Dominic Ford, Editor
From the Inner Planets feed
Venus will be well placed for observation in the evening sky, shining brightly at mag -4.4.
From Seattle, it will become visible at around 19:42 (PST) as the dusk sky fades, 39° above your western horizon. It will then sink towards the horizon, setting 4 hours and 23 minutes after the Sun at 23:45.
Venus's orbit lies closer to the Sun than the Earth's, meaning that it always appears close to the Sun and is very difficult to observe most of the time.
It is observable only for a few weeks each time it reaches greatest separation from the Sun – moments referred to as greatest elongation.
On these occasions, however, 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 or evening star.
These apparitions take 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.
On this occasion, it lies 46° to the Sun's east.
Venus in coming weeks
The key moments in this apparition of Venus are as follows:
|24 Mar 2020 00:31 PDT||– Venus at greatest elongation east|
|26 Mar 2020 17:47 PDT||– Venus at dichotomy|
|28 Apr 2020 07:25 PDT||– Venus at greatest brightness|
|03 Jun 2020 10:38 PDT||– Venus at inferior solar conjunction|
After greatest elongation, the distance between Venus and the Sun will decrease each night as it sinks back into the Sun's glare. The table below lists how long Venus will remain up after sunset each night; all times are given in Seattle local time.
|Altitude of Venus
|Direction of Venus
|17 Mar 2020||19:12||23:34||41°||west|
|24 Mar 2020||19:22||23:48||42°||west|
|31 Mar 2020||19:32||00:01||41°||west|
|07 Apr 2020||19:42||00:09||41°||west|
|14 Apr 2020||19:52||00:16||40°||west|
|21 Apr 2020||20:02||00:17||38°||west|
|28 Apr 2020||20:12||00:11||35°||west|
|05 May 2020||20:21||23:55||31°||west|
|12 May 2020||20:31||23:30||25°||west|
|19 May 2020||20:39||22:53||18°||west|
|26 May 2020||20:47||22:04||10°||north-west|
A graph of the angular separation of Venus from the Sun around the time of greatest elongation is available here.
The position of Venus when it reaches greatest elongation will be:
|Object||Right Ascension||Declination||Constellation||Magnitude||Angular Size|
The coordinates above are given in J2000.0.
At each apparition, Venus reaches a similar separation from the Sun – around 48°. This distance is set by the geometry of how big Venus's orbit is, and how far away it is from the Earth.
Nonetheless, some times of the year are more favourable for viewing Venus than others.
It appears most favourably in the evening sky around the time of the local spring equinox, and most favourably in the morning sky around the local autumn equinox.
These dates are reversed in the northern and southern hemispheres, such that a good apparition in one hemisphere will not be easily observable from the other.
This is comes about because Venus always lies close to the line of the ecliptic, shown in yellow in the planetarium above. This is the line through the zodiacal constellations that the Sun follows through the year, and marks the flat plane in space in which all of the planets circle the Sun.
When Venus remains in the sky for a few hours after the Sun has set, its altitude above the horizon depends on two factors.
One is its angular separation from the Sun. But equally important is how steeply the line of the ecliptic is inclined to the horizon.
If Venus is widely separated from the Sun along the ecliptic, this may not translate into a high altitude if the ecliptic meets the horizon at a very shallow angle, running almost parallel to it.
Conversely, if the ecliptic is almost perpendicular to the horizon, a much smaller separation from the Sun may place Venus higher in the sky.
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 March 24, the ecliptic is inclined at 65° to the western sunset horizon, as shown by the yellow line in the planetarium view above, meaning that on this occasion Venus is very favourably placed for viewing from Seattle.
|The sky on 24 March 2020|
30 days old
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.
|24 Mar 2020, 00:31 PDT||– Venus at greatest elongation east|
|13 Aug 2020, 06:03 PDT||– Venus at greatest elongation west|
|29 Oct 2021, 07:44 PDT||– Venus at greatest elongation east|
|20 Mar 2022, 14:22 PDT||– Venus at greatest elongation west|
© NASA/Ricardo Nunes