AST102IN Spring 2014
AST102IN Spring 2014
  • Видео 25
  • Просмотров 151 271
Lecture 25 - the Age, Shape, Size and Fate of the Universe
Watch before class on Monday, May 5 and post a question in the comments
Lecturer: Kate
Просмотров: 4 089

Видео

Lecture 24 - Dark Matter
Просмотров 2,9 тыс.10 лет назад
watch before class on Wednesday, April 30 and post a question in the comments. Lecturer: Maria
Lecture 23 - Cosmic Evolution
Просмотров 2,9 тыс.10 лет назад
Watch before class on Monday, April 28 and post a question in the comments. Lecturer: Maria
Lecture 22 - The Big Bang
Просмотров 2,1 тыс.10 лет назад
watch before class on Wednesday, April 23 and post a question in the comments Lecturer: Kate
Lecture 21 - The Expanding Universe
Просмотров 2 тыс.10 лет назад
Watch before class on Monday, April 21 and post a question in the comments Lecturer: Kate
Lecture 20 - The Milky Way Part 2
Просмотров 2,5 тыс.10 лет назад
Watch before class on Wednesday, April 16 and post a question in the comments
Lecture 19 - The Milky Way
Просмотров 3,6 тыс.10 лет назад
Watch before class on Monday, April 14 and post a question in the comments Lecturer: Maria
Lecture 18 - Multiple Star Systems
Просмотров 2,5 тыс.10 лет назад
watch and post a question in the comments before class on Wednesday, April 9 Lecturer: Maria
Lecture 17 - Star Formation
Просмотров 11 тыс.10 лет назад
Watch before class on Monday, April 7 AND POST A QUESTION IN THE COMMENTS Lecturer: Kate
Lecture 16 - Stellar End States
Просмотров 5 тыс.10 лет назад
Watch before class on Wednesday, April 2 AND POST A QUESTION IN THE COMMENTS Lecturer: Maria
Lecture 15 - Stellar Evolution
Просмотров 33 тыс.10 лет назад
watch AND POST A QUESTION before class on Monday, March 31 lecturer: Kate
Lecture 14 - The Nature of Stars
Просмотров 6 тыс.10 лет назад
watch before class on Wednesday, March 25 AND POST A QUESTION IN THE COMMENTS Lecturer: Maria
Lecture 13 - Fusion and Heat Transfer
Просмотров 2,6 тыс.10 лет назад
Lecturer: Kate watch before class on Monday, March 24
Lecture 12 - Light and Atoms
Просмотров 3,8 тыс.10 лет назад
Watch before class on Wednesday, March 5
Lecture 11 - Thermal Emission
Просмотров 3,4 тыс.10 лет назад
watch before class on Monday, March 3
Leture 10 - The Electromagnetic Spectrum
Просмотров 2,7 тыс.10 лет назад
Leture 10 - The Electromagnetic Spectrum
Lecture 9 - Light and Color
Просмотров 3,1 тыс.10 лет назад
Lecture 9 - Light and Color
Lecture 8 - Light Travel
Просмотров 2,7 тыс.10 лет назад
Lecture 8 - Light Travel
Lecture 7 - Newton's Laws and Gravity
Просмотров 2,4 тыс.10 лет назад
Lecture 7 - Newton's Laws and Gravity
Lecture 6 - Kepler's Laws
Просмотров 3,1 тыс.10 лет назад
Lecture 6 - Kepler's Laws
Lecture 5 - Models of the Solar System
Просмотров 3,2 тыс.10 лет назад
Lecture 5 - Models of the Solar System
Lecture 4 - Lunar Phases and Eclipses
Просмотров 4,9 тыс.10 лет назад
Lecture 4 - Lunar Phases and Eclipses
Lecture 3 - Earth's Tilt and the Seasons
Просмотров 6 тыс.10 лет назад
Lecture 3 - Earth's Tilt and the Seasons
Lecture 2 - Yearly Motions of the Night Sky and the Ecliptic
Просмотров 8 тыс.10 лет назад
Lecture 2 - Yearly Motions of the Night Sky and the Ecliptic
Lecture 1: Daily Motions of the Sky and The Celestial Sphere
Просмотров 28 тыс.10 лет назад
Lecture 1: Daily Motions of the Sky and The Celestial Sphere

