Solar & Lunar Eclipses, Lecture notes of Astronomy

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A total solar eclipse is one of the most spectacular natural
events to behold. Those who witness total solar eclipses
consider themselves fortunate. They carry an indelible
impression that is as much visual as it is emotional.
It is disheartening that most people never experience one of
the greatest astronomical and sensory events on our Planet.
225
Solar & Lunar Eclipses
It is an incredible coincidence that the Sun and
Moon appear the same size in the sky. It is even
more amazing that our Moon gets the chance to
perfectly eclipse the Sun. The odds of this coinci-
dence are brought to light when we consider that
our Moon is the only moon in our Solar System
that perfectly eclipses the Sun. All the other moons
of the Planets are either too large or too small
in their orbits to eclipse the Sun in precisely
the same manner as ours.
Although I have emphasized the glorious nature
of the total solar eclipse, I don’t want to undermine
the beauty of a total lunar eclipse. But they are two
different kinds of events. Total lunar eclipses are
great “casual” events that allow one to comfortably
sit and watch the coloration of the Moon gradually
change as it moves through the Earth’s shadow.
Overview of Solar and Lunar Eclipses
Both solar and lunar eclipses involve an alignment of the Earth,
Moon and Sun. A solar eclipse is the blocking of the Sun by the
Moon, either partially or totally. A lunar eclipse is the blocking of
the Moon’s light (from the Sun) by Earth’s shadow.
Solar eclipses can occur only at the time of New Moon; lunar
eclipses only at the time of Full Moon.
In order to see a total or annular solar eclipse, one must be
on a narrow path that can stretch for a thousand miles or so on
the Earth. Only those on the path will see the total or annular
eclipse those near it will see only a partial eclipse. On the
other hand, lunar eclipses can be seen by almost everyone
on the night side of the world.
Facing page. The bright “flare” at the top of this total solar eclipse picture is
known as a “diamond-ring effect” and is produced by a minute vestige of the
Sun’s surface that pokes through the edge of the Moon. Above. Everyone
gets to experience at least a few partial solar eclipses during their life.
Our
Moon is
the only
moon in
our Solar
System
that
perfectly
eclipses
the Sun.
Eclipses
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pf4
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A total solar eclipse is one of the most spectacular natural

events to behold. Those who witness total solar eclipses

consider themselves fortunate. They carry an indelible

impression that is as much visual as it is emotional.

It is disheartening that most people never experience one of

the greatest astronomical and sensory events on our Planet.

Solar & Lunar Eclipses

It is an incredible coincidence that the Sun and

Moon appear the same size in the sky. It is even

more amazing that our Moon gets the chance to

perfectly eclipse the Sun. The odds of this coinci-

dence are brought to light when we consider that

our Moon is the only moon in our Solar System

that perfectly eclipses the Sun. All the other moons

of the Planets are either too large or too small

in their orbits to eclipse the Sun in precisely

the same manner as ours.

Although I have emphasized the glorious nature

of the total solar eclipse, I don’t want to undermine

the beauty of a total lunar eclipse. But they are two

different kinds of events. Total lunar eclipses are

great “casual” events that allow one to comfortably

sit and watch the coloration of the Moon gradually

change as it moves through the Earth’s shadow.

Overview of Solar and Lunar Eclipses

Both solar and lunar eclipses involve an alignment of the Earth,

Moon and Sun. A solar eclipse is the blocking of the Sun by the

Moon, either partially or totally. A lunar eclipse is the blocking of

the Moon’s light (from the Sun) by Earth’s shadow.

Solar eclipses can occur only at the time of New Moon; lunar

eclipses only at the time of Full Moon.

In order to see a total or annular solar eclipse, one must be

on a narrow path that can stretch for a thousand miles or so on

the Earth. Only those on the path will see the total or annular

eclipse — those near it will see only a partial eclipse. On the

other hand, lunar eclipses can be seen by almost everyone

on the night side of the world.

Facing page. The bright “flare” at the top of this total solar eclipse picture is known as a “diamond-ring effect” and is produced by a minute vestige of the Sun’s surface that pokes through the edge of the Moon. Above. Everyone gets to experience at least a few partial solar eclipses during their life.

Our

Moon is

the only

moon in

our Solar

System

that

perfectly

eclipses

the Sun.

Eclipses

Umbra and Penumbra Shadows

These are the names of the shadows

responsible for all eclipses. The umbra

is the innermost and darkest shadow.

The penumbra is a secondary shadow

around the umbra. You will see a solar

eclipse if you are in the Moon’s umbra

or penumbra shadow. Lunar eclipses

occur when the Moon passes into

Earth’s umbra or penumbra shadow.

Umbra and penumbra shadows are

visible whenever it is sunny. If you look at the edge of an

object’s shadow, you will notice that it is fuzzy. This fuzzy edge

is the penumbra and the main body of the shadow is the umbra.

Solar Eclipses

There are three types of solar eclipses: total, annular and partial.

They are illustrated and explained below.

