ap-phys1_ap1-gravitation-presentation_2022-12-14

pdf

School

Bergen County Technical Schools *

*We aren’t endorsed by this school

Course

101

Subject

Physics

Date

Jan 9, 2024

Type

pdf

Pages

65

Uploaded by MasterFireFinch34

Report
AP Physics 1 Newton's Law of Universal Gravitation 2022-12-14 www.njctl.org https://njctl.org/video/?v=37GTvsrVHKE
Newton's Law of Universal Gravitation Click on the topic to go to that section · Gravitational Force · Gravitational Field · Orbital Motion · Kepler's Third Law of Motion · Surface Gravity · Gravitational Field in Space
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Return to Table of Contents Gravitational Force https://njctl.org/video/?v=bXA3KTy8giQ
Newton’s Law of Universal Gravitation It has been well known since ancient times that Earth is a sphere and objects that are near the surface tend fall down.
Newton’s Law of Universal Gravitation Newton connected the idea that objects, like apples, fall towards the center of Earth with the idea that the moon orbits around Earth...it's also falling towards the center of Earth. The moon just stays in circular motion since it has a velocity perpendicular to its acceleration. click here for a cool episode of "minute physics" about why Earth orbits the sun and doesn't crash into it!
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Newton’s Law of Universal Gravitation Newton concluded that all objects attract one another with a "gravitational force". The magnitude of the gravitational force decreases as the centers of the masses increases in distance. M 1 M 2 r M 1 M 2 r MORE Gravitational attraction LESS Gravitational attraction
Newton’s Law of Universal Gravitation Mathematically, the magnitude of the gravitational force is proportional to the masses of the objects and inversely proportional to the square of the distance between the two objects.
G = 6.67 x 10 -11 N-m 2 /kg 2 Gravitational Constant In 1798, Henry Cavendish measured G using a torsion beam balance. He did not initially set out to measure G, he was instead trying to measure the density of the Earth. Click here for an interesting video by "Sixty Symbols" about the unusual man Henry Cavandish and his contributions to science.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Newton’s Law of Universal Gravitation The direction of the force is along the line connecting the centers of the two masses. Each mass feels a force of attraction towards the other mass...along that line. r
Newton’s Law of Universal Gravitation Newton's third law tells us that the force on each mass is equal. That means that if I drop a pen, the force of Earth pulling the pen down is equal to the force of the pen pulling Earth up. However, since the mass of Earth is so much larger, that force causes the pen to accelerate down, while the movement of Earth up is completely unmeasurable.
1 What is the magnitude of the gravitational force between Earth and its moon? r = 3.8 x 10 8 m m Earth = 6.0 x 10 24 kg m moon = 7.3 x 10 22 kg A 2.0 x 10 18 N B 2.0 x 10 19 N C 2.0 x 10 20 N D 2.0 x 10 21 N E I need help Answer https://njctl.org/video/?v=yyzyTfviOy8
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
2 What is the magnitude of the gravitational force between Earth and its sun? r = 1.5 x 10 11 m m Earth = 6.0 x 10 24 kg m sun = 2.0 x 10 30 kg A 3.6 x 10 -18 N B 3.6 x 10 19 N C 3.6 x 10 21 N D 3.6 x 10 22 N E I need help Answer https://njctl.org/video/?v=ttgkGNRVkzc
3 The gravitational force between two objects is F. What is the force F' between those objects when the distance between them is halved? A 1/2 F B 1/4 F C 2F D 4F E I need help Answer https://njctl.org/video/?v=u8DhbTDSP1k
4 The gravitational force between two objects is F. What is the force F' between those objects when the mass of one object is doubled? A 1/4 F B 1/2 F C 2 F D 4 F E I need help Answer https://njctl.org/video/?v=ePppQNximvQ
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
5 The gravitational force between two objects is F. What is the force F' between those objects when the distance between them is doubled? A 1/4 F B 1/2 F C 2 F D 4 F E I need help Answer https://njctl.org/video/?v=ZBtWBMOzLG0
Newton’s Law of Universal Gravitation Recall that density is: Where m is mass and V is volume. And that the volume of a sphere is: Where r is the radius of the sphere. Now we can see what happens to the gravitational force between two objects when the mass, density, or volume is changed. https://njctl.org/video/?v=9V7uduz6o5Q
Newton’s Law of Universal Gravitation Since F G can be written as: R 1 R 2 For example, lets look at the gravitational force between two spheres shown to the right.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
