|
This wiki is closed in favour of the new wiki. Information shown is likely to be very out of date. |
Difference between revisions of "Black Hole"
Silverleaf81 (talk | contribs) m |
Silverleaf81 (talk | contribs) m |
||
| Line 3: | Line 3: | ||
A black hole is a theoretical entity predicted by the equations of general relativity. A black hole is formed when a star of sufficient mass undergoes gravitational collapse, with most or all of its mass compressed into a sufficiently small area of space, causing infinite spacetime curvature at that point (a ''singularity''). Such a massive spacetime curvature allows nothing, not even light, to escape from the ''event horizon'' or border. | A black hole is a theoretical entity predicted by the equations of general relativity. A black hole is formed when a star of sufficient mass undergoes gravitational collapse, with most or all of its mass compressed into a sufficiently small area of space, causing infinite spacetime curvature at that point (a ''singularity''). Such a massive spacetime curvature allows nothing, not even light, to escape from the ''event horizon'' or border. | ||
| − | Only one black hole is present in Sirius, located in [[Omicron-85]]. If the star has a low mass for a black hole, they can become [[Neutron Star|Neutron Stars]]. Several theories have been made on the stars of [[Omega-11]] and [[New Berlin]], if they would become black holes or neutron stars, or if they will just collapse forming a black object. | + | Only one black hole is present in Sirius, [[Razgriz Black Hole|located]] in [[Omicron-85]]. If the star has a low mass for a black hole, they can become [[Neutron Star|Neutron Stars]]. Several theories have been made on the stars of [[Omega-11]] and [[New Berlin]], if they would become black holes or neutron stars, or if they will just collapse forming a black object. |
Getting close to the ''event horizon'' will result in nearly instant death. | Getting close to the ''event horizon'' will result in nearly instant death. | ||
Revision as of 18:35, 1 February 2016
A black hole is a theoretical entity predicted by the equations of general relativity. A black hole is formed when a star of sufficient mass undergoes gravitational collapse, with most or all of its mass compressed into a sufficiently small area of space, causing infinite spacetime curvature at that point (a singularity). Such a massive spacetime curvature allows nothing, not even light, to escape from the event horizon or border.
Only one black hole is present in Sirius, located in Omicron-85. If the star has a low mass for a black hole, they can become Neutron Stars. Several theories have been made on the stars of Omega-11 and New Berlin, if they would become black holes or neutron stars, or if they will just collapse forming a black object.
Getting close to the event horizon will result in nearly instant death.
See Also
