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Venus Conjunctions with other Planets, 2017

Moon near Venus Dates, Apr 2017 to Oct 2017

The Venus Evening Apparition of 2016-17

Star map showing the path of Venus through the zodiac during the 2017 morning apparition (Copyright Martin J Powell, 2017)

The Path of Venus through the Zodiac Constellations during the planet's morning apparition in 2017 (move your cursor over the image - or click on it - to reveal the constellation names in their abbreviated three-letter form - the full names are listed here). Tick-marks indicate the first day of each month. Zodiac constellations are labelled in green and non-zodiac constellations in grey. The numbers along the sides of the chart (Right Ascension and Declination) are co-ordinates of celestial longitude and latitude which are used to locate the position of celestial bodies in the night sky. A print-friendly version is available here.

The Venus Morning Apparition of 2017

by Martin J Powell

Venus passes through inferior conjunction (when it is positioned between the Earth and the Sun) on March 25th 2017, positioned a siignificant 8º.3 North of the Sun's centre. For observers at latitudes North of about 50º North, Venus is positioned sufficiently far North of the Sun - and thus sufficiently far above the Eastern horizon - for it to be glimpsed in the bright dawn twilight from inferior conjunction day itself. Elsewhere the planet swiftly enters the dawn sky as a 'Morning Star' over the following week, visible in the twilight, low down over the Eastern horizon less than 30 minutes before sunrise (the exact period depending upon the observer's latitude).

2 0 1 7  March

 Orbitally, Venus is positioned at a relatively close 0.281 Astronomical Units (AU) from the Earth (42 million kms or 26.1 million statute miles), a distance which will continually increase over the next nine months, through to the end of the apparition. The planet is moving retrograde (East to West) at this time, positioned in the central Western region of the constellation of Pisces, the Fishes. Venus reaches a solar elongation of 10º West on March 29th, and on the same day the planet briefly leaves Pisces and enters the adjacent constellation of Pegasus, the Flying Horse. Venus clips the constellation's South-eastern corner, moving diagonally across it, before returning to Pisces just two hours later. The planet currently shines at an apparent magnitude of -4.1 and its apparent diameter (its angular width as seen from the Earth) is a sizeable 59" (i.e. 59 arcseconds, where 1 arcsecond = 1/3600th of a degree). Venus' apparent diameter will continually shrink during the apparition, as it slowly recedes from the Earth in space.

2 0 1 7  April

On April 3rd the apparition truly gets underway as Venus reaches an elongation of 15º West, making it more readily visible in the dawn twilight from all except higher Northern latitudes. By April 7th the planet is moving into the Circlet of Pisces, a group of faint stars which form the head of the Southernmost fish. On April 13th, whilst within the Circlet, Venus reaches its Western stationary point, some 1º.5 West of the variable star 19 Piscium or TX Piscium (mag. +5.0v). Now moving Southward, the planet passes 0º.5 North of Greek lower-case letter 'lambda' Psc (Lambda Piscium, mag. +4.5), located at the South-eastern corner of the Circlet, on April 17th. Venus leaves the Circlet on the following day, arcing its way around towards the South-east against the background stars.

Venus as a thin crescent photographed in the dawn sky by Vincenzo Mirabella in August 2015 (Photo: Vincenzo Mirabella/ALPO-Japan)

Venus as a thin crescent photographed through a 9¼" SCT telescope in the dawn twilight by Vincenzo Mirabella (Ardea, Italy) in August 2015. The planet was 7% illuminated and positioned 22° West of the Sun.

(Image: Vincenzo Mirabella/ALPO-Japan)

As it pulls away from the Sun, telescopes pointed towards Venus show a large, slender, Eastward-facing crescent, rippling in the Earth's turbulent atmosphere (click here to see how Venus typically appears through a small telescope at various phases). The planet's phase (i.e. the percentage of the disk which is illuminated) is only around 5% (phase = 0.05). The planet's large apparent diameter also means that the crescent can be glimpsed in the twilight by observers using binoculars, its apparently tiny crescent facing down towards the horizon.

At this early stage of the apparition, dedicated telescopic observers of Venus now begin their search for the elusive Ashen Light, which is a faint glowing of the night side of Venus through its thick clouds. The phenomenon is believed to be caused either by the planet's surface glowing red hot (due to its extremely high surface temperature) or due to electrical activity in its dense atmosphere. Observers searching for the Light will normally use ultraviolet and/or infrared filters in order to help reveal it, an occulting bar often being used to block the bright, visually-intrusive crescent from view. Observers in higher Southern latitudes are best placed to view the Light at this stage of the apparition due to the planet's higher altitude (angle above the horizon) before sunrise.

Observers at higher Northern latitudes have considerable difficulty viewing Venus at this early stage of the apparition, the planet rising in twilight and barely reaching a few degrees above the horizon before the sky becomes too bright to see it with ease. At latitude 60º North the planet's visibility worsens slightly over the next month because its position along the ecliptic (the path of the Sun, which the Moon and planets follow very closely) places it very low down above the Eastern horizon at dawn at this time of year. From these latitudes Venus will not become visible with greater ease until about mid July. Elsewhere the planet is rising 1¼ hours before sunrise (at 50º North), 1¾ hours before sunrise (at 30º North), 2 hours before sunrise (at the Equator) and 2½ hours before the Sun (at 35º South). At thirty minutes before sunrise, Venus stands just 7º high in the East at 50º North, 15º high in the East at 30º North, 23º high in the East at the Equator and 24º high in the ENE at 35º South.

On April 26th Venus attains its greatest brilliancy for this apparition, at magnitude -4.5. This is the position in the planet's orbit when its phase, its apparent size and its apparent magnitude combine to best visual effect, as seen from the Earth. At greatest brilliancy in the current apparition, Venus is positioned 37° West of the Sun with a 23% illuminated crescent (phase = 0.23) and an apparent diameter of 41".2. Southern hemisphere observers have the best view of the planet as it blazes brilliant white against a truly dark sky.

In late April Venus is joined in the dawn sky by the planet Mercury (mag. +3.0), now commencing its second morning apparition of 2017. Owing to the steep angle of the ecliptic to the local Eastern horizon at dawn at this time of year, this apparition of Mercury favours observers in the Southern hemisphere. It is one of two paired apparitions between Venus and Mercury which take place during the year (a paired apparition being when the two planets are visible together for a prolonged period of time, either in the morning sky or the evening sky). This particular pairing lasts through to early June; it is an interesting one because both planets reach their greatest elongations from the Sun during the period.

