1. Instructor Solutions Manual
for
Physics
by
Halliday, Resnick, and Krane
Paul Stanley
Beloit College
Volume 1: Chapters 1-24

2. A Note To The Instructor...
The solutions here are somewhat brief, as they are designed for the instructor, not for the student.
Check with the publishers before electronically posting any part of these solutions; website, ftp, or
server access must be restricted to your students.
I have been somewhat casual about subscripts whenever it is obvious that a problem is one
dimensional, or that the choice of the coordinate system is irrelevant to the numerical solution.
Although this does not change the validity of the answer, it will sometimes obfuscate the approach
if viewed by a novice.
There are some traditional formula, such as
2 2
vx = v0x + 2ax x,
which are not used in the text. The worked solutions use only material from the text, so there may
be times when the solution here seems unnecessarily convoluted and drawn out. Yes, I know an
easier approach existed. But if it was not in the text, I did not use it here.
I also tried to avoid reinventing the wheel. There are some exercises and problems in the text
which build upon previous exercises and problems. Instead of rederiving expressions, I simply refer
you to the previous solution.
I adopt a different approach for rounding of significant figures than previous authors; in partic-
ular, I usually round intermediate answers. As such, some of my answers will differ from those in
the back of the book.
Exercises and Problems which are enclosed in a box also appear in the Student’s Solution Manual
with considerably more detail and, when appropriate, include discussion on any physical implications
of the answer. These student solutions carefully discuss the steps required for solving problems, point
out the relevant equation numbers, or even specify where in the text additional information can be
found. When two almost equivalent methods of solution exist, often both are presented. You are
encouraged to refer students to the Student’s Solution Manual for these exercises and problems.
However, the material from the Student’s Solution Manual must not be copied.
Paul Stanley
Beloit College
stanley@clunet.edu
1

3. E1-1 (a) Megaphones; (b) Microphones; (c) Decacards (Deck of Cards); (d) Gigalows (Gigolos);
(e) Terabulls (Terribles); (f) Decimates; (g) Centipedes; (h) Nanonanettes (?); (i) Picoboos (Peek-a-
Boo); (j) Attoboys (’atta boy); (k) Two Hectowithits (To Heck With It); (l) Two Kilomockingbirds
(To Kill A Mockingbird, or Tequila Mockingbird).
E1-2 (a) $36, 000/52 week = $692/week. (b) $10, 000, 000/(20 × 12 month) = $41, 700/month. (c)
30 × 109 /8 = 3.75 × 109 .
E1-3 Multiply out the factors which make up a century.
365 days 24 hours 60 minutes
1 century = 100 years
1 year 1 day 1 hour
This gives 5.256 × 107 minutes in a century, so a microcentury is 52.56 minutes.
The percentage difference from Fermi’s approximation is (2.56 min)/(50 min) × 100% or 5.12%.
E1-4 (3000 mi)/(3 hr) = 1000 mi/timezone-hour. There are 24 time-zones, so the circumference
is approximately 24 × 1000 mi = 24, 000 miles.
E1-5 Actual number of seconds in a year is
24 hr 60 min 60 s
(365.25 days) = 3.1558 × 107 s.
1 day 1 hr 1 min
The percentage error of the approximation is then
3.1416 × 107 s − 3.1558 × 107 s
= −0.45 %.
3.1558 × 107 s
E1-6 (a) 10−8 seconds per shake means 108 shakes per second. There are
365 days 24 hr 60 min 60 s
= 3.1536 × 107 s/year.
1 year 1 day 1 hr 1 min
This means there are more shakes in a second.
(b) Humans have existed for a fraction of
106 years/1010 years = 10−4 .
That fraction of a day is
60 min 60 s
10−4 (24 hr) = 8.64 s.
1 hr 1 min
E1-7 We’ll assume, for convenience only, that the runner with the longer time ran exactly one
mile. Let the speed of the runner with the shorter time be given by v1 , and call the distance actually
ran by this runner d1 . Then v1 = d1 /t1 . Similarly, v2 = d2 /t2 for the other runner, and d2 = 1 mile.
We want to know when v1 > v2 . Substitute our expressions for speed, and get d1 /t1 > d2 /t2 .
Rearrange, and d1 /d2 > t1 /t2 or d1 /d2 > 0.99937. Then d1 > 0.99937 mile × (5280 feet/1 mile) or
d1 > 5276.7 feet is the condition that the first runner was indeed faster. The first track can be no
more than 3.3 feet too short to guarantee that the first runner was faster.
2

4. E1-8 We will wait until a day’s worth of minutes have been gained. That would be
60 min
(24 hr) = 1440 min.
1 hr
The clock gains one minute per day, so we need to wait 1,440 days, or almost four years. Of course,
if it is an older clock with hands that only read 12 hours (instead of 24), then after only 720 days
the clock would be correct.
E1-9 First find the “logarithmic average” by
1
log tav = log(5 × 1017 ) + log(6 × 10−15 ) ,
2
1
= log 5 × 1017 × 6 × 10−15 ,
2
1 √
= log 3000 = log 3000 .
2
Solve, and tav = 54.8 seconds.
E1-10 After 20 centuries the day would have increased in length by a total of 20 × 0.001 s = 0.02 s.
The cumulative effect would by the product of the average increase and the number of days; that
average is half of the maximum, so the cumulative effect is 1 (2000)(365)(0.02 s) = 7300 s. That’s
2
about 2 hours.
E1-11 Lunar months are based on the Earth’s position, and as the Earth moves around the orbit
the Moon has farther to go to complete a phase. In 27.3 days the Moon may have orbited through
360◦ , but since the Earth moved through (27.3/365) × 360◦ = 27◦ the Moon needs to move 27◦
farther to catch up. That will take (27◦ /360◦ ) × 27.3 days = 2.05 days, but in that time the Earth
would have moved on yet farther, and the moon will need to catch up again. How much farther?
(2.05/365) × 360◦ = 2.02◦ which means (2.02◦ /360◦ ) × 27.3 days = 0.153 days. The total so far is
2.2 days longer; we could go farther, but at our accuracy level, it isn’t worth it.
E1-12 (1.9 m)(3.281 ft/1.000 m) = 6.2 ft, or just under 6 feet, 3 inches.
E1-13 (a) 100 meters = 328.1 feet (Appendix G), or 328.1/3 = 10.9 yards. This is 28 feet longer
than 100 yards, or (28 ft)(0.3048 m/ft) = 8.5 m. (b) A metric mile is (1500 m)(6.214×10−4 mi/m) =
0.932 mi. I’d rather run the metric mile.
E1-14 There are
365.25 days 24 hr 60 min 60 s
300, 000 years = 9.5 × 1012 s
1 year 1 day 1 hr 1 min
that will elapse before the cesium clock is in error by 1 s. This is almost 1 part in 1013 . This kind
of accuracy with respect to 2572 miles is
1609 m
10−13 (2572 mi) = 413 nm.
1 mi
3

5. E1-15 The volume of Antarctica is approximated by the area of the base time the height; the
area of the base is the area of a semicircle. Then
1 2
V = Ah = πr h.
2
The volume is
1
V = (3.14)(2000 × 1000 m)2 (3000 m) = 1.88 × 1016 m3
2
3
100 cm
= 1.88 × 1016 m3 × = 1.88 × 1022 cm3 .
1m
E1-16 The volume is (77×104 m2 )(26 m) = 2.00×107 m3 . This is equivalent to
(2.00×107 m3 )(10−3 km/m)3 = 0.02 km3 .
E1-17 (a) C = 2πr = 2π(6.37 × 103 km) = 4.00 × 104 km. (b) A = 4πr2 = 4π(6.37 × 103 km)2 =
5.10 × 108 km. (c) V = 3 π(6.37 × 103 km)3 = 1.08 × 1012 km3 .
4
E1-18 The conversions: squirrel, 19 km/hr(1000 m/km)/(3600 s/hr) = 5.3 m/s;
rabbit, 30 knots(1.688ft/s/knot)(0.3048 m/ft) = 15 m/s;
snail, 0.030 mi/hr(1609 m/mi)/(3600 s/hr) = 0.013 m/s;
spider, 1.8 ft/s(0.3048 m/ft) = 0.55 m/s;
cheetah, 1.9 km/min(1000 m/km)/(60 s/min) = 32 m/s;
human, 1000 cm/s/(100 cm/m) = 10 m/s;
fox, 1100 m/min/(60 s/min) = 18 m/s;
lion, 1900 km/day(1000 m/km)/(86, 400 s/day) = 22 m/s.
The order is snail, spider, squirrel, human, rabbit, fox, lion, cheetah.
E1-19 One light-year is the distance traveled by light in one year, or (3 × 108 m/s) × (1 year).
Then
mi light-year 1609 m 1 hr 100 year
19, 200 ,
hr (3 × 108 m/s) × (1 year) 1 mi 3600 s 1 century
which is equal to 0.00286 light-year/century.
E1-20 Start with the British units inverted,
gal 231 in3 1.639 × 10−2 L mi
= 7.84 × 10−2 L/km.
30.0 mi gal in3 1.609 km
E1-21 (b) A light-year is
3600 s 24 hr
(3.00 × 105 km/s) (365 days) = 9.46 × 1012 km.
1 hr 1 day
A parsec is
1.50 × 108 km 360◦ 1.50 × 108 km 360◦
= = 3.09 × 1013 km.
0◦ 0 1 2π rad (1/3600)◦ 2π rad
(a) (1.5 × 108 km)/(3.09 × 1013 km/pc = 4.85 × 10−6 pc. (1.5 × 108 km)/(9.46 × 1012 km/ly) =
1.59 × 10−5 ly.
4

