What’s up in the sky in November?
A Celestial Show for Early Birds
On its orbit around the Sun, Venus will soon be swinging into prime position for Earthly stargazers. The planet will reach peak brightness in late November, when it will shine just before sunrise as the “Morning Star.”
Venus will reach peak brightness on November 27, 2026.
With an apparent magnitude of −4.87, the planet will shine more than 20 times brighter than Sirius, the brightest star in the sky.
While it will be visible in the pre-dawn sky from both hemispheres, northern observers will have a slightly better vantage point to view the spectacle as Venus will be above the horizon well before sunrise; south of the equator, it will first become visible during morning twilight, especially in the far south.
See how it will look in New York, USA, and Sydney, Australia.
Find Your Best Venus Moment
Of course, Venus will be a sight to behold even in the days and weeks before and after the peak date. So, if your sky is cloudy on the day, there are still plenty of chances to marvel at Venus in all its glory.
Here are some handy tools to help you plan your Venus spotting adventure:
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Our Planet Tracker Tool shows the apparent brightness of Venus and the other planets on a date of your choice. Click Brightness at the top, then use the controls at the bottom to choose the date.
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Our Night Sky Map helps you find Venus in your sky.
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If lighting is important to you—for example, if you want to take photos—use our Sun Calculator to check sunrise, sunset, and twilight times for your location.
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Before you head out, it might also be worth checking your local weather forecast.
Evening Prelude in September
This is the second time that Venus’s brightness peaks this year. The last time was on September 22, when the planet graced the evening skies with a slightly lower apparent magnitude of −4.78.
That time, stargazers in the Southern Hemisphere had a front-row seat as Venus was fairly high in the sky at sunset. North of the equator, it disappeared behind the horizon during evening twilight.
See how it looked in Sydney, Australia, and New York, USA.
Brightest During the Crescent Phase
The two moments of peak brightness occur on either side of Venus’s inferior conjunction on October 24, 2026, the moment when it passes (roughly) between Earth and the Sun. See what happens when it aligns perfectly.
For a few days around this date, Venus disappears from view entirely as it is swallowed by the Sun’s glare.
In the weeks before and after, however, we view Venus from an angle that makes a small portion of its illuminated side visible to us. In other words, we’re looking at Venus’s crescent phases—waning in September and waxing in November.
These are the moments the planet reaches peak brightness in the sky.
Why a Crescent Venus Is Brighter than a Full Venus
This may sound counterintuitive. After all, the Moon is clearly brightest at Full Moon.
But there’s a key difference between the two: their distance from Earth. The Moon’s distance, while varying by a few tens of thousands of kilometers, remains relatively constant as it cycles through the phases. That’s because it orbits Earth, so it always stays in our neighborhood, and its phases don’t have any direct influence on its distance from Earth.
With Venus, it’s a completely different story. It orbits the Sun, not Earth, so its distance from us varies much more dramatically and is directly linked to its phases.
At inferior conjunction on October 24—at its shortest distance from Earth—it is just shy of 41 million kilometers (25.5 million miles) away from us. This is the “New Venus” phase, when we face its nightside, and it becomes invisible to us—just like a New Moon.
At superior conjunction, on the other hand, it is at the far side of the Sun, as seen from Earth. This is the “Full Venus” phase when we face the entire illuminated half. At this point, however, Venus is much, much farther away from us: For example, the distance will be 259 million kilometers (161 million miles) at the next superior conjunction on August 11, 2027. That’s a difference of 218 million kilometers, or 135.5 million miles.
That’s why a thin Crescent Venus easily outshines a Full Venus in our sky: It is simply more than six times closer to us.
Despite its relative proximity, however, Venus will appear only as a bright light in the sky to the naked eye. It’s still very, very far away, so binoculars with sufficient magnification or, better yet, a small telescope are needed to clearly see its crescent shape.
Discover the hidden patterns of Venus’s movement across the sky