Venus at aphelion

Dominic Ford, Editor
From the Inner Planets feed


Objects: Venus

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 15h37m30s 21°43'S Libra 18.4"
Sun 12h46m 5°00'S Virgo 31'59"

The coordinates above are given in J2000.0.

From Cambridge, Venus will become visible at around 18:37 (EDT), 11° above your south-western horizon, as dusk fades to darkness. It will then sink towards the horizon, setting 1 hour and 43 minutes after the Sun at 20:02.

The sky on 1 Oct 2024

The sky on 1 October 2024
Sunrise
06:39
Sunset
18:25
Twilight ends
19:58
Twilight begins
05:05


Waning Crescent

0%

28 days old

Planets
Rise Culm. Set
Mercury 06:42 12:36 18:30
Venus 09:24 14:30 19:36
Moon 05:24 11:49 18:02
Mars 23:30 07:06 14:41
Jupiter 21:50 05:22 12:54
Saturn 17:30 23:03 04:35
All times shown in EDT.

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

06 Sep 1996  –  Venus at highest altitude in morning sky
05 Nov 1997  –  Venus at greatest elongation east
13 Dec 1997  –  Venus at highest altitude in evening sky
23 Feb 1998  –  Venus at highest altitude in morning sky

Image credit

© NASA/Ricardo Nunes

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