6 Two solid spheres made of the same material and radii R attract each other with a gravitational force F, when they are in contact with each other. The two spheres are replaced with two new spheres of the same material with radii 2R. What is the new gravitational force between them in terms of F? A 1/2 F B 2 F C 8 F D 16 F E I need help Answer https://njctl.org/video/?v=zx1QLxeYk3g
7 Two solid spheres made of the same material and radii R attract each other with a gravitational force F, when they are in contact with each other. One of the spheres is replaced with a new sphere of the same material with radii 3R. What is the new gravitational force between them in terms of F? A 3/4 F B 9/4 F C 27/4 F D 4/3 F E I need help Answer https://njctl.org/video/?v=xDGzmxYjARU
Return to Table of Contents Gravitational Field https://njctl.org/video/?v=3EVaDFPtrmY
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Gravitational Field While the force between two objects can always be computed by using the formula for F G ; it's sometimes convenient to consider one mass as creating a gravitational field and the other mass responding to that field.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Gravitational Field The magnitude of the gravitational field created by an object varies from location to location in space; it depends on the distance from the object and the object's mass. Gravitational field, g, is a vector. It's direction is always towards the object creating the field. That's the direction of the force that a test mass would experience if placed at that location. In fact, g is the acceleration that a mass would experience if placed at that location in space.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
8 Where is the gravitational field the strongest? A B C D E F I need help Answer https://njctl.org/video/?v=QEhFVZEEGQI
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
9 What happens to the gravitational field if the distance from the center of an object doubles? A It doubles B It quadruples C It is cut to one half D It is cut to one fourth E I need help Answer https://njctl.org/video/?v=eCGQOUVnHZM
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
10 What happens to the gravitational field if the mass of an object doubles? A It doubles B It quadruples C It is cut to one half D It is cut to one fourth E I need help Answer https://njctl.org/video/?v=DEDGMwPfDT0
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Return to Table of Contents Surface Gravity https://njctl.org/video/?v=jKshOWIusxI
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Surface Gravity Planets, stars, moons, all have a gravitational field...since they all have mass. That field is largest at the object's surface, where the distance from the center of the object is the smallest...when "r" is the radius of the object. By the way, only the mass of the planet that's closer to the center of the planet than you are contributes to its gravitational field. So the field actually gets smaller if you tunnel down below the surface. R M
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
11 Determine the surface gravity of Earth's moon. Its mass is 7.4 x 10 22 kg and its radius is 1.7 x 10 6 m. A 1.7 m/s 2 B 2.9 m/s 2 C 4.4 m/s 2 D 6.2 m/s 2 E I need help Answer https://njctl.org/video/?v=Y1UkIitc5FQ
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
12 Compute g for the surface of a planet whose radius is double that of the Earth and whose mass is triple that of Earth. A 1.89 m/s 2 B 3.36 m/s 2 C 5.91 m/s 2 D 7.32 m/s 2 E I need help https://njctl.org/video/?v=2xaHPOs5WQE Answer
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Surface Gravity Again density is: So . And that the volume of a sphere is: Now we can see what happens to the surface gravity of a planet when the mass, density, or volume is changed. https://njctl.org/video/?v=TwywDsJRYMc
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Surface Gravity For example, we can rewrite the equation for surface gravity in terms of density and radius.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
13 Compute g for the surface of a planet whose radius is double that of the Earth and whose density is the same as that of Earth. A 1/4 g earth B 1/2 g earth C 2 g earth D 4 g earth E I need help Answer https://njctl.org/video/?v=QnjFGRbMQhw
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
14 Compute g for the surface of a planet whose radius is the same as that of the Earth and whose density is 1/3 that of Earth. A 1/9 g earth B 1/3 g earth C 3 g earth D 9 g earth E I need help https://njctl.org/video/?v=cCIoIpFmnME Answer
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
15 Compute g for the surface of a planet whose radius is half that of Earth and whose density is 3/2 that of Earth. A 1.7 N/kg B 2.5 N/kg C 7.4 N/kg D 13 N/kg E I need help Answer https://njctl.org/video/?v=N86KjjUukLg
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Return to Table of Contents Gravitational Field in Space https://njctl.org/video/?v=YUJWRILEFJY
