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Keeping Time with the
Skies
By:K Sandeep Swamy(M.Sc,B.Ed)
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For thousands of years, humans have looked to the skies to track the passage of time. The
rhythmic cycles of the Sun, Moon, and stars have formed the foundation of our calendars
and timekeeping systems, connecting us to the cosmos and helping us organize our lives.
The Moon's Changing Appearance
Meera was surprised to see the Moon during daytime at the Patang
Mahotsav in Ahmedabad. She knew the Moon is spherical and shines by
reflecting sunlight, but wondered why its shape changes every night.
This observation led her to question: Why isn't the whole Moon visible
every night? What causes the Moon's changing shape?
Observing the Moon's
Phases
Spot the Moon
Begin observation after a full Moon day, looking for the Moon at sunrise in the western
direction.
Document Changes
Record the date, time of observation, and shade a circle to show the bright portion
of the Moon.
Track Daily Changes
Note whether the bright portion is increasing or decreasing, and if the Moon
appears closer to or farther from the Sun.
Continue Observations
After about 15 days, switch to observing at sunset for the next 15 days to
complete the cycle.
The Lunar Cycle
The Moon goes through a complete cycle of phases in about one month. During the waning period (Krishna Paksha), the bright portion decreases from a full
circle to nothing over two weeks. During the waxing period (Shukla Paksha), the bright portion increases from nothing to a full circle over the next two
weeks.
The day when the Moon appears as a full bright circle is called the full Moon day (Purnima), and the day when it is not visible is called the new Moon day
(Amavasya).
Locating the Moon in the Sky
Full Moon Position
On a full Moon day, the Moon is nearly
opposite the Sun4when the Sun rises in the
East, the Moon is almost setting in the West.
Half Moon Position
When the bright part decreases to a half
circle shape, the Moon is overhead at sunrise.
Crescent Moon Position
A few days later, the crescent Moon appears
even closer to the Sun in the sky.
Knowing the phase of the Moon and whether it is waxing or waning can help us find out where and when to look for the Moon on any given day. A waxing
Moon is easiest to spot at sunset, and a waning Moon at sunrise.
The Moon's Daily Movement
The Moon rises about 50 minutes later each day. This means that
sometimes moonrise happens in the afternoon, allowing you to spot the
Moon in the eastern sky during daylight.
This shift occurs because the Moon moves ahead in its orbit while the
Earth completes one rotation about its axis in 24 hours. Earth needs to
rotate some more for the Moon to appear in nearly the same spot in the
sky.
Understanding Moon Phases
Illumination Source
The Sun illuminates half of the Moon at all
times. The half facing the Sun is bright, while
the other half remains dark.
Earth's Perspective
From Earth, we can only see the illuminated
portion of the Moon that faces us, which
changes as the Moon orbits.
Orbital Position
As the Moon revolves around Earth, the angle
between the Sun, Moon, and Earth changes,
creating different phases.
Complete Cycle
The Moon completes one revolution around
Earth in about 29.5 days, creating a full cycle of
phases.
Exploring Moon Phases
Activity: Modeling Moon Phases
Take a small soft ball on a stick to represent the Moon
1.
Use a flashlight or lamp to represent the Sun
2.
Your head represents Earth
3.
Hold the ball at arm's length and observe how the illuminated portion
changes as you turn
4.
This activity demonstrates how the shape of the illuminated portion of the
Moon changes depending on its position relative to the Sun and Earth.
The Moon's Orbit and
Phases
As the Moon revolves around Earth, its position relative to the Sun changes. The diagram
shows how this creates different phases:
At position A: Full Moon - the entire illuminated side faces Earth
At positions B and H: Gibbous phase - more than half of the illuminated portion is
visible
At positions C and G: Half Moon - exactly half of the illuminated portion is visible
At positions D and F: Crescent phase - less than half of the illuminated portion is visible
At position E: New Moon - the non-illuminated side faces Earth
Common Misconception
Moon Phases b Earth's Shadow
A common misconception is that the Moon's phases are caused by Earth's
shadow falling on it. This is incorrect. The phases occur due to the changing
relative positions of the Sun, Moon, and Earth as the Moon revolves around Earth.
Earth's shadow on the Moon causes a lunar eclipse, which can only happen on a
full Moon day. Similarly, a solar eclipse can only happen on a new Moon day.
These eclipses don't occur every month due to the tilt of the Moon's orbit.
