Table of Contents

2018: Venus in November Morning Sky

Venus approaches Spica during November 2018

Morning Star Venus approaches Spica in the morning sky during November 2018. Early in the month, look for Venus and Spica with a binocular. Each morning the pair appears higher, with Venus closer to Spica. Venus passes closest on the morning of November 14 and almost as high on November 20. Watch Venus approach Spica, then separate.


Brilliant Morning Star Venus zooms into the morning sky during early November, after its inferior conjunction – between Earth and the sun – in late October.

On November 1, at 20 minutes before sunrise, brilliant Venus is low in the east-southeast.  A binocular helps you locate the planet.  The star Spica is noticeably above the gleaming planet.

Each morning, Venus and Spica rise earlier and each morning during the first half of the month, Venus gets closer to Spica. The pair appears higher in the sky and farther southeast each morning.

Spica and other stars seem to make a seemingly unchanging background for the motions of the planets that results from their solar orbits combined with the rotation and revolution of our planet Earth.

By November 5, about 30 minutes before sunrise, the moon is (10°) above Venus.  The next morning, the thinning crescent moon is (9°) to the left of the brilliant Morning Star.

On November 9, Venus rises at the beginning of morning twilight.  As the sky brightens, Venus appears higher in the sky.  On this morning, Venus appears nearly 3 times closer than at the beginning of the month.  The gap continues to close each day.

By November 14, Venus appears about 2 full moon diameters to the lower left of the star.  In space Venus is about 30 million miles away.  Spica is nearly 260 light years away, where 1 light year is nearly 6 trillion miles.  Clearly, they are not actually close in space, but appear in the same direction, much like seeing your neighbor’s house in front of the rising sun.  In space, though, we don’t have the depth perception as we have with terrestrial subjects.

Venus does not pass the star, in an event known as a quasi-conjunction.  This occurs when a planet approaches near a star or another planet, but it does not pass it.  Afterward, Venus moves away from Spica.

Venus continues to climb into the sky compared to Spica, but the planet appears to be separating from the star.  The pair is nearly at the same height on the morning of November 20.

Astronomers use angles to measure the apparent sizes of celestial objects and the separations between them in the sky.  The full moon’s apparent size is 0.5°.  Your index finger, at arm’s length, covers about 1°.  Your fist covers about 10° What follows are the angular separations of Venus and Spica during the month.







1 6.2° 11 1.6° 21 2.4°
2 5.5° 12 1.5° 22 2.7°
3 5.0° 13 1.3° 23 3.0°
4 4.4° 14 1.2° 24 3.3°
5 4.1° 15 1.2° 25 3.7°
6 3.6° 16 1.3° 26 4.1°
7 3.2 17 1.5° 27 4.5°
8 2.8 18 1.6° 28 4.8°
9 2.3 19 1.8° 29 5.3°
10 2.1 20 2.1° 30 5.8°




2018, October 26: Venus at Inferior Conjunction

The thin crescent of Venus as viewed
through a small telescope appears at the
upper left of the planet.  The crescent
is about 1% illuminated.

Important: Never look directly at the sun.  A Binocular or a small telescope might be needed to initially locate Venus. Do not to point any optical instrument at the sun. The light collecting properties of the binocular or a telescope can damage the device or cause irreparable damage to eyes if you are looking through them. With optical help from a telescope, Venus displays a very thin crescent.

At conjunction on October 26, 2018, Venus is 6.5° south of the sun.  In a clear sky, it could be visible to the unaided eye.  Stand under an overhang that blocks the sun to see it.  Carefully observe Venus through a telescope, because of its proximity to the sun, as noted above.  Venus displays a very thin crescent that is less than 1% illuminated.  The planet is 0.27 Astronomical Units away from Earth and displays a whopping 61” angular size, although this is about 3% of the moon’s apparent diameter.