2 0 1 7  May

Venus crosses the ecliptic in a Southward direction on May 9th and on May 11th it again exits the zodiac for a short period of time. The planet enters the constellation of Cetus, the Whale, at around 0200 UT, cutting across its North-western corner, returning to Pisces at around 1700 UT on the same day. This is the first of two excursions into the Whale constellation which the planet will make over the course of the next 30 days.

Venus and Mercury come to within 19º of each other around the 15th of the month, Mercury attaining its greatest elongation from the Sun (26º West) two days later, shining at an apparent magnitude of +0.6. The waning crescent Moon passes near the two planets between May 21st and 24th, providing an ideal photographic opportunity to capture our sole natural satellite and the two innermost planets of the Solar System together in the morning sky. On May 18th Venus passes 3º.5 South of the star Delta Piscium (Greek lower-case letter 'delta' Psc, mag. +4.4), positioned about half-way along the Southern Fish's body, and then 2º.8 South of the star Epsilon Piscium (Greek lower-case letter 'epsilon' Psc, mag. +4.3) on May 22nd.

From mid to late May, observers at mid-Southern latitudes see Venus attain its highest altitude in the sky before sunrise for the 2017 apparition. At 35° South, the planet rises 3¾ hours before the Sun, reaching an altitude of around 35° in the North-east at 30 minutes before sunrise. Elsewhere, Venus rises in the East 1½ hours before sunrise (at 50° North), 2¼ hours before sunrise (at 30° North) and almost three hours before sunrise (at the Equator). For Southern hemisphere observers this is the second best of Venus' five morning apparitions during its 8-year cycle, the planet typically attaining higher-than-average altitudes above the horizon when compared to the other four morning apparitions (for more details, see the accompanying article describing The Venus 8-year Cycle).

2 0 1 7  June

On June 2nd Venus, having faded slightly to mag. -4.2, passes 1°.8 South of the planet Uranus (mag. +5.9) in the first of three planetary conjunctions which take place during the 2017 morning apparition. A planetary conjunction (or appulse) takes place whenever two planets attain the same celestial longitude in the night sky (i.e. they appear to 'line up' when seen from the Earth). This first conjunction is best seen from the Southern hemisphere; details of this and the other planetary conjunctions involving Venus during the year are given in the 'planetary conjunctions' section below.

For Equatorial observers, early June sees the planet attain its highest altitude above the horizon before sunrise for the current apparition. Here Venus rises three hours before the Sun, reaching a significant 37° above the ENE horizon some 30 minutes ahead of sunrise. In fact, when assessed in terms of the planet's horizon altitude and visibility duration before sunrise, the 2017 morning apparition of Venus is best seen overall from Equatorial latitudes.

Around 1200 UT on June 3rd, Venus reaches its greatest Western elongation (45°.86 West of the Sun), positioned 1°.7 to the SSW of Uranus and 0°.9 SSW of the star Torcularis Septentrionalis (Greek lower-case letter 'omicron' Psc or Omicron Piscium, mag. +4.2) in the tail of the Northern Fish. Although the planet's greatest elongation from the Sun takes place on June 3rd, Venus is in fact positioned at an elongation of 45°.8 for a 12-day period from May 29th through to June 9th.

Contrary to what one might think, greatest elongation day is not necessarily the day on which Venus is above the horizon ahead of sunrise for the longest period of time. Since the angle of the ecliptic to the Eastern horizon at dawn varies with the observer's latitude, Venus is above the horizon for differing periods of time. At 60° North Venus rises just 50 minutes before sunrise, whilst at 50° North the planet rises 1¾ hours before the Sun. At other latitudes the visibility durations are as follows: two hours at 40° North; 2½ hours at 30° North; 2¾ hours at 20° North; three hours at the Equator; 3¼ hours at 15° South; 3½ hours at 25° South; 3¾ hours at 35° South and four hours at 45° South. Hence for the current apparition, observers at higher Southern latitudes are best placed to see Venus above the horizon for the longest period on greatest elongation day.

Telescopes now show Venus' disk half-illuminated (phase = 0.50) with an apparent diameter of 23".8. Theoretically, greatest elongation is the time at which the planet's terminator (the line separating the light and dark sides of the planet) appears perfectly straight through telescopes, essentially dividing Venus into two perfect halves; this is known as the dichotomy. However, telescopic observers often report the straight terminator several days earlier or later than the greatest elongation date. Interestingly, the date of dichotomy is usually reported early in evening apparitions and late in morning apparitions. The precise reason for this phenomenon - which is referred to as Schröter's Effect - is not known, however it may simply be due to the fact that the precise moment of dichotomy cannot be determined by an observer to within an accuracy any better than a few days.

Some eleven hours after reaching greatest elongation, Venus passes 1º.8 North of Torcularis Septentrionalis (Latin for 'North Press', a mistranslation of an original Greek word meaning 'flax', i.e. the cord that ties the two fishes' tails together). The planet will occult (pass in front of) this star during its 2027 morning apparition.

Venus enters Cetus once more at around 1415 UT on June 9th, passing 13°.2 South of the star Hamal (Greek lower-case letter 'alpha' Ari or Alpha Arietis, mag. +2.0) in neighbouring Aries, the Ram before entering Aries itself the following day at around 1905 UT. The planet passes 4º.6 South of Botein (Greek lower-case letter 'delta' Ari or Delta Arietis, mag. +4.3), the Ram's Easternmost bright star, on June 25th.

Greatest elongation day long having passed, telescopes show Venus with a 60% illuminated phase (slightly gibbous) in late June. The planet's phase will remain gibbous through the remainder of the apparition. The apparent diameter has reduced slightly to around 19" and the planet shines at an apparent visual magnitude of -4.1.

Venus enters Taurus, the Bull, on June 28th, passing 3º.3 North of the star 5 Tau (5 Tauri, mag. +4.1) on June 30th. The planet will spend most of July in this constellation, the most Northerly of the zodiac.

