I have noticed that the inclination of the moon at a given location varies throughout the night. From the UK, the terminator in a half-moon is clearly sloping from top left to bottom right early in the evening, but later on, as the moon is setting, it is clearly sloping from top right to bottom left. I know that the shape of the moon changes from night to night, but I just can't see why the inclination would change during a single night. I know that the appearance of the moon is due to a combination of the tilt of the earth's axis and the latitude of my position (the moon slopes oppositely in the southern hemisphere), but I just can't visualise in three dimensions exactly what is going on. Please can you help me to do this.


3 Answers 3


If you take a line from the middle of the terminator, but at 90 degrees to the termination, it more or less points towards the sun. Now consider the moon at first quarter: as the moon rises, the sun is due south, so imagine a line from the moon to the sun, and the terminator will be at 90 degrees to this, so pointing from bottom right to top left. At mid-day, the sun is in the west, and the terminator will be sloping bottom left to top right.


A relatively simple way to understand why the moon axis seems to rotate is to observe that the stars do the same thing. Watch over several hours as Cassiopeia - located near the North Star moves and you'll notice the orientation changes. Cassiopeia, for example, is shaped like a "W" when lowest in the sky, a "3" as it rises, an "M" as it reaches its highest point overhead, a Σ (Sigma) as it is setting. Below is the constellation as it appears lowest in the sky.

[Cassiopea at its lowest point

Image from IAU and Sky & Telescope magazine (Roger Sinnott & Rick Fienberg)

Because Cassiopeia is close to the north celestial pole observers in the Northern hemisphere can watch the constellation rotate through all 360 degrees through the year. Orion, however is near the celestial equator and the amount of apparent rotation relative to the ground is always less than 180 degrees and as little as 45 degrees - depending on your latitude.

The moon can be found anywhere from +28.5° to −28.5 (above or below) the celestial equator - its position relative to your observing latitude dictates the maximum amount of apparent rotation.


Adding to Chuck's answer, you may be interested in looking into the parallactic angle. Peter Meadows discusses it in a page on his site. There are a couple of things to keep in mind:

  • that page explains it in the context of observations of the Sun rather than the Moon,
  • the Moon's terminator doesn't point at the celestial poles.

PeterMeadows.com dawn PeterMeadows.com dusk


The naked eye view of the Sun just after sunrise and just before sunset at one the equinoxes and for an observer at at London (51.5°N, 0.0°E) . The two rectangles show the field of view for an alt/azi and equatorial telescope mounting.

  • $\begingroup$ Since links can break over time, I've included a bit of the relevant information. It's a great site! $\endgroup$
    – uhoh
    Feb 21, 2019 at 23:13

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