Physics 101 Formulas: A Comprehensive Guide for High School Students, Summaries of Physics

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Physics 101 Formulas
12/7/2017 1
Kinematics
𝒗𝒗𝑎𝑎𝑎𝑎𝑎𝑎 = 𝛥𝛥𝒙𝒙
𝛥𝛥𝛥𝛥 𝒂𝒂𝑎𝑎𝑎𝑎𝑎𝑎 = 𝛥𝛥𝒗𝒗
𝛥𝛥𝛥𝛥
𝑣𝑣 = 𝑣𝑣0 + 𝑎𝑎𝑎𝑎 𝑥𝑥 = 𝑥𝑥0 + 𝑣𝑣0𝑎𝑎 + 1
2𝑎𝑎𝑎𝑎2
𝑣𝑣2 = 𝑣𝑣0
2 + 2𝑎𝑎𝑎𝑎𝑥𝑥
𝑔𝑔 = 9.8 m/s2 = 32.2 ft/s2 (near Earth’s surface)
Dynamics
𝛴𝛴𝑭𝑭 = 𝑚𝑚𝒂𝒂 𝑊𝑊𝑊𝑊𝑊𝑊𝑔𝑔ℎ𝑎𝑎 = 𝑚𝑚𝑔𝑔 (near Earths surface)
𝑓𝑓𝑠𝑠,𝑚𝑚𝑎𝑎𝑚𝑚 = 𝜇𝜇𝑠𝑠𝐹𝐹𝑁𝑁
𝑓𝑓𝑘𝑘 = 𝜇𝜇𝑘𝑘𝐹𝐹𝑁𝑁 𝑎𝑎𝑐𝑐 = 𝑎𝑎2
𝑅𝑅 = 𝜔𝜔2𝑅𝑅
Universal Gravitation
Universal Gravitational Constant 𝐺𝐺 = 6.7 × 1011 N m2
kg2
𝐹𝐹𝑔𝑔 = 𝐺𝐺𝑚𝑚1𝑚𝑚2
𝑅𝑅2 𝑈𝑈𝑔𝑔 = 𝐺𝐺𝑚𝑚1𝑚𝑚2
𝑅𝑅
Work & Energy
𝑊𝑊𝐹𝐹 = 𝐹𝐹𝐹𝐹cos(𝜃𝜃) 𝐾𝐾 = 1
2𝑚𝑚𝑣𝑣2 = 𝑝𝑝2
2𝑚𝑚 𝑊𝑊𝑁𝑁𝑁𝑁𝑁𝑁 = 𝑎𝑎𝐾𝐾 = 𝐾𝐾𝑓𝑓 𝐾𝐾𝑖𝑖 𝐸𝐸 = 𝐾𝐾 + 𝑈𝑈
𝑊𝑊𝑛𝑛𝑐𝑐 = 𝑎𝑎𝐸𝐸 = 𝐸𝐸𝑓𝑓 𝐸𝐸𝑖𝑖 = (𝐾𝐾𝑓𝑓 + 𝑈𝑈𝑓𝑓) – (𝐾𝐾𝑖𝑖 + 𝑈𝑈𝑖𝑖) 𝑈𝑈𝑔𝑔𝑔𝑔𝑎𝑎𝑎𝑎 = 𝑚𝑚𝑔𝑔𝑚𝑚
Impulse & Momentum
Impulse: 𝑰𝑰 = 𝑭𝑭𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎 = 𝑎𝑎𝒑𝒑 𝑭𝑭𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎 = 𝑎𝑎𝒑𝒑 = 𝑚𝑚𝒗𝒗𝑓𝑓 𝑚𝑚𝒗𝒗𝑖𝑖 𝑭𝑭𝑎𝑎𝑎𝑎𝑎𝑎 = 𝑎𝑎𝒑𝒑/𝑎𝑎𝑎𝑎
𝛴𝛴𝑭𝑭𝑎𝑎𝑚𝑚𝛥𝛥𝑎𝑎𝑎𝑎 = 𝑎𝑎𝑷𝑷𝛥𝛥𝑡𝑡𝛥𝛥𝑎𝑎𝑡𝑡 = 𝑷𝑷𝛥𝛥𝑡𝑡𝛥𝛥𝑎𝑎𝑡𝑡,𝑓𝑓𝑖𝑖𝑛𝑛𝑎𝑎𝑡𝑡 𝑷𝑷𝛥𝛥𝑡𝑡𝛥𝛥𝑎𝑎𝑡𝑡,𝑖𝑖𝑛𝑛𝑖𝑖𝛥𝛥𝑖𝑖𝑎𝑎𝑡𝑡 (momentum conserved if 𝛴𝛴𝑭𝑭𝑎𝑎𝑚𝑚𝛥𝛥 = 0)
