Venus will reach half phase in its 2297 morning apparition. It will be shining brightly at mag -4.4.
From South El Monte , this apparition will not be one of the most prominent but prominent, reaching a peak altitude of 28° above the horizon at sunrise on 11 Feb 2297.
2297 morning apparition of Venus
| 31 Dec 2296 | – | Venus at inferior solar conjunction |
| 01 Feb 2297 | – | Venus at greatest brightness |
| 10 Feb 2297 | – | Venus at highest altitude in morning sky |
| 12 Mar 2297 | – | Venus at greatest elongation west |
| 12 Mar 2297 | – | Venus at dichotomy |
| 15 Oct 2297 | – | Venus at superior solar conjunction |
A graph of the phase of Venus is available here.
Apparitions of Venus
| 17 Mar 2295 | – | Evening apparition |
| 06 Aug 2295 | – | Morning apparition |
| 21 Oct 2296 | – | Evening apparition |
| 12 Mar 2297 | – | Morning apparition |
| 27 May 2298 | – | Evening apparition |
| 16 Oct 2298 | – | Morning apparition |
| 03 Jan 2300 | – | Evening apparition |
Observing Venus
Venus's orbit lies closer to the Sun than the Earth's, meaning that 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. These apparitions repeat roughly once every 1.6 years.
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.
Venus's phase
Venus's phase varies depending on its position relative to the Earth. When it passes between the Earth and Sun, for example, the side that is turned towards the Earth is entirely unilluminated, like a new moon.
Conversely, when it lies opposite to the Earth in its orbit, passing almost behind the Sun, it appears fully illuminated, like a full moon. However, at this time it is also at its most distant from the Earth, so it is actually fainter than at other times.
Venus shows an intermediate half phase – called dichotomy – at roughly the same moment that it appears furthest from the Sun, at greatest elongation. The exact times of the two events may differ by a few days, only because Venus's orbit is not quite perfectly aligned with the ecliptic.
Venus's position
The coordinates of Venus when it reaches dichotomy will be:
| Object | Right Ascension | Declination | Constellation | Angular Size |
| Venus | 20h15m20s | 17°14'S | Capricornus | 24.5" |
| Sun | 23h18m | 4°24'S | Aquarius | 32'13" |
The coordinates above are given in J2000.0.
The sky on 28 May 2025
| The sky on 28 May 2025 | ||||||||||||||||||||||||||||||||||
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7% 1 day old |
All times shown in PDT.
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Source
The circumstances of this event were computed using the DE430 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
| 12 Mar 2297 | – Venus at greatest elongation west |
| 10 May 2298 | – Venus at highest altitude in evening sky |
| 27 May 2298 | – Venus at greatest elongation east |
| 16 Oct 2298 | – Venus at highest altitude in morning sky |
Image credit
© NASA/Ricardo Nunes