planetary conjunction
notableMoon–Mars conjunction
The apparent ecliptic longitudes of Moon and Mars meet. Their calculated geocentric angular separation is 0.22°; this is a line-of-sight alignment, not a close physical approach.
Where to look
Local visibility depends on altitude, twilight, and horizon; conjunction geometry is calculated geocentrically.
Technical source record
2.1.19 · 2025-01-14T03:47:49.555Z · retrieved 2026-09-30
Calculated by: Astronomy Engine apparent geocentric ecliptic-longitude root search in 0.5-day samples, refined by bisection; reported angular separation from apparent geocentric equatorial vectors.
ObserverExample sky· UTC
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