𝒙𝒙𝑐𝑐𝑚𝑚 = 𝑚𝑚1𝒙𝒙1 + 𝑚𝑚2𝒙𝒙2
𝑚𝑚1 + 𝑚𝑚2
Elastic Collisions: Mass 𝒎𝒎𝒊𝒊 moving with 𝒗𝒗𝒊𝒊; Stationary mass 𝑴𝑴
𝑣𝑣𝑚𝑚,𝑓𝑓=𝑣𝑣𝑚𝑚,𝑖𝑖𝑚𝑚−𝑀𝑀
𝑚𝑚+𝑀𝑀 𝑣𝑣𝑀𝑀,𝑓𝑓=𝑣𝑣𝑚𝑚,𝑖𝑖2𝑚𝑚
𝑚𝑚+𝑀𝑀
Rotational Kinematics
𝜔𝜔 = 𝜔𝜔0 + 𝛼𝛼𝑎𝑎 𝜃𝜃= 𝜃𝜃0 + 𝜔𝜔0𝑎𝑎 + 1
2𝛼𝛼𝑎𝑎2 𝜔𝜔2 = 𝜔𝜔0
2 + 2𝛼𝛼𝑎𝑎𝜃𝜃
𝑎𝑎𝑥𝑥𝑁𝑁 = 𝑅𝑅𝑎𝑎𝜃𝜃 𝑣𝑣𝑁𝑁 = 𝑅𝑅𝜔𝜔 𝑎𝑎𝑁𝑁 = 𝑅𝑅𝛼𝛼
(rolling without slipping: 𝑎𝑎𝑥𝑥 = 𝑅𝑅𝑎𝑎𝜃𝜃 𝑣𝑣 = 𝑅𝑅𝜔𝜔 𝑎𝑎 = 𝑅𝑅𝛼𝛼 )
1 revolution = radians
Rotational Statics & Dynamics
𝜏𝜏= 𝐹𝐹𝐹𝐹 sin 𝜃𝜃
𝛴𝛴𝜏𝜏 = 0 and 𝛴𝛴𝐹𝐹 = 0 (static equilibrium)
𝛴𝛴𝜏𝜏 = 𝐼𝐼𝛼𝛼
𝑊𝑊 = 𝜏𝜏𝜃𝜃
𝑳𝑳 = 𝐼𝐼𝝎𝝎 𝛴𝛴𝝉𝝉𝑎𝑎𝑚𝑚𝛥𝛥𝑎𝑎𝑎𝑎 = 𝑎𝑎𝑳𝑳
(angular momentum conserved if 𝑎𝑎𝝉𝝉𝑎𝑎𝑚𝑚𝛥𝛥 = 0)
𝐾𝐾𝑔𝑔𝑡𝑡𝛥𝛥 = 1
2𝐼𝐼𝜔𝜔2 = 𝐿𝐿2
2𝐼𝐼
𝐾𝐾𝛥𝛥𝑡𝑡𝛥𝛥𝑎𝑎𝑡𝑡 = 𝐾𝐾𝛥𝛥𝑔𝑔𝑎𝑎𝑛𝑛𝑠𝑠 + 𝐾𝐾𝑔𝑔𝑡𝑡𝛥𝛥 = 1
2𝑚𝑚𝑣𝑣2 + 1
2𝐼𝐼𝜔𝜔2
𝐼𝐼=𝐼𝐼𝑐𝑐𝑚𝑚 +𝑚𝑚𝐹𝐹2 Parallel axis theorem
Moments of Inertia (I)
𝐼𝐼= 𝛴𝛴𝑚𝑚𝐹𝐹2
(for a collection of point particles)
𝐼𝐼 = 1
2𝑀𝑀𝑅𝑅2 (solid disk or cylinder)
𝐼𝐼 = 2
5𝑀𝑀𝑅𝑅2 (solid ball)
𝐼𝐼 = 2
3𝑀𝑀𝑅𝑅2 (hollow sphere)
𝐼𝐼 = 𝑀𝑀𝑅𝑅2 (hoop or hollow cylinder)
𝐼𝐼 = 1
12 𝑀𝑀𝐿𝐿2 (uniform rod about center)
𝐼𝐼 =
1
3 𝑀𝑀𝐿𝐿
2
(uniform rod about one end)
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Kinematics 𝒗𝒗 (^) 𝑎𝑎𝑎𝑎𝑎𝑎 = 𝛥𝛥𝒙𝒙𝛥𝛥𝛥𝛥 𝒂𝒂𝑎𝑎𝑎𝑎𝑎𝑎 = 𝛥𝛥𝒗𝒗𝛥𝛥𝛥𝛥