2 0 1 7  July

At around 0800 UT on July 3rd Venus begins to pass South of Taurus' most famous star cluster called the Pleiades (pronounced 'PLY-add-eez' or 'PLEE-add-eez'), also known as the Seven Sisters (Messier 45). The planet takes about 22 hours to traverse the 1° angular distance between the cluster's brightest Western star (Electra, mag. +3.7) and its brightest Eastern star (Atlas, mag. +3.6). The vertical angular distance between the cluster and the planet is about 7°. On July 6th the planet passes 5°.5 North of the eclipsing binary star Greek lower-case letter 'lambda' Tau (Lambda Tauri), whose magnitude varies from ca. 3.5 to 4.0 over a period of four days.

Since inferior conjunction in late March, Venus has been receding from the Earth in space at an average rate of about 996,000 kms (619,000 miles) per day. At 1502 UT on July 11th, Venus is positioned at precisely 1.000 AU from the Earth, i.e. the same distance as the average distance of the Earth from the Sun (149.5 million kms or 92.9 million statute miles).

Crescent Venus photographed by Stephane Gonzales in October 2015 (Photo: Stephane Gonzales)

Crescent Venus at 41% phase photographed through a 250mm Newtonian telescope by Stephane Gonzales (Surgeres, France) in October 2015. The photo hints at the pale 'lemon yellow' colouration which is often reported by dedicated telescopic observers of the planet.

(Image: Stephane Gonzales)

Between July 11th and 14th Venus passes a few degrees North of another, much larger star cluster known as the Hyades, a distinct 'V'-shaped grouping of stars forming the head of the Bull. At the apex of the 'V' is a star known variously as Prima Hyadum, Primus Hyadum or Hyadum I (Greek lower-case symbol 'gamma' Tau or Gamma Tauri, mag. +3.6). Venus passes 3°.3 North of the star at around midnight UT on July 11th. Sixteen hours later the planet passes 1°.6 North of Hyadum II (Greek lower-case symbol 'delta'1 Tau or Delta-1 Tauri, mag. +3.7), a triple star system positioned about half-way along the Northern arm of the 'V'. Also positioned along the Northern arm is the star Ain (Greek lower-case letter 'epsilon' Tauri, mag. +3.5), marking the base of the Bull's Northern horn. Venus passes just 11' (11 arcminutes, where 1 arcminute = 1/60th of a degree) North of the star at around 2130 UT on July 12th. Occupying the South-eastern corner of the Hyades cluster is the orange-red star Aldebaran (Greek lower-case symbol 'Alpha' Tau or Alpha Tauri, mag. +0.9), marking the 'eye' of the Bull. Its coloration derives from the fact that it is a red giant star. Most of the Hyades stars comprise a genuine cluster, moving through space together, however Aldebaran is not part of the group; it is a foreground star, positioned closer to the Earth than the cluster. Venus passes 3°.2 North of Aldebaran on July 14th.

Around mid July, observers situated at Northern Tropical latitudes see the planet attain its highest altitude before sunrise for the 2017 morning apparition. At 30° North, Venus rises almost three hours ahead of the Sun, reaching 29° above the Eastern horizon at half-an-hour before sunrise. Elsewhere the planet is also rising about three hours before the Sun; at 30 minutes before sunrise, Venus reaches 14° high in the ENE at 60° North, 20° high in the East at 50° North, 32° high in the ENE at the Equator and 23° high in the North-east at 35° South.

About half-way along the Bull's Southern horn is the unremarkable fifth-magnitude star 104 Tauri (mag. +4.9). At around 1115 UT on July 20th, observers in Southern Argentina and Southern Chile are able to observe the waning crescent Moon pass in front of this star, obscuring it from view, in an event called a lunar occultation. Elsewhere the Moon is seen in the vicinity of the star from around 10 to 14 hours UT on the same day. Venus itself passes 2°.2 North of the star on the following day (July 21st); it too will occult the star during the course of its morning apparition in July 2028.

On July 25th Venus passes 7°.2 South of the star Al Nath or El Nath (Greek lower-case letter 'beta' Tau or Beta Tauri, mag. +1.6), located at the tip of the Bull's Northern horn. The star also has the name Gamma Aurigae (Greek lower-case symbol 'gamma' Aur) since, apart from marking one of the Bull's horns, it also neatly completes the six-sided figure comprising the stars of Auriga, the Charioteer, located to the North-east of Taurus. The star marking the tip of the Bull's Southern horn is Zeta Tauri (Greek lower-case letter 'zeta' Tau, mag. +2.9v) and Venus passes just 23' (0°.4) North of it on July 27th.

Venus leaves Taurus and again departs the zodiac for a short while, entering the constellation of Orion, the Hunter, on July 29th. The planet then cuts across the North-eastern section of the constellation, just above the Hunter's club, passing 1°.5 North of the star Chi Orionis (Greek lower-case letter 'chi'1 Ori, mag. +4.4) on July 30th. Venus leaves Orion and crosses into Gemini, the Twins, on July 31st.

2 0 1 7  August

August commences with Venus passing 1°.3 South of the star 1 Gem (1 Geminorum, mag. +4.2), the Westernmost bright star in Gemini, marking the foot of the Northern twin. On August 3rd the planet passes 0°.5 South of the star Propus or Tejat Prior (Greek lower-case symbol 'eta' Gem or Eta Geminorum, mag. +3.5v) and on August 5th, 0°.5 South of the star Tejat Posterior (Greek lower-case symbol 'mu' Gem or Mu Geminorum, mag. +3.0v), which marks the Northern twin's knee.

At around 20 hours UT on August 5th, Venus attains its most Northerly declination (symbol Greek lower-case letter 'delta') for this apparition, at Greek lower-case letter 'delta' = +21° 58' 16" (or +21°.97 in decimal format). Across the world, the planet now rises at its most Northerly point along the local horizon, the actual point of rising depending upon the observer's latitude. In early August at higher Northern latitudes Venus rises in the North-east, whilst at latitudes further South it rises in the ENE. The planet is now 1°.3 South of the ecliptic, so it is by no means as far North as the planet is capable of travelling. Indeed, the next highest declination which Venus will attain will be +27°.81 during its evening apparition in May 2020, when it will be positioned in North-eastern Taurus, close to the border with Auriga. This will be the highest declination attained by planet until the year 2077.

Venus rising at dawn during the 2012-13 morning apparition (Copyright Martin J Powell, 2012)

Venus pictured in the dawn sky during the planet's 2012-13 morning apparition (click on the thumbnail for the full-size picture).

