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Lesson 1 of 7

Keeping Time with the Skies · Lesson 1 of 7

Observing the Moon’s Phases

“Follow the changing Moon and learn when and where its different phases are easiest to observe.”

Learning Objectives

• Recognise full, new, crescent, half, and gibbous appearances of the Moon. • Distinguish waxing from waning using a sequence of observations. • Connect Shukla Paksha and Krishna Paksha with the changing bright portion. • Record the Moon’s appearance and its separation from the Sun at a consistent observation time. • Use phase and time of day to decide where to look for the Moon.

A Moon in the Daytime Sky

During a kite festival in Ahmedabad, Meera notices the Moon above the colourful kites. It is daytime, yet the Moon is visible. This observation challenges the idea that the Moon belongs only to the night sky. A careful look at the sky can teach us more than an assumption about what should be there.

The Moon is a roughly spherical body that reflects sunlight. Its bright appearance therefore does not require the sky to be completely dark. On some days it is above our horizon while the Sun is also up, and its illuminated portion stands out against the blue sky. Clouds, haze, nearby buildings, and brightness near the Sun can make it difficult to spot.

There is another puzzle. Sometimes the Moon looks like a complete bright disc; at other times it looks like a curved sliver or only part of a circle. The solid Moon has not changed its physical shape. We will first learn to describe the changing appearance accurately, then investigate its cause in the next lesson.

Definition
Phase of the Moon

The apparent shape of the illuminated portion of the Moon seen from Earth at a particular time.

Names for the Changing Bright Portion

The names of the phases describe how much of the circular face appears bright. They refer to what we see from Earth, rather than to the shape of the whole Moon in space. Learning these names makes a month of observations easier to compare.

AppearanceHow to recognise it
Full MoonThe visible face appears as a complete bright disc; the day is also called Purnima.
New MoonThe bright face is turned away from Earth and the Moon is ordinarily not visible; the day is also called Amavasya.
CrescentLess than half of the apparent disc is bright, forming a curved sliver.
Half MoonAbout half of the apparent disc is bright.
GibbousMore than half of the apparent disc is bright, but it is not yet or no longer full.

A single crescent drawing does not tell us whether the bright portion is growing or shrinking. That requires a sequence, or information about its position and observation time. If the bright fraction grows from one day to the next, the Moon is waxing. If it shrinks, the Moon is waning. These words describe the direction of change, not a separate physical kind of Moon.

Definition
Waxing

The part of the Moon’s disc that appears illuminated from Earth is increasing. The waxing period from new Moon toward full Moon is generally called Shukla Paksha in India.

Definition
Waning

The part of the Moon’s disc that appears illuminated from Earth is decreasing. The waning period from full Moon toward new Moon is generally called Krishna Paksha in India.

Starting at full Moon, the appearance becomes waning gibbous, then waning half, then waning crescent, and finally new Moon. After new Moon, the sequence becomes waxing crescent, waxing half, waxing gibbous, and full Moon again. Each half of this cycle lasts roughly two weeks. A full-to-full or new-to-new cycle takes about 29.5 days, so “a month” here is an approximate natural cycle, not necessarily a named calendar month.

NewWaxing crescentWaxing halfWaxing gibbousFullWaning gibbousWaning halfWaning crescentRead across each row; the next phase after the last is new Moon.
One Repeating Cycle of Moon Phases— The yellow area is the bright part seen from Earth. Left–right orientation is shown for a typical northern view; a tilted view does not change the phase name.
Example — A Shrinking Bright Disc

Problem
On Monday the Moon looks nearly full. Several days later a smaller, but still greater-than-half, portion is bright. Describe the later phase.

  1. 1.More than half of the disc is illuminated, so the appearance is gibbous.
  2. 2.The bright portion has decreased between observations, so it is waning.
  3. 3.The later appearance is a waning gibbous Moon, within Krishna Paksha.
Example — A Growing Crescent

Problem
A thin crescent is followed several days later by a half-lit disc. Is this Shukla Paksha or Krishna Paksha?

  1. 1.Compare the bright portions: less than half has grown to about half.
  2. 2.An increasing bright portion is waxing.
  3. 3.This sequence belongs to Shukla Paksha. A crescent alone, without this comparison, would not establish the direction of change.

Where and When to Look

The Moon’s phase is connected with its position relative to the Sun in our sky. Here, “closer to the Sun” means a smaller separation in the directions we look, not that the Moon has travelled close to the Sun in space. Knowing both the phase and the time of observation helps us search in the right part of the sky.

Near full Moon, the Sun and Moon are approximately opposite in the sky. As the Sun rises in the east, the full Moon is near setting in the west. At sunset the opposite arrangement occurs: the full Moon is near rising in the east. A full Moon is therefore visible for much of the night when the sky is clear.

