Lunar occultation of Regulus

Dominic Ford, Editor
From the Lunar Occultations feed


Objects: Regulus

The Moon will pass in front of Regulus (Alpha Leonis), creating a lunar occultation visible from Mexico and the Contiguous United States. 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.

The occultation will be visible from Fairfield. It will begin with the disappearance of Regulus (Alpha Leonis) behind the Moon at 21:58 EDT, though at a low altitude of only 1.0 degrees, in the western sky. Its reappearance will be visible at 22:14 EDT, though at a low altitude of -1.9 degrees.

The map below shows the visibility of the occultation across the world. Separate contours show where the disappearance of Regulus (Alpha Leonis) 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 Regulus (Alpha Leonis) 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)
Mexico 02:29–03:15
The Contiguous United States 02:10–03:15

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.

At the time of the occultation, the Moon will be 0 days past new moon and will be 9% illuminated. Regulus (Alpha Leonis) will disappear behind the unilluminated side of the Moon and reappear from behind the unilluminated side of the Moon.

The position of Regulus (Alpha Leonis) at the moment of the occultation will be as follows:

Object Right Ascension Declination Constellation Magnitude Angular Size
Regulus (Alpha Leonis) 10h08m20s 11°58'N Leo 1.4 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
01 Nov 1980 19 Jun 1988 Occultations of Regulus (Alpha Leonis) 06 Oct 1988 30 Nov 1988
12 Oct 1987 11 Jul 1988 Occultations 25 Jul 1988 01 Oct 1988

The sky on 25 Nov 2024

The sky on 25 November 2024
Sunrise
06:50
Sunset
16:26
Twilight ends
18:04
Twilight begins
05:13


Waning Crescent

20%

24 days old

Planets
Rise Culm. Set
Mercury 08:30 12:58 17:26
Venus 10:15 14:43 19:11
Moon 01:23 07:34 13:35
Mars 20:42 04:05 11:28
Jupiter 17:13 00:40 08:07
Saturn 12:57 18:29 00:01
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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