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28 relations: Accretion disk, Angular momentum, Angular velocity, Christoph Scheiner, Convection, Doppler broadening, Doppler effect, Formation and evolution of the Solar System, Fourier transform, Galaxy, Galileo Galilei, Giovanni Domenico Cassini, Helioseismology, Jupiter, Line Spectra, Molecular cloud, Protostar, Rotation, Saturn, Shearing (physics), Solar cycle, Solar rotation, Solar System, Stellar rotation, Stellar wind, Sun, Sunspot, Ultra-cool dwarf.
Accretion disk
An accretion disk is a structure (often a circumstellar disk) formed by diffused material in orbital motion around a massive central body.
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Angular momentum
In physics, angular momentum (rarely, moment of momentum or rotational momentum) is the rotational equivalent of linear momentum.
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Angular velocity
In physics, the angular velocity of a particle is the rate at which it rotates around a chosen center point: that is, the time rate of change of its angular displacement relative to the origin.
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Christoph Scheiner
Christoph Scheiner SJ (25 July 1573 (or 1575) – 18 June 1650) was a Jesuit priest, physicist and astronomer in Ingolstadt.
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Convection
Convection is the heat transfer due to bulk movement of molecules within fluids such as gases and liquids, including molten rock (rheid).
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Doppler broadening
In atomic physics, Doppler broadening is the broadening of spectral lines due to the Doppler effect caused by a distribution of velocities of atoms or molecules.
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Doppler effect
The Doppler effect (or the Doppler shift) is the change in frequency or wavelength of a wave in relation to observer who is moving relative to the wave source.
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Formation and evolution of the Solar System
The formation and evolution of the Solar System began 4.6 billion years ago with the gravitational collapse of a small part of a giant molecular cloud.
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Fourier transform
The Fourier transform (FT) decomposes a function of time (a signal) into the frequencies that make it up, in a way similar to how a musical chord can be expressed as the frequencies (or pitches) of its constituent notes.
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Galaxy
A galaxy is a gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter.
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Galileo Galilei
Galileo Galilei (15 February 1564Drake (1978, p. 1). The date of Galileo's birth is given according to the Julian calendar, which was then in force throughout Christendom. In 1582 it was replaced in Italy and several other Catholic countries with the Gregorian calendar. Unless otherwise indicated, dates in this article are given according to the Gregorian calendar. – 8 January 1642) was an Italian polymath.
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Giovanni Domenico Cassini
Giovanni Domenico Cassini (8 June 1625 – 14 September 1712) was an Italian (naturalised French) mathematician, astronomer and engineer.
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Helioseismology
Helioseismology, a term coined by Douglas Gough, is the study of the structure and dynamics of the Sun through its oscillations.
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Jupiter
Jupiter is the fifth planet from the Sun and the largest in the Solar System.
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Line Spectra
LINE SPECTRA is a Canadian indie rock band formed in 2006 from Montreal, Quebec.
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Molecular cloud
A molecular cloud, sometimes called a stellar nursery (if star formation is occurring within), is a type of interstellar cloud, the density and size of which permit the formation of molecules, most commonly molecular hydrogen (H2).
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Protostar
A protostar is a very young star that is still gathering mass from its parent molecular cloud.
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Rotation
A rotation is a circular movement of an object around a center (or point) of rotation.
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Saturn
Saturn is the sixth planet from the Sun and the second-largest in the Solar System, after Jupiter.
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Shearing (physics)
Shearing in continuum mechanics refers to the occurrence of a shear strain, which is a deformation of a material substance in which parallel internal surfaces slide past one another.
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Solar cycle
The solar cycle or solar magnetic activity cycle is the nearly periodic 11-year change in the Sun's activity (including changes in the levels of solar radiation and ejection of solar material) and appearance (changes in the number and size of sunspots, flares, and other manifestations).
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Solar rotation
Solar rotation varies with latitude because the Sun is composed of a gaseous plasma.
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Solar System
The Solar SystemCapitalization of the name varies.
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Stellar rotation
Stellar rotation is the angular motion of a star about its axis.
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Stellar wind
A stellar wind is a flow of gas ejected from the upper atmosphere of a star.
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Sun
The Sun is the star at the center of the Solar System.
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Sunspot
Sunspots are temporary phenomena on the Sun's photosphere that appear as spots darker than the surrounding areas.
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Ultra-cool dwarf
An ultra-cool dwarf is a stellar or sub-stellar object of spectral class M that has an effective temperature under.
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Redirects here:
Differential rotation in stars.
References
[1] https://en.wikipedia.org/wiki/Differential_rotation
