In June 1997 the NEAR spacecraft , on its way to photograph the asteroid Eros, passed near the asteroid Mathilde. After passing Mathilde, on several occasions rocket propellant was expelled to adjust the spacecraft's momentum in order to follow a path that would approach the asteroid Eros, the final destination for the mission. After getting close to Eros, further small adjustments made the momentum just right to give a circular orbit of radius around the asteroid. So much propellant had been used that the final mass of the spacecraft while in circular orbit 45km(45×103m)around Eros was only . The spacecraft took 1.04days to make one complete circular orbit around Eros. Calculate what the mass of Eros must be.

Short Answer

Expert verified

The mass of the Eros is 6.67×1015kg.

Step by step solution

01

Identification of given data

A circular orbit of radius is45km45×103m.

The final mass of the spacecraft while in circular orbit is500kg.

The spacecraft took days to make one complete circular orbit around Eros.

02

Definition of force

A force is a push or pull on an object is because of the interaction of the thing with another object. Every time two things interact, a force is exerted on each of them. The acted force may be of attraction or repulsion. The two items no longer feel the force after the interaction ends.

03

Determining the mass of Eros

The net force on an object is equal to the rate of change of momentum and can be written as the sum of two components.

The parallel rate of change of momentumdpdt||and the perpendicular rate of change of momentumdpdtare the two elements that we are concerned with.

So, the net forceFneton the object is given by

Fnet=dpdt=dpdt||+dpdt

The rock's speed is affected by the parallel rate of change of momentum and given the speed is constant, therefore, the parallel rate is zero, and it equals the size of the momentum rate change.

dpdt||=0

The centrifugal forceFcequals the rate change, which is the change in direction owing to the perpendicular rate of change.

At speeds significantly slower than the speed of light, the magnitude of the perpendicular rate change is given by

Fc=dpdt=mv2R

The change in distance over time is the speed.

So, it is given by

v=dt

The engineer goes above the diameter of a circle as he travels through one cycle.

The circumference is given by,

2πR

where R is the radius of the circle.

So, the distance where the engineer travel is:

d=2πR

Therefore,

v=2πRt

The mass of the Eros,

vearth=vasteroidGMER=2πRtGMER=2πRt2ME=2πRt2RG

Now, put the values for R,t,andGtogetME, where is the time taken to complete one round by the spacecraft.

t=(1.04days)(24h/day)(3600s/h)=89.85×103s

ME=2πRt2RG1n=2π×45×103m89.85×103s245×103m6.67×10-11N·m2/kg2=6.67×1015kg

Therefore, the mass of the Eros is 6.67×1015kg.

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 Vaia!

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

Question: A student said, "When the Moon goes around the Earth, there is an inward force due to the Moon and an outward force due to centrifugal force, so the net force on the Moon is zero." Give two or more physics reasons why this is wrong.

The planets in our Solar System have orbits around the Sun that are nearly circular, and v<<c.Calculate the period T(a year-the time required to go around the Sun once) for a planet whose orbit radius is r. This is the relationship discovered by Kepler and explained by Newton. (It can be shown by advanced techniques that this result also applies to elliptical orbits if you replaceby the semi major axis, which is half the longer, major axis of the ellipse.) Use this analytical solution for circular motion to predict the Earth's orbital speed, using the data for Sun and Earth on the inside back cover of the textbook.

Tarzan swings back and forth on a vine. At the microscopic level, why is the tension force on Tarzan by the vine greater than it would be if he were hanging motionless?

A comet orbits a star in an elliptical orbit, as shown in Figure 5.41. The momentum of the comet at locationis shown in the diagram. At the instant the comet passes each location labeled A, B, C, D, E, and F, answer the following questions about the net force on the comet and the rate of change of the momentum of the comet:

(a) Draw an arrow representing the direction and relative magnitude of the gravitational force on the comet by the star.

(b) IsFnetzero to nonzero?

(c) IsFnetzero or nonzero?

(d) Isd|p|/dspositive, negative, or zero?

(e) Isdp¯/drzero or nonzero?

A planet orbits a star in an elliptical orbit. At a particular instant the momentum of the planet is (-2.6×1029,1.0×1029,0)kg.m/sand the force on the planet by the star is (-2.5×1022,1.4×1023,0)N. findF and role="math" localid="1654057870125" F.

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.

Sign-up for free