Ch01 Lecture part3 video

Gabe Prochter
20 Apr 202023:01

Summary

TLDRThis lecture delves into the celestial mechanics of the Moon, explaining its phases and movement across the sky due to Earth's rotation and the Moon's orbit. It explores the waxing and waning cycles, the Moon's different phases, and the rare occurrences of solar and lunar eclipses. The presentation also touches on the Earth's atmospheric effects during eclipses, causing the red hue of a lunar eclipse and the visibility of the Sun's corona during a solar eclipse. The lecture concludes with insights into predicting eclipse seasons based on the orbits of the Earth and Moon.

Takeaways

  • πŸŒ“ The Moon has different phases due to the relative positions of the Earth, Moon, and Sun, which affect how much of the Moon is illuminated and visible from Earth.
  • πŸŒ… The Moon rises in the east and sets in the west, following the Earth's rotation and its own orbit around the Earth.
  • πŸŒ‘ A new moon is when the Moon is not visible from Earth because the side facing us is not illuminated by the Sun.
  • πŸŒ’ Waxing phases include the crescent and gibbous phases, where the visible portion of the illuminated Moon increases from new to full moon.
  • πŸŒ• A full moon occurs when the entire face of the Moon is lit up and visible, which happens when the Moon is on the opposite side of the Earth from the Sun.
  • πŸŒ— Waning phases are when the illuminated portion of the Moon decreases from full to new moon, including the waning gibbous and crescent phases.
  • πŸ•’ The Moon's orbit around the Earth takes about 27.3 days, but a full lunar cycle (from new moon to new moon) takes about 29.5 days due to the Earth's movement around the Sun.
  • 🌞 Solar eclipses occur when the Moon's orbit aligns with the Earth's orbit around the Sun, casting a shadow on the Earth.
  • 🌜 Lunar eclipses happen when the Earth's shadow falls on the Moon, which can give the Moon a reddish hue due to the scattering of light by the Earth's atmosphere.
  • πŸ”­ The Earth's atmosphere bends red light towards the Moon during a lunar eclipse, causing it to appear red, which is a result of all the sunrises and sunsets on Earth being projected onto the Moon.
  • β˜€οΈ The visibility of the Moon and the occurrence of eclipses can be predicted based on the understanding of the Earth's and Moon's orbits, with eclipse seasons where solar and lunar eclipses are likely to happen.

Q & A

  • Why does the Moon appear to rise in the east and set in the west?

    -The Moon appears to rise in the east and set in the west due to the Earth's rotation on its axis. This is similar to how the Sun and stars move across the sky from east to west.

  • What causes the different phases of the Moon?

    -The different phases of the Moon are caused by the changing angles between the Earth, the Moon, and the Sun. As the Moon orbits the Earth, different portions of the Moon's surface are illuminated by the Sun, resulting in various visible phases.

  • What is the term used for the phase when the Moon is not visible from Earth?

    -The phase when the Moon is not visible from Earth is called the 'new moon.'

  • How is the waxing crescent phase of the Moon different from the waning crescent phase?

    -The waxing crescent phase occurs between the new moon and the first quarter, where the visible portion of the Moon is increasing. The waning crescent phase occurs between the third quarter and the new moon, where the visible portion is decreasing.

  • What is the term for the phase when half of the Moon is illuminated as seen from Earth?

    -When half of the Moon is illuminated as seen from Earth, it is called the 'first quarter' or 'last quarter' phase.

  • Why does the Moon's rise time change each day?

    -The Moon's rise time changes each day because the Moon orbits the Earth approximately 50 minutes later each day due to the Earth's rotation and the Moon's orbit around the Earth.

  • What is the difference between a sidereal month and a synodic month?

    -A sidereal month is the time it takes for the Moon to orbit the Earth once, which is about 27.3 days. A synodic month is the time it takes for the Moon to go through one full cycle of phases, from new moon back to new moon, which is about 29.5 days.

  • What causes a solar eclipse?

    -A solar eclipse occurs when the Moon is positioned directly between the Earth and the Sun, casting its shadow on the Earth and blocking the Sun's light.

  • What causes a lunar eclipse?

    -A lunar eclipse occurs when the Earth is positioned directly between the Sun and the Moon, casting the Earth's shadow on the Moon.

  • Why does the Moon appear red during a lunar eclipse?

