Venus in the Sky: When and How to See the Brightest Planet
Venus is one of the easiest planets to see with your own eyes. Often shining as a brilliant white “star” after sunset or before sunrise, Venus is the brightest planet in Earth’s sky. In this article, you’ll learn when to see Venus in 2026, how to find it in the sky, why it shines so brightly, and what makes this hot, toxic world so fascinating. Use the free Sky Tonight app to locate Venus in the sky above you.
Contents
- Venus at a glance
- Can you see Venus from Earth?
- When and where is Venus visible in 2026?
- What color is Venus?
- Why is Venus so bright?
- Why does Venus appear as the Morning or Evening Star?
- Venus facts
- Who discovered Venus?
- How many moons does Venus have?
- How big is Venus?
- Venus’ temperature
- Venus’ orbit and rotation
- How far away is Venus?
- Missions to Venus
- What is Venus made of?
- F.A.Q.
- Planet Venus: to sum up
Venus at a glance
- Visible right now: yes, in the evening sky above the western horizon
- Visible with the naked eye: yes, looks like a bright white “star”
- When to see in 2026: February through September in the evening sky; November onward in the morning sky.
- Greatest brightness in 2026: late September, at magnitude –4.8.
Can you see Venus from Earth?
Yes — Venus is easy to see from Earth, even without any equipment. It usually looks like a very bright white dot low above the horizon shortly before sunrise or after sunset. Venus is the brightest planet in our sky and the second-brightest natural object in the night sky after the Moon.
Here’s what Venus looks like through different observing tools:
- Naked eye: a steady, brilliant white point of light, often visible even in twilight.
- Binoculars: a very bright tiny disk rather than a detailed planet. With steady hands, good optics, and favorable conditions, you may notice that Venus is not perfectly round and even glimpse its phase.
- Telescope: a small bright disk with phases, from nearly full to crescent-shaped. You won’t see Venus’ surface, but you’ll be looking at its thick, reflective cloud cover.
When observing Venus near sunrise or sunset, make sure not to point binoculars or a telescope anywhere close to the Sun.
When and where is Venus visible in 2026?
From February through August 2026, the planet appears in the evening sky, improving its visibility. On August 15, Venus will reach its greatest eastern elongation, appearing farthest from the Sun in the evening sky.
Venus will remain well placed in the evening sky until late September. In early October, its visibility will depend strongly on your location. In the Northern Hemisphere, Venus will set almost together with the Sun and become lost in the solar glare. In the Southern Hemisphere, it will still be visible in the evening sky at the beginning of the month, but it will gradually sink deeper into twilight.
On October 2, Venus will change from direct to retrograde motion. By late October, the planet will be difficult to observe from most locations as it approaches solar conjunction on October 24.
Venus will reappear as the “Morning Star” in November, improving visibility towards the end of 2026. The planet will reach its maximum magnitude of -4.8 in September and November; for the rest of the year, its magnitude will remain around -4 or brighter.
May 15: Venus at perihelion
- Perihelion time: 03:01 GMT
On May 15, 2026, Venus reaches perihelion — its closest point to the Sun. The planet will be about 0.72 AU from the Sun.
Don’t expect a dramatic change in the sky, though. Venus’ orbit is almost circular, so its distance from the Sun changes only slightly during the year. Perihelion doesn’t make Venus suddenly flare up or look much larger. What you will see is Venus shining brightly as an Evening Star. After sunset, look for a dazzling white point of light in the western sky.
May 19: Moon near Venus
- Conjunction time: 01:49 GMT
- Conjunction distance: 2°56′
- Close approach time: 02:04 GMT
- Close approach distance: 2°56′
On May 19, the thin crescent Moon will pass close to Venus (mag –3.9) in the constellation Taurus. Look for them low above the western horizon in the evening twilight. Brilliant Venus will be easy to spot, even from a light-polluted city. It will be a beautiful sight — don’t miss it!
