Lunar occultation of Beta1 Scorpii

Dominic Ford, Editor
From the Lunar Occultations feed


Objects: Acrab

The Moon will pass in front of Beta1 Scorpii (Acrab), creating a lunar occultation visible from Sub-Saharan Africa and eastern Brazil. 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 Beta1 Scorpii (Acrab) 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 Beta1 Scorpii (Acrab) 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)
Angola 03:56–05:36
Brazil 02:45–03:37
Ivory Coast 03:00–04:03
Guinea 02:49–03:54
Senegal 02:47–03:39
Mali 02:59–03:43
Ghana 03:15–04:03
Gabon 03:53–04:48
Liberia 02:53–04:03
Namibia 03:58–05:37
Sierra Leone 02:50–03:54
Republic of the Congo 03:57–04:56
Democratic Republic of the Congo 03:59–05:03
Guinea-Bissau 02:47–03:43
Mauritania 02:56–03:25
Gambia 02:48–03:37
Cape Verde 02:38–03:33
Burkina Faso 03:22–03:38
Sao Tome and Principe 03:44–04:26
Saint Helena 03:00–04:40

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 Beta1 Scorpii (Acrab) at the moment of the occultation will be as follows:

Object Right Ascension Declination Constellation Magnitude Angular Size
Beta1 Scorpii (Acrab) 16h05m20s 19°48'S Scorpius 2.6 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
22 Sep 2020 05 Feb 2021 Occultations of Beta1 Scorpii (Acrab) 01 Apr 2021 09 Jan 2032
12 Dec 2020 05 Feb 2021 Occultations 08 Mar 2021 25 Jun 2021

The sky on 4 Mar 2021

The sky on 4 March 2021
Sunrise
06:20
Sunset
17:47
Twilight ends
19:18
Twilight begins
04:48


Waning Gibbous

54%

21 days old

Planets
Rise Culm. Set
Mercury 05:14 10:20 15:25
Venus 06:16 11:45 17:14
Moon 23:12 04:22 09:25
Mars 09:27 16:51 00:15
Jupiter 05:17 10:21 15:26
Saturn 04:52 09:47 14:42
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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