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Venus at greatest elongation east

Dominic Ford, Editor
From the Inner Planets feed

Objects: Venus
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Venus will reach its greatest separation from the Sun in its 2018 evening apparition. It will be shining brightly at mag -4.3.

From Seattle , this apparition will not be one of the most prominent, reaching a peak altitude of 25° above the horizon at sunset on 27 May 2018.

Begin typing the name of a town near to you, and then select the town from the list of options which appear below.

The table below lists how high above the horizon Venus will appear at sunset over the course of the apparition. All times are given in Seattle local time.

Date Sun
sets at
sets at
at sunset
at sunset
16 Feb 201817:3118:15south-west
26 Feb 201817:4718:44west
08 Mar 201818:0219:1311°west
18 Mar 201819:1820:4414°west
28 Mar 201819:3221:1316°west
07 Apr 201819:4621:4219°west
17 Apr 201820:0022:1120°west
27 Apr 201820:1422:3922°west
07 May 201820:2823:0523°west
17 May 201820:4123:2524°west
27 May 201820:5223:3825°west
06 Jun 201821:0223:4324°west
16 Jun 201821:0723:3923°west
26 Jun 201821:1023:3022°west
06 Jul 201821:0723:1520°west
16 Jul 201821:0122:5619°west
26 Jul 201820:5022:3517°west
05 Aug 201820:3722:1115°west

A graph of the angular separation of Venus from the Sun around the time of greatest elongation is available here.

Observing Venus

The 2018 evening apparition of Venus
17 May 2018 – Venus reaches highest point in evening sky
14 Aug 2018 – Venus at dichotomy
17 Aug 2018 – Venus at greatest elongation east
24 Sep 2018 – Venus at greatest brightness

Venus's orbit lies closer to the Sun than the Earth's, meaning it always appears close to the Sun and is lost in the Sun's glare much of the time.

It is observable for a few months each time it reaches greatest separation from the Sun – moments referred to as greatest elongation.

On these occasions, Venus is so bright and conspicuous that it becomes the third brightest object in the sky after the Sun and Moon. It is often called the morning star or the evening star.

These apparitions repeat roughly once every 1.6 years, taking place alternately in the morning and evening skies, depending whether Venus lies to the east of the Sun or to the west.

When it lies to the east, it rises and sets a short time after the Sun and is visible in early evening twilight. When it lies to the west of the Sun, it rises and sets a short time before the Sun and is visible shortly before sunrise.

At each apparition, Venus reaches a maximum separation from the Sun of around 48°. However, some times of the year are more favourable for viewing Venus than others. From Seattle, it reaches a peak altitude of between 15° and 43° above the horizon at sunset during each evening apparition, depending on the time of year. During its 2018 apparition, it will peak at 25° above the horizon at sunset on 27 May 2018.

This variability over the course of the year is due to the inclination of the ecliptic to the horizon.

The inclination of the ecliptic to the horizon

The inclination of the ecliptic to the horizon changes over the course of the year, affecting how high planets close to the Sun appear in the sky.

At all times, Venus lies close to a line across the sky called the ecliptic, which is shown in yellow in the planetarium above. This line traces the path that the Sun takes through the zodiacal constellations every year, and shows the plane of the Earth's orbit around the Sun. Since all the planets circle the Sun in almost exactly the same plane, it also closely follows the planes of the orbits of the other planets, too.

When Venus is widely separated from the Sun, it is separated from it along the line of the ecliptic. But, at different times of year, the ecliptic meets the horizon at different angles at sunset. This would translate into Venus being at different altitudes above the horizon, even if its separation from the Sun was constant.

If the ecliptic meets the horizon at a shallow angle, then Venus has to be very widely separated from the Sun to appear much above the horizon. Conversely, if the ecliptic is almost perpendicular to the horizon, Venus may appear much higher in the sky, even if it is actually much closer to the Sun.

The seasonal dependence of this is that at sunset, the ecliptic makes its steepest angle to the horizon at the spring equinox – in March in the northern hemisphere, and in September in the southern hemisphere. Conversely, it meets the horizon at its shallowest angle at the autumn equinox. Because the seasons are opposite in the northern and southern hemispheres, a good apparition of Venus in one hemisphere will usually be badly placed in the other.

At sunrise, these dates are also inverted, so that for morning apparitions of Venus, the ecliptic makes its steepest angle to the horizon at the autumn equinox, and its shallowest angle to the horizon at the spring equinox.

The optimum time for an apparition of Venus

The maximum altitude of Venus during all its evening apparitions between 2000 and 2050, as a function of the day of the year on which greatest western elongation occurs. Different colours show the altitudes observed from different latitudes. Click to expand.

For this reason, the day when Venus reaches its widest separation from the Sun (greatest elongation) is not necessarily the same day when it appears highest in the sky at sunset. Venus typically appears highest in the sky a few days or weeks closer to the spring equinox than the moment of greatest elongation.

The inclination of the ecliptic plane to the horizon at Seattle varies between 65° (sunset at the spring equinox) and 18° (sunset at the autumn equinox). On August 17, the ecliptic is inclined at 21° to the western sunset horizon, as shown by the yellow line in the planetarium above, meaning that this apparition of Venus will not be one of the most prominent, reaching a peak altitude of 25° above the horizon at sunset.

Venus's position

The position of Venus when it reaches greatest elongation will be:

Object Right Ascension Declination Constellation Magnitude Angular Size
Venus 12h34m30s -05°21' Virgo -4.3 24.3"
Sun 09h45m +13°28' Leo -26.7 31'35"

The coordinates above are given in J2000.0.

The sky on 17 August 2018
Twilight ends
Twilight begins

6-day old moon
Waxing Crescent


6 days old

Rise Culm. Set
Mercury 05:09 12:17 19:26
Venus 10:23 16:02 21:40
Moon 13:43 18:48 23:52
Mars 19:42 23:34 03:30
Jupiter 13:24 18:17 23:09
Saturn 17:20 21:35 01:55
All times shown in PDT.


The circumstances of this event were computed using the DE405 planetary ephemeris published by the Jet Propulsion Laboratory (JPL).

This event was automatically generated by searching the ephemeris for planetary alignments which are of interest to amateur astronomers, and the text above was generated based on an estimate of your location.

Related news

17 Aug 2018  –  Venus at greatest elongation east
05 Sep 2018  –  Venus at aphelion
24 Sep 2018  –  Venus at greatest brightness
26 Oct 2018  –  Venus at inferior solar conjunction

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Color scheme