Around early to mid August, observers at high and mid-Northern latitudes see Venus attain its highest altitude in the sky before sunrise for the 2017 apparition. From higher Northern latitudes, the planet is now rising in darkness, having spent the previous two months of the apparition rising in twilight. At latitude 60° North, the planet rises over 3½ hours ahead of the Sun, attaining an altitude of 19° above the Eastern horizon at 30 minutes before sunrise. At mid-Northern latitudes, the planet rises a little over three hours before the Sun, reaching 22° above the Eastern horizon at 30 minutes before sunrise. These altitudes are not particularly high; for naked-eye observers in the Northern hemisphere, the 2017 apparition is only the third best of Venus' five morning apparitions over the planet's 8-year cycle (see the accompanying article describing The Venus 8-year Cycle). From Northern latitudes this apparition sees Venus attain only moderate altitudes above the horizon at dawn when compared to the other four morning apparitions.

On August 6th Venus passes 1°.7 North of the star Lower-case Greek letter 'Nu' Gem (Nu Geminorum, mag. +4.1), the lower foot of the Northern twin, which the planet will occult in August of 2028. On August 8th the planet passes 5°.5 North of Alhena (Greek lower-case letter 'gamma' Gem or Gamma Geminorum, mag. +1.9) at the foot of the Southern twin, then on the 9th, 3°.2 South of Mebsuta (Greek lower-case letter 'epsilon' Gem or Epsilon Geminorum, mag. +3.0) positioned at the groin of the Northern twin. Venus now appears at the apex of an isoscelene triangle with Gemini's brightest stars Castor (Greek lower-case letter 'alpha' Gem or Alpha Geminorum, mag. +1.6) and Pollux (Greek lower-case letter 'beta' Gem or Beta Geminorum, mag. +1.1), the long sides of the triangle measuring a little over 15° and the angular distance of the short side (from Castor to Pollux) being 4°.5. The temporary celestial triangle points South-westwards towards Orion.

On August 13th Venus passes 1°.1 North of the optical double star Mekbuda (Greek lower-case letter 'zeta'Gem or Zeta Geminorum, mag. +3.9v), positioned at the right knee of the Southern twin, then passes 0°.5 North of the star Wasat (Greek lower-case letter 'delta' Gem or Delta Geminorum, mag. +3.5) on August 16th. Venus passes 10°.7 South of Castor itself on August 19th.

At around 1045 UT on August 21st, Pollux, Greek lower-case letter 'kappa' Gem (Kappa Geminorum, mag. +3.5) and Venus (mag. -4.0) form a straight line about 7°.2 in length, aligned roughly North-South. The angular distances between Pollux and  Greek lower-case letter 'kappa' Gem and between Greek lower-case letter 'kappa' Gem and Venus are about the same (ca. 3°.5). As luck would have it, the line points almost directly towards the bright star Procyon (Greek lower-case letter 'alpha' CMi or Alpha Canis Minoris, mag. +0.5) in the constellation of Canis Minor, the Lesser Dog, some 15°.7 to the South of Venus.

As millions look skyward to observe the total solar eclipse over the USA later that same day, Venus is positioned 34°.3 West of the Sun; at minus fourth magnitude the planet is easily seen against the twilit sky, caused by the eclipse totality (the positions of the planets in relation to the eclipsed Sun are discussed here). At around 1845 UT, shortly before the Moon's shadow leaves the coast of South Carolina and heads out into the Atlantic Ocean, Venus passes 7°.2 South of Gemini's brightest star Pollux.

On August 24th, the planet leaves Gemini and enters the constellation of Cancer, the Crab, passing 10°.4 North of the star Altarf (Greek lower-case letter 'beta' Cnc or Beta Cancri, mag. +3.5) three days later. Venus crosses the ecliptic heading Northwards on August 30th.

2 0 1 7  September

At the start of September Venus is positioned around 1° South of the star cluster known as Praesepe (pronounced 'PRE-SEEP-EE'), designated Messier 44 (M44 or NGC 2632). It is also known by the names Beehive Cluster (the reason being evident when one looks at the cluster through binoculars) or, more rarely, The Manger. Venus takes some 17 hours to traverse the angular width of the cluster, commencing its passage at around 1030 UT on September 1st and completing it at around 0330 UT on September 2nd. The planet passes just 5' (0°.08) North of the star Asellus Australis (Greek lower-case letter 'delta' Cnc or Delta Cancri, mag. +3.9), positioned to the South-east of the cluster, later that same day.

In early September Venus is rising 3½ hours before the Sun at latitude 60° North, reaching an altitude of 18° in the East at 30 minutes before sunrise. At 50° North the planet rises three hours ahead of the Sun, reaching 21° high in the East at 30 minutes before sunrise. At latitudes further South the durations, altitudes and directions at a half-hour before sunrise are as follows: 2½ hours before sunrise, reaching 23° in the East (at 30° North); two hours before sunrise, reaching 20° in the ENE (at the Equator) and 1½ hours before sunrise, reaching 10° in the ENE (at 35° South).

A gibbous Venus sketched by David Gray in June 2014 (Photo: David Gray/ALPO-Japan)

A Gibbous Venus sketched in June 2014 by David Gray (Kirk Merrington, UK) using a Dall-Kirkham 415mm telescope at 365x magnification. The subtle cloud features were revealed using deep yellow, blue and green-tricolor filters.

(Image: David Gray/ALPO-Japan)

On September 5th Venus passes 5°.6 North of the star Acubens (Greek lower-case letter 'alpha' Cnc or Alpha Cancri, mag. +4.2), which is positioned at the South-eastern corner of the Crab constellation's lambda-shaped (Greek lower-case letter 'lambda') pattern. Around this time, Venus is again joined in the dawn sky by the planet Mercury (mag. +1.3) in the second of two paired apparitions between the two planets during 2017. Unlike Mercury's previous morning apparition in April, this one favours Northern hemisphere observers. Venus enters Leo, the Lion, on September 10th, Mercury reaching greatest elongation two days later, at 18° West of the Sun. The two planets do not get close enough to reach conjunction, Mercury at best coming to within 11° of Venus on September 14th.

Also on September 14th, Venus passes 4°.7 North of the star Subra (Greek lower-case letter 'omicron' Leo or Omicron Leonis, mag. +3.5), marking the paw of the Lion's foreleg. Between September 15th and 22nd Venus is positioned South of the asterism known as the Sickle of Leo, at the Western end of the constellation, which appears to the naked-eye as a backward question-mark (A backward question-mark). The constellation's brightest star Regulus (Greek lower-case letter 'alpha' Leo or Alpha Leonis, mag. +1.4) is in the equivalent position of the dot.

