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Stellar rotation is the angular motion of a star about its axis. The rate of rotation can be measured from the spectrum of the star, or by timing the movements of active features on the surface. The rotation of a star produces an equatorial bulge due to centrifugal force. As stars are not solid bodies, they can also undergo differential rotation.
Thus the magnitude of the galaxy rotation is related to the galaxy's visible mass. [21] While precise fitting of the bulge, disk, and halo density profiles is a rather complicated process, it is straightforward to model the observables of rotating galaxies through this relationship.
The slightly longer stellar period is measured as the Earth rotation angle (ERA), formerly the stellar angle. [4] An increase of 360° in the ERA is a full rotation of the Earth. A sidereal day on Earth is approximately 86164.0905 seconds (23 h 56 min 4.0905 s or 23.9344696 h).
Pages Related to Stellar properties, Pages using the word stellar in a physics context. ... Stellar remnant; Stellar rotation; Stellar scintillation; Stellar seismology;
Stellar proper motions have been used to infer the presence of a super-massive black hole at the center of the Milky Way. [18] This now confirmed to exist black hole is called Sgr A*, and has a mass of 4.3 × 10 6 M ☉ (solar masses). Proper motions of the galaxies in the Local Group are discussed in detail in Röser. [19]
A rotating black hole is a black hole that possesses angular momentum. In particular, it rotates about one of its axes of symmetry. In particular, it rotates about one of its axes of symmetry. All celestial objects – planets , stars ( Sun ), galaxies , black holes – spin.
The following table lists the common coordinate systems in use by the astronomical community. The fundamental plane divides the celestial sphere into two equal hemispheres and defines the baseline for the latitudinal coordinates, similar to the equator in the geographic coordinate system.
Rotation period with respect to distant stars, the sidereal rotation period (compared to Earth's mean Solar days) Synodic rotation period (mean Solar day) Apparent rotational period viewed from Earth Sun [i] 25.379995 days (Carrington rotation) 35 days (high latitude) 25 d 9 h 7 m 11.6 s 35 d ~28 days (equatorial) [2] Mercury: 58.6462 days [3 ...