Natural Cycles for Timekeeping
1
Day
Based on Earth's rotation around its axis,
causing the apparent daily motion of the Sun.
One complete rotation takes 24 hours (a
mean solar day).
2
Month
Based on the Moon's cycle of phases, which
takes approximately 29.5 days to complete
one full cycle from new Moon to new Moon.
3
Year
Based on Earth's revolution around the Sun,
which takes approximately 365.25 days and
creates the cycle of seasons.
These natural cycles formed the basis for human timekeeping systems and calendars throughout history.
Measuring a Solar Day
Activity: Finding the Shortest Shadow
Fix a 1-meter stick vertically in a flat area that receives sunlight
1.
Mark the tip of the shadow every minute from 11:00 AM to 1:10 PM
2.
Identify when the shadow was shortest (when the Sun is at its highest)
3.
Record this time and repeat for several days
4.
Calculate the duration between shortest shadows on consecutive days
5.
The average duration should be approximately 24 hours, which is the length
of a mean solar day.
The Gregorian Calendar
Features of the
Gregorian Calendar
Widely used solar calendar with 365
days in a common year
Months have varying lengths: 30 or 31
days (except February with 28 days)
Adds a leap day every four years to
account for the extra quarter day
Years divisible by 4 are leap years, with
February having 29 days
Fine-Tuning the Calendar
Years divisible by 100 are not leap
years (e.g., 1700, 1800, 1900)
Exception: Years divisible by 400 are
leap years (e.g., 1600, 2000)
These adjustments keep the calendar
closely matched with the seasons
Without these corrections, the
calendar would gradually drift away
from the seasons
Types of Calendars
Lunar Calendars
Based on the Moon's phases, with months of
approximately 29.5 days. A lunar year has 12
lunar months (354 days), which is shorter
than the solar year. Seasons don't remain
synchronized to the same lunar months in
successive years.
Solar Calendars
Based on Earth's revolution around the Sun
(365.25 days). Months are adjusted to add up
to 365 days, with leap years adding an extra
day every four years. The Gregorian calendar
is a solar calendar that keeps seasons
synchronized.
Luni-Solar Calendars
Combines elements of both lunar and solar
calendars. Uses the Moon's phases for
counting days and months but adds an extra
month (intercalary month) every few years to
stay synchronized with the seasons.
The Indian National
Calendar
The Indian National Calendar is a solar calendar adopted by the Government of India in
1957 based on the recommendations of the Calendar Reform Committee chaired by
Meghnad Saha.
Key Features
365 days in a year, beginning on March 22 (day after spring equinox)
Months have either 30 or 31 days (unlike Gregorian calendar)
Month names taken from traditional Indian calendars
Leap years match the Gregorian calendar by adding a day to Chaitra
Month Structure
First month: Chaitra (begins March 22)
Second to sixth months have 31 days
Remaining months have 30 days
In leap years, the new year begins on March 21
Traditional Indian
Calendars
Lunar Calendar Features
Months: Chaitra, Vaisakha, Jyeshtha,
Ashadha, Shravana, Bhadrapada,
Ashwin, Kartika, Margashirsha, Pausha,
Magha, and Phalguna
Amant: New month starts after new
Moon
Purnimant: New month starts after full
Moon
Astronomical
Observations
Uttarayan: Sun's apparent northward
movement (December to June)
Dakshinayan: Sun's apparent southward
movement (June to December)
Ancient texts like Surya Siddhanta
recorded these observations
Festivals and Astronomical Events
Lunar-Based Festivals
Diwali: New Moon of Kartika
Holi: Full Moon of Phalguna
Buddha Purnima: Full Moon of Vaisakha
Eid-ul-Fitr: After sighting the crescent Moon at the end of Ramazan
Solar-Based Festivals
Makar Sankranti/Pongal
Bihu
Vaisakhi
Poila Baisakh
Puthandu
Lunar-based festivals occur on different dates in the Gregorian calendar each year, while solar-based festivals happen on nearly the same date every year.
Some solar festivals were originally tied to solstices or equinoxes but have shifted slightly over time due to the difference between sidereal and tropical
years.
