Lunar and Solar Eclipse Explained: A Beginner’s Guide to Eclipses

Science ABC
21 Apr 202007:26

Summary

TLDRThis script delves into the celestial mechanics behind solar and lunar eclipses. It explains Earth's elliptical orbit around the sun, which takes approximately 365 days, and the moon's roughly 27-day orbit around Earth. The script describes how solar eclipses occur when the moon blocks the sun, casting two types of shadows: the dark umbra and lighter penumbra. It outlines four types of solar eclipses, with the total solar eclipse being the most dramatic. Lunar eclipses, which happen when Earth comes between the sun and the moon, are also discussed, including total, partial, and penumbral lunar eclipses. The script concludes by highlighting the importance of safe viewing practices for solar eclipses and the historical and cultural significance of these celestial events.

Takeaways

  • 🌞 The sun may appear to partially or completely disappear due to solar eclipses, which occur when the moon passes between the Earth and the sun.
  • 🌍 Earth orbits the sun in an elliptical path, completing one revolution approximately every 365 days and 6 hours, which defines a year.
  • 🌕 The moon revolves around the Earth in about 27.322 days, and its relative size and distance make it appear the same size as the sun from Earth's perspective.
  • 🌑 A solar eclipse happens when the moon is positioned such that it blocks the sun's rays, casting a shadow on Earth.
  • 🌓 There are four types of solar eclipses: total, partial, annular, and hybrid (annular-total), depending on the moon's position relative to Earth.
  • 🌒 The moon casts two types of shadows on Earth during a solar eclipse: the umbra (dark) and the penumbra (lighter), affecting visibility of the eclipse.
  • 🌔 A total solar eclipse is the most dramatic, where the moon completely covers the sun, and can only be seen within the umbral shadow.
  • 🌕 An annular solar eclipse occurs when the moon's disk doesn't fully cover the sun, leaving a 'ring of fire' effect.
  • 🌜 Lunar eclipses occur when the Earth is positioned between the sun and the moon, casting its shadow on the moon.
  • 🌑 Lunar eclipses are of three types: total, partial, and penumbral, with the total lunar eclipse causing the moon to take on a reddish hue due to Earth's atmospheric refraction.
  • 👁️‍🗨️ Observing a solar eclipse without proper eye protection can lead to serious eye damage, unlike lunar eclipses, which are safe to view with the naked eye.

Q & A

  • Why does the sun sometimes partially or completely disappear from the sky?

    -The sun may partially or completely disappear from the sky due to a solar eclipse, which occurs when the moon moves between the sun and the Earth, blocking the sun's rays and casting a shadow on Earth.

  • What is the time Earth takes to complete one revolution around the sun?

    -Earth takes approximately 365 days and 6 hours to complete one revolution around the sun, which is roughly the length of one year.

  • Is Earth at the same spot in its orbit every year on a specific date?

    -Yes, since Earth takes the same amount of time to complete one revolution around the sun, it will be in the same spot every year on the same date.

  • How long does it take for the moon to complete one revolution around the Earth?

    -The moon takes about 27.322 days to complete one revolution around the Earth.

  • Why can the moon cover part or all of the sun despite being much smaller?

    -Although the moon is about 400 times smaller than the sun, it is also about 400 times closer to Earth, making both appear the same size in our sky.

  • What are the two types of shadows cast by the moon during a solar eclipse?

    -The two types of shadows cast by the moon during a solar eclipse are the Umbra, a small and very dark shadow, and the Penumbra, a larger and relatively lighter shadow.

  • What is the difference between a total solar eclipse and a partial solar eclipse?

    -A total solar eclipse occurs when the entire sun is completely blocked out by the moon, casting the Umbra on Earth. A partial solar eclipse happens when only a part of the sun is covered, casting the Penumbra.

  • What is an annular solar eclipse and how does it appear?

    -An annular solar eclipse occurs when the moon is not close enough to completely cover the sun, leaving the sun's outer edges visible, creating a 'ring of fire' appearance.