    -During a lunar eclipse, the Moon appears red because the Earth's atmosphere scatters shorter wavelength light (blue light), while longer wavelength light (red light) bends around the Earth and reaches the Moon, giving it a reddish hue.

  • How can the occurrence of solar and lunar eclipses be predicted?

    -The occurrence of solar and lunar eclipses can be predicted by understanding the orbits of the Earth around the Sun and the Moon around the Earth. The alignment of these orbits at certain periods allows for the prediction of eclipse seasons.

Outlines

00:00

πŸŒ• Introduction to Moon Phases and Movements

The paragraph introduces the concept of the moon's movements in the sky, explaining how the moon rises in the east and sets in the west due to Earth's rotation. It discusses the moon's phases, starting from a new moon where the moon is not visible, progressing through the waxing crescent, first quarter, waxing gibbous, full moon, waning gibbous, third quarter, and back to new moon. These phases result from the moon's position relative to Earth and the Sun, with specific terms like 'waxing' indicating increasing visibility and 'waning' indicating decreasing visibility.

05:00

πŸŒ— Moon Phases and Timing

This paragraph details how the moon's phases relate to its position in its orbit around Earth. It explains how the moon appears at different times of the day depending on its phase, such as the third quarter being visible in the morning and the first quarter in the afternoon or evening. The paragraph also mentions that the moon rises about 50 minutes later each day due to its orbit around Earth. Additionally, it touches on the phenomenon of eclipses, where the Earth's or Moon's shadow may block out the other, depending on the alignment.

10:03

πŸŒ’ Eclipses: Solar and Lunar Explained

The paragraph provides an explanation of solar and lunar eclipses. A solar eclipse occurs when the moon blocks the Sun's light from reaching Earth, and a lunar eclipse occurs when Earth's shadow falls on the moon. The paragraph explains that these events are rare due to the tilt in the orbits of the moon around Earth and Earth around the Sun. The moon's shadow during a solar eclipse only covers a small area on Earth, while Earth's shadow during a lunar eclipse can cover the entire moon. The paragraph also introduces the terms 'umbra' and 'penumbra' to describe the types of shadows cast during these eclipses.

15:03

πŸŒ‘ The Solar and Lunar Eclipse Phenomena

This paragraph delves deeper into the specifics of solar and lunar eclipses, describing how a solar eclipse progresses from partial to total coverage of the Sun by the moon, revealing the Sun's corona. It also explains the lunar eclipse phenomenon, where the moon appears red due to Earth's atmosphere bending red light while scattering blue light, a phenomenon linked to the scattering of light during sunrise and sunset. The paragraph emphasizes that these eclipses occur rarely due to the specific alignments required, with solar and lunar eclipses often occurring in close succession.

20:06

🌘 Predicting Eclipse Seasons

The final paragraph discusses the predictability of eclipses, referring to 'eclipse seasons' where solar and lunar eclipses happen within a short period. The predictability is based on the understanding of Earth's and the moon's orbits. The paragraph provides examples of past and future eclipses, mentioning the notable solar eclipse of 2017 and upcoming eclipses in 2024 and beyond. The conclusion encourages anticipation of future lectures related to celestial movements.

Mindmap

Keywords

πŸ’‘Moon

The Moon is Earth's natural satellite, which plays a central role in the video's discussion of celestial mechanics. It is defined as a celestial body that orbits a planet, and in this video, it is used to explain the concept of lunar phases and its movement in the sky, including its rise in the east and set in the west.

πŸ’‘Phases of the Moon

The phases of the Moon refer to the changing appearance of the illuminated portion of the Moon as viewed from Earth. The video explains the different phases, from new moon to full moon, and how they occur due to the relative positions of the Earth, Moon, and Sun. The script uses terms like 'waxing crescent' and 'waning gibbous' to describe these phases.

πŸ’‘Orbit

Orbit is the path that an object in space takes around another object due to gravity. In the context of the video, the Moon's orbit around the Earth and the Earth's orbit around the Sun are key to understanding the changing positions and appearances of these celestial bodies. The script mentions how the Moon's orbit leads to different rise and set times.

