Let's reproduce the calculations from Interstellar

ScienceClic English
8 May 202426:33

Summary

TLDRThis video explores the scientific accuracy of 'Interstellar', analyzing the ship's speed, artificial gravity, and black hole depictions. It delves into wormhole geometry, time dilation near a black hole, and the film's portrayal of gravitational anomalies. The video also discusses the theoretical physics behind the movie's climax, including the Tesseract and the potential for quantum gravity to save humanity.

Takeaways

  • 🚀 *Interstellar* explores the realism of its scientific concepts, such as black holes and wormholes, with calculations to verify their accuracy.
  • 🛰️ The ship in *Interstellar* travels at approximately 70,000 km/h, a speed feasible with advanced technology, taking two years to reach Saturn.
  • 🌍 Artificial gravity is created on the spaceship *Endurance* through centrifugal force, with realistic dimensions of about 60 meters in diameter.
  • 🌀 The movie's portrayal of a wormhole as a three-dimensional tunnel connecting two slices of space is consistent with theoretical physics.
  • 🌊 On Miller’s planet, 1 km high waves result from tidal forces due to its proximity to the supermassive black hole Gargantua, though the time dilation portrayed is exaggerated.
  • ⏳ Time dilation near Gargantua leads to one hour on Miller’s planet equating to seven years on Earth, achievable with a rapidly rotating black hole.
  • 🌌 Gargantua’s visual effects include a plasma accretion disk with gravitational lensing and Doppler effects, though some aspects were altered for cinematic purposes.
  • 🧑‍🔬 Professor Brand's equation suggests that gravitational anomalies may be caused by fields in a larger universe with extra dimensions.
  • 🕳️ Cooper survives falling into the black hole due to a theoretical gentle singularity, and enters a four-dimensional tesseract created by advanced beings.
  • 🏟️ The *Cooper Station* space habitat likely has a diameter between 50 to 100 meters, based on a baseball trajectory used to calculate its rotation and gravity.

Q & A

  • What is the main theme of the video 'Interstellar'?

    -The video discusses the scientific accuracy and concepts presented in the movie 'Interstellar', such as black holes, wormholes, and the behavior of time and space.

  • What is the estimated speed of the ship in 'Interstellar'?

    -The estimated speed of the ship in 'Interstellar' is around 70,000 km/h, calculated by dividing the distance of approximately 1.3 billion km by 2 years of travel time.

  • How does the artificial gravity system work in the ship Endurance?

    -The artificial gravity system in the ship Endurance works by using a rotating wheel, which creates a centrifugal force that pushes the characters against its outer walls, simulating gravity.

  • What is a wormhole and how does it appear in the movie 'Interstellar'?

    -A wormhole is a theoretical 'shortcut' through spacetime, connecting two distant points in the universe. In the movie, it appears as a three-dimensional tube connecting two celestial spheres.

  • What is the concept of time dilation as depicted in 'Interstellar'?

    -Time dilation in 'Interstellar' refers to the difference in the passage of time between two observers due to differences in their relative motion or gravitational fields. On Miller's planet, one hour corresponds to seven years on Earth.

  • How are the massive waves on Miller's planet explained?

    -The massive waves on Miller's planet are explained as tidal forces caused by the close proximity to the black hole Gargantua, which distorts the planet and creates immense waves.

  • What is the significance of the black hole Gargantua in 'Interstellar'?

    -Gargantua is a supermassive black hole with a strong gravitational pull that affects the time dilation experienced by the characters and the extreme tidal forces on nearby planets.

  • How does the Tesseract, a four-dimensional object, play a role in the movie?

    -The Tesseract in 'Interstellar' is a four-dimensional space that allows Cooper to interact with his past and communicate with his daughter Murphy, providing a means to send crucial data.

  • What is the role of the character Cooper in the movie 'Interstellar'?

    -Cooper, a former NASA pilot, plays the protagonist who embarks on an interstellar journey to find a new home for humanity and eventually interacts with a higher dimension to influence past events.

  • What scientific theories are explored in the movie's depiction of the universe?

    -The movie explores theories such as general relativity, quantum mechanics, and the possibility of extra dimensions, as well as the effects of black holes on time and space.

  • How does the movie 'Interstellar' visualize the scientific concept of gravitational anomalies?

    -Gravitational anomalies in 'Interstellar' are visualized as strange occurrences that guide characters to secret locations and are later explained as being influenced by higher-dimensional fields.