  • What is a hybrid solar eclipse and why is it rare?

    -A hybrid solar eclipse, also known as an annular-total solar eclipse, is when some parts of Earth witness an annular eclipse while others see a total eclipse. It is rare due to the delicate balance of the moon's position and Earth's curvature.

  • How often does the moon complete a revolution around the Earth and how does it appear to us?

    -The moon completes one revolution around the Earth in approximately 27 days. However, due to Earth's rotation and revolution around the sun, the moon appears to orbit us every 29 days.

  • What are the three types of lunar eclipses and how do they occur?

    -The three types of lunar eclipses are total, partial, and penumbral. They occur when the Earth is positioned between the sun and the moon, casting its shadow on the moon. A total lunar eclipse happens when the moon is fully within Earth's umbral shadow, a partial lunar eclipse when only part of the moon is in the umbral shadow, and a penumbral lunar eclipse when the moon passes through Earth's penumbral shadow.

  • Why is it dangerous to watch a solar eclipse without proper eye protection?

    -Watching a solar eclipse without proper eye protection is dangerous because the sun's radiation, including harmful ultraviolet rays, can damage the retina and cause permanent eye injuries.

Outlines

00:00

🌞 Understanding Solar Eclipses

This paragraph explains the phenomenon of solar eclipses, which occur when the moon passes between the Earth and the sun, casting a shadow on Earth. The moon's revolution around Earth, which takes approximately 27.322 days, is crucial for this event. The paragraph details the relative sizes and distances of the moon and sun, which appear the same size from Earth due to the moon's smaller size and closer proximity. It also describes the two types of shadows cast by the moon during an eclipse: the umbra, a small and very dark shadow, and the penumbra, a larger and lighter shadow. The paragraph further categorizes solar eclipses into four types: total, partial, annular, and the rare hybrid solar eclipse, each defined by the position of the moon relative to the sun and the resulting shadow on Earth.

05:04

🌑 Lunar Eclipses and Observation Safety

The second paragraph delves into lunar eclipses, which happen when the Earth is positioned between the sun and the moon. It discusses the three types of lunar eclipses: total, partial, and penumbral, each determined by the moon's position within Earth's shadow. A total lunar eclipse results in the moon taking on a 'sunset red' color due to the refraction of sunlight through Earth's atmosphere. The paragraph also emphasizes the safety of observing a lunar eclipse with the naked eye, contrasting it with the danger of viewing a solar eclipse without proper eye protection. It highlights the importance of using appropriate eye gear during a solar eclipse to prevent damage to the retina from the sun's intense radiation.

Mindmap

Keywords

💡Eclipse

An eclipse is a celestial event that occurs when one celestial body passes into the shadow of another, either partially or completely. In the context of the video, eclipses are the main theme, with a focus on solar and lunar eclipses. Solar eclipses happen when the moon blocks the sun, casting a shadow on Earth, while lunar eclipses occur when Earth's shadow falls on the moon. The video discusses different types of eclipses, such as total, partial, annular, and hybrid solar eclipses, as well as total, partial, and penumbral lunar eclipses.

💡Orbit

An orbit is the path that an object in space takes around another object due to gravity. In the video, Earth's orbit around the sun is mentioned as an elliptical path that it completes in approximately 365 days and 6 hours, which constitutes one year. The moon's orbit around Earth is also discussed, taking about 27.322 days to complete one revolution.

💡Solar Eclipse

A solar eclipse is an event where the moon passes between the sun and Earth, blocking the sun's light and casting a shadow on Earth. The video explains that a solar eclipse can be total, partial, annular, or hybrid, depending on the moon's position relative to the sun and Earth. This phenomenon is central to the video's discussion on celestial events.

💡Lunar Eclipse

A lunar eclipse occurs when the moon passes through Earth's shadow, which can be cast during a full moon when Earth is positioned between the sun and the moon. The video describes three types of lunar eclipses: total, partial, and penumbral, each with different visual effects on the moon's appearance.