After conjunction, Venus seemingly leaps into the morning sky. It appears to be chasing Spica. In just two weeks after moving between the earth and sun, this brilliant planet rises at the beginning of twilight.  The Spica chase continues until mid-November, as Venus approaches its greatest brightness.  Venus does not reach Spica, but passes within 1.2° during mid-November, a quasi-conjunction.  See the full article about the appearance of Venus here.

Venus in the Morning Sky, 2018-2019

Figure 1:  Venus shines in the morning sky with a crescent moon on September 17, 2017

Bookmark this page to return to it follow the progress of Venus in the morning sky,

For readers wanting a detailed and more technical description of the appearance, click here.

Venus returns to the morning sky in late 2018 and shines from the eastern sky until the middle of summer 2019.  The photo above (Figure 1) shows Venus on September 17, 2017, during the last morning appearance.  During  this appearance Venus has conjunctions with Jupiter and Saturn, and a close approach to Mercury.  Venus rises very rapidly in the morning sky after its inferior conjunction on October 26, 2018.  It seems to be chasing Spica into the sky.  By mid-December, Venus rises nearly four hours before sunrise, then begins to slide back toward the sun, taking nearly eight months to reach superior conjunction.

Figure 2:  Venus at Inferior Conjunction: October 26, 2018

The morning appearance begins on October 26, 2018, when Venus moves between the earth and sun (inferior conjunction) (Figure 2). It is typically not visible at these times, but Venus is not lined up with the earth and sun. It passes below imaginary line between the earth and sun. Venus might be visible in the clear sky. Around noon, stand under an overhang that blocks the sun. Binoculars or a small telescope might be needed to initially locate it. It is very important not to point any optical instrument at the sun. The light collecting properties of the binoculars or a telescope can damage the device or cause irreparable damage to eyes if you are looking through them. With optical help from a telescope, Venus displays a very thin crescent.

Figure 3:  The rising times of stars and planets compared to sunrise.  The rising of Venus compared to sunrise
is displayed on the green line.  The moon’s rising is shown by the circles.

Venus then quickly moves into the morning sky the chart above (Figure 3) shows the rising time interval of Venus compared to sunrise; the rising time intervals for stars and other planets are shown as well. The circles show the rising time intervals for the moon.  The setting times for Jupiter and Saturn are included.  This occurs in the western sky.  When these planets set at sunrise, they are at opposition.

When the rising line of Venus crosses the rising line of another star or planet they rise at the same time. They are closest within a day or so of this intersection. When a moon circle appears near the rising line, the moon appears near Venus within a day or so.

The three phases of twilight: Civil Twilight, when the sun is 6° below the horizon; Nautical Twilight, sun is 12° below the horizon; and Astronomical Twilight, sun is 18° below the horizon at this time; the sky is as dark as it gets naturally.

This chart was composed from data by the US naval observatory for Chicago, Illinois.

Note that Venus appears seemingly suddenly in the morning sky. It appears to be chasing the star Spica. After Venus reaches its greatest brilliance and greatest elongation, it begins a slow fade into the sun’s glare. On the way it passes Jupiter, and Antares, and Saturn, along with other sign posts.

Venus and Spica, November 2018

Venus seems to be chasing Spica into the sky.  These charts show the pair about 30 minutes before sunrise.

Figure 4:  November 4, 2018, Venus is
4.4° below Spica.

  • November 4 (Figure 4): Only nine days after its conjunction, Venus rises an hour before sunrise this morning it is 4.4° below Spica with the waning crescent moon nearly 27° above Spica; notice the contrast of brightness. Venus is about 100 times brighter than Spica.

Figure 5:  Venus is closing the gap on Spica.

  • November 6 (Figure 5): Brilliant Venus is 3.6° below Spica with the waning crescent moon 9° to the left of the planet. Watch Venus close the gap on Spica during the next week.
  • November 9: Venus rises at the beginning of twilight, about 100 minutes before sunrise. After today, Venus rises before the beginning of twilight until March 14, 2019.