Outlines

00:00

🌌 Introduction to 'Interstellar' and Scientific Accuracy

The video script introduces a deep dive into the scientific accuracy of the movie 'Interstellar' directed by Christopher Nolan. It discusses the movie's realistic portrayal of a black hole and the various scientific concepts it explores, such as the speed of the ship, its dimensions, the behavior of time around a black hole, and the appearance of a wormhole. The script mentions a collaboration with Kip Thorne, the main scientist behind the movie, and the use of his book 'The Science of Interstellar' to verify the movie's scientific claims. The video aims to recreate some visuals from the movie and understand the technical aspects of the film, such as the travel time to the wormhole near Saturn and the artificial gravity on the spaceship Endurance.

05:03

🔭 Simulating the Wormhole and Black Hole in 'Interstellar'

This section of the script discusses the attempt to simulate the wormhole and black hole as depicted in 'Interstellar'. It explains the process of creating a realistic wormhole image using a method called ray tracing, which involves tracing the path of light rays through curved spacetime. The script also explores the appearance of the inside of a wormhole and how it was visualized in the movie. Additionally, it delves into the characteristics of the black hole named Gargantua, including its massive size, the extreme tidal forces it generates, and the significant time dilation near it. The script compares the simulated images with those from the movie to assess their realism.

10:04

🌊 Tidal Forces and Time Dilation on Miller's Planet

The script examines the extreme tidal forces and time dilation on Miller's Planet, which is depicted as being very close to the black hole Gargantua. It discusses how these forces create enormous waves and how time passes much slower on the planet compared to Earth. The calculations provided aim to estimate the distance at which a planet would need to orbit a black hole to experience such phenomena. The script also addresses the discrepancy between the movie's portrayal of time dilation and the actual calculations based on general relativity, suggesting that for the extreme time dilation shown in the movie to be accurate, the planet would need to be in an unstable orbit extremely close to the black hole.

15:14

🌒 Visualizing the Black Hole and Gravitational Lensing

This part of the script focuses on the visual representation of the black hole Gargantua and the surrounding environment in 'Interstellar'. It describes the use of ray tracing to simulate the gravitational lensing effects caused by the black hole, which distorts the light from the accretion disk and creates the shadow of the black hole. The script also discusses the Doppler effect on the appearance of the accretion disk, where one side appears brighter and bluer while the other appears darker and redder due to the movement of the disk relative to the observer. The video script compares these simulated visuals with the images from the movie to highlight the artistic choices made in the film.

20:15

🔬 Theoretical Physics and the Quest for Quantum Gravity

The script explores the theoretical physics behind the movie's plot, particularly the professor's quest to understand gravity and the nature of the universe. It discusses the idea of our universe being one slice of a larger multiverse with additional dimensions, and how this concept is used to explain the gravitational anomalies observed in the movie. The script also touches on the concept of singularities within black holes and the speculative idea that one might survive a fall into a black hole with a gentle singularity. It describes how Cooper, the protagonist, uses this knowledge to communicate with his daughter Murphy across time and space.

25:17

🚀 The Cooper Station and the Future of Humanity

In this final section, the script discusses the construction of the Cooper Station, a massive centrifuge designed to save humanity by lifting off into space. It provides a unique approach to estimating the dimensions of the station by analyzing a scene where a baseball is hit and travels the length of the station. The script uses the principles of gravity and motion to calculate the radius and rotation speed of the station. It concludes by reflecting on the movie's attention to scientific detail and the thought-provoking concepts it presents, encouraging viewers to delve deeper into the scientific aspects of the film.

Mindmap

Keywords

💡Interstellar

Interstellar is a 2014 science fiction film directed by Christopher Nolan that explores space travel, black holes, and the survival of humanity. In the video, 'Interstellar' serves as the central subject for mathematical and scientific analysis, where various scenes and concepts from the movie are scrutinized for their scientific accuracy.

💡Black Hole

A black hole is a region in space where the gravitational pull is so intense that nothing, not even light, can escape it. The black hole in 'Interstellar,' called Gargantua, plays a crucial role in the film’s narrative. The video discusses the visual and physical representation of Gargantua, including the gravitational effects, time dilation, and the accretion disk.

💡Wormhole

A wormhole is a theoretical tunnel through space-time that connects two distant points in the universe. In 'Interstellar,' a wormhole near Saturn allows the characters to travel to distant planets. The video examines the scientific plausibility of the wormhole’s visual appearance and discusses how light would behave when passing through such a structure.

💡Time Dilation

Time dilation is a consequence of Einstein’s theory of relativity, where time passes differently depending on the strength of the gravitational field or speed of movement. In 'Interstellar,' time dilation occurs near the black hole Gargantua, where one hour on a planet close to the black hole equals seven years on Earth. The video analyzes the accuracy of this effect and its implications.

