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Dedicated To People Who Did Not Understand Interstellar


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Posted

Okay now I understood but future humans ancestors ela survive ayyaro  chepunte bagundedi 

 

choopistaru ga last lo cooper ni save chesi cooper station ki teesuku vastharu ga.....that's plan A

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Posted

PK  smoking gif aesthae cool manishi ani...bemmi laughing gif aaesthae kamedy manishi ani...ila Brahmi_0.gif?1350486327ee gif aesthae BP manishi ani anaesukovadamaenaaa..!!

 

ok Brahmi_0.gif?1350486327
 

Posted

aa millers planet is very close to black hole....black hole ki entha daggara ga unte antha time dilation ekkuva untadi

 

actual ga adi minor plot hole, antha time dilation (1 hr = 7 yrs) undali ante it should be literally on the surface of the black hole...and as shown millers planet blackhole ki antha close ga undatam kuda practically possible kadu

if miller planet is close to black hole, then why the tides are high.. there is no extrnal gravitational influence ??? 

 

even on planet earth we havee casio pathfinder watches with tidometer.. 

 

i didnt understand how come though they have sophisticated nuclear powered space ships but no pre estimation of tides

Posted

thanu adigedi other side of wormhole nunchi earth ki data transmission gurinchi

 

 

neeku warm whole nunchi video relay avutudhi.. remember they cant relay back the replies..

 

also the planet with high waves .. endeavoour chuttu orbit lo vunna it takes 23 years for their journey of 3 hours, why ??

 

oh yeah i got it now , there are certainly a few plot holes bhaiyya , but i liked the way he showed various things ...

 

and coming to the second question .... i actually got the same doubt too ... time ratios gurinchi sarigga explain cheyyaledu ... 

Posted

if miller planet is close to black hole, then why the tides are high.. there is no extrnal gravitational influence ??? 

 

even on planet earth we havee casio pathfinder watches with tidometer.. 

 

i didnt understand how come though they have sophisticated nuclear powered space ships but no pre estimation of tides

 

blackhole influence tho aa waves ani ekkado chadivaa....it's actually accurate anta

 

estimation emo gani, vadiki clear ga kanipisthundi ga amelia valla bisket avthundi

 

aina ila prathi chinna point lo flaws vethikithe kashtam...koncham fiction untundi kada

Posted

PK smoking gif aesthae cool manishi ani...bemmi laughing gif aaesthae kamedy manishi ani...ila Brahmi_0.gif?1350486327ee gif aesthae BP manishi ani anaesukovadamaenaaa..!!


lol
Posted

no plot lo flaws anatledhu.. adhi explain chesademo ani doubt.. black holes inlfuence tho vunte.. a planet pina bright light vundhi.. it is still rotating under strong influence of near by star..

 

but quasar loki cooper velletappudu his mass should be shrinked istead he enter whole new dimension of time...

 

how he escapes from that dimension is a mystery !! I guess Murph herself solves the mystery and gets him out..

blackhole influence tho aa waves ani ekkado chadivaa....it's actually accurate anta

 

estimation emo gani, vadiki clear ga kanipisthundi ga amelia valla bisket avthundi

 

aina ila prathi chinna point lo flaws vethikithe kashtam...koncham fiction untundi kada

 

Posted

something like this

 

 

Super-Chandrasekhar mass Supernovae[edit]
Main article: Champagne Supernova

In April 2003, the Supernova Legacy Survey observed a type Ia supernova, designated SNLS-03D3bb, in a galaxy approximately 4 billion light years away. According to a group of astronomers at the University of Toronto and elsewhere, the observations of this supernova are best explained by assuming that it arose from a white dwarf which grew to twice the mass of the Sun before exploding. They believe that the star, dubbed the "Champagne Supernova" by University of Oklahoma astronomer David R. Branch, may have been spinning so fast that centrifugal force allowed it to exceed the limit. Alternatively, the supernova may have resulted from the merger of two white dwarfs, so that the limit was only violated momentarily. Nevertheless, they point out that this observation poses a challenge to the use of type Ia supernovae as standard candles.[39][40][41]

Since the observation of the Champagne Supernova in 2003, more very bright type Ia supernovae are thought to have originated by white dwarfs whose masses exceeded the Chandrasekhar limit. These include SN 2006gzSN 2007if and SN 2009dc.[42] The super-Chandrasekhar mass white dwarfs that have originated these supernovae are believed to have had masses up to 2.4–2.8 solar masses.[42] One way to potentially explain the problem of the Champagne Supernova was considering it the result of an aspherical explosion of a white dwarf. However, spectropolarimetric observations of SN 2009dc showed it had a polarization smaller than 0.3, making the large asphericity theory unlikely.[42]

Tolman–Oppenheimer–Volkoff limit[edit]

After a supernova explosion, a neutron star may be left behind. Like white dwarfs these objects are extremely compact and are supported by degeneracy pre

Posted

something like this

 

 

Super-Chandrasekhar mass Supernovae[edit]
Main article: Champagne Supernova

In April 2003, the Supernova Legacy Survey observed a type Ia supernova, designated SNLS-03D3bb, in a galaxy approximately 4 billion light years away. According to a group of astronomers at the University of Toronto and elsewhere, the observations of this supernova are best explained by assuming that it arose from a white dwarf which grew to twice the mass of the Sun before exploding. They believe that the star, dubbed the "Champagne Supernova" by University of Oklahoma astronomer David R. Branch, may have been spinning so fast that centrifugal force allowed it to exceed the limit. Alternatively, the supernova may have resulted from the merger of two white dwarfs, so that the limit was only violated momentarily. Nevertheless, they point out that this observation poses a challenge to the use of type Ia supernovae as standard candles.[39][40][41]

Since the observation of the Champagne Supernova in 2003, more very bright type Ia supernovae are thought to have originated by white dwarfs whose masses exceeded the Chandrasekhar limit. These include SN 2006gzSN 2007if and SN 2009dc.[42] The super-Chandrasekhar mass white dwarfs that have originated these supernovae are believed to have had masses up to 2.4–2.8 solar masses.[42] One way to potentially explain the problem of the Champagne Supernova was considering it the result of an aspherical explosion of a white dwarf. However, spectropolarimetric observations of SN 2009dc showed it had a polarization smaller than 0.3, making the large asphericity theory unlikely.[42]

Tolman–Oppenheimer–Volkoff limit[edit]

After a supernova explosion, a neutron star may be left behind. Like white dwarfs these objects are extremely compact and are supported by degeneracy pre

 

what limit is he talking about here ? .. can u please give me the whole article bro ...

Posted

Nolan's an expert in making people watching his movies feel intelligent.

 

He got me with The Dark Knight. :)

Posted

naaku naachindhi movie.. kaani konni dots connect kaale.. asalu ame edho theory raastadhi kadha - asalu em kanukkuntadho artham kaale

Posted

allu-brahmi.gif

 

andariki ardamkavali ani nuvve pade tapana chusthu unte...ba.........

Posted

Waiting for that hobbit movie. Interstellar, is for teenagers. 

 

I'm yet to find my way out of the movie crib :)

Posted

allu-brahmi.gif

 

andariki ardamkavali ani nuvve pade tapana chusthu unte...ba.........

 

halloween kadha.. cinema choosinte, chadivinta athanu raasindhi.

 

inception thone stop chesa Nolan gaadi cinemaalu.

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