Do any coordinate systems include self magnification?

In summary: The sky would include more than 180 degrees of the constellations. Suppose the neutron star was near Earth and spinning on Earth's axis. An observer at the surface equator would be able to see both the southern cross and Polaris. A time-lapse photo would show non-circular rings around Polaris. Orion and Taurus could be visible on one horizon while both Lyra and Bootes were still visible on the other. When a star set it would rise on the other horizon in much less than a day. Orion would be thin at rising, get fat while overhead and then tighten his belt before setting. It would still look like a 180 degree dome. If the Sun was in orbit then
  • #1
DarkStar42
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0
Take a neutron star, its surface will be gravitationally self magnified so that it looks bigger to the distant observer, than it 'really' is, plus you can see some of the rear facing surface.

If you take the centre of the neutron star, then this process must go on there also, although unseen.

I was wondering if any coordinate system incorporated this process, say by building the shape of space from the inside of the neutron star, outwards, as the distant observer might 'see' it..?
 
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  • #2
DarkStar42 said:
...
If you take the centre of the neutron star, then this process must go on there also, although unseen...
...

From the center of the neutron star the neutron star occupies 360 degrees same as center of Earth. From the surface of the neutron star the neutron star occupies 180 degrees same as surface of Earth. You could see stars that should be over the horizon.
 
  • #3
stefan r said:
From the center of the neutron star the neutron star occupies 360 degrees same as center of Earth. From the surface of the neutron star the neutron star occupies 180 degrees same as surface of Earth. You could see stars that should be over the horizon.

a distant observer can see more than 50% of the neutron star's surface.

4335232013_3755299c6c_o.jpg
 

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  • #4
DarkStar42 said:
a distant observer can see more than 50% of the neutron star's surface.

View attachment 228304

That picture is nice. An observer on that equator would see 180 degrees of neutron star and 180 degrees (180° by 360°) of space same as an observer on Earth.

The sky would include more than 180 degrees of the constellations. Suppose the neutron star was near Earth and spinning on Earth's axis. An observer at the surface equator would be able to see both the southern cross and Polaris. A time-lapse photo would show non-circular rings around Polaris. Orion and Taurus could be visible on one horizon while both Lyra and Bootes were still visible on the other. When a star set it would rise on the other horizon in much less than a day. Orion would be thin at rising, get fat while overhead and then tighten his belt before setting. It would still look like a 180 degree dome. If the Sun was in orbit then it would be daylight for much more than half the day even at the equator at equinox. You would get white nights at mid latitudes during the summers.
 

1. What is self-magnification in a coordinate system?

Self-magnification in a coordinate system refers to the phenomenon where the scale of the coordinate system changes as it moves away from the origin. This means that the distances between points increase or decrease depending on their location within the coordinate system.

2. Which coordinate systems include self-magnification?

Polar coordinates, logarithmic coordinates, and exponential coordinates are some examples of coordinate systems that include self-magnification. These systems are commonly used in mathematics, physics, and engineering to represent complex or non-linear relationships.

3. How does self-magnification affect measurements in a coordinate system?

Self-magnification can make measurements in a coordinate system more challenging as the scale is not consistent throughout. This can lead to errors in calculations and interpretations of data. It is important to understand and account for self-magnification when working with these types of coordinate systems.

4. Can self-magnification be beneficial in any way?

While self-magnification can make measurements more complex, it can also offer advantages in certain situations. For example, it can help to visualize and understand non-linear relationships or patterns in data. Additionally, it can be useful in creating maps or graphs that accurately represent exponential or logarithmic functions.

5. Are there any practical applications of coordinate systems with self-magnification?

Yes, coordinate systems with self-magnification have many practical applications in various fields. For instance, polar coordinates are commonly used in navigation and astronomy, while logarithmic coordinates are used in economics and biology. These systems allow for a better understanding and representation of complex relationships and phenomena.

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