6. E1-22 First find the “logarithmic average” by
1
log dav = log(2 × 1026 ) + log(1 × 10−15 ) ,
2
1
= log 2 × 1026 × 1 × 10−15 ,
2
1
= log 2 × 1011 = log 2 × 1011 .
2
Solve, and dav = 450 km.
E1-23 The number of atoms is given by (1 kg)/(1.00783 × 1.661 × 10−27 kg), or 5.974 × 1026
atoms.
E1-24 (a) (2 × 1.0 + 16)u(1.661 × 10−27 kg) = 3.0 × 10−26 kg.
(b) (1.4 × 1021 kg)/(3.0 × 10−26 kg) = 4.7 × 1046 molecules.
E1-25 The coffee in Paris costs $18.00 per kilogram, or
0.4536 kg
$18.00 kg−1 = $8.16 lb−1 .
1 lb
It is cheaper to buy coffee in New York (at least according to the physics textbook, that is.)
E1-26 The room volume is (21 × 13 × 12)ft3 (0.3048 m/ft)3 = 92.8 m3 . The mass contained in the
room is
(92.8 m3 )(1.21 kg/m3 ) = 112 kg.
E1-27 One mole of sugar cubes would have a volume of NA × 1.0 cm3 , where NA is the Avogadro
√
constant. Since the volume of a cube is equal to the length cubed, V = l3 , then l = 3 NA cm
= 8.4 × 107 cm.
E1-28 The number of seconds in a week is 60 × 60 × 24 × 7 = 6.05 × 105 . The “weight” loss per
second is then
(0.23 kg)/(6.05 × 105 s) = 3.80 × 10−1 mg/s.
E1-29 The definition of the meter was wavelengths per meter; the question asks for meters per
wavelength, so we want to take the reciprocal. The definition is accurate to 9 figures, so the reciprocal
should be written as 1/1, 650, 763.73 = 6.05780211 × 10−7 m = 605.780211 nm.
E1-30 (a) 37.76 + 0.132 = 37.89. (b) 16.264 − 16.26325 = 0.001.
E1-31 The easiest approach is to first solve Darcy’s Law for K, and then substitute the known
SI units for the other quantities. Then
VL m3 (m)
K= has units of
AHt (m2 ) (m) (s)
which can be simplified to m/s.
5

7. E1-32 The Planck length, lP , is found from
[lP ] = [ci ][Gj ][hk ],
L = (LT−1 )i (L3 T−2 M−1 )j (ML2 T−1 )k ,
= Li+3j+2k T−i−2j−k M−j+k .
Equate powers on each side,
L: 1 = i + 3j + 2k,
T: 0 = −i − 2j − k,
M: 0 = −j + k.
Then j = k, and i = −3k, and 1 = 2k; so k = 1/2, j = 1/2, and i = −3/2. Then
[lP ] = [c−3/2 ][G1/2 ][h1/2 ],
= (3.00 × 108 m/s)−3/2 (6.67 × 10−11 m3 /s2 · kg)1/2 (6.63 × 10−34 kg · m2 /s)1/2 ,
= 4.05 × 10−35 m.
E1-33 The Planck mass, mP , is found from
[mP ] = [ci ][Gj ][hk ],
M = (LT−1 )i (L3 T−2 M−1 )j (ML2 T−1 )k ,
= Li+3j+2k T−i−2j−k M−j+k .
Equate powers on each side,
L: 0 = i + 3j + 2k,
T: 0 = −i − 2j − k,
M: 1 = −j + k.
Then k = j + 1, and i = −3j − 1, and 0 = −1 + 2k; so k = 1/2, and j = −1/2, and i = 1/2. Then
[mP ] = [c1/2 ][G−1/2 ][h1/2 ],
= (3.00 × 108 m/s)1/2 (6.67 × 10−11 m3 /s2 · kg)−1/2 (6.63 × 10−34 kg · m2 /s)1/2 ,
= 5.46 × 10−8 kg.
P1-1 There are 24 × 60 = 1440 traditional minutes in a day. The conversion plan is then fairly
straightforward
1440 trad. min
822.8 dec. min = 1184.8 trad. min.
1000 dec. min
This is traditional minutes since midnight, the time in traditional hours can be found by dividing
by 60 min/hr, the integer part of the quotient is the hours, while the remainder is the minutes. So
the time is 19 hours, 45 minutes, which would be 7:45 pm.
P1-2 (a) By similar triangles, the ratio of the distances is the same as the ratio of the diameters—
390:1.
(b) Volume is proportional to the radius (diameter) cubed, or 3903 = 5.93 × 107 .
(c) 0.52◦ (2π/360◦ ) = 9.1 × 10−3 rad. The diameter is then (9.1 × 10−3 rad)(3.82 × 105 km) =
3500 km.
6

8. P1-3 (a) The circumference of the Earth is approximately 40,000 km; 0.5 seconds of an arc is
0.5/(60 × 60 × 360) = 3.9 × 10−7 of a circumference, so the north-south error is ±(3.9 × 10−7 )(4 ×
107 m) = ±15.6 m. This is a range of 31 m.
(b) The east-west range is smaller, because the distance measured along a latitude is smaller than
the circumference by a factor of the cosine of the latitude. Then the range is 31 cos 43.6◦ = 22 m.
(c) The tanker is in Lake Ontario, some 20 km off the coast of Hamlin?
P1-4 Your position is determined by the time it takes for your longitude to rotate ”underneath”
the sun (in fact, that’s the way longitude was measured originally as in 5 hours west of the Azores...)
the rate the sun sweep over at equator is 25,000 miles/86,400 s = 0.29 miles/second. The correction
factor because of latitude is the cosine of the latitude, so the sun sweeps overhead near England at
approximately 0.19 mi/s. Consequently a 30 mile accuracy requires an error in time of no more than
(30 mi)/(0.19 mi/s) = 158 seconds.
Trip takes about 6 months, so clock accuracy needs to be within (158 s)/(180 day) = 1.2 sec-
onds/day.
(b) Same, except 0.5 miles accuracy requires 2.6 s accuracy, so clock needs to be within 0.007
s/day!
P1-5 Let B be breaths/minute while sleeping. Each breath takes in (1.43 g/L)(0.3 L) = 0.429 g;
and lets out (1.96 g/L)(0.3 L) = 0.288 g. The net loss is 0.141 g. Multiply by the number of breaths,
(8 hr)(60 min./hr)B(0.141 g) = B(67.68 g). I’ll take a short nap, and count my breaths, then finish
the problem.
I’m back now, and I found my breaths to be 8/minute. So I lose 541 g/night, or about 1 pound.
P1-6 The mass of the water is (1000 kg/m3 )(5700 m3 ) = 5.7 × 106 kg. The rate that water leaks
drains out is
(5.7 × 106 kg)
= 132 kg/s.
(12 hr)(3600 s/hr)
2
P1-7 Let the radius of the grain be given by rg . Then the surface area of the grain is Ag = 4πrg ,
3
and the volume is given by Vg = (4/3)πrg .
If N grains of sand have a total surface area equal to that of a cube 1 m on a edge, then
N Ag = 6 m2 . The total volume Vt of this number of grains of sand is N Vg . Eliminate N from these
two expressions and get
(6 m2 ) (6 m2 )rg
Vt = N V g = Vg = .
Ag 3
Then Vt = (2 m2 )(50 × 10−6 m) = 1 × 10−4 m3 .
The mass of a volume Vt is given by
2600 kg
1 × 10−4 m3 = 0.26 kg.
1 m3
P1-8 For a cylinder V = πr2 h, and A = 2πr2 + 2πrh. We want to minimize A with respect to
changes in r, so
dA d V
= 2πr2 + 2πr ,
dr dr πr2
V
= 4πr − 2 .
r2
Set this equal to zero; then V = 2πr3 . Notice that h = 2r in this expression.
7

9. P1-9 (a) The volume per particle is
(9.27 × 10−26 kg)/(7870 kg/m3 ) = 1.178 × 10−28 m3 .
The radius of the corresponding sphere is
3(1.178 × 10−28 m3 )
= 1.41 × 10−10 m.
3
r=
4π
Double this, and the spacing is 282 pm.
(b) The volume per particle is
(3.82 × 10−26 kg)/(1013 kg/m3 ) = 3.77 × 10−29 m3 .
The radius of the corresponding sphere is
3(3.77 × 10−29 m3 )
= 2.08 × 10−10 m.
3
r=
4π
Double this, and the spacing is 416 pm.
P1-10 (a) The area of the plate is (8.43 cm)(5.12 cm) = 43.2 cm2 . (b) (3.14)(3.7 cm)2 = 43 cm2 .
8

10. E2-1 Add the vectors as is shown in Fig. 2-4. If a has length a = 4 m and b has length b = 3 m
then the sum is given by s. The cosine law can be used to find the magnitude s of s,
s2 = a2 + b2 − 2ab cos θ,
where θ is the angle between sides a and b in the figure.
(a) (7 m)2 = (4 m)2 + (3 m)2 − 2(4 m)(3 m) cos θ, so cos θ = −1.0, and θ = 180◦ . This means
that a and b are pointing in the same direction.
(b) (1 m)2 = (4 m)2 + (3 m)2 − 2(4 m)(3 m) cos θ, so cos θ = 1.0, and θ = 0◦ . This means that
a and b are pointing in the opposite direction.
(c) (5 m)2 = (4 m)2 + (3 m)2 − 2(4 m)(3 m) cos θ, so cos θ = 0, and θ = 90◦ . This means that a
and b are pointing at right angles to each other.
E2-2 (a) Consider the figures below.
(b) Net displacement is 2.4 km west, (5.2 − 3.1 = 2.1) km south. A bird would fly
2.42 + 2.12 km = 3.2 km.
E2-3 Consider the figure below.
a
a+b b -b
a-b
a
E2-4 (a) The components are (7.34) cos(252◦ ) = −2.27ˆ and (7.34) sin(252◦ ) = −6.98ˆ
i j.
(b) The magnitude is (−25)2 + (43)2 = 50; the direction is θ = tan−1 (43/ − 25) = 120◦ . We
did need to choose the correct quadrant.
E2-5 The components are given by the trigonometry relations
O = H sin θ = (3.42 km) sin 35.0◦ = 1.96 km
and
A = H cos θ = (3.42 km) cos 35.0◦ = 2.80 km.
9

