When & Where is Venus Visible in 2026? Observe 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.

Venus at a glance

• Visible right now: yes, in the evening sky. Best seen from the Southern Hemisphere; from northern latitudes, stays very low above the horizon.
• Visible with the naked eye: yes, looks like a bright white “star”.
• When to see in 2026: February through early October in the evening sky; November onward in the morning sky.
• Greatest brightness in 2026: late September (mag –4.80); late November (mag –4.89)

Contents

• Venus at a glance
• Is Venus visible from Earth?
• Where is Venus located in the sky in 2026?
• When can you see Venus in the sky in 2026?

  • Late September 2026: Venus at its brightest in the evening sky
  • October 3: Venus goes retrograde
  • October 5–7: Venus near Mercury
  • October 24: Venus at inferior solar conjunction
  • November 3–9: Venus near Spica
  • November 14: Venus ends retrograde motion
  • November 19: Venus near Spica
  • Late November 2026: Venus at its brightest in the morning sky
  • June 16, 2027: Venus near Aldebaran
• What color is Venus?
• Why is Venus so bright?
  • Venus’ atmosphere is highly reflective
  • Venus’ phases affect its brightness
• Why does Venus appear as the Morning or Evening Star?
  • Elongation: how Venus switches between morning and evening
  • Dual visibility of Venus: when the planet appears in both morning and evening
• Venus facts
  • Fun facts about Venus
• Who discovered Venus?
• How many moons does Venus have?
  • Zoozve — a quasi-moon of Venus
• How big is Venus?
  • Is Venus bigger than Earth?
• Venus’ temperature
• Venus’ orbit and rotation
  • How long is a day on Venus?
  • How long is a year on Venus?
  • Why does Venus rotate backwards?
• How far away is Venus?
  • How far is Venus from the Sun?
  • How far is Venus from the Earth?
  • When is Venus closest to Earth?
• Missions to Venus
  • Historical missions to Venus
  • Upcoming missions to Venus
  • How long does it take to get to Venus?
• What is Venus made of?
  • Formation of Venus
  • Venus’ structure
• Frequently asked questions about Venus
  • Is Venus the brightest planet?
  • How hot is Venus?
  • Does Venus have a surface?
  • How old is Venus?
  • Is Venus the morning star?
• Planet Venus: to sum up
  • Explore the other Solar System planets
  • Learn more space facts

Is Venus visible 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.

Where is Venus located in the sky in 2026?

Venus changes its position noticeably during the last months of 2026, moving from the evening to the morning sky.

• September 2026: Venus is in Virgo, shining low above the western horizon after sunset. As September progresses, Venus sinks lower into the evening twilight.

• October 2026: Venus remains close to the Sun in the sky and becomes increasingly difficult to observe. In early October, it can still be found very low in the evening twilight, but later in the month it disappears into the Sun’s glare. On October 24, Venus passes through inferior conjunction, moving between the Earth and the Sun. After that, it switches from the evening sky to the morning sky.

• November 2026: Venus returns to the morning sky in Virgo, where it performs a striking retrograde loop around Spica, Virgo’s brightest star. By late November, the planet reaches the peak brightness of its morning apparition — and of 2026 overall — at about magnitude –4.89.

• December 2026: Venus moves eastward from Virgo into Libra and becomes an increasingly prominent object in the predawn sky. It rises several hours before the Sun and remains extremely bright throughout the month. Around mid-December, Venus stands noticeably higher above the eastern horizon before sunrise, making it easier to observe.

When can you see Venus in the sky in 2026?

Venus is one of the easiest planets to spot with the naked eye, but some dates offer especially interesting views. Below, you’ll find the best dates to observe Venus, with exact event times, angular separations, and tips on when and where to look.

Late September 2026: Venus at its brightest in the evening sky

Venus becomes exceptionally bright in late September, reaching its peak brightness of the 2026 evening apparition. Shining at around magnitude –4.80, it will be impossible to miss in the western sky shortly after sunset. Look for the planet in Virgo. The view is especially favorable from the Southern Hemisphere; at more northerly latitudes, Venus stays much closer to the horizon.

Venus reaches its greatest illuminated extent around September 18, when about 26% of its disk is illuminated. This is not exactly the same as greatest brightness: greatest illuminated extent refers to the maximum apparent area of Venus’s sunlit portion, while its peak brightness occurs around September 24, when the planet is about 21% illuminated.

Interestingly, this isn’t quite the brightest Venus will get in 2026. After passing between the Earth and the Sun in late October, the planet will reappear in the morning sky and reach another — slightly brighter — peak toward the end of November (mag –4.89). So September offers a more convenient chance to see Venus near its maximum brilliance: no early alarm required — just look outside after sunset.