Some 13° to the East of Venus, Mars (mag. +1.8) is now emerging out of the dawn twilight into the start of its 2017-19 apparition. This is an important apparition for the Red Planet which, in July 2018, will see it reach its closest point to the Earth in almost fifteen years. On September 16th Mars and Mercury are in close conjunction with each other, just 0°.1 apart, the pair being positioned 11°.2 to the ESE of Venus. The conjunction is a difficult one to observe, however, taking place just 17° from the Sun and visible only from the Northern hemisphere. The waning crescent Moon passes near the three planets between September 17th and 19th.

Between September 18th and 19th the Moon passes to the South of Venus, forming a triangular arrangement with nearby Regulus as seen from locations North of the Equator. At around 0055 UT on September 18th, observers in the Eastern Indian Ocean are able to see the Moon pass in front of Venus, obscuring it from view, in an event called a lunar occultation. Here the event is seen in darkness and/or twilight, depending upon the precise location of the observer. In Australia, New Zealand, Indonesia and Papua New Guinea observers see the event in daylight. Further details of this event can be found by following the link in the 'Moon near Venus Dates' section below.

At 1730 UT on the same day (September 19th local time), Mars is seen to be occulted by the Moon in twilit conditions by observers located within a narrow strip of the North-western Pacific Ocean. Venus is 10° to the WNW of the Red Planet at this time. The re-appearance of Mars is visible just after Moonrise at around 1830 UT from the remote island of Minami-Tori-shima (Marcus Island).

A third lunar occultation takes place on this day: at around 2050 UT Mercury, now at magnitude -0.9 and just 16° West of the Sun, is also occulted by the thin waning crescent Moon. The event is seen in twilight just after Moonrise from South-eastern China, Taiwan and the Philippines.

Between the two latter events, the Moon, Mercury and Mars form a tight trio less than 2° apart, the closest grouping between these three celestial bodies before the year 2036. Venus is positioned about 11° to the WNW of the trio. From the Northern Mariana Islands, the Moon is seen nicely positioned midway between Mercury and Mars in the brightening twilight shortly after Moonrise on September 19th local time.

Mercury and Venus continue to be visible together as 'morning stars' through to about the 20th of the month, after which Mercury heads out of view into the twilight.

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Venus passes 0°.5 North of Regulus on September 19th, a relatively close pass which is visible shortly before dawn twilight from Eastern India, Northern Pakistan, Western China and Western central Russia. Venus will occult Regulus during its morning apparition in 2044, the brightest star to be occulted by the planet up until that year; the occultation will be visible at dawn from Eastern Asia.

By late September Venus' solar elongation has reduced to 25° and it appears only slightly gibbous through telescopes, showing a 90% illuminated phase. The apparent disk diameter is around 11", i.e. only half the size it had been in mid June and a third of the size it had been in mid May. With such a small disk size, little can now be discerned in the way of the planet's characteristic cloud markings.

Mid-Southern hemisphere observers now have a rapidly shortening window in which to observe Venus. At latitude 35° South, the planet rises in twilight only an hour ahead of the Sun, attaining just 5° in altitude in the ENE at 30 minutes before sunrise.

2 0 1 7  October

Since the first appearance of Mars in the dawn sky in mid-September, Venus has been closing in on the Red Planet at an average rate of 0°.6 per day. On October 5th the two planets meet, Venus passing just 0°.2 North of Mars in a planetary conjunction which is best seen from the Northern hemisphere. The star Greek lower-case letter 'sigma' Leo (Sigma Leonis, mag. +4.0), at the foot of the Lion's hind leg, is positioned just 0°.3 to the NNE of Venus at the time of the conjunction. One hour after the event, Venus passes 0°.3 South of the star. Further details of the event can be seen in the 'planetary conjunctions' section below.

Venus enters Virgo, the Virgin, on October 9th, a constellation which Southern hemisphere observers are already having some difficulty viewing in the dawn twilight. The planet passes 3°.3 South of the star Lower-case Greek letter 'Nu' Vir (Nu Virginis, mag. +4.0), at the top of the Maiden's head, on October 11th, then 0°.8 North of Zavijah (Greek lower-case letter 'beta' Vir or Beta Virginis, mag. +3.6), at the back of her head, on October 12th.

From mid October, observers situated at mid-Southern latitudes are the first to lose sight of Venus from the dawn sky as it slips into the bright Eastern horizon.

Venus crosses the celestial equator (where the declination of a celestial body is 0°) heading Southwards on October 17th, causing the planet to rise due East across the inhabited world. On October 18th Venus passes 0°.2 North of the star Zaniah (Greek lower-case letter 'eta' Vir or Eta Virginis, mag. +3.8) then five days later (23rd) 1°.3 South of the double star Porrima or Arich (Greek lower-case letter 'gamma' Vir or Gamma Virginis, mag. +3.5). The planet passes 0°.2 South of another double star, Theta Virginis (Greek lower-case letter 'theta' Vir, mag. +4.4) on October 29th.

In late October Venus is rising two hours before sunrise at 60º North, 1¾ hours before sunrise at 50º North, 1¼ hours before the Sun at 30º North and one hour before the Sun at the Equator. At thirty minutes before sunrise, Venus attains an altitude of 9º in the ESE at 60º North, 10º in the ESE at 50º North, 10º high in the East at 30º North and just 7º high in the East at the Equator. Telescopes turned towards Venus now show a tiny disk measuring a little over 10" across and showing a phase of around 95% - so slightly gibbous that the planet effectively appears 'full'.

2 0 1 7  November

On November 1st Venus passes 3º.8 North of Virgo's brightest star, Spica (Greek lower-case letter 'alpha' Vir or Alpha Virginis, mag. +1.0), a blue-white star which dominates the South-eastern region of the constellation.

By November 6th Venus' solar elongation has reduced to just 15º and from the latitudes which are still able to see it, the planet is rising in twilight again. Around this time, Jupiter (mag. -1.5) emerges from the dawn twilight into the morning sky at the start of its 2017-18 apparition. It is 4º.5 to the ESE of Venus on November 9th, the gap between the two closing over the coming days. On November 10th Jupiter is 3º.5 to the ESE of Venus, on the 11th it is 2º.4 to the ESE and on the 12th it is 1º.3 to the South-east. At around 0610 UT on November 13th the two planets meet in conjunction, Venus passing 0º.3 to the North of Jupiter. At the moment of conjunction the pair are positioned just 21' (0º.3) West of Virgo's border with Libra, the Balance or Scales, which Venus enters later that same day.

