Venus Occultation September 14, 2026: Moon Covers Venus
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Venus as seen from NASA — the brilliant planet will be occulted by the Moon on September 14, 2026

Sky Event Guide · September 2026

Venus Occultation September 14, 2026: The Moon Covers Venus — Complete Observer's Guide

One of the most striking celestial events of 2026: the crescent Moon slides directly in front of brilliant Venus, covering it completely. This guide provides exact regional timings, scientific context, and the telescope setup that captures the disappearing act at its best.

DateSeptember 14, 2026
Event typeLunar occultation
VisibilityEurope, Africa, Middle East, Asia (daytime)
Best toolTelescope or binoculars
By Telescope Advisor Editorial Team Published: Updated: Editorial Standards

Quick Answer: What Is the Venus Occultation and How to See It

On September 14, 2026, the waxing crescent Moon passes directly in front of Venus — an event astronomers call a lunar occultation. Venus, the brightest planet in the sky, disappears behind the Moon's dark limb and then reappears on the opposite side up to an hour later. This is one of the most dramatic and photogenic sky events of 2026.

The occultation is not visible from North or South America. It is visible from parts of Europe, Africa, the Middle East, western Russia, and southern Asia, and the entire event runs between 09:26 and 13:42 UTC — which falls in the early-morning-to-midday hours when the Moon and Venus are below the horizon in the Americas. Everywhere the occultation is visible, it happens in broad daylight, so binoculars or a telescope are essential.

US and Canadian readers are not shut out entirely: on the evening of September 14, the Moon and Venus still appear together low in the western sky after sunset, separated by roughly 5–6° — an attractive pairing in binoculars, though not an occultation. The most recent Venus occultation visible from the contiguous United States was June 17, 2026; the next is October 11, 2029.

The best telescope for this event is a mid-aperture instrument with good tracking capability. The Celestron NexStar 8SE is our top recommendation because its computerized GoTo mount can track Venus automatically during daylight (when manual finder alignment is difficult), and its 8-inch aperture delivers stunning detail on both the Moon's terrain and Venus's crescent phase. For budget-conscious observers, the Celestron AstroMaster 70AZ is a capable alternative.

Naked eye

During twilight/darkness, the event is visible naked-eye — Venus winks out behind the Moon. In daytime, you need binoculars or a telescope.

Binoculars

10×50 or 15×70 binoculars show Venus approaching the Moon's limb and the disappearance. The wide field helps you find the pair during daytime.

Telescope (best)

A telescope at 40–100× reveals Venus's crescent phase sliding behind lunar mountains. Timing the exact moment of disappearance is scientifically valuable.



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What Is a Lunar Occultation?

An occultation occurs when one celestial body passes in front of another, hiding it from view. A lunar occultation of a planet happens when the Moon — moving along its orbital path at about 1 km/second relative to Earth — passes directly between Earth and that planet. The geometry is similar to a solar eclipse, but the Moon covers a planet instead of the Sun.

Venus is occulted by the Moon several times per year from some location on Earth, but a given location may only see one every few years. The September 14, 2026 event is notable because it is widely visible across Europe, Africa, the Middle East, western Russia, and southern Asia, with the Moon at a favorable phase (waxing crescent, ~14–15% illuminated) that creates dramatic visual contrast: a thin, delicate crescent Moon sliding in front of brilliant Venus.

Key Facts About the September 14 Event

Moon phaseWaxing crescent (14%)
Venus magnitude−4.8
Venus phase~30% illuminated (crescent)
Venus distance0.46 AU (69 million km)
Venus angular size36 arcseconds
Venus separation~42° from Sun
ConstellationVirgo
Event duration~40–60 minutes
DisappearanceBehind Moon's dark (night) limb
ReappearanceFrom Moon's bright (day) limb

Why Occultations Are Scientifically Important

  • Lunar topography: Precise timing of occultations helps refine our knowledge of the Moon's limb profile — the exact shape of its edge with its mountains and valleys.
  • Double star discovery: Occultations of stars by the Moon have revealed hundreds of previously unknown double stars. For planets, timing reveals atmospheric effects.
  • Orbital refinement: Each occultation provides a precise data point for the orbits of both the Moon and the occulted planet, improving ephemeris accuracy.
  • Amateur contribution: Timed observations by amateur astronomers — even with modest equipment — are valuable to professional researchers. The International Occultation Timing Association (IOTA) collects and analyzes these observations.