11. The stated angle is measured from the east-west axis, counter clockwise from east. So O is measured
against the north-south axis, with north being positive; A is measured against east-west with east
being positive.
Since her individual steps are displacement vectors which are only north-south or east-west, she
must eventually take enough north-south steps to equal 1.96 km, and enough east-west steps to
equal 2.80 km. Any individual step can only be along one or the other direction, so the minimum
total will be 4.76 km.
E2-6 Let rf = 124ˆ km and ri = (72.6ˆ + 31.4ˆ km. Then the ship needs to travel
i i j)
∆r = rf − ri = (51.4ˆ + 31.4ˆ km.
i j)
√
Ship needs to travel 51.42 + 31.42 km = 60.2 km in a direction θ = tan−1 (31.4/51.4) = 31.4◦ west
of north.
E2-7 (a) In unit vector notation we need only add the components; a+ b = (5ˆ ˆ
i+3j)+(−3ˆ ˆ =
i+2j)
(5 − 3)ˆ + (3 + 2)ˆ = 2ˆ + 5ˆ
i j i j.
√
(b) If we define c = a + b and write the magnitude of c as c, then c = c2 + c2 = 22 + 52 =
x y
5.39. The direction is given by tan θ = cy /cx which gives an angle of 68.2◦ , measured counterclock-
wise from the positive x-axis.
E2-8 (a) a + b = (4 − 1)ˆ + (−3 + 1)ˆ + (1 + 4)k = 3ˆ − 2ˆ + 5k.
i j ˆ i j ˆ
ˆ + (−3 − 1)ˆ + (1 − 4)k = 5ˆ − 4ˆ − 3k.
(b) a − b = (4 − −1)i j ˆ i j ˆ
(c) Rearrange, and c = b − a, or b − a = (−1 − 4)ˆ + (1 − −3)ˆ + (4 − 1)k = −5ˆ + 4ˆ + 3k.
i j ˆ i j ˆ
E2-9 (a) The magnitude of a is 4.02 + (−3.0)2 = 5.0; the direction is θ = tan−1 (−3.0/4.0) =
323◦ . √
(b) The magnitude of b is 6.02 + 8.03 = 10.0; the direction is θ = tan−1 (6.0/8.0) = 36.9◦ .
(c) The resultant vector is a + b = (4.0 + 6.0)ˆ + (−3.0 + 8.0)ˆ The magnitude of a + b
i j. is
(10.0)2 + (5.0)2 = 11.2; the direction is θ = tan−1 (5.0/10.0) = 26.6◦ .
(d) The resultant vector is a − b = (4.0 − 6.0)ˆ + (−3.0 − 8.0)ˆ The magnitude of a − b
i j. is
(−2.0)2 + (−11.0)2 = 11.2; the direction is θ = tan−1 (−11.0/ − 2.0) = 260◦ .
(e) The resultant vector is b − a = (6.0 − 4.0)ˆ + (8.0 − −3.0)ˆ The magnitude of b − a
i j. is
(2.0)2 + (11.0)2 = 11.2; the direction is θ = tan−1 (11.0/2.0) = 79.7◦ .
E2-10 (a) Find components of a; ax = (12.7) cos(28.2◦ ) = 11.2, ay = (12.7) sin(28.2◦ ) = 6.00.
Find components of b; bx = (12.7) cos(133◦ ) = −8.66, by = (12.7) sin(133◦ ) = 9.29. Then
r = a + b = (11.2 − 8.66)ˆ + (6.00 + 9.29)ˆ = 2.54ˆ + 15.29ˆ
i j i j.
√
(b) The magnitude of r is 2.542 + 15.292 = 15.5.
(c) The angle is θ = tan−1 (15.29/2.54) = 80.6◦ .
E2-11 Consider the figure below.
10

12. E2-12 Consider the figure below.
E2-13 Our axes will be chosen so that ˆ points toward 3 O’clock and ˆ points toward 12 O’clock.
i j
(a)
The two relevant positions are ri = (11.3 cm)ˆ and rf = (11.3 cm)ˆ Then
i j.
∆r = rf − ri
= (11.3 cm)ˆ − (11.3 cm)ˆ
j i.
(b)
The two relevant positions are now ri = (11.3 cm)ˆ and rf = (−11.3 cm)ˆ Then
j j.
∆r = rf − ri
= (11.3 cm)ˆ − (−11.3 cm)ˆ
j j
ˆ
= (22.6 cm)j.
(c)
The two relevant positions are now ri = (−11.3 cm)ˆ and rf = (−11.3 cm)ˆ Then
j j.
∆r = rf − ri
= (−11.3 cm)ˆ − (−11.3 cm)ˆ
j j
= (0 cm)j.ˆ
E2-14 (a) The components of r1 are
r1x = (4.13 m) cos(225◦ ) = −2.92 m
and
r1y = (4.13 m) sin(225◦ ) = −2.92 m.
11

13. The components of r2 are
r1x = (5.26 m) cos(0◦ ) = 5.26 m
and
r1y = (5.26 m) sin(0◦ ) = 0 m.
The components of r3 are
r1x = (5.94 m) cos(64.0◦ ) = 2.60 m
and
r1y = (5.94 m) sin(64.0◦ ) = 5.34 m.
(b) The resulting displacement is
(−2.92 + 5.26 + 2.60)ˆ + (−2.92 + 0 + 5.34)ˆ m = (4.94ˆ + 2.42ˆ m.
i j i j)
√
(c) The magnitude of the resulting displacement is 4.942 + 2.422 m = 5.5 m. The direction of
the resulting displacement is θ = tan−1 (2.42/4.94) = 26.1◦ . (d) To bring the particle back to the
starting point we need only reverse the answer to (c); the magnitude will be the same, but the angle
will be 206◦ .
E2-15 The components of the initial position are
r1x = (12, 000 ft) cos(40◦ ) = 9200 ft
and
r1y = (12, 000 ft) sin(40◦ ) = 7700 ft.
The components of the final position are
r2x = (25, 8000 ft) cos(163◦ ) = −24, 700 ft
and
r2y = (25, 800 ft) sin(163◦ ) = 7540 ft.
The displacement is
r = r2 − r1 = (−24, 700 − 9, 200)ˆ + (7, 540 − 9, 200)ˆ = (−33900ˆ − 1660ˆ ft.
i j) i j)
E2-16 (a) The displacement vector is r = (410ˆ − 820ˆ mi, where positive x is east and positive
i j)
y is north. The magnitude of the displacement is (410)2 + (−820)2 mi = 920 mi. The direction is
θ = tan−1 (−820/410) = 300◦ .
(b) The average velocity is the displacement divided by the total time, 2.25 hours. Then
vav = (180ˆ − 360ˆ mi/hr.
i j)
(c) The average speed is total distance over total time, or (410 + 820)/(2.25) mi/hr = 550 mi/hr.
12

14. E2-17 (a) Evaluate r when t = 2 s.
3 4
r = [(2 m/s )t3 − (5 m/s)t]ˆ + [(6 m) − (7 m/s )t4 ]ˆ
i j
3 3 ˆ + [(6 m) − (7 m/s4 )(2 s)4 ]ˆ
= [(2 m/s )(2 s) − (5 m/s)(2 s)]i j
ˆ + [(6 m) − (112 m)]ˆ
= [(16 m) − (10 m)]i j
= [(6 m)]ˆ + [−(106 m)]ˆ
i j.
(b) Evaluate:
dr 3 4
v= = [(2 m/s )3t2 − (5 m/s)]ˆ + [−(7 m/s )4t3 ]ˆ
i j
dt
3 4
= [(6 m/s )t2 − (5 m/s)]ˆ + [−(28 m/s )t3 ]ˆ
i j.
Into this last expression we now evaluate v(t = 2 s) and get
3 4
v = [(6 m/s )(2 s)2 − (5 m/s)]ˆ + [−(28 m/s )(2 s)3 ]ˆ
i j
= [(24 m/s) − (5 m/s)]ˆ + [−(224 m/s)]ˆ
i j
= [(19 m/s)]ˆ + [−(224 m/s)]ˆ
i j,
for the velocity v when t = 2 s.
(c) Evaluate
dv 3 4
a= = [(6 m/s )2t]ˆ + [−(28 m/s )3t2 ]ˆ
i j
dt
3 4
= [(12 m/s )t]ˆ + [−(84 m/s )t2 ]ˆ
i j.
Into this last expression we now evaluate a(t = 2 s) and get
3 4
a = [(12 m/s )(2 s)]ˆ + [−(84 m/s )(2 2)2 ]ˆ
i j
2 ˆ 2 ˆ
= [(24 m/s )]i + [−(336 m/s )]j.
E2-18 (a) Let ui point north, ˆ point east, and k point up. The displacement is (8.7ˆ + 9.7ˆ +
j ˆ i j
ˆ km. The average velocity is found by dividing each term by 3.4 hr; then
2.9k)
vav = (2.6ˆ + 2.9ˆ + 0.85) km/hr.
i j
√
The magnitude of the average velocity is 2.62 + √ 2 + 0.852 km/hr = 4.0 km/hr.
2.9
(b) The horizontal velocity has a magnitude of 2.62 + 2.92 km/hr = 3.9 km/hr. The angle with
the horizontal is given by θ = tan−1 (0.85/3.9) = 13◦ .
E2-19 (a) The derivative of the velocity is
a = [(6.0 m/s2 ) − (8.0 m/s3 )t]ˆ
i
so the acceleration at t = 3 s is a = (−18.0 m/s2 )ˆ (b) The acceleration is zero when (6.0 m/s2 ) −
i.
(8.0 m/s3 )t = 0, or t = 0.75 s. (c) The velocity is never zero; there is no way to “cancel” out the
y component. (d) The speed equals 10 m/s when 10 = vx + 82 , or vx = ±6.0 m/s. This happens
2
2 3
when (6.0 m/s ) − (8.0 m/s )t = ±6.0 m/s, or when t = 0 s.
13