πŸ’‘Eclipse

An eclipse is an astronomical event that occurs when one celestial body moves into the shadow of another. The video discusses two types of eclipses: solar and lunar. A solar eclipse happens when the Moon passes between the Earth and the Sun, casting a shadow on Earth, while a lunar eclipse occurs when the Earth is between the Sun and the Moon, casting a shadow on the Moon. The script provides examples of how and when these events occur.

πŸ’‘Solar Eclipse

A solar eclipse is a type of eclipse that happens when the Moon moves between the Sun and Earth, blocking the Sun's light either partially or completely. The video describes the experience of a solar eclipse, mentioning the 'diamond ring' effect and the visibility of the Sun's corona, as well as the conditions required for this event to occur.

πŸ’‘Lunar Eclipse

A lunar eclipse occurs when the Earth is positioned between the Sun and the Moon, casting its shadow on the Moon. The video explains that during a lunar eclipse, the Moon can take on a reddish hue, often referred to as a 'blood moon,' due to the scattering of light by the Earth's atmosphere. The script provides the phenomenon's cause and effect.

πŸ’‘Atmosphere

The atmosphere is a layer of gases surrounding a planet that is held in place by gravity. The video discusses the Earth's atmosphere and its role in the color changes observed during lunar eclipses and at sunrises and sunsets. It explains how the scattering of blue light and the bending of red light affect the appearance of celestial bodies.

πŸ’‘Waxing and Waning

Waxing and waning describe the increase and decrease in the visible illuminated portion of the Moon, respectively. The video uses these terms to describe the progression of the lunar phases, from new moon to full moon and back to new moon. Waxing indicates the growth of the visible illuminated portion, while waning indicates its reduction.

πŸ’‘Crescent

A crescent refers to the thin, curved shape of the illuminated portion of the Moon during its first and last quarter phases. The video mentions 'waxing crescent' to describe the phase where the illuminated portion is increasing, and 'waning crescent' for when it is decreasing.

πŸ’‘Gibbous

Gibbous is used to describe a phase of the Moon where more than half of the Moon's surface is illuminated but not the entire disk. The video distinguishes between 'waxing gibbous,' where the illuminated portion is increasing towards a full moon, and 'waning gibbous,' where it is decreasing after a full moon.

πŸ’‘Umbra and Penumbra

Umbra and penumbra are terms used to describe parts of a shadow. The video explains that during a solar eclipse, the umbra is the dark central shadow where the Sun is completely obscured, while the penumbra is the lighter outer shadow where only part of the Sun is obscured. These terms help illustrate the varying degrees of eclipse visibility.

Highlights

The Moon rises in the east and sets in the west due to Earth's rotation on its axis.

The Moon's phases change as it orbits the Earth, with the full moon being completely lit up and the new moon not visible.

The waxing and waning phases of the Moon are explained by the varying amounts of the Moon's surface illuminated by the Sun.

The Moon's orbit around the Earth and Earth's orbit around the Sun result in different rise and set times for the Moon.

The Moon's orbit is slightly tilted relative to Earth's orbit around the Sun, causing infrequent eclipses.

A lunar eclipse occurs when the Earth's shadow falls on the Moon, and a solar eclipse when the Moon blocks the Sun.

The duration of a lunar month is approximately 29.5 days, which is longer than the Moon's sidereal month due to Earth's movement around the Sun.

The phenomenon of the Moon's phases can be observed by the time of day the Moon is visible and its position in the sky.

The Earth's atmosphere scatters blue light, causing the sky to appear blue during the day and the Sun to appear red during sunrise and sunset.

During a lunar eclipse, the Moon takes on a reddish hue due to the Earth's atmosphere bending red light towards the Moon.

Eclipse seasons, where solar and lunar eclipses occur close together in time, can be predicted based on the orbits of the Earth and Moon.

A solar eclipse is visible only in a narrow path on Earth, with the rest of the planet experiencing a partial eclipse or no eclipse at all.

The 'diamond ring' effect is observed during a solar eclipse when the last rays of the Sun peek through valleys on the Moon's surface.

The Sun's corona is visible during a total solar eclipse, revealing the Sun's atmosphere.

The occurrence of eclipses is rare due to the specific alignment needed between the Earth, Moon, and Sun.

Historical and future dates of solar and lunar eclipses are charted, showing the predictability of these celestial events.

The upcoming solar eclipse on April 8th, 2024, will be visible from Mexico through Texas and the eastern United States.