𝑣𝑣 = 𝑣𝑣 0 + 𝑎𝑎𝑎𝑎 𝑥𝑥 = 𝑥𝑥 0 + 𝑣𝑣 0 𝑎𝑎 +

𝑎𝑎𝑎𝑎^2

𝑔𝑔 = 9.8 m/s^2 = 32.2 ft/s^2 (near Earth’s surface)

Dynamics 𝛴𝛴𝑭𝑭 = 𝑚𝑚𝒂𝒂 𝑊𝑊𝑊𝑊𝑊𝑊𝑔𝑔ℎ𝑎𝑎 = 𝑚𝑚𝑔𝑔 (near Earth’s surface) 𝑓𝑓𝑠𝑠,𝑚𝑚𝑎𝑎𝑚𝑚 = 𝜇𝜇𝑠𝑠 𝐹𝐹𝑁𝑁

𝑓𝑓𝑘𝑘 = 𝜇𝜇𝑘𝑘 𝐹𝐹𝑁𝑁 𝑎𝑎 (^) 𝑐𝑐 = 𝑎𝑎

2 𝑅𝑅 =^ 𝜔𝜔^

Universal Gravitation

Universal Gravitational Constant 𝐺𝐺 = 6.7 × 10 –^11 N ∙ m

2 kg^2 𝐹𝐹𝑔𝑔 = 𝐺𝐺𝑚𝑚𝑅𝑅^1 2 𝑚𝑚 2 𝑈𝑈𝑔𝑔 = − 𝐺𝐺𝑚𝑚𝑅𝑅^1 𝑚𝑚^2

Work & Energy

𝑊𝑊𝐹𝐹 = 𝐹𝐹𝐹𝐹cos(𝜃𝜃) 𝐾𝐾 = 12 𝑚𝑚𝑣𝑣 2 = 𝑝𝑝^

2 2𝑚𝑚 𝑊𝑊𝑁𝑁𝑁𝑁𝑁𝑁^ =^ 𝑎𝑎𝐾𝐾^ =^ 𝐾𝐾𝑓𝑓^ –^ 𝐾𝐾𝑖𝑖^ 𝐸𝐸^ =^ 𝐾𝐾^ +^ 𝑈𝑈 𝑊𝑊𝑛𝑛𝑐𝑐 = 𝑎𝑎𝐸𝐸 = 𝐸𝐸𝑓𝑓 – 𝐸𝐸𝑖𝑖 = (𝐾𝐾𝑓𝑓 + 𝑈𝑈𝑓𝑓) – (𝐾𝐾𝑖𝑖 + 𝑈𝑈𝑖𝑖) 𝑈𝑈𝑔𝑔𝑔𝑔𝑎𝑎𝑎𝑎 = 𝑚𝑚𝑔𝑔𝑚𝑚

Impulse & Momentum Impulse: 𝑰𝑰 = 𝑭𝑭𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎 = 𝑎𝑎𝒑𝒑 𝑭𝑭𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎 = 𝑎𝑎𝒑𝒑 = 𝑚𝑚𝒗𝒗𝑓𝑓 – 𝑚𝑚𝒗𝒗 (^) 𝑖𝑖 𝑭𝑭 (^) 𝑎𝑎𝑎𝑎𝑎𝑎 = 𝑎𝑎𝒑𝒑/𝑎𝑎𝑎𝑎

𝛴𝛴𝑭𝑭𝑎𝑎𝑚𝑚𝛥𝛥𝑎𝑎𝑎𝑎 = 𝑎𝑎𝑷𝑷𝛥𝛥𝑡𝑡𝛥𝛥𝑎𝑎𝑡𝑡 = 𝑷𝑷𝛥𝛥𝑡𝑡𝛥𝛥𝑎𝑎𝑡𝑡,𝑓𝑓𝑖𝑖𝑛𝑛𝑎𝑎𝑡𝑡 – 𝑷𝑷𝛥𝛥𝑡𝑡𝛥𝛥𝑎𝑎𝑡𝑡,𝑖𝑖𝑛𝑛𝑖𝑖𝛥𝛥𝑖𝑖𝑎𝑎𝑡𝑡 (momentum conserved if 𝛴𝛴𝑭𝑭𝑎𝑎𝑚𝑚𝛥𝛥 = 0) 𝒙𝒙 (^) 𝑐𝑐𝑚𝑚 = 𝑚𝑚^1 𝑚𝑚^ 𝒙𝒙^11 ++^ 𝑚𝑚𝑚𝑚^22 𝒙𝒙^2

