Introduction
The space occupied by the cosmos is characterized by topology and geometry properties. Cosmologists concern themselves with curve properties as they unswervingly associate to the mass in the world. Topography influences evolution in the universe over time. Geometry does not dictate the shape of the globe though questions on whether it is limited in magnitude remain of great interest. Cosmologists classify the topography of the universe as positive, zero, or negative. When the total value of internal angles of a triangle drawn on flat space is 180 degrees, the topography is zero. Positive topography happens when the total value of angles is more than 180 degrees while a total value of angles less than 180 degrees indicates negative topography.
Main Body
Einstein’s equation relates topography to the bulk quantity contained in the world if the energy concentration of the free space in the universe is zero. Topography depends on whether the standard mass concentration is above the significant level or not. If the density remains on significant levels, the cosmos flattens. If the concentration is high, the cosmos assumes positive topography. The space within the universe provides a spherical surface that in its absence would cause the universe to collapse in a critical situation. In such serious situations, the cosmos must be limited in magnitude. Positive topography of the universe lacks evidenced support and the question of whether it is negative or flat remains a subject of discussion. The topography is necessary for supporting the universe as it developed from nothing.
Conclusion
In my opinion, it is not easy to label the topography of the universe because evolution is still taking place. However, topographic features of the universe contain physical significance in supporting the evolution of the universe. Cosmologists should do more studies to establish a universally accepted topography grade of the universe.