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Difference between revisions of "Southern Celestial Rotation"

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{{#ev:youtube|https://www.youtube.com/watch?v=t30-YbayyXE}}
 
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According to P-Brane's explanation the observer is seeing a wide range of stars squished into a small area by perspective. Rotation appears as an anti-rotation due to a mirrored motion of the North.
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'''Q.''' How can two people on opposite sides of the earth both see the South Pole Star simultaneously?
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'''A.''' Since those areas are many hours apart from each other, when it is day for one area it is night or dusk for the other. It is questioned whether it is the case that observers would see the same stars.
  
 
==Bi-Polar Model==
 
==Bi-Polar Model==

Revision as of 07:28, 1 May 2019

The Southern Celestial Rotation refers to the anti-rotation of the stars observed in the southern regions of the earth.

Monopole Model

P-Brane explains the anti-rotation of the stars as a consequence of perspective. The author uses the sun's crepuscular rays as an example for how something can seem to be rotating in two different directions, much like how spinning in the chair and looking up and down can cause the appearance of two different rotations.

According to P-Brane's explanation the observer is seeing a wide range of stars squished into a small area by perspective. Rotation appears as an anti-rotation due to a mirrored motion of the North.

Q. How can two people on opposite sides of the earth both see the South Pole Star simultaneously? A. Since those areas are many hours apart from each other, when it is day for one area it is night or dusk for the other. It is questioned whether it is the case that observers would see the same stars.

Bi-Polar Model

Under the Bi-Polar Model the anti-rotation in the south is explained with the existence of a South Pole and a rotating southern celestial system above it.

See the Bi-Polar Model