Figure 6: Venus closes about one degree of Spica in mid-November. There is no conjunction but this is the closest approach — a quasi conjunction

  • November 14: (Figure 6): The Spica chase ends when brilliant Venus closes to 1.2° of the star.  Venus does not pass Spica.  Because the separation is less than 5°, this is known as a “quasi-conjunction.”

Venus at Greatest Brightness

Figure 7:  This chart shows the location of Venus
during its 11-day stage of greatest brightness.

  • November 24: Now rising over 3 hours before the sun, brilliant Venus starts its stage of greatest brightness (Figure 7). For the next 11 days it displays its greatest visual intensity. It is important to note that this is not a singular event, but the duration of this greatest brightness occurs across several mornings.  More formally, Venus is near its greatest illuminated extent, defined as a geometrical configuration when Venus has an elongation of 40° – midway between inferior conjunction and greatest elongation.  This occurs December 1, when Venus’ illuminated portion covers more area of the sky than any other time during its apparition. (For a more technical explanation of greatest illuminated extent, see  For our description, greatest brilliancy occurs during a 11-day period when Venus displays its greatest visual brightness.  Its brightness measured with light-sensitive equipment may slightly change, but our eyes cannot perceive that minute difference. 

Figure 8:  Look for Venus and Sirius about 2 hours before sunrise in late November.

  • November 29: As Venus is in the middle of its stage of greatest brightness, notice that it is about the same altitude (16°) as brightest star Sirius in the southwest, at about 100 minutes before sunrise. While it is not appropriate in formal astronomy to visually compare respective brightness of objects that are widely separated (101° in this case), notice that Venus is distinctly brighter (about 25 times) than Sirius – the brightest planet compared to the brightest star. Venus is now 5.3° to the lower left of Spica, about two weeks after their quasi-conjunction (Figure 8).

A Morning Planet Dance


Figure 9:  The morning planet dance of Venus, Jupiter, and Mercury in late December 2018.

  • December 19:  Today is the greatest time interval between Venus rising and sunrise. While the Venus rising time is still 3:23 a.m. CST (in Chicago), sunrise changed 4 minutes earlier during the past week.  The gap between sunrise and Venus rising now decreases, on average, about 1 minute each morning until Venus rises at Astronomical Twilight less than three months from this morning. Brilliant Venus is 28° up in the southeast, 4.3° above Zubenelgenubi (α Lib).  Bright Jupiter is 27° to the lower left of Venus.  Jupiter is 0.8° to upper right of Omega Ophiuchi (ω Oph) and 5.3° to the upper left of Antares, although the star is only 3° in altitude.  Use binoculars to find it.  Mercury is 2.5° to the upper right of Jupiter and 1° to the upper right of Psi Ophiuchi (ψ Oph). (See Figure 9)
  • December 20: This morning Jupiter is 1.6° below Mercury and 0.6° to the upper right of Omega Ophiuchi. Mercury is 0.6° to the lower left of Psi Ophiuchi.
  • December 21: Mercury, Jupiter and Antares are nearly in a line, spanning 6.1°; the Jupiter-to-Antares gap is 5.2°.  Jupiter is 0.9° to the lower right of Mercury, their closest separation, and 0.4° to the upper left of Omega Ophiuchi.
  • December 22: Jupiter is 1.2° to the right of Mercury (m = −0.4) and 0.2° to the upper left of Omega Ophiuchi.
  • December 23: Jupiter is 2° to the upper right of Mercury, which has an altitude of 5°.  The giant planet is 0.22° to the upper left of Omega Ophiuchi.  It passes 5.2° to the upper left of Antares and Mercury passes 6.1° to the upper left of the star.  Venus is nearly 25° to the upper right of Jupiter and 2.9° to the upper left of Zubenelgenubi.

