The atmospheric pressure at Venus's surface is approximately 92 times Earth's atmospheric pressure. In other words, standing on Venus would subject you to pressure comparable to being roughly 900 meters beneath Earth's ocean surface.
This enormous pressure comes from the mass of Venus's atmosphere, which is far denser and more extensive than Earth's. Although Venus is only slightly smaller than Earth, its atmosphere has about 90 times the surface pressure because it is dominated by a deep layer of carbon dioxide. Near the surface, the pressure is high enough for carbon dioxide to behave as a supercritical fluid rather than an ordinary gas.
Venus's pressure is closely tied to its extreme heat. The thick carbon-dioxide atmosphere traps infrared radiation in a runaway greenhouse effect, keeping surface temperatures near 462°C. The planet is hotter than Mercury despite orbiting farther from the Sun.
Some references round the value to 93 Earth atmospheres or describe it as about 92–93 times Earth pressure. The quiz's 92 is the accepted approximate value, while 200, 50, and 10 are far outside the measured range. At about 50 kilometers above the surface, pressure and temperature become much more Earth-like.