Through a telescope, Venus will look like a thin crescent. Oddly enough, the planet does not appear brightest when most of its disk is lit. As its illuminated fraction decreases, Venus is also moving closer to Earth and appearing larger in our sky. Around greatest brilliancy, its increased apparent size more than makes up for the narrow crescent, producing that dazzling glow.

City	Time zone	Best time (local)	Venus altitude	Sun altitude
New York, USA	EDT (UTC−4)	Sep 24, 7:17 PM	4°	−6°
New Delhi, India	IST (UTC+5:30)	Sep 24, 6:39 PM	10°	−6°
Singapore	SGT (UTC+8)	Sep 24, 7:21 PM	23°	−6°
Sydney, Australia	AEST (UTC+10)	Sep 24, 6:18 PM	30°	−6°
São Paulo, Brazil	BRT (UTC−3)	Sep 24, 6:26 PM	29°	−6°

• Best time is when the Sun is about 6° below the horizon and Venus is still visible.
• Altitude shows how high Venus is above the horizon: 0° is on the horizon, 30° is about one-third of the way up the sky, and 90° is directly overhead.
• If Venus is below about 10°, choose a spot with a clear, unobstructed horizon.

October 3: Venus goes retrograde

On October 3, 2026, Venus begins its retrograde motion, which will last until November 14. The change itself isn’t noticeable from one night to the next, but if you track Venus against the background stars over several weeks, you’ll see it trace a small loop in the sky before resuming its usual eastward motion. Learn more about why planets sometimes appear to move backward in our infographic on retrograde motion.

October 5–7: Venus near Mercury

• Conjunction time: October 5, 14:50 GMT
• Conjunction distance: 5°28′
• Close approach time: October 7, 04:09 GMT
• Close approach distance: 5°02′

On October 5–7, Venus (mag –4.6) and Mercury (mag 0.0) will appear near each other in the evening sky. The event strongly favors the Southern Hemisphere: there, both planets will stand fairly high above the western horizon after sunset. In the Northern Hemisphere, however, the pair will be very low or already below the horizon by the time the sky gets dark enough, making the conjunction difficult or impossible to observe.

October 24: Venus at inferior solar conjunction

On October 24, 2026, Venus will pass between the Earth and the Sun — an event called inferior solar conjunction. At that time, the planet will appear only about 6° from the Sun in our sky and will be lost in the solar glare for ordinary observers.

Do not attempt to search for Venus with binoculars or a telescope near the Sun to avoid eye damage!

This event marks Venus’s transition from the evening sky to the morning sky. From early November, observers can start looking for Venus low above the eastern horizon before sunrise. By mid-November, it will be much easier to spot as it moves farther from the Sun.

November 3–9: Venus near Spica

• Conjunction time: November 3, 12:59 GMT
• Conjunction distance: 2°21′
• Close approach time: November 9, 11:24 GMT
• Close approach distance: 1°09′

From November 3 to 9, Venus will pass close to Spica, the brightest star in Virgo. The planet will be moving retrograde at the time, so instead of simply passing the star once, it will trace part of a loop around it. Venus and Spica will be in conjunction on November 3, and by November 9, Venus will approach the star to just over 1° — roughly the width of your little finger held at arm’s length.

The pair will be visible in the morning sky before sunrise, with brilliant Venus easily outshining Spica. They will remain low above the horizon, so choose an observing spot with a clear, unobstructed view in that direction.

City	Time zone	Best time (local)	Separation	Spica altitude	Venus altitude	Sun altitude
New York, USA	EST (UTC−5)	Nov 9, 5:56 AM	1.16°	12°	13°	−8°
London, UK	GMT (UTC+0)	Nov 9, 6:18 AM	1.16°	9°	10°	−8°
New Delhi, India	IST (UTC+5:30)	Nov 9, 6:05 AM	1.16°	14°	14°	−8°
Singapore	SGT (UTC+8)	Nov 9, 6:17 AM	1.16°	14°	15°	−8°
Sydney, Australia	AEDT (UTC+11)	Nov 9, 5:10 AM	1.17°	6°	7°	−8°
São Paulo, Brazil	BRT (UTC−3)	Nov 9, 4:43 AM	1.15°	10°	11°	−8°

• Best time is when the Sun is about 8° below the horizon and Venus and Spica are still visible.
• Altitude shows how high the objects are above the horizon: 0° is on the horizon, 30° is about one-third of the way up the sky, and 90° is directly overhead.
• If the pair is below about 10°, choose a spot with a clear, unobstructed horizon.