💡Gravitational Anomalies

Gravitational anomalies in 'Interstellar' refer to strange events that occur due to disruptions in the gravitational field. Cooper discovers these anomalies early in the film, and they eventually lead him to NASA. The video suggests that these anomalies are tied to extra-dimensional forces, explaining how gravity may behave differently in higher-dimensional spaces.

💡Accretion Disk

An accretion disk is a rotating disk of matter that forms around a massive object like a black hole due to its gravitational pull. In 'Interstellar,' the black hole Gargantua is surrounded by a luminous accretion disk. The video explains how the light from the disk is distorted by gravitational lensing and why certain visual effects, such as the Doppler effect, were minimized for the movie.

💡Centrifugal Force

Centrifugal force is the apparent force that pushes objects outward when they are in a rotating frame of reference. In 'Interstellar,' the spaceship Endurance creates artificial gravity by rotating like a wheel. The video provides a mathematical explanation of how the centrifugal force on the spaceship mimics Earth’s gravity, making the environment comfortable for the crew.

💡Photon Sphere

A photon sphere is a region around a black hole where gravity is so strong that light can orbit the black hole. The video explains how the characters in 'Interstellar' would have to avoid this region to prevent unstable orbits. It also describes the theoretical effects of time dilation near the photon sphere and its relevance to the plot.

💡Tesseract

A tesseract is a four-dimensional cube, which serves as the key to the film's climax. In 'Interstellar,' Cooper enters a tesseract near the singularity of a black hole, allowing him to interact with different points in time within his daughter’s bedroom. The video explores the idea of higher-dimensional spaces and how the tesseract serves as a narrative device for explaining time travel and communication across time.

💡Singularity

A singularity is a point in space where gravitational forces become infinite, causing the laws of physics to break down. In 'Interstellar,' the singularity inside the black hole Gargantua plays a crucial role when Cooper plunges into it. The video delves into the various types of singularities, including the speculative 'gentle' singularity, which allows Cooper to survive, and discusses the challenges of understanding what happens inside a black hole.

Highlights

Interstellar, directed by Christopher Nolan, presents realistic images of a black hole and explores scientific concepts like time dilation and wormholes.

The video attempts to mathematically verify the accuracy of various concepts presented in the film.

The speed of the ship in the movie is estimated to be around 70,000 km/h, which is considered realistic given the context.

Artificial gravity in the ship is achieved through centrifugal force, calculated to have a radius of roughly 30 m or 60 m in diameter.

The appearance of the wormhole in the movie is simulated using a method called Ray tracing, which involves tracing light rays through each pixel of a camera.

The inside of the wormhole is explored, with simulations suggesting different visual effects based on the geometry of the wormhole.

The movie's depiction of extreme tidal forces on Miller's planet due to proximity to a black hole is analyzed.

Time dilation on Miller's planet is discussed, with the movie showing a factor of 60,000, which is higher than calculated estimates.

The visual appearance of the black hole Gargantua in Interstellar is examined, with simulations attempting to reproduce the movie's images.

The concept of a fourth dimension is introduced through the Tesseract, a four-dimensional object in the movie.

Cooper's survival near a black hole's singularity is explored, suggesting the possibility of a gentle singularity in older black holes.

The movie imagines gravity as the force that can cross dimensions and communicate across time.

Murphy uses the data sent by Cooper to understand how to control gravity, which is crucial for humanity's survival in the movie.

The dimensions of the space station in the movie are estimated using the trajectory of a baseball hit inside the station.

The movie's scientific accuracy is praised, with detailed calculations and simulations enhancing the understanding of complex concepts.

The video concludes by enjoying simulations built throughout, showcasing the intersection of science and cinema in Interstellar.

Transcripts

play00:00

warning this video contains

play00:04

spoilers here's what Interstellar could

play00:06

have looked like

play00:08

[Music]

play00:25

[Music]