The Science Behind Occultations

Occultations are among the most precisely predictable celestial events, and they offer unique scientific opportunities that cannot be replicated by other observing methods.

The Geometry of an Occultation

The Moon orbits Earth at an average distance of 384,400 km, moving at about 1.022 km/second relative to Earth's center. Venus on September 14, 2026, is approximately 0.46 AU (69 million km) from Earth — close enough that its disc spans about 36 arcseconds, roughly twice the apparent size of Saturn's globe. From our perspective, the Moon appears to approach Venus from the west, cover it, and then reveal it on the opposite side.

The exact timing of the occultation depends on your location on Earth due to parallax — the Moon is close enough that observers in different cities see it in a slightly different position against the background sky. This means the disappearance and reappearance times vary by up to several minutes across a continent. The timing tables below account for this.

What You Are Actually Seeing

When Venus disappears behind the Moon's dark limb, you are watching the planet pass behind the lunar mountains and craters along the terminator. This is where a planetary occultation differs from a stellar one. When the Moon covers a star, the disappearance really is instantaneous — a star is a point source, so it simply switches off. Venus is not a point source. At 36 arcseconds across it is a resolvable disc, and the lunar limb takes roughly 70 to 90 seconds to slide across it. What you actually watch is Venus's crescent being progressively bitten away, thinning to a sliver before the last of it vanishes. Through a telescope you may see the remaining sliver flicker as it passes behind individual peaks and valleys on the Moon's limb. The reappearance runs the same sequence in reverse, though it is harder to catch against the glare of the bright limb.

A note on the daytime challenge

Everywhere the occultation is visible — Europe, Africa, the Middle East, and Asia — it occurs in broad daylight. Venus is bright enough (magnitude −4.8) to be visible in a blue daytime sky through binoculars or a telescope, but finding it requires precision. Use a computerized GoTo mount (like the NexStar 8SE) or a planetarium app to determine the exact separation between the Moon and Venus at your location and time. Scan slowly — Venus will appear as a brilliant white point against the blue sky, unmistakable once found.



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Visibility by Region: Who Sees What

The Venus occultation on September 14, 2026, is visible across a broad swath of the Earth, but the experience differs dramatically by region.

Region Time of Day Visibility Notes
North & South America Overnight / pre-dawn Not visible Moon and Venus are below the horizon for the whole 09:26–13:42 UTC window. A close (non-occulting) pairing is visible low in the west after sunset on September 14 instead.
Western Europe (Spain, France, Italy) Late morning Daytime — optical aid required Event begins around 11:26 CEST. Pair is low (roughly 8–15° altitude), so a clear western-to-southern horizon matters.
Central & Eastern Europe Late morning / midday Daytime — optical aid required Germany 11:29–12:42 CEST; Poland 11:36–12:47 CEST. Higher and easier than Iberia.
Middle East (Iran, Iraq, Gulf) Early afternoon Daytime — best altitude worldwide Venus near culmination, roughly 40° up. The best-placed region on Earth for this event.
North & East Africa Midday / early afternoon Daytime — optical aid required Egypt 12:37–14:26 EEST; Ethiopia, Sudan, Kenya all well placed.
South & Southeast Asia Late afternoon Daytime — optical aid required India 17:00–19:10 IST; also Thailand, Malaysia, Indonesia, Vietnam, China.
Australia, Pacific, Japan — Not visible Outside the occultation footprint.

Best viewing region: the Middle East

Iran, Iraq, and the Gulf states get the most favourable geometry — Venus is near its highest point in the sky, roughly 40° up, when the occultation occurs. Higher altitude means less atmospheric turbulence and a darker blue background, both of which help daytime contrast. Southern Europe sees the event but very low down; the Canary Islands fall outside the footprint entirely.

Timing by Country

Times below are the span from the earliest disappearance to the latest reappearance anywhere in that country — they are not disappearance/reappearance times for a single city. Because the Moon's parallax shifts its apparent position by up to two degrees across the Earth, per-site times differ by several minutes even within one country. For exact times at your coordinates, use IOTA's prediction tools.