Elastic Collisions: Mass 𝒎𝒎 (^) 𝒊𝒊 moving with 𝒗𝒗 (^) 𝒊𝒊 ; Stationary mass 𝑴𝑴 𝑣𝑣𝑚𝑚,𝑓𝑓 = 𝑣𝑣𝑚𝑚,𝑖𝑖𝑚𝑚−𝑀𝑀𝑚𝑚+𝑀𝑀 𝑣𝑣𝑀𝑀,𝑓𝑓 = 𝑣𝑣𝑚𝑚,𝑖𝑖𝑚𝑚+𝑀𝑀2𝑚𝑚

Rotational Kinematics 𝜔𝜔 = 𝜔𝜔 0 + 𝛼𝛼𝑎𝑎 𝜃𝜃 = 𝜃𝜃 0 + 𝜔𝜔 0 𝑎𝑎 + 12 𝛼𝛼𝑎𝑎^2 𝜔𝜔 2 = 𝜔𝜔 02 + 2𝛼𝛼𝑎𝑎𝜃𝜃 𝑎𝑎𝑥𝑥𝑁𝑁 = 𝑅𝑅𝑎𝑎𝜃𝜃 𝑣𝑣𝑁𝑁 = 𝑅𝑅𝜔𝜔 𝑎𝑎𝑁𝑁 = 𝑅𝑅𝛼𝛼 (rolling without slipping: 𝑎𝑎𝑥𝑥 = 𝑅𝑅𝑎𝑎𝜃𝜃 𝑣𝑣 = 𝑅𝑅𝜔𝜔 𝑎𝑎 = 𝑅𝑅𝛼𝛼 ) 1 revolution = 2π radians

Rotational Statics & Dynamics 𝜏𝜏 = 𝐹𝐹𝐹𝐹 sin 𝜃𝜃 𝛴𝛴𝜏𝜏 = 0 and 𝛴𝛴𝐹𝐹 = 0 (static equilibrium) 𝛴𝛴𝜏𝜏 = 𝐼𝐼𝛼𝛼 𝑊𝑊 = 𝜏𝜏𝜃𝜃 𝑳𝑳 = 𝐼𝐼𝝎𝝎 𝛴𝛴𝝉𝝉𝑎𝑎𝑚𝑚𝛥𝛥𝑎𝑎𝑎𝑎 = 𝑎𝑎𝑳𝑳 (angular momentum conserved if 𝑎𝑎𝝉𝝉𝑎𝑎𝑚𝑚𝛥𝛥 = 0) 𝐾𝐾𝑔𝑔𝑡𝑡𝛥𝛥 = 12 𝐼𝐼𝜔𝜔 2 = 𝐿𝐿

2 2𝐼𝐼 𝐾𝐾𝛥𝛥𝑡𝑡𝛥𝛥𝑎𝑎𝑡𝑡 = 𝐾𝐾𝛥𝛥𝑔𝑔𝑎𝑎𝑛𝑛𝑠𝑠 + 𝐾𝐾𝑔𝑔𝑡𝑡𝛥𝛥 = 12 𝑚𝑚𝑣𝑣 2 + 12 𝐼𝐼𝜔𝜔 2 𝐼𝐼 = 𝐼𝐼𝑐𝑐𝑚𝑚 + 𝑚𝑚𝐹𝐹^2 Parallel axis theorem

Moments of Inertia (I) 𝐼𝐼 = 𝛴𝛴𝑚𝑚𝐹𝐹^2 (for a collection of point particles) 𝐼𝐼 =

2 𝑀𝑀𝑅𝑅^

(^2) (solid disk or cylinder)

𝐼𝐼 =

5 𝑀𝑀𝑅𝑅^

(^2) (solid ball)

𝐼𝐼 =

3 𝑀𝑀𝑅𝑅^

(^2) (hollow sphere) 𝐼𝐼 = 𝑀𝑀𝑅𝑅 2 (hoop or hollow cylinder) 𝐼𝐼 =

(^2) (uniform rod about center )

𝐼𝐼 =

𝑀𝑀𝐿𝐿^2 (uniform rod about one end )

Last Name: First Name: Lab Section: Exam Day: Exam Time

Fluids 𝑃𝑃 = 𝐹𝐹𝐴𝐴 , 𝑃𝑃(𝑑𝑑) = 𝑃𝑃(0) + 𝜌𝜌𝑔𝑔𝑑𝑑 change in pressure with depth 𝑑𝑑

𝜌𝜌 = 𝑀𝑀𝑉𝑉 (density) Buoyant force 𝐹𝐹𝐵𝐵 = 𝜌𝜌𝑔𝑔𝑉𝑉𝑑𝑑𝑖𝑖𝑠𝑠 = weight of displaced fluid Flow rate 𝑄𝑄 = 𝑣𝑣 1 𝐴𝐴 1 = 𝑣𝑣 2 𝐴𝐴 2 continuity equation

