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  2. Galactic coordinate system - Wikipedia

    en.wikipedia.org/wiki/Galactic_coordinate_system

    The galactic coordinate system is a celestial coordinate system in spherical coordinates, with the Sun as its center, the primary direction aligned with the approximate center of the Milky Way Galaxy, and the fundamental plane parallel to an approximation of the galactic plane but offset to its north.

  3. Astronomical coordinate systems - Wikipedia

    en.wikipedia.org/wiki/Astronomical_coordinate...

    The galactic coordinate system uses the approximate plane of the Milky Way Galaxy as its fundamental plane. The Solar System is still the center of the coordinate system, and the zero point is defined as the direction towards the Galactic Center. Galactic latitude resembles the elevation above the galactic plane and galactic longitude ...

  4. Jeans equations - Wikipedia

    en.wikipedia.org/wiki/Jeans_equations

    Combining the Vlasov equation with the Poisson equation for gravity: =. gives the Jeans equations. More explicitly, If n = n ( x , t ) is the density of stars in space, as a function of position x = ( x 1 , x 2 , x 3 ) and time t , v = ( v 1 , v 2 , v 3 ) is the velocity, and Φ = Φ( x , t ) is the gravitational potential , the Jeans equations ...

  5. Oort constants - Wikipedia

    en.wikipedia.org/wiki/Oort_constants

    Figure 1: Geometry of the Oort constants derivation, with a field star close to the Sun in the midplane of the Galaxy. Consider a star in the midplane of the Galactic disk with Galactic longitude at a distance from the Sun. Assume that both the star and the Sun have circular orbits around the center of the Galaxy at radii of and from the Galactic Center and rotational velocities of and ...

  6. Proper motion - Wikipedia

    en.wikipedia.org/wiki/Proper_motion

    Knowledge of the proper motion, distance, and radial velocity allows calculations of an object's motion from the Solar System's frame of reference and its motion from the galactic frame of reference – that is motion in respect to the Sun, and by coordinate transformation, that in respect to the Milky Way. [4]

  7. Astrometric solving - Wikipedia

    en.wikipedia.org/wiki/Astrometric_solving

    Astrometric solving or Plate solving or Astrometric calibration of an astronomical image is a technique used in astronomy and applied on celestial images. Solving an image is finding match between the imaged stars and a star catalogue.

  8. Supergalactic coordinate system - Wikipedia

    en.wikipedia.org/wiki/Supergalactic_coordinate...

    The supergalactic coordinate system is a spherical coordinate system in which the equator lies in the supergalactic plane. By convention, supergalactic latitude is usually abbreviated SGB, and supergalactic longitude as SGL, by analogy to b and l conventionally used for galactic coordinates. Supergalactic and Ecliptic plane

  9. Category:Astronomical coordinate systems - Wikipedia

    en.wikipedia.org/wiki/Category:Astronomical...

    Download QR code; Print/export ... Pages in category "Astronomical coordinate systems" ... Galactic coordinate system; Galactic quadrant;