May 21: Venus near M35 star cluster
- Close approach time: 00:40 GMT
- Conjunction time: 00:46 GMT
- Close approach & conjunction distance: 0°45′
On May 21, Venus will pass close to the M35 star cluster in the constellation Gemini. The planet will shine brilliantly at about magnitude -3.9, while M35, also known as the Shoe-Buckle Cluster, will be much fainter at about magnitude 5.1.
Venus itself will be easy to see with the naked eye in the evening sky. M35, however, is best observed with binoculars or a small telescope: under very dark skies, it may be barely visible as a faint glow, but binoculars will reveal it as a small cluster of stars. The pair will be close enough to fit in the same binocular field of view.
Around the same dates, the Moon and Jupiter will also add to the evening scene. On May 20, the waxing crescent Moon will pass near Jupiter and Pollux in Gemini, not far from Castor.
June 9: Jupiter near Venus
- Conjunction time: 12:35 GMT
- Conjunction distance: 1°38′
- Close approach time: 19:47 GMT
- Close approach distance: 1°36′
On June 9, Jupiter and Venus — the two brightest planets — will appear close together in the evening sky, above the northwestern horizon. With magnitudes of –1.9 for Jupiter and –4 for Venus, the pair will be strikingly bright and easy to spot with the naked eye. Mercury will also share the constellation Gemini with them, adding a third planet to the scene — though it will be much fainter and more challenging to see in the twilight. This beautiful conjunction has earned its place on our list of the best astronomical events of 2026.
Late September: Venus at its brightest in 2026
In late September 2026, don’t miss Venus at its brightest for 2026. Shining at magnitude –4.8, it will blaze low in the southwestern sky shortly after sunset in Virgo. Venus will be unmistakable to the naked eye, but a telescope will reveal an impressive thin crescent, just 22% illuminated. This is one of the best skywatching events of 2026 — read more in our roundup.
June 16, 2027: Venus near Aldebaran
- Conjunction time: 10:11 GMT
- Conjunction distance: 4°42′
On June 16, 2027, Venus will pass near Aldebaran. Both objects will be easily visible to the naked eye a couple of hours before local sunrise. Dimmer Uranus will also be located nearby, but it will only be visible with a pair of binoculars and may be completely outshined by the rising Sun.
What color is Venus?
Venus appears white or yellowish-white when viewed through a telescope. The reason is that it’s covered with a thick carbon dioxide atmosphere and sulphuric acid clouds.
The planet's cloud cover obscures direct observations, so the color of the Venusian surface is not accurately known. However, based on data collected by spacecraft missions, scientists believe that it likely exhibits various shades of red, brown, and gray.
Why is Venus so bright?
Venus looks like a dazzling white “star” because it reflects sunlight extremely well. The planet is wrapped in thick, bright clouds that bounce much of the sunlight back into space, making Venus stand out even in twilight. Its relative closeness to Earth also plays a role, helping Venus appear especially large and bright in our sky.
But its brightness isn’t always the same. As Venus moves around the Sun, its phase and distance from Earth change. Venus reaches its greatest brightness when it is relatively close to us — even though, surprisingly, its disk is not fully illuminated at that time. Let’s take a closer look.
Venus’ atmosphere is highly reflective
The gaseous Venusian atmosphere was initially discovered in 1761 by the Russian polymath Mikhail Lomonosov. Observing the transit of Venus across the solar disk, Lomonosov spotted a light ring around the planet’s disk. He correctly assumed that this phenomenon might be caused by the refraction of the Sun’s rays in the thick Venusian atmosphere.
Venus's atmosphere consists of 96.5% carbon dioxide, 3.5% nitrogen, and traces of other gases. Thick clouds composed of sulfuric acid and water vapor cover the planet’s surface and reflect about 77% of the sunlight that reaches Venus: that’s why this planet is so bright.
Venus’ phases affect its brightness
Venus doesn’t always shine with the same intensity. Similar to the Moon, Venus goes through phases as it orbits the Sun. Here's a quick breakdown of each phase (more on the celestial mechanics behind these phases in our dedicated article):
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New phase occurs at inferior conjunction, when Venus passes between the Sun and Earth. If it passes directly in front of the Sun, it appears as a small black dot moving across the Sun’s surface. However, this event can only be observed safely using special solar filters — never look at the Sun directly!
