3. Astrologers claim that when Jupiter is 'lined-up' with the Earth and Sun, its gravitational pull on humans is significant, and thus affects our life. A) Calculate the gravitational pull from Jupiter on a human (m=70 kg) when Jupiter is 'in-line' with the Earth and Sun. B) Calculate the gravitational pull from a skyscraper on a human walking through any downtown, or city center (Assume a skyscraper has a mass of 1.2 x 10° kg, and the distance between the center of masses is 175 m). C) Calculate the pull from a large cliff (M=8.8 x 10' kg and R=14 m). D) How many times bigger are the answers in B and C than the answer in part A? Comment on these results.

Principles of Physics: A Calculus-Based Text
5th Edition
ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
Publisher:Raymond A. Serway, John W. Jewett
Chapter11: Gravity, Planetary Orbits, And The Hydrogen Atom
Section: Chapter Questions
Problem 44P
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Question answer #3
Background:
GmM
Newton formulated the Universal Law of Gravitation: F =
R2
where,
F
= the gravitational force between two masses.
G = the gravitational constant, G = 6.67 x 101" N• m²/kg?
the mass of one object
mass of other object
distance between the center of the objects
m
%3D
M =
R =
Also, we learned that weight, w=mg. Equating weight with Newton's Law of Gravitation
we get: mg =
GmM
or canceling m:
R2
GM
g =
R2
This can be used to calculate the acceleration of gravity on any planet/object/body.
Objective:
Investigate several phenomena using Newton's Universal Law of Gravitation. Understand
the difference between accuracy and precision.
Procedure:
Perform the indicated calculations. The following information can be used for the
calculations.
1.99 x 100 kg
5.98 x 1024 kg
7.36 x 102 kg
2 x 100 kg
1.90 x 1027 kg
Mass of Sun
1.50 x 10" m
6.38 x 10° m
1.74 x 10 m
12,000 m
6.3 x 10 m
Earth-Sun distance
Radius of Earth
Mass of Earth
Mass of Moon
Radius of Moon
Radius of neutron star
Mass of neutron star
Mass of Jupiter
Earth-Jupiter distance (in-line)
Error and Uncertainty:
All measurements contain error and thus uncertainty. We can calculate errors depending on
the nature of the experiment. We define two main types of uncertainty:
Precision is how well independent measurements (E, and E2) match. Precision can be
quantified using
formula: Percent Difference =
E-E
x100
(E, +E)/2
Percent difference is used when there is not an accepted value; it is used to compare two
independent quantities.
Accuracy is how close a measurement (E) is to an accepted value (A). Accuracy can be
quantified using the formula: Percent Error =|A- E|/A×100
Percent error is used to compare a quantity/measurement to an accepted value.
Transcribed Image Text:Background: GmM Newton formulated the Universal Law of Gravitation: F = R2 where, F = the gravitational force between two masses. G = the gravitational constant, G = 6.67 x 101" N• m²/kg? the mass of one object mass of other object distance between the center of the objects m %3D M = R = Also, we learned that weight, w=mg. Equating weight with Newton's Law of Gravitation we get: mg = GmM or canceling m: R2 GM g = R2 This can be used to calculate the acceleration of gravity on any planet/object/body. Objective: Investigate several phenomena using Newton's Universal Law of Gravitation. Understand the difference between accuracy and precision. Procedure: Perform the indicated calculations. The following information can be used for the calculations. 1.99 x 100 kg 5.98 x 1024 kg 7.36 x 102 kg 2 x 100 kg 1.90 x 1027 kg Mass of Sun 1.50 x 10" m 6.38 x 10° m 1.74 x 10 m 12,000 m 6.3 x 10 m Earth-Sun distance Radius of Earth Mass of Earth Mass of Moon Radius of Moon Radius of neutron star Mass of neutron star Mass of Jupiter Earth-Jupiter distance (in-line) Error and Uncertainty: All measurements contain error and thus uncertainty. We can calculate errors depending on the nature of the experiment. We define two main types of uncertainty: Precision is how well independent measurements (E, and E2) match. Precision can be quantified using formula: Percent Difference = E-E x100 (E, +E)/2 Percent difference is used when there is not an accepted value; it is used to compare two independent quantities. Accuracy is how close a measurement (E) is to an accepted value (A). Accuracy can be quantified using the formula: Percent Error =|A- E|/A×100 Percent error is used to compare a quantity/measurement to an accepted value.
mass of the body being orbited and R is the average distance from the body. A) Calculate
Earth's orbital velocity around the Sun. B) How fast is Earth traveling in m.p.h.? C)
Calculate Earth's orbital velocity using a second method. (Hint: The Earth orbits the
Sun in approximately a circle every 365 days. Speed = Distance/Time. Distance = the
circumference of Earth's orbit = 2rR and Time is number of seconds in a year.) D)
Compare the orbital velocities (speeds) from Parts A and C by calculating the percent
difference of the two velocities and comment (are they about the same?).
Earth
M (Sun)
3. Astrologers claim that when Jupiter is 'lined-up' with the Earth and Sun, its gravitational
pull on humans is significant, and thus affects our life. A) Calculate the gravitational pull
from Jupiter on a human (m=70 kg) when Jupiter is 'in-line' with the Earth and Sun. B)
Calculate the gravitational pull from a skyscraper on a human walking through any
downtown, or city center (Assume a skyscraper has a mass of 1.2 x 10° kg, and the
distance between the center of masses is 175 m). C) Calculate the pull from a large cliff
(M=8.8 x 10' kg and R=14 m). D) How many times bigger are the answers in B and C
than the answer in part A? Comment on these results.
m = 70 kg
R
A)
M (Jupiter)
m = 70 kg
B)
M (skyscraper)
m = 70 kg
C)
M (cliff)
ourses/1045543/pages/labs
%
&
*
Transcribed Image Text:mass of the body being orbited and R is the average distance from the body. A) Calculate Earth's orbital velocity around the Sun. B) How fast is Earth traveling in m.p.h.? C) Calculate Earth's orbital velocity using a second method. (Hint: The Earth orbits the Sun in approximately a circle every 365 days. Speed = Distance/Time. Distance = the circumference of Earth's orbit = 2rR and Time is number of seconds in a year.) D) Compare the orbital velocities (speeds) from Parts A and C by calculating the percent difference of the two velocities and comment (are they about the same?). Earth M (Sun) 3. Astrologers claim that when Jupiter is 'lined-up' with the Earth and Sun, its gravitational pull on humans is significant, and thus affects our life. A) Calculate the gravitational pull from Jupiter on a human (m=70 kg) when Jupiter is 'in-line' with the Earth and Sun. B) Calculate the gravitational pull from a skyscraper on a human walking through any downtown, or city center (Assume a skyscraper has a mass of 1.2 x 10° kg, and the distance between the center of masses is 175 m). C) Calculate the pull from a large cliff (M=8.8 x 10' kg and R=14 m). D) How many times bigger are the answers in B and C than the answer in part A? Comment on these results. m = 70 kg R A) M (Jupiter) m = 70 kg B) M (skyscraper) m = 70 kg C) M (cliff) ourses/1045543/pages/labs % & *
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