play00:33

welcome back to science click today

play00:36

let's try to remake the calculations

play00:38

from

play00:39

Interstellar released in 2014

play00:42

Interstellar directed by Christopher

play00:44

Nolan left its mark on audiences by

play00:47

presenting realistic images of a black

play00:49

hole but is the movie accurate what is

play00:52

the speed of the ship what are its

play00:54

Dimensions how does time behave around a

play00:57

black hole what does the inside of a

play00:59

worm whole look like in this video we

play01:02

will go back over the Journey of the

play01:04

film's characters and attempt to

play01:05

mathematically verify the accuracy of

play01:08

the different concepts we will also try

play01:10

to rebuild some visuals from the movie

play01:13

this may be a bit technical but just

play01:15

keep in mind you don't need to

play01:17

understand all the

play01:18

calculations we will at times rely on

play01:21

information from the book the science of

play01:22

interstellar written by Kip Thorn the

play01:25

main scientist behind the

play01:27

movie this video was originally made in

play01:30

collaboration with the French Channel

play01:31

gab which talks about science in popular

play01:34

movies he usually doesn't make videos in

play01:36

English but kindly agreed to let us

play01:37

translate his voice for this one so

play01:39

don't be surprised if the visual style

play01:41

of the video changes at times when we

play01:43

present the

play01:46

storyline at the start of interstellar

play01:49

the situation on Earth is critical

play01:51

humans are facing food shortages air is

play01:53

close to unbreathable dust is

play01:55

omnipresent the planet no longer seems

play01:58

habitable on this apocalyptic Earth we

play02:01

follow Cooper a former NASA pilot who

play02:03

lives with his two children in the

play02:05

bedroom of his daughter Murphy strange

play02:07

events occur events that Cooper ends up

play02:10

identifying as gravitational

play02:13

anomalies one day one of these anomalies

play02:15

mysteriously reveals coordinates which

play02:18

once followed lead to a secret NASA base

play02:21

as if the library had wanted to guide

play02:23

them there in this NASA Center we learn

play02:26

that a wormhole has opened near Saturn

play02:28

forming a passage to planets and that

play02:31

NASA is about to launch a critical

play02:33

Mission a space crew will cross the

play02:35

Wormhole and try to reach three

play02:37

potentially habitable

play02:39

exoplanets of course Cooper arrives just

play02:42

in time for the adventure as a former

play02:44

NASA pilot he is recruited and thus

play02:46

embarks on an Interstellar Journey

play02:48

aboard the

play02:54

endurance after takeoff the crew goes

play02:56

into hibernation the ship will take two

play02:59

years to arrive at the Wormhole near

play03:02

Saturn is this travel time

play03:05

realistic we can roughly estimate the

play03:07

speed of the ship by taking the shortest

play03:10

straight line between Earth and Saturn

play03:12

and factoring in the radius of their

play03:14

orbits we can assume that the ship

play03:15

travels approximately 1.3 billion km

play03:19

divided by 2 years this gives us a speed

play03:22

of around 70,000

play03:25

kmph as a basis for comparison the

play03:27

fastest ever manned flight was Apollo 10

play03:30

with a speed of 40,000 km hour assuming

play03:34

that interstellar's Technologies are

play03:36

better than ours this 2-year duration is

play03:39

therefore

play03:41

realistic the characters need artificial

play03:43

gravity to feel comfortable the inurance

play03:46

forms a wheel which turns on itself and

play03:48

pushes the characters against its outer

play03:50

Walls by centrifugal effect the

play03:53

centrifugal acceleration is given by 4K

play03:56

^ 2 R / t^ 2 where R is the radius of

play03:59

the wheel and T its period of rotation

play04:03

in this scene we can time a half period

play04:05

of 5.7 seconds which gives us a total

play04:08

period of 11.4

play04:10

seconds this must equal 9.8 m/s squared

play04:15

the value of gravity on Earth we deduced

play04:18

that the radius of the wheel must be

play04:20

roughly 30 m or 60 m in

play04:23

diameter a fairly realistic value given

play04:26

the International Space Station is 70 m

play04:35

cross the endurance's crew wakes up near

play04:38

Saturn we observe For the First Time The

play04:40

Wormhole that they will have to

play04:43

cross a wormhole is a distortion of

play04:46

space a sort of tube which connects two

play04:49

slices of the

play04:51

universe it is difficult to draw because

play04:53

the surface of the tube is actually

play04:56

three-dimensional a volume within which

play04:58

the ship can move

play05:02

light can also pass through it and we

play05:04

can receive an image of what is on the

play05:06

other

play05:08

side but is its appearance in the movie

play05:11

realistic to find out let's try to

play05:14

simulate

play05:15

it we start with a cylinder connecting

play05:19

two sheets of space let's smooth out

play05:22

this cylinder to have a better

play05:24

transition for the movie Nolan chose a

play05:27

very short cylinder and a relatively

play05:29

quick transition to get the appearance

play05:31

he

play05:32

liked let's place a camera and choose

play05:35

two images to represent the sky the

play05:38

celestial sphere of each of these two

play05:40

Universe

play05:41

slices the camera receives light rays

play05:44

some of which arrive directly from the

play05:46

same slice it is on and others after

play05:48

crossing the Wormhole all these light

play05:50

rays arrive on the pixels of the

play05:54

camera without going into details we can

play05:57

perform a method called Ray tracing

play05:59

which which involves sending a light Ray

play06:01

through each pixel of the camera and

play06:03

rewinding its trajectory to determine

play06:05

where it came from in the sky and what

play06:07

color is received by the camera on that

play06:10

pixel in practice this amounts to using

play06:13

the geodesic equation a general

play06:15

relativity equation which allows us to

play06:17

trace trajectories through curved

play06:20

SpaceTime by repeating the operation for

play06:22

each pixel we obtain an

play06:25

image a result which when put in motion

play06:28

is quite similar to that of the

play06:33

movie we can now play around with

play06:36

varying the geometry of the Wormhole to

play06:38

see what it might have looked like if

play06:40

Nolan had made different

play06:42

choices with a very long Wormhole light

play06:44

can orbit several times before reaching

play06:46

us and we can observe an infinite number

play06:49

of repeating images of the

play06:51

[Music]

play06:54

universe in interstellar the endurance

play06:57

enters the Wormhole to cross it we

play07:00

discover the inside of the

play07:03

Wormhole is this scene

play07:05

realistic to find out let's move our

play07:08

virtual camera along the surface of the

play07:11

tube this time around the images are

play07:13

quite different from what the movie

play07:15

shows us the visual effects team

play07:18

probably wanted to help the viewer

play07:19

better understand that the spaceship is

play07:21

moving along the surface of a cylinder

play07:23

and Crossing into a fourth

play07:26

dimension if this scene had been

play07:28

simulated we could have witnessed

play07:30

hypnotizing images such as

play07:38

[Music]

