|Tue, 03 Oct 2017 at||01:44 EDT||(106 days ago)|
Dominic Ford, Editor
From the Inner Planets feed
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 perihelion will be:
|Object||Right Ascension||Declination||Constellation||Angular Size|
The coordinates above are given in J2000.0.
From Ashburn (click to change), Venus will be difficult to observe as it will appear no higher than 18° above the horizon. It will be visible in the dawn sky, rising at 05:05 (EST) – 2 hours and 1 minute before the Sun – and reach an altitude of 18° above the eastern horizon before fading from view as dawn breaks at around 06:48.
|The sky on 03 October 2017|
All times shown in EDT.
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.
|03 Jun 2017, 01:58 EDT||– Venus at greatest elongation west|
|17 Aug 2018, 03:58 EDT||– Venus at greatest elongation east|
|06 Jan 2019, 01:02 EST||– Venus at greatest elongation west|
|24 Mar 2020, 03:31 EDT||– Venus at greatest elongation east|
© NASA/Ricardo Nunes