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Gravitational field in space While gravity gets weaker as you get farther from a planet, it never becomes zero. There is always some gravitational field present due to every planet, star and moon in the universe.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Gravitational field in space The local gravitational field is usually dominated by nearby masses since gravity gets weaker as the inverse square of the distance. The contribution of a planet to the local gravitational field can be calculated using the same equation we've been using. You just have to be careful about "r".
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Gravitational field in space The contribution of a planet to the local gravitational field can be calculated using the same equation we've been using. You just have to be careful about "r". If a location, "A", is a height "h" above a planet of radius "R", it is a distance "r" from the planet's center, where r = R + h. R M A h r
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
16 Determine the gravitational field of Earth at a height of 6.4 x 10 6 m (1 Earth radius). Earth's mass is 6.0 x 10 24 kg and its radius is 6.4 x 10 6 m. A 1.7 m/s 2 B 2.5 m/s 2 C 4.2 m/s 2 D 6.9 m/s 2 E I need help Answer https://njctl.org/video/?v=db3OrEImsAw
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
17 Determine the gravitational field of Earth at a height 2.88 x 10 8 m above its surface (the height of the moon above Earth). Earth's mass is 6.0 x 10 24 kg and its radius is 6.4 x 10 6 m. A 6.1x10 -4 m/s 2 B 1.4x10 -4 m/s 2 C 8.2x10 -3 m/s 2 D 4.6x10 -3 m/s 2 E I need help Answer https://njctl.org/video/?v=URSbcVVAtSk
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
It orbits at an altitude of approximately 350 km (190 mi) above the surface of the Earth, and travels at an average speed of 27,700 kilometers (17,210 mi) per hour. This means the astronauts see 15 sunrises everyday! The International Space Station (ISS) is a research facility that is in a Low Earth Orbit and can be seen from Earth with the naked eye! Its on-orbit construction began in 1998. The International Space Station (ISS) https://njctl.org/video/?v=5b3bElqVQP8
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
18 The occupants of the space station appear to be weightless, they float. Determine the strength of Earth's gravitational field acting on astronaut's in the international space station. Earth's mass is 6.0 x 10 24 kg and its radius is 6.4 x 10 6 m. The ISS is 350km (3.5 x 10 5 m) above the surface of the earth. A 1.3 m/s 2 B 3.9 m/s 2 C 5.7 m/s 2 D 8.8 m/s 2 E I need help Answer https://njctl.org/video/?v=nFzzP6XcPAU
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
19 How does the gravitational field acting on the occupants in the space station compare to that acting on you now. A It's the same. B It's slightly less. C It's about half as strong. D There is no gravity acting on them. E I need help https://njctl.org/video/?v=gLAWZz1FIL0 Answer
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Return to Table of Contents Orbital Motion https://njctl.org/video/?v=eaC8Dv5Q_iU
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
R r Earth ISS h Orbital Motion We've already determined that the gravitational field acting on the occupants of the space station, and on the space station itself, is not very different than the field acting on us here on Earth's surface. How come they don't fall to Earth? This diagram should look really familiar….
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Orbital Motion The gravitational field will be pointed towards the center of Earth and represents the acceleration that a mass would experience at that location (regardless of the mass). In this case any object would simply fall to Earth. How could that be avoided? Earth a ISS
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Orbital Motion If the object has a tangential velocity perpendicular to its acceleration, it will go in a circle. It will keep falling to Earth, but never strike Earth. a v Click here for an interesting look at why the astronauts inside the space station appear to be weightless.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Orbital Motion Here is Newton's own drawing of a thought experiment where a cannon on a very high mountain (above the atmosphere) shoots a shell with increasing speed, shown by trajectories for the shell of D, E, F, and G and finally so fast that it never falls to earth, but goes into orbit. click here for another look at trajectories and orbital motion by Kahn Academy
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Orbital Motion We can calculate the velocity necessary to maintain a stable orbit at a distance "r" from the center of a planet of mass "M". a v
