Moon at Last Quarter
2015 May 11
Dominic Ford – originally published on In-The-Sky.org
From London (click to change), the Moon will be visible in the dawn sky. It will rise at 02:04 (GMT), 3 hours and 12 minutes before the Sun, and attain an altitude of 20° above the south-eastern horizon before fading from view as dawn breaks at around 04:50.
The Moon‘s orbital motion carries it around the Earth once every four weeks, and as a result its phases cycle from new moon, through first quarter, full moon and last quarter, back to new moon once every 29.5 days.
This motion also means that the Moon travels more than 12° across the sky from one night to the next, causing it to rise and set nearly an hour later each day. Click here for more information about the Moon’s phases.
The Moon’s path in coming days
Over the next few days, the distance between the Moon and the Sun will decrease each night, and it will rise later in the night each day. Eventually it will only be visible very shortly before sunrise and it will sink into the Sun’s glare as it approaches new moon (all times given below in London local time).
|Altitude of Moon
|Direction of Moon
|06 May 2015||20:24||07:04||11°||south-west|
|07 May 2015||20:26||07:50||15°||south-west|
|08 May 2015||20:28||08:44||18°||south|
|09 May 2015||20:29||09:44||21°||south|
|10 May 2015||20:31||10:51||22°||south|
|11 May 2015||20:32||12:03||22°||south-east|
|12 May 2015||20:34||13:16||21°||south-east|
|13 May 2015||20:35||14:30||19°||south-east|
|14 May 2015||20:37||15:46||16°||east|
|15 May 2015||20:38||17:05||11°||east|
|16 May 2015||20:40||18:21||7°||east|
|17 May 2015||20:41||19:35||1°||east|
Observing the Moon at last quarter
The period when the Moon shows half phase is ideal for observing the Moon with a pair of binoculars or a small telescope, because the mountains and craters on its surface are presented very clearly. Even though only half of the Moon’s face is illuminated, this is a time when the terminator line which divides the illuminated and unilluminated portions of the Moon’s disk is clearly visible.
Along this line, an observer on the Moon would see the Sun rising above the horizon. As it does so, it illuminates the lunar landscape at a low angle, making mountains and crater rims cast long shadows which are easy to see from Earth, even through a modest pair of binoculars.
Although the Moon is always separated from the Sun by the same amount – 90° – when it passes last quarter, it is more favourably placed in the pre-dawn sky at some times of year than others.
Specifically, it appears high up in the pre-dawn sky around the autumn equinox, but much lower towards the horizon around the spring equinox.
This is because it always lies close to a line across the sky called the ecliptic. This is the line through the zodiacal constellations that the Sun follows through the year, and marks the flat plane in space in which all of the planets circle the Sun.
The altitude at which the Moon appears above the horizon at sunrise depends how steeply the line of the ecliptic is inclined to the horizon. If the plane of the ecliptic meet the horizon at a very shallow angle, the Moon will rise or set along a line which is almost parallel to the horizon, and a large separation from the Sun along this line would still only correspond to a very low altitude in the sky.
The inclination of the ecliptic plane to the horizon at London varies between 61° (sunrise at the autumn equinox) and 15° (sunrise at the spring equinox). On May 11, the ecliptic is inclined at 19° to the eastern dawn horizon, as shown by the yellow line in the planetarium view above, meaning that on this occasion the Moon is poorly placed for viewing from London.
The Moon’s position
At the moment it reaches last quarter, the Moon’s distance from the Earth will be 371,000 km. Its exact position will be as follows:
|Object||Right Ascension||Declination||Constellation||Angular Size|
The coordinates above are given in J2000.0.
The details of this observing event were provided courtesy of In-The-Sky.org