Mock Practice Test-5
Read each of the following passages and answer the items that follow. Your answers to these items should be based on the passages only.
After evidence was obtained in the 1920s that the universe is expanding, it became reasonable to ask: will the universe continue to expand indefinitely, or is there enough mass in it for the mutual attraction of its constituents to bring this expansion to a half? It can be calculated that the critical density of matter needed to break the expansion and “close” the universe, is equivalent to three hydrogen atoms per cubic meter. But the density of the observable
universe—luminous matter in the form of galaxies comes to only a fraction of theis. If the expansion of the universe is to stop, there must be enough invisible matter in the universe to exceed the luminous matter in density by a factor of roughly 70.
Our contribution to the search for this “missing matter” has been to study the rotational velocity of galaxies at various distance from their centre of rotation. It has been known for some time that outside the bright nucleus of a typical spiral galaxy luminosity falls off rapidly with distance from the centre. If luminosity is a true indicator of mass, most of the mass would be concentrated toward the centre. Outside the nucleus the rotational velocity would decrease geometrically with the distance from the centre, in conformity with Kepler’s law. Instead we have found that the rotational velocity in spiral galaxies either remains constant with increasing distance from the centre or increases slightly. This unexpected result indicates that the fall off in luminous mass with distance from the debtor is balanced by an increase in non-luminous mass.
Our findings suggest that as much as 90 per cent of the mass of the universe is not radiating at any wavelength with enough intensity to be detected on the Earth. Such dark matter could be in the form of extremely dim stars of low mass of large planets like Jupiter, or of black holes, either small or massive. While it has not yet been determined whether this mass is sufficient to “close” the universe, some physicists consider it significant that estimates are converging on the critical value.
The authors’ suggestion that “as much as 90 per cent of the mass of the universe is not radiating at any wavelength with enough intensity to be detected on the Earth” (last para) would be most weakened if which of the following were discovered to be true?
A The density of the observable universe is greater than most previous estimates have suggested.
B The bright nucleus of a typical spiral galaxy also contains some non-luminous matter.
C Some galaxies do not rotate or rotate too slowly for their rotational velocity to be measured.
D Spiral galaxies are less common than types of galaxies that contain little non-luminous matter.