November 14: Venus ends retrograde motion

On November 14, 2026, Venus ends its retrograde motion and begins moving eastward against the background stars again. This change won’t be noticeable from one morning to the next, but if you track the planet over several weeks, you’ll see its apparent loop in the sky come to an end. After turning direct, Venus will move away from Spica and continue climbing into a more favorable position in the morning sky. Learn more about why planets sometimes appear to move backward in our article on retrograde motion.

November 19: Venus near Spica

• Conjunction time: 22:45 GMT
• Conjunction distance: 1°48′

On November 19, Venus will pass Spica for the second time this month. After ending its retrograde motion on November 14, Venus will begin moving eastward again, reaching a second conjunction with the star this month.

The pair will be visible in the morning sky before sunrise. By mid-November, Venus will be climbing higher into the predawn sky, so this second encounter with Spica will generally be easier to observe than their meeting earlier in the month. Look for them above the eastern to southeastern horizon, preferably from a location with a clear view in that direction.

City	Time zone	Best time (local)	Separation	Spica altitude	Venus altitude	Sun altitude
New York, USA	EST (UTC−5)	Nov 19, 6:07 AM	1.75°	20°	22°	−8°
London, UK	GMT (UTC+0)	Nov 19, 6:34 AM	1.73°	16°	18°	−8°
New Delhi, India	IST (UTC+5:30)	Nov 19, 6:12 AM	1.72°	23°	24°	−8°
Singapore	SGT (UTC+8)	Nov 19, 6:18 AM	1.71°	24°	24°	−8°
Sydney, Australia	AEDT (UTC+11)	Nov 19, 5:03 AM	1.70°	13°	12°	−8°
São Paulo, Brazil	BRT (UTC−3)	Nov 19, 4:38 AM	1.75°	18°	17°	−8°

• Best time is when the Sun is about 8° below the horizon and Venus and Spica are still visible.
• Altitude shows how high the objects are above the horizon: 0° is on the horizon, 30° is about one-third of the way up the sky, and 90° is directly overhead.
• If the pair is below about 10°, choose a spot with a clear, unobstructed horizon.

Late November 2026: Venus at its brightest in the morning sky

In late November, Venus reaches its greatest brightness of 2026, shining at about magnitude –4.89 in the morning sky. The peak occurs around November 25, when the planet is visible before sunrise and stands much higher above the horizon than it did earlier in the month.

This is Venus’s brightest appearance of the year, slightly exceeding its September evening peak. By then, the planet will have emerged well from the Sun’s glare, making late November one of the best times to see the dazzling “Morning Star.”

Interestingly, Venus will be only about 23% illuminated at the time, appearing as a crescent through a telescope. Despite showing less than a quarter of its sunlit side, the planet looks exceptionally bright because it is still relatively close to Earth and therefore appears large in our sky.

City	Time zone	Best time (local)	Venus altitude	Sun altitude
New York, USA	EST (UTC−5)	Nov 25, 6:24 AM	27°	−6°
London, UK	GMT (UTC+0)	Nov 25, 6:53 AM	22°	−6°
New Delhi, India	IST (UTC+5:30)	Nov 25, 6:26 AM	30°	−6°
Singapore	SGT (UTC+8)	Nov 25, 6:27 AM	30°	−6°
Sydney, Australia	AEDT (UTC+11)	Nov 25, 5:08 AM	17°	−6°
São Paulo, Brazil	BRT (UTC−3)	Nov 25, 4:46 AM	22°	−6°

• Best time is when the Sun is about 6° below the horizon and Venus is still visible.
• Altitude shows how high Venus is above the horizon: 0° is on the horizon, 30° is about one-third of the way up the sky, and 90° is directly overhead.
• If Venus is below about 10°, choose a spot with a clear, unobstructed horizon.

June 16, 2027: Venus near Aldebaran

• Close approach time: 17:46 GMT
• Close approach distance: 4°45′
• Conjunction time: June 17, 10:16 GMT
• Conjunction distance: 4°49′

On June 16, 2027, Venus will pass near Aldebaran. Both objects will be visible to the naked eye for about an hour 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 sulfuric 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 the surface itself is mostly dark and relatively neutral in color, with grayish and brownish tones. The familiar orange-red appearance seen in some Venus lander images is strongly influenced by the planet’s dense atmosphere, which filters and scatters sunlight before it reaches the surface.

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

Mikhail Lomonosov is traditionally credited with discovering Venus’s atmosphere in 1761 after observing the planet’s transit across the Sun. He reported a luminous arc around Venus near the edge of the solar disk, which he interpreted as evidence of an atmosphere.