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Full phase happens at superior conjunction, when Venus is behind the Sun as seen from Earth. This phase is completely unobservable because the Sun’s glare blocks the view.
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Quarter phases occur at greatest elongations, when Venus appears farthest from the Sun in the sky.
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Gibbous phase lasts between the full phase and greatest elongations when more than half of Venus is illuminated.
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Crescent phase is seen between the new phase and greatest elongations.
The phases of Venus were first observed by Galileo Galilei in 1610, providing key evidence that planets orbit the Sun. They are easily visible through a small telescope, especially the crescent phase, which can sometimes even be seen with binoculars or, in rare cases, even with the naked eye by those with exceptional vision.
Surprisingly, unlike the Moon, Venus is not at its brightest when fully illuminated. That’s because its brightness depends on both its phase and its distance from Earth. When Venus is in its full phase, it’s actually at its farthest point from us, making it appear smaller and dimmer. However, during its crescent phase, Venus is much closer, and while only part of its surface is lit, its apparent size is much larger. Venus reaches peak brightness when less than half of its disk is illuminated because this is when its visible surface area covers the largest angular size from Earth.
Why does Venus appear as the Morning or Evening Star?
Venus is visible either before sunrise or after sunset because it always stays relatively close to the Sun in our sky. This happens because Venus is an inner planet: it orbits the Sun inside Earth’s orbit. From our point of view, Venus never moves across the whole night sky like Mars, Jupiter, or Saturn. Instead, it appears only in the morning or evening twilight, earning its famous nicknames: the Morning Star and the Evening Star.
Elongation: how Venus switches between morning and evening
The apparent distance between Venus and the Sun in the sky is called elongation. The larger the elongation, the farther Venus appears from the Sun and the easier it is to observe in darker twilight.
When Venus is at eastern elongation, it appears east of the Sun in the sky. This means it sets after the Sun and becomes visible in the evening as the Evening Star. When Venus is at western elongation, it appears west of the Sun, rises before the Sun, and shines in the morning as the Morning Star.
Venus is often easier to observe around its greatest elongation — the moment when it reaches its greatest apparent separation from the Sun as seen from Earth. Around this time, the planet appears farther from the Sun’s glare and usually remains visible longer in twilight.
The greatest elongations of Venus take place roughly every 9 months. The greatest western elongation is also called the morning one, as, during this period, Venus shines brightly in the predawn sky — hence the name “morning star”. The greatest eastern elongation is referred to as the evening one, as Venus appears in the sky around sundown.
If you want to make sure that the bright dot you’re looking at is Venus, use an astronomy app like Sky Tonight or Star Walk 2. Simply point your device at the sky, and the app will show you the name of any celestial body.
Dual visibility of Venus: when the planet appears in both morning and evening
Venus is called the "evening star" and the "morning star," depending on when it appears in the sky. But in rare cases around its inferior conjunction, it can be visible in both the morning and evening skies for a few days. This rare phenomenon last occurred in March 2025, briefly delighting observers in the Northern Hemisphere. The next such opportunity will only be in 2033.
The dual visibility happens when Venus reaches inferior conjunction at a point where its ecliptic latitude is at its greatest. This means Venus isn't exactly aligned with the Sun but positioned slightly above it from our perspective.
The astronomical season also influences Venus’ visibility. During spring and summer, the ecliptic makes a steep angle with the horizon in the evening and sits low down in the morning. In other words, the Sun sets quickly in the evening and rises slowly in the morning. Because of this arrangement, Venus is still visible in the evening sky just before the inferior conjunction and begins to be visible in the morning sky as well a few days before the conjunction.
Observing Venus near inferior conjunction is particularly interesting if you have a telescope. At this time, the planet has the largest visible size because it is closest to the Earth, but its illumination is minimal — literally fractions of a percent. However, be extremely careful when watching the planet near the Sun.