15. E2-20 If v is constant then so is v 2 = vx + vy . Take the derivative;
2 2
d d
2vx vx + 2vy vy = 2(vx ax + vy ay ).
dt dt
But if the value is constant the derivative is zero.
E2-21 Let the actual flight time, as measured by the passengers, be T . There is some time
difference between the two cities, call it ∆T = Namulevu time - Los Angeles time. The ∆T will be
positive if Namulevu is east of Los Angeles. The time in Los Angeles can then be found from the
time in Namulevu by subtracting ∆T .
The actual time of flight from Los Angeles to Namulevu is then the difference between when the
plane lands (LA times) and when the plane takes off (LA time):
T = (18:50 − ∆T ) − (12:50)
= 6:00 − ∆T,
where we have written times in 24 hour format to avoid the AM/PM issue. The return flight time
can be found from
T = (18:50) − (1:50 − ∆T )
= 17:00 + ∆T,
where we have again changed to LA time for the purpose of the calculation.
(b) Now we just need to solve the two equations and two unknowns.
17:00 + ∆T = 6:00 − ∆T
2∆T = 6:00 − 17:00
∆T = −5:30.
Since this is a negative number, Namulevu is located west of Los Angeles.
(a) T = 6:00 − ∆T = 11 : 30, or eleven and a half hours.
(c) The distance traveled by the plane is given by d = vt = (520 mi/hr)(11.5 hr) = 5980 mi.
We’ll draw a circle around Los Angeles with a radius of 5980 mi, and then we look for where it
intersects with longitudes that would belong to a time zone ∆T away from Los Angeles. Since the
Earth rotates once every 24 hours and there are 360 longitude degrees, then each hour corresponds
to 15 longitude degrees, and then Namulevu must be located approximately 15◦ × 5.5 = 83◦ west of
Los Angeles, or at about longitude 160 east. The location on the globe is then latitude 5◦ , in the
vicinity of Vanuatu.
When this exercise was originally typeset the times for the outbound and the inbound flights were
inadvertently switched. I suppose that we could blame this on the airlines; nonetheless, when the answers
were prepared for the back of the book the reversed numbers put Namulevu east of Los Angeles. That would
put it in either the North Atlantic or Brazil.
E2-22 There is a three hour time zone difference. So the flight is seven hours long, but it takes
3 hr 51 min for the sun to travel same distance. Look for when the sunset distance has caught up
with plane:
dsunset = dplane ,
v sunset (t − 1:35) = v plane t,
(t − 1:35)/3:51 = t/7:00,
so t = 3:31 into flight.
14

16. E2-23 The distance is
d = vt = (112 km/hr)(1 s)/(3600 s/hr) = 31 m.
E2-24 The time taken for the ball to reach the plate is
d (18.4 m)
t= = (3600 s/hr)/(1000 m/km) = 0.414 s.
v (160 km/hr)
E2-25 Speed is distance traveled divided by time taken; this is equivalent to the inverse of the
slope of the line in Fig. 2-32. The line appears to pass through the origin and through the point
(1600 km, 80 × 106 y), so the speed is v = 1600 km/80 × 106 y= 2 × 10−5 km/y. Converting,
1000 m 100 cm
v = 2 × 10−5 km/y = 2 cm/y
1 km 1m
E2-26 (a) For Maurice Greene v av = (100 m)/(9.81 m) = 10.2 m/s. For Khalid Khannouchi,
(26.219 mi) 1609 m 1hr
v av = = 5.594 m/s.
(2.0950 hr) 1 mi 3600 s
(b) If Maurice Greene ran the marathon with an average speed equal to his average sprint speed
then it would take him
(26.219 mi) 1609 m 1hr
t= = 1.149 hr,
10.2 m/s 1 mi 3600 s
or 1 hour, 9 minutes.
E2-27 The time saved is the difference,
(700 km) (700 km)
∆t = − = 1.22 hr,
(88.5 km/hr) (104.6 km/hr)
which is about 1 hour 13 minutes.
E2-28 The ground elevation will increase by 35 m in a horizontal distance of
x = (35.0 m)/ tan(4.3◦ ) = 465 m.
The plane will cover that distance in
(0.465 km) 3600 s
t= = 1.3 s.
(1300 km/hr) 1hr
E2-29 Let v1 = 40 km/hr be the speed up the hill, t1 be the time taken, and d1 be the distance
traveled in that time. We similarly define v2 = 60 km/hr for the down hill trip, as well as t2 and d2 .
Note that d2 = d1 .
15

17. v1 = d1 /t1 and v2 = d2 /t2 . v av = d/t, where d total distance and t is the total time. The total
distance is d1 + d2 = 2d1 . The total time t is just the sum of t1 and t2 , so
d
v av =
t
2d1
=
t 1 + t2
2d1
=
d1 /v1 + d2 /v2
2
= ,
1/v1 + 1/v2
Take the reciprocal of both sides to get a simpler looking expression
2 1 1
= + .
v av v1 v2
Then the average speed is 48 km/hr.
E2-30 (a) Average speed is total distance divided by total time. Then
(240 ft) + (240 ft)
v av = = 5.7 ft/s.
(240 ft)/(4.0 ft/s) + (240 ft)/(10 ft/s)
(b) Same approach, but different information given, so
(60 s)(4.0 ft/s) + (60 s)(10 ft/s)
v av = = 7.0 ft/s.
(60 s) + (60 s)
E2-31 The distance traveled is the total area under the curve. The “curve” has four regions: (I)
a triangle from 0 to 2 s; (II) a rectangle from 2 to 10 s; (III) a trapezoid from 10 to 12 s; and (IV)
a rectangle from 12 to 16 s.
The area underneath the curve is the sum of the areas of the four regions.
1 1
d= (2 s)(8 m/s) + (8.0 s)(8 m/s) + (2 s)(8 m/s + 4 m/s) + (4.0 s)(4 m/s) = 100 m.
2 2
E2-32 The acceleration is the slope of a velocity-time curve,
(8 m/s) − (4 m/s)
a= = −2 m/s2 .
(10 s) − (12 s)
E2-33 The initial velocity is vi = (18 m/s)ˆ the final velocity is vf = (−30 m/s)ˆ The average
i, i.
acceleration is then
∆v vf − vi (−30 m/s)ˆ − (18 m/s)ˆ
i i
aav = = = ,
∆t ∆t 2.4 s
which gives aav = (−20.0 m/s2 )ˆ
i.
16

18. E2-34 Consider the figure below.
10
5
0
1 2 3 4 5
-5
-10
E2-35 (a) Up to A vx > 0 and is constant. From A to B vx is decreasing, but still positive. From
B to C vx = 0. From C to D vx < 0, but |vx | is decreasing.
(b) No. Constant acceleration would appear as (part of) a parabola; but it would be challenging
to distinguish between a parabola and an almost parabola.
E2-36 (a) Up to A vx > 0 and is decreasing. From A to B vx = 0. From B to C vx > 0 and is
increasing. From C to D vx > 0 and is constant.
(b) No. Constant acceleration would appear as (part of) a parabola; but it would be challenging
to distinguish between a parabola and an almost parabola.
E2-37 Consider the figure below.
v
x
a v
E2-38 Consider the figure below.
17

19. 16 16 The acceleration
12 12 is a constant
2 cm/s/s during
8 8 the entire time
v(cm/s)
x(cm)
4 4 interval.
0 0
−4 −4
0 1 2 3 4 5 6 t(s) 0 1 2 3 4 5 6 t(s)
E2-39 (a) A must have units of m/s2 . B must have units of m/s3 .
(b) The maximum positive x position occurs when vx = 0, so
dx
vx = = 2At − 3Bt2
dt
implies vx = 0 when either t = 0 or t = 2A/3B = 2(3.0 m/s2 )/3(1.0 m/s3 ) = 2.0 s.
(c) Particle starts from rest, then travels in positive direction until t = 2 s, a distance of
x = (3.0 m/s2 )(2.0 s)2 − (1.0 m/s3 )(2.0 s)3 = 4.0 m.
Then the particle moves back to a final position of
x = (3.0 m/s2 )(4.0 s)2 − (1.0 m/s3 )(4.0 s)3 = −16.0 m.
The total path followed was 4.0 m + 4.0 m + 16.0 m = 24.0 m.
(d) The displacement is −16.0 m as was found in part (c).
(e) The velocity is vx = (6.0 m/s2 )t − (3.0 m/s3 )t2 . When t = 0, vx = 0.0 m/s. When t = 1.0 s,
vx = 3.0 m/s. When t = 2.0 s, vx = 0.0 m/s. When t = 3.0 s, vx = −9.0 m/s. When t = 4.0 s,
vx = −24.0 m/s.
(f) The acceleration is the time derivative of the velocity,
dvx
ax = = (6.0 m/s2 ) − (6.0 m/s3 )t.
dt
When t = 0 s, ax = 6.0 m/s2 . When t = 1.0 s, ax = 0.0 m/s2 . When t = 2.0 s, ax = −6.0 m/s2 .
When t = 3.0 s, ax = −12.0 m/s2 . When t = 4.0 s, ax = −18.0 m/s2 .
(g) The distance traveled was found in part (a) to be −20 m The average speed during the time
interval is then vx,av = (−20 m)/(2.0 s) = −10 m/s.
E2-40 v0x = 0, vx = 360 km/hr = 100 m/s. Assuming constant acceleration the average velocity
will be
1
vx,av = (100 m/s + 0) = 50 m/s.
2
The time to travel the distance of the runway at this average velocity is
t = (1800 m)/(50 m/s) = 36 s.
The acceleration is
ax = 2x/t2 = 2(1800 m)/(36.0 s)2 = 2.78 m/s2 .
18