Комментарии

  • @군주-b9v
    @군주-b9v Месяц назад

    Gonzalez Mary Harris Nancy Thomas Brenda

  • @TheZafootz
    @TheZafootz 2 месяца назад

    great lecture, I'd like to say a few things for you to think about. When you say a star runs out of fuel that's not entirely true. What happens is the core of hydrogen fusion grows outward into a shell as the heavier helium falls into a new core as this happens the core of helium gets larger and the shell of hydrogen fusion expands. In the process of a new helium core being formed it steals heat and energy from the hydrogen shell causing the star itself to expand into a red giant. So as the helium core gets larger the shell of hydrogen fusion expands until the helium core gathers enough density to begin fusion again. When this happens the star stops expanding because now the helium atoms are now sinking into a newly formed core of carbon. So when the helium core stops growing its size and begins falling inward again creating a newly dense core of carbon the expansion of the red giant stops and the star becomes stable again. The same process happens again with each newly formed core of new elements in very high mass stars and like you stated they do this all the way to the element of Iron. This is the point where the heat and energy that the iron core steals from the fusion shells of the lighter elements does not stop even if the iron core gets dense enough to fuse into a heavier element, that fusion process has the same effect it steals energy from the outer shells and as the iron core does this the shells of lighter elements get burned up by the process of the iron core stealing energy from them. If the stars are massive enough they can cause the iron to fuse into more heavier elements but sense this process steals energy from its outer shells they begin to fall inward. So when heat and energy is absorbed by the iron core that in turn makes the stars expansion process from the fusion in the stars shells to weaken so the star begins to shrink. The Super Nova explosion happens from the parts of the iron core fusing into heavier elements like gold and such but as this process happens it constantly is stealing heat and energy from its outer fusion shells causing them to collapse inward tell they are fully absorbed by the fusion of the iron core into heavier elements until there's nothing left of the lighter elements to collapse inward then all that remains is the outer explosion of the iron fusion into heavier elements. It is only the expansion effect of iron fusing into heavier elements that remains and there is nothing left in the outer shells to collapse then inward movement stops and only outward expansion movement remains. This is when the super nova occurs when the core of the star absorbs outer shells and the fusion of the iron into heavier elements is thrown out into space along with any new elements the iron core fused in its short time it had to absorb its outer shells heat and energy until they are completely absorbed then there's nothing that can collapses anymore and all that's left is the outer explosion/expansion of the iron core fusing into these heavier elements. This causes the material to have no where else to go other then outward into space as a super nova explosion. So I believe for a brief moment a star has an iron core and absorbs its outer shells and fuses iron into heavier elements then after all outer shells are absorbed then the fusion explosion of iron into gold and such causes the iron core to explode into a super nova. This is why after a super nova there is no left over dense core that remains after because the brief fusion process of iron into the heavier elements absorbs all of the energy of the stars outer shells tell there's nothing to absorb and hold back the explosion effect from the iron fusion and then creates the super nova. So it makes sense that a stars Iron core can become dense enough to make newly dense heavier element cores within it but because that process absorbs energy these denser cores from iron fusion only last a very brief and short period of time. So I think its not the rebound effect that causes the super nova its the fusion of iron into heavier elements that steals energy from its outer shells until they are fully absorbed and all that remains is the outer explosion of the iron fusion remains that causes the super nova. If there was a rebound effect that we are told happens then there would be some sort of core that would remain that the material thrown out would have bounced off of but after a super nova there is no left over core. This is what makes me believe that this process I explained happens and not the rebound effect we are told that happens. Of course this is all just good guess work and that's all anyone can really speculate on because there is no way to test or experiment a super nova in a lab and all super nova's are so far away that observational evidence is impossible to collect. So this is my best guess on what happens to a star when it becomes a super nova and that's what I wanted to share. I hope this wasn't too long for you to read and I look forward to watching more of your videos. Thanks again!

  • @RaniShrividya
    @RaniShrividya 2 месяца назад

    The best channel I have come across. Thank you ma'am.

  • @specialrelativity8222
    @specialrelativity8222 5 месяцев назад

    best

  • @phdnk
    @phdnk 7 месяцев назад

    Why don't slightly endothermic Ni(p,γ)Cu or Ni(α,γ)Zn processes happen in heavy stars anytime during Si burn but before core collapse begins? Assume stellar core has gravitational energy to spend, there is more than enough energy to convert significant portion of Fe/Ni core into Cu/Zn. Why this does not happen ? Skip talking abut: - stellar evolution - supernovae - s-,r- processes - Cu & Zn real origin, skip Discovery channel talk, focus on the topic at hand. University level explanation is expected, that uses binding energy, photodissociation rates, Saha equation, nuclear statistical equilibrium e.t.c The core might initially be either degenerate or non-degenerate, address both states.

