Lunar occultation of Venus

Dominic Ford, Editor
From the Lunar Occultations feed


Objects: Venus

The Moon will pass in front of Venus, creating a lunar occultation visible from Africa, Asia, Europe and western Russia. Although the occultation will only be visible across part of the world – because the Moon is so close to the Earth that its position in the sky varies by as much as two degrees across the world – a close conjunction between the pair will be more widely visible.

Unfortunately the occultation will not be visible from Fairfield.

The map below shows the visibility of the occultation across the world. Separate contours show where the disappearance of Venus is visible (shown in red), and where its reappearance is visible (shown in blue). Solid contours show where each event is likely to be visible through binoculars at a reasonable altitude in the sky. Dotted contours indicate where each event occurs above the horizon, but may not be visible due to the sky being too bright or the Moon being very close to the horizon.

Outside the contours, the Moon will not pass in front of Venus at any time, or is below the horizon at the time of the occultation. However, a close conjunction between the pair will be visible across much of the world.

The map can be downloaded in PNG , PDF or SVG format. A KMZ file , is also available, which can be opened in Google Earth to provide a higher resolution map.

The animation below shows the path of the occultation across the Earth's globe. The red circle shows where the Moon appears in front of Venus.

[Unable to display this video because your browser does not support HTML5]
You can download this video in MP4 or OGG format.

A complete list of the countries and territories where the occultation will be visible is as follows:

Country Time span
(UTC)
Algeria 11:45–14:11
Sudan 12:51–15:17
Saudi Arabia 13:38–15:29
Iran 13:58–15:32
Libya 12:24–14:54
Chad 12:22–14:51
Mali 11:35–13:46
Niger 11:49–14:26
Mauritania 11:31–13:19
Egypt 13:07–15:17
Democratic Republic of the Congo 12:43–14:38
Turkey 13:30–15:21
Russia 13:51–15:19
Nigeria 11:56–14:20
Ukraine 13:43–14:55
Ethiopia 13:38–15:12
Spain 12:07–13:26
Central African Republic 12:27–14:43
Iraq 13:49–15:29
Morocco 11:40–13:27
Cameroon 12:12–14:21
Yemen 14:02–15:19
Turkmenistan 14:07–15:32
France 12:39–13:30
Romania 13:35–14:37
Oman 14:26–15:29
Italy 12:53–14:12
Ivory Coast 11:41–13:15
Republic of the Congo 12:30–14:16
Western Sahara 11:31–13:11
Burkina Faso 11:42–13:36
Gabon 12:23–13:57
Afghanistan 14:22–15:32
Guinea 11:36–13:00
Ghana 11:46–13:27
Syria 13:43–15:19
Kazakhstan 14:00–15:26
Senegal 11:32–12:55
Greece 13:19–14:49
Pakistan 14:30–15:30
Tunisia 12:34–14:02
Bulgaria 13:30–14:38
Serbia 13:27–14:20
Eritrea 13:44–15:16
Azerbaijan 13:59–15:24
Portugal 12:04–13:13
Benin 11:51–13:40
Belarus 13:53–14:25
Jordan 13:40–15:18
Hungary 13:35–14:06
Liberia 11:43–12:53
Georgia 13:54–15:18
Croatia 13:22–14:04
Uganda 13:40–14:35
United Arab Emirates 14:19–15:29
Sierra Leone 11:39–12:50
Bosnia and Herzegovina 13:25–14:07
Togo 11:49–13:30
Moldova 13:44–14:34
Guinea-Bissau 11:35–12:48
Somalia 14:17–15:02
Armenia 13:58–15:21
Macedonia 13:26–14:24
Albania 13:22–14:19
Uzbekistan 14:10–15:27
Kenya 13:56–14:36
Equatorial Guinea 12:14–13:50
Israel 13:39–15:13
Djibouti 14:09–15:06
Montenegro 13:25–14:12
Kuwait 14:04–15:29
Qatar 14:15–15:29
The Canary Islands 11:35–13:03
Cyprus 13:38–15:06
Corsica 13:02–13:40
Gambia 11:34–12:49
Lebanon 13:42–15:11
Slovakia 13:46–14:01
Slovenia 13:31–13:46
Cape Verde 11:31–12:34
Mallorca 12:38–13:30
Palestinian Territory 13:39–15:12
Sao Tome and Principe 12:16–13:35
Poland 13:50–13:59
Menorca 12:43–13:32
Bahrain 14:14–15:29
Ibiza 12:33–13:28
Andorra 12:45–13:22
Malta 13:00–14:06
Melilla 12:11–13:22
RAF Akrotiri 13:38–15:05
Gibraltar 12:08–13:17
Vatican 13:12–13:48
Monaco 13:07–13:29
San Marino 13:20–13:42
Madeira 11:44–13:00
The Savage Islands 11:39–13:00
Isla de Alborán 12:13–13:21
Islas Chafarinas 12:13–13:22

Lunar occultations are only ever visible from a small fraction of the Earth's surface. Since the Moon is much closer to the Earth than other celestial objects, its exact position in the sky differs depending on your exact location on Earth due to its large parallax. The position of the Moon as seen from two points on opposite sides of the Earth varies by up to two degrees, or four times the diameter of the full moon.

This means that if the Moon is aligned to pass in front of a particular object for an observer on one side of the Earth, it will appear up to two degrees away from that object on the other side of the Earth.

The position of Venus at the moment of the occultation will be as follows:

Object Right Ascension Declination Constellation Magnitude Angular Size
Venus 18h21m20s 27°21'S Sagittarius -4.6 0'32"

The coordinates above are given in J2000.0.

Next/previous occultations

« Previous Next »
Visible from the Contiguous United States Worldwide Worldwide Visible from the Contiguous United States
01 Apr 2044 30 Apr 2044 Occultations of Venus 11 Dec 2045 18 Nov 2052
08 Sep 2045 10 Nov 2045 Occultations 11 Dec 2045 07 Sep 2046

The sky on 22 Nov 2024

The sky on 22 November 2024
Sunrise
06:47
Sunset
16:28
Twilight ends
18:05
Twilight begins
05:10


Waning Crescent

47%

21 days old

Planets
Rise Culm. Set
Mercury 08:40 13:06 17:32
Venus 10:13 14:39 19:06
Moon 22:16 05:32 12:36
Mars 20:52 04:15 11:38
Jupiter 17:26 00:53 08:20
Saturn 13:09 18:41 00:13
All times shown in EST.

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

22 Oct 2045  –  Venus at greatest elongation east
27 Nov 2045  –  Venus at highest altitude in evening sky
09 Feb 2046  –  Venus at highest altitude in morning sky
13 Mar 2046  –  Venus at greatest elongation west

Image credit

The Moon in conjunction with Venus and Jupiter, with the Very Large Telescope in the foreground. Image © Y. Beletsky, ESO, 2009.

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