20. E2-41 (a) Apply Eq. 2-26,
vx = v0x + ax t,
2
(3.0 × 107 m/s) = (0) + (9.8 m/s )t,
3.1 × 106 s = t.
(b) Apply Eq. 2-28 using an initial position of x0 = 0,
1
x = x0 + v0x + ax t2 ,
2
1 2
x = (0) + (0) + (9.8 m/s )(3.1 × 106 s)2 ,
2
x = 4.7 × 1013 m.
E2-42 v0x = 0 and vx = 27.8 m/s. Then
t = (vx − v0x )/a = ((27.8 m/s) − (0)) /(50 m/s2 ) = 0.56 s.
I want that car.
E2-43 The muon will travel for t seconds before it comes to a rest, where t is given by
t = (vx − v0x )/a = (0) − (5.20 × 106 m/s) /(−1.30 × 1014 m/s2 ) = 4 × 10−8 s.
The distance traveled will be
1 1
x = ax t2 + v0x t = (−1.30 × 1014 m/s2 )(4 × 10−8 s)2 + (5.20 × 106 m/s)(4 × 10−8 s) = 0.104 m.
2 2
E2-44 The average velocity of the electron was
1
vx,av = (1.5 × 105 m/s + 5.8 × 106 m/s) = 3.0 × 106 m/s.
2
The time to travel the distance of the runway at this average velocity is
t = (0.012 m)/(3.0 × 106 m/s) = 4.0 × 10−9 s.
The acceleration is
ax = (vx − v0x )/t = ((5.8 × 106 m/s) − (1.5 × 105 m/s))/(4.0 × 10−9 s) = 1.4 × 1015 m/s2 .
E2-45 It will be easier to solve the problem if we change the units for the initial velocity,
km 1000 m hr m
v0x = 1020 = 283 ,
hr km 3600 s s
and then applying Eq. 2-26,
vx = v0x + ax t,
(0) = (283 m/s) + ax (1.4 s),
2
−202 m/s = ax .
The problem asks for this in terms of g, so
2 g
−202 m/s 2 = 21g.
9.8 m/s
19

21. E2-46 Change miles to feet and hours to seconds. Then vx = 81 ft/s and v0x = 125 ft/s. The
time is then
2
t = ((81 ft/s) − (125 ft/s)) /(−17 ft/s ) = 2.6 s.
E2-47 (a) The time to stop is
2
t = ((0 m/s) − (24.6 m/s)) /(−4.92 m/s ) = 5.00 s.
(b) The distance traveled is
1 1 2
x= ax t2 + v0x t = (−4.92 m/s )(5.00 s)2 + (24.6 m/s)(5.00 s) = 62 m.
2 2
E2-48 Answer part (b) first. The average velocity of the arrow while decelerating is
1
vy ,av = ((0) + (260 ft/s)) = 130 ft/s.
2
The time for the arrow to travel 9 inches (0.75 feet) is
t = (0.75 ft)/(130 ft/s) = 5.8 × 10−3 s.
(a) The acceleration of the arrow is then
2
ay = (vy − v0y )/t = ((0) − (260 ft/s))/(5.8 × 10−3 s) = −4.5 × 104 ft/s .
E2-49 The problem will be somewhat easier if the units are consistent, so we’ll write the maxi-
mum speed as
ft min ft
1000 = 16.7 .
min 60 s s
(a) We can find the time required for the acceleration from Eq. 2-26,
vx = v0x + ax t,
2
(16.7 ft/s) = (0) + (4.00 ft/s )t,
4.18 s = t.
And from this and Eq 2-28 we can find the distance
1
x = x0 + v0x + ax t2 ,
2
1 2
x = (0) + (0) + (4.00 ft/s )(4.18 s)2 ,
2
x = 34.9 ft.
(b) The motion of the elevator is divided into three parts: acceleration from rest, constant speed
motion, and deceleration to a stop. The total distance is given at 624 ft and in part (a) we found
the distance covered during acceleration was 34.9 ft. By symmetry, the distance traveled during
deceleration should also be 34.9 ft. The distance traveled at constant speed is then (624 − 34.9 −
34.9) ft = 554 ft. The time required for the constant speed portion of the trip is found from Eq.
2-22, rewritten as
∆x 554 ft
∆t = = = 33.2 s.
v 16.7 ft/s
The total time for the trip is the sum of times for the three parts: accelerating (4.18 s), constant
speed (33.2 s), and decelerating (4.18 s). The total is 41.6 seconds.
20

22. E2-50 (a) The deceleration is found from
2 2
ax = (x − v0 t) = ((34 m) − (16 m/s)(4.0 s)) = −3.75 m/s2 .
t2 (4.0 s)2
(b) The impact speed is
vx = v0x + ax t = (16 m/s) + (−3.75 m/s2 )(4.0 s) = 1.0 m/s.
E2-51 Assuming the drops fall from rest, the time to fall is
2y 2(−1700 m)
t= = = 19 s.
ay (−9.8 m/s2 )
The velocity of the falling drops would be
vy = ay t = (−9.8 m/s2 )(19 s) = 190 m/s,
or about 2/3 the speed of sound.
E2-52 Solve the problem out of order.
(b) The time to fall is
2y 2(−120 m)
t= = = 4.9 s.
ay (−9.8 m/s2 )
(a) The speed at which the elevator hits the ground is
vy = ay t = (−9.8 m/s2 )(4.9 s) = 48 m/s.
(d) The time to fall half-way is
2y 2(−60 m)
t= = = 3.5 s.
ay (−9.8 m/s2 )
(c) The speed at the half-way point is
vy = ay t = (−9.8 m/s2 )(3.5 s) = 34 m/s.
E2-53 The initial velocity of the “dropped” wrench would be zero. I choose vertical to be along
the y axis with up as positive, which is the convention of Eq. 2-29 and Eq. 2-30. It turns out that
it is much easier to solve part (b) before solving part (a).
(b) We solve Eq. 2-29 for the time of the fall.
vy = v0y − gt,
2
(−24.0 m/s) = (0) − (9.8 m/s )t,
2.45 s = t.
(a) Now we can use Eq. 2-30 to find the height from which the wrench fell.
1
y = y0 + v0y t − gt2 ,
2
1 2
(0) = y0 + (0)(2.45 s) − (9.8 m/s )(2.45 s)2 ,
2
0 = y0 − 29.4 m
We have set y = 0 to correspond to the final position of the wrench: on the ground. This results in
an initial position of y0 = 29.4 m; it is positive because the wrench was dropped from a point above
where it landed.
21

23. E2-54 (a) It is easier to solve the problem from the point of view of an object which falls from the
highest point. The time to fall from the highest point is
2y 2(−53.7 m)
t= = = 3.31 s.
ay (−9.81 m/s2 )
The speed at which the object hits the ground is
vy = ay t = (−9.81 m/s2 )(3.31 s) = −32.5 m/s.
But the motion is symmetric, so the object must have been launched up with a velocity of vy =
32.5 m/s.
(b) Double the previous answer; the time of flight is 6.62 s.
E2-55 (a) The time to fall the first 50 meters is
2y 2(−50 m)
t= = = 3.2 s.
ay (−9.8 m/s2 )
(b) The total time to fall 100 meters is
2y 2(−100 m)
t= = = 4.5 s.
ay (−9.8 m/s2 )
The time to fall through the second 50 meters is the difference, 1.3 s.
E2-56 The rock returns to the ground with an equal, but opposite, velocity. The acceleration is
then
ay = ((−14.6 m/s) − (14.6 m/s))/(7.72 s) = 3.78 m/s2 .
That would put them on Mercury.
E2-57 (a) Solve Eq. 2-30 for the initial velocity. Let the distances be measured from the ground
so that y0 = 0.
1
y = y0 + v0y t − gt2 ,
2
1 2
(36.8 m) = (0) + v0y (2.25 s) − (9.8 m/s )(2.25 s)2 ,
2
36.8 m = v0y (2.25 s) − 24.8 m,
27.4 m/s = v0y .
(b) Solve Eq. 2-29 for the velocity, using the result from part (a).
vy = v0y − gt,
2
vy = (27.4 m/s) − (9.8 m/s )(2.25 s),
vy = 5.4 m/s.
(c) We need to solve Eq. 2-30 to find the height to which the ball rises, but we don’t know how
long it takes to get there. So we first solve Eq. 2-29, because we do know the velocity at the highest
point (vy = 0).
vy = v0y − gt,
2
(0) = (27.4 m/s) − (9.8 m/s )t,
2.8 s = t.
22

24. And then we find the height to which the object rises,
1
y = y0 + v0y t − gt2 ,
2
1 2
y = (0) + (27.4 m/s)(2.8 s) − (9.8 m/s )(2.8 s)2 ,
2
y = 38.3m.
This is the height as measured from the ground; so the ball rises 38.3 − 36.8 = 1.5 m above the point
specified in the problem.
E2-58 The time it takes for the ball to fall 2.2 m is
2y 2(−2.2 m)
t= = = 0.67 s.
ay (−9.8 m/s2 )
The ball hits the ground with a velocity of
vy = ay t = (−9.8 m/s2 )(0.67 s) = −6.6 m/s.
The ball then bounces up to a height of 1.9 m. It is easier to solve the falling part of the motion,
and then apply symmetry. The time is would take to fall is
2y 2(−1.9 m)
t= = = 0.62 s.
ay (−9.8 m/s2 )
The ball hits the ground with a velocity of
vy = ay t = (−9.8 m/s2 )(0.62 s) = −6.1 m/s.
But we are interested in when the ball moves up, so vy = 6.1 m/s.
The acceleration while in contact with the ground is
ay = ((6.1 m/s) − (−6.6 m/s))/(0.096 s) = 130 m/s2 .
E2-59 The position as a function of time for the first object is
1
y1 = − gt2 ,
2
The position as a function of time for the second object is
1
y2 = − g(t − 1 s)2
2
The difference,
∆y = y2 − y1 = f rac12g ((2 s)t − 1) ,
is the set equal to 10 m, so t = 1.52 s.
E2-60 Answer part (b) first.
(b) Use the quadratic equation to solve
1
(−81.3 m) = (−9.81 m/s2 )t2 + (12.4 m/s)t
2
for time. Get t = −3.0 s and t = 5.53 s. Keep the positive answer.
(a) Now find final velocity from
vy = (−9.8 m/s2 )(5.53 s) + (12.4 m/s) = −41.8 m/s.
23

