© NASA/Ricardo Nunes

Venus at greatest brightness

Dominic Ford, Editor
From the Inner Planets feed

Objects: Venus
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Venus will reach its greatest brightness in its 2135 morning apparition. It will be shining brightly at mag -4.5.

From Fairfield , this apparition will be exceptionally well placed and prominent, reaching a peak altitude of 42° above the horizon at sunrise on 28 Sep 2135.

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2135 morning apparition of Venus

12 Jul 2135 – Venus at inferior solar conjunction
17 Aug 2135 – Venus at greatest brightness
20 Sep 2135 – Venus at dichotomy
22 Sep 2135 – Venus at greatest elongation west
28 Sep 2135 – Venus at highest altitude in morning sky

A graph of the brightness of Venus is available here.

Apparitions of Venus

25 Sep 2133 – Evening apparition
15 Feb 2134 – Morning apparition
03 May 2135 – Evening apparition
22 Sep 2135 – Morning apparition
08 Dec 2136 – Evening apparition
29 Apr 2137 – Morning apparition
13 Jul 2138 – Evening 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 brightness

Venus's brightness depends on two factors: its closeness to the Earth, and its phase. Its 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 reaches its brightest when it is still a crescent – with less than half of its disk illuminated. This is because it is much closer to the Earth during its crescent phases than at other times.

As a result, during evening apparitions, Venus reaches maximum brightness a few days after it is at greatest separation from the Sun, which always coincides with it showing half-phase (dichotomy).

Conversely, during morning apparitions, Venus reaches maximum brightness a few days before it is at greatest separation from the Sun.

Venus's position

The coordinates of Venus when it reaches its greatest brightness will be:

Object Right Ascension Declination Constellation Angular Size
Venus 06h56m10s 17°09'N Gemini 37.8"
Sun 09h39m 14°01'N Leo 31'35"

The coordinates above are given in J2000.0.

The sky on 28 Mar 2024

The sky on 28 March 2024
Sunrise
06:40
Sunset
19:13
Twilight ends
20:47
Twilight begins
05:06

18-day old moon
Waning Gibbous

87%

18 days old

Planets
Rise Culm. Set
Mercury 07:08 13:57 20:46
Venus 06:08 11:53 17:38
Moon 21:47 02:58 08:00
Mars 05:29 10:52 16:16
Jupiter 08:21 15:22 22:23
Saturn 05:52 11:26 17:00
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

03 May 2135  –  Venus at greatest elongation east
22 Sep 2135  –  Venus at greatest elongation west
28 Sep 2135  –  Venus at highest altitude in morning sky
08 Dec 2136  –  Venus at greatest elongation east

Image credit

© NASA/Ricardo Nunes

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Fairfield

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41.14°N
73.26°W
EDT

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