Country UTC span Local time
Spain09:26–10:3111:26–12:31 CEST
France09:26–10:3811:26–12:38 CEST
Italy09:27–10:4611:27–12:46 CEST
Germany09:29–10:4211:29–12:42 CEST
Poland09:36–10:4711:36–12:47 CEST
Greece09:31–11:0012:31–14:00 EEST
Turkey09:37–11:1612:37–14:16 TRT
Egypt09:37–11:2612:37–14:26 EEST
Israel09:47–11:1712:47–14:17 IDT
Iran10:10–12:0713:40–15:37 IRDT
Saudi Arabia09:48–12:1312:48–15:13 AST
United Arab Emirates10:27–12:0614:27–16:06 GST
Kenya10:50–11:5513:50–14:55 EAT
Pakistan11:04–12:2116:04–17:21 PKT
India11:30–13:4017:00–19:10 IST
Thailand12:26–13:4119:26–20:41 ICT
Indonesia12:30–13:4319:30–20:43 WIB
Worked example — Tehran, Iran: Venus disappears at about 13:59 IRDT and reappears at about 14:54 IRDT, both in daylight — a roughly 55-minute occultation, consistent with the 40–60 minute duration cited elsewhere on this page. Times are approximate; use IOTA's tools for precise predictions at your coordinates.

A note on the United Kingdom: the UK does not appear in In-The-Sky's visibility footprint, and British observers report Venus rising already occulted, with the reappearance very low. Do not rely on UK times without checking IOTA predictions first.

Occultation circumstances computed from JPL's DE440 planetary ephemeris; visibility footprint via In-The-Sky.org; per-site predictions via IOTA.

How to Observe the Venus Occultation

Observing a daytime occultation requires a different approach than an evening event. Here is a step-by-step plan for success.

Daytime Observing (Europe, Africa, Middle East, Asia)

  1. Calculate your exact times. Use the country table above or IOTA's prediction tools to get your disappearance and reappearance times to the nearest minute.
  2. Find the Moon first. The thin waxing crescent Moon is easy to spot in the daytime sky. Use it as your anchor.
  3. Locate Venus. Venus will be just to the east of the Moon before the occultation. At magnitude −4.8, it is visible in a blue sky through any binoculars or telescope. Scan slowly — it will appear as a brilliant white point.
  4. Track the approach. Start watching at least five minutes before disappearance. The approach is deceptively slow — Venus is 36 arcseconds wide, and the lunar limb takes roughly 70–90 seconds to cover it completely, progressively biting into the crescent.
  5. Time the disappearance. If possible, record the exact second Venus finally vanishes behind the Moon. Use a stopwatch synchronized to an accurate time source (time.gov). Report your timing to IOTA.
  6. Watch the reappearance. Venus will reappear from behind the Moon's bright limb up to an hour later. The reappearance is harder to see because the bright lunar limb washes out contrast — use higher magnification.

What the Americas See Instead

  1. No occultation from the Americas. The Moon and Venus are below the horizon for the whole 09:26–13:42 UTC window.
  2. Evening of September 14: About 45 minutes after sunset, look low in the west-southwest. The crescent Moon and Venus appear together, roughly 5–6° apart, both fitting comfortably in a binocular field of view.
  3. Naked eye first. Venus at magnitude −4.8 is obvious low in the twilight; the thin crescent Moon sits right beside it.
  4. Note the separation. It is a close pairing, but the Moon has already moved past Venus — by the evening of September 15 the gap has grown to well over 10°.
  5. Next US-visible occultation: The next time the Moon covers Venus from the contiguous United States is October 11, 2029.

Safety warning: daytime Sun

During this daytime event — for European, African, Middle Eastern, and Asian observers — the Sun is in the sky. Never point binoculars or a telescope at or near the Sun — severe eye damage will result. The Moon and Venus are about 42° from the Sun, but you must still be aware of the Sun's position at all times. If using a GoTo telescope, ensure the mount's safety limits are set.

Best Telescopes for the Venus Occultation

The Venus occultation benefits from a telescope that can track the planet automatically (for daytime acquisition) and provide enough magnification to show Venus's crescent phase and the lunar limb detail. These two picks cover the premium and budget categories.