The lecture series will continue to explore the movement of celestial bodies and our understanding of their motion.

Transcripts

play00:00

hello everyone welcome to part three of

play00:03

our first lecture today now we're to

play00:07

talk about the moon the last part of

play00:11

what we see the sky

play00:14

changing over time now our Moon the moon

play00:19

it does rise in the set or rise in the

play00:23

east and sets in the west

play00:28

now just like everything else this has

play00:32

to do with the fact that the Earth spins

play00:34

on its axis but just like the planets

play00:38

the Sun and the stars okay you're gonna

play00:42

see the moon move from the east to the

play00:45

west in the night or the daytime sky

play00:49

nighttime sky depending on what time of

play00:51

day it or what time of the month it is

play00:56

but how does this actually work the moon

play01:01

when you look at it you will notice that

play01:04

it has different phases so sometimes it

play01:08

looks like this where you can see the

play01:10

whole moon lit up other times not so

play01:14

much why well these phases how much of

play01:20

the moon you see lit up

play01:22

well it goes from we call new which

play01:26

means that you can't see the moon at all

play01:31

back to new or you can't see them there

play01:34

at all but in between you can see

play01:38

different amounts of the moon lit up

play01:46

different amounts the moon lit up to

play01:49

where you have a full moon where you can

play01:52

see the entire moon that faces us you

play01:57

can see the whole thing lit up now we

play02:02

call this new when you can't see it at

play02:05

all

play02:07

up through the first quarter we can you

play02:10

see a quarter of the moon lit up

play02:12

that is called the waxing crescent phase

play02:16

of the moon from first quarter to full

play02:20

we call that waxing gibbous but once

play02:26

it's full we start seeing less and let

play02:28

it less less less and less of it lit up

play02:31

we call that waxing gibbous or waning

play02:35

gibbous so waning means less and less

play02:38

waxing means more and more and then you

play02:42

go from third quarter back to new again

play02:46

waning we call that waning crescent so

play02:53

why do we have these phases well it has

play02:56

to do with where we are relative to the

play03:00

Sun and where the moon is relative to us

play03:04

so if you are here on the planet and you

play03:13

are the sun's over here to the left you

play03:18

are this is clearly noon

play03:21

right because you are looking at the Sun

play03:24

well if the moon happens to be here the

play03:31

side of the Moon that you can see this

play03:34

side of the moon

play03:35

well that side of the Moon is in

play03:37

darkness it's not lit up the side of the

play03:41

moon it's lit up by the Sun is facing

play03:44

away from us and that would be a new

play03:47

moon now about a week later you're gonna

play03:53

be here or the moon is gonna be here as

play03:57

it goes around the earth because of

play03:59

orbits around the earth in this

play04:00

direction so one week later the moon

play04:03

would be here if you're standing on the

play04:06

earth and you happen to be right here on

play04:07

the earth first of all because the Earth

play04:10

spins this direction if you're here on

play04:15

the earth that is gonna be sunset but if

play04:19

you're looking up and you see the moon

play04:22

if the moon happens to be here

play04:25

well the left-hand side of the moon is

play04:28

lit up by a Sun you're gonna see the

play04:31

left-hand side lit by the Sun it's gonna

play04:34

be first quarter the right-hand side of

play04:37

the Moon is facing space so it's dark on

play04:43

the other hand if you wait a while the

play04:47

moon eventually goes around the earth

play04:50

it's gonna be here at full if you're

play04:54

here on the earth it's midnight but if

play05:00

you're looking at the Sun at the moon

play05:01

the moon the side of the Moon you can

play05:04

see is fully lit up that's a full moon

play05:12

if the moon a week after that the moon's

play05:18

gonna be here if you're here on the

play05:22

earth first of all because there's the

play05:25

spinning that is a round sunrise

play05:33

looking at the moon and the moon happens

play05:35

to be up here it's gonna be third

play05:39

quarter and if you look at the moon its

play05:45

third quarter you will notice the

play05:48

left-hand side is lit up if you're here

play05:53

on the earth and the moon happen is the

play05:55

first quarter okay you're looking down

play05:59

at the moon it's the right hand side is

play06:01

