Rotation

Galaxy rotation curve

The rotation curve of a disc galaxy (also called a velocity curve) is a plot of the orbital speeds of visible stars or gas in that galaxy versus their radial distance from that galaxy's centre. It is typically rendered graphically as a plot, and the data observed from each side of a spiral galaxy are generally asymmetric, so that data from each side are averaged to create the curve. A significant discrepancy exists between the experimental curves observed, and a curve derived by applying gravity theory to the matter observed in a galaxy. Theories involving dark matter are the main postulated solutions to account for the variance. The rotational/orbital speeds of galaxies/stars do not follow the rules found in other orbital systems such as stars/planets and planets/moons that have most of their mass at the centre. Stars revolve around their galaxy's centre at equal or increasing speed over a large range of distances. In contrast, the orbital velocities of planets in planetary systems and moons orbiting planets decline with distance according to Kepler’s third law. This reflects the mass distributions within those systems. The mass estimations for galaxies based on the light they emit are far too low to explain the velocity observations. The galaxy rotation problem is the discrepancy between observed galaxy rotation curves and the theoretical prediction, assuming a centrally dominated mass associated with the observed luminous material. When mass profiles of galaxies are calculated from the distribution of stars in spirals and mass-to-light ratios in the stellar disks, they do not match with the masses derived from the observed rotation curves and the law of gravity. A solution to this conundrum is to hypothesize the existence of dark matter and to assume its distribution from the galaxy's center out to its halo. Though dark matter is by far the most accepted explanation of the rotation problem, other proposals have been offered with varying degrees of success. Of the , one of the most notable is modified Newtonian dynamics (MOND), which involves modifying the laws of gravity. (Wikipedia).

Galaxy rotation curve
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Teach Astronomy - Rotation Curve of the Galaxy

http://www.teachastronomy.com/ Maps of star and gas motions reveal the rotation curve of the Milky Way galaxy shown as a plot of orbital speed or circular velocity as a function of distance from the galactic center. In the Milky Way the speed is zero at the center and it rises rapidly to

From playlist 18. Galaxies

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Teach Astronomy - Rotation Curves

http://www.teachastronomy.com/ The best way to measure the mass of any spiral galaxy is a rotation curve. In this observational technique the slit of a spectrograph is laid across the major axis of a galaxy, and astronomers measure the circular velocity of stars or gas in the disk as a fu

From playlist 19. Galaxies 2

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Teach Astronomy - Galaxy Luminosity Function

http://www.teachastronomy.com/ The galaxy luminosity function is a basic tool that astronomers use for describing the demographics of galaxies. It's quoted in terms of the number of galaxies per unit volume, or per unit megaparsec, per unit luminosity interval, or per unit magnitude. The

From playlist 20. Galaxy Interaction and Motion

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Teach Astronomy - Flat Rotation Curves

http://www.teachastronomy.com/ Newton's law of gravity gives astronomers a way of estimating the mass of something from the motions of objects within it. In the solar system or when an object has its mass concentrated in the center, the circular velocity declines with increasing distance

From playlist 18. Galaxies

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Teach Astronomy - Motions in the Disk

http://www.teachastronomy.com/ Stars near the Sun have radial velocities measured by the Doppler shift in the range of ten to twenty kilometers per second. Because us and the stars around us are all moving together at similar speeds around the center of our galaxy the differential speeds

From playlist 18. Galaxies

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From playlist ASTRONOMY 1 INTRODUCTION

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From playlist ASTRONOMY 28 THE MILKY WAY GALAXY

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http://www.teachastronomy.com/ The mass of spiral galaxies is typically measured by following the rotation of stars in their circular orbits around the center of the galaxy. The way this circular velocity varies with distance from the galactic center gives a measure of the mass, although

From playlist 19. Galaxies 2

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Teach Astronomy - Formation of Spirals

http://www.teachastronomy.com/ When a large primordial gas cloud has a large amount of rotation or angular momentum the collapse will occur preferentially along the rotation axis leading to a disc-like formation. The disc will subsequently shear, and gas pockets will collapse within the d

From playlist 20. Galaxy Interaction and Motion

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The Distribution of Dark Matter in Galaxies : from observations to cosmological sim..by Mousumi Das

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From playlist LESS TRAVELLED PATH TO THE DARK UNIVERSE

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M94 - Rings and Rotation Curves - Deep Sky Videos

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From playlist Messier Objects

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From Pythagoras to Einstein: The Geometry of Space and Time

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From playlist Science

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From playlist Less Travelled Path of Dark Matter: Axions and Primordial Black Holes (Online)

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From playlist Astrophysics Seminar

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Experimental Physics I: Final Presentation: Galactic rotation curve and structure of the Milky Way.

MIT 8.13-14 Experimental Physics I & II "Junior Lab", Spring 2017 View the complete course: https://ocw.mit.edu/8-13-14S17 Instructor: Saarik Kalia For his final student presentation in the course Experimental Physics I ("Junior Lab"), Saarik Kalia gave a talk on the topic Observation of

From playlist How We Teach: MIT 8.13-14 Experimental Physics I & II “Junior Lab”, Fall 2016 - Spring 2017

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The 'Observed' Phase-Space of Dark Matter in Galaxies by Subhabrata Majumdar

PROGRAM LESS TRAVELLED PATH TO THE DARK UNIVERSE ORGANIZERS: Arka Banerjee (IISER Pune), Subinoy Das (IIA, Bangalore), Koushik Dutta (IISER, Kolkata), Raghavan Rangarajan (Ahmedabad University) and Vikram Rentala (IIT Bombay) DATE & TIME: 13 March 2023 to 24 March 2023 VENUE: Ramanujan

From playlist LESS TRAVELLED PATH TO THE DARK UNIVERSE

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Teach Astronomy - Binary Galaxies

http://www.teachastronomy.com/ Binary galaxies are pairs of galaxies bound by gravity orbiting each other. In a sense it's directly analogous to a binary star situation where the stars are orbiting each other held together by gravity. The difference is that galaxies are huge massive obje

From playlist 20. Galaxy Interaction and Motion

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Cold Dark Matter and Galaxy Formation by Andrea Valerio Macciò

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From playlist Cosmology - The Next Decade

Related pages

Spiral galaxy | Mass-to-light ratio | Gravitational constant | Oort constants