Venus facts
- Planet type: terrestrial
- Radius: 6051.8 km (3760.4 miles)
- Mass: 4.867×10²⁴ kg
- Aphelion: 108.939 million km (67.691 million miles)
- Perihelion: 107.476 million km (66.782 million miles)
- Distance from Earth: ranges from about 40 million to 261 million km (25 million to 162 million miles)
- Surface temperature: 438 °C to 482 °C (820 °F - 900 °F)
- Solar day length: 116.75 Earth days
- Sidereal day length: 243.022 Earth days
- Year length: 224.701 Earth days
- Age: 4.503 billion years
- Named after: the Roman goddess of love and beauty
Fun facts about Venus
Here are a few mind-blowing facts about the planet Venus.
- Venus is the hottest planet in all the Solar System.
- Venus has rains of sulfuric acid that never reach the surface.
- Venus spins on its axis in the opposite direction compared to most other planets.
- In the Venusian atmosphere, winds blow at incredibly high speeds — up to 300 km/h (186 mph).
- Venus has no moons or rings. However, it has a quasi-moon named Zoozve!
- Venus has the longest day of any planet in the Solar System — it lasts about 243 Earth days.
- A year on Venus lasts about 225 Earth days, which is shorter than a sidereal day on Venus — one full rotation on its axis, taking about 243 Earth days.
- The atmospheric pressure on Venus is about 92 times greater than on the Earth. It is equivalent to the pressure experienced at depths of approximately 1 km (0.62 miles) in the Earth's oceans.
- Multiple spacecraft have successfully landed on Venus, but their operational lifetimes were very short due to the harsh conditions on the planet's surface.
Take our fun and educational quiz about Venus to learn more interesting facts and test your knowledge about this fascinating planet!
Who discovered Venus?
As Venus is very bright, it has been observed by ancient astronomers from different civilizations since the dawn of time. Thus, we can’t know for sure who discovered Venus. In the 16th century, Copernicus placed Venus in the heliocentric system as a planet orbiting the Sun. In 1610, Galileo viewed the planet through a telescope and discovered its phases, which are similar to the lunar ones. This discovery proved the Copernican theory that planets orbit the Sun and not vice versa.
How many moons does Venus have?
Actually, Venus has no moons at all! Venus and Mercury are the only planets of the Solar System that don’t have any natural satellites orbiting them. Scientists suggest that Venus might once have had a moon formed as a result of a collision. Later, another collision destroyed this satellite.
The main possible reason Venus doesn’t have any moons is its proximity to the Sun. The strong gravitational influence of the Sun makes it challenging for moons to form and remain in a stable orbit.
Zoozve — a quasi-moon of Venus
524522 Zoozve (also known as 2002 VE68) is a potentially hazardous asteroid and Venus’s quasi-moon — an object that appears to orbit a planet but is not gravitationally bound to it. Zoozve was discovered in 2002.
Why is Venus’ quasi-moon called Zoozve? This weird name originated from a quirky mix-up: Latif Nasser, co-host of the Radiolab podcast, stumbled upon a poster where Venus was shown having a moon named “ZOOZVE”. After some investigation, it turned out that "ZOOZVE" emerged from a misreading of “2002 VE” by the poster’s creator, Alex Foster. Captivated by the odd name, Nasser embarked on a mission to have the quasi-moon renamed, and in February 2024, the International Astronomical Union approved “Zoozve” as its official name!
How big is Venus?
Venus has a mean radius of 6,052 km (3,760 miles). A trip around the equator of this planet would cover a distance of about 38,025 km (23,627 miles). Unlike many other Solar System planets with an equatorial bulge, Venus is a nearly perfect sphere, so its radius doesn’t differ at the poles and the equator. The equatorial bulge doesn’t form because Venus rotates very slowly around its axis.
Is Venus bigger than Earth?
Venus is slightly smaller than the Earth — its diameter equals about 95% that of our planet. The mass of Venus (4.867×10²⁴ kg) is about 81% that of the Earth.
