Lunar occultation of Antares

Dominic Ford, Editor
From the Lunar Occultations feed


Objects: Antares

The Moon will pass in front of Antares (Alpha Scorpii), creating a lunar occultation visible from South America, Central America and Western Africa. 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 Columbus.

The map below shows the visibility of the occultation across the world. Separate contours show where the disappearance of Antares (Alpha Scorpii) 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 Antares (Alpha Scorpii) 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.

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

Country Time span
(UTC)
Brazil 02:10–05:08
Peru 01:55–03:55
Argentina 02:45–04:30
Bolivia 02:23–04:26
Colombia 01:57–03:34
Mexico 01:29–02:31
Paraguay 02:50–04:31
Chile 02:31–04:00
Ecuador 01:39–03:19
Uruguay 03:23–04:16
Ivory Coast 04:39–05:28
Nicaragua 01:47–02:40
Honduras 01:45–02:34
Guatemala 01:40–02:32
Liberia 04:39–05:27
Panama 01:52–02:51
Venezuela 02:37–03:24
Guinea 04:44–05:20
Sierra Leone 04:44–05:17
Costa Rica 01:47–02:46
Belize 01:49–02:27
El Salvador 01:43–02:34
Saint Helena 04:27–05:30
Clipperton Island 01:28–02:26

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 Antares (Alpha Scorpii) at the moment of the occultation will be as follows:

Object Right Ascension Declination Constellation Magnitude Angular Size
Antares (Alpha Scorpii) 16h29m20s 26°25'S Scorpius 1.1 0'00"

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
25 Jan 1987 14 May 1987 Occultations of Antares (Alpha Scorpii) 08 Jul 1987 08 Feb 1991
25 Apr 1987 07 Jun 1987 Occultations 05 Jul 1987 03 Sep 1987

The sky on 30 Jun 2024

The sky on 30 June 2024
Sunrise
06:03
Sunset
21:04
Twilight ends
23:06
Twilight begins
04:01


Waning Crescent

27%

24 days old

Planets
Rise Culm. Set
Mercury 07:24 14:49 22:15
Venus 06:36 14:05 21:33
Moon 01:52 08:44 15:50
Mars 02:51 09:48 16:45
Jupiter 04:01 11:19 18:37
Saturn 00:36 06:19 12:01
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.

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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