25. E2-61 The total time the pot is visible is 0.54 s; the pot is visible for 0.27 s on the way down.
We’ll define the initial position as the highest point and make our measurements from there. Then
y0 = 0 and v0y = 0. Define t1 to be the time at which the falling pot passes the top of the window
y1 , then t2 = t1 + 0.27 s is the time the pot passes the bottom of the window y2 = y1 − 1.1 m. We
have two equations we can write, both based on Eq. 2-30,
1
y1 = y0 + v0y t1 − gt2 ,
2 1
1
y1 = (0) + (0)t1 − gt2 ,
2 1
and
1
y2 = y0 + v0y t2 − gt2 ,
2 2
1
y1 − 1.1 m = (0) + (0)t2 − g(t1 + 0.27 s)2 ,
2
Isolate y1 in this last equation and then set the two expressions equal to each other so that we can
solve for t1 ,
1 1
− gt2 = 1.1 m − g(t1 + 0.27 s)2 ,
2 1 2
1 1
− gt2 = 1.1 m − g(t2 + [0.54 s]t1 + 0.073 s2 ),
2 1 2 1
1
0 = 1.1 m − g([0.54 s]t1 + 0.073 s2 ).
2
This last line can be directly solved to yield t1 = 0.28 s as the time when the falling pot passes the
top of the window. Use this value in the first equation above and we can find y1 = − 1 (9.8 m/s2 )(0.28
2
s)2 = −0.38 m. The negative sign is because the top of the window is beneath the highest point, so
the pot must have risen to 0.38 m above the top of the window.
P2-1 (a) The net shift is (22 m)2 + (17 m)2 ) = 28 m.
(b) The vertical displacement is (17 m) sin(52◦ ) = 13 m.
P2-2 Wheel “rolls” through half of a turn, or πr = 1.41 m. The vertical displacement is 2r =
0.90 m. The net displacement is
(1.41 m)2 + (0.90 m)2 = 1.67 m0.
The angle is
θ = tan−1 (0.90 m)/(1.41 m) = 33◦ .
P2-3 We align the coordinate system so that the origin corresponds to the starting position of
the fly and that all positions inside the room are given by positive coordinates.
(a) The displacement vector can just be written,
∆r = (10 ft)ˆ + (12 ft)ˆ + (14 ft)k.
i j ˆ
√
(b) The magnitude of the displacement vector is |∆r| = 102 + 122 + 142 ft= 21 ft.
24

26. (c) The straight line distance between two points is the shortest possible distance, so the length
of the path taken by the fly must be greater than or equal to 21 ft.
(d) If the fly walks it will need to cross two faces. The shortest path will be the diagonal across
these two faces. If the lengths of sides of the room are l1 , l2 , and l3 , then the diagonal length across
two faces will be given by
2
(l1 + l2 )2 + l3 ,
where we want to choose the li from the set of 10 ft, 12 ft, and 14 ft that will minimize the length.
The minimum distance is when l1 = 10 ft, l2 = 12 ft, and l3 = 14. Then the minimal distance the
fly would walk is 26 ft.
P2-4 Choose vector a to lie on the x axis. Then a = aˆ and b = bxˆ + byˆ where bx = b cos θ and
i i j
by = b sin θ. The sum then has components
rx = a + b cos θ and ry = b sin θ.
Then
2 2
r2 = (a + b cos θ) + (b sin θ) ,
= a2 + 2ab cos θ + b2 .
P2-5 (a) Average speed is total distance divided by total time. Then
(35.0 mi/hr)(t/2) + (55.0 mi/hr)(t/2)
v av = = 45.0 mi/hr.
(t/2) + (t/2)
(b) Average speed is total distance divided by total time. Then
(d/2) + (d/2)
v av = = 42.8 mi/hr.
(d/2)/(35.0 mi/hr) + (d/2)/(55.0 mi/hr)
(c) Average speed is total distance divided by total time. Then
d+d
v av = = 43.9 mi/hr
(d)/(45.0 mi/hr) + (d)/(42.8 mi/hr)
P2-6 (a) We’ll do just one together. How about t = 2.0 s?
x = (3.0 m/s)(2.0 s) + (−4.0 m/s2 )(2.0 s)2 + (1.0 m/s3 )(2.0 s)3 = −2.0 m.
The rest of the values are, starting from t = 0, x = 0.0 m, 0.0 m, -2.0 m, 0.0 m, and 12.0 m.
(b) Always final minus initial. The answers are xf − xi = −2.0 m − 0.0 m = −2.0 m and xf − xi =
12.0 m − 0.0 m = 12.0 m.
(c) Always displacement divided by (change in) time.
(12.0 m) − (−2.0 m)
v av = = 7.0 m/s,
(4.0 s) − (2.0 s)
and
(0.0 m) − (0.0 m)
v av = = 0.0 m/s.
(3.0 s) − (0.0 s)
25

27. P2-7 (a) Assume the bird has no size, the trains have some separation, and the bird is just
leaving one of the trains. The bird will be able to fly from one train to the other before the two
trains collide, regardless of how close together the trains are. After doing so, the bird is now on the
other train, the trains are still separated, so once again the bird can fly between the trains before
they collide. This process can be repeated every time the bird touches one of the trains, so the bird
will make an infinite number of trips between the trains.
(b) The trains collide in the middle; therefore the trains collide after (51 km)/(34 km/hr) = 1.5
hr. The bird was flying with constant speed this entire time, so the distance flown by the bird is (58
km/hr)(1.5 hr) = 87 km.
P2-8 (a) Start with a perfect square:
(v1 − v2 )2 > 0,
2 2
v1 + v2 > 2v1v2,
2 2
(v1 + v2 )t1 t2 > 2v1 v2 t1 t2 ,
2 2 2 2
d1 + d2 + (v1 + v2 )t1 t2 > d2 + d2 + 2v1 v2 t1 t2 ,
1 2
2 2
(v1 t1 + v2 t2 )(t1 + t2 ) > (d1 + d2 )2 ,
2 2
v1 t1 + v2 t2 d1 + d2
> ,
d1 + d2 t1 + t 2
v1 d1 + v2 d2 v1 t1 + v2 t2
>
d1 + d2 t 1 + t2
Actually, it only works if d1 + d2 > 0!
(b) If v1 = v2 .
P2-9 (a) The average velocity during the time interval is v av = ∆x/∆t, or
(A + B(3 s)3 ) − (A + B(2 s)3 ) 3
v av = = (1.50 cm/s )(19 s3 )/(1 s) = 28.5 cm/s.
(3 s) − (2 s)
3
(b) v = dx/dt = 3Bt2 = 3(1.50 cm/s )(2 s)2 = 18 cm/s.
3
(c) v = dx/dt = 3Bt2 = 3(1.50 cm/s )(3 s)2 = 40.5 cm/s.
3
(d) v = dx/dt = 3Bt2 = 3(1.50 cm/s )(2.5 s)2 = 28.1 cm/s.
(e) The midway position is (xf + xi )/2, or
xmid = A + B[(3 s)3 + (2 s)3 )]/2 = A + (17.5 s3 )B.
This occurs when t = 3
(17.5 s3 ). The instantaneous velocity at this point is
3
v = dx/dt = 3Bt2 = 3(1.50 cm/s )( 3 (17.5 s3 ))2 = 30.3 cm/s.
P2-10 Consider the figure below.
x x x x
1 t 1 t 1 t 1 t
(a) (b) (c) (d)
26

28. P2-11 (a) The average velocity is displacement divided by change in time,
3 3
(2.0 m/s )(2.0 s)3 − (2.0 m/s )(1.0 s)3 14.0 m
v av = = = 14.0 m/s.
(2.0 s) − (1.0 s) 1.0 s
The average acceleration is the change in velocity. So we need an expression for the velocity, which
is the time derivative of the position,
dx d 3 3
v= = (2.0 m/s )t3 = (6.0 m/s )t2 .
dt dt
From this we find average acceleration
3 3
(6.0 m/s )(2.0 s)2 − (6.0 m/s )(1.0 s)2 18.0 m/s 2
aav = = = 18.0 m/s .
(2.0 s) − (1.0 s) 1.0 s
(b) The instantaneous velocities can be found directly from v = (6.0 m/s2 )t2 , so v(2.0 s) = 24.0
m/s and v(1.0 s) = 6.0 m/s. We can get an expression for the instantaneous acceleration by taking
the time derivative of the velocity
dv d 3 3
a= = (6.0 m/s )t2 = (12.0 m/s )t.
dt dt
Then the instantaneous accelerations are a(2.0 s) = 24.0 m/s2 and a(1.0 s) = 12.0 m/s2
(c) Since the motion is monotonic we expect the average quantities to be somewhere between
the instantaneous values at the endpoints of the time interval. Indeed, that is the case.
P2-12 Consider the figure below.
a(m/s^2) v(m/s) x(m)
15 75
10 50
5 25
0 0
0 2 4 6 8 10 0 2 4 6 8 10 0 2 4 6 8 10
t(s) t(s) t(s)
P2-13 Start with v f = v i + at, but v f = 0, so v i = −at, then
1 2 1 1
x= at + v i t = at2 − at2 = − at2 ,
2 2 2
2 2
so t = −2x/a = −2(19.2 ft)/(−32 ft/s ) = 1.10 s. Then v i = −(−32 ft/s )(1.10 s) = 35.2 ft/s.
Converting,
35.2 ft/s(1/5280 mi/ft)(3600 s/h) = 24 mi/h.
27