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Orbital Motion From that, we can calculate the period, T, of any object's orbit. a v or
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
20 Compute g at a distance of 7.3 x 10 8 m from the center of a spherical object whose mass is 3.0 x 10 27 kg. A 0.38 m/s 2 B 0.55 m/s 2 C 0.71 m/s 2 D 0.88 m/s 2 E I need help Answer https://njctl.org/video/?v=F0s9Fko1Sjo
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
21 Use your previous answer to determine the velocity, both magnitude and direction, for an object orbiting at a distance of 7.3 x 10 8 m from the center of a spherical object whose mass is 3.0 x 10 27 kg. A 3.1x10 3 m/s B 8.8x10 3 m/s C 1.6x10 4 m/s D 5.5x10 4 m/s E I need help Answer https://njctl.org/video/?v=bNoSgTF46qo
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
22 Use your previous answer to determine the orbital period of for an object orbiting at a distance of 7.3 x 10 8 m from the center of a spherical object whose mass is 3.0 x 10 27 kg. A 2.9x10 5 s B 6.5x10 5 s C 3.8x10 6 s D 7.9x10 6 s E I need help Answer https://njctl.org/video/?v=Mr2_Zmrl-e8
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
23 Compute g at a height of 59 earth radii above the surface of Earth. A 8.8x10 -3 m/s 2 B 2.7x10 -3 m/s 2 C 7.2x10 -2 m/s 2 D 3.1x10 -2 m/s 2 E I need help Answer https://njctl.org/video/?v=K-BzHvwo1-4
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
24 Use your previous answer to determine the velocity, both magnitude and direction, for an object orbiting at height of 59 R E above the surface of Earth. A 1000 m/s B 1500 m/s C 1700 m/s D 2000 m/s E I need help Answer https://njctl.org/video/?v=OR-8wZhTKxs
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
25 Use your previous answer to determine the orbital period of an object orbiting at height of 59 R E above the surface of Earth. A 1.2x10 6 s B 2.4x10 6 s C 4.9x10 6 s D 7.3x10 6 s E I need help Answer https://njctl.org/video/?v=yg40bp3KX90
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
26 Two satellites orbit two different planets with the same radius but different densities. The density of the first planet is ρ and the density of the second planet is 2 ρ . Both satellites are at the same height above their planets. What is the orbital speed of the second satellite in terms if the orbital speed of the first? A v 2 = √ (2)v 1 B v 2 = 2v 1 C v 2 = 4v 1 D v 2 = v 1 /2 E I need help Answer https://njctl.org/video/?v=LSwSDuGY46U
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
27 Two satellites orbit two different planets at the same distance to the center of the planet and with the same density but different radii. The radius of the first planet is R and the radius of the second planet is 2R. What is the orbital speed of the second satellite in terms if the orbital speed of the first? A v 2 = √ (2)v 1 B v 2 = 2v 1 C v 2 = v 1 D v 2 = 2 √ (2)v 1 E I need help Answer https://njctl.org/video/?v=Zv6Diz7sFGM
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Return to Table of Contents Kepler's Third Law of Motion https://njctl.org/video/?v=GjFOJyRQ-0k
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Orbital Motion Now, we can find the relationship between the period, T, and the orbital radius, r, for any orbit.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
Kepler's Third Law Kepler had noted that the ratio of T 2 / r 3 yields the same result for all the planets. That is, the square of the period of any planet's orbit divided by the cube of its distance from the sun always yields the same number. We have now shown why: (4 π 2 ) / (GM) is a constant; its the same for all orbiting objects, where M is the mass of the object being orbited; it is independent of the object that is orbiting.
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
If you know the period (T) of a planet's orbit, you can determine its distance (r) from the sun. Since all planets orbiting the sun have the same period to distance ratio, the following is true: r (white) 3 r (green) 3 T (white) 2 T (green) 2 = Kepler's Third Law
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
28 The period of the Moon is 27.3 days and its orbital radius is 3.8 x 10 8 m. What would be the orbital radius of an object orbiting Earth with a period of 20 days? A 1.0x10 8 m B 2.2x10 8 m C 3.1x10 8 m D 4.0x10 8 m E I need help Answer https://youtu.be/W5mgMtgE-Kg
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help
29 What is the orbital period (in days) of an unknown object orbiting the sun with an orbital radius of twice that of earth? A 470 days B 690 days C 854 days D 1032 days E I need help Answer https://njctl.org/video/?v=Uxg0EcFN9b4
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
  • Access to all documents
  • Unlimited textbook solutions
  • 24/7 expert homework help