Editor's Pick — Best for Tracking the Occultation
Celestron NexStar 8SE telescope — best for tracking the Venus occultation

Celestron NexStar 8SE Computerized Telescope

203mm aperture 2032mm focal length GoTo mount SkyAlign tech

The NexStar 8SE is a strong choice for the Venus occultation for one critical reason: its computerized GoTo mount can be aligned and slewed in the daytime sky. During the day you cannot see enough stars to use the standard SkyAlign routine. Instead, the relevant feature is Celestron's Solar System Align, which lets you align the mount on a single daytime object — the Moon works well here — and then slew accurately to Venus. (SkyAlign, the mode most people know, needs three bright objects and is a nighttime procedure; it will not help you at midday.) This automated pointing is the difference between success and frustration for a daytime event.

Once locked onto Venus, the 8-inch (203mm) aperture at 80–120× delivers a stunning view: Venus appears as a brilliant 30%-illuminated crescent 36 arcseconds across, and the Moon's terminator — the sunrise line where the occultation occurs — shows razor-sharp craters and mountains. You will see the lunar limb progressively bite into Venus's crescent, a breathtaking sight. The 8-inch aperture also gathers enough light to maintain excellent contrast even in the bright daytime sky.

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Celestron AstroMaster 70AZ telescope — budget option for Venus occultation viewing

Celestron AstroMaster 70AZ — Best budget option

70mm aperture 900mm focal length Alt-azimuth mount Budget-friendly

The AstroMaster 70AZ is a solid budget choice for the occultation. At 70mm aperture, Venus is brilliantly visible in daytime, and the 900mm focal length with a 10mm eyepiece provides 90× — enough to clearly show Venus's crescent phase and the lunar limb detail at the point of disappearance. The alt-azimuth mount is simple to set up and requires no power or electronics, making it the most portable option.

Daytime acquisition challenge: Unlike the NexStar 8SE, the AstroMaster has no GoTo capability. You must manually find Venus in the daytime sky with the finder scope. Practice this in the days leading up to September 14 — locate Venus during daylight with your naked eye first (using the Moon as a guide), then center it in the finder. It is doable with preparation but requires more skill than an automated mount.

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Photographing the Venus Occultation

The Venus occultation is one of the year's most rewarding astrophotography targets — but it is also one of the most technically challenging, especially for the daytime event in the Americas.

Smartphone through eyepiece (afocal)

  • ✓ Hold phone camera against telescope eyepiece
  • ✓ Set exposure manually to avoid overexposing Venus
  • ✓ Use a phone adapter for stability — hand shake ruins the shot
  • ✓ Record video (4K if possible) and extract frames
  • ✓ Venus will appear small but the Moon fills the frame

DSLR prime focus (through telescope)

  • ✓ Attach DSLR via T-ring directly to telescope
  • ✓ ISO 100–400, 1/250 to 1/1000 second (Venus is bright!)
  • ✓ Shoot in burst mode during disappearance/reappearance
  • ✓ Observe from the shadow of a building so the Sun is physically blocked from your aperture
  • ✓ Focus on the Moon's terminator for sharpest lunar limb

DSLR on tripod (wide-angle)

  • ✓ 200–400mm lens captures Moon + Venus with context
  • ✓ ISO 200–800, 1/30 to 1/250 second
  • ✓ Manual focus on the Moon's edge
  • ✓ Take a sequence every 30 seconds to build a time-lapse
  • ✓ Best for wide-field context shots during the daytime event
Key photographic challenge: Venus and the Moon have vastly different surface brightnesses. The Moon's sunlit crescent is bright, but Venus at magnitude −4.8 is orders of magnitude brighter per unit area. In a single exposure, you may overexpose Venus to show the Moon's terrain, or underexpose the Moon to keep Venus properly exposed. For the disappearing/reappearing sequence, expose for Venus and allow the Moon to appear overexposed — the visual impact of Venus vanishing is more important than lunar surface detail.

Venus Occultation September 14, 2026 — FAQ

What is a lunar occultation of Venus?

