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 Oceania, Peru and northern Chile. 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)
Peru 10:13–11:07
Chile 10:16–10:51
Fiji 07:01–08:18
New Caledonia 07:10–07:59
Solomon Islands 06:51–07:55
Vanuatu 06:56–08:01
French Polynesia 07:55–09:34
Kiribati 06:50–07:49
Samoa 07:04–08:19
Tonga 07:08–08:26
American Samoa 07:07–08:22
Cook Islands 07:30–08:54
Niue 07:12–08:31
Tuvalu 06:53–08:00
Wallis and Futuna 07:00–08:13
Nauru 06:46–07:44
New Zealand 07:27–08:25
Marshall Islands 06:56–07:29
Pitcairn 08:55–10:16
Baker Island 07:08–07:36
Howland Island 07:11–07:32
Tokelau 07:04–08:05

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
10 Jun 1968 12 May 1971 Occultations of Antares (Alpha Scorpii) 05 Jul 1971 28 May 1972
16 May 1971 16 May 1971 Occultations 10 Jun 1971 08 Jul 1971

The sky on 22 Nov 2024

The sky on 22 November 2024
Sunrise
07:23
Sunset
17:10
Twilight ends
18:45
Twilight begins
05:47


Waning Crescent

45%

21 days old

Planets
Rise Culm. Set
Mercury 09:15 13:45 18:15
Venus 10:48 15:18 19:49
Moon 22:59 06:12 13:13
Mars 21:34 04:54 12:13
Jupiter 18:09 01:32 08:56
Saturn 13:47 19:20 00:53
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.

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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