lit up so you can tell what phase the

play06:04

moon is in just like looking at it and

play06:07

by knowing what time of day it is when

play06:10

you can see it okay if you see the moon

play06:13

at night if you're here at night you're

play06:17

looking at the moon if it's mostly full

play06:20

or close to full or just after full

play06:24

you're only gonna see it at night okay

play06:27

the third quarter moon you're gonna see

play06:29

in the morning first quarter moon you're

play06:32

gonna see in the afternoon or evening

play06:37

all right

play06:39

now the moon because the earth orbits

play06:42

around the Sun and the moon orbits

play06:44

around the earth you're gonna have

play06:47

different rise time and set times

play06:49

depending on where the moon is as it

play06:53

orbits around the earth it's about 50

play06:57

minutes later each day so if you see the

play07:01

moon rise today tomorrow the moon is

play07:05

gonna rise 50 minutes and later alright

play07:10

that just has to do with the fact that

play07:12

the Earth or the moon orbits around the

play07:14

earth and the Earth orbits around the

play07:16

Sun now there will be times when the

play07:21

moon's orbit around the Earth and the

play07:26

Earth's orbit around the Sun coincide

play07:30

which to say that the moon will

play07:32

occasionally block out the Sun and the

play07:37

earth will occasionally block out the

play07:41

moon by which I mean the Earth's shadow

play07:44

will cast onto the moon such that the

play07:48

moon is not lit up by the the Sun now

play07:53

this only happens very very infrequently

play08:00

the Earth's orbit around the Sun and the

play08:05

moon's orbit around the Earth are

play08:08

slightly tilted relative to each other

play08:11

so you don't have overlap all of the

play08:15

time now one thing to note the Earth's

play08:22

orbit around the Sun that takes a year

play08:28

the moon's orbit around the Earth takes

play08:34

twenty three or twenty seven point three

play08:36

days that is not how long it takes for

play08:41

the moon to go through one full cycle so

play08:43

for a full cycle what I mean is from

play08:47

like a new moon through

play08:52

a first quarter through full moon

play08:57

through third quarter and back to new

play09:01

so from new all the way back to new

play09:04

actually takes twenty nine point five

play09:08

days twenty nine and a half days

play09:12

why is it different well the moon goes

play09:16

once around the earth every 27 days

play09:19

twenty seven point three days but if the

play09:24

Earth or the moon goes once around the

play09:27

earth keep in mind in one month the

play09:31

earth has moved around the Sun because

play09:35

the Earth orbits around the Sun so when

play09:39

the moon goes fully around the earth

play09:42

once well it will be here but that this

play09:49

position that is not full because the

play09:52

moon is not directly between the Earth

play09:55

and the Sun for the moon to get full it

play09:58

has to go a couple of days further to

play10:03

get here which is why it takes a little

play10:07

bit longer for a full cycle of the moon

play10:11

so from new back to new or full back to

play10:17

full as opposed to how long it takes the

play10:20

moon to go once around the earth this is

play10:23

called acid aerial month you should note

play10:26

the same thing happens with the earth

play10:28

and days so you guys think about the

play10:33

earth have spinning around once on its

play10:35

axis as being 24 hours it's actually not

play10:41

it's actually 23 hours and 56 minutes it

play10:46

takes the earth to spend once on this

play10:47

axis but a day is 24 hours it's the same

play10:52

kind of thing

play10:54

it's d real day as opposed to actual day

play10:58

is different than a well it's the same

play11:03

thing as a stereo month as opposed

play11:06

- an actual month all right now every

play11:12

once in a while as I said the moon the

play11:16

earth and the Sun will line up such that

play11:20

the moon casts a shadow on the earth or

play11:25

if the moon is over here the earth can

play11:34

cast a shadow on the moon now if the

play11:41

moon blocks out the Sun we call that a

play11:43

solar eclipse if the Earth's shadow hits

play11:49

the moon we call that a lunar eclipse

play11:51

but it only happens every once in a

play11:54

while because remember the moon's tilt

play11:57

as it orbits the earth is different than

play12:01

the earth's tilt as it orbits the Sun

play12:04

which means only every once in a while

play12:07

does the moon actually cast a shadow on

play12:09

the earth or vice versa

play12:13

now if the moon casts a shadow on the

play12:16

