• Study Resource
  • Explore
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Motion: Forces and Cases of Motion
Motion: Forces and Cases of Motion

Forming disk galaxies in magneto-hydro
Forming disk galaxies in magneto-hydro

... highly supersonic flows occurring in cosmology, and to treating subsonic turbulence within the gas of virialized halos. These properties make it superior to smoothed particle hydrodynamics and adaptive mesh refinement codes that use a stationary Cartesian mesh. AREPO also follows the dynamics of dar ...
Chapter 10 study guide answers
Chapter 10 study guide answers

... 34. If you blow up a balloon and let it go…why does it fly forward? Draw a diagram with labels. Action-Reaction Pairs. Newton’s 3rd law. Air from balloon pushes on air outside of the balloon. The air outside of the balloon pushes back at the balloon. 35. What is the Law of Conservation of Momentum? ...
presentation source
presentation source

Two-Gyro Performance, Scheduling and Acquisitions
Two-Gyro Performance, Scheduling and Acquisitions

... – This problem was identified by the OTA SEs in some follow-on analysis of the previous problem’s test results. However, the cause of this problem is different. – Problem only occurs with Target-ReAcq style Acqs/ReAcqs where both PASS and the onboard ReAcq process are effectively accounting for a po ...
Forces and Motion
Forces and Motion

... and opposite force on the first object • Momentum – Product of an object’s mass and its velocity – Objects momentum at rest is zero – Unit kg m/s ...
Quick facts #2: The two
Quick facts #2: The two

... the two stars orbiting each other are similar. Even for planetary motion there is a small but important correction to be made once the orbital motion of the Sun is taken into account. The good news is that we can apply all our old results, with suitable modifications. ...
Notes Forces- Gravitational, Mag., Elec. File
Notes Forces- Gravitational, Mag., Elec. File

... tell us how attracted they are to each other.) ...
Spring 2011 Final Review Guide
Spring 2011 Final Review Guide

Newton’s Laws of Motion - University of Mississippi
Newton’s Laws of Motion - University of Mississippi

Ch. 13 Quiz - westscidept
Ch. 13 Quiz - westscidept

... _____ 1. Force is A) a push B) a pull C) the ability to change motion D) all of the above _____ 2. Forces that are opposite and equal are called A) balanced B) friction C) unbalanced D) gravitational _____ 3. The force that opposes the motion of an object is called A) acceleration B) friction C) den ...
Ch.4 Questions Holt Physics key page 2
Ch.4 Questions Holt Physics key page 2

... forces required to lift them on Earth? 16. Draw a force diagram to identif)' all the actionreaction pairs that exist for a horse pulling a cart. ...
Document
Document

Kinematics - Gymnázium Slovanské náměstí
Kinematics - Gymnázium Slovanské náměstí

Assignment 8 Solutions
Assignment 8 Solutions

... Bonus: [7 points] A 0.50-kg ball that is tied to the end of a 1.5-m light cord is revolved in a horizontal plane with the cord making a 30⁰ angle with the vertical. a. Determine the ball’s speed. b. If, instead the ball is revolved so that its speed is 4.0 m/s, what angle does the cord make with th ...
Document
Document

21.ForcesReview
21.ForcesReview

Newton`s Laws PPT
Newton`s Laws PPT

... unbalanced force. This a short video clip that demonstrates this law. http://www.youtube.com/watch?v=8zsE3mpZ6Hw&feature=related ...
PRACTICE Final Exam: MULTIPLE CHOICE PROBLEMS
PRACTICE Final Exam: MULTIPLE CHOICE PROBLEMS

The Milky Way Galaxy
The Milky Way Galaxy

... The Rotation Curve of the Milky Way To map out vr throughout Galaxy, divide the Galaxy into quadrants based on value of galactic longitude. Quad I (l<90) - looking to material closest to GC, [ω - ω0] gets larger and vr increases. At point of closest approach (subcentral or tangent point) vr is at m ...
MilkyWay
MilkyWay

Lecture 12.Gravitati.. - Faculty Web Sites at the University of Virginia
Lecture 12.Gravitati.. - Faculty Web Sites at the University of Virginia

... “weightlessness”. They do have a gravitational force acting on them, though! The satellite and all its contents are in free fall, so there is no normal force. This is what leads to the experience of weightlessness. ...
solns
solns

... is the mass within radius r. To make this force independent of r, we must have m(r) = Ar2 for some constant A. If the radius of the planet is R and its total mass M , then m(R) = M implies A = M/R2 . To find the density, we differentiate the above expression for m(r), using the fundamental theorem o ...
Physics Today
Physics Today

What have we learned?
What have we learned?

< 1 ... 275 276 277 278 279 280 281 282 283 ... 432 >

Modified Newtonian dynamics



In physics, modified Newtonian dynamics (MOND) is a theory that proposes a modification of Newton's laws to account for observed properties of galaxies. Created in 1983 by Israeli physicist Mordehai Milgrom, the theory's original motivation was to explain the fact that the velocities of stars in galaxies were observed to be larger than expected based on Newtonian mechanics. Milgrom noted that this discrepancy could be resolved if the gravitational force experienced by a star in the outer regions of a galaxy was proportional to the square of its centripetal acceleration (as opposed to the centripetal acceleration itself, as in Newton's Second Law), or alternatively if gravitational force came to vary inversely with radius (as opposed to the inverse square of the radius, as in Newton's Law of Gravity). In MOND, violation of Newton's Laws occurs at extremely small accelerations, characteristic of galaxies yet far below anything typically encountered in the Solar System or on Earth.MOND is an example of a class of theories known as modified gravity, and is an alternative to the hypothesis that the dynamics of galaxies are determined by massive, invisible dark matter halos. Since Milgrom's original proposal, MOND has successfully predicted a variety of galactic phenomena that are difficult to understand from a dark matter perspective. However, MOND and its generalisations do not adequately account for observed properties of galaxy clusters, and no satisfactory cosmological model has been constructed from the theory.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report