In the days following the conjunction, Venus pulls away Eastwards from Jupiter at average rate of 0°.9 per day and its solar elongation continues to reduce. By November 28th the planet is positioned just 10º West of the Sun and is increasingly difficult to view from most latitudes, observers at high-Northern latitudes losing sight of Venus from around this time.

2 0 1 7  December

Venus enters Scorpius, the Scorpion, on December 3rd and then Ophiuchus, the Serpent Bearer, on December 7th. From early December, observers at mid-Northern latitudes lose sight of Venus as it sinks into the bright South-eastern horizon. Observers at Equatorial and Northern Tropical latitudes lose the planet from view by the middle of the month, bringing the 2017 morning apparition to a formal close.

Venus passes 2°.2 South of Mercury on December 15th in an unobservable planetary conjunction just 6° from the Sun. Mercury is now entering its seventh and final apparition of 2017, having undergone four morning apparitions and three evening apparitions during the year. The current morning apparition lasts through into January and slightly favours Northern hemisphere observers.

Venus crosses the ecliptic heading Southwards on December 20th and enters Sagittarius, the Archer, on December 22nd. On December 25th Venus passes 1º.1 South of Saturn (mag. +0.5) in another unobservable planetary conjunction, this one taking place just 3°.5 West of the Sun. Venus attains its most Southerly declination for this apparition, at -23° 42' 32" (-23°.71 in decimal format), on December 28th.

2 0 1 8  January

Venus reaches superior conjunction (passing behind the Sun as seen from the Earth) in Eastern-central Sagittarius on January 9th, positioned 0°.7 South of the Sun. The planet is now at a very distant 1.711 AU (255.9 million kms or 159 million statute miles) from the Earth. Were it to be visible from the Earth at this point, Venus would have an apparent diameter of just 9".8 and would shine at a magnitude of -3.8.

Having passed from the morning to the evening sky, Venus remains out of view - lost in the solar glare - for a further month, as it makes its slow passage on the far side of its orbit from the Earth. The planet becomes visible once again from around early February 2018, when it is seen shortly after sunset from Equatorial latitudes as an 'Evening Star' in the WSW, heralding the 2018 evening apparition of Venus which lasts through to October of that year.

 [Terms in yellow italics are explained in greater detail in an associated article describing planetary movements in the night sky.]

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Finding Venus in Your Local Night Sky using AstroViewer®

Where in the night sky should I look for Venus tonight? In which direction and how high up will it be?

The location of a planet (or any other celestial body) in your local night sky depends upon several factors: the constellation in which it is positioned, your geographical latitude and longitude and the date and time at which you observe. To find a planet in the night sky at any particular date and time, we must know two things: a direction in which to look along the observer's horizon (e.g. Southeast, East-Southeast) and an angle to look above the horizon (known as altitude or elevation).

The following Javascript program can also be used to help find Venus (and any other planets) in your night sky throughout the year: 

'Mini-AstroViewer' Java applet

For additional information on the fully-functional

version of the program, see here.

Mini-AstroViewer® is an easy-to-use Java applet which shows the positions of the celestial bodies in the night sky for any location on the globe at any time of the year (Javascript must be enabled in your browser for the program to function).

To activate the program, click on the button below (the program will open in a pop-up window).

Please enable JAVATM to use the Mini-AstroViewer night sky map.

The default location is New York, USA. To select your own location and then find Venus, refer to the 'Finding Venus ..' box below.

An animated tutorial showing how to locate a planet in the night sky using Mini-AstroViewer® can be seen here.

  • The applet also shows the positions of the planets in their orbits, viewed from a point in space far above the Solar System (click on the tab marked 'Solar System' at the top of the applet; use the left-hand scroll bar to zoom out).

Finding Venus in Your Own Night Sky using Mini-AstroViewer®

Sun, Moon and planet colours as they appear in AstroViewer®. The program displays the Moon in its correct phase

To set your own location, click on the 'Location' button and click on your approximate position on the pop-up world map. If you know your precise latitude and longitude, you can refine your position by pressing the left/right and up/down arrows to move the cross-hair in 1° increments (to find your latitude and longitude, visit the Heavens Above website, select your country and enter the name of your nearest town or city using the 'Town Search' facility). Having plotted your geographical co-ordinates, click 'OK' and the night sky over your own location will appear in the window, valid for the current time, which is displayed in UT (Universal Time, equivalent to GMT). The applet will initialise displaying the current UT time according to your browser's clock and Time Zone settings (if you would prefer to have the Local Time displayed, use the fully-functional version of the program at

The red circle represents the horizon around you; the lower half of the display represents the part of the sky you are facing. The centre of the circle is the point directly above your head (known as the zenith). The ecliptic (the path along which the Sun, Moon and planets will be found) is marked by a red dashed line, passing as it does through the zodiac constellations. The blue dashed line marks the apparent position of the celestial equator, which arcs across the sky from the due East point on the horizon to the due West point. The program plots stars down to magnitude +5.0.

The bottom scroll bar rotates the horizon view, allowing for a view in any compass direction; the left-hand scroll bar zooms the sky in or out, and the right-hand scroll bar pans up (to the zenith) or down (to the horizon) whenever the view has been zoomed.

Mini-AstroViewer demonstration (click to visit AstroViewer website)

For a detailed animation showing how to use the

Mini-AstroViewer® program, click here.

Information on a celestial body can be viewed by clicking on the object (in the case of a planet, its magnitude, distance, elongation and apparent diameter). Note that if the elongation (its angular distance from the Sun as seen from the Earth) is less than about 15°, the planet will not normally be visible because it is too near the Sun. Remember that local twilight can affect the visibility of a particular planet, even at elongations greater than 15°, making observation difficult or even impossible. This particularly applies throughout the local summer months at higher latitudes.

To locate Venus, first see if it is above the horizon at the time you are requesting. If it is visible within the circle, move the bottom scroll bar left or right to rotate the image until the planet is positioned on the vertical red line (the altitude scale). Zoom in to the area using the left-hand scroll bar where necessary (see animation opposite).

