Lunar occultation of Spica

Dominic Ford, Editor
From the Lunar Occultations feed


Objects: Spica

The Moon will pass in front of Spica (Alpha Virginis), creating a lunar occultation visible from countries and territories including Fiji, French Polynesia, Samoa and Tonga amongst others. 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 Cambridge.

The map below shows the visibility of the occultation across the world. Separate contours show where the disappearance of Spica (Alpha Virginis) 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 Spica (Alpha Virginis) 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)
Fiji 05:49–07:32
French Polynesia 06:55–08:16
Samoa 06:08–07:46
Tonga 06:12–07:41
American Samoa 06:14–07:49
Cook Islands 06:45–08:04
Kiribati 05:27–07:23
Niue 06:22–07:49
Tuvalu 05:36–07:20
Wallis and Futuna 05:58–07:36
Pitcairn 07:24–08:03
Baker Island 05:56–07:04
Howland Island 05:58–07:00
Jarvis Island 06:59–07:30
Tokelau 06:06–07:38

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 Spica (Alpha Virginis) at the moment of the occultation will be as follows:

Object Right Ascension Declination Constellation Magnitude Angular Size
Spica (Alpha Virginis) 13h25m10s 11°09'S Virgo 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
27 Mar 2043 28 Jun 2050 Occultations of Spica (Alpha Virginis) 22 Aug 2050 09 Dec 2050
12 Feb 2049 14 Jul 2050 Occultations 29 Jul 2050 10 Aug 2050

The sky on 22 Nov 2024

The sky on 22 November 2024
Sunrise
06:41
Sunset
16:16
Twilight ends
17:55
Twilight begins
05:02


Waning Crescent

48%

21 days old

Planets
Rise Culm. Set
Mercury 08:36 12:57 17:19
Venus 10:09 14:31 18:53
Moon 22:03 05:23 12:29
Mars 20:40 04:06 11:33
Jupiter 17:14 00:45 08:16
Saturn 13:02 18:32 00:03
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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