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

Lunar occultation of Jupiter

Dominic Ford, Editor
From the Lunar Occultations feed

Objects: Jupiter

The Moon will pass in front of Jupiter, creating a lunar occultation visible from Latin America and the Caribbean, Africa, Southern Europe and France. 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 Jupiter 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.

Map showing where the occultation is visible

Outside the contours, the Moon will not pass in front of Jupiter 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 Jupiter.

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)
Brazil 00:53–03:13
Algeria 03:24–04:36
Mali 03:24–04:33
Colombia 00:44–02:24
Mauritania 03:12–04:33
Peru 00:44–02:10
Venezuela 00:57–02:46
Mexico 00:45–01:44
Spain 03:28–04:29
Niger 03:48–04:31
Morocco 03:19–04:34
France 03:34–04:24
Western Sahara 03:12–04:31
Libya 03:38–04:36
Ecuador 00:36–02:02
Guyana 01:14–02:53
Senegal 03:12–04:22
Guinea 03:22–04:15
Bolivia 01:09–02:04
Tunisia 03:36–04:36
Suriname 01:19–03:01
Nicaragua 00:46–01:53
Honduras 00:48–01:51
Portugal 03:27–04:25
Guatemala 00:46–01:45
Panama 00:45–02:03
French Guiana 01:27–03:07
Burkina Faso 03:47–04:16
Cuba 01:18–01:56
Costa Rica 00:45–01:54
Dominican Republic 01:21–02:14
Sierra Leone 03:33–04:06
Guinea-Bissau 03:17–04:15
Haiti 01:19–02:07
Belize 00:52–01:45
El Salvador 00:47–01:47
The Canary Islands 03:13–04:27
Jamaica 01:12–01:58
Gambia 03:15–04:17
Puerto Rico 01:31–02:22
Cape Verde 02:54–04:16
Trinidad and Tobago 01:20–02:45
Mallorca 03:33–04:29
Italy 03:35–04:31
Bahamas 01:35–01:54
Guadeloupe 01:34–02:39
Saint Vincent and the Grenadines 01:26–02:42
The Portuguese Azores 03:24–03:53
Menorca 03:34–04:29
Barbados 01:30–02:47
British Virgin Islands 01:37–02:25
Cayman Islands 01:11–01:48
Martinique 01:31–02:42
Curacao 01:10–02:21
Saint Kitts and Nevis 01:36–02:34
Saint Lucia 01:29–02:42
U.S. Virgin Islands 01:34–02:27
Ibiza 03:33–04:29
Andorra 03:34–04:23
Antigua and Barbuda 01:37–02:36
Dominica 01:33–02:40
Anguilla 01:39–02:31
Bonaire, Saint Eustatius and Saba 01:12–02:31
Grenada 01:24–02:41
Melilla 03:30–04:30
Gibraltar 03:29–04:28
Ivory Coast 03:52–03:59
Montserrat 01:36–02:35
Aruba 01:09–02:17
Sint Maarten 01:38–02:31
Saint Barthelemy 01:38–02:31
Saint Martin 01:39–02:30
Turks and Caicos Islands 01:45–01:54
Navassa Island 01:18–02:00
Madeira 03:19–04:20
The Savage Islands 03:17–04:24
Isla de Alborán 03:30–04:30
Islas Chafarinas 03:30–04:31

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 Jupiter at the moment of the occultation will be as follows:

Object Right Ascension Declination Constellation Magnitude Angular Size
Jupiter 21h32m00s 15°44'S Capricornus -2.8 0'47"

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
02 Feb 2089 20 Jul 2092 Occultations of Jupiter 13 Sep 2092 13 Sep 2092
29 Jul 2092 01 Aug 2092 Occultations 25 Aug 2092 13 Sep 2092

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

21-day old moon
Waning Crescent

44%

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.

Warning

Never attempt to point a pair of binoculars or a telescope at an object close to the Sun. Doing so may result in immediate and permanent blindness.

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

13 Aug 2092  –  Jupiter at opposition
12 Oct 2092  –  Jupiter ends retrograde motion
22 Jul 2093  –  Jupiter enters retrograde motion
20 Sep 2093  –  Jupiter at opposition

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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