On successive mornings after full Moon, observe at sunrise. The waning Moon appears progressively nearer the Sun’s direction. Near the waning half phase it is high in the sky, and a later waning crescent is nearer the eastern sky before sunrise. “High” does not mean directly over every observer’s head; the exact height depends on place, date, and the Moon’s path.

For the waxing half of the cycle, sunset is a useful observation time. A young waxing crescent lies relatively near the setting Sun in the western sky. Later waxing phases are farther from the Sun’s direction, and near waxing half the Moon is high at sunset. These patterns also explain why a waxing gibbous Moon can be seen in the eastern sky during the afternoon.

Phase and timeUseful place to searchRelationship to the Sun
Full Moon at sunriseNear the western horizonApproximately opposite the rising Sun
Waning half near sunriseHigh in the skyAbout a quarter-turn from the Sun
Waning crescent before sunriseToward the eastern skyRelatively close to the Sun’s direction
Waxing crescent after sunsetToward the western skyRelatively close to the Sun’s direction
Waxing half near sunsetHigh in the skyAbout a quarter-turn from the Sun
Example — Planning an Observation

Problem
You want to look for a thin waning crescent. Would just after sunset or just before sunrise be the better starting time?

  1. 1.A waning crescent belongs to the late part of the full-to-new sequence.
  2. 2.This Moon lies relatively near the Sun’s direction and is seen before the Sun rises.
  3. 3.Begin before sunrise with a clear eastern horizon. A very thin crescent may still be hard to see, so failure to spot it does not prove that the Moon is absent.
The Moon Does Not Rise Only at Sunset

Rising near sunset is characteristic of a full Moon. Other phases rise at other times, including during daylight. Do not use a full-Moon pattern as a rule for the whole cycle.

Build a Month-long Observation Record

A regular record lets you discover a pattern instead of relying on memory. Begin at sunrise on the day after a full Moon, when the Moon is usually easy to find toward the west. Use the same safe observation spot when possible and record the date and actual time.

Draw a circle for the Moon’s disc and shade the dark portion, leaving the observed bright shape unshaded. From the second successful observation onward, compare it with the previous observation: has the bright portion increased or decreased, and is its separation from the Sun’s direction smaller or larger? Write “not observed” when clouds, buildings, or glare prevent a reliable observation. Do not invent a phase drawing to fill an empty row.

Date and timeSunrise or sunsetDrawing or visibility noteBright portion compared with last sightingSun–Moon separation compared with last sighting
Enter your date and timeSunriseDraw the observed disc; shade the dark partFirst observation: no comparisonFirst observation: no comparison
Enter the next observationSunriseDraw what you actually see, or explain why it was not seenIncreased / decreased / uncertainSmaller / larger / uncertain
Continue through the cycleSunset after the new-Moon intervalKeep drawings and notes in date orderCompare reliable observationsCompare directions, not physical distances

After roughly two weeks, the new Moon is too close to the Sun’s direction and has too little bright surface facing us to be ordinarily visible. For the following two weeks, switch to observing near sunset and follow the waxing sequence. Do not look directly at the Sun to measure separation; use its general direction, the horizon, and the observation time. Ask whether the Moon’s apparent position and bright portion changed together.

At the end, arrange the drawings in order. Look for the decrease from full to new, the increase back to full, and the repeating changes in position. A missing observation is a limit of the record, not evidence that the cycle stopped. These observations raise the next question: why does a spherical Moon produce this particular sequence?

Quiz

Quick check

A Moon is more than half bright, and its bright portion is decreasing. Which description fits?

Quick check

What does the term phase describe?

Quick check

Which sequence belongs to Shukla Paksha?

Quick check

Where is a full Moon approximately located at sunrise?

Quick check

A cloudy morning prevents a clear sighting. What should your observation table contain?

Quick check

Which is a better starting time to look for a waxing crescent?

Practice Problems

Practice Problems
  1. Describe the difference between a crescent and a gibbous Moon, and between waxing and waning.
  2. Arrange these appearances after a full Moon: new, waning crescent, waning half, waning gibbous. Explain your order.
  3. Explain how the Moon can be visible while the Sun is above the horizon.
  4. Prepare the observation table described in this lesson. State how you will handle a cloudy day and a gap between sightings.
  5. Compare where you would look for a full Moon at sunrise and a waxing crescent at sunset.
  6. Two drawings show equally thin crescents. What further observation could help you decide which one is waxing?
  7. From a sequence of your own observations, describe how the bright fraction and the Sun–Moon separation change together.

Key Takeaways

Key Takeaways

• Moon phases describe the bright part seen from Earth; the spherical Moon itself does not change shape. • Crescent, half, gibbous, full, and new describe different visible bright fractions. • Waxing means an increasing illuminated fraction and corresponds to Shukla Paksha; waning corresponds to Krishna Paksha. • Full Moon is approximately opposite the Sun, while a crescent lies closer to the Sun’s direction. • Sunrise observations suit waning phases and sunset observations suit waxing phases. • A reliable observation record distinguishes actual sightings from missing or uncertain observations.