Venus and Mars Conjunctions
Brilliant white Venus beside the steady red ember of Mars makes one of the prettiest color contrasts in the sky. The two meet a little less than once a year on average, roughly every fourteen months; here are the upcoming and most recent pairings.
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Computing the next conjunction…
| Conjunction date | In the zodiac | How close | Gap since previous |
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Dates and positions are computed live in your browser and are accurate to well under a degree. "How close" is the separation along the ecliptic; the zodiac position is the tropical longitude (0° at the spring equinox).
About this pairing
Venus, at about magnitude minus 4, outshines Mars by a wide margin, so in a Venus-Mars conjunction Venus is the dazzling one and Mars the smaller, distinctly orange point nearby. Their meetings come a little over a year apart on average, and the closest can bring them within a fraction of a degree.
Because Venus is never far from the Sun, these conjunctions sit low in the morning or evening twilight. Mars, an outer planet, ranges all around the zodiac, so the meeting point drifts from one pairing to the next; the table below shows where each one falls and how close the two pass.
For the wider pattern of how often any two planets line up, see the Synodic-Period Calculator, and for a live map of where the planets sit right now, the Live Orrery.
Watching this pair
This is the sky's best color lesson. Put the two in one binocular field and the contrast is immediate: Venus a hard blue-white glare off its unbroken clouds, Mars a small ember tinted by oxidized dust. A camera on a tripod catches the difference even better than the eye does, and a Venus-Mars pairing over a twilight skyline makes a striking photograph with no special gear.
A telescope during the meeting rewards Venus more than Mars. Venus runs through Moon-like phases, and near its meetings with Mars it often shows a fat gibbous or half disk at modest magnification, while Mars, far across the solar system at these times, stays a tiny featureless dot. The pairing makes the geometry vivid: one neighbor caught near our side of the Sun, the other almost behind it.
Photographing Venus and Mars
A Venus-Mars meeting is within reach of a phone, but a little care lifts the result. Brace the phone or set a camera on a tripod, tap to focus on Venus, and lower the exposure so the bright planet stays a clean point rather than a bloom. During late twilight, a wide frame that keeps the horizon and a foreground low in the shot lets the two planets ride the fading color band, so the scene reads as a landscape rather than two dots on black.
To bring out the hue of Mars, resist letting the sky go fully black; the contrast reads best while a little blue still lingers behind the pair. A moderate telephoto tightens the two without losing that background, and because Venus is so much brighter you should expose for Venus and let Mars sit as the fainter, warmer point beside it. Bracketing a few frames is worth doing, since the pair sits low and the thicker air near the horizon can dim Mars more than you expect.
Why Venus outshines the red planet
The size of that gap comes down to three things pulling the same way. Venus is nearly twice the diameter of Mars, orbits closer to both the Sun and to us, and its unbroken cloud deck returns about seventy percent of the sunlight that strikes it, against roughly a quarter for the dusty Martian surface. During most conjunctions Mars also lies near the far side of its orbit from Earth, at its smallest and faintest, which widens the gap further.
Because Venus never wanders far from the Sun, every Venus-Mars meeting sits in morning or evening twilight, and the best of them fall when Venus is near its greatest elongation and the pair stands highest in a darker sky. Venus itself returns to nearly the same place every eight years, the rhythm that draws the Venus pentagram, though Mars has wandered on by then, so each meeting falls in a fresh stretch of the zodiac.
There is a quiet geometric catch to this pairing worth knowing. A conjunction puts Mars in the same direction as Venus, and Venus never strays far from the Sun, so Mars too must sit fairly close to the Sun in our sky whenever the two meet. That rules out the one thing that would make Mars spectacular: it can never be near opposition, on the far side of the sky from the Sun, at a Venus-Mars conjunction, and opposition is when Mars comes closest to Earth and blazes at its brightest. Every meeting of these two therefore catches the red planet somewhere on the modest side of its range, often near the far end of its orbit, small and dim. It is part of why Venus wins the contrast so completely, and why the color of Mars, rather than its brightness, is what you come to these pairings to see.
Frequently asked questions
How often do Venus and Mars meet?
A little less than once a year on average, roughly every fourteen months. Because Venus stays close to the Sun, the pairing is always low in the morning or evening twilight, and the meetings cluster near the times Mars passes behind the Sun; the exact dates are in the table above.
How do you tell Venus and Mars apart?
Venus is the dazzling white one, near magnitude minus 4, while Mars is a fainter, distinctly orange point nearby. The color and brightness contrast is the easiest way to identify them.
Why is Mars so much fainter than Venus?
Several things stack up the same way: Venus is larger, closer to both the Sun and to us, and wrapped in bright unbroken cloud, while Mars is smaller and its rusty surface reflects far less light. During a conjunction Mars also stands near the far side of its orbit from Earth, at its smallest and dimmest, which widens the gap further.
Which Venus-Mars conjunctions are the best to watch?
The ones that fall farthest from the Sun in the sky. When a meeting comes while Venus is near its greatest elongation, the pair stands higher in a darker twilight and the color contrast shows at its best; meetings buried deep in bright twilight are technically close but hard to enjoy.
When is the best time of night to see a Venus-Mars conjunction?
During deep twilight, about 30 to 60 minutes after sunset for an evening meeting or before sunrise for a morning one, when the sky is dark enough for Mars to show its color but the pair has not yet sunk into the horizon haze. A clear, low horizon in the right direction matters more than any equipment.
Other conjunctions
Keep exploring
Planetary Alignment Calculator
Conjunction and opposition dates for any pair of planets, and multi-planet line-ups.
SkyToday in the Sky
Where the Sun, Moon and planets sit right now, and the next sky events.
InteractiveThe Live Orrery
Watch the planets move and see these meetings unfold from above.