Venus’ temperature
Venus has an average surface temperature of about 462 °C (864 °F), which makes it one of the hottest places in the Solar System. This incredible heat is primarily a result of Venus’ thick atmosphere, which is composed mainly of carbon dioxide. It creates the greenhouse effect, which traps solar radiation and elevates temperatures to such extreme levels. Additionally, the planet’s proximity to the Sun contributes to its exceptionally high temperatures.
Are you curious how Venus’s temperature compares to those of the other planets? Check out this Solar System thermometer infographic — and meet a creature that thrives no matter the heat or cold!
Venus’ orbit and rotation
How long is a day on Venus?
It depends on what kind of “day” we mean. Venus takes about 243 Earth days to complete one rotation on its axis — this is called a sidereal day. In that sense, Venus has the slowest rotation — and the longest sidereal day — of any planet in the Solar System.
A solar day — the time from one sunrise to the next — is much shorter: about 117 Earth days. This happens because Venus rotates very slowly in a retrograde direction, while also orbiting the Sun.
How long is a year on Venus?
While on the Earth we are accustomed to a year consisting of approximately 365 days, Venus dances to a different celestial rhythm. The duration of a Venusian year, or its orbital period around the Sun, is roughly 225 Earth days. Surprisingly, this means that a Venusian year is actually shorter than a Venusian day!
Why does Venus rotate backwards?
Venus rotates in the opposite direction of most planets in the Solar System, a phenomenon known as retrograde rotation (not to be confused with retrograde motion). As a result, the Sun rises in the west and sets in the east on Venus, contrasting with the east-to-west motion of the Sun in the Earth’s sky. The cause of Venus’s retrograde rotation is still poorly understood.
One prominent theory suggests that a collision with a giant asteroid early in Venus’s history could have reversed its rotation. A similar thing might have happened to Uranus, causing the planet to spin on its side.
Another possible cause could be a gravitational interaction between Venus and the Sun. Over time, the Sun’s gravitational pull could have slowed down Venus’s rotation and eventually reversed it.
How far away is Venus?
How far is Venus from the Sun?
Venus is the second planet from the Sun; its distance from our star is just over 70% the distance between Earth and the Sun. As Venus’ elliptical orbit is the least eccentric of any of the planets, there is no significant difference between its closest (107.4 million km) and farthest (108.9 million km) points from the Sun. The average distance is 108.2 million km.
How far is Venus from the Earth?
The distance between Venus and Earth is constantly changing as both planets move around the Sun. At its closest approach, Venus can come within about 38 million km (24 million miles) of Earth. At its farthest, when Venus and Earth are on opposite sides of the Sun, the distance can grow to about 261 million km (162 million miles). Although Venus comes closer to Earth than any other planet at closest approach, Mercury spends more time as Earth’s nearest planetary neighbor on average.
Missions to Venus
Historical missions to Venus
Venus was long thought to have lush jungles and large bodies of water, like Earth, because no one could see the planet’s surface through its thick clouds. However, spacecraft missions have revealed a vastly different reality: a hellish volcanic planet with extremely high temperatures and crushing atmospheric pressure. Overall, more than 40 spacecraft have explored Venus, but not all of them have reached their goals. Here is a short list of the most successful missions to Venus:
- Mariner 2 — first successful Venus flyby (1962)
- Venera 7 — first successful landing on Venus (1970)
- Venera 9 and Venera 10 — orbiting and landing on Venus (1975)
- Magellan — imaging the entire Venus surface (1989)
- Galileo — Venus flyby en route to Jupiter (1989)
- Cassini — Venus flybys en route to Saturn (1998 and 1999)
- Venus Express — first European Venus orbiter (2005)
- Akatsuki — first Japanese Venus orbiter (2015)
Upcoming missions to Venus
Several exciting new missions are set to launch in the coming years, aiming to uncover what lies beneath the planet’s thick clouds and explore its mysterious past.
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Shukrayaan-1 (ISRO, planned for 2028) — India’s first Venus mission, will investigate the atmosphere and surface.
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DAVINCI (NASA, planned for 2030) — will drop a probe into Venus’s atmosphere to study its chemistry and structure.