The direction of Venus at the requested time will be indicated at the bottom (W, SW, etc). The altitude of the planet (its angle above the horizon) can be read off on the altitude scale (it is marked at 10° intervals). Hence if it is three notches up, its altitude is 30° at the displayed time (to understand how to determine a planet's altitude in the night sky, refer to the two diagrams below). If Venus' altitude is less than about 5° it may be difficult to see because of the dimming effect of the Earth's atmosphere and, in town and city locations, the effects of light pollution or skyglow.

If Venus is not shown within the circle, it is below the horizon and you will have to wait until the next evening (for evening apparitions) or the next morning (for morning apparitions) before you can see it (provided it is not too near the Sun).

For evening apparitions (i.e. when Venus is an 'Evening Star') adjust the time display to the approximate time of the next sunset at your location (alternatively, simply click the 'hours/minutes forward' buttons (Forward in time button) until the Sun is positioned just below the horizon). Venus will become visible soon after sunset, so you should note down the direction and altitude of the planet at this time. For morning apparitions (i.e. when Venus is a 'Morning Star') click the 'hours forward' button (Forward in time button) repeatedly until the planet is above the eastern horizon, then note down the direction and altitude of the planet at this particular time.

Diagram showing how altitude (or elevation) is determined for a celestial body in the night sky


Direction and Altitude diagram

Angular altitude (or elevation) is measured as 0º at the horizon (when an object is at the point of rising or setting), 45º when 'half way up the sky' and 90º when directly above the observer's head (at the zenith). In the above picture, the bright star has an altitude of about 60º (i.e. it is "60º high").

Using direction and altitude to find a star or planet in the night sky - in this case, the star/planet is in the South-east (SE) at an altitude of 20º.


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The Current Night Sky over Houston, Texas, USA  Flag of the USA

Requested location

Would you like to see your own town or city shown here?


Requested locations may appear on another planet page (see links below) depending upon the number of requests received by the author at any given time.

A list of the night sky locations currently displayed on this website can be seen on the main Naked-eye planets page.

The graphic shows the sky at the location indicated when this page was loaded in your browser; if several minutes have since passed, click the 'Refresh' button at the top of your browser (or press the F5 key) to see the current sky.

The Night Sky location displayed here is periodically changed by the website author.

Additional AstroViewer® Information

Mini-AstroViewer® is a lightweight version of AstroViewer®, an interactive night sky map that helps you find your way in the night sky quickly and easily. Due to its intuitive interface, it is well suited to beginners in astronomy.

The fully functional, free-to-use version can be accessed at the AstroViewer® website. It has additional features such as a Local Time display, a planet visibility chart for any selected location, a 3D Solar System map, the ability to store user-generated world locations, a 'Find Celestial Body' facility, printing and language options and greater flexibility in the night sky display (see details here).

A fully-functional version for offline use can be obtained upon the purchase of a license key, following the download and installation of a test version.

AstroViewer® is produced by Dirk Matussek.

Current night sky over Houston, TX

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Venus Conjunctions with other Planets: Morning Apparition, 2017

Viewed from the orbiting Earth, whenever two planets appear to pass each other in the night sky (a line-of-sight effect) the event is known as a planetary conjunction or an appulse. However, not all planetary conjunctions will be visible from the Earth because many of them take place too close to the Sun. Furthermore, not all of them will be seen from across the world; the observers' latitude will affect the altitude (angle above the horizon) at which the two planets are seen at the time of the event, and the local season will affect the sky brightness at that particular time. A flat, unobstructed horizon will normally be required to observe most of them.

Planetary conjunctions are generally considered most noteworthy when they involve two bright planets, and none are more spectacular than those involving Venus. During the course of one Earth year, Venus is seen to complete over 1½ circuits of the zodiac, and in doing so it passes each of the planets in the sky - a few of them on more than one occasion.

Sketch by Giovanni Isopi showing the telescopic view of a Venus-Jupiter conjunction in August 2014 (Image: Giovanni Isopi)

A Venus-Jupiter Conjunction sketched by Giovanni Isopi (Frosinone, Italy) as seen through an 8" SCT telescope at 80x magnification. The conjunction took place at dawn on August 18th 2014, the pair being separated by 0°.2. A similar conjunction between the two planets in November 2017 will see them positioned 0°.3 apart.

(Image: Giovanni Isopi)

Because Venus never appears more than 47° from the Sun, it follows that any planetary conjunction involving Venus will also never occur above this angular distance, i.e. its solar elongation will always be less than 47°. For an Earthbound observer, a superior planet (i.e. Mars and beyond) seen at such a small elongation poses something of a problem, since it will then be considerably more distant from the Earth (and therefore fainter) than when it is closest and brightest in the sky (namely, at opposition, when its elongation is 180° from the Sun).

Jupiter is affected to a much lesser extent since it is always above magnitude -1.6 (brighter than Sirius, the brightest star in the sky). Conjunctions between Venus and Jupiter are arguably the most spectacular to view, Venus always being the brighter of the two.

A significant factor in determining whether a morning conjunction is 'poor', 'good' or 'very good' is the altitude that the fainter planet   (in this case Jupiter) attains before it disappears from view in the brightening dawn twilight. The November 13th 2017 conjunction between Venus and Jupiter is a difficult one, taking place very late in the apparition when the pair are positioned just 14° from the Sun. Such a narrow elongation means that the event takes place in twilight, thus losing much of its visual spectacle. The Northern hemisphere is best placed to view it, though the pair's altitude when Jupiter disappears from view is less than 10°.

A close conjunction between Venus and Mars takes place on October 5th 2017. The small separation between the two planets (0°.2) allows them to be fitted within the field-of-view of a telescope eyepiece at low or medium power. Adding to the spectacle is the star Greek lower-case letter 'sigma' Leo (Sigma Leonis, mag. +4.0), which is positioned just 0°.3 to the NNE of Venus. The narrow solar elongation of the two planets (23° West) does however mean that the Red Planet is very distant and appears no brighter than magnitude +1.8, almost as faint as it can get. The two planets are positioned in Leo, placing them at a low but observable altitude from Northern hemisphere locations before Mars is enveloped in the dawn twilight. From latitude 60° North the pair reach an altitude of 12° in the East when the Red Planet disappears from view, whilst at mid-Northern latitudes they reach up to 15°. At latitudes South of the Northern Tropics the altitude at which Mars disappears progressively reduces, until the pair are not seen at all South of ca. 33° South.