Venus at Morning Greatest Elongation

Figure 10:  Venus at greatest elongation,
January 5, 2009

  • January 5, 2019: Venus reaches its greatest elongation from the sun (47.0°) (Figure 10). It is 13.6° above Antares. Jupiter is 14.2° to the lower left of Venus and 5.9° from Antares.  Venus and Spica are 35.3° apart. Through a telescope, Venus is nearly the same angular diameter as Mars when it was at its closest last summer (July 31).  Venus appears at its morning half phase.

Venus-Jupiter:  A Widely-Spaced Conjunction

Figure 11:  Venus, Jupiter, and Antares,
January 17, 2019.  Venus
approaches Jupiter

  • January 17: At 6:15 a.m. CST (60 minutes before sunrise), brilliant Venus is 20° up in the southeast (Figure 11). Venus passes 7.8° to the upper left of Antares.  Bright Jupiter is 5.1° to the lower left of Venus and 7.2° from Antares.  Venus is now two times farther from Earth than when we marked its greatest brilliancy, 49 days ago.  Through a telescope, Venus’ terminator is slightly, but distinctly, convex — indicating a morning gibbous phase.

Figure 12: A widely-spaced Venus-Jupiter conjunction.

  • January 22: Venus passes to the upper left of Jupiter this morning in a widely-spaced conjunction (2.4°) (Figure 12). Venus is 22° up in the southeast at 6:30 a.m. CST (40 minutes before sunrise). Venus passes Jupiter (1.1°) again on November 24, 2019, when they appear in the western evening sky on Venus’ next evening apparition. Venus and Jupiter resume their close (epoch) conjunctions with a difficult-to-see grouping on February 11, 2021 (0.4°). An easier-viewed epoch conjunction occurs on April 30, 2022 (0.5°).  Both of these close conjunctions occur in the morning sky.

Venus continues to move eastward against the starry background, away from Jupiter and toward Saturn.

Venus-Saturn Conjunction

Figure 13:  A Venus-Saturn conjunction,
February 18, 2019

  • February 18: At 6 a.m. CST (about 40 minutes before sunrise), Saturn is 13° up in the southeast. This morning is the Venus-Saturn conjunction (Figure 13).  Venus is 1.1° to the upper left of Saturn.  As with Jupiter (described on January 22), Venus has another conjunction with Saturn in the evening sky later this year.  On December 10, 2019, they appear 1.8° apart.  This is followed by a very close conjunction (0.4°) on February 6, 2021 in the morning sky close to sunrise.

Heading Into Twilight & A Close Approach to Mercury

  • March 14: Venus rises at Astronomical Twilight (93 minutes before sunrise) and for the rest of this apparition rises earlier during the phases of twilight. Through a telescope, Venus is growing in its morning gibbous phase. This morning, Jupiter is 90° west of the sun.  It is 52° to the upper right of Venus.  Saturn is 20.8° to Venus’ upper right.

Figure 14: A Venus-Mercury quasi-conjunction,
April 16, 2019

  • April 16: Venus and Mercury have a quasi-conjunction (4.3°) (Figure 14). (See the definition in the November 14 note.)  Mercury has a wide greatest elongation (27.7°), but the ecliptic is at a low angle for viewing. Even with its earliest rising on April 3, Mercury rose 8 minutes before Nautical Twilight, about 65 minutes before sunrise.  You’ll need binoculars to see it in the east-northeast sky.  This morning, Mercury rises 15 minutes after Nautical Twilight.

Figure 15:  A Venus-Mercury-Moon grouping,
May 2, 2019

  • May 2: The waning crescent moon (27.1 d) is 4.3° to the lower right of Venus. Mercury is 8.5° to the lower left of Venus, just above the horizon (Figure 15).  The time interval between Astronomical Twilight and sunrise grows 24 minutes from this morning through mid-June.  While Venus is rising at the same time interval before sunrise for the next month, it appears in a brighter sky.  Note this on the rising chart (Figure 3).

