physics 1a, section 6

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Physics 1A, Section 6 October 6, 2008

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Physics 1A, Section 6. October 6, 2008. Section Business. Section 6 office hour: Caltech/Downs 101 Tuesdays 4:00 - 5:30 PM See other choices on course web site: http://www.its.caltech.edu/~tmu/ph1a Section web site: http://www.submm.caltech.edu/~cdd/PHYS1A_2008. - PowerPoint PPT Presentation

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Page 1: Physics 1A, Section 6

Physics 1A, Section 6

October 6, 2008

Page 2: Physics 1A, Section 6

Section Business

• Section 6 office hour:– Caltech/Downs 101– Tuesdays 4:00 - 5:30 PM

• See other choices on course web site:– http://www.its.caltech.edu/~tmu/ph1a

• Section web site:– http://www.submm.caltech.edu/~cdd/PHYS1A_2008

Page 3: Physics 1A, Section 6

Week 1 Reading/Lecture Review• T.M.U. chapters 1-2 + lectures:

– units & dimensions– dimensional analysis (estimation)– law(s) of falling bodies

• constant acceleration (compare eq. 2.14-2.16): s = s0 + v0t + ½ at2

v = v0 + at

– distance, velocity, acceleration (general case):• v = ds/dt• a = dv/dt

Page 4: Physics 1A, Section 6

• Oresme (14th century): v t

s t2

(both correct)

A modern look athistorical laws of falling bodies

Page 5: Physics 1A, Section 6

A modern look athistorical laws of falling bodies• Galileo (17th century):

time 1 2 3 4 5 …

s 1 3 5 7 9 …

Page 6: Physics 1A, Section 6

• Galileo (17th century):

time 1 2 3 4 5 …

s 1 3 5 7 9 …

s 1 4 9 16 25 …

A modern look athistorical laws of falling bodies

Page 7: Physics 1A, Section 6

• Galileo (17th century):

s t2 (correct)

time 1 2 3 4 5 …

s 1 3 5 7 9 …

s 1 4 9 16 25 …

A modern look athistorical laws of falling bodies

Page 8: Physics 1A, Section 6

• da Vinci (15th century):

time 1 2 3 4 5 …

s 1 2 3 4 5 …

A modern look athistorical laws of falling bodies

Page 9: Physics 1A, Section 6

• da Vinci (15th century):

time 1 2 3 4 5 …

s 1 2 3 4 5 …

s 1 3 6 10 15 …

A modern look athistorical laws of falling bodies

Page 10: Physics 1A, Section 6

• da Vinci (15th century):

s (t)(t + 1)/2 = t2/2 + t/2

time 1 2 3 4 5 …

s 1 2 3 4 5 …

s 1 3 6 10 15 …

A modern look athistorical laws of falling bodies

Page 11: Physics 1A, Section 6

• da Vinci (15th century):

s (t)(t + 1)/2 = t2/2 + t/2

v = ds/dt t + 1/2 (moving at the start)

time 1 2 3 4 5 …

s 1 2 3 4 5 …

s 1 3 6 10 15 …

A modern look athistorical laws of falling bodies

Page 12: Physics 1A, Section 6

• Albert of Saxony (14th century): v s

A modern look athistorical laws of falling bodies

Page 13: Physics 1A, Section 6

• Albert of Saxony (14th century): v s

ds/dt = ks

A modern look athistorical laws of falling bodies

Page 14: Physics 1A, Section 6

• Albert of Saxony (14th century): v s

ds/dt = ks s = Cekt

A modern look athistorical laws of falling bodies

Page 15: Physics 1A, Section 6

• Albert of Saxony (14th century): v s

ds/dt = ks s = Cekt

v = Ckekt

A modern look athistorical laws of falling bodies

Page 16: Physics 1A, Section 6

• Albert of Saxony (14th century): v s

ds/dt = ks s = Cekt

v = Ckekt

Takes an infinite time to start from infinitesimal velocity!

A modern look athistorical laws of falling bodies

Page 17: Physics 1A, Section 6

Quiz Problem

35

Page 18: Physics 1A, Section 6

Quiz Problem

35

• Answer:

a) a(t) = jt + a0

v(t) = jt2/2 + a0t + v0

x(t) = jt3/6 + a0t2/2 + v0t + x0

b) (see graph)

c) A was ahead at t = 0.5 s.

d) J will win.0 0.5 1 1.5

time (s)

x

Car A

Car J

Page 19: Physics 1A, Section 6

Quiz Problem

46

Page 20: Physics 1A, Section 6

Quiz Problem

46• Answer:

a) D’ = VsT

= sqrt{W2 + (X-VrT)2}

b) tan ‘ = (X-VrT)/W

c) Vs > Vr

d) (Vs2-Vr

2)T2 + 2XVrT – (W2+X2) = 0

Use quadratic formula.

e) T = W/sqrt{Vs2-Vr

2}

f) T = W/Vs

X = WVr/Vs

Page 21: Physics 1A, Section 6

Thursday, October 9:

• T.M.U., Problem 3-7

• Quiz Problem 19

• Optional, but helpful, to look at these in advance.