play07:48

these exiting the Wormhole the Explorers

play07:51

arrived near a super massive black hole

play07:53

called Gargantua this black hole has

play07:55

planets orbiting around it and our

play07:57

crew's first destination is one of the

play07:59

Millis

play08:01

Planet this planet is very special it is

play08:03

completely covered in water and its

play08:05

orbit is very close to Gargantua so

play08:08

close in fact that extreme phenomena

play08:10

arise near a black hole tidal forces are

play08:13

gigantic and Gargantua attracts the

play08:16

planet more on one side than the other

play08:18

distorting it and forming immense 1 km

play08:20

high waves on its

play08:23

surface because of its proximity to the

play08:25

black hole time also passes more slowly

play08:28

so much so that for each hour that

play08:30

passes on this planet 7 years pass on

play08:33

Earth in short Miller's planet is

play08:35

mysterious and deserves our

play08:40

attention let's start with the waves Kip

play08:44

Thorn indicates that they stretch over 1

play08:46

km in height how close to the black hole

play08:49

would the planet need to be for such

play08:51

waves to

play08:53

form we can attempt a rough estimate we

play08:57

can assume that these waves are in fact

play08:59

Tides generated not by the attraction of

play09:02

the moon but by that of the black hole

play09:05

the waves in the movie look thinner than

play09:07

simple Tides they might be closer to

play09:09

what we call tidal BS but for a rough

play09:11

estimate our approach should still work

play09:14

the waves thus result from the

play09:16

combination of gravity from the black

play09:18

hole and the centrifugal effect produced

play09:20

by the orbit of the planet we can

play09:23

calculate the resulting net force with

play09:25

Newtonian physics this is the tidal

play09:28

Force

play09:30

this Force displaces water from low tide

play09:32

left and right to high tide up and

play09:36

down the force supplies each water

play09:39

droplet a certain energy which we can

play09:41

calculate as the product of the vertical

play09:43

displacement which is the radius of the

play09:45

planet and the average value of the

play09:47

force along this

play09:50

path it is this energy brought by the

play09:53

tidal Force which allows the water to

play09:56

rise it must therefore equal the

play09:58

gravitational energy that the water

play10:01

acquires from this equality we can

play10:03

deduce the distance at which the planet

play10:05

should orbit for such tides to

play10:08

form if the planet's dimensions are

play10:10

similar to those of Earth knowing that

play10:12

the black hole weighs 100 million solar

play10:15

masses then the planet should orbit at a

play10:17

distance of 4.5 billion

play10:20

km to compare the spart Shield radius of

play10:23

the black hole which we can deduce from

play10:25

its mass is 300 million km across

play10:29

if we bring this diagram to scale and

play10:31

compare it to this image from the movie

play10:33

showing Gargantua a scene from Millis

play10:35

Planet the results seems

play10:40

coherent but is this close enough to

play10:43

also explain the strong time

play10:46

dilation each hour that passes on the

play10:48

planet corresponds to seven years on

play10:50

Earth time passes 7times 365 time 24

play10:56

times slower a factor of 60,000

play10:59

for a static black hole this is the time

play11:02

dilation experienced by a planet in

play11:05

circular orbit if we insert the distance

play11:08

obtained with the calculation of the

play11:10

tides we get a time dilation of only 5%

play11:13

far from what the movie shows us there

play11:16

is an

play11:17

incoherence to obtain a factor of 60,000

play11:20

the planet would have to orbit just

play11:22

above the photon sphere where light

play11:24

itself can remain in orbit an absurd

play11:27

result because any orbit so close is

play11:30

inevitably

play11:32

unstable but this calculation is only

play11:35

valid for a static black hole general

play11:37

relativity allows black holes to rotate

play11:40

the faster a black hole spins the more

play11:43

likely stable orbits exist near its

play11:45

Horizon the calculations are more

play11:48

complex but we can determine that it is

play11:50

possible to reach a factor of 60,000

play11:53

provided that the planet orbits 6,000 km

play11:56

from The Horizon and that the black hole

play11:58

spins at a trillion of a percent slower

play12:00

than the speed of light extremely fast

play12:04

but not impossible in theory of course

play12:07

this situation remains incompatible with

play12:09

what the movie shows

play12:12

us the visual appearance of the black

play12:15

hole is surely what brought attention to

play12:18

Interstellar in France jeanpier Lum had

play12:20

done a first simulation in 1979 but in

play12:24

2014 it is the first time that we see

play12:26

such images in theaters could we

play12:29

reproduce these simulations at our

play12:33

scale let's try the ray tracing method

play12:36

we place a camera in the center of a

play12:38

celestial sphere in front of a black

play12:40

hole rotating almost at maximum speed

play12:44

general relativity allows us to rewind

play12:46

the trajectory of light rays to find

play12:48

their origin in the sky some rays are

play12:51

blocked by the black hole and the

play12:53

corresponding pixels do not receive any

play12:56

light in this way we can stru an

play13:00

image the rays are deflected by

play13:03

gravitational lensing causing Optical

play13:07

distortions we observe the shadow of the

play13:10

black hole the area from which we

play13:12

received no light for a static black

play13:15

hole this Shadow would be a disc but for

play13:17

a spinning black hole it seems squashed

play13:19

on one side because SpaceTime spins and

play13:21

drags light with it in the movie this

play13:25

phenomenon was reduced to render the

play13:27

visual effect less strange

play13:31

a round Gargantua orbits an extremely

play13:33

luminous plasma disc let's place a disc

play13:37

in our

play13:40

simulation we see that its image is

play13:42

distorted the back of the disc seems

play13:45

folded above and below because the black

play13:47

hole bends the Rays coming from

play13:50

it in reality such an accretion disc

play13:53

would be extremely hot it would emit

play13:56

intense radiation which would instantly

play13:58

destroy the ship the disc temperature

play14:01

has therefore been drastically brought

play14:03

down for the movie implying that it is

play14:05

also very thin given its lower internal

play14:09

pressure this plasma rotates very

play14:11

quickly around the black hole such that

play14:14

the light we received from it is

play14:15

propelled on one side and slowed down on

play14:17

the other this is the Doppler effect the

play14:21

disc appears bright and slightly blue

play14:23

where it moves towards us and dark and

play14:25

red where it moves away from us this

play14:28

effect was considered too strange and

play14:30

was not included in the

play14:32

film we can play around with comparing

play14:34

our simulation to images from

play14:37

[Music]

play14:54

Interstellar here's what it could have

play14:56

looked like if they had included the

play14:58

asymmetry the Doppler effect and a

play15:00

higher temperature dis

play15:14

[Music]

play15:32

[Music]

play15:46

[Music]