Related Documents

Physics Tutorial_ Ohm's Law and the V-I-R Relationship.pdf
Ch 2 Online HW.docx
Kami Export - 8.4_RotationalandReflectionalSymmetry_worksheet.pdf
Lab 8.pdf
PHY 213 Lab 4 Worksheet Magnets and Magnetic fields.docx
Projectile Lab - MarcusL and IsabellaW.docx
Copy of Rec08_Induction.pdf
Exp. 7 Mirrors and Lenses #2.docx
Lab THE LAW OF REFRACTION.docx
LAB Assignment Spring Propelled Projectile (1).docx
Lab2_VanLe.docx
Lab11_VanLe.docx
Recommended textbooks for you
Text book image
Physics for Scientists and Engineers, Technology ...
Physics
ISBN:9781305116399
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Physics for Scientists and Engineers: Foundations...
Physics
ISBN:9781133939146
Author:Katz, Debora M.
Publisher:Cengage Learning
Text book image
College Physics
Physics
ISBN:9781285737027
Author:Raymond A. Serway, Chris Vuille
Publisher:Cengage Learning
Text book image
Principles of Physics: A Calculus-Based Text
Physics
ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Physics for Scientists and Engineers with Modern ...
Physics
ISBN:9781337553292
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Physics for Scientists and Engineers
Physics
ISBN:9781337553278
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
SEE MORE TEXTBOOKS
Recommended textbooks for you
Text book image
Physics for Scientists and Engineers, Technology ...
Physics
ISBN:9781305116399
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Physics for Scientists and Engineers: Foundations...
Physics
ISBN:9781133939146
Author:Katz, Debora M.
Publisher:Cengage Learning
Text book image
College Physics
Physics
ISBN:9781285737027
Author:Raymond A. Serway, Chris Vuille
Publisher:Cengage Learning
Text book image
Principles of Physics: A Calculus-Based Text
Physics
ISBN:9781133104261
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Physics for Scientists and Engineers with Modern ...
Physics
ISBN:9781337553292
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
Text book image
Physics for Scientists and Engineers
Physics
ISBN:9781337553278
Author:Raymond A. Serway, John W. Jewett
Publisher:Cengage Learning
SEE MORE TEXTBOOKS