Why do annular eclipses occur? The Moon’s orbit, like those

of all orbiting bodies, is an ellipse; so the distance from the Moon

to the Earth varies (see page 102). Annular eclipses occur when

the Moon is farther away in its orbit than usual, making the

apparent size of the Moon slightly smaller than the apparent

size of the Sun. In these instances, the Moon is simply too

small to totally block the Sun.

Solar & Lunar Eclipses

a

b

b

Sun

This exaggerated illustration depicts the formation of the umbra at (a) and the surrounding penumbra at (b). The geometry of these shadows is a result of the Sun’s diameter.

Total Solar Eclipse Moon completely blocks Sun. The irregularly shaped halo around the Moon is the Sun’s corona.

Annular Solar Eclipse Moon moves completely in front of the Sun but does not cover the Sun.

Partial Solar Eclipse Moon only partially blocks Sun. Those out- side the path of a total or annular eclipse only see a partial eclipse.

Eclipses

Moon at Full Moon

1 2

Umbra Shadow

Penumbra

Penumbra

Sunlight

TOTAL LUNAR ECLIPSES occur when the Moon enters the Earth’s umbra shadow. The Moon does not turn completely dark during a total lunar eclipse, instead, it turns a pretty red-orange color. A lunar eclipse is visible to almost half of the world. PARTIAL LUNAR ECLIPSES occur when only part of the Moon enters the Earth’s umbra shadow. Partial lunar eclipses will show one edge of the Moon turning a slight orange color. PENUMBRAL LUNAR ECLIPSES occur when the Moon only enters the Earth’s penumbra shadow. Penumbral lunar eclipses may not be noticeable.

Solar & Lunar Eclipses

Moon at New Moon

Sunlight

UMBRA. The darkest part of the shadow where a total eclipse can only be seen. On Earth, the umbra can reach 170 miles (270 km) wide and travel one-third of the way around the world in a few hours. PENUMBRA. The secondary shadow where only a partial eclipse of the Sun will be seen. The penumbra is thousands of miles wide and straddles the path of the umbra on the Earth’s surface. Observers outside of the penumbra will not see the Sun eclipsed.

The umbra path for the total solar eclipse of August 21, 2017. The penumbra stretches for thousands of miles on both sides of the umbra.

Lunar Eclipses^ Eclipses

Total Solar Eclipses

Observing Solar Eclipses

During a solar

eclipse, the Moon’s

progress can be

viewed with a

telescope that is

properly fitted with

a solar filter. Please

see page 222 on

safely observing

the Sun for more

information.

There are novel

ways to view the

progress of solar

eclipses. My favorite is

using trees. If you look at a tree’s shadow (the tree must have

leaves) during a solar eclipse, you will notice that mixed in with

the shadow are hundreds of crescent Suns. A tree with leaves

creates a multitude of pinholes (like a pinhole camera) that project

the outline of the Sun. Some trees work better than others.

Partial and Annular Eclipses. Partial eclipses can last for

several hours. They are not noticeable unless a substantial portion

of the Sun is covered by the Moon. Even with half of the Sun

eclipsed, you may not notice any appreciable difference in sunlight.

To observe an annular solar eclipse, consult the local media,

internet or popular monthly astronomy magazines for the location

of the eclipse path. You cannot see the annular eclipse if you are

not in its path. It will not get dark during an annular eclipse and the

Moon will only be completely in front of the Sun for several minutes.

A solar or eclipse viewer/filter is needed to view the Sun during

the entire partial and annular eclipse.

Total Solar Eclipse & Totality. Remember, to see a total

solar eclipse, you must be on the eclipse path. Consult the local

media, internet or popular monthly astronomy magazines for details

and locations of the path.

A total solar eclipse will last for several hours and is treated

as a partial eclipse until the time of totality, that is, when the

Moon completely blocks the Sun’s light. During the one to five

The multitude of crescents in this picture are the eclipsed Sun, projected through pinholes formed from the interweaving of leaves on a tree.

Observing Lunar Eclipses

minutes of totality, no solar filter is required. Everyone stands

and stares in wonder. Many things happen during totality. The

sky darkens a little (it does not get completely dark), and almost

immediately, the white shimmering corona is seen surrounding

the Moon. Around the Moon’s edge, the thin red ring of the

chromosphere may be visible along with prominences and flares

protruding outward. If you look at the sky around the Moon, you

will probably see a few stars and Planets (usually Venus and

Mercury) and if you scan the whole sky, you will see the umbra

shadow circling the sky and extending almost to the horizon.

The sky near the horizon is still light but may have a red coloring

like that at sunset. The entire scene is incredible. There is noth-

ing like it! No camera can capture the experience of totality, and

everyone is touched differently. People clap, cheer, cry and pray.

I recommend that everyone experience a total solar eclipse!

OBSERVING LUNAR ECLIPSES

No special equipment or caution is necessary to view lunar

eclipses but binoculars and telescopes can be used to enhance

the event. Lunar eclipses are especially enjoyable when you can

sit outside, talk with others and casually watch the event unfold.