earth it looks like this this is the

play12:19

moon shadow on the earth it only hits a

play12:22

small spot on the earth if the Earth's

play12:25

shadow hits the moon the whole moon can

play12:28

be covered but that's just because

play12:30

remember the moon is smaller than the

play12:33

earth it casts a smaller shadow so the

play12:38

moon shadow only covers a little part of

play12:41

the earth and what's going on is that

play12:46

the moon is exactly aligned such that

play12:51

shadow hits the earth now usually the

play12:55

moon will be like up here and the shadow

play12:57

doesn't hit the earth or I'll be down

play13:00

here the shadow doesn't hit the earth

play13:02

only every once in a while does the

play13:04

moon's orbit around the earth coincide

play13:08

with the Earth's orbit around the Sun

play13:11

such that the moon's shadow is actually

play13:14

hitting the earth but when that happens

play13:18

and you get the

play13:20

shadow on the earth and you see a solar

play13:25

eclipse the Sun is blotted out by the

play13:28

sky because the moon is in front of it

play13:32

now you can only see it if you happen to

play13:35

be right here in the middle okay if

play13:39

you're out here on the earth you're not

play13:41

going to see any kind of shadow at all

play13:44

you're not gonna see in eclipse at all

play13:46

if you're here which is in what's known

play13:50

as the penumbra the penumbra of the

play13:54

shadow is where you can see part of this

play13:58

the Sun blotted out by the moon but only

play14:00

part so only part of the Sun is blotted

play14:03

out if you're in the middle it's called

play14:06

the Umbra of the shadow and you're in

play14:09

complete shadow the whole Sun is if you

play14:15

were to watch this you would see the

play14:18

moon the Sun start to move in front of

play14:21

the moon or the moon start to move in

play14:24

front of the Sun sorry and eventually

play14:26

you would get most the Sun blotted out

play14:30

almost all the Sun bought it out and

play14:33

then the entire Sun blotted out and what

play14:36

you see when the entire Sun has blotted

play14:38

out is this which is the atmosphere we

play14:43

will talk about this later on in this

play14:45

class about the atmosphere of the Sun

play14:47

that is known as the Sun's corona and

play14:52

then when the Sun starts to or the moon

play14:56

starts to leave start starts to stop

play15:00

blocking out the Sun the very first

play15:03

thing that happens is you will see a

play15:05

little bit of the Sun lit up that's

play15:08

often known as the diamond ring if you

play15:11

ever get a chance to see a solar eclipse

play15:15

I highly recommend it it is actually

play15:18

pretty amazing in the sky

play15:20

it's the only time only time you could

play15:24

ever see the sun's atmosphere now

play15:30

you will also get times when the moon is

play15:34

in the Earth's shadow okay we call that

play15:37

a lunar eclipse when the moon goes into

play15:41

the earth shadows something weird

play15:43

happens though it doesn't go dark it

play15:46

actually becomes bright red it's like

play15:51

weird dull red color that is often

play15:55

called a blood mmm because it is so red

play16:00

now why is red why is it not just like

play16:05

disappear because it's in the earth

play16:07

shadow well that actually has to do with

play16:10

the atmosphere of the earth so what's

play16:14

going on here is that light from the Sun

play16:18

hits the Earth's atmosphere here and red

play16:25

light gets bent by the atmosphere so red

play16:28

light coming through the Earth's

play16:30

atmosphere it's bent towards the moon

play16:35

whereas blue light blue light gets

play16:38

scattered blue light is scattered by our

play16:41

atmosphere which is why during the day

play16:44

the sky looks blue blue lights getting

play16:47

bounced around in our atmosphere at

play16:49

random directions and so if you're on

play16:52

the earth looking at the Sun if you're

play16:54

like here on the earth looking at the

play16:57

Sun okay all around you you're gonna see

play17:01

atmosphere and that atmosphere is gonna

play17:06

look blue because blue light is

play17:07

scattered red light is not scattered red

play17:10

light goes through the atmosphere but it

play17:13

is bent so this is why at like in the

play17:17

evening or in the morning like say

play17:20

you're here this is the morning you're

play17:24

looking towards the Sun the Sun is

play17:28

rising but the Sun has to go through the

play17:31

sun's light has to go through a lot of

play17:33

atmosphere here before you can see it

play17:37

and because of that the blue light is

play17:40

