The Moon at apogee

Dominic Ford, Editor
From the Moon feed


Objects: The Moon

The Moon will reach the furthest point along its orbit to the Earth and will appear slightly smaller than at other times.

The Moon's distance from the Earth varies because its orbit is not perfectly circular – it is slightly oval-shaped, tracing out a path called an ellipse.

As the Moon traverses this elliptical path around the Earth each month, its distance varies by 14%, between 356,500 km at perigee (closest approach to the Earth) and 406,700 km at apogee (furthest from the Earth).

Its angular size also varies by the same small factor, between 29.4 arcmin and 33.5 arcmin and its brightness also changes, though this is hard to detect in practice since the Moon's phases are changing at the same time.

The chart below shows this variation in the Moon's angular size to scale. The change is small enough that it is virtually impossible to perceive except by comparing photographs:

Full Moon
at perigee
Full Moon
at apogee

The exact period of the Moon's cycle between perigee (closest approach), apogee (furthest recess) and back again is 27.555 days – a period of time called an anomalistic month. This is very close to the Moon's orbital period (27.322 days), but slightly longer. For more information on why these periods don't exactly match, see In-The-Sky.org's glossary article for the term month.

As the apogee of 27 September 2013 will occur when the moon is around last quarter phase, it will appear in the morning sky.

The Moon illusion

Although the angular size of the Moon only changes by a very modest amount in reality, a very common optical illusion is that the Moon appears very much larger than it really is when it is close to the horizon. This is called the Moon illusion – and is nothing more than an optical illusion. Any photograph will reveal that the Moon is exactly the same size regardless of whether it appears on the horizon or directly overhead.

The reason why we perceive this optical illusion is hotly debated. However, it may explain why some people are convinced that the Moon appears larger on some nights than others, despite the actual changes in its true size being so small.

Celestial coordinates

On this occasion the Moon will recede to a distance of 404,000 km from the Earth and appear with an angular diameter of 29.54 arcmin.

The position of the Moon at the moment of apogee will be:

Object Right Ascension Declination Constellation Angular Size
The Moon 06h46m40s 18°20'N Gemini 29'32"

The coordinates above are given in J2000.0.

The sky on 27 Nov 2024

The sky on 27 November 2024
Sunrise
06:47
Sunset
16:13
Twilight ends
17:53
Twilight begins
05:07


Waning Crescent

8%

26 days old

Planets
Rise Culm. Set
Mercury 08:15 12:41 17:06
Venus 10:12 14:37 19:02
Moon 03:16 08:44 14:02
Mars 20:23 03:50 11:17
Jupiter 16:52 00:22 07:53
Saturn 12:42 18:13 23:44
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.

Related news

26 Sep 2013  –  Moon at Last Quarter
04 Oct 2013  –  New Moon
11 Oct 2013  –  Moon at First Quarter
18 Oct 2013  –  Full Moon

Image credit

Simulated image courtesy of Tom Ruen.

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