Since the atmospheric pressure at the surface of Venus is 93 times the atmospheric pressure at the surface of the Earth, use the given values with Equation 2 to estimate the equivalent depth in the Earth's ocean. *Using attached figures for calculation* For Venus, the atmospheric pressure at the surface is much higher than on Earth. We can compare this to depth in the ocean by using the simple equation fora static fluid that calculates the pressure, P, using the density of the liquid, p (rho), and gravity of the planet, g, and the height (or depth), h. This equation isgiven by:P = pghmkgBy rearranging this expression and using the Earth's gravity (g = 9:807or meters per second squared), the average density of salt water (p = 1024orkilograms per cubic meter), and the pressure at the surface of the Earth (PEarth = 101325kgor kg per meter per second squared or Pascals), we canms2calculate the depth in the ocean that produces a pressure equivalent to the surface of Venus. By doing some algebra in the previous equation, we get a newequation:hpg

Pressure at the surface of earth = 101325 kg/ms2 Since pressure at the surface of Venus is 93 times…

Answered: Since the atmospheric pressure at the…

Algebra and Trigonometry (6th Edition)

6th Edition

ISBN:9780134463216

Author:Robert F. Blitzer

Publisher:Robert F. Blitzer

ChapterP: Prerequisites: Fundamental Concepts Of Algebra

Section: Chapter Questions

Problem 1MCCP: In Exercises 1-25, simplify the given expression or perform the indicated operation (and simplify,...

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Since the atmospheric pressure at the surface of Venus is 93 times the atmospheric pressure at the surface of the Earth, use the given values with Equation 2 to estimate the equivalent depth in the Earth's ocean.

*Using attached figures for calculation*

For Venus, the atmospheric pressure at the surface is much higher than on Earth. We can compare this to depth in the ocean by using the simple equation for
a static fluid that calculates the pressure, P, using the density of the liquid, p (rho), and gravity of the planet, g, and the height (or depth), h. This equation is
given by:
P = pgh
m
kg
By rearranging this expression and using the Earth's gravity (g = 9:807
or meters per second squared), the average density of salt water (p = 1024
or
kilograms per cubic meter), and the pressure at the surface of the Earth (PEarth = 101325
kg
or kg per meter per second squared or Pascals), we can
ms2
calculate the depth in the ocean that produces a pressure equivalent to the surface of Venus. By doing some algebra in the previous equation, we get a new
equation:
h
pg

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