A Bright Twilight Conjunction With Aldebaran

Figure 16:  Venus-Aldebaran,
June 17, 2019

  • June 17: Now rising less than hour before sunrise, Venus passes 4.7° to the upper left of Aldebaran (Figure 16). This will test your observing skills with a telescope. Venus is in a slow slide into the sun’s glare, rising, on average, about 1.7 minutes later each day.

Heading Toward Conjunction


Figure 17:  Venus and the moon, July 1, 2019

  • July 1: At 4:55 a.m. CDT (35 minutes before sunrise), a very thin crescent moon (28.0 d) stands 6.3° to the right of Venus (Figure 17). The planet is 3.6° off the east-northeast horizon, another challenge for your observing location and your observing skills.

July 21: Clearly rising in bright twilight, Venus rises farthest north, azimuth equals 57°, the same position the sun rose at the summer solstice. Tomorrow, Venus rises at Civil Twilight (sun’s altitude is −6°), about 30 minutes before sunrise.Figure 18:  Venus at Superior Conjunction,
August 14, 2019

  • August 14: Venus is at superior conjunction, 1:07 a.m. CDT (Figure 17).  This appearance of Venus ends.


Appearances with Moon

  • November 6, 2018 (8.9°)
  • December 3, 2018 (5.6°)
  • January 1, 2019 (5.4°)
  • January 31, 2019 (2°)
  • March 2, 2019 (4.3°)
  • April 1, 2019 (8.7°)
  • May 2, 2019 (4.3°)
  • June 1, 2019 (6°)
  • July 1, 2019 (6.3°)

2018, September 18: Start Looking for Vesta

  • September 18: With binoculars begin looking for Vesta (4 Vesta, m = 6.4), moving eastward among the stars of Sagittarius.  In a week it passes south of Saturn. Tonight, the minor planet is 1.3° to the lower right of 9 Sagittarii (9 Sag, m = 5.9), a star in the central area of the Lagoon Nebula (M8, NGC 6523).

2018: September 16-30: Venus at Greatest Brightness

September 12, 2018: Venus, Jupiter and the crescent Moon.

  • September 16: The moon reaches its First Quarter phase, 6:15 p.m. CDT.  Venus (m = −4.8) begins its period of greatest brightness, a two-week interval where it displays its greatest visual brightness.  On September 21, Venus is at its greatest illuminated extent. Many of us know this time as “greatest brilliancy.”  The two events are about a half-day apart. The instance of greatest brilliance is nearly impossible to see; rather, I note the time period when the planet displays its greatest visual brightness.  The hundredths of a magnitude that distinguish greatest brilliancy are imperceptible to our eyes.  Venus has an elongation of 40° ‒ midway between greatest elongation and inferior conjunction.  Through a telescope it has an evening crescent phase with a 25% illumination and a 40” apparent size. With these factors Venus presents to us an illuminated phase that covers more area of the sky than any other time during its apparition and it is at its brightest. (For a more technical explanation of greatest illuminated extent, see

2018, September 12: Venus, Jupiter, and Moon

The sky is very clear this evening. The crescent moon, overexposed in the image, shows Earthshine. Sunlight reflected from Earth falls on the night portion of the moon and gently illuminates it.  Brilliant Venus is just above the southwest horizon.  In about 10 days, Venus begins its cycle of greatest brightness. Jupiter appears over 17 degrees to the upper left of Venus.  Jupiter gets closer to Venus during the month, but there is no conjunction.

2018: September 8: Mercury, Regulus and the Moon #astronomy #moon

September 8: Before sunrise, locate the thin waning crescent moon (28.0 d, 2%) 1.8° to the upper left of Regulus with Mercury 4.4° below the star. Mercury (m = −1.2) is only 4.5° up in the east-northeast 30 minutes before sunrise. You’ll need a clear horizon and binoculars to see the trio in bright twilight.