getting scattered out by the atmosphere

play17:42

and the Sun is going to

play17:44

renner because blue lights bein

play17:46

scattered out now when you're here on

play17:50

the earth and it's noon

play17:52

you're not looking through nearly as

play17:55

much atmosphere and the Sun schooling a

play17:58

Sun you're here in the evening again

play18:01

you're looking through a lot of

play18:03

atmosphere at the Sun and blue lights

play18:06

being scattered out so the Sun looks

play18:08

redder that's why we have red Sun rises

play18:11

and Sun Sun Sun sets it has to do with a

play18:14

scattering of blue blue light but red

play18:18

light it gets through it's not scattered

play18:22

it's through the atmosphere which is why

play18:25

the Sun looks kind of reddish during

play18:27

this sunrise and sunset but it's that

play18:30

same red light that goes through our

play18:32

atmosphere and gets bent it's tilted a

play18:37

little bit and it gets projected onto

play18:39

the moon during a solar eclipse or doing

play18:42

it during a lunar eclipse oh sorry so

play18:44

during a lunar eclipse the red light

play18:46

going through the Earth's atmosphere

play18:49

it's tilted and projected onto the moon

play18:52

so when you see a lunar eclipse and

play18:56

looks red what you're literally seen

play18:58

literally is all the sunrises and

play19:02

sunsets on the earth projected onto the

play19:05

moon so these kinds of eclipses happen

play19:10

rarely because usually the moon will be

play19:13

like here and the moon shadow doesn't

play19:16

hit the earth where the the moon will be

play19:19

here like a full moon but the Earth's

play19:22

shadow does not hit it only every once

play19:27

in a while will the the moon shadow

play19:31

align right such that it hits the earth

play19:34

or the Earth's shadow will align just

play19:37

right and will hit the moon usually you

play19:41

will find these happen coincidentally

play19:47

which is to say that you have Eclipse

play19:50

seasons so if if you have a solar

play19:54

eclipse you're probably gonna have a

play19:56

lunar

play19:57

it's a couple of months later a so for

play20:02

example you know solar eclipse September

play20:06

13th

play20:06

lunar eclipse September 28th okay two

play20:10

weeks later so you have what I call the

play20:15

clip seasons and you can predict these

play20:16

things you can predict win exactly these

play20:19

eclipses are going to happen once you

play20:21

understand the Earth's orbit around the

play20:23

Sun and the moon's orbit around the

play20:26

Earth if you understand how those things

play20:28

work you can predict when this is gonna

play20:30

happen okay

play20:34

so again usually the moon shadow doesn't

play20:39

hit the earth and the Earth's shadow

play20:42

does not hit the moon every once in a

play20:47

while though when things line up just

play20:51

right okay the moon will be here and it

play20:59

casts a shadow on the earth or the moon

play21:02

be here and the earth will cast a shadow

play21:04

on it only every once in a while but

play21:09

again you can predict these things

play21:11

because we understand the Earth's orbit

play21:14

around the Sun and we understand the

play21:17

moon's orbit around the Earth we can

play21:19

predict these things what happen okay so

play21:22

here is a chart of when these things

play21:25

will happen in the past in the future in

play21:30

2004 or 2017 sorry there was a lunar or

play21:39

a solar eclipse so the moon shadow

play21:41

passed across the United States that was

play21:47

pretty remarkable if you guys are you

play21:49

saw that it was great if not well

play21:52

there's never a chance in 2024 April 8th

play21:58

we're gonna have a solar eclipse that

play22:01

goes up through Mexico through Texas and

play22:05

through the eastern seaboard of the

play22:07

United States but you know there other

play22:10

time

play22:11

December 14th 2020 there will be a solar

play22:15

eclipse that happens through South

play22:17

America 2030 through South Africa ok so

play22:26

all these times and dates are when

play22:29

you're gonna see be able to see this

play22:32

kind of event now that is it for our

play22:36

first lecture in this series of lectures

play22:41

that have to do with this class and stay

play22:47

tuned for continuing lectures that he'll

play22:50

have to do about stuff moving this guy

play22:53

and how we understand how that stuff

play22:57

moves to the sky

Rate This
β˜…
β˜…
β˜…
β˜…
β˜…

5.0 / 5 (0 votes)

Related Tags
Lunar PhasesMoon OrbitSolar EclipseLunar EclipseEarth RotationCelestial MechanicsAstronomy ClassSky ObservationSpace EducationEclipse Seasons