A lunar occultation occurs when the Moon passes directly in front of Venus, hiding it from view. On September 14, 2026, the waxing crescent Moon covers Venus — then brilliant at magnitude −4.8 — for approximately 40–60 minutes, creating one of the most dramatic sky events of the year.

When is the Venus occultation in September 2026?

The occultation occurs on September 14, 2026, between 09:26 and 13:42 UTC — the middle of the day for every region where it is visible (Europe, Africa, the Middle East, western Russia, and southern Asia). It is not visible from the Americas. See the country table above for the span of times in your country.

Do I need a telescope to see the Venus occultation?

Yes — binoculars or a telescope are essential everywhere the occultation is visible, because it is a daytime event in every location within the footprint. Venus is bright enough to see in a blue daytime sky, but you need optical aid to find it and to watch the crescent being bitten away.

What is the best telescope for the Venus occultation?

Our top recommendation is the Celestron NexStar 8SE. Its computerized GoTo mount can be aligned on the Moon (using Solar System Align) and then find Venus in the daytime sky — a critical advantage for a daylight event. Its 8-inch aperture delivers stunning detail on Venus's 30%-lit crescent and the lunar mountains at the occultation point. For budget observers, the Celestron AstroMaster 70AZ is a capable alternative if you practice daytime Venus acquisition in advance.

Is it safe to observe a daytime occultation?

Yes — as long as you are aware of the Sun's position. Venus and the Moon are about 42° from the Sun on September 14, 2026. However, you must never point your telescope or binoculars at or near the Sun. Use a GoTo mount with safety limits set, or carefully verify your aim before looking through the eyepiece.

Can I photograph the Venus occultation with a smartphone?

Yes, but with limitations. Pointing a smartphone camera through a telescope eyepiece (afocal method) can capture the event. Use manual exposure control (tap and drag to reduce exposure) to avoid overexposing Venus. A phone-eyepiece adapter is highly recommended. For better results, use a DSLR through the telescope or on a telephoto lens.

What does Venus look like during the occultation?

Through a telescope, Venus appears as a brilliant 30%-illuminated crescent 36 arcseconds wide. As it approaches the Moon's dark limb, the lunar edge takes roughly 70–90 seconds to bite into the crescent, progressively thinning it to a sliver before the last of it vanishes. On reappearance, Venus emerges from the Moon's bright limb, initially hidden by glare before becoming visible.

Is the Venus occultation visible from Europe?

Yes, but in late-morning daylight, not twilight. Continental Europe sees the event low in the south-eastern sky (roughly 8–15° altitude in Iberia, higher further east and north). The Canary Islands fall outside the footprint, and the UK is not in In-The-Sky's visibility list — check IOTA predictions for any site before planning.

Can I see the Venus occultation from the United States?

No — the September 14, 2026 occultation is not visible from the contiguous United States (or anywhere in the Americas). The most recent Venus occultation visible from the contiguous US was June 17, 2026; the next will be October 11, 2029. Instead, US and Canadian observers can watch the Moon and Venus pairing up low in the west-southwest after sunset on the evening of September 14, roughly 5–6° apart.

How long does the Venus occultation last?

From disappearance to reappearance, the occultation lasts approximately 40–60 minutes, depending on your exact location. During this time, Venus is completely hidden behind the Moon. The exact duration varies because of parallax — observers south of the center line see a shorter occultation than those near the center.

Can I submit my timing observations to science?

Yes! The International Occultation Timing Association (IOTA) welcomes amateur timing observations of occultations. Record the exact second of disappearance and reappearance (using a stopwatch synced to time.gov), note your precise location (GPS coordinates), and the telescope/aperture used. Submit your observation on the IOTA website. Your data helps refine lunar topography and planet ephemerides.



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Sources & References

Occultation visibility, timings, and the physical data for Venus in this guide are verified against the JPL planetary ephemeris and authoritative astronomy references. Times are UTC unless otherwise noted.

Correction notice — updated August 17, 2026

This guide was substantially corrected after an accuracy audit. Earlier versions incorrectly stated the occultation was visible from the Americas (it is not — it is a daytime event in Europe, Africa, the Middle East, and Asia), gave per-city times that were not sourced, and misstated Venus's distance, phase, angular size, and magnitude. All figures now reflect JPL Horizons and In-The-Sky.org (JPL DE440).

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