Cultural Significance of Celestial Bodies
Moon in Indian Arts
The Moon and moonlight have inspired various art forms in India:
Music: Ragas like Chandrakauns, Chandranandan, and
Shubhapantuvarali
Dance: Mudras like Chandrakala and Ardhachandran in Bharatanatyam,
Kathak, Odissi, and Kuchipudi
Visual Arts
Traditional painting styles and crafts feature celestial bodies:
Madhubani and Warli paintings
Tribal art by Saura, Gond, and others
Dhokra brass sculptures
Artificial Satellites
Besides the Moon, Earth's natural satellite, there are many artificial
satellites orbiting our planet. These human-made objects appear as tiny
moving specks in the night sky, especially visible just before sunrise or
after sunset.
Most artificial satellites orbit about 800 km above Earth's surface and take
roughly 100 minutes to complete one orbit. They serve various purposes
including communication, navigation, weather monitoring, disaster
management, and scientific research.
Indian Space Missions
Cartosat Series
Earth observation satellites that capture high-quality images for mapping,
urban planning, and disaster management. These images are used in
platforms like Bhuvan.
AstroSat
India's first dedicated multi-wavelength space observatory for studying
celestial objects and astronomical phenomena.
Chandrayaan Missions
Series of lunar exploration missions including Chandrayaan-1, 2, and 3,
designed to study the Moon's surface and composition.
Aditya L1
Mission to study the Sun from the first Lagrangian point, providing insights
into solar activities and their effects.
Mangalyaan
Mars Orbiter Mission that successfully reached Mars orbit, making India the
first country to do so in its first attempt.
Student Satellites
Small satellites built by Indian students, such as AzaadiSat, InspireSat-1, and
Jugnu, promoting space education.
Spotting Artificial Satellites
How to Spot Satellites
Find a location with a clear view of the sky, away from light pollution
1.
Look just before sunrise or after sunset when satellites reflect sunlight
but the sky is dark
2.
Watch for steadily moving points of light crossing the sky
3.
Satellites move much faster than stars and planets
4.
Use mobile apps or websites that provide satellite pass predictions for
your location
5.
Space Debris Concern
After their useful life, many satellites and rocket parts become
space junk. This debris crowds space and could collide with
working satellites. While small debris burns up in the atmosphere,
larger pieces can crash on Earth. Countries are working together
to address this issue.
Pioneers of Indian Space Science
Vikram Sarabhai (1919-1971)
Known as the Father of the Indian Space Programme, Vikram Sarabhai was
a researcher in space science and nuclear physics who pioneered the
effort to launch India's first artificial satellites.
The Vikram Sarabhai Space Centre (VSSC) in Thiruvananthapuram, which
develops rockets and launch vehicle technology for ISRO, is named after
him.
His vision of using space technology for national development and
education has guided India's space program since its inception.
Meghnad Saha: Astrophysicist and Calendar
Reformer
Scientific Contributions
Meghnad Saha (1893-1956) was a pioneering Indian astrophysicist who
developed the Saha equation, which explains the spectral classification of
stars based on their temperature and ionization states.
His work revolutionized our understanding of stellar physics and helped
astronomers determine the physical properties of stars by analyzing their
spectra.
Calendar Reform
As chairperson of the Calendar Reform Committee established by the
Government of India in 1952, Saha led the effort to create a unified national
calendar.
The committee's recommendations resulted in the adoption of the Indian
National Calendar in 1957, which is still used alongside the Gregorian
calendar for official purposes.
The Saha Institute of Nuclear Physics in Kolkata is named in his honor.
Key Takeaways: Celestial Timekeeping
Moon Phases
The illuminated part of the Moon changes shape due to its position
relative to the Earth and Sun as it orbits. A full cycle takes about 29.5
days.
Natural Cycles
Day (Earth's rotation), month (Moon's phases), and year (Earth's
revolution) are natural cycles that formed the basis for calendars.
Calendar Types
Lunar calendars follow the Moon's cycle, solar calendars follow
seasonal cycles, and luni-solar calendars adapt to both.
Artificial Satellites
Human-made satellites orbit Earth, providing valuable information for
communication, navigation, weather monitoring, and scientific
research.
Exploring Further:
Questions to Ponder
Moon Observations
Have you ever seen the Moon during
the day? Why is it sometimes visible
when the Sun is up?
If you lived on the Moon instead of
Earth, what would you mean by a day, a
month, or a year?
What would happen if Earth had two
moons instead of one? How would that
change the night sky?
Calendar Investigations
If we didn't have clocks or calendars,
how else could we measure time?
Why do some festivals fall on different
dates each year in the Gregorian
calendar?
How are tides related to the Moon's
position and phases?