For the most part, the Moon will turn a dark red-orange when

it is completely in Earth’s umbra shadow. Various hues of red and

orange will slowly dance across the Moon’s surface as it enters,

passes through and exits the umbra. Since the umbra is consid-

erably larger than the Moon, total lunar eclipses can last up to

32 hours. If the Moon crosses the umbra dead center, it takes

about an hour to completely enter the umbra. It will stay in the

umbra for 1 2 hours and finish as it started, taking an hour to

leave.

Eclipses

Eclipses

2000 – 2050 Solar and Lunar Eclipse Tables for

North America on Pages 230–

The solar and lunar eclipse tables on the following pages

summarize the location and time of these events. Since the

intensity of the event and the exact time vary considerably

depending on your viewing location, please consult your local

media, the internet or the popular monthly astronomy

magazines for details. Enjoy.

Solar Eclipses in North America

SOLAR Eclipses 2000 – 2031

July 30, 2000 Partial Around Sunset Alaska , Western Canada, Northwest December 25, 2000 Partial Around Noon Midwest , Continental US, Southern Canada December 14, 2001 Partial Early to Hawaii , Continental US Late Afternoon June 10, 2002 Partial Late Afternoon West , Midwest, Hawaii, Alaska, West Canada May 30, 2003 Partial Around Sunset Alaska April 8, 2005 Partial Late Afternoon Florida , South, Southwest July 21, 2009 Partial Around Sunset Hawaii May 20, 2012 Annular Around Sunset West , Hawaii, Alaska, Western Canada May 9, 2013 Partial Late Afternoon Hawaii October 23, 2014 Partial Mid Afternoon West , Midwest, Alaska, Western Canada March 8, 2016 Partial Around Sunset Hawaii , Alaska August 21, 2017 Total Around Noon Across the US! Hawaii, Canada & Alaska June 10, 2021 Partial Early Morning Northeast , East October 14, 2023 Annular Late Morning West, Continental US, Canada April 8, 2024 Total Around Noon Midwest , Continental US, Canada, Hawaii October 2, 2024 Partial Early Morning Hawaii August 12, 2026 Partial Early to Late Alaska to Northeast Morning January 26, 2028 Partial Late Morning Florida , South, East, Midwest January 14, 2029 Partial Around Noon Canada , Continental US June 11, 2029 Partial Around Sunset Alaska , Canada, Northwest November 14, 2031 Partial Mid Afternoon Hawaii , Southwest, South, Florida

Date of Solar Eclipse

Time of Day to View^1

Type of Locations^2 Solar Eclipse

(^1) Check media sources for specific times for your location. (^2) First listed area is most favorable viewing location.

Solar Eclipses in North America

SOLAR Eclipses 2033 – 2051

March 30, 2033 Total Morning Alaska , Canada, Hawaii, West, Midwest September 1, 2035 Partial Around Sunset Hawaii August 21, 2036 Partial Morning Alaska January 5, 2038 Partial Early Morning East , Florida July 2, 2038 Partial Early Morning Florida , Southeast, East June 21, 2039 Annular Early Morning Alaska , Canada, Hawaii, West, Midwest November 4, 2040 Partial Around Noon East , Continental US, Canada October 24, 2041 Partial Late Afternoon Hawaii April 19, 2042 Partial Around Sunset Alaska , Northwest Canada, Hawaii April 9, 2043 Partial Around Noon Alaska , Western Canada, Hawaii, Northwest August 22, 2044 Total Around Sunset Northwest , Alaska, Canada, Hawaii, West February 16, 2045 Partial Late Afternoon Hawaii August 12, 2045 Total Around Noon South to West , Hawaii, Canada, Alaska February 5, 2046 Annular Mid Afternoon Hawaii , Alaska, West June 11, 2048 Annular Early Morning Northern Midwest/ Canada , East, South, Florida May 31, 2049 Partial Morning Florida November 14, 2050 Partial Early Morning East Canada , Northeast April 10, 2051 Partial Around Sunset Alaska , Northwest Canada

Date of Solar Eclipse

Time of Day to View^1

Type of Locations^2 Solar Eclipse

(^1) Check media sources for specific times for your location. (^2) First listed area is most favorable viewing location.

Eclipse Tables

Eclipse Tables

Lunar Eclipses in North America

LUNAR Eclipses 2044 – 2051

September 7, 2044 Total Before Sunrise Hawaii, Alaska, West July 17, 2046 Partial Early Evening East Coast January 11, 2047 Total Early Evening Continental US, Canada, Alaska July 7, 2047 Total Before Sunrise Hawaii, Alaska, West December 31, 2047 Total Around Midnight Hawaii, Alaska, Continental US, Canada June 25, 2048 Partial Around Midnight Midwest, East December 19, 2048 Penumbra Around Midnight Hawaii, Alaska, Continental US, Canada October 29, 2050 Total Evening Continental US, Canada, Alaska April 25, 2051 Total Early Evening Continental US, Canada

Date of Lunar Eclipse

Time of Day to View^1

Type of Locations Lunar Eclipse

(^1) Check media sources for specific times for your location.

Facing page. Beautiful shades of orange and brown dance across the Moon during total lunar eclipses.

Eclipse Tables