play15:50

while our Interstellar mission is going

play15:51

on back on Earth the professor refines

play15:54

his mathematical model trying to account

play15:56

for the discovery of the gravitational

play15:58

anomalies

play15:59

this Quest had already led him towards a

play16:02

very complex equation to solve and his

play16:04

goal in solving this equation is to have

play16:06

answers about the nature of gravity and

play16:09

then use this new knowledge to launch a

play16:10

gigantic spaceship into space and save

play16:14

Humanity but we are not there yet at

play16:18

this stage of the research the

play16:19

professor's conclusion is that the

play16:21

gravitational anomalies must be caused

play16:23

by something outside our

play16:25

universe according to him our space

play16:28

could be one slice inside a larger

play16:30

universe with one more Dimension the

play16:33

anomalies would be caused by Fields

play16:35

present in this bigger space outside our

play16:38

world we see the details of this model

play16:40

on Professor Bran's blackboards in the

play16:43

movie The Universe would contain three

play16:45

brains our brain a brain above and a

play16:48

brain below forming a sort of Sandwich

play16:51

between these two brains the geometry of

play16:54

the universe would be curved into an

play16:56

anti- deit geometry a geometry allowing

play16:59

distances to be greatly stretched above

play17:01

and below our universe such that gravity

play17:03

cannot Escape in fact in our universe

play17:07

gravity propagates in all directions and

play17:09

its intensity is therefore distributed

play17:12

over spheres which is why the force of

play17:14

gravity is inversely proportional to the

play17:16

square of the distance just like the

play17:18

surface of a

play17:20

sphere but if we were to add an extra

play17:22

dimension of space gravity wouldn't form

play17:24

spheres but hyperspheres extending

play17:27

beyond our slice of universe

play17:29

and gravity would decrease like the cube

play17:32

of the distance which we obviously do

play17:34

not

play17:35

observe with the anti- deito warping

play17:38

gravity remains confined near our

play17:40

universe and still behaves as one/ r s

play17:44

the other two brains help in delimiting

play17:47

this warping leaving enough volume

play17:49

outside for possible Adventures within

play17:51

the fourth

play17:52

dimension this is a necessary Precision

play17:55

to justify the end of the movie

play17:59

back on Earth Murphy has now taken over

play18:02

from Professor brand in their quest for

play18:04

Gravity it's now her task to find a

play18:07

solution to the equation and describe

play18:09

the nature of the fields to explain the

play18:10

anomalies observed on Earth although the

play18:13

professor's model seemed promising at

play18:15

first no results follow and Murphy ends

play18:18

up realizing what he had known all along

play18:20

without telling her to complete the

play18:22

model they need information about the

play18:25

quantum nature of gravity Murphy must

play18:28

understand what happens at a point where

play18:30

gravity meets Quantum for example by

play18:32

diving near the singularity of a black

play18:35

hole coincidentally this is exactly what

play18:38

her Father Joseph Cooper is doing in

play18:40

another

play18:41

[Music]

