Venus will reach half phase in its 1952–1953 evening apparition. It will be shining brightly at mag -4.4.
From Cambridge , this apparition will be well placed and prominent, reaching a peak altitude of 41° above the horizon at sunset on 16 Feb 1953.
1952–1953 evening apparition of Venus
| 24 Jun 1952 | – | Venus at superior solar conjunction |
| 31 Jan 1953 | – | Venus at greatest elongation east |
| 02 Feb 1953 | – | Venus at dichotomy |
| 16 Feb 1953 | – | Venus at highest altitude in evening sky |
| 08 Mar 1953 | – | Venus at greatest brightness |
A graph of the phase of Venus is available here.
Apparitions of Venus
| 11 Apr 1950 | – | Morning apparition |
| 25 Jun 1951 | – | Evening apparition |
| 13 Nov 1951 | – | Morning apparition |
| 31 Jan 1953 | – | Evening apparition |
| 22 Jun 1953 | – | Morning apparition |
| 05 Sep 1954 | – | Evening apparition |
| 25 Jan 1955 | – | Morning 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 | 00h04m00s | 1°26'N | Pisces | 24.8" |
| Sun | 21h08m | 16°26'S | Capricornus | 32'27" |
The coordinates above are given in J2000.0.
The sky on 23 Nov 2024
| The sky on 23 November 2024 | ||||||||||||||||||||||||||||||||||
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41% 22 days old |
All times shown in EST.
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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
| 31 Jan 1953 | – Venus at greatest elongation east |
| 16 Feb 1953 | – Venus at highest altitude in evening sky |
| 22 Jun 1953 | – Venus at greatest elongation west |
| 09 Aug 1953 | – Venus at highest altitude in morning sky |
Image credit
© NASA/Ricardo Nunes