  • @mejiqal
    @mejiqal 9 месяцев назад

    be aware of her explanation about empty space and the expanding universe because everything she explain is complete wrong ..she dosent understand what is empty space nither expanding universe.....she just remember what she learned but she dont understand what she talk about empty space and expanding universe ...even the top expert include albert enisten didnt know what they talk...do deep research and you will be shook when you ask the right questions about emapty space and expanding universe...

  • @fedinvestment
    @fedinvestment 10 месяцев назад

    Good

  • @anikshaha3024
    @anikshaha3024 Год назад

    Thank you. Your lecture clear my all problems. Thank thanks

  • @rustambaloch1742
    @rustambaloch1742 Год назад

    How can I get the notes in pdf??

  • @monocacy664
    @monocacy664 Год назад

    who else is here for SEES?

  • @이이-n4z8y
    @이이-n4z8y Год назад

    Yea, not listening to someone who was granted an education based on gender and not merit.

    • @michaeldamolsen
      @michaeldamolsen Год назад

      Kate Follette is an award winning scientist with articles published in Nature and Science as well as several other reputable journals. Your claim is incredibly arrogant and completely unfounded.

    • @이이-n4z8y
      @이이-n4z8y Год назад

      @@michaeldamolsen Yea, gifted things because of p.c. while meeating no standards to deserve them. Where have you been for the past 60 years?

  • @applepie3566
    @applepie3566 Год назад

    Mam but earth only cones around sun isnt it.

  • @alexnevermind5963
    @alexnevermind5963 Год назад

    This is one of the best explanations of this process. Now, can you do a video on the concept of " dredge up" in stars during the asymptotic branch in particular?😃👍

  • @salahsana3481
    @salahsana3481 Год назад

    Good job. Thanks

  • @zakzeus.shuufHunaak
    @zakzeus.shuufHunaak Год назад

    Zeus regel

  • @abdulrahimalharby6778
    @abdulrahimalharby6778 Год назад

    Thank you: you are adding a greater understanding to the human learning by offering valuable insight by expending valuable time of your own life so with a greater appreciation I’m much obliged to thank you.

  • @persianmedicine2458
    @persianmedicine2458 Год назад

    You must be emitting very long wavelength since your energy in lecturing is approaching negative infinity. Seriously, can you put more energy in talking or lecturing?

  • @vapeymcvape5000
    @vapeymcvape5000 2 года назад

    Maybe turn off your fan before recording?

  • @justincase3030
    @justincase3030 2 года назад

    Fahrenheit 🤮

  • @Tinker1950
    @Tinker1950 2 года назад

    Far too painful and confused to watch.

  • @ar77315
    @ar77315 2 года назад

    Moon covers its orbit in 28 days then why we say lunar month is about 30 days?

    • @michaeldamolsen
      @michaeldamolsen Год назад

      It all depends how you define a month. Counting the time it takes for the Moon to return to the same location compared to the background stars is called a sidereal month, and takes 27.32 days. If you instead count the time for the Moon to show the same phase again, this is a synodic month, which lasts 29.53 days. There are other less common types of month, but these are the two being asked about. The reason for the difference is that Earth moves in its orbit around the Sun during the month. So when the Moon returns to the same spot in the sky (a sidereal month), the Sun is no longer in the same place. Hence it takes an extra two days for the Moon to get into the same position, relative to the Sun (synodic month), and thus show the same phase. I know this was asked long ago, but I maybe new viewers have the same question.

    • @ashutoshtripathi8927
      @ashutoshtripathi8927 Год назад

      @@michaeldamolsen yea

  • @balasbramanithangavel5933
    @balasbramanithangavel5933 2 года назад

    Introductory lecture. Many details are left out.

  • @WaySensei
    @WaySensei 2 года назад

    Are small changes in the energy output of the sun due to the the pressure/feedback loop detectable?

  • @WaySensei
    @WaySensei 2 года назад

    Zero zero zero zero zero lol. Here’s a question: how do we know how energy transfer occurs inside a star? Is this through applying the laws of physics to a computer model of the sun?

  • @time2cclear
    @time2cclear 2 года назад

    how is it that i can see the moon sometimes at noon , 2 pm , 4pm in east Tennessee where i live ? how is this possible ?