play18:44

galaxy following tars Cooper detaches

play18:47

himself from the endurance and Falls

play18:49

towards the horizon of the black hole

play18:52

can he survive without being

play18:55

spaghettified up until the 1960s

play18:58

singular ities were considered as

play19:00

pointlike in the 1970s however

play19:03

physicists understood that these

play19:05

singularities undergo chaotic

play19:07

distortions they are known as bkl

play19:10

singularities in the 1990s researchers

play19:13

discovered that when we fall into a

play19:15

black hole all the matter falling behind

play19:17

us seems to pile up because of the

play19:19

slowing down of time we Face a mass

play19:22

inflation

play19:24

Singularity finally we discovered around

play19:27

2010 that older black holes have a third

play19:30

Singularity stemming from the

play19:32

accumulation of matter that fell prior

play19:35

this Singularity is gentle it generates

play19:37

relatively weak tidal

play19:39

forces while this is still highly

play19:41

speculative it might be possible to

play19:44

survive there but we would have to dive

play19:46

almost at the speed of light to prevent

play19:48

the other Singularity from catching up

play19:50

with us this is precisely the advice

play19:54

that romaly offers Cooper in the film

play19:56

Gargantua is an old black hole

play19:58

containing a gentle Singularity he could

play20:01

survive it by diving at high

play20:04

speed it is this possibility although

play20:07

very speculative that Nolan chose for

play20:09

his movie in a mysterious way Cooper

play20:12

manages to accelerate enough to hit this

play20:15

Singularity first and

play20:19

survive no one knows what lies at the

play20:22

center of a black hole we would probably

play20:24

need a theory of quantum

play20:26

gravity nonetheless in the movie Nolan

play20:29

imagines that when Cooper hits the

play20:31

singularity he is transported by a

play20:33

four-dimensional object called the

play20:35

Tesseract an object believed to have

play20:37

been placed there by the same beings who

play20:39

opened the

play20:41

Wormhole this Tesseract is a sort of

play20:43

four-dimensional cube while a

play20:45

three-dimensional Cube's faces are

play20:47

two-dimensional squares the Tesseract

play20:49

faces are not squares but

play20:51

three-dimensional cubes and this

play20:53

structure allows for Koopa to stay

play20:55

inside one of the faces of the Tesseract

play20:57

while the tesseract transports him back

play20:59

to Earth all the way to Murphy's room by

play21:03

the way if this journey feels quite fast

play21:06

despite the huge distance it is because

play21:07

the Tesseract has been lifted above our

play21:10

brain into the anti- DEA warping we

play21:12

mentioned previously where distances are

play21:15

greatly

play21:16

contracted the Tesseract acts as an

play21:18

elevator towards the fourth dimension of

play21:22

space once he arrives Cooper can see

play21:25

Murphy's room in the past which is

play21:28

possible because light can travel within

play21:30

the faces of the Tesseract up to his

play21:32

eyes however in the model imagined by

play21:35

Nolan light cannot go back in time from

play21:37

Cooper to Murphy he therefore has no way

play21:40

to communicate with her at least this is

play21:43

until Cooper discovers that gravity can

play21:45

cross this barrier and return to the

play21:47

past an idea which is probably inspired

play21:50

by the fact that in theories describing

play21:52

universes with additional dimensions in

play21:54

the context of brain cosmology all

play21:56

fundamental interactions are generally

play21:58

can find within the brains except

play22:01

gravity which propagates through all

play22:03

Dimensions Cooper can therefore send the

play22:06

quantum data to Murphy using gravity