𝑃𝑃 1 + 12 𝜌𝜌𝑣𝑣 12 + 𝜌𝜌𝑔𝑔𝑚𝑚 1 = 𝑃𝑃 2 + 12 𝜌𝜌𝑣𝑣 22 + 𝜌𝜌𝑔𝑔𝑚𝑚 2 Bernoulli equation

Simple Harmonic Motion Hooke’s Law: 𝐹𝐹𝑠𝑠 = – 𝑘𝑘𝑥𝑥 𝑈𝑈𝑠𝑠𝑝𝑝𝑔𝑔𝑖𝑖𝑛𝑛𝑔𝑔 = 12 𝑘𝑘𝑥𝑥 2 𝑥𝑥(𝑎𝑎) = 𝐴𝐴 cos(𝜔𝜔𝑎𝑎) or 𝑥𝑥(𝑎𝑎) = 𝐴𝐴 sin(𝜔𝜔𝑎𝑎) 𝑣𝑣(𝑎𝑎) = – 𝐴𝐴𝜔𝜔sin(𝜔𝜔𝑎𝑎) 𝑜𝑜𝐹𝐹 𝑣𝑣(𝑎𝑎) = 𝐴𝐴𝜔𝜔cos(𝜔𝜔𝑎𝑎) 𝑎𝑎(𝑎𝑎) = – 𝐴𝐴𝜔𝜔 2 cos(𝜔𝜔𝑎𝑎) or 𝑎𝑎(𝑎𝑎) = – 𝐴𝐴𝜔𝜔 2 sin(𝜔𝜔𝑎𝑎)

Harmonic Waves 𝑣𝑣 = 𝜆𝜆 𝑁𝑁 = 𝜆𝜆 𝑓𝑓 𝑣𝑣 = 𝑐𝑐 = 3 × 10^8 m/s for electromagnetic waves (light, microwaves, etc.)

𝑣𝑣 2 = (^) 𝑚𝑚 𝐹𝐹 �𝐿𝐿 for wave on a string 𝜆𝜆𝑛𝑛 = (^2) 𝑛𝑛 𝐿𝐿 (wavelength, of the 𝑛𝑛𝛥𝛥ℎ^ harmonic)

Sound Waves

Loudness: 𝛽𝛽 = 10 log 10 � 𝐼𝐼𝐼𝐼 0 � (in dB), where 𝐼𝐼 0 = 10 –^12 W/m^2 𝐼𝐼 = 4𝜋𝜋𝑃𝑃𝑔𝑔 2 (sound intensity)

𝛽𝛽 2 − 𝛽𝛽 1 = (10 dB)^ log 10 �

𝑓𝑓𝑡𝑡𝑜𝑜𝑠𝑠𝑎𝑎𝑔𝑔𝑎𝑎𝑎𝑎𝑔𝑔 = 𝑓𝑓𝑠𝑠𝑡𝑡𝑠𝑠𝑔𝑔𝑐𝑐𝑎𝑎^ (𝑎𝑎 𝑎𝑎𝑤𝑤𝑤𝑤𝑤𝑤𝑤𝑤^ −𝑎𝑎𝑜𝑜𝑜𝑜𝑜𝑜𝑤𝑤𝑜𝑜𝑤𝑤𝑤𝑤𝑜𝑜)

𝑤𝑤𝑤𝑤𝑤𝑤𝑤𝑤 −𝑎𝑎𝑜𝑜𝑜𝑜𝑠𝑠𝑜𝑜𝑠𝑠𝑤𝑤 (Doppler Effect)

𝜔𝜔^2 = 𝑚𝑚𝑘𝑘 𝑇𝑇 = 2 𝜔𝜔𝜋𝜋 = 2 𝜋𝜋�𝑚𝑚 𝑘𝑘 𝑓𝑓 = 1 /𝑇𝑇

For a simple pendulum 𝜔𝜔 2 = 𝑔𝑔𝐿𝐿 , 𝑇𝑇 = 2 𝜋𝜋 L / g

𝜌𝜌𝑤𝑤𝑎𝑎𝛥𝛥𝑎𝑎𝑔𝑔 = 1000 kg/m^3 1 m^3 = 1000 liters 1 atm = 1.01 𝑥𝑥 105 Pa 1 Pa = 1 N/m^2

(area of circle A=πr^2 )