💡Umbra

The umbra is the darkest and most central part of a shadow, where the light source is completely blocked. In the video, it is mentioned that during a solar eclipse, the moon's umbra can cover parts of Earth, leading to a total solar eclipse where the sun is completely obscured.

💡Penumbra

The penumbra is a lighter, outer part of a shadow where only some of the light source is blocked. In the context of the video, a penumbral lunar eclipse occurs when the moon passes through Earth's penumbral shadow, causing the moon to appear slightly darker.

💡Perigee

Perigee refers to the point in the moon's orbit when it is closest to Earth. The video explains that a total solar eclipse can only occur when the moon is near perigee, as this is when the moon's apparent size is large enough to completely cover the sun.

💡Path of Totality

The path of totality is the specific area on Earth's surface where a total solar eclipse is visible. The video mentions that this path is created by the moon's umbra as it moves across Earth during an eclipse, and observers within this path can witness the sun being completely blocked by the moon.

💡Annular Solar Eclipse

An annular solar eclipse is a type of solar eclipse where the moon is too far from Earth to completely cover the sun, leaving a ring of fire or an annulus visible around the moon. The video describes this as occurring when the moon's disk is not large enough to cover the entire sun.

💡Hybrid Solar Eclipse

A hybrid solar eclipse, also known as an annular-total solar eclipse, is a rare type of eclipse where different parts of Earth experience either an annular or total solar eclipse. The video explains that this happens due to the delicate balance of the moon's position relative to Earth and the sun.

💡Refraction

Refraction is the bending of light as it passes through different media, such as Earth's atmosphere. The video describes how refraction causes the moon to take on a reddish hue during a total lunar eclipse, as the shorter blue wavelengths of light are scattered while the longer red wavelengths are bent towards the moon.

Highlights

Earth travels around the sun in an elliptical orbit, completing one revolution in approximately 365 days and 6 hours.

The moon revolves around the Earth in about 27.322 days.

A solar eclipse occurs when the moon passes between the sun and the Earth, casting a shadow on Earth.

The moon appears the same size as the sun in our sky due to its relative distance and size.

The moon's shadow during a solar eclipse is limited to a certain area due to its small size compared to Earth.

There are two types of shadows cast during a solar eclipse: Umbra and Penumbra.

A total solar eclipse happens when the moon completely blocks the sun from a certain location on Earth.

A partial solar eclipse occurs when the moon only covers a part of the sun.

An annular solar eclipse happens when the moon's disk isn't big enough to cover the entire sun, leaving a ring of fire.

A hybrid solar eclipse is rare and appears as an annular eclipse in some areas and total in others.

A lunar eclipse occurs when the Earth comes between the sun and the moon.

Total lunar eclipses turn the moon a dramatic 'sunset red' due to Earth's atmospheric refraction.

Partial lunar eclipses are when only part of the moon passes through Earth's umbral shadow.

Penumbral lunar eclipses are subtle and may not be noticeable unless actively observed.

Lunar eclipses can be safely observed with the naked eye, unlike solar eclipses.

Viewing a solar eclipse without proper eye protection can cause permanent eye damage.

Solar and lunar eclipses are now celebrated by stargazers, a far cry from being considered bad omens.

Transcripts

play00:03

Why does the sun sometimes partially or even completely disappear from the sky for a few

play00:07

minutes?

play00:08

Let’s start with the basics.

play00:09

Earth, our home planet, is locked in an elliptical path around the sun.

play00:15

This elliptical path is known as the orbit of our planet.

play00:18

Earth travels around the sun along that orbit and completes one revolution in approximately

play00:22

365 days and 6 hours.

play00:25

As you may have noticed, this is roughly the length of one year.

play00:29

So, does that mean Earth is at exactly the same spot in its orbit every year on your

play00:34

birthday?