Venus and Uranus are involved in a relatively wide conjunction on June 2nd 2017. Uranus is a tricky object to observe whenever it is involved in conjunctions with Venus because Uranus is only just visible to the naked-eye and Venus is, of course, the brightest of the naked-eye planets. Consequently the glare caused by Venus' brilliance (mag. -4.2) makes it difficult to see the much fainter Uranus (+5.9) beside it. Binocular observers in particular may find it easier to position Venus just outside the binocular field of view so that Uranus may be more comfortably seen.

Twilight quickly renders Uranus unobservable (even through binoculars), so any conjunctions taking place less than about 20° from the Sun will be difficult or impossible to see. Fortunately, the 2017 conjunction takes place only one day after Venus' greatest elongation date, hence it is about as far from the Sun as is theoretically possible. Despite this, however, only the Southern hemisphere is able to observe the conjunction with ease. Equatorial latitudes are best placed to observe it, the pair reaching an altitude of 32° in the East before the sky becomes too bright for Uranus to be seen. For much of the Northern hemisphere, the planets' location in Pisces means that the angle of the ecliptic to the Eastern horizon at dawn is shallow, so that the conjunction is not visible at all North of mid-Northern latitudes.

The three planetary conjunctions with Venus which are viewable during the 2017 morning apparition are summarised in the table below.

Table showing the visible Venus conjunctions with other planets during the morning apparition of 2017 (Copyright Martin J Powell, 2017)

Venus conjunctions with other planets during the 2017 morning apparition The column headed 'UT' is the Universal Time (equivalent to GMT) of the conjunction (in hrs : mins). The separation (column 'Sep') is the angular distance between the two planets, measured relative to Venus, e.g. on 2017 Nov 13, Jupiter is positioned 0°.3 South of Venus at the time shown. The 'Fav. Hem' column shows the Hemisphere in which the conjunction is best observed (Northern, Southern and/or Equatorial). The expression 'Not high N/S lats' indicates that observers at latitudes further North than about 45°N (or further South than about 45°S) will most likely find the conjunction difficult or impossible to observe because of low altitude and/or bright twilight.

In the 'When Visible' column, a distinction is made between Dawn/Morning visibility and Dusk/Evening visibility; the terms Dawn/Dusk refer specifically to the twilight period before sunrise/after sunset, whilst the terms Evening/Morning refer to the period after darkness falls/before twilight begins (some conjunctions take place in darkness, others do not, depending upon latitude). The 'Con' column shows the constellation in which the planets are positioned at the time of the conjunction.

To find the direction in which the conjunctions are seen on any of the dates in the table, note down the constellation in which the planets are located ('Con' column) on the required date and find the constellation's rising direction (for Dawn/Morning apparitions) or setting direction (for Dusk/Evening apparitions) for your particular latitude in the Rise-Set direction table.

The table is extracted from two other tables showing Venus conjunctions with other planets from 2010 to 2020 on the Venus Conjunctions page.

Although any given conjunction takes place at a particular instant in time, it is worth pointing out that, because of the planets' relatively slow daily motions, such events are interesting to observe for several days both before and after the actual conjunction date.

There are in fact two methods of defining a planetary conjunction date: one is measured in Right Ascension (i.e. perpendicular to the celestial equator) and the other is measured along the ecliptic, which is inclined at 23½° to the Earth's equatorial plane (this is due to the tilt of the Earth's axis in space). An animation showing how conjunction dates are determined by each method can be found on the Jupiter-Uranus 2010-11 triple conjunction page. Although conjunction dates measured along the ecliptic are technically more accurate (separations between planets can be significantly closer) the Right Ascension method is the more commonly used, and it is the one which is adopted here.

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Moon near Venus Dates, April to October 2017

The Moon is easy to find, and on one or two days in each month, it passes Venus in the sky. Use the following table to see on which dates the Moon passes near the planet between April and October 2017:

Date Range


Conjunction (Geocentric)

Solar Elong.

Moon Phase

Date & Time

Sep. & Dir.


Apr 23/24

Apr 23, 17:58 UT

.2 N


Waning Crescent


May 22/23

May 22, 12:30 UT

.4 N


Jun 20/21

Jun 20, 21:11 UT

.4 N


Jul 19/20

Jul 20, 11:11 UT

.7 N


Aug 18/19

Aug 19, 04:43 UT

.2 N


Sep 17/18*

Sep 18, 00:55 UT

.5 N


Oct 17/18

Oct 18, 00:20 UT

.9 S


* A lunar occultation takes place, visible in darkness/twilight from the Eastern Indian Ocean and in daylight from Australia, New Zealand, Indonesia and Papua New Guinea. See The National Astronomical Observatory of Japan website for visibility track and timings.

Moon near Venus dates for the morning apparition of 2017. The Date Range shows the range of dates worldwide (allowing for Time Zone differences across East and West hemispheres). Note that the dates, times and separations at conjunction (i.e. when the two bodies were at the same Right Ascension) are measured from the Earth's centre (geocentric) and not from the Earth's surface (times are Universal Time [UT], equivalent to GMT). The Sep. & Dir. column gives the angular distance (separation) and direction of the planet relative to the Moon, e.g. on July 20th 2017 at 11:11 UT, Venus is positioned 2°.7 North of the Moon's centre.


A waning crescent Moon and Venus photographed on the morning of June 24th, 2014 (Photo: Copyright Martin J Powell, 2014)




The Waning Crescent Moon and Venus in the Eastern sky at dawn at the Northern hemisphere's midsummer in June 2014.

Because Venus never appears more than 47° from the Sun, the Moon always shows a crescent phase whenever it passes the planet in the sky: a waxing crescent during evening apparitions and a waning crescent during morning apparitions.

The Moon moves relatively quickly against the background stars (in an Eastward direction, at about its own angular width [0º.5] each hour, or about 12º.2 per day) and because it is relatively close to the Earth, an effect called parallax causes it to appear in a slightly different position (against the background stars) when seen from any two locations on the globe at any given instant; the further apart the locations, the greater the Moon's apparent displacement against the background stars. Therefore, for any given date and time listed in the table, the Moon will appear closer to Venus when seen from some locations than others. For this reason, the dates shown in the table should be used only for general guidance.

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Naked-eye Venus: Apparitions, Conjunctions and Elongations, 2010-2020

The Naked-eye appearance of Venus

Naked Eye Planet Index

Planetary Movements through the Zodiac










Copyright © Martin J Powell  March 2017

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