  • @muratcan__22
    @muratcan__22 2 года назад

    too good

  • @billynomates920
    @billynomates920 2 года назад

    bit of a difference between a 15 inch naval shell and a bullet but you're right, he'd have been better off going with bullet.

  • @TheZafootz
    @TheZafootz 2 года назад

    With all due respect I want to disagree with the orbital change that is state by many videos like this and my realization is that electrons are at a lower energy state and also a lower frequency when at a higher orbit from the nucleus. As for the higher energy state is when the electron is at a lower orbit or increase its number or orbits per second by being closer to the nucleus then when at a higher orbit. if the electrons are all moving at the same speed that does not change from orbit to orbit then its number of orbits per second must very. This is what connects an electrons frequency of light with its orbit distance and to its known energy state. As atoms cool down(in witch all atoms are doing) the electrons slowly drift out to higher orbits causing their number of orbits or its frequency to slowly drop. This can be do to Entropy or some other natural reason but over all it makes more sense that the electrons frequency increases when its orbit size decreases thus increasing the number of orbits it does per second and when at a higher orbit they are at a lower frequency or a lower number of orbits per second but they are all moving at the same speed, the speed of Light.

  • @මලින්දසමරසිංහ

    Wonderfully explained Madam .Thank You.

  • @wati52
    @wati52 3 года назад

    Great explanation.

  • @nishabhardwaj80
    @nishabhardwaj80 3 года назад

    your lectures are really informative. good job

  • @mierafalemu9751
    @mierafalemu9751 3 года назад

    it is really amazing lecture.it made me to love astronomy more.

  • @sunkaridinesh4226
    @sunkaridinesh4226 3 года назад

    EXCELLENT SUPER DUPER BUMPER MASTER XTRA ORDINARY FANTASTIC

  • @prachi579
    @prachi579 3 года назад

    Hats off to your lecture! Amazing explanation. Each word and each sentence is important. Very precise! Thank you so much :)

  • @prachi579
    @prachi579 3 года назад

    Love these lectures!!!

  • @izureki
    @izureki 3 года назад

    Great sister 👍👍👍👍👍👍👍

  • @syedaliaizaz2031
    @syedaliaizaz2031 3 года назад

    thanks a lot

  • @apurvsahu5889
    @apurvsahu5889 3 года назад

    Wait...why low mass stars expands...😅

  • @kouserimam5938
    @kouserimam5938 4 года назад

    I know this is too late and may be you won't read my comment but you should know what I am going to tell you. Thank you very much for these amazing lectures. Tomorrow is my interview and your videos really helped me a lot. Thank you very much Ma'am for these lectures. I will always pray for you...

  • @thepeoplesuncle
    @thepeoplesuncle 4 года назад

    A 100 watt bulb does not put out 100 watts of brightness it simply means that a 100 watt bulb pulls out 100 watts from the socket it's plugged in to.

  • @Keithlfpieterse
    @Keithlfpieterse 4 года назад

    Thanks for the upload. I am enjoying this series of lectures in the midst of the COVID-19 pandemic. I have been interested in astronomy for quite some time and to this day watch a variety of documentaries on the subject. For the record, your presentations are informative, accessible to a broad public and not as stuffed with the hype and ego of some of the NASA and JPL presentations. Thank you. Rest assured I shall be watching all the lectures in this series and maybe...just maybe slip in a comment at the very end. Take care and I wish you well with your enthusiasm for the subject and your chosen career!

  • @mariossavvides2287
    @mariossavvides2287 4 года назад

    Good delivery.. Thanks!

  • @Incognito-vc9wj
    @Incognito-vc9wj 4 года назад

    Excellent presentation Thankyou.

  • @scis3385
    @scis3385 5 лет назад

    I never studied Astronomy that way! Awesome🤖👏🏼

  • @scis3385
    @scis3385 5 лет назад

    I never studied Astronomy that way! Awesome🤖👏🏼

  • @danielvonbose557
    @danielvonbose557 5 лет назад

    Only Bad Astronomers Feel Good Knowing Mnemonics.

  • @visheshgoyal5903
    @visheshgoyal5903 5 лет назад

    Great vedio

  • @visheshgoyal5903
    @visheshgoyal5903 5 лет назад

    Great vedio

  • @firozbhati9578
    @firozbhati9578 5 лет назад

    Thanks a lot, 7:50 which software you are using

  • @christopherwilliamsutjiono5382
    @christopherwilliamsutjiono5382 5 лет назад

    Does the mass of the star decrease during planetary nebula because the outer layers are ejected or because the core contracts?