Thick clouds made primarily of sulfuric acid droplets cover Venus, while water vapor is present only in trace amounts in the atmosphere. These bright clouds reflect about 77% of the sunlight that reaches the planet, helping make Venus so brilliant in our sky.

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):

• 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!

• 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.

• Quarter phases occur at greatest elongations, when Venus appears farthest from the Sun in the sky.

• Gibbous phase lasts between the full phase and greatest elongations when more than half of Venus is illuminated.

• 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 not occur until 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.

This rare dual visibility depends mainly on Venus passing well north of the Sun during inferior conjunction. The effect is strongest at high northern latitudes, where this northward offset can keep Venus just above the horizon both before sunrise and after sunset.

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 38 million to 261 million km (24 million to 162 million miles)
• Surface temperature: 438 °C to 482 °C (820–900 °F)
• Solar day length: 116.75 Earth days
• Sidereal day length: 243.022 Earth days
• Year length: 224.701 Earth days
• Age: 4.5 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 360 km/h (224 mph).
• Venus has no moons or rings. However, it has a quasi-moon named Zoozve!
• Venus rotates incredibly slowly: its sidereal day lasts about 243 Earth days, longer than on any other planet in the Solar System.
• 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 showed that Venus orbits the Sun and ruled out the traditional Ptolemaic model, providing powerful evidence in favor of heliocentrism.

How many moons does Venus have?

Venus has no moons. Unlike Mercury, whose proximity to the Sun makes it difficult to retain a moon, Venus’s moonless state remains an open question in planetary science. Some hypotheses suggest that Venus may once have had a satellite that was later lost or destroyed, possibly through major collisions or long-term orbital evolution. However, there is no confirmed explanation yet.

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.

When is Venus closest to Earth?

Venus comes closest to Earth around inferior conjunction, when it passes between Earth and the Sun. The next such event will occur on October 24, 2026. Around this time, Venus will be near its minimum distance from Earth — roughly 40 million km (25 million miles) away.

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 been launched to explore Venus, but not all of them have reached their goals. Here is a short list of the most successful missions to Venus:

• Mariner 2 — launched in 1962; became the first successful spacecraft to fly by Venus later that year and returned the first close-up measurements of the planet.

• Venera 7 — launched in 1970; became the first spacecraft to successfully land on another planet and transmit data from its surface.

• Venera 9 and Venera 10 — launched in 1975; entered orbit around Venus and deployed landers that returned the first images from the surface of another planet.

• Magellan — launched in 1989; entered orbit around Venus in 1990 and used radar to map most of the planet’s surface in unprecedented detail.

• Galileo — launched in 1989; flew past Venus in 1990 on its way to Jupiter and collected additional data on the planet’s atmosphere and cloud structure.

• Cassini — launched in 1997; performed Venus flybys in 1998 and 1999 on its way to Saturn, using the encounters for gravity assists and scientific observations of the planet and its atmosphere.

• Venus Express — launched in 2005; entered orbit around Venus in 2006 and spent years studying the planet’s atmosphere, plasma environment, and climate.

• Akatsuki — launched in 2010; successfully entered orbit around Venus in 2015 and studied the planet’s weather, cloud patterns, and atmospheric dynamics until the mission ended in September 2025.

Venus exploration has produced several major milestones in the history of spaceflight — from the first successful landing on another planet to the first images transmitted from another planet’s surface. If you’d like to test your knowledge of other groundbreaking achievements in space exploration, try our quiz about the most important space milestones.

Upcoming missions to Venus

Several exciting new missions are set to launch in the coming years, aiming to uncover what lies beneath Venus’s thick clouds and explore the planet’s mysterious past.

• Venus Orbiter Mission (ISRO, planned for March 2028) — India’s first mission to Venus will study the planet’s surface, atmosphere, and ionosphere.

• DAVINCI (NASA, planned for the early 2030s) — will study Venus from above its clouds down to the surface. Its descent probe will measure the atmosphere’s chemistry, temperature, pressure, and winds as it falls toward the surface.

• VERITAS (NASA, no earlier than 2031) — will map Venus’s surface in high resolution and investigate the planet’s geology and interior.

• Envision (ESA, planned for November 2031) — will study Venus from its core to its upper atmosphere, investigating its geology, climate, and evolution.

Together, these missions could help scientists determine whether Venus was once more Earth-like and why the two sister planets evolved so differently.

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.

Frequently asked questions about Venus

Is Venus the brightest planet?

Yes. Venus is the brightest planet in Earth’s sky and can reach a magnitude of about –4.9. That means Venus can appear roughly 6 times brighter than Jupiter, the second-brightest planet, which typically reaches only about –2.9. Venus can even be seen with the naked eye in daylight if you know exactly where to look.

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.