/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q22P The mass of Mars is 6.4×1023 a... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

The mass of Mars is 6.4×1023and its radius is 3.6×106 m. What is the value of constant g on Mars?

Short Answer

Expert verified

The value of constant g on mars is 3.709 m/sec2.

Step by step solution

01

Identification of the given data

The given data can be listed below as,

  • The mass of Mars is,m=6.4×1023kg.
  • The radius of Mars is, r=3.4×106m.
  • Assume universal gas constant (G) =6.7×10-11
02

Significance of Newton’s second law on a sled

This law states that the force acting on Mars depends on Mars’s mass and mars acceleration.

The mass of Mars and acceleration of the Mars product give the force required to accelerate Mars.

03

Determination of acceleration due to gravity on Mars.

Let g be acceleration due to gravity on Mars.

As we know that according to the second law of motion,

F = mg …………………….(1)

Also, according to universal gravitational law,

F=GMmr2 …â¶Ä¦â¶Ä¦â¶Ä¦â¶Ä¦â¶Ä¦â¶Ä¦â¶Ä¦.(2)

Now, 1 = 2,

Therefore,

mg=GMmr2g=GMr2

g=6.7×10-11×6.4×10233.4×1062=6.7×6.4×10-11+23-6-63.4×3.4=42.88×100=3.709

Thus, the value of constant g on Mars is 3.709 m/sec2

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

A roughly spherical asteroid has a mass of 3.11×1020kgand a radius of 270 km. (a) What is the value of the constant g at a location on the surface of the asteroid? (b) What would be the magnitude of the gravitational force exerted by the asteroid on a 70 kg astronaut standing on the asteroid’s surface? (c) How does this compare to the gravitational force on the same astronaut when standing on the surface of the Earth?

Use data from the inside back cover to calculate the gravitational and electric forces two electrons exert on each other when they are1×10-10mapart (about one atomic radius). Which interactions between two electrons is stronger, the gravitational attraction or the electric repulsion? If the two electrons are at rest, will they begin to move toward each other or away from each other? Note that since both the gravitational and the electric forces depend on the inverse square distance, this comparison holds true at all distances, not just at a distance of1×10-10m.

A star of mass 7×1030kg is located at <5×1012,2×1012,0>m.A planet of mass 3×1024kg and is located at <3×1012,4×1012,0>m and is moving with a velocity of <0.3×104,1.5×104,0>m/s (a) At a time 1×106s later what is the new velocity of the planet? (b) Where is the planet at this later time? (c) Explain briefly why the procedures you followed in parts (a) and (b) were able to produce usable results but wouldn’t work if the later time had been 1×109s instead of 1×106s after the initial time. Explain briefly how you could use a computer to get around this difficulty.

A bowling ball is initially at rest. A Ping-Pong ball moving in the +z direction hits the bowling ball and bounces off it, traveling back in the –z direction. Consider a time interval ∆t extending from slightly before to slightly after the collision. (a) In this time interval, what is the sign of ∆Pz for the system consisting of both balls? (b) In this time interval, what is the sign of ∆Pz for the system consisting of the bowling ball alone?

A satellite that is spinning clockwise has four low-mass solar panels sticking out as shown. A tiny meteor traveling at high speed rips through one of the solar panels and continues in the same direction but at reduced speed. Afterward, calculate the vxandvycomponents of the center of mass velocity of the satellite. In Figure 3.64 v1→andv2→ are the initial and final velocities of the meteor, andv→ is the initial velocity of the center of the mass of the satellite, in the x-direction.

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.