Venus's 225-day orbit around the Sun will carry it to its furthest point to the Sun – its aphelion – at a distance of 0.73 AU.
In practice, however, Venus's orbit is very close to circular; its distance from the Sun varies by only about 1.5% between perihelion and aphelion. This makes Venus's orbit more perfectly circular than that of any of the Solar System's other planets. As a result, its surface receives almost exactly the same amount of energy from the Sun at perihelion (closest approach to the Sun) and aphelion (furthest recess from the Sun).
The position of Venus at the moment it passes aphelion will be:
| Object | Right Ascension | Declination | Constellation | Angular Size |
| Venus | 00h07m10s | 0°53'S | Pisces | 12.8" |
| Sun | 02h10m | 13°08'N | Aries | 31'47" |
The coordinates above are given in J2000.0.
From South El Monte, Venus will be visible in the dawn sky, rising at 04:51 (PDT) – 1 hour and 20 minutes before the Sun – and reaching an altitude of 12° above the eastern horizon before fading from view as dawn breaks at around 05:55.
The sky on 12 Sep 2025
| The sky on 12 September 2025 | ||||||||||||||||||||||||||||||||||
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63% 20 days 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
| 25 Jan 1955 | – Venus at greatest elongation west |
| 10 Apr 1956 | – Venus at highest altitude in evening sky |
| 12 Apr 1956 | – Venus at greatest elongation east |
| 01 Sep 1956 | – Venus at greatest elongation west |
Image credit
© NASA/Ricardo Nunes