ecliptic longitude and distance from the Sun for all 8 planets on any date using simplified Keplerian orbital mechanics.

Select Date

Approximate positions only. Computed using simplified Keplerian mean motion with first-order equation-of-center correction. Perturbations from other planets are not modeled. Accuracy is typically 1–3 degrees.

Select a date and click Calculate Positions

Summary

Compute approximate ecliptic longitude and distance from the Sun for all 8 planets on any date using simplified Keplerian orbital mechanics.

How it works

  1. Select a date using the date picker (defaults to today).
  2. Click "Calculate Positions" to run the orbital mechanics computation.
  3. The calculator computes the Julian Day Number for the selected date.
  4. For each planet, it derives the mean anomaly from the orbital period and mean longitude at J2000.0.
  5. Using the equation of center approximation, it converts mean anomaly to true anomaly.
  6. Ecliptic longitude is computed and normalized to 0–360 degrees.
  7. Heliocentric distance is computed from the elliptical orbit equation using true anomaly.
  8. Results are displayed in a sortable table with longitude, distance, and constellation zone.

Use cases

Frequently Asked Questions

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Last updated: 2026-05-29 · Reviewed by Nham Vu