play00:35

Well, since it takes the same amount of time every year to complete one revolution around

play00:39

the sun, it’s only fair to assume that on your birthday, Earth will be in the exact

play00:43

same spot every year.

play00:44

We have actually answered that question in another video that you can watch by clicking

play00:48

on the 'i' button at the top right corner of the screen.

play00:52

Just as Earth moves around the sun in an elliptical orbit every year, our natural satellite—the

play00:57

moon—also revolves around the Earth.

play00:58

It takes about 27.322 days for the moon to complete one revolution around our planet.

play01:05

So, Earth revolves around the sun, and the moon revolves around Earth.

play01:09

Pretty neat, right?

play01:10

Due to all the inter-related motion happening between these three celestial bodies, several

play01:14

physical phenomena occur.

play01:16

When the new moon, during its revolution around the Earth, moves between the sun and the Earth,

play01:21

it blocks out the sun’s rays, which casts a shadow on parts of the planet.

play01:26

This is called an eclipse of the sun or a solar eclipse.

play01:30

In other words, a solar eclipse happens when the moon passes in a direct line between the

play01:34

sun and the Earth.

play01:36

Now, you may be thinking that the moon is infinitesimally small compared to the sun,

play01:40

so why is it ever able to cover part of or sometimes even the entire sun?

play01:44

Although the moon is indeed about 400 times smaller than the sun, it also happens to be

play01:49

around 400 times closer to us than the sun.

play01:52

This is why both the moon and the sun appear to be the same size in our sky.

play01:56

The moon is very small compared to the sun and to Earth, which is why the moon’s shadow

play02:00

isn’t big enough to engulf our entire planet.

play02:03

Therefore, the moon’s shadow is always limited to a certain area.

play02:07

This area changes even DURING an eclipse, as both the celestial bodies are in constant

play02:11

motion with respect to one another.

play02:13

When the moon eclipses the sun, it casts two types of shadows on Earth: the first is the

play02:18

Umbra, which is a small and very dark shadow.

play02:20

If you’re in a place on Earth where Umbra is cast, the entire central portion of the

play02:24

sun will be blocked out from your perspective.

play02:26

The second type of shadow is known as the penumbra; it is a larger and relatively ‘lighter’

play02:31

shadow than the umbra.

play02:32

If the penumbra passes over you, then only a small part of the sun will be blocked out

play02:36

from your point of view.

play02:37

Depending on the type of shadow the moon casts on Earth, solar eclipses are broadly classified

play02:41

into four types:

play02:43

The first is a total solar eclipse.

play02:45

This is the most spectacular of all eclipses because, during a total solar eclipse, the

play02:50

entire sun is completely blocked out by the moon.

play02:52

This can only happen when the moon is near perigee, the point of the moon’s orbit when

play02:56

it is closest to the Earth.

play02:58

You can only see a total solar eclipse if you’re standing within the umbral shadow.

play03:01

Since the Earth keeps rotating, the umbral shadow doesn’t stay at one point on Earth—it

play03:05

keeps moving too!

play03:07

The imaginary line created by the umbral shadow is known as the path of totality.

play03:11

If you’re in any of the places through which this imaginary line passes, you can see when

play03:15

the sun gets completely blocked out by the moon.

play03:20

Next up is a partial solar eclipse.

play03:23

This type of eclipse is observed when the moon covers only a part of the sun and casts

play03:27

a penumbra on Earth.

play03:29

Since it only covers a part of the sun, this phenomena is known as a partial solar eclipse.

play03:35

When the moon passes through the center of the sun, but its disk isn’t big enough to

play03:38

cover the entire disk of the sun, then an annular solar eclipse occurs.

play03:43

When this happens, the sun’s outer edges remain visible, making it look like a shiny,

play03:47

fiery ring in the sky.

play03:49

Unlike a total eclipse, during an annular eclipse, the moon doesn’t completely block

play03:53

out the sun.

