Venus at perihelion

Dominic Ford, Editor
From the Inner Planets feed


Objects: Venus

Venus's 225-day orbit around the Sun will carry it to its closest point to the Sun – its perihelion – at a distance of 0.72 AU from the Sun.

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
Venus 13h33m20s 7°25'S Virgo 18.1"
Sun 16h26m 21°42'S Ophiuchus 32'26"

The coordinates above are given in J2000.0.

From Fairfield, Venus will be visible in the dawn sky, rising at 03:13 (EDT) – 3 hours and 43 minutes before the Sun – and reaching an altitude of 32° above the south-eastern horizon before fading from view as dawn breaks at around 06:37.

The sky on 29 Jun 2024

The sky on 29 June 2024
Sunrise
05:20
Sunset
20:29
Twilight ends
22:37
Twilight begins
03:12


Waning Crescent

35%

23 days old

Planets
Rise Culm. Set
Mercury 06:36 14:07 21:38
Venus 05:52 13:24 20:57
Moon 00:47 07:15 13:57
Mars 02:11 09:10 16:09
Jupiter 03:22 10:44 18:05
Saturn 00:02 05:44 11:25
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

30 Oct 1999  –  Venus at greatest elongation west
17 Jan 2001  –  Venus at greatest elongation east
06 Feb 2001  –  Venus at highest altitude in evening sky
07 Jun 2001  –  Venus at greatest elongation west

Image credit

© NASA/Ricardo Nunes

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