29. P2-14 (b) The average speed during while traveling the 160 m is
v av = (33.0 m/s + 54.0 m/s)/2 = 43.5 m/s.
The time to travel the 160 m is t = (160 m)/(43.5 m/s) = 3.68 s.
(a) The acceleration is
2x 2vi 2(160 m) 2(33.0 m/s)
a= − = − = 5.69 m/s2 .
t2 t (3.68 s)2 (3.68 s)
(c) The time required to get up to a speed of 33 m/s is
t = v/a = (33.0 m/s)/(5.69 m/s2 ) = 5.80 s.
(d) The distance moved from start is
1 2 1
d= at = (5.69 m/s2 )(5.80 s)2 = 95.7 m.
2 2
P2-15 (a) The distance traveled during the reaction time happens at constant speed; treac = d/v =
(15 m)/(20 m/s) = 0.75 s.
(b) The braking distance is proportional to the speed squared (look at the numbers!) and in
this case is dbrake = v 2 /(20 m/s2 ). Then dbrake = (25 m/s)2 /(20 m/s2 ) = 31.25 m. The reaction time
distance is dreac = (25 m/s)(0.75 s) = 18.75 m. The stopping distance is then 50 m.
P2-16 (a) For the car xc = ac t2 /2. For the truck xt = v t t. Set both xi to the same value, and
then substitute the time from the truck expression:
x = ac t2 /2 = ac (x/v t )2 /2,
or
x = 2v t 2 /ac = 2(9.5 m/s)2 /(2.2 m/s) = 82 m.
(b) The speed of the car will be given by v c = ac t, or
v c = ac t = ac x/v t = (2.2 m/s)(82 m)/(9.5 m/s) = 19 m/s.
P2-17 The runner covered a distance d1 in a time interval t1 during the acceleration phase and
a distance d2 in a time interval t2 during the constant speed phase. Since the runner started from
rest we know that the constant speed is given by v = at1 , where a is the runner’s acceleration.
The distance covered during the acceleration phase is given by
1 2
d1 = at .
2 1
The distance covered during the constant speed phase can also be found from
d2 = vt2 = at1 t2 .
We want to use these two expressions, along with d1 + d2 = 100 m and t2 = (12.2 s) − t1 , to get
1 2
100 m = d1 + d2 = at + at1 (12.2 s − t1 ),
2 1
1
= − at2 + a(12.2 s)t1 ,
2 1
2
= −(1.40 m/s )t2 + (34.2 m/s)t1 .
1
28

30. This last expression is quadratic in t1 , and is solved to give t1 = 3.40 s or t1 = 21.0 s. Since the race
only lasted 12.2 s we can ignore the second answer.
(b) The distance traveled during the acceleration phase is then
1 2 2
d1 = at = (1.40 m/s )(3.40 s)2 = 16.2 m.
2 1
P2-18 (a) The ball will return to the ground with the same speed it was launched. Then the total
time of flight is given by
t = (v f − v i )/g = (−25 m/s − 25 m/s)/(9.8 m/s2 ) = 5.1 s.
(b) For small quantities we can think in terms of derivatives, so
δt = (δv f − δv i )/g,
or τ = 2 /g.
P2-19 Use y = −gt2 /2, but only keep the absolute value. Then y50 = (9.8 m/s2 )(0.05 s)2 /2 =
1.2 cm; y100 = (9.8 m/s2 )(0.10 s)2 /2 = 4.9 cm; y150 = (9.8 m/s2 )(0.15 s)2 /2 = 11 cm; y200 =
(9.8 m/s2 )(0.20 s)2 /2 = 20 cm; y250 = (9.8 m/s2 )(0.25 s)2 /2 = 31 cm.
P2-20 The truck will move 12 m in (12 m)/(55 km/h) = 0.785 s. The apple will fall y = −gt2 /2 =
−(9.81 m/s2 )(0.785 s)2 /2 = −3.02 m.
2
P2-21 The rocket travels a distance d1 = 1 at2 = 1 (20 m/s )(60 s)2 = 36, 000 m during the accel-
2 1 2
2
eration phase; the rocket velocity at the end of the acceleration phase is v = at = (20 m/s )(60 s) =
1200 m/s. The second half of the trajectory can be found from Eqs. 2-29 and 2-30, with y0 = 36, 000
m and v0y = 1200 m/s.
(a) The highest point of the trajectory occurs when vy = 0, so
vy = v0y − gt,
2
(0) = (1200 m/s) − (9.8 m/s )t,
122 s = t.
This time is used to find the height to which the rocket rises,
1
y = y0 + v0y t − gt2 ,
2
1 2
= (36000 m) + (1200 m/s)(122s) − (9.8 m/s )(122 s)2 = 110000 m.
2
(b) The easiest way to find the total time of flight is to solve Eq. 2-30 for the time when the
rocket has returned to the ground. Then
1
y = y0 + v0y t − gt2 ,
2
1 2
(0) = (36000 m) + (1200 m/s)t − (9.8 m/s )t2 .
2
This quadratic expression has two solutions for t; one is negative so we don’t need to worry about
it, the other is t = 270 s. This is the free-fall part of the problem, to find the total time we need to
add on the 60 seconds of accelerated motion. The total time is then 330 seconds.
29

31. P2-22 (a) The time required for the player to “fall” from the highest point a distance of y = 15 cm
is 2y/g; the total time spent in the top 15 cm is twice this, or 2 2y/g = 2 2(0.15 m)/(9.81 m/s) =
0.350 s.
(b) The time required for the player to “fall” from the highest point a distance of 76 cm is
2(0.76 m)/(9.81 m/s) = 0.394 s, the time required for the player to fall from the highest point a
distance of (76 − 15 = 61) cm is 2(0.61 m)/g = 0.353 s. The time required to fall the bottom 15
cm is the difference, or 0.041 s. The time spent in the bottom 15 cm is twice this, or 0.081 s.
P2-23 (a) The average speed between A and B is v av = (v + v/2)/2 = 3v/4. We can also write
v av = (3.0 m)/∆t = 3v/4. Finally, v/2 = v − g∆t. Rearranging, v/2 = g∆t. Combining all of the
above,
v 4(3.0 m)
=g or v 2 = (8.0 m)g.
2 3v
Then v = (8.0 m)(9.8 m/s2 ) = 8.85 m/s.
(b) The time to the highest point above B is v/2 = gt, so the distance above B is
2
g v g v v v v2
y = − t2 + t = − + = .
2 2 2 2g 2 2g 8g
Then y = (8.85 m/s)2 /(8(9.8 m/s2 )) = 1.00 m.
P2-24 (a) The time in free fall is t = −2y/g = −2(−145 m)/(9.81 m/s2 ) = 5.44 s.
(b) The speed at the bottom is v = −gt = −(9.81 m/s2 )(5.44 s) = −53.4 m/s.
(c) The time for deceleration is given by v = −25gt, or t = −(−53.4 m/s)/(25 × 9.81 /s2 ) =
0.218 s. The distance through which deceleration occurred is
25g 2
y= t + vt = (123 m/s2 )(0.218 s)2 + (−53.4 m/s)(0.218 s) = −5.80 m.
2
P2-25 Find the time she fell from Eq. 2-30,
1 2
(0 ft) = (144 ft) + (0)t − (32 ft/s )t2 ,
2
which is a simple quadratic with solutions t = ±3.0 s. Only the positive solution is of interest. Use
this time in Eq. 2-29 to find her speed when she hit the ventilator box,
2
vy = (0) − (32 ft/s )(3.0 s) = −96 ft/s.
This becomes the initial velocity for the deceleration motion, so her average speed during deceleration
is given by Eq. 2-27,
1 1
v av,y = (vy + v0y ) = ((0) + (−96 ft/s)) = −48 ft/s.
2 2
This average speed, used with the distance of 18 in (1.5 ft), can be used to find the time of deceleration
v av,y = ∆y/∆t,
and putting numbers into the expression gives ∆t = 0.031 s. We actually used ∆y = −1.5 ft, where
the negative sign indicated that she was still moving downward. Finally, we use this in Eq. 2-26 to
find the acceleration,
(0) = (−96 ft/s) + a(0.031 s),
which gives a = +3100 ft/s2 . In terms of g this is a = 97g, which can be found by multiplying
through by 1 = g/(32 ft/s2 ).
30

32. P2-26 Let the speed of the disk when it comes into contact with the ground be v1 ; then the
average speed during the deceleration process is v1 /2; so the time taken for the deceleration process
is t1 = 2d/v1 , where d = −2 mm. But d is also give by d = at2 /2 + v1 t1 , so
1
2
100g 2d 2d d2
d= + v1 = 200g 2 + 2d,
2 v1 v1 v1
2
or v1 = −200gd. The negative signs are necessary!.
The disk was dropped from a height h = −y and it first came into contact with the ground when
it had a speed of v1 . Then the average speed is v1 /2, and we can repeat most of the above (except
a = −g instead of 100g), and then the time to fall is t2 = 2y/v1 ,
2
g 2y 2y y2
y= + v1 = 2g 2 + 2y,
2 v1 v1 v1
2
or v1 = −2gy. The negative signs are necessary!.
Equating, y = 100d = 100(−2 mm) = −0.2 m, so h = 0.2 m. Note that although 100g’s sounds
like plenty, you still shouldn’t be dropping your hard disk drive!
P2-27 Measure from the feet! Jim is 2.8 cm tall in the photo, so 1 cm on the photo is 60.7
cm in real-life. Then Jim has fallen a distance y1 = −3.04 m while Clare has fallen a distance
y2 = −5.77 m. Clare jumped first, and the time she has been falling is t2 ; Jim jumped seconds, the
time he has been falling is t1 = t2 − ∆t. Then y2 = −gt2 /2 and y1 = −gt2 /2, or t2 = −2y2 /g =
2 1
−2(−5.77 m)/(9.81 m/s2 ) = 1.08 s and t1 = −2y1 /g = −2(3.04 m)/(9.81 m/s2 ) = 0.79 s. So
Jim waited 0.29 s.
P2-28 (a) Assuming she starts from rest and has a speed of v1 when she opens her chute, then
her average speed while falling freely is v1 /2, and the time taken to fall y1 = −52.0 m is t1 = 2y1 /v1 .
2
Her speed v1 is given by v1 = −gt1 , or v1 = −2gy1 . Then v1 = − −2(9.81 m/s2 )(−52.0 m) =
−31.9 m/s. We must use the negative answer, because she fall down! The time in the air is then
t1 = −2y1 /g = −2(52.0 m)/(9.81 m/s2 ) = 3.26 s.
Her final speed is v2 = −2.90 m/s, so the time for the deceleration is t2 = (v2 − v1 )/a, where
a = 2.10 m/s2 . Then t2 = (−2.90 m/s − −31.9 m/s)/(2.10 m/s2 ) = 13.8 s.
Finally, the total time of flight is t = t1 + t2 = 3.26 s + 13.8 s = 17.1 s.
(b) The distance fallen during the deceleration phase is
g (2.10 m/s2 )
y2 = − t2 + v1 t2 = −
2 (13.8 s)2 + (−31.9 m/s)(13.8 s) = −240 m.
2 2
The total distance fallen is y = y1 + y2 = −52.0 m − 240 m = −292 m. It is negative because she was
falling down.
P2-29 Let the speed of the bearing be v1 at the top of the windows and v2 at the bottom.
These speeds are related by v2 = v1 − gt12 , where t12 = 0.125 s is the time between when the
bearing is at the top of the window and at the bottom of the window. The average speed is
v av = (v1 + v2 )/2 = v1 − gt12 /2. The distance traveled in the time t12 is y12 = −1.20 m, so
y12 = v av t12 = v1 t12 − gt2 /2,
12
and expression that can be solved for v1 to yield
y12 + gt2 /2
12 (−1.20 m) + (9.81 m/s2 )(0.125 s)2 /2
v1 = = = −8.99 m/s.
t12 (0.125 s)
31