play03:55

The fourth type of eclipse is the rarest of all; when the moon’s position between the

play03:59

sun and the Earth is so delicately balanced that Earth’s curvature plays a role, we

play04:04

call it a hybrid solar eclipse.

play04:06

During this type of eclipse, some parts of the Earth witness an annular solar eclipse,

play04:10

while other parts see a total solar eclipse.

play04:13

For that reason, this type of eclipse is also known as an annular-total solar eclipse.

play04:18

Since the moon continually revolves around the Earth, it’s only natural that it sometimes

play04:22

comes between the sun and the Earth, while at other times it goes BEHIND the Earth, so

play04:26

that the Earth comes between the moon and the sun.

play04:29

When the latter happens, we see a lunar eclipse.

play04:31

The moon completes one revolution around our planet in approximately 27 days and rotates

play04:36

at the same rate as it revolves around the Earth; however, since the Earth rotates on

play04:40

its axis and also moves in its own orbit around the sun, from our perspective, the moon appears

play04:45

to orbit us every 29 days.

play04:48

Earth casts two types of shadows on the moon—umbra and penumbra—when it is oriented between

play04:53

the sun and the moon.

play04:55

Lunar eclipses can be divided into three types, the first being a total lunar eclipse.

play04:59

The most picturesque and dramatic of all, a total lunar eclipse happens when the moon,

play05:04

Earth and the sun are perfectly aligned so that the moon falls under the umbral shadow

play05:08

of our planet.

play05:10

During a total eclipse, Earth completely blocks any sunlight from reaching the moon.

play05:14

Due to this, the moon loses its characteristic whitish-grey color and becomes a ‘sunset

play05:19

red’.

play05:20

This happens due to refraction from the Earth’s atmosphere.

play05:22

The shorter, blue wavelengths of sunlight are scattered outward by the atmosphere, whie

play05:26

the longer red wavelengths are refracted inward toward the moon, giing it a reddish tinge

play05:31

during a total lunar eclipse.

play05:34

Next is a partial lunar eclipse, which happens when the moon, Earth and sun align in such

play05:38

a way that only PART of the moon passes through the umbral shadow cast by the Earth.

play05:42

During a partial eclipse, you can see Earth’s shadow covering a small part of the moon’s

play05:47

surface.

play05:48

Then there’s a penumbral lunar eclipse.

play05:50

As the name suggests, you can see this type of eclipse when the moon passes through Earth’s

play05:53

penumbral shadow.

play05:55

This celestial event is so subtle that many of us don’t even notice it visually, as

play05:59

the moon appears only slightly darker than its usual hue.

play06:02

So, unless you are ACTIVELY LOOKING to observe the penumbral eclipse, it can be very easy

play06:06

to miss.

play06:09

You can watch a lunar eclipse if you’re on the nighttime-side of Earth, and for those

play06:12

who were wondering, it’s safe to watch a lunar eclipse with the naked eye.

play06:15

In contrast, it’s highly dangerous to watch a solar eclipse with the naked eye.

play06:20

Observing a solar eclipse without appropriate precautions can potentially cause permanent

play06:23

eye injuries.

play06:25

The light from the sun that reaches the Earth consists of a broad range of radiation, from

play06:29

ultraviolet radiation at wavelengths longer than 290 nanometers all the way to radio waves

play06:34

existing in the meter range.

play06:36

The tissues in our eyes transmit a considerable portion of this radiation to the back of the

play06:39

eye—the light-sensitive retina.

play06:42

This can result in damage to the light-sensitive rod and cone cells in the eye.

play06:45

Basically, just make sure that you’re wearing appropriate eye gear when you observe this

play06:49

spectacular cosmic phenomenon.

play06:51

Solar and lunar eclipses bring millions of stargazers out into the streets every year;

play06:55

they unite people in a remarkable cosmic way.

play06:58

Given that the same celestial events used to strike fear in the hearts of people and

play07:02

were considered bad omens, humanity has certainly come a long way when it comes to understanding

play07:06

the forces of nature!

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