play22:08

giving his daughter all the elements

play22:09

necessary to solve the equation we

play22:12

finally understand that he was behind

play22:14

the gravitational anomalies from the

play22:17

beginning recall once again though that

play22:19

the things we have just described are

play22:21

simply the physical rules set by Nolan

play22:23

for this very speculative sequence of

play22:26

the movie

play22:28

thanks to the data Murphy understands

play22:30

that it is possible to control gravity

play22:33

we can reduce the intensity of gravity

play22:35

on the surface of the Earth to lift off

play22:38

a huge space station and save

play22:41

Humanity the kooper station a large

play22:44

centrifuge thus heads towards Saturn to

play22:46

cross the Wormhole for our last

play22:49

calculation let's try to determine the

play22:52

dimensions of this space station we

play22:55

could imagine several methods but let me

play22:57

propose an unexpected Ed approach in

play23:00

this scene of the movie we see a

play23:02

baseball player hitting a ball which

play23:04

travels through the entire station and

play23:06

ends up breaking a window on the

play23:08

opposite side above the field the ball

play23:11

experiences no force and therefore moves

play23:13

in a straight line at constant

play23:16

speed but from the inside the trajectory

play23:19

of the ball seems curved because we are

play23:21

spinning with the

play23:25

wheel at this stage we don't know the

play23:28

param

play23:29

of this trajectory the speed of the ball

play23:32

the angle of the trajectory the radius

play23:34

of the wheel and its rotation

play23:37

speed but we see in the movie that the

play23:39

gravity in the station is similar to

play23:41

Earth's this gives us a restriction on

play23:44

the rotation of the wheel it must spin

play23:47

at a precise speed to generate this

play23:50

gravity we also know that the ball ends

play23:52

up breaking a window above the field we

play23:55

can therefore restrict the angle of the

play23:57

trajectory such that it reaches is a

play23:58

point above the

play24:00

field watching the scene we can time the

play24:03

trajectory of the ball and measure 4.6

play24:06

seconds between the hit and the impact

play24:08

and we can then estimate its initial

play24:10

speed by analyzing frame by frame and

play24:13

comparing to the size of the player we

play24:15

find an estimate of 30

play24:18

m/s with all these restrictions we

play24:21

determine the radius of the wheel

play24:23

approximately 50 m or 100 m in diameter

play24:27

for roughly 3 00 m in circumference a

play24:30

relatively small station which would

play24:32

rotate at four revolutions per minute

play24:36

the trajectories of baseballs would be

play24:38

chaotic to say the

play24:41

least with other methods by comparing

play24:44

with the size of a building for instance

play24:46

we find very different values sometimes

play24:48

even 1 km I'll leave it up to you to

play24:51

develop your own techniques to estimate

play24:53

these

play24:56

Dimensions born from the creative mind

play24:59

of an expert in relativity Interstellar

play25:02

is a unique movie with breathtaking

play25:04

visuals through these few calculations

play25:06

we can appreciate the attention to

play25:08

detail brought to the construction of

play25:10

the scenario and delve deeper into

play25:12

issues that may not seem obvious at

play25:14

first viewing as a conclusion let's

play25:17

enjoy once again some of the simulations

play25:19

we've built throughout this video

play25:26

[Music]

play25:35

[Music]

play25:41

[Music]

play26:06

[Music]

play26:13

[Music]

Rate This

5.0 / 5 (0 votes)

Related Tags
InterstellarBlack HolesWormholesTime DilationSpace TravelScientific AccuracyCinematographyAstrophysicalKip ThorneChristopher Nolan