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VERITAS (NASA, planned for 2031) — will map Venus’s surface in high resolution.
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EnVision (ESA, planned for 2031) — will explore Venus’s interior and climate evolution from orbit.
These missions promise to reveal whether Venus was once Earth-like, and why the two sister planets took such different paths.
How long does it take to get to Venus?
On average, it takes spacecraft between 3 to 5 months to reach Venus. The flight duration depends on several factors, including the spacecraft’s trajectory and the relative positions of Earth and Venus in their orbits. The Soviet Venera 1 spacecraft (1961) made it to Venus’s vicinity in just 97 days (a little more than 3 months) but missed the planet by about 100,000 km (62,000 miles). NASA’s space probe Mariner 2 (1962) reached Venus in 110 days (about 3 months and 20 days). ESA’s Venus Express (2005) took 153 days (around 5 months) to get to Venus.
What is Venus made of?
Unfortunately, little information is available about the internal structure of Venus.
Formation of Venus
Venus formed together with the other Solar System planets. About 4.5 billion years ago, a giant cloud of interstellar gas and dust collapsed under its own gravity and flattened into a protoplanetary disk. Venus and the other rocky planets formed in the inner part of this disk, while the gas giants settled in the outer regions of the young Solar System.
Venus’ structure
Due to the similarity in size and mass between Venus and the Earth, scientists believe the planets share a similar interior. Both have an iron core surrounded by a hot-rock mantle and a thin rocky crust. On both planets, this outer crust can change shape and erupt into volcanoes as heat and pressure move through the interior.
F.A.Q.
How hot is Venus?
The thick Venusian atmosphere traps heat, causing surface temperatures ranging from 438 to 482 °C (820 to 900 °F). This is why Venus is hotter than Mercury, which is the planet closest to the Sun.
Does Venus have a surface?
Yes, Venus has a solid surface beneath its dense atmosphere. The surface of Venus is made up of rocky materials similar to those found on Earth. It is covered with volcanoes, mountains, expansive plains and vast plateaus.
How old is Venus?
Like other celestial bodies in the Solar System, Venus formed approximately 4.5 billion years ago during the early stages of the Solar System's evolution. It originated from the accretion and collision of numerous protoplanets and planetesimals. As these objects came together, their gravitational interactions led to the gradual formation of the planet Venus.
Is Venus the morning star?
Yes — Venus can be the Morning Star, but not always. It appears as the Morning Star when it is visible before sunrise, shining in the eastern sky. At other times, Venus becomes the Evening Star, appearing after sunset in the western sky. This happens because Venus orbits closer to the Sun than Earth does, so from our point of view it always stays near the Sun in the sky. Depending on which side of the Sun Venus appears on, we see it either in the morning or in the evening.
Planet Venus: to sum up
Venus is the brightest planet in Earth’s sky and one of the easiest worlds to spot without any equipment. Depending on its position relative to the Sun, it appears either before sunrise as the Morning Star or after sunset as the Evening Star. In 2026, Venus will be visible mostly in the evening sky.
There’s more to Venus than its dazzling appearance: it is extremely hot, covered by thick clouds, has no moons, and rotates slowly in the opposite direction to most planets. Through binoculars or a telescope, you may even notice its changing phases.
If you want to quickly find Venus in the sky from your location, use the free astronomy app Sky Tonight.
Explore the other Solar System planets
We hope you enjoyed the article about Venus! You can also check out our articles about the other planets in the Solar System:
- Mercury – the smallest and fastest planet;
- Mars – our potential future home;
- Jupiter – the biggest planet;
- Saturn – the “Lord of the Rings” (and moons!);
- Uranus – the coldest planet;
- Neptune – the farthest planet;
- and Pluto, which was famously demoted from planet status (and the decision remains a hot topic in the astronomical community for almost 20 years).
Learn more space facts
Want to learn more facts about space? Then you'll love our quiz about the “most-est” objects in the Solar System! Find out which of them is the hottest or fastest, and where the tallest mountain and deepest canyon are located.