33. Now that we know v1 we can find the height of the building above the top of the window. The time
the object has fallen to get to the top of the window is t1 = −v1 /g = −(−8.99 m/s)/(9.81 m/s2 ) =
0.916 m.
The total time for falling is then (0.916 s) + (0.125 s) + (1.0 s) = 2.04 s. Note that we remembered
to divide the last time by two! The total distance from the top of the building to the bottom is then
y = −gt2 /2 = −(9.81 m/s2 )(2.04 s)2 /2 = 20.4 m.
P2-30 Each ball falls from a highest point through a distance of 2.0 m in
t= −2(2.0 m)/(9.8 m/s2 ) = 0.639 s.
The time each ball spends in the air is twice this, or 1.28 s. The frequency of tosses per ball is the
reciprocal, f = 1/T = 0.781 s−1 . There are five ball, so we multiply this by 5, but there are two
hands, so we then divide that by 2. The tosses per hand per second then requires a factor 5/2, and
the tosses per hand per minute is 60 times this, or 117.
P2-31 Assume each hand can toss n objects per second. Let τ be the amount of time that any
one object is in the air. Then 2nτ is the number of objects that are in the air at any time, where
the “2” comes from the fact that (most?) jugglers have two hands. We’ll estimate n, but τ can be
found from Eq. 2-30 for an object which falls a distance h from rest:
1
0 = h + (0)t − gt2 ,
2
solving, t = 2h/g. But τ is twice this, because the object had to go up before it could come down.
So the number of objects that can be juggled is
4n 2h/g
We estimate n = 2 tosses/second. So the maximum number of objects one could juggle to a height
h would be
3.6 h/meters.
P2-32 (a) We need to look up the height of the leaning tower to solve this! If the height is h = 56 m,
then the time taken to fall a distance h = −y1 is t1 = −2y1 /g = −2(−56 m)/(9.81 m/s2 ) = 3.4 s.
The second object, however, has only fallen a a time t2 = t1 − ∆t = 3.3 s, so the distance the second
object falls is y2 = −gt2 /2 = −(9.81 m/s2 )(3.3 s)2 /2 = 53.4. The difference is y1 − y2 = 2.9 m.
2
(b) If the vertical separation is ∆y = 0.01 m, then we can approach this problem in terms of
differentials,
δy = at δt,
so δt = (0.01 m)/[((9.81 m/s2 )(3.4 s)] = 3×10−4 s.
P2-33 Use symmetry, and focus on the path from the highest point downward. Then ∆tU = 2tU ,
where tU is the time from the highest point to the upper level. A similar expression exists for
the lower level, but replace U with L. The distance from the highest point to the upper level is
yU = −gt2 /2 = −g(∆tU /2)2 /2. The distance from the highest point to the lower level is yL =
U
−gt2 /2 = −g(∆tL /2)2 /2. Now H = yU − yL = −g∆t2 /8 − −g∆t2 /8, which can be written as
L U L
8H
g= .
∆t2 − ∆t2
L U
32

34. E3-1 The Earth orbits the sun with a speed of 29.8 km/s. The distance to Pluto is 5900×106 km.
The time it would take the Earth to reach the orbit of Pluto is
t = (5900×106 km)/(29.8 km/s) = 2.0×108 s,
or 6.3 years!
E3-2 (a) a = F/m = (3.8 N)/(5.5 kg) = 0.69 m/s2 .
(b) t = v f /a = (5.2 m/s)/(0.69 m/s2 ) = 7.5 s.
(c) x = at2 /2 = (0.69 m/s2 )(7.5 s)2 /2 = 20 m.
E3-3 Assuming constant acceleration we can find the average speed during the interval from Eq.
2-27
1 1
v av,x =(vx + v0x ) = (5.8×106 m/s) + (0) = 2.9×106 m/s.
2 2
From this we can find the time spent accelerating from Eq. 2-22, since ∆x = v av,x ∆t. Putting in
the numbers ∆t = 5.17×10−9 s. The acceleration is then
∆vx (5.8×106 m/s) − (0)
ax = = = 1.1×1015 m/s2 .
∆t (5.17×10−9 s)
The net force on the electron is from Eq. 3-5,
Fx = max = (9.11×10−31 kg)(1.1×1015 m/s2 ) = 1.0×10−15 N.
E3-4 The average speed while decelerating is v av = 0.7 × 107 m/s. The time of deceleration is
t = x/v av = (1.0×10−14 m)/(0.7×107 m/s) = 1.4×10−21 s. The deceleration is a = ∆v/t = (−1.4×
107 m/s)/(1.4×10−21 s) = −1.0×1028 m/s2 . The force is F = ma = (1.67×10−27 kg)(1.0×1028 m/s2 ) =
17 N.
E3-5 The net force on the sled is 92 N−90 N= 2 N; subtract because the forces are in opposite
directions. Then
Fx (2 N)
ax = = = 8.0×10−2 m/s2 .
m (25 kg)
E3-6 53 km/hr is 14.7 m/s. The average speed while decelerating is v av = 7.4 m/s. The time
of deceleration is t = x/v av = (0.65 m)/(7.4 m/s) = 8.8×10−2 s. The deceleration is a = ∆v/t =
(−14.7 m/s)/(8.8×10−2 s) = −17×102 m/s2 . The force is F = ma = (39kg)(1.7×102 m/s2 ) = 6600 N.
E3-7 Vertical acceleration is a = F/m = (4.5×10−15 N)/(9.11×10−31 kg) = 4.9×1015 m/s2 . The
electron moves horizontally 33 mm in a time t = x/vx = (0.033 m)/(1.2×107 m/s) = 2.8×10−9 s.
The vertical distance deflected is y = at2 /2 = (4.9×1015 m/s2 )(2.8×10−9 s)2 /2 = 1.9×10−2 m.
E3-8 (a) a = F/m = (29 N)/(930 kg) = 3.1×10−2 m/s2 .
(b) x = at2 /2 = (3.1×10−2 m/s2 )(86400 s)2 /2 = 1.2×108 m.
(c) v = at = (3.1×10−2 m/s2 )(86400 s) = 2700 m/s.
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35. E3-9 Write the expression for the motion of the first object as Fx = m1 a1x and that of the
second object as Fx = m2 a2x . In both cases there is only one force, F , on the object, so Fx = F .
We will solve these for the mass as m1 = F/a1 and m2 = F/a2 . Since a1 > a2 we can conclude that
m2 > m1
(a) The acceleration of and object with mass m2 − m1 under the influence of a single force of
magnitude F would be
F F 1
a= = = 2 ) − 1/(12.0 m/s2 )
,
m2 − m1 F/a2 − F/a1 1/(3.30 m/s
which has a numerical value of a = 4.55 m/s2 .
(b) Similarly, the acceleration of an object of mass m2 + m1 under the influence of a force of
magnitude F would be
1 1
a= = 2 ) + 1/(12.0 m/s2 )
,
1/a2 + 1/a1 1/(3.30 m/s
which is the same as part (a) except for the sign change. Then a = 2.59 m/s2 .
E3-10 (a) The required acceleration is a = v/t = 0.1c/t. The required force is F = ma = 0.1mc/t.
Then
F = 0.1(1200×103 kg)(3.00×108 m/s)/(2.59×105 s) = 1.4×108 N,
and
F = 0.1(1200×103 kg)(3.00×108 m/s)/(5.18×106 s) = 6.9×106 N,
(b) The distance traveled during the acceleration phase is x1 = at2 /2, the time required to
1
travel the remaining distance is t2 = x2 /v where x2 = d − x1 . d is 5 light-months, or d = (3.00×
108 m/s)(1.30×107 s) = 3.90×1015 m. Then
d − x1 2d − at2
1 2d − vt1
t = t1 + t 2 = t 1 + = t1 + = t1 + .
v 2v 2v
If t1 is 3 days, then
2(3.90×1015 m) − (3.00×107 m/s)(2.59×105 s)
t = (2.59×105 s) + = 1.30×108 s = 4.12 yr,
2(3.00×107 m/s)
if t1 is 2 months, then
2(3.90×1015 m) − (3.00×107 m/s)(5.18×106 s)
t = (5.18×106 s) + = 1.33×108 s = 4.20 yr,
2(3.00×107 m/s)
E3-11 (a) The net force on the second block is given by
Fx = m2 a2x = (3.8 kg)(2.6 m/s2 ) = 9.9 N.
There is only one (relevant) force on the block, the force of block 1 on block 2.
(b) There is only one (relevant) force on block 1, the force of block 2 on block 1. By Newton’s
third law this force has a magnitude of 9.9 N. Then Newton’s second law gives Fx = −9.9
N= m1 a1x = (4.6 kg)a1x . So a1x = −2.2 m/s2 at the instant that a2x = 2.6 m/s2 .
E3-12 (a) W = (5.00 lb)(4.448 N/lb) = 22.2 N; m = W/g = (22.2 N)/(9.81 m/s2 ) = 2.26 kg.
(b) W = (240 lb)(4.448 N/lb) = 1070 N; m = W/g = (1070 N)/(9.81 m/s2 ) = 109 kg.
(c) W = (3600 lb)(4.448 N/lb) = 16000 N; m = W/g = (16000 N)/(9.81 m/s2 ) = 1630 kg.
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